**Authors**
Thomas W. Judson

**License**
GFDL-1.2-no-invariants-or-later

Abstract Algebra Theory and Applications Abstract Algebra Theory and Applications Thomas W. Judson Stephen F. Austin State University Sage Exercises for Abstract Algebra Robert A. Beezer University of Puget Sound Traducción al español Antonio Behn Universidad de Chile August 1, 2018 Edition: Annual Edition 2018 Website: abstract.pugetsound.edu © 1997–2018 Thomas W. Judson, Robert A. Beezer Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the appendix entitled “GNU Free Documentation License.” Acknowledgements I would like to acknowledge the following reviewers for their helpful comments and sugges- tions. • David Anderson, University of Tennessee, Knoxville • Robert Beezer, University of Puget Sound • Myron Hood, California Polytechnic State University • Herbert Kasube, Bradley University • John Kurtzke, University of Portland • Inessa Levi, University of Louisville • Geoffrey Mason, University of California, Santa Cruz • Bruce Mericle, Mankato State University • Kimmo Rosenthal, Union College • Mark Teply, University of Wisconsin I would also like to thank Steve Quigley, Marnie Pommett, Cathie Griffin, Kelle Karshick, and the rest of the staff at PWS Publishing for their guidance throughout this project. It has been a pleasure to work with them. Robert Beezer encouraged me to make Abstract Algebra: Theory and Applications avail- able as an open source textbook, a decision that I have never regretted. With his assistance, the book has been rewritten in PreTeXt (pretextbook.org), making it possible to quickly output print, web, pdf versions and more from the same source. The open source version of this book has received support from the National Science Foundation (Awards #DUE- 1020957 and #DUE–1625223). v Preface This text is intended for a one or two-semester undergraduate course in abstract algebra. Traditionally, these courses have covered the theoretical aspects of groups, rings, and fields. However, with the development of computing in the last several decades, applications that involve abstract algebra and discrete mathematics have become increasingly important, and many science, engineering, and computer science students are now electing to minor in mathematics. Though theory still occupies a central role in the subject of abstract algebra and no student should go through such a course without a good notion of what a proof is, the importance of applications such as coding theory and cryptography has grown significantly. Until recently most abstract algebra texts included few if any applications. However, one of the major problems in teaching an abstract algebra course is that for many students it is their first encounter with an environment that requires them to do rigorous proofs. Such students often find it hard to see the use of learning to prove theorems and propositions; applied examples help the instructor provide motivation. This text contains more material than can possibly be covered in a single semester. Certainly there is adequate material for a two-semester course, and perhaps more; however, for a one-semester course it would be quite easy to omit selected chapters and still have a useful text. The order of presentation of topics is standard: groups, then rings, and finally fields. Emphasis can be placed either on theory or on applications. A typical one-semester course might cover groups and rings while briefly touching on field theory, using Chapters 1 through 6, 9, 10, 11, 13 (the first part), 16, 17, 18 (the first part), 20, and 21. Parts of these chapters could be deleted and applications substituted according to the interests of the students and the instructor. A two-semester course emphasizing theory might cover Chapters 1 through 6, 9, 10, 11, 13 through 18, 20, 21, 22 (the first part), and 23. On the other hand, if applications are to be emphasized, the course might cover Chapters 1 through 14, and 16 through 22. In an applied course, some of the more theoretical results could be assumed or omitted. A chapter dependency chart appears below. (A broken line indicates a partial dependency.) vi vii Chapters 1–6 Chapter 8 Chapter 9 Chapter 7 Chapter 10 Chapter 11 Chapter 13 Chapter 16 Chapter 12 Chapter 14 Chapter 17 Chapter 15 Chapter 18 Chapter 20 Chapter 19 Chapter 21 Chapter 22 Chapter 23 Though there are no specific prerequisites for a course in abstract algebra, students who have had other higher-level courses in mathematics will generally be more prepared than those who have not, because they will possess a bit more mathematical sophistication. Occasionally, we shall assume some basic linear algebra; that is, we shall take for granted an elementary knowledge of matrices and determinants. This should present no great problem, since most students taking a course in abstract algebra have been introduced to matrices and determinants elsewhere in their career, if they have not already taken a sophomore or junior-level course in linear algebra. Exercise sections are the heart of any mathematics text. An exercise set appears at the end of each chapter. The nature of the exercises ranges over several categories; computa- tional, conceptual, and theoretical problems are included. A section presenting hints and solutions to many of the exercises appears at the end of the text. Often in the solutions a proof is only sketched, and it is up to the student to provide the details. The exercises range in difficulty from very easy to very challenging. Many of the more substantial prob- lems require careful thought, so the student should not be discouraged if the solution is not forthcoming after a few minutes of work. There are additional exercises or computer projects at the ends of many of the chapters. The computer projects usually require a knowledge of programming. All of these exercises viii and projects are more substantial in nature and allow the exploration of new results and theory. Sage (sagemath.org) is a free, open source, software system for advanced mathematics, which is ideal for assisting with a study of abstract algebra. Sage can be used either on your own computer, a local server, or on CoCalc (cocalc.com). Robert Beezer has written a comprehensive introduction to Sage and a selection of relevant exercises that appear at the end of each chapter, including live Sage cells in the web version of the book. All of the Sage code has been subject to automated tests of accuracy, using the most recent version available at this time: SageMath Version 8.2 (released 2018-05-05). Thomas W. Judson Nacogdoches, Texas 2018 Contents Acknowledgements v Preface vi 1 Preliminaries 1 1.1 A Short Note on Proofs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1 1.2 Sets and Equivalence Relations . . . . . . . . . . . . . . . . . . . . . . . . . 3 1.3 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 15 2 The Integers 17 2.1 Mathematical Induction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17 2.2 The Division Algorithm . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20 2.3 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 24 2.4 Programming Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 26 3 Groups 27 3.1 Integer Equivalence Classes and Symmetries . . . . . . . . . . . . . . . . . . 27 3.2 Definitions and Examples . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31 3.3 Subgroups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 36 3.4 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 38 3.5 Additional Exercises: Detecting Errors . . . . . . . . . . . . . . . . . . . . . 41 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 43 4 Cyclic Groups 44 4.1 Cyclic Subgroups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44 4.2 Multiplicative Group of Complex Numbers . . . . . . . . . . . . . . . . . . 47 4.3 The Method of Repeated Squares . . . . . . . . . . . . . . . . . . . . . . . . 50 4.4 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52 4.5 Programming Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 55 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 55 5 Permutation Groups 56 5.1 Definitions and Notation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 56 5.2 Dihedral Groups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 62 5.3 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 66 ix x CONTENTS 6 Cosets and Lagrange’s Theorem 69 6.1 Cosets . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 69 6.2 Lagrange’s Theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 71 6.3 Fermat’s and Euler’s Theorems . . . . . . . . . . . . . . . . . . . . . . . . . 72 6.4 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73 7 Introduction to Cryptography 75 7.1 Private Key Cryptography . . . . . . . . . . . . . . . . . . . . . . . . . . . . 75 7.2 Public Key Cryptography . . . . . . . . . . . . . . . . . . . . . . . . . . . . 77 7.3 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 80 7.4 Additional Exercises: Primality and Factoring . . . . . . . . . . . . . . . . . 82 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 83 8 Algebraic Coding Theory 84 8.1 Error-Detecting and Correcting Codes . . . . . . . . . . . . . . . . . . . . . 84 8.2 Linear Codes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 90 8.3 Parity-Check and Generator Matrices . . . . . . . . . . . . . . . . . . . . . 93 8.4 Efficient Decoding . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 98 8.5 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 101 8.6 Programming Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 105 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 105 9 Isomorphisms 106 9.1 Definition and Examples . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 106 9.2 Direct Products . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110 9.3 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 113 10 Normal Subgroups and Factor Groups 117 10.1 Factor Groups and Normal Subgroups . . . . . . . . . . . . . . . . . . . . . 117 10.2 The Simplicity of the Alternating Group . . . . . . . . . . . . . . . . . . . . 119 10.3 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 122 11 Homomorphisms 124 11.1 Group Homomorphisms . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 124 11.2 The Isomorphism Theorems . . . . . . . . . . . . . . . . . . . . . . . . . . . 126 11.3 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 129 11.4 Additional Exercises: Automorphisms . . . . . . . . . . . . . . . . . . . . . 130 12 Matrix Groups and Symmetry 132 12.1 Matrix Groups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 132 12.2 Symmetry . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 138 12.3 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 144 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 146 13 The Structure of Groups 148 13.1 Finite Abelian Groups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 148 13.2 Solvable Groups . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 152 13.3 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 155 13.4 Programming Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 157 CONTENTS xi 14 Group Actions 158 14.1 Groups Acting on Sets . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 158 14.2 The Class Equation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 161 14.3 Burnside’s Counting Theorem . . . . . . . . . . . . . . . . . . . . . . . . . . 162 14.4 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 168 14.5 Programming Exercise . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 170 References and Suggested Reading . . . . . . . . . . . . . . . . . . . . . . . . . . 170 15 The Sylow Theorems 172 15.1 The Sylow Theorems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 172 15.2 Examples and Applications . . . . . . . . . . . . . . . . . . . . . . . . . . . 175 15.3 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 178 15.4 A Project . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 179 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 180 16 Rings 181 16.1 Rings . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 181 16.2 Integral Domains and Fields . . . . . . . . . . . . . . . . . . . . . . . . . . . 184 16.3 Ring Homomorphisms and Ideals . . . . . . . . . . . . . . . . . . . . . . . . 186 16.4 Maximal and Prime Ideals . . . . . . . . . . . . . . . . . . . . . . . . . . . . 189 16.5 An Application to Software Design . . . . . . . . . . . . . . . . . . . . . . . 191 16.6 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 194 16.7 Programming Exercise . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 198 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 198 17 Polynomials 200 17.1 Polynomial Rings . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 200 17.2 The Division Algorithm . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 203 17.3 Irreducible Polynomials . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 206 17.4 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 211 17.5 Additional Exercises: Solving the Cubic and Quartic Equations . . . . . . . 213 18 Integral Domains 216 18.1 Fields of Fractions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 216 18.2 Factorization in Integral Domains . . . . . . . . . . . . . . . . . . . . . . . . 219 18.3 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 226 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 228 19 Lattices and Boolean Algebras 229 19.1 Lattices . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 229 19.2 Boolean Algebras . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 232 19.3 The Algebra of Electrical Circuits . . . . . . . . . . . . . . . . . . . . . . . . 237 19.4 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 239 19.5 Programming Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 241 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 242 20 Vector Spaces 243 20.1 Definitions and Examples . . . . . . . . . . . . . . . . . . . . . . . . . . . . 243 20.2 Subspaces . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 244 20.3 Linear Independence . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 245 20.4 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 247 xii CONTENTS References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 250 21 Fields 251 21.1 Extension Fields . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 251 21.2 Splitting Fields . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 259 21.3 Geometric Constructions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 262 21.4 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 266 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 268 22 Finite Fields 269 22.1 Structure of a Finite Field . . . . . . . . . . . . . . . . . . . . . . . . . . . . 269 22.2 Polynomial Codes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 273 22.3 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 279 22.4 Additional Exercises: Error Correction for BCH Codes . . . . . . . . . . . . 281 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 282 23 Galois Theory 283 23.1 Field Automorphisms . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 283 23.2 The Fundamental Theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . 287 23.3 Applications . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 293 23.4 Exercises . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 297 References and Suggested Readings . . . . . . . . . . . . . . . . . . . . . . . . . . 299 A GNU Free Documentation License 301 B Hints and Solutions to Selected Exercises 308 C Notation 322 Index 325 1 Preliminaries A certain amount of mathematical maturity is necessary to find and study applications of abstract algebra. A basic knowledge of set theory, mathematical induction, equivalence relations, and matrices is a must. Even more important is the ability to read and understand mathematical proofs. In this chapter we will outline the background needed for a course in abstract algebra. 1.1 A Short Note on Proofs Abstract mathematics is different from other sciences. In laboratory sciences such as chem- istry and physics, scientists perform experiments to discover new principles and verify theo- ries. Although mathematics is often motivated by physical experimentation or by computer simulations, it is made rigorous through the use of logical arguments. In studying abstract mathematics, we take what is called an axiomatic approach; that is, we take a collection of objects S and assume some rules about their structure. These rules are called axioms. Using the axioms for S, we wish to derive other information about S by using logical argu- ments. We require that our axioms be consistent; that is, they should not contradict one another. We also demand that there not be too many axioms. If a system of axioms is too restrictive, there will be few examples of the mathematical structure. A statement in logic or mathematics is an assertion that is either true or false. Consider the following examples: • 3 + 56 − 13 + 8/2. • All cats are black. • 2 + 3 = 5. • 2x = 6 exactly when x = 4. • If ax2 + bx + c = 0 and a ̸= 0, then √ −b ± b2 − 4ac x= . 2a • x3 − 4x2 + 5x − 6. All but the first and last examples are statements, and must be either true or false. A mathematical proof is nothing more than a convincing argument about the accuracy of a statement. Such an argument should contain enough detail to convince the audience; for instance, we can see that the statement “2x = 6 exactly when x = 4” is false by evaluating 2 · 4 and noting that 6 ̸= 8, an argument that would satisfy anyone. Of course, audiences 1 2 CHAPTER 1. PRELIMINARIES may vary widely: proofs can be addressed to another student, to a professor, or to the reader of a text. If more detail than needed is presented in the proof, then the explanation will be either long-winded or poorly written. If too much detail is omitted, then the proof may not be convincing. Again it is important to keep the audience in mind. High school students require much more detail than do graduate students. A good rule of thumb for an argument in an introductory abstract algebra course is that it should be written to convince one’s peers, whether those peers be other students or other readers of the text. Let us examine different types of statements. A statement could be as simple as “10/5 = 2;” however, mathematicians are usually interested in more complex statements such as “If p, then q,” where p and q are both statements. If certain statements are known or assumed to be true, we wish to know what we can say about other statements. Here p is called the hypothesis and q is known as the conclusion. Consider the following statement: If ax2 + bx + c = 0 and a ̸= 0, then √ −b ± b2 − 4ac x= . 2a The hypothesis is ax2 + bx + c = 0 and a ̸= 0; the conclusion is √ −b ± b2 − 4ac x= . 2a Notice that the statement says nothing about whether or not the hypothesis is true. How- ever, if this entire statement is true and we can show that ax2 + bx + c = 0 with a ̸= 0 is true, then the conclusion must be true. A proof of this statement might simply be a series of equations: ax2 + bx + c = 0 b c x2 + x = − a a ( )2 ( )2 b b b c x2 + x + = − a 2a 2a a ( ) b 2 b2 − 4ac x+ = 2a 4a2 √ b ± b2 − 4ac x+ = 2a 2a √ −b ± b2 − 4ac x= . 2a If we can prove a statement true, then that statement is called a proposition. A proposition of major importance is called a theorem. Sometimes instead of proving a theorem or proposition all at once, we break the proof down into modules; that is, we prove several supporting propositions, which are called lemmas, and use the results of these propositions to prove the main result. If we can prove a proposition or a theorem, we will often, with very little effort, be able to derive other related propositions called corollaries. Some Cautions and Suggestions There are several different strategies for proving propositions. In addition to using different methods of proof, students often make some common mistakes when they are first learning how to prove theorems. To aid students who are studying abstract mathematics for the 1.2. SETS AND EQUIVALENCE RELATIONS 3 first time, we list here some of the difficulties that they may encounter and some of the strategies of proof available to them. It is a good idea to keep referring back to this list as a reminder. (Other techniques of proof will become apparent throughout this chapter and the remainder of the text.) • A theorem cannot be proved by example; however, the standard way to show that a statement is not a theorem is to provide a counterexample. • Quantifiers are important. Words and phrases such as only, for all, for every, and for some possess different meanings. • Never assume any hypothesis that is not explicitly stated in the theorem. You cannot take things for granted. • Suppose you wish to show that an object exists and is unique. First show that there actually is such an object. To show that it is unique, assume that there are two such objects, say r and s, and then show that r = s. • Sometimes it is easier to prove the contrapositive of a statement. Proving the state- ment “If p, then q” is exactly the same as proving the statement “If not q, then not p.” • Although it is usually better to find a direct proof of a theorem, this task can some- times be difficult. It may be easier to assume that the theorem that you are trying to prove is false, and to hope that in the course of your argument you are forced to make some statement that cannot possibly be true. Remember that one of the main objectives of higher mathematics is proving theorems. Theorems are tools that make new and productive applications of mathematics possible. We use examples to give insight into existing theorems and to foster intuitions as to what new theorems might be true. Applications, examples, and proofs are tightly interconnected— much more so than they may seem at first appearance. 1.2 Sets and Equivalence Relations Set Theory A set is a well-defined collection of objects; that is, it is defined in such a manner that we can determine for any given object x whether or not x belongs to the set. The objects that belong to a set are called its elements or members. We will denote sets by capital letters, such as A or X; if a is an element of the set A, we write a ∈ A. A set is usually specified either by listing all of its elements inside a pair of braces or by stating the property that determines whether or not an object x belongs to the set. We might write X = {x1 , x2 , . . . , xn } for a set containing elements x1 , x2 , . . . , xn or X = {x : x satisfies P} if each x in X satisfies a certain property P. For example, if E is the set of even positive integers, we can describe E by writing either E = {2, 4, 6, . . .} or E = {x : x is an even integer and x > 0}. 4 CHAPTER 1. PRELIMINARIES We write 2 ∈ E when we want to say that 2 is in the set E, and −3 ∈ / E to say that −3 is not in the set E. Some of the more important sets that we will consider are the following: N = {n : n is a natural number} = {1, 2, 3, . . .}; Z = {n : n is an integer} = {. . . , −1, 0, 1, 2, . . .}; Q = {r : r is a rational number} = {p/q : p, q ∈ Z where q ̸= 0}; R = {x : x is a real number}; C = {z : z is a complex number}. We can find various relations between sets as well as perform operations on sets. A set A is a subset of B, written A ⊂ B or B ⊃ A, if every element of A is also an element of B. For example, {4, 5, 8} ⊂ {2, 3, 4, 5, 6, 7, 8, 9} and N ⊂ Z ⊂ Q ⊂ R ⊂ C. Trivially, every set is a subset of itself. A set B is a proper subset of a set A if B ⊂ A but B ̸= A. If A is not a subset of B, we write A ̸⊂ B; for example, {4, 7, 9} ̸⊂ {2, 4, 5, 8, 9}. Two sets are equal, written A = B, if we can show that A ⊂ B and B ⊂ A. It is convenient to have a set with no elements in it. This set is called the empty set and is denoted by ∅. Note that the empty set is a subset of every set. To construct new sets out of old sets, we can perform certain operations: the union A ∪ B of two sets A and B is defined as A ∪ B = {x : x ∈ A or x ∈ B}; the intersection of A and B is defined by A ∩ B = {x : x ∈ A and x ∈ B}. If A = {1, 3, 5} and B = {1, 2, 3, 9}, then A ∪ B = {1, 2, 3, 5, 9} and A ∩ B = {1, 3}. We can consider the union and the intersection of more than two sets. In this case we write ∪n Ai = A1 ∪ . . . ∪ An i=1 and ∩ n Ai = A1 ∩ . . . ∩ An i=1 for the union and intersection, respectively, of the sets A1 , . . . , An . When two sets have no elements in common, they are said to be disjoint; for example, if E is the set of even integers and O is the set of odd integers, then E and O are disjoint. Two sets A and B are disjoint exactly when A ∩ B = ∅. Sometimes we will work within one fixed set U , called the universal set. For any set A ⊂ U , we define the complement of A, denoted by A′ , to be the set A′ = {x : x ∈ U and x ∈ / A}. We define the difference of two sets A and B to be A \ B = A ∩ B ′ = {x : x ∈ A and x ∈ / B}. 1.2. SETS AND EQUIVALENCE RELATIONS 5 Example 1.1. Let R be the universal set and suppose that A = {x ∈ R : 0 < x ≤ 3} and B = {x ∈ R : 2 ≤ x < 4}. Then A ∩ B = {x ∈ R : 2 ≤ x ≤ 3} A ∪ B = {x ∈ R : 0 < x < 4} A \ B = {x ∈ R : 0 < x < 2} A′ = {x ∈ R : x ≤ 0 or x > 3}. Proposition 1.2. Let A, B, and C be sets. Then 1. A ∪ A = A, A ∩ A = A, and A \ A = ∅; 2. A ∪ ∅ = A and A ∩ ∅ = ∅; 3. A ∪ (B ∪ C) = (A ∪ B) ∪ C and A ∩ (B ∩ C) = (A ∩ B) ∩ C; 4. A ∪ B = B ∪ A and A ∩ B = B ∩ A; 5. A ∪ (B ∩ C) = (A ∪ B) ∩ (A ∪ C); 6. A ∩ (B ∪ C) = (A ∩ B) ∪ (A ∩ C). Proof. We will prove (1) and (3) and leave the remaining results to be proven in the exercises. (1) Observe that A ∪ A = {x : x ∈ A or x ∈ A} = {x : x ∈ A} =A and A ∩ A = {x : x ∈ A and x ∈ A} = {x : x ∈ A} = A. Also, A \ A = A ∩ A′ = ∅. (3) For sets A, B, and C, A ∪ (B ∪ C) = A ∪ {x : x ∈ B or x ∈ C} = {x : x ∈ A or x ∈ B, or x ∈ C} = {x : x ∈ A or x ∈ B} ∪ C = (A ∪ B) ∪ C. A similar argument proves that A ∩ (B ∩ C) = (A ∩ B) ∩ C. Theorem 1.3 De Morgan’s Laws. Let A and B be sets. Then 1. (A ∪ B)′ = A′ ∩ B ′ ; 2. (A ∩ B)′ = A′ ∪ B ′ . 6 CHAPTER 1. PRELIMINARIES Proof. (1) If A ∪ B = ∅, then the theorem follows immediately since both A and B are the empty set. Otherwise, we must show that (A ∪ B)′ ⊂ A′ ∩ B ′ and (A ∪ B)′ ⊃ A′ ∩ B ′ . Let x ∈ (A ∪ B)′ . Then x ∈ / A ∪ B. So x is neither in A nor in B, by the definition of the union of sets. By the definition of the complement, x ∈ A′ and x ∈ B ′ . Therefore, x ∈ A′ ∩ B ′ and we have (A ∪ B)′ ⊂ A′ ∩ B ′ . To show the reverse inclusion, suppose that x ∈ A′ ∩ B ′ . Then x ∈ A′ and x ∈ B ′ , and so x ∈ / A and x ∈/ B. Thus x ∈ / A ∪ B and so x ∈ (A ∪ B)′ . Hence, (A ∪ B)′ ⊃ A′ ∩ B ′ and so (A ∪ B)′ = A′ ∩ B ′ . The proof of (2) is left as an exercise. Example 1.4. Other relations between sets often hold true. For example, (A \ B) ∩ (B \ A) = ∅. To see that this is true, observe that (A \ B) ∩ (B \ A) = (A ∩ B ′ ) ∩ (B ∩ A′ ) = A ∩ A′ ∩ B ∩ B ′ = ∅. Cartesian Products and Mappings Given sets A and B, we can define a new set A × B, called the Cartesian product of A and B, as a set of ordered pairs. That is, A × B = {(a, b) : a ∈ A and b ∈ B}. Example 1.5. If A = {x, y}, B = {1, 2, 3}, and C = ∅, then A × B is the set {(x, 1), (x, 2), (x, 3), (y, 1), (y, 2), (y, 3)} and A × C = ∅. We define the Cartesian product of n sets to be A1 × · · · × An = {(a1 , . . . , an ) : ai ∈ Ai for i = 1, . . . , n}. If A = A1 = A2 = · · · = An , we often write An for A × · · · × A (where A would be written n times). For example, the set R3 consists of all of 3-tuples of real numbers. Subsets of A×B are called relations. We will define a mapping or function f ⊂ A×B from a set A to a set B to be the special type of relation where (a, b) ∈ f if for every element a ∈ A there exists a unique element b ∈ B. Another way of saying this is that for every f element in A, f assigns a unique element in B. We usually write f : A → B or A → B. Instead of writing down ordered pairs (a, b) ∈ A × B, we write f (a) = b or f : a 7→ b. The set A is called the domain of f and f (A) = {f (a) : a ∈ A} ⊂ B is called the range or image of f . We can think of the elements in the function’s domain as input values and the elements in the function’s range as output values. 1.2. SETS AND EQUIVALENCE RELATIONS 7 A B f 1 a 2 b 3 c A g B 1 a 2 b 3 c Figure 1.6: Mappings and relations Example 1.7. Suppose A = {1, 2, 3} and B = {a, b, c}. In Figure 1.6 we define relations f and g from A to B. The relation f is a mapping, but g is not because 1 ∈ A is not assigned to a unique element in B; that is, g(1) = a and g(1) = b. Given a function f : A → B, it is often possible to write a list describing what the function does to each specific element in the domain. However, not all functions can be described in this manner. For example, the function f : R → R that sends each real number to its cube is a mapping that must be described by writing f (x) = x3 or f : x 7→ x3 . Consider the relation f : Q → Z given by f (p/q) = p. We know that 1/2 = 2/4, but is f (1/2) = 1 or 2? This relation cannot be a mapping because it is not well-defined. A relation is well-defined if each element in the domain is assigned to a unique element in the range. If f : A → B is a map and the image of f is B, i.e., f (A) = B, then f is said to be onto or surjective. In other words, if there exists an a ∈ A for each b ∈ B such that f (a) = b, then f is onto. A map is one-to-one or injective if a1 ̸= a2 implies f (a1 ) ̸= f (a2 ). Equivalently, a function is one-to-one if f (a1 ) = f (a2 ) implies a1 = a2 . A map that is both one-to-one and onto is called bijective. Example 1.8. Let f : Z → Q be defined by f (n) = n/1. Then f is one-to-one but not onto. Define g : Q → Z by g(p/q) = p where p/q is a rational number expressed in its lowest terms with a positive denominator. The function g is onto but not one-to-one. Given two functions, we can construct a new function by using the range of the first function as the domain of the second function. Let f : A → B and g : B → C be mappings. Define a new map, the composition of f and g from A to C, by (g ◦ f )(x) = g(f (x)). 8 CHAPTER 1. PRELIMINARIES A B C f g 1 a X 2 b Y 3 c Z A C g◦f 1 X 2 Y 3 Z Figure 1.9: Composition of maps Example 1.10. Consider the functions f : A → B and g : B → C that are defined in Figure 1.9 (top). The composition of these functions, g ◦ f : A → C, is defined in Figure 1.9 (bottom). Example 1.11. Let f (x) = x2 and g(x) = 2x + 5. Then (f ◦ g)(x) = f (g(x)) = (2x + 5)2 = 4x2 + 20x + 25 and (g ◦ f )(x) = g(f (x)) = 2x2 + 5. In general, order makes a difference; that is, in most cases f ◦ g ̸= g ◦ f . √ Example 1.12. Sometimes it is the case that f ◦ g = g ◦ f . Let f (x) = x3 and g(x) = 3 x. Then √ √ (f ◦ g)(x) = f (g(x)) = f ( 3 x ) = ( 3 x )3 = x and √ 3 (g ◦ f )(x) = g(f (x)) = g(x3 ) = x3 = x. Example 1.13. Given a 2 × 2 matrix ( ) a b A= , c d we can define a map TA : R2 → R2 by TA (x, y) = (ax + by, cx + dy) for (x, y) in R2 . This is actually matrix multiplication; that is, ( )( ) ( ) a b x ax + by = . c d y cx + dy Maps from Rn to Rm given by matrices are called linear maps or linear transforma- tions. 1.2. SETS AND EQUIVALENCE RELATIONS 9 Example 1.14. Suppose that S = {1, 2, 3}. Define a map π : S → S by π(1) = 2, π(2) = 1, π(3) = 3. This is a bijective map. An alternative way to write π is ( ) ( ) 1 2 3 1 2 3 = . π(1) π(2) π(3) 2 1 3 For any set S, a one-to-one and onto mapping π : S → S is called a permutation of S. Theorem 1.15. Let f : A → B, g : B → C, and h : C → D. Then 1. The composition of mappings is associative; that is, (h ◦ g) ◦ f = h ◦ (g ◦ f ); 2. If f and g are both one-to-one, then the mapping g ◦ f is one-to-one; 3. If f and g are both onto, then the mapping g ◦ f is onto; 4. If f and g are bijective, then so is g ◦ f . Proof. We will prove (1) and (3). Part (2) is left as an exercise. Part (4) follows directly from (2) and (3). (1) We must show that h ◦ (g ◦ f ) = (h ◦ g) ◦ f. For a ∈ A we have (h ◦ (g ◦ f ))(a) = h((g ◦ f )(a)) = h(g(f (a))) = (h ◦ g)(f (a)) = ((h ◦ g) ◦ f )(a). (3) Assume that f and g are both onto functions. Given c ∈ C, we must show that there exists an a ∈ A such that (g ◦ f )(a) = g(f (a)) = c. However, since g is onto, there is an element b ∈ B such that g(b) = c. Similarly, there is an a ∈ A such that f (a) = b. Accordingly, (g ◦ f )(a) = g(f (a)) = g(b) = c. If S is any set, we will use idS or id to denote the identity mapping from S to itself. Define this map by id(s) = s for all s ∈ S. A map g : B → A is an inverse mapping of f : A → B if g ◦ f = idA and f ◦ g = idB ; in other words, the inverse function of a function simply “undoes” the function. A map is said to be invertible if it has an inverse. We usually write f −1 for the inverse of f . √ Example 1.16. The function f (x) = x3 has inverse f −1 (x) = 3 x by Example 1.12. Example 1.17. The natural logarithm and the exponential functions, f (x) = ln x and f −1 (x) = ex , are inverses of each other provided that we are careful about choosing domains. Observe that f (f −1 (x)) = f (ex ) = ln ex = x and f −1 (f (x)) = f −1 (ln x) = eln x = x whenever composition makes sense. 10 CHAPTER 1. PRELIMINARIES Example 1.18. Suppose that ( ) 3 1 A= . 5 2 Then A defines a map from R2 to R2 by TA (x, y) = (3x + y, 5x + 2y). We can find an inverse map of TA by simply inverting the matrix A; that is, TA−1 = TA−1 . In this example, ( ) 2 −1 A−1 = ; −5 3 hence, the inverse map is given by TA−1 (x, y) = (2x − y, −5x + 3y). It is easy to check that TA−1 ◦ TA (x, y) = TA ◦ TA−1 (x, y) = (x, y). Not every map has an inverse. If we consider the map TB (x, y) = (3x, 0) given by the matrix ( ) 3 0 B= , 0 0 then an inverse map would have to be of the form TB−1 (x, y) = (ax + by, cx + dy) and (x, y) = T ◦ TB−1 (x, y) = (3ax + 3by, 0) for all x and y. Clearly this is impossible because y might not be 0. Example 1.19. Given the permutation ( ) 1 2 3 π= 2 3 1 on S = {1, 2, 3}, it is easy to see that the permutation defined by ( ) −1 1 2 3 π = 3 1 2 is the inverse of π. In fact, any bijective mapping possesses an inverse, as we will see in the next theorem. Theorem 1.20. A mapping is invertible if and only if it is both one-to-one and onto. Proof. Suppose first that f : A → B is invertible with inverse g : B → A. Then g ◦ f = idA is the identity map; that is, g(f (a)) = a. If a1 , a2 ∈ A with f (a1 ) = f (a2 ), then a1 = g(f (a1 )) = g(f (a2 )) = a2 . Consequently, f is one-to-one. Now suppose that b ∈ B. To show that f is onto, it is necessary to find an a ∈ A such that f (a) = b, but f (g(b)) = b with g(b) ∈ A. Let a = g(b). Conversely, let f be bijective and let b ∈ B. Since f is onto, there exists an a ∈ A such that f (a) = b. Because f is one-to-one, a must be unique. Define g by letting g(b) = a. We have now constructed the inverse of f . 1.2. SETS AND EQUIVALENCE RELATIONS 11 Equivalence Relations and Partitions A fundamental notion in mathematics is that of equality. We can generalize equality with equivalence relations and equivalence classes. An equivalence relation on a set X is a relation R ⊂ X × X such that • (x, x) ∈ R for all x ∈ X (reflexive property); • (x, y) ∈ R implies (y, x) ∈ R (symmetric property); • (x, y) and (y, z) ∈ R imply (x, z) ∈ R (transitive property). Given an equivalence relation R on a set X, we usually write x ∼ y instead of (x, y) ∈ R. ∼ we will If the equivalence relation already has an associated notation such as =, ≡, or =, use that notation. Example 1.21. Let p, q, r, and s be integers, where q and s are nonzero. Define p/q ∼ r/s if ps = qr. Clearly ∼ is reflexive and symmetric. To show that it is also transitive, suppose that p/q ∼ r/s and r/s ∼ t/u, with q, s, and u all nonzero. Then ps = qr and ru = st. Therefore, psu = qru = qst. Since s ̸= 0, pu = qt. Consequently, p/q ∼ t/u. Example 1.22. Suppose that f and g are differentiable functions on R. We can define an equivalence relation on such functions by letting f (x) ∼ g(x) if f ′ (x) = g ′ (x). It is clear that ∼ is both reflexive and symmetric. To demonstrate transitivity, suppose that f (x) ∼ g(x) and g(x) ∼ h(x). From calculus we know that f (x) − g(x) = c1 and g(x) − h(x) = c2 , where c1 and c2 are both constants. Hence, f (x) − h(x) = (f (x) − g(x)) + (g(x) − h(x)) = c1 − c2 and f ′ (x) − h′ (x) = 0. Therefore, f (x) ∼ h(x). Example 1.23. For (x1 , y1 ) and (x2 , y2 ) in R2 , define (x1 , y1 ) ∼ (x2 , y2 ) if x21 +y12 = x22 +y22 . Then ∼ is an equivalence relation on R2 . Example 1.24. Let A and B be 2 × 2 matrices with entries in the real numbers. We can define an equivalence relation on the set of 2 × 2 matrices, by saying A ∼ B if there exists an invertible matrix P such that P AP −1 = B. For example, if ( ) ( ) 1 2 −18 33 A= and B = , −1 1 −11 20 then A ∼ B since P AP −1 = B for ( ) 2 5 P = . 1 3 Let I be the 2 × 2 identity matrix; that is, ( ) 1 0 I= . 0 1 Then IAI −1 = IAI = A; therefore, the relation is reflexive. To show symmetry, suppose that A ∼ B. Then there exists an invertible matrix P such that P AP −1 = B. So A = P −1 BP = P −1 B(P −1 )−1 . 12 CHAPTER 1. PRELIMINARIES Finally, suppose that A ∼ B and B ∼ C. Then there exist invertible matrices P and Q such that P AP −1 = B and QBQ−1 = C. Since C = QBQ−1 = QP AP −1 Q−1 = (QP )A(QP )−1 , the relation is transitive. Two matrices that are equivalent in this manner are said to be similar. P of a set X is a collection of nonempty sets X1 , X2 , . . . such that Xi ∩Xj = A partition ∪ ∅ for i ̸= j and k Xk = X. Let ∼ be an equivalence relation on a set X and let x ∈ X. Then [x] = {y ∈ X : y ∼ x} is called the equivalence class of x. We will see that an equivalence relation gives rise to a partition via equivalence classes. Also, whenever a partition of a set exists, there is some natural underlying equivalence relation, as the following theorem demonstrates. Theorem 1.25. Given an equivalence relation ∼ on a set X, the equivalence classes of X form a partition of X. Conversely, if P = {Xi } is a partition of a set X, then there is an equivalence relation on X with equivalence classes Xi . Proof. Suppose there exists an equivalence relation ∼ on the set X. For any∪x ∈ X, the reflexive property shows that x ∈ [x] and so [x] is nonempty. Clearly X = x∈X [x]. Now let x, y ∈ X. We need to show that either [x] = [y] or [x] ∩ [y] = ∅. Suppose that the intersection of [x] and [y] is not empty and that z ∈ [x] ∩ [y]. Then z ∼ x and z ∼ y. By symmetry and transitivity x ∼ y; hence, [x] ⊂ [y]. Similarly, [y] ⊂ [x] and so [x] = [y]. Therefore, any two equivalence classes are either disjoint or exactly the same. Conversely, suppose that P = {Xi } is a partition of a set X. Let two elements be equivalent if they are in the same partition. Clearly, the relation is reflexive. If x is in the same partition as y, then y is in the same partition as x, so x ∼ y implies y ∼ x. Finally, if x is in the same partition as y and y is in the same partition as z, then x must be in the same partition as z, and transitivity holds. Corollary 1.26. Two equivalence classes of an equivalence relation are either disjoint or equal. Let us examine some of the partitions given by the equivalence classes in the last set of examples. Example 1.27. In the equivalence relation in Example 1.21, two pairs of integers, (p, q) and (r, s), are in the same equivalence class when they reduce to the same fraction in its lowest terms. Example 1.28. In the equivalence relation in Example 1.22, two functions f (x) and g(x) are in the same partition when they differ by a constant. Example 1.29. We defined an equivalence class on R2 by (x1 , y1 ) ∼ (x2 , y2 ) if x21 + y12 = x22 + y22 . Two pairs of real numbers are in the same partition when they lie on the same circle about the origin. Example 1.30. Let r and s be two integers and suppose that n ∈ N. We say that r is congruent to s modulo n, or r is congruent to s mod n, if r − s is evenly divisible by n; that is, r − s = nk for some k ∈ Z. In this case we write r ≡ s (mod n). For example, 41 ≡ 17 (mod 8) since 41 − 17 = 24 is divisible by 8. We claim that congruence modulo n forms an equivalence relation of Z. Certainly any integer r is equivalent to itself since r − r = 0 is divisible by n. We will now show that the relation is symmetric. If r ≡ s 1.3. EXERCISES 13 (mod n), then r − s = −(s − r) is divisible by n. So s − r is divisible by n and s ≡ r (mod n). Now suppose that r ≡ s (mod n) and s ≡ t (mod n). Then there exist integers k and l such that r − s = kn and s − t = ln. To show transitivity, it is necessary to prove that r − t is divisible by n. However, r − t = r − s + s − t = kn + ln = (k + l)n, and so r − t is divisible by n. If we consider the equivalence relation established by the integers modulo 3, then [0] = {. . . , −3, 0, 3, 6, . . .}, [1] = {. . . , −2, 1, 4, 7, . . .}, [2] = {. . . , −1, 2, 5, 8, . . .}. Notice that [0] ∪ [1] ∪ [2] = Z and also that the sets are disjoint. The sets [0], [1], and [2] form a partition of the integers. The integers modulo n are a very important example in the study of abstract algebra and will become quite useful in our investigation of various algebraic structures such as groups and rings. In our discussion of the integers modulo n we have actually assumed a result known as the division algorithm, which will be stated and proved in Chapter 2. 1.3 Exercises 1. Suppose that A = {x : x ∈ N and x is even}, B = {x : x ∈ N and x is prime}, C = {x : x ∈ N and x is a multiple of 5}. Describe each of the following sets. (a) A ∩ B (c) A ∪ B (b) B ∩ C (d) A ∩ (B ∪ C) 2. If A = {a, b, c}, B = {1, 2, 3}, C = {x}, and D = ∅, list all of the elements in each of the following sets. (a) A × B (c) A × B × C (b) B × A (d) A × D 3. Find an example of two nonempty sets A and B for which A × B = B × A is true. 4. Prove A ∪ ∅ = A and A ∩ ∅ = ∅. 5. Prove A ∪ B = B ∪ A and A ∩ B = B ∩ A. 6. Prove A ∪ (B ∩ C) = (A ∪ B) ∩ (A ∪ C). 7. Prove A ∩ (B ∪ C) = (A ∩ B) ∪ (A ∩ C). 8. Prove A ⊂ B if and only if A ∩ B = A. 9. Prove (A ∩ B)′ = A′ ∪ B ′ . 10. Prove A ∪ B = (A ∩ B) ∪ (A \ B) ∪ (B \ A). 14 CHAPTER 1. PRELIMINARIES 11. Prove (A ∪ B) × C = (A × C) ∪ (B × C). 12. Prove (A ∩ B) \ B = ∅. 13. Prove (A ∪ B) \ B = A \ B. 14. Prove A \ (B ∪ C) = (A \ B) ∩ (A \ C). 15. Prove A ∩ (B \ C) = (A ∩ B) \ (A ∩ C). 16. Prove (A \ B) ∪ (B \ A) = (A ∪ B) \ (A ∩ B). 17. Which of the following relations f : Q → Q define a mapping? In each case, supply a reason why f is or is not a mapping. p+1 p+q (a) f (p/q) = (c) f (p/q) = p−2 q2 3p 3p2 p (b) f (p/q) = (d) f (p/q) = − 3q 7q 2 q 18. Determine which of the following functions are one-to-one and which are onto. If the function is not onto, determine its range. (a) f : R → R defined by f (x) = ex (b) f : Z → Z defined by f (n) = n2 + 3 (c) f : R → R defined by f (x) = sin x (d) f : Z → Z defined by f (x) = x2 19. Let f : A → B and g : B → C be invertible mappings; that is, mappings such that f and g −1 exist. Show that (g ◦ f )−1 = f −1 ◦ g −1 . −1 20. (a) Define a function f : N → N that is one-to-one but not onto. (b) Define a function f : N → N that is onto but not one-to-one. 21. Prove the relation defined on R2 by (x1 , y1 ) ∼ (x2 , y2 ) if x21 + y12 = x22 + y22 is an equivalence relation. 22. Let f : A → B and g : B → C be maps. (a) If f and g are both one-to-one functions, show that g ◦ f is one-to-one. (b) If g ◦ f is onto, show that g is onto. (c) If g ◦ f is one-to-one, show that f is one-to-one. (d) If g ◦ f is one-to-one and f is onto, show that g is one-to-one. (e) If g ◦ f is onto and g is one-to-one, show that f is onto. 23. Define a function on the real numbers by x+1 f (x) = . x−1 What are the domain and range of f ? What is the inverse of f ? Compute f ◦ f −1 and f −1 ◦ f . 24. Let f : X → Y be a map with A1 , A2 ⊂ X and B1 , B2 ⊂ Y . 1.3. EXERCISES 15 (a) Prove f (A1 ∪ A2 ) = f (A1 ) ∪ f (A2 ). (b) Prove f (A1 ∩ A2 ) ⊂ f (A1 ) ∩ f (A2 ). Give an example in which equality fails. (c) Prove f −1 (B1 ∪ B2 ) = f −1 (B1 ) ∪ f −1 (B2 ), where f −1 (B) = {x ∈ X : f (x) ∈ B}. (d) Prove f −1 (B1 ∩ B2 ) = f −1 (B1 ) ∩ f −1 (B2 ). (e) Prove f −1 (Y \ B1 ) = X \ f −1 (B1 ). 25. Determine whether or not the following relations are equivalence relations on the given set. If the relation is an equivalence relation, describe the partition given by it. If the relation is not an equivalence relation, state why it fails to be one. (a) x ∼ y in R if x ≥ y (c) x ∼ y in R if |x − y| ≤ 4 (b) m ∼ n in Z if mn > 0 (d) m ∼ n in Z if m ≡ n (mod 6) 26. Define a relation ∼ on R2 by stating that (a, b) ∼ (c, d) if and only if a2 +b2 ≤ c2 +d2 . Show that ∼ is reflexive and transitive but not symmetric. 27. Show that an m × n matrix gives rise to a well-defined map from Rn to Rm . 28. Find the error in the following argument by providing a counterexample. “The reflexive property is redundant in the axioms for an equivalence relation. If x ∼ y, then y ∼ x by the symmetric property. Using the transitive property, we can deduce that x ∼ x.” 29. Projective Real Line. Define a relation on R2 \{(0, 0)} by letting (x1 , y1 ) ∼ (x2 , y2 ) if there exists a nonzero real number λ such that (x1 , y1 ) = (λx2 , λy2 ). Prove that ∼ defines an equivalence relation on R2 \ (0, 0). What are the corresponding equivalence classes? This equivalence relation defines the projective line, denoted by P(R), which is very important in geometry. References and Suggested Readings [1] Artin, M. Abstract Algebra. 2nd ed. Pearson, Upper Saddle River, NJ, 2011. [2] Childs, L. A Concrete Introduction to Higher Algebra. 2nd ed. Springer-Verlag, New York, 1995. [3] Dummit, D. and Foote, R. Abstract Algebra. 3rd ed. Wiley, New York, 2003. [4] Ehrlich, G. Fundamental Concepts of Algebra. PWS-KENT, Boston, 1991. [5] Fraleigh, J. B. A First Course in Abstract Algebra. 7th ed. Pearson, Upper Saddle River, NJ, 2003. [6] Gallian, J. A. Contemporary Abstract Algebra. 7th ed. Brooks/Cole, Belmont, CA, 2009. [7] Halmos, P. Naive Set Theory. Springer, New York, 1991. One of the best references for set theory. [8] Herstein, I. N. Abstract Algebra. 3rd ed. Wiley, New York, 1996. [9] Hungerford, T. W. Algebra. Springer, New York, 1974. One of the standard graduate algebra texts. 16 CHAPTER 1. PRELIMINARIES [10] Lang, S. Algebra. 3rd ed. Springer, New York, 2002. Another standard graduate text. [11] Lidl, R. and Pilz, G. Applied Abstract Algebra. 2nd ed. Springer, New York, 1998. [12] Mackiw, G. Applications of Abstract Algebra. Wiley, New York, 1985. [13] Nickelson, W. K. Introduction to Abstract Algebra. 3rd ed. Wiley, New York, 2006. [14] Solow, D. How to Read and Do Proofs. 5th ed. Wiley, New York, 2009. [15] van der Waerden, B. L. A History of Algebra. Springer-Verlag, New York, 1985. An account of the historical development of algebra. 2 The Integers The integers are the building blocks of mathematics. In this chapter we will investigate the fundamental properties of the integers, including mathematical induction, the division algorithm, and the Fundamental Theorem of Arithmetic. 2.1 Mathematical Induction Suppose we wish to show that n(n + 1) 1 + 2 + ··· + n = 2 for any natural number n. This formula is easily verified for small numbers such as n = 1, 2, 3, or 4, but it is impossible to verify for all natural numbers on a case-by-case basis. To prove the formula true in general, a more generic method is required. Suppose we have verified the equation for the first n cases. We will attempt to show that we can generate the formula for the (n + 1)th case from this knowledge. The formula is true for n = 1 since 1(1 + 1) 1= . 2 If we have verified the first n cases, then n(n + 1) 1 + 2 + · · · + n + (n + 1) = +n+1 2 n2 + 3n + 2 = 2 (n + 1)[(n + 1) + 1] = . 2 This is exactly the formula for the (n + 1)th case. This method of proof is known as mathematical induction. Instead of attempting to verify a statement about some subset S of the positive integers N on a case-by-case basis, an impossible task if S is an infinite set, we give a specific proof for the smallest integer being considered, followed by a generic argument showing that if the statement holds for a given case, then it must also hold for the next case in the sequence. We summarize mathematical induction in the following axiom. Principle 2.1 First Principle of Mathematical Induction. Let S(n) be a statement about integers for n ∈ N and suppose S(n0 ) is true for some integer n0 . If for all integers k with k ≥ n0 , S(k) implies that S(k + 1) is true, then S(n) is true for all integers n greater than or equal to n0 . 17 18 CHAPTER 2. THE INTEGERS Example 2.2. For all integers n ≥ 3, 2n > n + 4. Since 8 = 23 > 3 + 4 = 7, the statement is true for n0 = 3. Assume that 2k > k + 4 for k ≥ 3. Then 2k+1 = 2 · 2k > 2(k + 4). But 2(k + 4) = 2k + 8 > k + 5 = (k + 1) + 4 since k is positive. Hence, by induction, the statement holds for all integers n ≥ 3. Example 2.3. Every integer 10n+1 + 3 · 10n + 5 is divisible by 9 for n ∈ N. For n = 1, 101+1 + 3 · 10 + 5 = 135 = 9 · 15 is divisible by 9. Suppose that 10k+1 + 3 · 10k + 5 is divisible by 9 for k ≥ 1. Then 10(k+1)+1 + 3 · 10k+1 + 5 = 10k+2 + 3 · 10k+1 + 50 − 45 = 10(10k+1 + 3 · 10k + 5) − 45 is divisible by 9. Example 2.4. We will prove the binomial theorem using mathematical induction; that is, n ( ) ∑ n n k n−k (a + b) = a b , k k=0 where a and b are real numbers, n ∈ N, and ( ) n n! = k k!(n − k)! is the binomial coefficient. We first show that ( ) ( ) ( ) n+1 n n = + . k k k−1 This result follows from ( ) ( ) n n n! n! + = + k k−1 k!(n − k)! (k − 1)!(n − k + 1)! (n + 1)! = k!(n + 1 − k)! ( ) n+1 = . k If n = 1, the binomial theorem is easy to verify. Now assume that the result is true for n greater than or equal to 1. Then (a + b)n+1 = (a + b)(a + b)n ( n ( ) ) ∑ n k n−k = (a + b) a b k k=0 ∑n ( ) n ( ) n k+1 n−k ∑ n k n+1−k = a b + a b k k k=0 k=0 2.1. MATHEMATICAL INDUCTION 19 ∑n ( ) ∑n ( ) n+1 n k n+1−k n k n+1−k =a + a b + a b + bn+1 k−1 k k=1 k=1 ∑n [( ) ( )] n n = an+1 + + ak bn+1−k + bn+1 k−1 k k=1 ∑ n + 1) n+1 ( = ak bn+1−k . k k=0 We have an equivalent statement of the Principle of Mathematical Induction that is often very useful. Principle 2.5 Second Principle of Mathematical Induction. Let S(n) be a statement about integers for n ∈ N and suppose S(n0 ) is true for some integer n0 . If S(n0 ), S(n0 + 1), . . . , S(k) imply that S(k + 1) for k ≥ n0 , then the statement S(n) is true for all integers n ≥ n0 . A nonempty subset S of Z is well-ordered if S contains a least element. Notice that the set Z is not well-ordered since it does not contain a smallest element. However, the natural numbers are well-ordered. Principle 2.6 Principle of Well-Ordering. Every nonempty subset of the natural num- bers is well-ordered. The Principle of Well-Ordering is equivalent to the Principle of Mathematical Induction. Lemma 2.7. The Principle of Mathematical Induction implies that 1 is the least positive natural number. Proof. Let S = {n ∈ N : n ≥ 1}. Then 1 ∈ S. Assume that n ∈ S. Since 0 < 1, it must be the case that n = n + 0 < n + 1. Therefore, 1 ≤ n < n + 1. Consequently, if n ∈ S, then n + 1 must also be in S, and by the Principle of Mathematical Induction, and S = N. Theorem 2.8. The Principle of Mathematical Induction implies the Principle of Well- Ordering. That is, every nonempty subset of N contains a least element. Proof. We must show that if S is a nonempty subset of the natural numbers, then S contains a least element. If S contains 1, then the theorem is true by Lemma 2.7. Assume that if S contains an integer k such that 1 ≤ k ≤ n, then S contains a least element. We will show that if a set S contains an integer less than or equal to n + 1, then S has a least element. If S does not contain an integer less than n + 1, then n + 1 is the smallest integer in S. Otherwise, since S is nonempty, S must contain an integer less than or equal to n. In this case, by induction, S contains a least element. Induction can also be very useful in formulating definitions. For instance, there are two ways to define n!, the factorial of a positive integer n. • The explicit definition: n! = 1 · 2 · 3 · · · (n − 1) · n. • The inductive or recursive definition: 1! = 1 and n! = n(n − 1)! for n > 1. Every good mathematician or computer scientist knows that looking at problems recursively, as opposed to explicitly, often results in better understanding of complex issues. 20 CHAPTER 2. THE INTEGERS 2.2 The Division Algorithm An application of the Principle of Well-Ordering that we will use often is the division algorithm. Theorem 2.9 Division Algorithm. Let a and b be integers, with b > 0. Then there exist unique integers q and r such that a = bq + r where 0 ≤ r < b. Proof. This is a perfect example of the existence-and-uniqueness type of proof. We must first prove that the numbers q and r actually exist. Then we must show that if q ′ and r′ are two other such numbers, then q = q ′ and r = r′ . Existence of q and r. Let S = {a − bk : k ∈ Z and a − bk ≥ 0}. If 0 ∈ S, then b divides a, and we can let q = a/b and r = 0. If 0 ∈ / S, we can use the Well- Ordering Principle. We must first show that S is nonempty. If a > 0, then a − b · 0 ∈ S. If a < 0, then a − b(2a) = a(1 − 2b) ∈ S. In either case S ̸= ∅. By the Well-Ordering Principle, S must have a smallest member, say r = a − bq. Therefore, a = bq + r, r ≥ 0. We now show that r < b. Suppose that r > b. Then a − b(q + 1) = a − bq − b = r − b > 0. In this case we would have a − b(q + 1) in the set S. But then a − b(q + 1) < a − bq, which would contradict the fact that r = a − bq is the smallest member of S. So r ≤ b. Since 0∈/ S, r ̸= b and so r < b. Uniqueness of q and r. Suppose there exist integers r, r′ , q, and q ′ such that a = bq + r, 0 ≤ r < b and a = bq ′ + r′ , 0 ≤ r′ < b. Then bq +r = bq ′ +r′ . Assume that r′ ≥ r. From the last equation we have b(q −q ′ ) = r′ −r; therefore, b must divide r′ − r and 0 ≤ r′ − r ≤ r′ < b. This is possible only if r′ − r = 0. Hence, r = r′ and q = q ′ . Let a and b be integers. If b = ak for some integer k, we write a | b. An integer d is called a common divisor of a and b if d | a and d | b. The greatest common divisor of integers a and b is a positive integer d such that d is a common divisor of a and b and if d′ is any other common divisor of a and b, then d′ | d. We write d = gcd(a, b); for example, gcd(24, 36) = 12 and gcd(120, 102) = 6. We say that two integers a and b are relatively prime if gcd(a, b) = 1. Theorem 2.10. Let a and b be nonzero integers. Then there exist integers r and s such that gcd(a, b) = ar + bs. Furthermore, the greatest common divisor of a and b is unique. Proof. Let S = {am + bn : m, n ∈ Z and am + bn > 0}. Clearly, the set S is nonempty; hence, by the Well-Ordering Principle S must have a smallest member, say d = ar + bs. We claim that d = gcd(a, b). Write a = dq + r′ where 0 ≤ r′ < d. If r′ > 0, then r′ = a − dq 2.2. THE DIVISION ALGORITHM 21 = a − (ar + bs)q = a − arq − bsq = a(1 − rq) + b(−sq), which is in S. But this would contradict the fact that d is the smallest member of S. Hence, r′ = 0 and d divides a. A similar argument shows that d divides b. Therefore, d is a common divisor of a and b. Suppose that d′ is another common divisor of a and b, and we want to show that d′ | d. If we let a = d′ h and b = d′ k, then d = ar + bs = d′ hr + d′ ks = d′ (hr + ks). So d′ must divide d. Hence, d must be the unique greatest common divisor of a and b. Corollary 2.11. Let a and b be two integers that are relatively prime. Then there exist integers r and s such that ar + bs = 1. The Euclidean Algorithm Among other things, Theorem 2.10 allows us to compute the greatest common divisor of two integers. Example 2.12. Let us compute the greatest common divisor of 945 and 2415. First observe that 2415 = 945 · 2 + 525 945 = 525 · 1 + 420 525 = 420 · 1 + 105 420 = 105 · 4 + 0. Reversing our steps, 105 divides 420, 105 divides 525, 105 divides 945, and 105 divides 2415. Hence, 105 divides both 945 and 2415. If d were another common divisor of 945 and 2415, then d would also have to divide 105. Therefore, gcd(945, 2415) = 105. If we work backward through the above sequence of equations, we can also obtain numbers r and s such that 945r + 2415s = 105. Observe that 105 = 525 + (−1) · 420 = 525 + (−1) · [945 + (−1) · 525] = 2 · 525 + (−1) · 945 = 2 · [2415 + (−2) · 945] + (−1) · 945 = 2 · 2415 + (−5) · 945. So r = −5 and s = 2. Notice that r and s are not unique, since r = 41 and s = −16 would also work. To compute gcd(a, b) = d, we are using repeated divisions to obtain a decreasing se- quence of positive integers r1 > r2 > · · · > rn = d; that is, b = aq1 + r1 a = r1 q2 + r2 r1 = r2 q3 + r3 22 CHAPTER 2. THE INTEGERS .. . rn−2 = rn−1 qn + rn rn−1 = rn qn+1 . To find r and s such that ar + bs = d, we begin with this last equation and substitute results obtained from the previous equations: d = rn = rn−2 − rn−1 qn = rn−2 − qn (rn−3 − qn−1 rn−2 ) = −qn rn−3 + (1 + qn qn−1 )rn−2 .. . = ra + sb. The algorithm that we have just used to find the greatest common divisor d of two integers a and b and to write d as the linear combination of a and b is known as the Euclidean algorithm. Prime Numbers Let p be an integer such that p > 1. We say that p is a prime number, or simply p is prime, if the only positive numbers that divide p are 1 and p itself. An integer n > 1 that is not prime is said to be composite. Lemma 2.13 Euclid. Let a and b be integers and p be a prime number. If p | ab, then either p | a or p | b. Proof. Suppose that p does not divide a. We must show that p | b. Since gcd(a, p) = 1, there exist integers r and s such that ar + ps = 1. So b = b(ar + ps) = (ab)r + p(bs). Since p divides both ab and itself, p must divide b = (ab)r + p(bs). Theorem 2.14 Euclid. There exist an infinite number of primes. Proof. We will prove this theorem by contradiction. Suppose that there are only a finite number of primes, say p1 , p2 , . . . , pn . Let P = p1 p2 · · · pn + 1. Then P must be divisible by some pi for 1 ≤ i ≤ n. In this case, pi must divide P − p1 p2 · · · pn = 1, which is a contradiction. Hence, either P is prime or there exists an additional prime number p ̸= pi that divides P . Theorem 2.15 Fundamental Theorem of Arithmetic. Let n be an integer such that n > 1. Then n = p1 p2 · · · pk , where p1 , . . . , pk are primes (not necessarily distinct). Furthermore, this factorization is unique; that is, if n = q1 q2 · · · ql , then k = l and the qi ’s are just the pi ’s rearranged. 2.2. THE DIVISION ALGORITHM 23 Proof. Uniqueness. To show uniqueness we will use induction on n. The theorem is certainly true for n = 2 since in this case n is prime. Now assume that the result holds for all integers m such that 1 ≤ m < n, and n = p1 p2 · · · pk = q1 q2 · · · ql , where p1 ≤ p2 ≤ · · · ≤ pk and q1 ≤ q2 ≤ · · · ≤ ql . By Lemma 2.13, p1 | qi for some i = 1, . . . , l and q1 | pj for some j = 1, . . . , k. Since all of the pi ’s and qi ’s are prime, p1 = qi and q1 = pj . Hence, p1 = q1 since p1 ≤ pj = q1 ≤ qi = p1 . By the induction hypothesis, n′ = p2 · · · pk = q2 · · · ql has a unique factorization. Hence, k = l and qi = pi for i = 1, . . . , k. Existence. To show existence, suppose that there is some integer that cannot be written as the product of primes. Let S be the set of all such numbers. By the Principle of Well- Ordering, S has a smallest number, say a. If the only positive factors of a are a and 1, then a is prime, which is a contradiction. Hence, a = a1 a2 where 1 < a1 < a and 1 < a2 < a. Neither a1 ∈ S nor a2 ∈ S, since a is the smallest element in S. So a1 = p1 · · · pr a2 = q1 · · · qs . Therefore, a = a1 a2 = p1 · · · pr q1 · · · qs . So a ∈ / S, which is a contradiction. Historical Note Prime numbers were first studied by the ancient Greeks. Two important results from antiquity are Euclid’s proof that an infinite number of primes exist and the Sieve of Eratos- thenes, a method of computing all of the prime numbers less than a fixed positive integer n. One problem in number theory is to find a function f such that f (n) is prime for each n integer n. Pierre Fermat (1601?–1665) conjectured that 22 + 1 was prime for all n, but later it was shown by Leonhard Euler (1707–1783) that 5 22 + 1 = 4,294,967,297 is a composite number. One of the many unproven conjectures about prime numbers is Goldbach’s Conjecture. In a letter to Euler in 1742, Christian Goldbach stated the conjec- ture that every even integer with the exception of 2 seemed to be the sum of two primes: 4 = 2 + 2, 6 = 3 + 3, 8 = 3 + 5, . . .. Although the conjecture has been verified for the numbers up through 4 × 1018 , it has yet to be proven in general. Since prime numbers play an important role in public key cryptography, there is currently a great deal of interest in determining whether or not a large number is prime. Sage Sage’s original purpose was to support research in number theory, so it is perfect for the types of computations with the integers that we have in this chapter. 24 CHAPTER 2. THE INTEGERS 2.3 Exercises 1. Prove that n(n + 1)(2n + 1) 12 + 2 2 + · · · + n2 = 6 for n ∈ N. 2. Prove that n2 (n + 1)2 13 + 23 + · · · + n3 = 4 for n ∈ N. 3. Prove that n! > 2n for n ≥ 4. 4. Prove that n(3n − 1)x x + 4x + 7x + · · · + (3n − 2)x = 2 for n ∈ N. 5. Prove that 10n+1 + 10n + 1 is divisible by 3 for n ∈ N. 6. Prove that 4 · 102n + 9 · 102n−1 + 5 is divisible by 99 for n ∈ N. 7. Show that 1∑ n √ n a1 a2 · · · an ≤ ak . n k=1 8. Prove the Leibniz rule for f (n) (x), where f (n) is the nth derivative of f ; that is, show that ∑n ( ) (n) n (k) (f g) (x) = f (x)g (n−k) (x). k k=0 9. Use induction to prove that 1 + 2 + 22 + · · · + 2n = 2n+1 − 1 for n ∈ N. 10. Prove that 1 1 1 n + + ··· + = 2 6 n(n + 1) n+1 for n ∈ N. 11. If x is a nonnegative real number, then show that (1+x)n −1 ≥ nx for n = 0, 1, 2, . . .. 12. Power Sets. Let X be a set. Define the power set of X, denoted P(X), to be the set of all subsets of X. For example, P({a, b}) = {∅, {a}, {b}, {a, b}}. For every positive integer n, show that a set with exactly n elements has a power set with exactly 2n elements. 13. Prove that the two principles of mathematical induction stated in Section 2.1 are equivalent. 14. Show that the Principle of Well-Ordering for the natural numbers implies that 1 is the smallest natural number. Use this result to show that the Principle of Well-Ordering implies the Principle of Mathematical Induction; that is, show that if S ⊂ N such that 1 ∈ S and n + 1 ∈ S whenever n ∈ S, then S = N. 15. For each of the following pairs of numbers a and b, calculate gcd(a, b) and find integers r and s such that gcd(a, b) = ra + sb. 2.3. EXERCISES 25 (a) 14 and 39 (d) 471 and 562 (b) 234 and 165 (e) 23771 and 19945 (c) 1739 and 9923 (f) −4357 and 3754 16. Let a and b be nonzero integers. If there exist integers r and s such that ar + bs = 1, show that a and b are relatively prime. 17. Fibonacci Numbers. The Fibonacci numbers are 1, 1, 2, 3, 5, 8, 13, 21, . . . . We can define them inductively by f1 = 1, f2 = 1, and fn+2 = fn+1 + fn for n ∈ N. (a) Prove that fn < 2n . (b) Prove that fn+1 fn−1 = fn2 + (−1)n , n ≥ 2. √ √ √ (c) Prove that fn = [(1 + 5 )n − (1 − 5 )n ]/2n 5. √ (d) Show that limn→∞ fn /fn+1 = ( 5 − 1)/2. (e) Prove that fn and fn+1 are relatively prime. 18. Let a and b be integers such that gcd(a, b) = 1. Let r and s be integers such that ar + bs = 1. Prove that gcd(a, s) = gcd(r, b) = gcd(r, s) = 1. 19. Let x, y ∈ N be relatively prime. If xy is a perfect square, prove that x and y must both be perfect squares. 20. Using the division algorithm, show that every perfect square is of the form 4k or 4k + 1 for some nonnegative integer k. 21. Suppose that a, b, r, s are pairwise relatively prime and that a2 + b2 = r2 a2 − b2 = s2 . Prove that a, r, and s are odd and b is even. 22. Let n ∈ N. Use the division algorithm to prove that every integer is congruent mod n to precisely one of the integers 0, 1, . . . , n − 1. Conclude that if r is an integer, then there is exactly one s in Z such that 0 ≤ s < n and [r] = [s]. Hence, the integers are indeed partitioned by congruence mod n. 23. Define the least common multiple of two nonzero integers a and b, denoted by lcm(a, b), to be the nonnegative integer m such that both a and b divide m, and if a and b divide any other integer n, then m also divides n. Prove there exists a unique least common multiple for any two integers a and b. 24. If d = gcd(a, b) and m = lcm(a, b), prove that dm = |ab|. 25. Show that lcm(a, b) = ab if and only if gcd(a, b) = 1. 26. Prove that gcd(a, c) = gcd(b, c) = 1 if and only if gcd(ab, c) = 1 for integers a, b, and c. 27. Let a, b, c ∈ Z. Prove that if gcd(a, b) = 1 and a | bc, then a | c. 26 CHAPTER 2. THE INTEGERS 28. Let p ≥ 2. Prove that if 2p − 1 is prime, then p must also be prime. 29. Prove that there are an infinite number of primes of the form 6n + 5. 30. Prove that there are an infinite number of primes of the form 4n − 1. 31. Using the fact that 2 is prime, show√that there do not exist integers p and q such that p2 = 2q 2 . Demonstrate that therefore 2 cannot be a rational number. 2.4 Programming Exercises 1. The Sieve of Eratosthenes. One method of computing all of the prime numbers less than a certain fixed positive integer N is to list all of the numbers n such that 1 < n < N . Begin by eliminating all of the multiples of 2. Next eliminate all of the multiples of 3. Now eliminate all of the multiples of 5. Notice that 4 has already been crossed out. Continue √ in this manner, noticing that we do not have to go all the way to N ; it suffices to stop at N . Using this method, compute all of the prime numbers less than N = 250. We can also use this method to find all of the integers that are relatively prime to an integer N . Simply eliminate the prime factors of N and all of their multiples. Using this method, find all of the numbers that are relatively prime to N = 120. Using the Sieve of Eratosthenes, write a program that will compute all of the primes less than an integer N . 2. Let N0 = N ∪ {0}. Ackermann’s function is the function A : N0 × N0 → N0 defined by the equations A(0, y) = y + 1, A(x + 1, 0) = A(x, 1), A(x + 1, y + 1) = A(x, A(x + 1, y)). Use this definition to compute A(3, 1). Write a program to evaluate Ackermann’s function. Modify the program to count the number of statements executed in the program when Ackermann’s function is evaluated. How many statements are executed in the evaluation of A(4, 1)? What about A(5, 1)? 3. Write a computer program that will implement the Euclidean algorithm. The program should accept two positive integers a and b as input and should output gcd(a, b) as well as integers r and s such that gcd(a, b) = ra + sb. References and Suggested Readings [1] Brookshear, J. G. Theory of Computation: Formal Languages, Automata, and Com- plexity. Benjamin/Cummings, Redwood City, CA, 1989. Shows the relationships of the theoretical aspects of computer science to set theory and the integers. [2] Hardy, G. H. and Wright, E. M. An Introduction to the Theory of Numbers. 6th ed. Oxford University Press, New York, 2008. [3] Niven, I. and Zuckerman, H. S. An Introduction to the Theory of Numbers. 5th ed. Wiley, New York, 1991. [4] Vanden Eynden, C. Elementary Number Theory. 2nd ed. Waveland Press, Long Grove IL, 2001. 3 Groups We begin our study of algebraic structures by investigating sets associated with single operations that satisfy certain reasonable axioms; that is, we want to define an operation on a set in a way that will generalize such familiar structures as the integers Z together with the single operation of addition, or invertible 2 × 2 matrices together with the single operation of matrix multiplication. The integers and the 2 × 2 matrices, together with their respective single operations, are examples of algebraic structures known as groups. The theory of groups occupies a central position in mathematics. Modern group theory arose from an attempt to find the roots of a polynomial in terms of its coefficients. Groups now play a central role in such areas as coding theory, counting, and the study of symmetries; many areas of biology, chemistry, and physics have benefited from group theory. 3.1 Integer Equivalence Classes and Symmetries Let us now investigate some mathematical structures that can be viewed as sets with single operations. The Integers mod n The integers mod n have become indispensable in the theory and applications of algebra. In mathematics they are used in cryptography, coding theory, and the detection of errors in identification codes. We have already seen that two integers a and b are equivalent mod n if n divides a − b. The integers mod n also partition Z into n different equivalence classes; we will denote the set of these equivalence classes by Zn . Consider the integers modulo 12 and the corresponding partition of the integers: [0] = {. . . , −12, 0, 12, 24, . . .}, [1] = {. . . , −11, 1, 13, 25, . . .}, .. . [11] = {. . . , −1, 11, 23, 35, . . .}. When no confusion can arise, we will use 0, 1, . . . , 11 to indicate the equivalence classes [0], [1], . . . , [11] respectively. We can do arithmetic on Zn . For two integers a and b, define addition modulo n to be (a + b) (mod n); that is, the remainder when a + b is divided by n. Similarly, multiplication modulo n is defined as (ab) (mod n), the remainder when ab is divided by n. 27 28 CHAPTER 3. GROUPS Example 3.1. The following examples illustrate integer arithmetic modulo n: 7 + 4 ≡ 1 (mod 5) 7 · 3 ≡ 1 (mod 5) 3 + 5 ≡ 0 (mod 8) 3 · 5 ≡ 7 (mod 8) 3 + 4 ≡ 7 (mod 12) 3 · 4 ≡ 0 (mod 12). In particular, notice that it is possible that the product of two nonzero numbers modulo n can be equivalent to 0 modulo n. Example 3.2. Most, but not all, of the usual laws of arithmetic hold for addition and multiplication in Zn . For instance, it is not necessarily true that there is a multiplicative inverse. Consider the multiplication table for Z8 in Table 3.3. Notice that 2, 4, and 6 do not have multiplicative inverses; that is, for n = 2, 4, or 6, there is no integer k such that kn ≡ 1 (mod 8). · 0 1 2 3 4 5 6 7 0 0 0 0 0 0 0 0 0 1 0 1 2 3 4 5 6 7 2 0 2 4 6 0 2 4 6 3 0 3 6 1 4 7 2 5 4 0 4 0 4 0 4 0 4 5 0 5 2 7 4 1 6 3 6 0 6 4 2 0 6 4 2 7 0 7 6 5 4 3 2 1 Table 3.3: Multiplication table for Z8 Proposition 3.4. Let Zn be the set of equivalence classes of the integers mod n and a, b, c ∈ Zn . 1. Addition and multiplication are commutative: a+b≡b+a (mod n) ab ≡ ba (mod n). 2. Addition and multiplication are associative: (a + b) + c ≡ a + (b + c) (mod n) (ab)c ≡ a(bc) (mod n). 3. There are both additive and multiplicative identities: a + 0 ≡ a (mod n) a · 1 ≡ a (mod n). 4. Multiplication distributes over addition: a(b + c) ≡ ab + ac (mod n). 3.1. INTEGER EQUIVALENCE CLASSES AND SYMMETRIES 29 5. For every integer a there is an additive inverse −a: a + (−a) ≡ 0 (mod n). 6. Let a be a nonzero integer. Then gcd(a, n) = 1 if and only if there exists a multiplicative inverse b for a (mod n); that is, a nonzero integer b such that ab ≡ 1 (mod n). Proof. We will prove (1) and (6) and leave the remaining properties to be proven in the exercises. (1) Addition and multiplication are commutative modulo n since the remainder of a + b divided by n is the same as the remainder of b + a divided by n. (6) Suppose that gcd(a, n) = 1. Then there exist integers r and s such that ar + ns = 1. Since ns = 1 − ar, it must be the case that ar ≡ 1 (mod n). Letting b be the equivalence class of r, ab ≡ 1 (mod n). Conversely, suppose that there exists an integer b such that ab ≡ 1 (mod n). Then n divides ab − 1, so there is an integer k such that ab − nk = 1. Let d = gcd(a, n). Since d divides ab − nk, d must also divide 1; hence, d = 1. Symmetries A B A B identity D C D C A B C D 180◦ rotation D C B A A B B A reflection vertical axis D C C D A B D C reflection horizontal axis D C A B Figure 3.5: Rigid motions of a rectangle A symmetry of a geometric figure is a rearrangement of the figure preserving the arrangement of its sides and vertices as well as its distances and angles. A map from the plane to itself preserving the symmetry of an object is called a rigid motion. For example, if we look at the rectangle in Figure 3.5, it is easy to see that a rotation of 180◦ or 360◦ returns a rectangle in the plane with the same orientation as the original rectangle and the same relationship among the vertices. A reflection of the rectangle across either the vertical 30 CHAPTER 3. GROUPS axis or the horizontal axis can also be seen to be a symmetry. However, a 90◦ rotation in either direction cannot be a symmetry unless the rectangle is a square. B B ( ) identity A B C id = A B C A C A C B A ( ) rotation A B C ρ1 = B C A A C C B B C ( ) rotation A B C ρ2 = C A B A C B A B C ( ) reflection A B C µ1 = A C B A C A B B B ( ) reflection A B C µ2 = C B A A C C A B A ( ) reflection A B C µ3 = B A C A C B C Figure 3.6: Symmetries of a triangle Let us find the symmetries of the equilateral triangle △ABC. To find a symmetry of △ABC, we must first examine the permutations of the vertices A, B, and C and then ask if a permutation extends to a symmetry of the triangle. Recall that a permutation of a set S is a one-to-one and onto map π : S → S. The three vertices have 3! = 6 permutations, so the triangle has at most six symmetries. To see that there are six permutations, observe there are three different possibilities for the first vertex, and two for the second, and the remaining vertex is determined by the placement of the first two. So we have 3·2·1 = 3! = 6 different arrangements. To denote the permutation of the vertices of an equilateral triangle that sends A to B, B to C, and C to A, we write the array ( ) A B C . B C A Notice that this particular permutation corresponds to the rigid motion of rotating the triangle by 120◦ in a clockwise direction. In fact, every permutation gives rise to a symmetry of the triangle. All of these symmetries are shown in Figure 3.6. A natural question to ask is what happens if one motion of the triangle △ABC is followed by another. Which symmetry is µ1 ρ1 ; that is, what happens when we do the permutation ρ1 and then the permutation µ1 ? Remember that we are composing functions 3.2. DEFINITIONS AND EXAMPLES 31 here. Although we usually multiply left to right, we compose functions right to left. We have (µ1 ρ1 )(A) = µ1 (ρ1 (A)) = µ1 (B) = C (µ1 ρ1 )(B) = µ1 (ρ1 (B)) = µ1 (C) = B (µ1 ρ1 )(C) = µ1 (ρ1 (C)) = µ1 (A) = A. This is the same symmetry as µ2 . Suppose we do these motions in the opposite order, ρ1 then µ1 . It is easy to determine that this is the same as the symmetry µ3 ; hence, ρ1 µ1 ̸= µ1 ρ1 . A multiplication table for the symmetries of an equilateral triangle △ABC is given in Table 3.7. Notice that in the multiplication table for the symmetries of an equilateral triangle, for every motion of the triangle α there is another motion β such that αβ = id; that is, for every motion there is another motion that takes the triangle back to its original orientation. ◦ id ρ1 ρ2 µ1 µ2 µ3 id id ρ1 ρ2 µ1 µ2 µ3 ρ1 ρ1 ρ2 id µ3 µ1 µ2 ρ2 ρ2 id ρ1 µ2 µ3 µ1 µ 1 µ1 µ 2 µ 3 id ρ1 ρ2 µ 2 µ2 µ 3 µ 1 ρ2 id ρ1 µ 3 µ3 µ 1 µ 2 ρ1 ρ2 id Table 3.7: Symmetries of an equilateral triangle 3.2 Definitions and Examples The integers mod n and the symmetries of a triangle or a rectangle are examples of groups. A binary operation or law of composition on a set G is a function G × G → G that assigns to each pair (a, b) ∈ G × G a unique element a ◦ b, or ab in G, called the composition of a and b. A group (G, ◦) is a set G together with a law of composition (a, b) 7→ a ◦ b that satisfies the following axioms. • The law of composition is associative. That is, (a ◦ b) ◦ c = a ◦ (b ◦ c) for a, b, c ∈ G. • There exists an element e ∈ G, called the identity element, such that for any element a∈G e ◦ a = a ◦ e = a. • For each element a ∈ G, there exists an inverse element in G, denoted by a−1 , such that a ◦ a−1 = a−1 ◦ a = e. A group G with the property that a ◦ b = b ◦ a for all a, b ∈ G is called abelian or commutative. Groups not satisfying this property are said to be nonabelian or non- commutative. 32 CHAPTER 3. GROUPS Example 3.8. The integers Z = {. . . , −1, 0, 1, 2, . . .} form a group under the operation of addition. The binary operation on two integers m, n ∈ Z is just their sum. Since the integers under addition already have a well-established notation, we will use the operator + instead of ◦; that is, we shall write m + n instead of m ◦ n. The identity is 0, and the inverse of n ∈ Z is written as −n instead of n−1 . Notice that the set of integers under addition have the additional property that m + n = n + m and therefore form an abelian group. Most of the time we will write ab instead of a ◦ b; however, if the group already has a natural operation such as addition in the integers, we will use that operation. That is, if we are adding two integers, we still write m + n, −n for the inverse, and 0 for the identity as usual. We also write m − n instead of m + (−n). It is often convenient to describe a group in terms of an addition or multiplication table. Such a table is called a Cayley table. Example 3.9. The integers mod n form a group under addition modulo n. Consider Z5 , consisting of the equivalence classes of the integers 0, 1, 2, 3, and 4. We define the group operation on Z5 by modular addition. We write the binary operation on the group additively; that is, we write m + n. The element 0 is the identity of the group and each element in Z5 has an inverse. For instance, 2 + 3 = 3 + 2 = 0. Table 3.10 is a Cayley table for Z5 . By Proposition 3.4, Zn = {0, 1, . . . , n − 1} is a group under the binary operation of addition mod n. + 0 1 2 3 4 0 0 1 2 3 4 1 1 2 3 4 0 2 2 3 4 0 1 3 3 4 0 1 2 4 4 0 1 2 3 Table 3.10: Cayley table for (Z5 , +) Example 3.11. Not every set with a binary operation is a group. For example, if we let modular multiplication be the binary operation on Zn , then Zn fails to be a group. The element 1 acts as a group identity since 1 · k = k · 1 = k for any k ∈ Zn ; however, a multiplicative inverse for 0 does not exist since 0 · k = k · 0 = 0 for every k in Zn . Even if we consider the set Zn \ {0}, we still may not have a group. For instance, let 2 ∈ Z6 . Then 2 has no multiplicative inverse since 0·2=0 1·2=2 2·2=4 3·2=0 4·2=2 5 · 2 = 4. By Proposition 3.4, every nonzero k does have an inverse in Zn if k is relatively prime to n. Denote the set of all such nonzero elements in Zn by U (n). Then U (n) is a group called the group of units of Zn . Table 3.12 is a Cayley table for the group U (8). 3.2. DEFINITIONS AND EXAMPLES 33 · 1 3 5 7 1 1 3 5 7 3 3 1 7 5 5 5 7 1 3 7 7 5 3 1 Table 3.12: Multiplication table for U (8) Example 3.13. The symmetries of an equilateral triangle described in Section 3.1 form a nonabelian group. As we observed, it is not necessarily true that αβ = βα for two symmetries α and β. Using Table 3.7, which is a Cayley table for this group, we can easily check that the symmetries of an equilateral triangle are indeed a group. We will denote this group by either S3 or D3 , for reasons that will be explained later. Example 3.14. We use M2 (R) to denote the set of all 2 × 2 matrices. Let GL2 (R) be the subset of M2 (R) consisting of invertible matrices; that is, a matrix ( ) a b A= c d is in GL2 (R) if there exists a matrix A−1 such that AA−1 = A−1 A = I, where I is the 2 × 2 identity matrix. For A to have an inverse is equivalent to requiring that the determinant of A be nonzero; that is, det A = ad − bc ̸= 0. The set of invertible matrices forms a group called the general linear group. The identity of the group is the identity matrix ( ) 1 0 I= . 0 1 The inverse of A ∈ GL2 (R) is ( ) 1 d −b A−1 = . ad − bc −c a The product of two invertible matrices is again invertible. Matrix multiplication is associa- tive, satisfying the other group axiom. For matrices it is not true in general that AB = BA; hence, GL2 (R) is another example of a nonabelian group. Example 3.15. Let ( ) ( ) 1 0 0 1 1= I= 0 1 −1 0 ( ) ( ) 0 i i 0 J= K= , i 0 0 −i where i2 = −1. Then the relations I 2 = J 2 = K 2 = −1, IJ = K, JK = I, KI = J, JI = −K, KJ = −I, and IK = −J hold. The set Q8 = {±1, ±I, ±J, ±K} is a group called the quaternion group. Notice that Q8 is noncommutative. Example 3.16. Let C∗ be the set of nonzero complex numbers. Under the operation of multiplication C∗ forms a group. The identity is 1. If z = a + bi is a nonzero complex number, then a − bi z −1 = 2 a + b2 is the inverse of z. It is easy to see that the remaining group axioms hold. 34 CHAPTER 3. GROUPS A group is finite, or has finite order, if it contains a finite number of elements; otherwise, the group is said to be infinite or to have infinite order. The order of a finite group is the number of elements that it contains. If G is a group containing n elements, we write |G| = n. The group Z5 is a finite group of order 5; the integers Z form an infinite group under addition, and we sometimes write |Z| = ∞. Basic Properties of Groups Proposition 3.17. The identity element in a group G is unique; that is, there exists only one element e ∈ G such that eg = ge = g for all g ∈ G. Proof. Suppose that e and e′ are both identities in G. Then eg = ge = g and e′ g = ge′ = g for all g ∈ G. We need to show that e = e′ . If we think of e as the identity, then ee′ = e′ ; but if e′ is the identity, then ee′ = e. Combining these two equations, we have e = ee′ = e′ . Inverses in a group are also unique. If g ′ and g ′′ are both inverses of an element g in a group G, then gg ′ = g ′ g = e and gg ′′ = g ′′ g = e. We want to show that g ′ = g ′′ , but g ′ = g ′ e = g ′ (gg ′′ ) = (g ′ g)g ′′ = eg ′′ = g ′′ . We summarize this fact in the following proposition. Proposition 3.18. If g is any element in a group G, then the inverse of g, denoted by g −1 , is unique. Proposition 3.19. Let G be a group. If a, b ∈ G, then (ab)−1 = b−1 a−1 . Proof. Let a, b ∈ G. Then abb−1 a−1 = aea−1 = aa−1 = e. Similarly, b−1 a−1 ab = e. But by the previous proposition, inverses are unique; hence, (ab)−1 = b−1 a−1 . Proposition 3.20. Let G be a group. For any a ∈ G, (a−1 )−1 = a. Proof. Observe that a−1 (a−1 )−1 = e. Consequently, multiplying both sides of this equation by a, we have (a−1 )−1 = e(a−1 )−1 = aa−1 (a−1 )−1 = ae = a. It makes sense to write equations with group elements and group operations. If a and b are two elements in a group G, does there exist an element x ∈ G such that ax = b? If such an x does exist, is it unique? The following proposition answers both of these questions positively. Proposition 3.21. Let G be a group and a and b be any two elements in G. Then the equations ax = b and xa = b have unique solutions in G. Proof. Suppose that ax = b. We must show that such an x exists. We can multiply both sides of ax = b by a−1 to find x = ex = a−1 ax = a−1 b. To show uniqueness, suppose that x1 and x2 are both solutions of ax = b; then ax1 = b = ax2 . So x1 = a−1 ax1 = a−1 ax2 = x2 . The proof for the existence and uniqueness of the solution of xa = b is similar. Proposition 3.22. If G is a group and a, b, c ∈ G, then ba = ca implies b = c and ab = ac implies b = c. 3.2. DEFINITIONS AND EXAMPLES 35 This proposition tells us that the right and left cancellation laws are true in groups. We leave the proof as an exercise. We can use exponential notation for groups just as we do in ordinary algebra. If G is a group and g ∈ G, then we define g 0 = e. For n ∈ N, we define gn = g · g · · · g | {z } n times and g −n = g −1 · g −1 · · · g −1 . | {z } n times Theorem 3.23. In a group, the usual laws of exponents hold; that is, for all g, h ∈ G, 1. g m g n = g m+n for all m, n ∈ Z; 2. (g m )n = g mn for all m, n ∈ Z; 3. (gh)n = (h−1 g −1 )−n for all n ∈ Z. Furthermore, if G is abelian, then (gh)n = g n hn . We will leave the proof of this theorem as an exercise. Notice that (gh)n ̸= g n hn in general, since the group may not be abelian. If the group is Z or Zn , we write the group operation additively and the exponential operation multiplicatively; that is, we write ng instead of g n . The laws of exponents now become 1. mg + ng = (m + n)g for all m, n ∈ Z; 2. m(ng) = (mn)g for all m, n ∈ Z; 3. m(g + h) = mg + mh for all n ∈ Z. It is important to realize that the last statement can be made only because Z and Zn are commutative groups. Historical Note Although the first clear axiomatic definition of a group was not given until the late 1800s, group-theoretic methods had been employed before this time in the development of many areas of mathematics, including geometry and the theory of algebraic equations. Joseph-Louis Lagrange used group-theoretic methods in a 1770–1771 memoir to study methods of solving polynomial equations. Later, Évariste Galois (1811–1832) succeeded in developing the mathematics necessary to determine exactly which polynomial equations could be solved in terms of the polynomials’coefficients. Galois’ primary tool was group theory. The study of geometry was revolutionized in 1872 when Felix Klein proposed that ge- ometric spaces should be studied by examining those properties that are invariant under a transformation of the space. Sophus Lie, a contemporary of Klein, used group theory to study solutions of partial differential equations. One of the first modern treatments of group theory appeared in William Burnside’s The Theory of Groups of Finite Order [1], first published in 1897. 36 CHAPTER 3. GROUPS 3.3 Subgroups Definitions and Examples Sometimes we wish to investigate smaller groups sitting inside a larger group. The set of even integers 2Z = {. . . , −2, 0, 2, 4, . . .} is a group under the operation of addition. This smaller group sits naturally inside of the group of integers under addition. We define a subgroup H of a group G to be a subset H of G such that when the group operation of G is restricted to H, H is a group in its own right. Observe that every group G with at least two elements will always have at least two subgroups, the subgroup consisting of the identity element alone and the entire group itself. The subgroup H = {e} of a group G is called the trivial subgroup. A subgroup that is a proper subset of G is called a proper subgroup. In many of the examples that we have investigated up to this point, there exist other subgroups besides the trivial and improper subgroups. Example 3.24. Consider the set of nonzero real numbers, R∗ , with the group operation of multiplication. The identity of this group is 1 and the inverse of any element a ∈ R∗ is just 1/a. We will show that Q∗ = {p/q : p and q are nonzero integers} is a subgroup of R∗ . The identity of R∗ is 1; however, 1 = 1/1 is the quotient of two nonzero integers. Hence, the identity of R∗ is in Q∗ . Given two elements in Q∗ , say p/q and r/s, their product pr/qs is also in Q∗ . The inverse of any element p/q ∈ Q∗ is again in Q∗ since (p/q)−1 = q/p. Since multiplication in R∗ is associative, multiplication in Q∗ is associative. Example 3.25. Recall that C∗ is the multiplicative group of nonzero complex numbers. Let H = {1, −1, i, −i}. Then H is a subgroup of C∗ . It is quite easy to verify that H is a group under multiplication and that H ⊂ C∗ . Example 3.26. Let SL2 (R) be the subset of GL2 (R)consisting of matrices of determinant one; that is, a matrix ( ) a b A= c d is in SL2 (R) exactly when ad − bc = 1. To show that SL2 (R) is a subgroup of the general linear group, we must show that it is a group under matrix multiplication. The 2×2 identity matrix is in SL2 (R), as is the inverse of the matrix A: ( ) −1 d −b A = . −c a It remains to show that multiplication is closed; that is, that the product of two matrices of determinant one also has determinant one. We will leave this task as an exercise. The group SL2 (R) is called the special linear group. Example 3.27. It is important to realize that a subset H of a group G can be a group without being a subgroup of G. For H to be a subgroup of G it must inherit G’s binary operation. The set of all 2 × 2 matrices, M2 (R), forms a group under the operation of addition. The 2 × 2 general linear group is a subset of M2 (R) and is a group under matrix multiplication, but it is not a subgroup of M2 (R). If we add two invertible matrices, we do not necessarily obtain another invertible matrix. Observe that ( ) ( ) ( ) 1 0 −1 0 0 0 + = , 0 1 0 −1 0 0 but the zero matrix is not in GL2 (R). 3.3. SUBGROUPS 37 Example 3.28. One way of telling whether or not two groups are the same is by examining their subgroups. Other than the trivial subgroup and the group itself, the group Z4 has a single subgroup consisting of the elements 0 and 2. From the group Z2 , we can form another group of four elements as follows. As a set this group is Z2 × Z2 . We perform the group operation coordinatewise; that is, (a, b) + (c, d) = (a + c, b + d). Table 3.29 is an addition table for Z2 × Z2 . Since there are three nontrivial proper subgroups of Z2 × Z2 , H1 = {(0, 0), (0, 1)}, H2 = {(0, 0), (1, 0)}, and H3 = {(0, 0), (1, 1)}, Z4 and Z2 × Z2 must be different groups. + (0, 0) (0, 1) (1, 0) (1, 1) (0, 0) (0, 0) (0, 1) (1, 0) (1, 1) (0, 1) (0, 1) (0, 0) (1, 1) (1, 0) (1, 0) (1, 0) (1, 1) (0, 0) (0, 1) (1, 1) (1, 1) (1, 0) (0, 1) (0, 0) Table 3.29: Addition table for Z2 × Z2 Some Subgroup Theorems Let us examine some criteria for determining exactly when a subset of a group is a subgroup. Proposition 3.30. A subset H of G is a subgroup if and only if it satisfies the following conditions. 1. The identity e of G is in H. 2. If h1 , h2 ∈ H, then h1 h2 ∈ H. 3. If h ∈ H, then h−1 ∈ H. Proof. First suppose that H is a subgroup of G. We must show that the three conditions hold. Since H is a group, it must have an identity eH . We must show that eH = e, where e is the identity of G. We know that eH eH = eH and that eeH = eH e = eH ; hence, eeH = eH eH . By right-hand cancellation, e = eH . The second condition holds since a subgroup H is a group. To prove the third condition, let h ∈ H. Since H is a group, there is an element h′ ∈ H such that hh′ = h′ h = e. By the uniqueness of the inverse in G, h′ = h−1 . Conversely, if the three conditions hold, we must show that H is a group under the same operation as G; however, these conditions plus the associativity of the binary operation are exactly the axioms stated in the definition of a group. Proposition 3.31. Let H be a subset of a group G. Then H is a subgroup of G if and only if H ̸= ∅, and whenever g, h ∈ H then gh−1 is in H. Proof. First assume that H is a subgroup of G. We wish to show that gh−1 ∈ H whenever g and h are in H. Since h is in H, its inverse h−1 must also be in H. Because of the closure of the group operation, gh−1 ∈ H. Conversely, suppose that H ⊂ G such that H ̸= ∅ and gh−1 ∈ H whenever g, h ∈ H. If g ∈ H, then gg −1 = e is in H. If g ∈ H, then eg −1 = g −1 is also in H. Now let h1 , h2 ∈ H. We must show that their product is also in H. However, h1 (h−1 2 ) −1 = h h ∈ H. Hence, 1 2 H is a subgroup of G. 38 CHAPTER 3. GROUPS Sage The first half of this text is about group theory. Sage includes Groups, Algorithms and Programming (gap), a program designed primarly for just group theory, and in con- tinuous development since 1986. Many of Sage’s computations for groups ultimately are performed by GAP. 3.4 Exercises 1. Find all x ∈ Z satisfying each of the following equations. (a) 3x ≡ 2 (mod 7) (d) 9x ≡ 3 (mod 5) (b) 5x + 1 ≡ 13 (mod 23) (e) 5x ≡ 1 (mod 6) (c) 5x + 1 ≡ 13 (mod 26) (f) 3x ≡ 1 (mod 6) 2. Which of the following multiplication tables defined on the set G = {a, b, c, d} form a group? Support your answer in each case. (a) (c) ◦ a b c d ◦ a b c d a a c d a a a b c d b b b c d b b c d a c c d a b c c d a b d d a b c d d a b c (b) (d) ◦ a b c d ◦ a b c d a a b c d a a b c d b b a d c b b a c d c c d a b c c b a d d d c b a d d d b c 3. Write out Cayley tables for groups formed by the symmetries of a rectangle and for (Z4 , +). How many elements are in each group? Are the groups the same? Why or why not? 4. Describe the symmetries of a rhombus and prove that the set of symmetries forms a group. Give Cayley tables for both the symmetries of a rectangle and the symmetries of a rhombus. Are the symmetries of a rectangle and those of a rhombus the same? 5. Describe the symmetries of a square and prove that the set of symmetries is a group. Give a Cayley table for the symmetries. How many ways can the vertices of a square be permuted? Is each permutation necessarily a symmetry of the square? The symmetry group of the square is denoted by D4 . 6. Give a multiplication table for the group U (12). 7. Let S = R \ {−1} and define a binary operation on S by a ∗ b = a + b + ab. Prove that (S, ∗) is an abelian group. 8. Give an example of two elements A and B in GL2 (R) with AB ̸= BA. 9. Prove that the product of two matrices in SL2 (R) has determinant one. 3.4. EXERCISES 39 10. Prove that the set of matrices of the form 1 x y 0 1 z 0 0 1 is a group under matrix multiplication. This group, known as the Heisenberg group, is important in quantum physics. Matrix multiplication in the Heisenberg group is defined by 1 x y 1 x′ y ′ 1 x + x′ y + y ′ + xz ′ 0 1 z 0 1 z ′ = 0 1 z + z′ . 0 0 1 0 0 1 0 0 1 11. Prove that det(AB) = det(A) det(B) in GL2 (R). Use this result to show that the binary operation in the group GL2 (R) is closed; that is, if A and B are in GL2 (R), then AB ∈ GL2 (R). 12. Let Zn2 = {(a1 , a2 , . . . , an ) : ai ∈ Z2 }. Define a binary operation on Zn2 by (a1 , a2 , . . . , an ) + (b1 , b2 , . . . , bn ) = (a1 + b1 , a2 + b2 , . . . , an + bn ). Prove that Zn2 is a group under this operation. This group is important in algebraic coding theory. 13. Show that R∗ = R \ {0} is a group under the operation of multiplication. 14. Given the groups R∗ and Z, let G = R∗ × Z. Define a binary operation ◦ on G by (a, m) ◦ (b, n) = (ab, m + n). Show that G is a group under this operation. 15. Prove or disprove that every group containing six elements is abelian. 16. Give a specific example of some group G and elements g, h ∈ G where (gh)n ̸= g n hn . 17. Give an example of three different groups with eight elements. Why are the groups different? 18. Show that there are n! permutations of a set containing n items. 19. Show that 0 + a ≡ a + 0 ≡ a (mod n) for all a ∈ Zn . 20. Prove that there is a multiplicative identity for the integers modulo n: a · 1 ≡ a (mod n). 21. For each a ∈ Zn find an element b ∈ Zn such that a + b ≡ b + a ≡ 0 (mod n). 22. Show that addition and multiplication mod n are well defined operations. That is, show that the operations do not depend on the choice of the representative from the equivalence classes mod n. 23. Show that addition and multiplication mod n are associative operations. 24. Show that multiplication distributes over addition modulo n: a(b + c) ≡ ab + ac (mod n). 25. Let a and b be elements in a group G. Prove that abn a−1 = (aba−1 )n for n ∈ Z. 40 CHAPTER 3. GROUPS 26. Let U (n) be the group of units in Zn . If n > 2, prove that there is an element k ∈ U (n) such that k 2 = 1 and k ̸= 1. −1 27. Prove that the inverse of g1 g2 · · · gn is gn−1 gn−1 · · · g1−1 . 28. Prove the remainder of Proposition 3.21: if G is a group and a, b ∈ G, then the equation xa = b has a unique solution in G. 29. Prove Theorem 3.23. 30. Prove the right and left cancellation laws for a group G; that is, show that in the group G, ba = ca implies b = c and ab = ac implies b = c for elements a, b, c ∈ G. 31. Show that if a2 = e for all elements a in a group G, then G must be abelian. 32. Show that if G is a finite group of even order, then there is an a ∈ G such that a is not the identity and a2 = e. 33. Let G be a group and suppose that (ab)2 = a2 b2 for all a and b in G. Prove that G is an abelian group. 34. Find all the subgroups of Z3 × Z3 . Use this information to show that Z3 × Z3 is not the same group as Z9 . (See Example 3.28 for a short description of the product of groups.) 35. Find all the subgroups of the symmetry group of an equilateral triangle. 36. Compute the subgroups of the symmetry group of a square. 37. Let H = {2k : k ∈ Z}. Show that H is a subgroup of Q∗ . 38. Let n = 0, 1, 2, . . . and nZ = {nk : k ∈ Z}. Prove that nZ is a subgroup of Z. Show that these subgroups are the only subgroups of Z. 39. Let T = {z ∈ C∗ : |z| = 1}. Prove that T is a subgroup of C∗ . 40. Let G consist of the 2 × 2 matrices of the form ( ) cos θ − sin θ , sin θ cos θ where θ ∈ R. Prove that G is a subgroup of SL2 (R). 41. Prove that √ G = {a + b 2 : a, b ∈ Q and a and b are not both zero} is a subgroup of R∗ under the group operation of multiplication. 42. Let G be the group of 2 × 2 matrices under addition and {( ) } a b H= :a+d=0 . c d Prove that H is a subgroup of G. 43. Prove or disprove: SL2 (Z), the set of 2 × 2 matrices with integer entries and deter- minant one, is a subgroup of SL2 (R). 44. List the subgroups of the quaternion group, Q8 . 45. Prove that the intersection of two subgroups of a group G is also a subgroup of G. 46. Prove or disprove: If H and K are subgroups of a group G, then H ∪ K is a subgroup of G. 47. Prove or disprove: If H and K are subgroups of a group G, then HK = {hk : h ∈ H and k ∈ K} is a subgroup of G. What if G is abelian? 3.5. ADDITIONAL EXERCISES: DETECTING ERRORS 41 48. Let G be a group and g ∈ G. Show that Z(G) = {x ∈ G : gx = xg for all g ∈ G} is a subgroup of G. This subgroup is called the center of G. 49. Let a and b be elements of a group G. If a4 b = ba and a3 = e, prove that ab = ba. 50. Give an example of an infinite group in which every nontrivial subgroup is infinite. 51. If xy = x−1 y −1 for all x and y in G, prove that G must be abelian. 52. Prove or disprove: Every proper subgroup of an nonabelian group is nonabelian. 53. Let H be a subgroup of G and C(H) = {g ∈ G : gh = hg for all h ∈ H}. Prove C(H) is a subgroup of G. This subgroup is called the centralizer of H in G. 54. Let H be a subgroup of G. If g ∈ G, show that gHg −1 = {ghg −1 : h ∈ H} is also a subgroup of G. 3.5 Additional Exercises: Detecting Errors 1. UPC Symbols. Universal Product Code (upc) symbols are found on most products in grocery and retail stores. The upc symbol is a 12-digit code identifying the manufacturer of a product and the product itself (Figure 3.32). The first 11 digits contain information about the product; the twelfth digit is used for error detection. If d1 d2 · · · d12 is a valid upc number, then 3 · d1 + 1 · d2 + 3 · d3 + · · · + 3 · d11 + 1 · d12 ≡ 0 (mod 10). (a) Show that the upc number 0-50000-30042-6, which appears in Figure 3.32, is a valid upc number. (b) Show that the number 0-50000-30043-6 is not a valid upc number. (c) Write a formula to calculate the check digit, d12 , in the upc number. (d) The upc error detection scheme can detect most transposition errors; that is, it can determine if two digits have been interchanged. Show that the transposition error 0-05000-30042-6 is not detected. Find a transposition error that is detected. Can you find a general rule for the types of transposition errors that can be detected? (e) Write a program that will determine whether or not a upc number is valid. 42 CHAPTER 3. GROUPS Figure 3.32: A upc code 2. It is often useful to use an inner product notation for this type of error detection scheme; hence, we will use the notion (d1 , d2 , . . . , dk ) · (w1 , w2 , . . . , wk ) ≡ 0 (mod n) to mean d1 w1 + d2 w2 + · · · + dk wk ≡ 0 (mod n). Suppose that (d1 , d2 , . . . , dk ) · (w1 , w2 , . . . , wk ) ≡ 0 (mod n) is an error detection scheme for the k-digit identification number d1 d2 · · · dk , where 0 ≤ di < n. Prove that all single-digit errors are detected if and only if gcd(wi , n) = 1 for 1 ≤ i ≤ k. 3. Let (d1 , d2 , . . . , dk ) · (w1 , w2 , . . . , wk ) ≡ 0 (mod n) be an error detection scheme for the k-digit identification number d1 d2 · · · dk , where 0 ≤ di < n. Prove that all transposition errors of two digits di and dj are detected if and only if gcd(wi − wj , n) = 1 for i and j between 1 and k. 4. ISBN Codes. Every book has an International Standard Book Number (isbn) code. This is a 10-digit code indicating the book’s publisher and title. The tenth digit is a check digit satisfying (d1 , d2 , . . . , d10 ) · (10, 9, . . . , 1) ≡ 0 (mod 11). One problem is that d10 might have to be a 10 to make the inner product zero; in this case, 11 digits would be needed to make this scheme work. Therefore, the character X is used for the eleventh digit. So isbn 3-540-96035-X is a valid isbn code. (a) Is isbn 0-534-91500-0 a valid isbn code? What about isbn 0-534-91700-0 and isbn 0-534-19500-0? (b) Does this method detect all single-digit errors? What about all transposition errors? (c) How many different isbn codes are there? (d) Write a computer program that will calculate the check digit for the first nine digits of an isbn code. (e) A publisher has houses in Germany and the United States. Its German prefix is 3-540. If its United States prefix will be 0-abc, find abc such that the rest of the isbn code will be the same for a book printed in Germany and in the United States. Under the 3.5. ADDITIONAL EXERCISES: DETECTING ERRORS 43 isbn coding method the first digit identifies the language; German is 3 and English is 0. The next group of numbers identifies the publisher, and the last group identifies the specific book. References and Suggested Readings [1] Burnside, W. Theory of Groups of Finite Order. 2nd ed. Cambridge University Press, Cambridge, 1911; Dover, New York, 1953. A classic. Also available at books.google.com. [2] Gallian, J. A. and Winters, S. “Modular Arithmetic in the Marketplace,” The Amer- ican Mathematical Monthly 95 (1988): 548–51. [3] Gallian, J. A. Contemporary Abstract Algebra. 7th ed. Brooks/Cole, Belmont, CA, 2009. [4] Hall, M. Theory of Groups. 2nd ed. American Mathematical Society, Providence, 1959. [5] Kurosh, A. E. The Theory of Groups, vols. I and II. American Mathematical Society, Providence, 1979. [6] Rotman, J. J. An Introduction to the Theory of Groups. 4th ed. Springer, New York, 1995. 4 Cyclic Groups The groups Z and Zn , which are among the most familiar and easily understood groups, are both examples of what are called cyclic groups. In this chapter we will study the properties of cyclic groups and cyclic subgroups, which play a fundamental part in the classification of all abelian groups. 4.1 Cyclic Subgroups Often a subgroup will depend entirely on a single element of the group; that is, knowing that particular element will allow us to compute any other element in the subgroup. Example 4.1. Suppose that we consider 3 ∈ Z and look at all multiples (both positive and negative) of 3. As a set, this is 3Z = {. . . , −3, 0, 3, 6, . . .}. It is easy to see that 3Z is a subgroup of the integers. This subgroup is completely deter- mined by the element 3 since we can obtain all of the other elements of the group by taking multiples of 3. Every element in the subgroup is “generated” by 3. Example 4.2. If H = {2n : n ∈ Z}, then H is a subgroup of the multiplicative group of nonzero rational numbers, Q∗ . If a = 2m and b = 2n are in H, then ab−1 = 2m 2−n = 2m−n is also in H. By Proposition 3.31, H is a subgroup of Q∗ determined by the element 2. Theorem 4.3. Let G be a group and a be any element in G. Then the set ⟨a⟩ = {ak : k ∈ Z} is a subgroup of G. Furthermore, ⟨a⟩ is the smallest subgroup of G that contains a. Proof. The identity is in ⟨a⟩ since a0 = e. If g and h are any two elements in ⟨a⟩, then by the definition of ⟨a⟩ we can write g = am and h = an for some integers m and n. So gh = am an = am+n is again in ⟨a⟩. Finally, if g = an in ⟨a⟩, then the inverse g −1 = a−n is also in ⟨a⟩. Clearly, any subgroup H of G containing a must contain all the powers of a by closure; hence, H contains ⟨a⟩. Therefore, ⟨a⟩ is the smallest subgroup of G containing a. Remark 4.4. If we are using the “+” notation, as in the case of the integers under addition, we write ⟨a⟩ = {na : n ∈ Z}. For a ∈ G, we call ⟨a⟩ the cyclic subgroup generated by a. If G contains some element a such that G = ⟨a⟩, then G is a cyclic group. In this case a is a generator of G. If a is an element of a group G, we define the order of a to be the smallest positive integer n such that an = e, and we write |a| = n. If there is no such integer n, we say that the order of a is infinite and write |a| = ∞ to denote the order of a. 44 4.1. CYCLIC SUBGROUPS 45 Example 4.5. Notice that a cyclic group can have more than a single generator. Both 1 and 5 generate Z6 ; hence, Z6 is a cyclic group. Not every element in a cyclic group is necessarily a generator of the group. The order of 2 ∈ Z6 is 3. The cyclic subgroup generated by 2 is ⟨2⟩ = {0, 2, 4}. The groups Z and Zn are cyclic groups. The elements 1 and −1 are generators for Z. We can certainly generate Zn with 1 although there may be other generators of Zn , as in the case of Z6 . Example 4.6. The group of units, U (9), in Z9 is a cyclic group. As a set, U (9) is {1, 2, 4, 5, 7, 8}. The element 2 is a generator for U (9) since 21 = 2 22 = 4 23 = 8 24 = 7 25 = 5 26 = 1. Example 4.7. Not every group is a cyclic group. Consider the symmetry group of an equilateral triangle S3 . The multiplication table for this group is Table 3.7. The subgroups of S3 are shown in Figure 4.8. Notice that every subgroup is cyclic; however, no single element generates the entire group. S3 {id, ρ1 , ρ2 } {id, µ1 } {id, µ2 } {id, µ3 } {id} Figure 4.8: Subgroups of S3 Theorem 4.9. Every cyclic group is abelian. Proof. Let G be a cyclic group and a ∈ G be a generator for G. If g and h are in G, then they can be written as powers of a, say g = ar and h = as . Since gh = ar as = ar+s = as+r = as ar = hg, G is abelian. Subgroups of Cyclic Groups We can ask some interesting questions about cyclic subgroups of a group and subgroups of a cyclic group. If G is a group, which subgroups of G are cyclic? If G is a cyclic group, what type of subgroups does G possess? Theorem 4.10. Every subgroup of a cyclic group is cyclic. Proof. The main tools used in this proof are the division algorithm and the Principle of Well-Ordering. Let G be a cyclic group generated by a and suppose that H is a subgroup of G. If H = {e}, then trivially H is cyclic. Suppose that H contains some other element g distinct from the identity. Then g can be written as an for some integer n. Since H is a 46 CHAPTER 4. CYCLIC GROUPS subgroup, g −1 = a−n must also be in H. Since either n or −n is positive, we can assume that H contains positive powers of a and n > 0. Let m be the smallest natural number such that am ∈ H. Such an m exists by the Principle of Well-Ordering. We claim that h = am is a generator for H. We must show that every h′ ∈ H can be written as a power of h. Since h′ ∈ H and H is a subgroup of G, h′ = ak for some integer k. Using the division algorithm, we can find numbers q and r such that k = mq + r where 0 ≤ r < m; hence, ak = amq+r = (am )q ar = hq ar . So ar = ak h−q . Since ak and h−q are in H, ar must also be in H. However, m was the smallest positive number such that am was in H; consequently, r = 0 and so k = mq. Therefore, h′ = ak = amq = hq and H is generated by h. Corollary 4.11. The subgroups of Z are exactly nZ for n = 0, 1, 2, . . .. Proposition 4.12. Let G be a cyclic group of order n and suppose that a is a generator for G. Then ak = e if and only if n divides k. Proof. First suppose that ak = e. By the division algorithm, k = nq +r where 0 ≤ r < n; hence, e = ak = anq+r = anq ar = ear = ar . Since the smallest positive integer m such that am = e is n, r = 0. Conversely, if n divides k, then k = ns for some integer s. Consequently, ak = ans = (an )s = es = e. Theorem 4.13. Let G be a cyclic group of order n and suppose that a ∈ G is a generator of the group. If b = ak , then the order of b is n/d, where d = gcd(k, n). Proof. We wish to find the smallest integer m such that e = bm = akm . By Proposi- tion 4.12, this is the smallest integer m such that n divides km or, equivalently, n/d divides m(k/d). Since d is the greatest common divisor of n and k, n/d and k/d are relatively prime. Hence, for n/d to divide m(k/d) it must divide m. The smallest such m is n/d. Corollary 4.14. The generators of Zn are the integers r such that 1 ≤ r < n and gcd(r, n) = 1. Example 4.15. Let us examine the group Z16 . The numbers 1, 3, 5, 7, 9, 11, 13, and 15 are the elements of Z16 that are relatively prime to 16. Each of these elements generates Z16 . For example, 1·9=9 2·9=2 3 · 9 = 11 4·9=4 5 · 9 = 13 6·9=6 7 · 9 = 15 8·9=8 9·9=1 10 · 9 = 10 11 · 9 = 3 12 · 9 = 12 13 · 9 = 5 14 · 9 = 14 15 · 9 = 7. 4.2. MULTIPLICATIVE GROUP OF COMPLEX NUMBERS 47 4.2 Multiplicative Group of Complex Numbers The complex numbers are defined as C = {a + bi : a, b ∈ R}, where i2 = −1. If z = a + bi, then a is the real part of z and b is the imaginary part of z. To add two complex numbers z = a + bi and w = c + di, we just add the corresponding real and imaginary parts: z + w = (a + bi) + (c + di) = (a + c) + (b + d)i. Remembering that i2 = −1, we multiply complex numbers just like polynomials. The product of z and w is (a + bi)(c + di) = ac + bdi2 + adi + bci = (ac − bd) + (ad + bc)i. Every nonzero complex number z = a + bi has a multiplicative inverse; that is, there exists a z −1 ∈ C∗ such that zz −1 = z −1 z = 1. If z = a + bi, then a − bi z −1 = . a2 + b2 The complex conjugate of a complex number z =√a + bi is defined to be z = a − bi. The absolute value or modulus of z = a + bi is |z| = a2 + b2 . Example 4.16. Let z = 2 + 3i and w = 1 − 2i. Then z + w = (2 + 3i) + (1 − 2i) = 3 + i and zw = (2 + 3i)(1 − 2i) = 8 − i. Also, 2 3 z −1 = − i 13 √ 13 |z| = 13 z = 2 − 3i. y z1 = 2 + 3i z3 = −3 + 2i 0 x z2 = 1 − 2i Figure 4.17: Rectangular coordinates of a complex number 48 CHAPTER 4. CYCLIC GROUPS There are several ways of graphically representing complex numbers. We can represent a complex number z = a + bi as an ordered pair on the xy plane where a is the x (or real) coordinate and b is the y (or imaginary) coordinate. This is called the rectangular or Cartesian representation. The rectangular representations of z1 = 2 + 3i, z2 = 1 − 2i, and z3 = −3 + 2i are depicted in Figure 4.17. y a + bi r θ 0 x Figure 4.18: Polar coordinates of a complex number Nonzero complex numbers can also be represented using polar coordinates. To specify any nonzero point on the plane, it suffices to give an angle θ from the positive x axis in the counterclockwise direction and a distance r from the origin, as in Figure 4.18. We can see that z = a + bi = r(cos θ + i sin θ). Hence, √ r = |z| = a2 + b2 and a = r cos θ b = r sin θ. We sometimes abbreviate r(cos θ + i sin θ) as r cis θ. To assure that the representation of z is well-defined, we also require that 0◦ ≤ θ < 360◦ . If the measurement is in radians, then 0 ≤ θ < 2π. Example 4.19. Suppose that z = 2 cis 60◦ . Then a = 2 cos 60◦ = 1 and √ b = 2 sin 60◦ = 3. √ Hence, the rectangular representation is z = 1 + 3 i. Conversely, if we are given a rectangular representation √ of a complex √ number, it is often useful to know the number’s polar representation. If z = 3 2 − 3 2 i, then √ √ r = a2 + b2 = 36 = 6 and ( ) b θ = arctan = arctan(−1) = 315◦ , a √ √ so 3 2 − 3 2 i = 6 cis 315◦ . 4.2. MULTIPLICATIVE GROUP OF COMPLEX NUMBERS 49 The polar representation of a complex number makes it easy to find products and powers of complex numbers. The proof of the following proposition is straightforward and is left as an exercise. Proposition 4.20. Let z = r cis θ and w = s cis ϕ be two nonzero complex numbers. Then zw = rs cis(θ + ϕ). Example 4.21. If z = 3 cis(π/3) and w = 2 cis(π/6), then zw = 6 cis(π/2) = 6i. Theorem 4.22 DeMoivre. Let z = r cis θ be a nonzero complex number. Then [r cis θ]n = rn cis(nθ) for n = 1, 2, . . .. Proof. We will use induction on n. For n = 1 the theorem is trivial. Assume that the theorem is true for all k such that 1 ≤ k ≤ n. Then z n+1 = z n z = rn (cos nθ + i sin nθ)r(cos θ + i sin θ) = rn+1 [(cos nθ cos θ − sin nθ sin θ) + i(sin nθ cos θ + cos nθ sin θ)] = rn+1 [cos(nθ + θ) + i sin(nθ + θ)] = rn+1 [cos(n + 1)θ + i sin(n + 1)θ]. Example 4.23. Suppose that z = 1+i and we wish to compute z 10 . Rather than computing (1 + i)10 directly, it is much easier to switch to polar coordinates and calculate z 10 using DeMoivre’s Theorem: z 10 = (1 + i)10 (√ ( π ))10 = 2 cis 4( ) √ 10 5π = ( 2 ) cis 2 (π ) = 32 cis 2 = 32i. The Circle Group and the Roots of Unity The multiplicative group of the complex numbers, C∗ , possesses some interesting subgroups. Whereas Q∗ and R∗ have no interesting subgroups of finite order, C∗ has many. We first consider the circle group, T = {z ∈ C : |z| = 1}. The following proposition is a direct result of Proposition 4.20. Proposition 4.24. The circle group is a subgroup of C∗ . Although the circle group has infinite order, it has many interesting finite subgroups. Suppose that H = {1, −1, i, −i}. Then H is a subgroup of the circle group. Also, 1, −1, i, and −i are exactly those complex numbers that satisfy the equation z 4 = 1. The complex numbers satisfying the equation z n = 1 are called the nth roots of unity. 50 CHAPTER 4. CYCLIC GROUPS Theorem 4.25. If z n = 1, then the nth roots of unity are ( ) 2kπ z = cis , n where k = 0, 1, . . . , n − 1. Furthermore, the nth roots of unity form a cyclic subgroup of T of order n Proof. By DeMoivre’s Theorem, ( ) 2kπ z n = cis n = cis(2kπ) = 1. n The z’s are distinct since the numbers 2kπ/n are all distinct and are greater than or equal to 0 but less than 2π. The fact that these are all of the roots of the equation z n = 1 follows from from Corollary 17.9, which states that a polynomial of degree n can have at most n roots. We will leave the proof that the nth roots of unity form a cyclic subgroup of T as an exercise. A generator for the group of the nth roots of unity is called a primitive nth root of unity. Example 4.26. The 8th roots of unity can be represented as eight equally spaced points on the unit circle (Figure 4.27). The primitive 8th roots of unity are √ √ 2 2 ω= + i 2√ 2√ 2 2 ω3 = − + i √2 √2 2 2 ω5 = − − i √ 2 √ 2 2 2 7 ω = − i. 2 2 y i ω3 ω −1 0 1 x ω5 ω7 −i Figure 4.27: 8th roots of unity 4.3 The Method of Repeated Squares Computing large powers can be very time-consuming. Just as anyone can compute 22 or 28 , everyone knows how to compute 1,000,000 22 . 4.3. THE METHOD OF REPEATED SQUARES 51 However, such numbers are so large that we do not want to attempt the calculations; moreover, past a certain point the computations would not be feasible even if we had every computer in the world at our disposal. Even writing down the decimal representation of a very large number may not be reasonable. It could be thousands or even millions of digits long. However, if we could compute something like 237,398,332 (mod 46,389), we could very easily write the result down since it would be a number between 0 and 46,388. If we want to compute powers modulo n quickly and efficiently, we will have to be clever.1 The first thing to notice is that any number a can be written as the sum of distinct powers of 2; that is, we can write a = 2k1 + 2k2 + · · · + 2kn , where k1 < k2 < · · · < kn . This is just the binary representation of a. For example, the binary representation of 57 is 111001, since we can write 57 = 20 + 23 + 24 + 25 . The laws of exponents still work in Zn ; that is, if b ≡ ax (mod n) and c ≡ ay (mod n), k then bc ≡ ax+y (mod n). We can compute a2 (mod n) in k multiplications by computing 0 a2 (mod n) 21 a (mod n) .. . k a2 (mod n). Each step involves squaring the answer obtained in the previous step, dividing by n, and taking the remainder. Example 4.28. We will compute 271321 (mod 481). Notice that 321 = 20 + 26 + 28 ; hence, computing 271321 (mod 481) is the same as computing 0 +26 +28 0 6 8 2712 ≡ 2712 · 2712 · 2712 (mod 481). i So it will suffice to compute 2712 (mod 481) where i = 0, 6, 8. It is very easy to see that 1 2712 = 73,441 ≡ 329 (mod 481). 2 We can square this result to obtain a value for 2712 (mod 481): 2 1 2712 ≡ (2712 )2 (mod 481) ≡ (329)2 (mod 481) ≡ 108,241 (mod 481) ≡ 16 (mod 481). n n n+1 We are using the fact that (a2 )2 ≡ a2·2 ≡ a2 (mod n). Continuing, we can calculate 6 2712 ≡ 419 (mod 481) 1 The results in this section are needed only in Chapter 7 52 CHAPTER 4. CYCLIC GROUPS and 8 2712 ≡ 16 (mod 481). Therefore, 0 +26 +28 271321 ≡ 2712 (mod 481) 20 26 8 ≡ 271 · 271 · 2712 (mod 481) ≡ 271 · 419 · 16 (mod 481) ≡ 1,816,784 (mod 481) ≡ 47 (mod 481). The method of repeated squares will prove to be a very useful tool when we explore rsa cryptography in Chapter 7. To encode and decode messages in a reasonable manner under this scheme, it is necessary to be able to quickly compute large powers of integers mod n. Sage Sage support for cyclic groups is a little spotty — but we can still make effective use of Sage and perhaps this situation could change soon. 4.4 Exercises 1. Prove or disprove each of the following statements. (a) All of the generators of Z60 are prime. (b) U (8) is cyclic. (c) Q is cyclic. (d) If every proper subgroup of a group G is cyclic, then G is a cyclic group. (e) A group with a finite number of subgroups is finite. 2. Find the order of each of the following elements. (a) 5 ∈ Z12 (d) −i ∈ C∗ √ (b) 3 ∈ R (e) 72 ∈ Z240 √ (c) 3 ∈ R∗ (f) 312 ∈ Z471 3. List all of the elements in each of the following subgroups. (a) The subgroup of Z generated by 7 (b) The subgroup of Z24 generated by 15 (c) All subgroups of Z12 (d) All subgroups of Z60 (e) All subgroups of Z13 (f) All subgroups of Z48 (g) The subgroup generated by 3 in U (20) 4.4. EXERCISES 53 (h) The subgroup generated by 5 in U (18) (i) The subgroup of R∗ generated by 7 (j) The subgroup of C∗ generated by i where i2 = −1 (k) The subgroup of C∗ generated by 2i √ (l) The subgroup of C∗ generated by (1 + i)/ 2 √ (m) The subgroup of C∗ generated by (1 + 3 i)/2 4. Find the subgroups of GL2 (R) generated by each of the following matrices. ( ) ( ) ( ) 0 1 1 −1 1 −1 (a) (c) (e) −1 0 1 0 −1 0 ( ) ( ) (√ ) 0 1/3 1 −1 3/2 1/2 (b) (d) (f) √ 3 0 0 1 −1/2 3/2 5. Find the order of every element in Z18 . 6. Find the order of every element in the symmetry group of the square, D4 . 7. What are all of the cyclic subgroups of the quaternion group, Q8 ? 8. List all of the cyclic subgroups of U (30). 9. List every generator of each subgroup of order 8 in Z32 . 10. Find all elements of finite order in each of the following groups. Here the “∗” indicates the set with zero removed. (a) Z (b) Q∗ (c) R∗ 11. If a24 = e in a group G, what are the possible orders of a? 12. Find a cyclic group with exactly one generator. Can you find cyclic groups with exactly two generators? Four generators? How about n generators? 13. For n ≤ 20, which groups U (n) are cyclic? Make a conjecture as to what is true in general. Can you prove your conjecture? 14. Let ( ) ( ) 0 1 0 −1 A= and B= −1 0 1 −1 be elements in GL2 (R). Show that A and B have finite orders but AB does not. 15. Evaluate each of the following. (a) (3 − 2i) + (5i − 6) (d) (9 − i)(9 − i) (b) (4 − 5i) − (4i − 4) (e) i45 (c) (5 − 4i)(7 + 2i) (f) (1 + i) + (1 + i) 16. Convert the following complex numbers to the form a + bi. 54 CHAPTER 4. CYCLIC GROUPS (a) 2 cis(π/6) (c) 3 cis(π) (b) 5 cis(9π/4) (d) cis(7π/4)/2 17. Change the following complex numbers to polar representation. (a) 1 − i (c) 2 + 2i (e) −3i √ √ (b) −5 (d) 3 + i (f) 2i + 2 3 18. Calculate each of the following expressions. (a) (1 + i)−1 (e) ((1 − i)/2)4 (b) (1 − i)6 √ √ √ (f) (− 2 − 2 i)12 (c) ( 3 + i)5 (d) (−i)10 (g) (−2 + 2i)−5 19. Prove each of the following statements. (a) |z| = |z| (d) |z + w| ≤ |z| + |w| (b) zz = |z|2 (e) |z − w| ≥ ||z| − |w|| (c) z −1 = z/|z|2 (f) |zw| = |z||w| 20. List and graph the 6th roots of unity. What are the generators of this group? What are the primitive 6th roots of unity? 21. List and graph the 5th roots of unity. What are the generators of this group? What are the primitive 5th roots of unity? 22. Calculate each of the following. (a) 2923171 (mod 582) (c) 20719521 (mod 4724) (b) 2557341 (mod 5681) (d) 971321 (mod 765) 23. Let a, b ∈ G. Prove the following statements. (a) The order of a is the same as the order of a−1 . (b) For all g ∈ G, |a| = |g −1 ag|. (c) The order of ab is the same as the order of ba. 24. Let p and q be distinct primes. How many generators does Zpq have? 25. Let p be prime and r be a positive integer. How many generators does Zpr have? 26. Prove that Zp has no nontrivial subgroups if p is prime. 27. If g and h have orders 15 and 16 respectively in a group G, what is the order of ⟨g⟩ ∩ ⟨h⟩? 28. Let a be an element in a group G. What is a generator for the subgroup ⟨am ⟩ ∩ ⟨an ⟩? 29. Prove that Zn has an even number of generators for n > 2. 4.5. PROGRAMMING EXERCISES 55 30. Suppose that G is a group and let a, b ∈ G. Prove that if |a| = m and |b| = n with gcd(m, n) = 1, then ⟨a⟩ ∩ ⟨b⟩ = {e}. 31. Let G be an abelian group. Show that the elements of finite order in G form a subgroup. This subgroup is called the torsion subgroup of G. 32. Let G be a finite cyclic group of order n generated by x. Show that if y = xk where gcd(k, n) = 1, then y must be a generator of G. 33. If G is an abelian group that contains a pair of cyclic subgroups of order 2, show that G must contain a subgroup of order 4. Does this subgroup have to be cyclic? 34. Let G be an abelian group of order pq where gcd(p, q) = 1. If G contains elements a and b of order p and q respectively, then show that G is cyclic. 35. Prove that the subgroups of Z are exactly nZ for n = 0, 1, 2, . . .. 36. Prove that the generators of Zn are the integers r such that 1 ≤ r < n and gcd(r, n) = 1. 37. Prove that if G has no proper nontrivial subgroups, then G is a cyclic group. 38. Prove that the order of an element in a cyclic group G must divide the order of the group. 39. Prove that if G is a cyclic group of order m and d | m, then G must have a subgroup of order d. 40. For what integers n is −1 an nth root of unity? 41. If z = r(cos θ + i sin θ) and w = s(cos ϕ + i sin ϕ) are two nonzero complex numbers, show that zw = rs[cos(θ + ϕ) + i sin(θ + ϕ)]. 42. Prove that the circle group is a subgroup of C∗ . 43. Prove that the nth roots of unity form a cyclic subgroup of T of order n. 44. Let α ∈ T. Prove that αm = 1 and αn = 1 if and only if αd = 1 for d = gcd(m, n). 45. Let z ∈ C∗ . If |z| ̸= 1, prove that the order of z is infinite. 46. Let z = cos θ + i sin θ be in T where θ ∈ Q. Prove that the order of z is infinite. 4.5 Programming Exercises 1. Write a computer program that will write any decimal number as the sum of distinct powers of 2. What is the largest integer that your program will handle? 2. Write a computer program to calculate ax (mod n) by the method of repeated squares. What are the largest values of n and x that your program will accept? References and Suggested Readings [1] Koblitz, N. A Course in Number Theory and Cryptography. 2nd ed. Springer, New York, 1994. [2] Pomerance, C. “Cryptology and Computational Number Theory—An Introduction,” in Cryptology and Computational Number Theory, Pomerance, C., ed. Proceedings of Symposia in Applied Mathematics, vol. 42, American Mathematical Society, Provi- dence, RI, 1990. Thisbook gives an excellent account of how the method of repeated squares is used in cryptography. 5 Permutation Groups Permutation groups are central to the study of geometric symmetries and to Galois the- ory, the study of finding solutions of polynomial equations. They also provide abundant examples of nonabelian groups. Let us recall for a moment the symmetries of the equilateral triangle △ABC from Chapter 3. The symmetries actually consist of permutations of the three vertices, where a permutation of the set S = {A, B, C} is a one-to-one and onto map π : S → S. The three vertices have the following six permutations. ( ) ( ) ( ) A B C A B C A B C A B C C A B B C A ( ) ( ) ( ) A B C A B C A B C A C B C B A B A C We have used the array ( ) A B C B C A to denote the permutation that sends A to B, B to C, and C to A. That is, A 7→ B B 7→ C C 7→ A. The symmetries of a triangle form a group. In this chapter we will study groups of this type. 5.1 Definitions and Notation In general, the permutations of a set X form a group SX . If X is a finite set, we can assume X = {1, 2, . . . , n}. In this case we write Sn instead of SX . The following theorem says that Sn is a group. We call this group the symmetric group on n letters. Theorem 5.1. The symmetric group on n letters, Sn , is a group with n! elements, where the binary operation is the composition of maps. Proof. The identity of Sn is just the identity map that sends 1 to 1, 2 to 2, . . ., n to n. If f : Sn → Sn is a permutation, then f −1 exists, since f is one-to-one and onto; hence, every permutation has an inverse. Composition of maps is associative, which makes the group operation associative. We leave the proof that |Sn | = n! as an exercise. 56 5.1. DEFINITIONS AND NOTATION 57 A subgroup of Sn is called a permutation group. Example 5.2. Consider the subgroup G of S5 consisting of the identity permutation id and the permutations ( ) 1 2 3 4 5 σ= 1 2 3 5 4 ( ) 1 2 3 4 5 τ= 3 2 1 4 5 ( ) 1 2 3 4 5 µ= . 3 2 1 5 4 The following table tells us how to multiply elements in the permutation group G. ◦ id σ τ µ id id σ τ µ σ σ id µ τ τ τ µ id σ µ µ τ σ id Remark 5.3. Though it is natural to multiply elements in a group from left to right, functions are composed from right to left. Let σ and τ be permutations on a set X. To compose σ and τ as functions, we calculate (σ ◦ τ )(x) = σ(τ (x)). That is, we do τ first, then σ. There are several ways to approach this inconsistency. We will adopt the convention of multiplying permutations right to left. To compute στ , do τ first and then σ. That is, by στ (x) we mean σ(τ (x)). (Another way of solving this problem would be to write functions on the right; that is, instead of writing σ(x), we could write (x)σ. We could also multiply permutations left to right to agree with the usual way of multiplying elements in a group. Certainly all of these methods have been used. Example 5.4. Permutation multiplication is not usually commutative. Let ( ) 1 2 3 4 σ= 4 1 2 3 ( ) 1 2 3 4 τ= . 2 1 4 3 Then ( ) 1 2 3 4 στ = , 1 4 3 2 but ( ) 1 2 3 4 τσ = . 3 2 1 4 Cycle Notation The notation that we have used to represent permutations up to this point is cumbersome, to say the least. To work effectively with permutation groups, we need a more streamlined method of writing down and manipulating permutations. A permutation σ ∈ SX is a cycle of length k if there exist elements a1 , a2 , . . . , ak ∈ X such that σ(a1 ) = a2 58 CHAPTER 5. PERMUTATION GROUPS σ(a2 ) = a3 .. . σ(ak ) = a1 and σ(x) = x for all other elements x ∈ X. We will write (a1 , a2 , . . . , ak ) to denote the cycle σ. Cycles are the building blocks of all permutations. Example 5.5. The permutation ( ) 1 2 3 4 5 6 7 σ= = (162354) 6 3 5 1 4 2 7 is a cycle of length 6, whereas ( ) 1 2 3 4 5 6 τ= = (243) 1 4 2 3 5 6 is a cycle of length 3. Not every permutation is a cycle. Consider the permutation ( ) 1 2 3 4 5 6 = (1243)(56). 2 4 1 3 6 5 This permutation actually contains a cycle of length 2 and a cycle of length 4. Example 5.6. It is very easy to compute products of cycles. Suppose that σ = (1352) and τ = (256). If we think of σ as 1 7→ 3, 3 7→ 5, 5 7→ 2, 2 7→ 1, and τ as 2 7→ 5, 5 7→ 6, 6 7→ 2, then for στ remembering that we apply τ first and then σ, it must be the case that 1 7→ 3, 3 7→ 5, 5 7→ 6, 6 7→ 2 7→ 1, or στ = (1356). If µ = (1634), then σµ = (1652)(34). Two cycles in SX , σ = (a1 , a2 , . . . , ak ) and τ = (b1 , b2 , . . . , bl ), are disjoint if ai ̸= bj for all i and j. Example 5.7. The cycles (135) and (27) are disjoint; however, the cycles (135) and (347) are not. Calculating their products, we find that (135)(27) = (135)(27) (135)(347) = (13475). The product of two cycles that are not disjoint may reduce to something less complicated; the product of disjoint cycles cannot be simplified. Proposition 5.8. Let σ and τ be two disjoint cycles in SX . Then στ = τ σ. 5.1. DEFINITIONS AND NOTATION 59 Proof. Let σ = (a1 , a2 , . . . , ak ) and τ = (b1 , b2 , . . . , bl ). We must show that στ (x) = τ σ(x) for all x ∈ X. If x is neither in {a1 , a2 , . . . , ak } nor {b1 , b2 , . . . , bl }, then both σ and τ fix x. That is, σ(x) = x and τ (x) = x. Hence, στ (x) = σ(τ (x)) = σ(x) = x = τ (x) = τ (σ(x)) = τ σ(x). Do not forget that we are multiplying permutations right to left, which is the opposite of the order in which we usually multiply group elements. Now suppose that x ∈ {a1 , a2 , . . . , ak }. Then σ(ai ) = a(i mod k)+1 ; that is, a1 7→ a2 a2 →7 a3 .. . ak−1 7→ ak ak 7→ a1 . However, τ (ai ) = ai since σ and τ are disjoint. Therefore, στ (ai ) = σ(τ (ai )) = σ(ai ) = a(i mod k)+1 = τ (a(i mod k)+1 ) = τ (σ(ai )) = τ σ(ai ). Similarly, if x ∈ {b1 , b2 , . . . , bl }, then σ and τ also commute. Theorem 5.9. Every permutation in Sn can be written as the product of disjoint cycles. Proof. We can assume that X = {1, 2, . . . , n}. If σ ∈ Sn and we define X1 to be {σ(1), σ 2 (1), . . .}, then the set X1 is finite since X is finite. Now let i be the first integer in X that is not in X1 and define X2 by {σ(i), σ 2 (i), . . .}. Again, X2 is a finite set. Continuing in this manner, we can define finite disjoint sets X3 , X4 , . . .. Since X is a finite set, we are guaranteed that this process will end and there will be only a finite number of these sets, say r. If σi is the cycle defined by { σ(x) x ∈ Xi σi (x) = x x∈ / Xi , then σ = σ1 σ2 · · · σr . Since the sets X1 , X2 , . . . , Xr are disjoint, the cycles σ1 , σ2 , . . . , σr must also be disjoint. Example 5.10. Let ( ) 1 2 3 4 5 6 σ= 6 4 3 1 5 2 ( ) 1 2 3 4 5 6 τ= . 3 2 1 5 6 4 Using cycle notation, we can write σ = (1624) 60 CHAPTER 5. PERMUTATION GROUPS τ = (13)(456) στ = (136)(245) τ σ = (143)(256). Remark 5.11. From this point forward we will find it convenient to use cycle notation to represent permutations. When using cycle notation, we often denote the identity permuta- tion by (1). Transpositions The simplest permutation is a cycle of length 2. Such cycles are called transpositions. Since (a1 , a2 , . . . , an ) = (a1 an )(a1 an−1 ) · · · (a1 a3 )(a1 a2 ), any cycle can be written as the product of transpositions, leading to the following proposi- tion. Proposition 5.12. Any permutation of a finite set containing at least two elements can be written as the product of transpositions. Example 5.13. Consider the permutation (16)(253) = (16)(23)(25) = (16)(45)(23)(45)(25). As we can see, there is no unique way to represent permutation as the product of transposi- tions. For instance, we can write the identity permutation as (12)(12), as (13)(24)(13)(24), and in many other ways. However, as it turns out, no permutation can be written as the product of both an even number of transpositions and an odd number of transpositions. For instance, we could represent the permutation (16) by (23)(16)(23) or by (35)(16)(13)(16)(13)(35)(56), but (16) will always be the product of an odd number of transpositions. Lemma 5.14. If the identity is written as the product of r transpositions, id = τ1 τ2 · · · τr , then r is an even number. Proof. We will employ induction on r. A transposition cannot be the identity; hence, r > 1. If r = 2, then we are done. Suppose that r > 2. In this case the product of the last two transpositions, τr−1 τr , must be one of the following cases: (ab)(ab) = id (bc)(ab) = (ac)(bc) (cd)(ab) = (ab)(cd) (ac)(ab) = (ab)(bc), where a, b, c, and d are distinct. The first equation simply says that a transposition is its own inverse. If this case occurs, delete τr−1 τr from the product to obtain id = τ1 τ2 · · · τr−3 τr−2 . 5.1. DEFINITIONS AND NOTATION 61 By induction r − 2 is even; hence, r must be even. In each of the other three cases, we can replace τr−1 τr with the right-hand side of the corresponding equation to obtain a new product of r transpositions for the identity. In this new product the last occurrence of a will be in the next-to-the-last transposition. We can continue this process with τr−2 τr−1 to obtain either a product of r − 2 transpositions or a new product of r transpositions where the last occurrence of a is in τr−2 . If the identity is the product of r − 2 transpositions, then again we are done, by our induction hypothesis; otherwise, we will repeat the procedure with τr−3 τr−2 . At some point either we will have two adjacent, identical transpositions canceling each other out or a will be shuffled so that it will appear only in the first transposition. However, the latter case cannot occur, because the identity would not fix a in this instance. Therefore, the identity permutation must be the product of r − 2 transpositions and, again by our induction hypothesis, we are done. Theorem 5.15. If a permutation σ can be expressed as the product of an even number of transpositions, then any other product of transpositions equaling σ must also contain an even number of transpositions. Similarly, if σ can be expressed as the product of an odd number of transpositions, then any other product of transpositions equaling σ must also contain an odd number of transpositions. Proof. Suppose that σ = σ1 σ2 · · · σm = τ1 τ2 · · · τn , where m is even. We must show that n is also an even number. The inverse of σ is σm · · · σ1 . Since id = σσm · · · σ1 = τ1 · · · τn σm · · · σ1 , n must be even by Lemma 5.14. The proof for the case in which σ can be expressed as an odd number of transpositions is left as an exercise. In light of Theorem 5.15, we define a permutation to be even if it can be expressed as an even number of transpositions and odd if it can be expressed as an odd number of transpositions. The Alternating Groups One of the most important subgroups of Sn is the set of all even permutations, An . The group An is called the alternating group on n letters. Theorem 5.16. The set An is a subgroup of Sn . Proof. Since the product of two even permutations must also be an even permutation, An is closed. The identity is an even permutation and therefore is in An . If σ is an even permutation, then σ = σ1 σ2 · · · σr , where σi is a transposition and r is even. Since the inverse of any transposition is itself, σ −1 = σr σr−1 · · · σ1 is also in An . Proposition 5.17. The number of even permutations in Sn , n ≥ 2, is equal to the number of odd permutations; hence, the order of An is n!/2. 62 CHAPTER 5. PERMUTATION GROUPS Proof. Let An be the set of even permutations in Sn and Bn be the set of odd permu- tations. If we can show that there is a bijection between these sets, they must contain the same number of elements. Fix a transposition σ in Sn . Since n ≥ 2, such a σ exists. Define λσ : An → Bn by λσ (τ ) = στ. Suppose that λσ (τ ) = λσ (µ). Then στ = σµ and so τ = σ −1 στ = σ −1 σµ = µ. Therefore, λσ is one-to-one. We will leave the proof that λσ is surjective to the reader. Example 5.18. The group A4 is the subgroup of S4 consisting of even permutations. There are twelve elements in A4 : (1) (12)(34) (13)(24) (14)(23) (123) (132) (124) (142) (134) (143) (234) (243). One of the end-of-chapter exercises will be to write down all the subgroups of A4 . You will find that there is no subgroup of order 6. Does this surprise you? Historical Note Lagrange first thought of permutations as functions from a set to itself, but it was Cauchy who developed the basic theorems and notation for permutations. He was the first to use cycle notation. Augustin-Louis Cauchy (1789–1857) was born in Paris at the height of the French Revolution. His family soon left Paris for the village of Arcueil to escape the Reign of Terror. One of the family’s neighbors there was Pierre-Simon Laplace (1749– 1827), who encouraged him to seek a career in mathematics. Cauchy began his career as a mathematician by solving a problem in geometry given to him by Lagrange. Cauchy wrote over 800 papers on such diverse topics as differential equations, finite groups, applied mathematics, and complex analysis. He was one of the mathematicians responsible for making calculus rigorous. Perhaps more theorems and concepts in mathematics have the name Cauchy attached to them than that of any other mathematician. 5.2 Dihedral Groups Another special type of permutation group is the dihedral group. Recall the symmetry group of an equilateral triangle in Chapter 3. Such groups consist of the rigid motions of a regular n-sided polygon or n-gon. For n = 3, 4, . . ., we define the nth dihedral group to be the group of rigid motions of a regular n-gon. We will denote this group by Dn . We can number the vertices of a regular n-gon by 1, 2, . . . , n (Figure 5.19). Notice that there are exactly n choices to replace the first vertex. If we replace the first vertex by k, then the second vertex must be replaced either by vertex k + 1 or by vertex k − 1; hence, there are 2n possible rigid motions of the n-gon. We summarize these results in the following theorem. 5.2. DIHEDRAL GROUPS 63 1 n 2 n−1 3 4 Figure 5.19: A regular n-gon Theorem 5.20. The dihedral group, Dn , is a subgroup of Sn of order 2n. 1 2 8 2 1 3 rotation 7 3 8 4 6 4 7 5 5 6 1 1 8 2 2 8 reflection 7 3 3 7 6 4 4 6 5 5 Figure 5.21: Rotations and reflections of a regular n-gon 1 1 6 2 2 6 5 3 3 5 4 4 1 1 5 2 2 5 4 3 3 4 Figure 5.22: Types of reflections of a regular n-gon Theorem 5.23. The group Dn , n ≥ 3, consists of all products of the two elements r and s, satisfying the relations rn = 1 64 CHAPTER 5. PERMUTATION GROUPS s2 = 1 srs = r−1 . Proof. The possible motions of a regular n-gon are either reflections or rotations (Fig- ure 5.21). There are exactly n possible rotations: 360◦ 360◦ 360◦ id, ,2 · , . . . , (n − 1) · . n n n We will denote the rotation 360◦ /n by r. The rotation r generates all of the other rotations. That is, 360◦ rk = k · . n Label the n reflections s1 , s2 , . . . , sn , where sk is the reflection that leaves vertex k fixed. There are two cases of reflections, depending on whether n is even or odd. If there are an even number of vertices, then two vertices are left fixed by a reflection, and s1 = sn/2+1 , s2 = sn/2+2 , . . . , sn/2 = sn . If there are an odd number of vertices, then only a single vertex is left fixed by a reflection and s1 , s2 , . . . , sn are distinct (Figure 5.22). In either case, the order of each sk is two. Let s = s1 . Then s2 = 1 and rn = 1. Since any rigid motion t of the n-gon replaces the first vertex by the vertex k, the second vertex must be replaced by either k + 1 or by k − 1. If the second vertex is replaced by k + 1, then t = rk . If the second vertex is replaced by k − 1, then t = srk . Hence, r and s generate Dn . That is, Dn consists of all finite products of r and s, Dn = {1, r, r2 , . . . , rn−1 , s, sr, sr2 , . . . , srn−1 }. We will leave the proof that srs = r−1 as an exercise. Example 5.24. The group of rigid motions of a square, D4 , consists of eight elements. With the vertices numbered 1, 2, 3, 4 (Figure 5.25), the rotations are r = (1234) r2 = (13)(24) r3 = (1432) r4 = (1) and the reflections are s1 = (24) s2 = (13). The order of D4 is 8. The remaining two elements are rs1 = (12)(34) r3 s1 = (14)(23). 5.2. DIHEDRAL GROUPS 65 1 2 4 3 Figure 5.25: The group D4 The Motion Group of a Cube We can investigate the groups of rigid motions of geometric objects other than a regular n-sided polygon to obtain interesting examples of permutation groups. Let us consider the group of rigid motions of a cube. One of the first questions that we can ask about this group is “what is its order?” A cube has 6 sides. If a particular side is facing upward, then there are four possible rotations of the cube that will preserve the upward-facing side. Hence, the order of the group is 6 · 4 = 24. We have just proved the following proposition. 1 2 4 3 3 4 2 1 Figure 5.26: The motion group of a cube Proposition 5.27. The group of rigid motions of a cube contains 24 elements. Theorem 5.28. The group of rigid motions of a cube is S4 . Proof. From Proposition 5.27, we already know that the motion group of the cube has 24 elements, the same number of elements as there are in S4 . There are exactly four diagonals in the cube. If we label these diagonals 1, 2, 3, and 4, we must show that the motion group of the cube will give us any permutation of the diagonals (Figure 5.26). If we can obtain all of these permutations, then S4 and the group of rigid motions of the cube must be the same. To obtain a transposition we can rotate the cube 180◦ about the axis joining the midpoints of opposite edges (Figure 5.29). There are six such axes, giving all transpositions in S4 . Since every element in S4 is the product of a finite number of transpositions, the motion group of a cube must be S4 . 66 CHAPTER 5. PERMUTATION GROUPS 1 2 2 1 4 3 4 3 3 4 3 4 2 1 1 2 Figure 5.29: Transpositions in the motion group of a cube Sage A permutation group is a very concrete representation of a group, and Sage support for permutations groups is very good — making Sage a natural place for beginners to learn about group theory. 5.3 Exercises 1. Write the following permutations in cycle notation. (a) (c) ( ) ( ) 1 2 3 4 5 1 2 3 4 5 2 4 1 5 3 3 5 1 4 2 (b) (d) ( ) ( ) 1 2 3 4 5 1 2 3 4 5 4 2 5 1 3 1 4 3 2 5 2. Compute each of the following. (a) (1345)(234) (i) (123)(45)(1254)−2 (b) (12)(1253) (j) (1254)100 (c) (143)(23)(24) (k) |(1254)| (d) (1423)(34)(56)(1324) (l) |(1254)2 | (e) (1254)(13)(25) (m) (12)−1 (f) (1254)(13)(25)2 (n) (12537)−1 (g) (1254)−1 (123)(45)(1254) (o) [(12)(34)(12)(47)]−1 (h) (1254)2 (123)(45) (p) [(1235)(467)]−1 3. Express the following permutations as products of transpositions and identify them as even or odd. (a) (14356) (d) (17254)(1423)(154632) (b) (156)(234) (e) (142637) (c) (1426)(142) 5.3. EXERCISES 67 4. Find (a1 , a2 , . . . , an )−1 . 5. List all of the subgroups of S4 . Find each of the following sets: (a) {σ ∈ S4 : σ(1) = 3} (b) {σ ∈ S4 : σ(2) = 2} (c) {σ ∈ S4 : σ(1) = 3 and σ(2) = 2}. Are any of these sets subgroups of S4 ? 6. Find all of the subgroups in A4 . What is the order of each subgroup? 7. Find all possible orders of elements in S7 and A7 . 8. Show that A10 contains an element of order 15. 9. Does A8 contain an element of order 26? 10. Find an element of largest order in Sn for n = 3, . . . , 10. 11. What are the possible cycle structures of elements of A5 ? What about A6 ? 12. Let σ ∈ Sn have order n. Show that for all integers i and j, σ i = σ j if and only if i ≡ j (mod n). 13. Let σ = σ1 · · · σm ∈ Sn be the product of disjoint cycles. Prove that the order of σ is the least common multiple of the lengths of the cycles σ1 , . . . , σm . 14. Using cycle notation, list the elements in D5 . What are r and s? Write every element as a product of r and s. 15. If the diagonals of a cube are labeled as Figure 5.26, to which motion of the cube does the permutation (12)(34) correspond? What about the other permutations of the diagonals? 16. Find the group of rigid motions of a tetrahedron. Show that this is the same group as A4 . 17. Prove that Sn is nonabelian for n ≥ 3. 18. Show that An is nonabelian for n ≥ 4. 19. Prove that Dn is nonabelian for n ≥ 3. 20. Let σ ∈ Sn be a cycle. Prove that σ can be written as the product of at most n − 1 transpositions. 21. Let σ ∈ Sn . If σ is not a cycle, prove that σ can be written as the product of at most n − 2 transpositions. 22. If σ can be expressed as an odd number of transpositions, show that any other product of transpositions equaling σ must also be odd. 23. If σ is a cycle of odd length, prove that σ 2 is also a cycle. 24. Show that a 3-cycle is an even permutation. 25. Prove that in An with n ≥ 3, any permutation is a product of cycles of length 3. 26. Prove that any element in Sn can be written as a finite product of the following permutations. (a) (12), (13), . . . , (1n) (b) (12), (23), . . . , (n − 1, n) (c) (12), (12 . . . n) 68 CHAPTER 5. PERMUTATION GROUPS 27. Let G be a group and define a map λg : G → G by λg (a) = ga. Prove that λg is a permutation of G. 28. Prove that there exist n! permutations of a set containing n elements. 29. Recall that the center of a group G is Z(G) = {g ∈ G : gx = xg for all x ∈ G}. Find the center of D8 . What about the center of D10 ? What is the center of Dn ? 30. Let τ = (a1 , a2 , . . . , ak ) be a cycle of length k. (a) Prove that if σ is any permutation, then στ σ −1 = (σ(a1 ), σ(a2 ), . . . , σ(ak )) is a cycle of length k. (b) Let µ be a cycle of length k. Prove that there is a permutation σ such that στ σ −1 = µ. 31. For α and β in Sn , define α ∼ β if there exists an σ ∈ Sn such that σασ −1 = β. Show that ∼ is an equivalence relation on Sn . 32. Let σ ∈ SX . If σ n (x) = y, we will say that x ∼ y. (a) Show that ∼ is an equivalence relation on X. (b) If σ ∈ An and τ ∈ Sn , show that τ −1 στ ∈ An . (c) Define the orbit of x ∈ X under σ ∈ SX to be the set Ox,σ = {y : x ∼ y}. Compute the orbits of each of the following elements in S5 : α = (1254) β = (123)(45) γ = (13)(25). (d) If Ox,σ ∩ Oy,σ ̸= ∅, prove that Ox,σ = Oy,σ . The orbits under a permutation σ are the equivalence classes corresponding to the equivalence relation ∼. (e) A subgroup H of SX is transitive if for every x, y ∈ X, there exists a σ ∈ H such that σ(x) = y. Prove that ⟨σ⟩ is transitive if and only if Ox,σ = X for some x ∈ X. 33. Let α ∈ Sn for n ≥ 3. If αβ = βα for all β ∈ Sn , prove that α must be the identity permutation; hence, the center of Sn is the trivial subgroup. 34. If α is even, prove that α−1 is also even. Does a corresponding result hold if α is odd? 35. Show that α−1 β −1 αβ is even for α, β ∈ Sn . 36. Let r and s be the elements in Dn described in Theorem 5.23 (a) Show that srs = r−1 . (b) Show that rk s = sr−k in Dn . (c) Prove that the order of rk ∈ Dn is n/ gcd(k, n). 6 Cosets and Lagrange’s Theorem Lagrange’s Theorem, one of the most important results in finite group theory, states that the order of a subgroup must divide the order of the group. This theorem provides a powerful tool for analyzing finite groups; it gives us an idea of exactly what type of subgroups we might expect a finite group to possess. Central to understanding Lagranges’s Theorem is the notion of a coset. 6.1 Cosets Let G be a group and H a subgroup of G. Define a left coset of H with representative g ∈ G to be the set gH = {gh : h ∈ H}. Right cosets can be defined similarly by Hg = {hg : h ∈ H}. If left and right cosets coincide or if it is clear from the context to which type of coset that we are referring, we will use the word coset without specifying left or right. Example 6.1. Let H be the subgroup of Z6 consisting of the elements 0 and 3. The cosets are 0 + H = 3 + H = {0, 3} 1 + H = 4 + H = {1, 4} 2 + H = 5 + H = {2, 5}. We will always write the cosets of subgroups of Z and Zn with the additive notation we have used for cosets here. In a commutative group, left and right cosets are always identical. Example 6.2. Let H be the subgroup of S3 defined by the permutations {(1), (123), (132)}. The left cosets of H are (1)H = (123)H = (132)H = {(1), (123), (132)} (12)H = (13)H = (23)H = {(12), (13), (23)}. The right cosets of H are exactly the same as the left cosets: H(1) = H(123) = H(132) = {(1), (123), (132)} H(12) = H(13) = H(23) = {(12), (13), (23)}. 69 70 CHAPTER 6. COSETS AND LAGRANGE’S THEOREM It is not always the case that a left coset is the same as a right coset. Let K be the subgroup of S3 defined by the permutations {(1), (12)}. Then the left cosets of K are (1)K = (12)K = {(1), (12)} (13)K = (123)K = {(13), (123)} (23)K = (132)K = {(23), (132)}; however, the right cosets of K are K(1) = K(12) = {(1), (12)} K(13) = K(132) = {(13), (132)} K(23) = K(123) = {(23), (123)}. The following lemma is quite useful when dealing with cosets. (We leave its proof as an exercise.) Lemma 6.3. Let H be a subgroup of a group G and suppose that g1 , g2 ∈ G. The following conditions are equivalent. 1. g1 H = g2 H; 2. Hg1−1 = Hg2−1 ; 3. g1 H ⊂ g2 H; 4. g2 ∈ g1 H; 5. g1−1 g2 ∈ H. In all of our examples the cosets of a subgroup H partition the larger group G. The following theorem proclaims that this will always be the case. Theorem 6.4. Let H be a subgroup of a group G. Then the left cosets of H in G partition G. That is, the group G is the disjoint union of the left cosets of H in G. Proof. Let g1 H and g2 H be two cosets of H in G. We must show that either g1 H ∩g2 H = ∅ or g1 H = g2 H. Suppose that g1 H ∩ g2 H ̸= ∅ and a ∈ g1 H ∩ g2 H. Then by the definition of a left coset, a = g1 h1 = g2 h2 for some elements h1 and h2 in H. Hence, g1 = g2 h2 h−1 1 or g1 ∈ g2 H. By Lemma 6.3, g1 H = g2 H. Remark 6.5. There is nothing special in this theorem about left cosets. Right cosets also partition G; the proof of this fact is exactly the same as the proof for left cosets except that all group multiplications are done on the opposite side of H. Let G be a group and H be a subgroup of G. Define the index of H in G to be the number of left cosets of H in G. We will denote the index by [G : H]. Example 6.6. Let G = Z6 and H = {0, 3}. Then [G : H] = 3. Example 6.7. Suppose that G = S3 , H = {(1), (123), (132)}, and K = {(1), (12)}. Then [G : H] = 2 and [G : K] = 3. Theorem 6.8. Let H be a subgroup of a group G. The number of left cosets of H in G is the same as the number of right cosets of H in G. 6.2. LAGRANGE’S THEOREM 71 Proof. Let LH and RH denote the set of left and right cosets of H in G, respectively. If we can define a bijective map ϕ : LH → RH , then the theorem will be proved. If gH ∈ LH , let ϕ(gH) = Hg −1 . By Lemma 6.3, the map ϕ is well-defined; that is, if g1 H = g2 H, then Hg1−1 = Hg2−1 . To show that ϕ is one-to-one, suppose that Hg1−1 = ϕ(g1 H) = ϕ(g2 H) = Hg2−1 . Again by Lemma 6.3, g1 H = g2 H. The map ϕ is onto since ϕ(g −1 H) = Hg. 6.2 Lagrange’s Theorem Proposition 6.9. Let H be a subgroup of G with g ∈ G and define a map ϕ : H → gH by ϕ(h) = gh. The map ϕ is bijective; hence, the number of elements in H is the same as the number of elements in gH. Proof. We first show that the map ϕ is one-to-one. Suppose that ϕ(h1 ) = ϕ(h2 ) for elements h1 , h2 ∈ H. We must show that h1 = h2 , but ϕ(h1 ) = gh1 and ϕ(h2 ) = gh2 . So gh1 = gh2 , and by left cancellation h1 = h2 . To show that ϕ is onto is easy. By definition every element of gH is of the form gh for some h ∈ H and ϕ(h) = gh. Theorem 6.10 Lagrange. Let G be a finite group and let H be a subgroup of G. Then |G|/|H| = [G : H] is the number of distinct left cosets of H in G. In particular, the number of elements in H must divide the number of elements in G. Proof. The group G is partitioned into [G : H] distinct left cosets. Each left coset has |H| elements; therefore, |G| = [G : H]|H|. Corollary 6.11. Suppose that G is a finite group and g ∈ G. Then the order of g must divide the number of elements in G. Corollary 6.12. Let |G| = p with p a prime number. Then G is cyclic and any g ∈ G such that g ̸= e is a generator. Proof. Let g be in G such that g ̸= e. Then by Corollary 6.11, the order of g must divide the order of the group. Since |⟨g⟩| > 1, it must be p. Hence, g generates G. Corollary 6.12 suggests that groups of prime order p must somehow look like Zp . Corollary 6.13. Let H and K be subgroups of a finite group G such that G ⊃ H ⊃ K. Then [G : K] = [G : H][H : K]. Proof. Observe that |G| |G| |H| [G : K] = = · = [G : H][H : K]. |K| |H| |K| Remark 6.14 The converse of Lagrange’s Theorem is false. The group A4 has order 12; however, it can be shown that it does not possess a subgroup of order 6. According to Lagrange’s Theorem, subgroups of a group of order 12 can have orders of either 1, 2, 3, 4, or 6. However, we are not guaranteed that subgroups of every possible order exist. To prove that A4 has no subgroup of order 6, we will assume that it does have such a subgroup H and show that a contradiction must occur. Since A4 contains eight 3-cycles, we know that H must contain a 3-cycle. We will show that if H contains one 3-cycle, then it must contain more than 6 elements. 72 CHAPTER 6. COSETS AND LAGRANGE’S THEOREM Proposition 6.15. The group A4 has no subgroup of order 6. Proof. Since [A4 : H] = 2, there are only two cosets of H in A4 . Inasmuch as one of the cosets is H itself, right and left cosets must coincide; therefore, gH = Hg or gHg −1 = H for every g ∈ A4 . Since there are eight 3-cycles in A4 , at least one 3-cycle must be in H. Without loss of generality, assume that (123) is in H. Then (123)−1 = (132) must also be in H. Since ghg −1 ∈ H for all g ∈ A4 and all h ∈ H and (124)(123)(124)−1 = (124)(123)(142) = (243) (243)(123)(243)−1 = (243)(123)(234) = (142) we can conclude that H must have at least seven elements (1), (123), (132), (243), (243)−1 = (234), (142), (142)−1 = (124). Therefore, A4 has no subgroup of order 6. In fact, we can say more about when two cycles have the same length. Theorem 6.16. Two cycles τ and µ in Sn have the same length if and only if there exists a σ ∈ Sn such that µ = στ σ −1 . Proof. Suppose that τ = (a1 , a2 , . . . , ak ) µ = (b1 , b2 , . . . , bk ). Define σ to be the permutation σ(a1 ) = b1 σ(a2 ) = b2 .. . σ(ak ) = bk . Then µ = στ σ −1 . Conversely, suppose that τ = (a1 , a2 , . . . , ak ) is a k-cycle and σ ∈ Sn . If σ(ai ) = b and σ(a(i mod k)+1 ) = b′ , then µ(b) = b′ . Hence, µ = (σ(a1 ), σ(a2 ), . . . , σ(ak )). Since σ is one-to-one and onto, µ is a cycle of the same length as τ . 6.3 Fermat’s and Euler’s Theorems The Euler ϕ-function is the map ϕ : N → N defined by ϕ(n) = 1 for n = 1, and, for n > 1, ϕ(n) is the number of positive integers m with 1 ≤ m < n and gcd(m, n) = 1. From Proposition 3.4, we know that the order of U (n), the group of units in Zn , is ϕ(n). For example, |U (12)| = ϕ(12) = 4 since the numbers that are relatively prime to 12 are 1, 5, 7, and 11. For any prime p, ϕ(p) = p − 1. We state these results in the following theorem. Theorem 6.17. Let U (n) be the group of units in Zn . Then |U (n)| = ϕ(n). The following theorem is an important result in number theory, due to Leonhard Euler. 6.4. EXERCISES 73 Theorem 6.18 Euler’s Theorem. Let a and n be integers such that n > 0 and gcd(a, n) = 1. Then aϕ(n) ≡ 1 (mod n). Proof. By Theorem 6.17 the order of U (n) is ϕ(n). Consequently, aϕ(n) = 1 for all a ∈ U (n); or aϕ(n) − 1 is divisible by n. Therefore, aϕ(n) ≡ 1 (mod n). If we consider the special case of Euler’s Theorem in which n = p is prime and recall that ϕ(p) = p − 1, we obtain the following result, due to Pierre de Fermat. Theorem 6.19 Fermat’s Little Theorem. Let p be any prime number and suppose that p ∤ a (p does not divide a). Then ap−1 ≡ 1 (mod p). Furthermore, for any integer b, bp ≡ b (mod p). Sage Sage can create all the subgroups of a group, so long as the group is not too large. It can also create the cosets of a subgroup. Historical Note Joseph-Louis Lagrange (1736–1813), born in Turin, Italy, was of French and Italian descent. His talent for mathematics became apparent at an early age. Leonhard Euler recognized Lagrange’s abilities when Lagrange, who was only 19, communicated to Euler some work that he had done in the calculus of variations. That year he was also named a professor at the Royal Artillery School in Turin. At the age of 23 he joined the Berlin Academy. Frederick the Great had written to Lagrange proclaiming that the “greatest king in Europe” should have the “greatest mathematician in Europe” at his court. For 20 years Lagrange held the position vacated by his mentor, Euler. His works include contributions to number theory, group theory, physics and mechanics, the calculus of variations, the theory of equations, and differential equations. Along with Laplace and Lavoisier, Lagrange was one of the people responsible for designing the metric system. During his life Lagrange profoundly influenced the development of mathematics, leaving much to the next generation of mathematicians in the form of examples and new problems to be solved. 6.4 Exercises 1. Suppose that G is a finite group with an element g of order 5 and an element h of order 7. Why must |G| ≥ 35? 2. Suppose that G is a finite group with 60 elements. What are the orders of possible subgroups of G? 3. Prove or disprove: Every subgroup of the integers has finite index. 4. Prove or disprove: Every subgroup of the integers has finite order. 5. List the left and right cosets of the subgroups in each of the following. (a) ⟨8⟩ in Z24 (e) An in Sn (b) ⟨3⟩ in U (8) (f) D4 in S4 (c) 3Z in Z (g) T in C∗ (d) A4 in S4 (h) H = {(1), (123), (132)} in S4 74 CHAPTER 6. COSETS AND LAGRANGE’S THEOREM 6. Describe the left cosets of SL2 (R) in GL2 (R). What is the index of SL2 (R) in GL2 (R)? 7. Verify Euler’s Theorem for n = 15 and a = 4. 8. Use Fermat’s Little Theorem to show that if p = 4n + 3 is prime, there is no solution to the equation x2 ≡ −1 (mod p). 9. Show that the integers have infinite index in the additive group of rational numbers. 10. Show that the additive group of real numbers has infinite index in the additive group of the complex numbers. 11. Let H be a subgroup of a group G and suppose that g1 , g2 ∈ G. Prove that the following conditions are equivalent. (a) g1 H = g2 H (b) Hg1−1 = Hg2−1 (c) g1 H ⊂ g2 H (d) g2 ∈ g1 H (e) g1−1 g2 ∈ H 12. If ghg −1 ∈ H for all g ∈ G and h ∈ H, show that right cosets are identical to left cosets. That is, show that gH = Hg for all g ∈ G. 13. What fails in the proof of Theorem 6.8 if ϕ : LH → RH is defined by ϕ(gH) = Hg? 14. Suppose that g n = e. Show that the order of g divides n. 15. Show that any two permutations α, β ∈ Sn have the same cycle structure if and only if there exists a permutation γ such that β = γαγ −1 . If β = γαγ −1 for some γ ∈ Sn , then α and β are conjugate. 16. If |G| = 2n, prove that the number of elements of order 2 is odd. Use this result to show that G must contain a subgroup of order 2. 17. Suppose that [G : H] = 2. If a and b are not in H, show that ab ∈ H. 18. If [G : H] = 2, prove that gH = Hg. 19. Let H and K be subgroups of a group G. Prove that gH ∩ gK is a coset of H ∩ K in G. 20. Let H and K be subgroups of a group G. Define a relation ∼ on G by a ∼ b if there exists an h ∈ H and a k ∈ K such that hak = b. Show that this relation is an equivalence relation. The corresponding equivalence classes are called double cosets. Compute the double cosets of H = {(1), (123), (132)} in A4 . 21. Let G be a cyclic group of order n. Show that there are exactly ϕ(n) generators for G. 22. Let n = pe11 pe22 · · · pekk , where p1 , p2 , . . . , pk are distinct primes. Prove that ( )( ) ( ) 1 1 1 ϕ(n) = n 1 − 1− ··· 1 − . p1 p2 pk 23. Show that ∑ n= ϕ(d) d|n for all positive integers n. 7 Introduction to Cryptography Cryptography is the study of sending and receiving secret messages. The aim of cryptogra- phy is to send messages across a channel so that only the intended recipient of the message can read it. In addition, when a message is received, the recipient usually requires some assurance that the message is authentic; that is, that it has not been sent by someone who is trying to deceive the recipient. Modern cryptography is heavily dependent on abstract algebra and number theory. The message to be sent is called the plaintext message. The disguised message is called the ciphertext. The plaintext and the ciphertext are both written in an alphabet, con- sisting of letters or characters. Characters can include not only the familiar alphabetic characters A, . . ., Z and a, . . ., z but also digits, punctuation marks, and blanks. A cryp- tosystem, or cipher, has two parts: encryption, the process of transforming a plaintext message to a ciphertext message, and decryption, the reverse transformation of changing a ciphertext message into a plaintext message. There are many different families of cryptosystems, each distinguished by a particular encryption algorithm. Cryptosystems in a specified cryptographic family are distinguished from one another by a parameter to the encryption function called a key. A classical cryptosystem has a single key, which must be kept secret, known only to the sender and the receiver of the message. If person A wishes to send secret messages to two different people B and C, and does not wish to have B understand C’s messages or vice versa, A must use two separate keys, so one cryptosystem is used for exchanging messages with B, and another is used for exchanging messages with C. Systems that use two separate keys, one for encoding and another for decoding, are called public key cryptosystems. Since knowledge of the encoding key does not allow anyone to guess at the decoding key, the encoding key can be made public. A public key cryptosystem allows A and B to send messages to C using the same encoding key. Anyone is capable of encoding a message to be sent to C, but only C knows how to decode such a message. 7.1 Private Key Cryptography In single or private key cryptosystems the same key is used for both encrypting and decrypting messages. To encrypt a plaintext message, we apply to the message some func- tion which is kept secret, say f . This function will yield an encrypted message. Given the encrypted form of the message, we can recover the original message by applying the inverse transformation f −1 . The transformation f must be relatively easy to compute, as must f −1 ; however, f must be extremely difficult to guess from available examples of coded messages. 75 76 CHAPTER 7. INTRODUCTION TO CRYPTOGRAPHY Example 7.1. One of the first and most famous private key cryptosystems was the shift code used by Julius Caesar. We first digitize the alphabet by letting A = 00, B = 01, . . . , Z = 25. The encoding function will be f (p) = p + 3 mod 26; that is, A 7→ D, B 7→ E, . . . , Z 7→ C. The decoding function is then f −1 (p) = p − 3 mod 26 = p + 23 mod 26. Suppose we receive the encoded message DOJHEUD. To decode this message, we first digitize it: 3, 14, 9, 7, 4, 20, 3. Next we apply the inverse transformation to get 0, 11, 6, 4, 1, 17, 0, or ALGEBRA. Notice here that there is nothing special about either of the numbers 3 or 26. We could have used a larger alphabet or a different shift. Cryptanalysis is concerned with deciphering a received or intercepted message. Meth- ods from probability and statistics are great aids in deciphering an intercepted message; for example, the frequency analysis of the characters appearing in the intercepted message often makes its decryption possible. Example 7.2. Suppose we receive a message that we know was encrypted by using a shift transformation on single letters of the 26-letter alphabet. To find out exactly what the shift transformation was, we must compute b in the equation f (p) = p + b mod 26. We can do this using frequency analysis. The letter E = 04 is the most commonly occurring letter in the English language. Suppose that S = 18 is the most commonly occurring letter in the ciphertext. Then we have good reason to suspect that 18 = 4 + b mod 26, or b = 14. Therefore, the most likely encrypting function is f (p) = p + 14 mod 26. The corresponding decrypting function is f −1 (p) = p + 12 mod 26. It is now easy to determine whether or not our guess is correct. Simple shift codes are examples of monoalphabetic cryptosystems. In these ciphers a character in the enciphered message represents exactly one character in the original message. Such cryptosystems are not very sophisticated and are quite easy to break. In fact, in a simple shift as described in Example 7.1, there are only 26 possible keys. It would be quite easy to try them all rather than to use frequency analysis. Let us investigate a slightly more sophisticated cryptosystem. Suppose that the encoding function is given by f (p) = ap + b mod 26. We first need to find out when a decoding function f −1 exists. Such a decoding function exists when we can solve the equation c = ap + b mod 26 7.2. PUBLIC KEY CRYPTOGRAPHY 77 for p. By Proposition 3.4, this is possible exactly when a has an inverse or, equivalently, when gcd(a, 26) = 1. In this case f −1 (p) = a−1 p − a−1 b mod 26. Such a cryptosystem is called an affine cryptosystem. Example 7.3. Let us consider the affine cryptosystem f (p) = ap + b mod 26. For this cryptosystem to work we must choose an a ∈ Z26 that is invertible. This is only possible if gcd(a, 26) = 1. Recognizing this fact, we will let a = 5 since gcd(5, 26) = 1. It is easy to see that a−1 = 21. Therefore, we can take our encryption function to be f (p) = 5p + 3 mod 26. Thus, ALGEBRA is encoded as 3, 6, 7, 23, 8, 10, 3, or DGHXIKD. The decryption function will be f −1 (p) = 21p − 21 · 3 mod 26 = 21p + 15 mod 26. A cryptosystem would be more secure if a ciphertext letter could represent more than one plaintext letter. To give an example of this type of cryptosystem, called a polyalphabetic cryptosystem, we will generalize affine codes by using matrices. The idea works roughly the same as before; however, instead of encrypting one letter at a time we will encrypt pairs of letters. We can store a pair of letters p1 and p2 in a vector ( ) p1 p= . p2 Let A be a 2 × 2 invertible matrix with entries in Z26 . We can define an encoding function by f (p) = Ap + b, where b is a fixed column vector and matrix operations are performed in Z26 . The decoding function must be f −1 (p) = A−1 p − A−1 b. Example 7.4. Suppose that we wish to encode the word HELP. The corresponding digit string is 7, 4, 11, 15. If ( ) 3 5 A= , 1 2 then ( ) −1 2 21 A = . 25 3 If b = (2, 2)t , then our message is encrypted as RRGR. The encrypted letter R represents more than one plaintext letter. Frequency analysis can still be performed on a polyalphabetic cryptosystem, because we have a good understanding of how pairs of letters appear in the English language. The pair th appears quite often; the pair qz never appears. To avoid decryption by a third party, we must use a larger matrix than the one we used in Example 7.4. 7.2 Public Key Cryptography If traditional cryptosystems are used, anyone who knows enough to encode a message will also know enough to decode an intercepted message. In 1976, W. Diffie and M. Hellman proposed public key cryptography, which is based on the observation that the encryption and 78 CHAPTER 7. INTRODUCTION TO CRYPTOGRAPHY decryption procedures need not have the same key. This removes the requirement that the encoding key be kept secret. The encoding function f must be relatively easy to compute, but f −1 must be extremely difficult to compute without some additional information, so that someone who knows only the encrypting key cannot find the decrypting key without prohibitive computation. It is interesting to note that to date, no system has been proposed that has been proven to be “one-way;” that is, for any existing public key cryptosystem, it has never been shown to be computationally prohibitive to decode messages with only knowledge of the encoding key. The RSA Cryptosystem The rsa cryptosystem introduced by R. Rivest, A. Shamir, and L. Adleman in 1978, is based on the difficulty of factoring large numbers. Though it is not a difficult task to find two large random primes and multiply them together, factoring a 150-digit number that is the product of two large primes would take 100 million computers operating at 10 million instructions per second about 50 million years under the fastest algorithms available in the early 1990s. Although the algorithms have improved, factoring a number that is a product of two large primes is still computationally prohibitive. The rsa cryptosystem works as follows. Suppose that we choose two random 150- digit prime numbers p and q. Next, we compute the product n = pq and also compute ϕ(n) = m = (p − 1)(q − 1), where ϕ is the Euler ϕ-function. Now we start choosing random integers E until we find one that is relatively prime to m; that is, we choose E such that gcd(E, m) = 1. Using the Euclidean algorithm, we can find a number D such that DE ≡ 1 (mod m). The numbers n and E are now made public. Suppose now that person B (Bob) wishes to send person A (Alice) a message over a public line. Since E and n are known to everyone, anyone can encode messages. Bob first digitizes the message according to some scheme, say A = 00, B = 02, . . . , Z = 25. If necessary, he will break the message into pieces such that each piece is a positive integer less than n. Suppose x is one of the pieces. Bob forms the number y = xE mod n and sends y to Alice. For Alice to recover x, she need only compute x = y D mod n. Only Alice knows D. Example 7.5. Before exploring the theory behind the rsa cryptosystem or attempting to use large integers, we will use some small integers just to see that the system does indeed work. Suppose that we wish to send some message, which when digitized is 25. Let p = 23 and q = 29. Then n = pq = 667 and ϕ(n) = m = (p − 1)(q − 1) = 616. We can let E = 487, since gcd(616, 487) = 1. The encoded message is computed to be 25487 mod 667 = 169. This computation can be reasonably done by using the method of repeated squares as described in Chapter 4. Using the Euclidean algorithm, we determine that 191E = 1+151m; therefore, the decrypting key is (n, D) = (667, 191). We can recover the original message by calculating 169191 mod 667 = 25. Now let us examine why the rsa cryptosystem works. We know that DE ≡ 1 (mod m); hence, there exists a k such that DE = km + 1 = kϕ(n) + 1. 7.2. PUBLIC KEY CRYPTOGRAPHY 79 There are two cases to consider. In the first case assume that gcd(x, n) = 1. Then by Theorem 6.18, y D = (xE )D = xDE = xkm+1 = (xϕ(n) )k x = (1)k x = x mod n. So we see that Alice recovers the original message x when she computes y D mod n. For the other case, assume that gcd(x, n) ̸= 1. Since n = pq and x < n, we know x is a multiple of p or a multiple of q, but not both. We will describe the first possibility only, since the second is entirely similar. There is then an integer r, with r < q and x = rp. Note that we have gcd(x, q) = 1 and that m = ϕ(n) = (p − 1)(q − 1) = ϕ(p)ϕ(q). Then, using Theorem 6.18, but now mod q, xkm = xkϕ(p)ϕ(q) = (xϕ(q) )kϕ(p) = (1)kϕ(p) = 1 mod q. So there is an integer t such that xkm = 1 + tq. Thus, Alice also recovers the message in this case, y D = xkm+1 = xkm x = (1 + tq)x = x + tq(rp) = x + trn = x mod n. We can now ask how one would go about breaking the rsa cryptosystem. To find D given n and E, we simply need to factor n and solve for D by using the Euclidean algorithm. If we had known that 667 = 23 · 29 in Example 7.5, we could have recovered D. Message Verification There is a problem of message verification in public key cryptosystems. Since the encoding key is public knowledge, anyone has the ability to send an encoded message. If Alice receives a message from Bob, she would like to be able to verify that it was Bob who actually sent the message. Suppose that Bob’s encrypting key is (n′ , E ′ ) and his decrypting key is (n′ , D′ ). Also, suppose that Alice’s encrypting key is (n, E) and her decrypting key is (n, D). Since encryption keys are public information, they can exchange coded messages at their convenience. Bob wishes to assure Alice that the message he is sending is authentic. Before Bob sends the message x to Alice, he decrypts x with his own key: ′ x′ = xD mod n′ . Anyone can change x′ back to x just by encryption, but only Bob has the ability to form x′ . Now Bob encrypts x′ with Alice’s encryption key to form y ′ = x′ mod n, E a message that only Alice can decode. Alice decodes the message and then encodes the result with Bob’s key to read the original message, a message that could have only been sent by Bob. Historical Note Encrypting secret messages goes as far back as ancient Greece and Rome. As we know, Julius Caesar used a simple shift code to send and receive messages. However, the formal study of encoding and decoding messages probably began with the Arabs in the 1400s. In the fifteenth and sixteenth centuries mathematicians such as Alberti and Viete discovered that monoalphabetic cryptosystems offered no real security. In the 1800s, F. W. Kasiski established methods for breaking ciphers in which a ciphertext letter can represent more 80 CHAPTER 7. INTRODUCTION TO CRYPTOGRAPHY than one plaintext letter, if the same key was used several times. This discovery led to the use of cryptosystems with keys that were used only a single time. Cryptography was placed on firm mathematical foundations by such people as W. Friedman and L. Hill in the early part of the twentieth century. The period after World War I saw the development of special-purpose machines for encrypting and decrypting messages, and mathematicians were very active in cryptography during World War II. Efforts to penetrate the cryptosystems of the Axis nations were organized in England and in the United States by such notable mathematicians as Alan Turing and A. A. Albert. The Allies gained a tremendous advantage in World War II by breaking the ciphers produced by the German Enigma machine and the Japanese Purple ciphers. By the 1970s, interest in commercial cryptography had begun to take hold. There was a growing need to protect banking transactions, computer data, and electronic mail. In the early 1970s, ibm developed and implemented luzifer, the forerunner of the National Bureau of Standards’ Data Encryption Standard (DES). The concept of a public key cryptosystem, due to Diffie and Hellman, is very recent (1976). It was further developed by Rivest, Shamir, and Adleman with the rsa cryptosys- tem (1978). It is not known how secure any of these systems are. The trapdoor knapsack cryptosystem, developed by Merkle and Hellman, has been broken. It is still an open ques- tion whether or not the rsa system can be broken. In 1991, rsa Laboratories published a list of semiprimes (numbers with exactly two prime factors) with a cash prize for whoever was able to provide a factorization (http://www.emc.com/emc-plus/rsa-labs/historical/the- rsa-challenge-numbers.htm). Although the challenge ended in 2007, many of these numbers have not yet been factored. There been a great deal of controversy about research in cryptography and cryptography itself. In 1929, when Henry Stimson, Secretary of State under Herbert Hoover, dismissed the Black Chamber (the State Department’s cryptography division) on the ethical grounds that “gentlemen do not read each other’s mail.” During the last two decades of the twentieth century, the National Security Agency wanted to keep information about cryptography secret, whereas the academic community fought for the right to publish basic research. Currently, research in mathematical cryptography and computational number theory is very active, and mathematicians are free to publish their results in these areas. Sage Sage’s early development featured powerful routines for number theory, and later included significant support for algebraic structures and other areas of discrete mathematics. So it is a natural tool for the study of cryptology, including topics like RSA, elliptic curve cryptography, and AES (Advanced Encryption Standard). 7.3 Exercises 1. Encode IXLOVEXMATH using the cryptosystem in Example 7.1. 2. Decode ZLOOA WKLVA EHARQ WKHA ILQDO, which was encoded using the cryptosystem in Example 7.1. 3. Assuming that monoalphabetic code was used to encode the following secret message, what was the original message? APHUO EGEHP PEXOV FKEUH CKVUE CHKVE APHUO EGEHU EXOVL EXDKT VGEFT EHFKE UHCKF TZEXO VEZDT TVKUE XOVKV ENOHK ZFTEH TEHKQ LEROF PVEHP PEXOV ERYKP GERYT GVKEG XDRTE RGAGA 7.3. EXERCISES 81 What is the significance of this message in the history of cryptography? 4. What is the total number of possible monoalphabetic cryptosystems? How secure are such cryptosystems? 5. Prove that a 2×2 matrix A with entries in Z26 is invertible if and only if gcd(det(A), 26) = 1. 6. Given the matrix ( ) 3 4 A= , 2 3 use the encryption function f (p) = Ap + b to encode the message CRYPTOLOGY, where b = (2, 5)t . What is the decoding function? 7. Encrypt each of the following rsa messages x so that x is divided into blocks of integers of length 2; that is, if x = 142528, encode 14, 25, and 28 separately. (a) n = 3551, E = 629, x = 31 (b) n = 2257, E = 47, x = 23 (c) n = 120979, E = 13251, x = 142371 (d) n = 45629, E = 781, x = 231561 8. Compute the decoding key D for each of the encoding keys in Exercise 7.3.7. 9. Decrypt each of the following rsa messages y. (a) n = 3551, D = 1997, y = 2791 (b) n = 5893, D = 81, y = 34 (c) n = 120979, D = 27331, y = 112135 (d) n = 79403, D = 671, y = 129381 10. For each of the following encryption keys (n, E) in the rsa cryptosystem, compute D. (a) (n, E) = (451, 231) (b) (n, E) = (3053, 1921) (c) (n, E) = (37986733, 12371) (d) (n, E) = (16394854313, 34578451) 11. Encrypted messages are often divided into blocks of n letters. A message such as THE WORLD WONDERS WHY might be encrypted as JIW OCFRJ LPOEVYQ IOC but sent as JIW OCF RJL POE VYQ IOC. What are the advantages of using blocks of n letters? 12. Find integers n, E, and X such that XE ≡ X (mod n). Is this a potential problem in the rsa cryptosystem? 13. Every person in the class should construct an rsa cryptosystem using primes that are 10 to 15 digits long. Hand in (n, E) and an encoded message. Keep D secret. See if you can break one another’s codes. 82 CHAPTER 7. INTRODUCTION TO CRYPTOGRAPHY 7.4 Additional Exercises: Primality and Factoring In the rsa cryptosystem it is important to be able to find large prime numbers easily. Also, this cryptosystem is not secure if we can factor a composite number that is the product of two large primes. The solutions to both of these problems are quite easy. To find out if a number n is prime or to factor n, we can use trial division. We simply divide n by √ d = 2, 3, . . . , n. Either a factorization will be obtained, or n is prime if no d divides n. The problem is that such a computation is prohibitively time-consuming if n is very large.1. A better algorithm for factoring odd positive integers is Fermat’s factorization algorithm. (a) Let n = ab be an odd composite number. Prove that n can be written as the difference of two perfect squares: n = x2 − y 2 = (x − y)(x + y). Consequently, a positive odd integer can be factored exactly when we can find integers x and y such that n = x2 − y 2 . (b) Write a program to implement the following factorization algorithm based on the ob- servation in part (a). The expression ceiling(sqrt(n)) means the smallest integer greater than or equal to the square root of n. Write another program to do fac- torization using trial division and compare the speed of the two algorithms. Which algorithm is faster and why? x := ceiling ( sqrt ( n ) ) y := 1 1 : while x ^2 - y ^2 > n do y := y + 1 if x ^2 - y ^2 < n then x := x + 1 y := 1 goto 1 else if x ^2 - y ^2 = 0 then a := x - y b := x + y write n = a * b 2. Primality Testing. Recall Fermat’s Little Theorem from Chapter 6. Let p be prime with gcd(a, p) = 1. Then ap−1 ≡ 1 (mod p). We can use Fermat’s Little Theorem as a screening test for primes. For example, 15 cannot be prime since 215−1 ≡ 214 ≡ 4 (mod 15). However, 17 is a potential prime since 217−1 ≡ 216 ≡ 1 (mod 17). We say that an odd composite number n is a pseudoprime if 2n−1 ≡ 1 (mod n). Which of the following numbers are primes and which are pseudoprimes? 7.4. ADDITIONAL EXERCISES: PRIMALITY AND FACTORING 83 (a) 342 (c) 601 (e) 771 (b) 811 (d) 561 (f) 631 3. Let n be an odd composite number and b be a positive integer such that gcd(b, n) = 1. If bn−1 ≡ 1 (mod n), then n is a pseudoprime base b. Show that 341 is a pseudoprime base 2 but not a pseudoprime base 3. 4. Write a program to determine all primes less than 2000 using trial division. Write a second program that will determine all numbers less than 2000 that are either primes or pseudoprimes. Compare the speed of the two programs. How many pseudoprimes are there below 2000? There exist composite numbers that are pseudoprimes for all bases to which they are relatively prime. These numbers are called Carmichael numbers. The first Carmichael number is 561 = 3 · 11 · 17. In 1992, Alford, Granville, and Pomerance proved that there are an infinite number of Carmichael numbers [4]. However, Carmichael numbers are very rare. There are only 2163 Carmichael numbers less than 25 × 109 . For more sophisticated primality tests, see [1], [6], or [7]. References and Suggested Readings [1] Bressoud, D. M. Factorization and Primality Testing. Springer-Verlag, New York, 1989. [2] Diffie, W. and Hellman, M. E. “New Directions in Cryptography,” IEEE Trans. In- form. Theory 22 (1976), 644–54. [3] Gardner, M. “Mathematical games: A new kind of cipher that would take millions of years to break,” Scientific American 237 (1977), 120–24. [4] Granville, A. “Primality Testing and Carmichael Numbers,” Notices of the American Mathematical Society 39(1992), 696–700. [5] Hellman, M. E. “The Mathematics of Public Key Cryptography,” Scientific American 241(1979), 130–39. [6] Koblitz, N. A Course in Number Theory and Cryptography. 2nd ed. Springer, New York, 1994. [7] Pomerance, C., ed. “Cryptology and Computational Number Theory”, Proceedings of Symposia in Applied Mathematics 42(1990) American Mathematical Society, Prov- idence, RI. [8] Rivest, R. L., Shamir, A., and Adleman, L., “A Method for Obtaining Signatures and Public-key Cryptosystems,” Comm. ACM 21(1978), 120–26. 8 Algebraic Coding Theory Coding theory is an application of algebra that has become increasingly important over the last several decades. When we transmit data, we are concerned about sending a message over a channel that could be affected by “noise.” We wish to be able to encode and decode the information in a manner that will allow the detection, and possibly the correction, of errors caused by noise. This situation arises in many areas of communications, including radio, telephone, television, computer communications, and digital media technology. Probability, combinatorics, group theory, linear algebra, and polynomial rings over finite fields all play important roles in coding theory. 8.1 Error-Detecting and Correcting Codes Let us examine a simple model of a communications system for transmitting and receiving coded messages (Figure 8.1). m-digit message Encoder n-digit code word Transmitter Noise Receiver n-digit received word Decoder m-digit received message or error Figure 8.1: Encoding and decoding messages Uncoded messages may be composed of letters or characters, but typically they consist of binary m-tuples. These messages are encoded into codewords, consisting of binary n- tuples, by a device called an encoder. The message is transmitted and then decoded. We 84 8.1. ERROR-DETECTING AND CORRECTING CODES 85 will consider the occurrence of errors during transmission. An error occurs if there is a change in one or more bits in the codeword. A decoding scheme is a method that either converts an arbitrarily received n-tuple into a meaningful decoded message or gives an error message for that n-tuple. If the received message is a codeword (one of the special n-tuples allowed to be transmitted), then the decoded message must be the unique message that was encoded into the codeword. For received non-codewords, the decoding scheme will give an error indication, or, if we are more clever, will actually try to correct the error and reconstruct the original message. Our goal is to transmit error-free messages as cheaply and quickly as possible. Example 8.2. One possible coding scheme would be to send a message several times and to compare the received copies with one another. Suppose that the message to be encoded is a binary n-tuple (x1 , x2 , . . . , xn ). The message is encoded into a binary 3n-tuple by simply repeating the message three times: (x1 , x2 , . . . , xn ) 7→ (x1 , x2 , . . . , xn , x1 , x2 , . . . , xn , x1 , x2 , . . . , xn ). To decode the message, we choose as the ith digit the one that appears in the ith place in at least two of the three transmissions. For example, if the original message is (0110), then the transmitted message will be (0110 0110 0110). If there is a transmission error in the fifth digit, then the received codeword will be (0110 1110 0110), which will be correctly decoded as (0110).1 This triple-repetition method will automatically detect and correct all single errors, but it is slow and inefficient: to send a message consisting of n bits, 2n extra bits are required, and we can only detect and correct single errors. We will see that it is possible to find an encoding scheme that will encode a message of n bits into m bits with m much smaller than 3n. Example 8.3. Even parity, a commonly used coding scheme, is much more efficient than the simple repetition scheme. The ascii (American Standard Code for Information Interchange) coding system uses binary 8-tuples, yielding 28 = 256 possible 8-tuples. How- ever, only seven bits are needed since there are only 27 = 128 ascii characters. What can or should be done with the extra bit? Using the full eight bits, we can detect single transmission errors. For example, the ascii codes for A, B, and C are A = 6510 = 010000012 , B = 6610 = 010000102 , C = 6710 = 010000112 . Notice that the leftmost bit is always set to 0; that is, the 128 ascii characters have codes 000000002 = 010 , .. . 011111112 = 12710 . The bit can be used for error checking on the other seven bits. It is set to either 0 or 1 so that the total number of 1 bits in the representation of a character is even. Using even parity, the codes for A, B, and C now become A = 010000012 , B = 010000102 , 1 We will adopt the convention that bits are numbered left to right in binary n-tuples. 86 CHAPTER 8. ALGEBRAIC CODING THEORY C = 110000112 . Suppose an A is sent and a transmission error in the sixth bit is caused by noise over the communication channel so that (0100 0101) is received. We know an error has occurred since the received word has an odd number of 1s, and we can now request that the codeword be transmitted again. When used for error checking, the leftmost bit is called a parity check bit. By far the most common error-detecting codes used in computers are based on the addition of a parity bit. Typically, a computer stores information in m-tuples called words. Common word lengths are 8, 16, and 32 bits. One bit in the word is set aside as the parity check bit, and is not used to store information. This bit is set to either 0 or 1, depending on the number of 1s in the word. Adding a parity check bit allows the detection of all single errors because changing a single bit either increases or decreases the number of 1s by one, and in either case the parity has been changed from even to odd, so the new word is not a codeword. (We could also construct an error detection scheme based on odd parity; that is, we could set the parity check bit so that a codeword always has an odd number of 1s.) The even parity system is easy to implement, but has two drawbacks. First, multiple errors are not detectable. Suppose an A is sent and the first and seventh bits are changed from 0 to 1. The received word is a codeword, but will be decoded into a C instead of an A. Second, we do not have the ability to correct errors. If the 8-tuple (1001 1000) is received, we know that an error has occurred, but we have no idea which bit has been changed. We will now investigate a coding scheme that will not only allow us to detect transmission errors but will actually correct the errors. Transmitted Received Word Codeword 000 001 010 011 100 101 110 111 000 0 1 1 2 1 2 2 3 111 3 2 2 1 2 1 1 0 Table 8.4: A repetition code Example 8.5. Suppose that our original message is either a 0 or a 1, and that 0 encodes to (000) and 1 encodes to (111). If only a single error occurs during transmission, we can detect and correct the error. For example, if a (101) is received, then the second bit must have been changed from a 1 to a 0. The originally transmitted codeword must have been (111). This method will detect and correct all single errors. In Table 8.4, we present all possible words that might be received for the transmitted codewords (000) and (111). Table 8.4 also shows the number of bits by which each received 3-tuple differs from each original codeword. Maximum-Likelihood Decoding The coding scheme presented in Example 8.5 is not a complete solution to the problem because it does not account for the possibility of multiple errors. For example, either a (000) or a (111) could be sent and a (001) received. We have no means of deciding from the received word whether there was a single error in the third bit or two errors, one in the first bit and one in the second. No matter what coding scheme is used, an incorrect message could be received. We could transmit a (000), have errors in all three bits, and receive the codeword (111). It is important to make explicit assumptions about the likelihood and 8.1. ERROR-DETECTING AND CORRECTING CODES 87 distribution of transmission errors so that, in a particular application, it will be known whether a given error detection scheme is appropriate. We will assume that transmission errors are rare, and, that when they do occur, they occur independently in each bit; that is, if p is the probability of an error in one bit and q is the probability of an error in a different bit, then the probability of errors occurring in both of these bits at the same time is pq. We will also assume that a received n-tuple is decoded into a codeword that is closest to it; that is, we assume that the receiver uses maximum-likelihood decoding.2 p 0 0 q q 1 p 1 Figure 8.6: Binary symmetric channel A binary symmetric channel is a model that consists of a transmitter capable of sending a binary signal, either a 0 or a 1, together with a receiver. Let p be the probability that the signal is correctly received. Then q = 1 − p is the probability of an incorrect reception. If a 1 is sent, then the probability that a 1 is received is p and the probability that a 0 is received is q (Figure 8.6). The probability that no errors occur during the transmission of a binary codeword of length n is pn . For example, if p = 0.999 and a message consisting of 10,000 bits is sent, then the probability of a perfect transmission is (0.999)10,000 ≈ 0.00005. Theorem 8.7. If a binary n-tuple (x1 , . . . , xn ) is transmitted across a binary symmetric channel with probability p that no error will occur in each coordinate, then the probability that there are errors in exactly k coordinates is ( ) n k n−k q p . k Proof. Fix k different coordinates. We first compute the probability that an error has occurred in this fixed set of coordinates. The probability of an error occurring in a particular one of these k coordinates is q; the probability that an error will not occur in any of the remaining n − k coordinates is p. The probability of each of these n independent events is q k pn−k . The number of possible error patterns with exactly k errors occurring is equal to ( ) n n! = , k k!(n − k)! the number of combinations of n things taken k at a time. Each of these error patterns has probability q k pn−k of occurring; hence, the probability of all of these error patterns is ( ) n k n−k q p . k 2 This section requires a knowledge of probability, but can be skipped without loss of continuity. 88 CHAPTER 8. ALGEBRAIC CODING THEORY Example 8.8. Suppose that p = 0.995 and a 500-bit message is sent. The probability that the message was sent error-free is pn = (0.995)500 ≈ 0.082. The probability of exactly one error occurring is ( ) n qpn−1 = 500(0.005)(0.995)499 ≈ 0.204. 1 The probability of exactly two errors is ( ) n 2 n−2 500 · 499 q p = (0.005)2 (0.995)498 ≈ 0.257. 2 2 The probability of more than two errors is approximately 1 − 0.082 − 0.204 − 0.257 = 0.457. Block Codes If we are to develop efficient error-detecting and error-correcting codes, we will need more sophisticated mathematical tools. Group theory will allow faster methods of encoding and decoding messages. A code is an (n, m)-block code if the information that is to be coded can be divided into blocks of m binary digits, each of which can be encoded into n binary digits. More specifically, an (n, m)-block code consists of an encoding function E : Zm 2 → Z2 n and a decoding function D : Zn2 → Zm 2 . A codeword is any element in the image of E. We also require that E be one-to-one so that two information blocks will not be encoded into the same codeword. If our code is to be error-correcting, then D must be onto. Example 8.9. The even-parity coding system developed to detect single errors in ascii characters is an (8, 7)-block code. The encoding function is E(x7 , x6 , . . . , x1 ) = (x8 , x7 , . . . , x1 ), where x8 = x7 + x6 + · · · + x1 with addition in Z2 . Let x = (x1 , . . . , xn ) and y = (y1 , . . . , yn ) be binary n-tuples. The Hamming distance or distance, d(x, y), between x and y is the number of bits in which x and y differ. The distance between two codewords is the minimum number of transmission errors required to change one codeword into the other. The minimum distance for a code, dmin , is the minimum of all distances d(x, y), where x and y are distinct codewords. The weight, w(x), of a binary codeword x is the number of 1s in x. Clearly, w(x) = d(x, 0), where 0 = (00 · · · 0). Example 8.10. Let x = (10101), y = (11010), and z = (00011) be all of the codewords in some code C. Then we have the following Hamming distances: d(x, y) = 4, d(x, z) = 3, d(y, z) = 3. The minimum distance for this code is 3. We also have the following weights: w(x) = 3, w(y) = 3, w(z) = 2. 8.1. ERROR-DETECTING AND CORRECTING CODES 89 The following proposition lists some basic properties about the weight of a codeword and the distance between two codewords. The proof is left as an exercise. Proposition 8.11. Let x, y, and z be binary n-tuples. Then 1. w(x) = d(x, 0); 2. d(x, y) ≥ 0; 3. d(x, y) = 0 exactly when x = y; 4. d(x, y) = d(y, x); 5. d(x, y) ≤ d(x, z) + d(z, y). The weights in a particular code are usually much easier to compute than the Hamming distances between all codewords in the code. If a code is set up carefully, we can use this fact to our advantage. Suppose that x = (1101) and y = (1100) are codewords in some code. If we transmit (1101) and an error occurs in the rightmost bit, then (1100) will be received. Since (1100) is a codeword, the decoder will decode (1100) as the transmitted message. This code is clearly not very appropriate for error detection. The problem is that d(x, y) = 1. If x = (1100) and y = (1010) are codewords, then d(x, y) = 2. If x is transmitted and a single error occurs, then y can never be received. Table 8.12 gives the distances between all 4-bit codewords in which the first three bits carry information and the fourth is an even parity check bit. We can see that the minimum distance here is 2; hence, the code is suitable as a single error-detecting code. 0000 0011 0101 0110 1001 1010 1100 1111 0000 0 2 2 2 2 2 2 4 0011 2 0 2 2 2 2 4 2 0101 2 2 0 2 2 4 2 2 0110 2 2 2 0 4 2 2 2 1001 2 2 2 4 0 2 2 2 1010 2 2 4 2 2 0 2 2 1100 2 4 2 2 2 2 0 2 1111 4 2 2 2 2 2 2 0 Table 8.12: Distances between 4-bit codewords To determine exactly what the error-detecting and error-correcting capabilities for a code are, we need to analyze the minimum distance for the code. Let x and y be codewords. If d(x, y) = 1 and an error occurs where x and y differ, then x is changed to y. The received codeword is y and no error message is given. Now suppose d(x, y) = 2. Then a single error cannot change x to y. Therefore, if dmin = 2, we have the ability to detect single errors. However, suppose that d(x, y) = 2, y is sent, and a noncodeword z is received such that d(x, z) = d(y, z) = 1. Then the decoder cannot decide between x and y. Even though we are aware that an error has occurred, we do not know what the error is. Suppose dmin ≥ 3. Then the maximum-likelihood decoding scheme corrects all single errors. Starting with a codeword x, an error in the transmission of a single bit gives y 90 CHAPTER 8. ALGEBRAIC CODING THEORY with d(x, y) = 1, but d(z, y) ≥ 2 for any other codeword z ̸= x. If we do not require the correction of errors, then we can detect multiple errors when a code has a minimum distance that is greater than or equal to 3. Theorem 8.13. Let C be a code with dmin = 2n + 1. Then C can correct any n or fewer errors. Furthermore, any 2n or fewer errors can be detected in C. Proof. Suppose that a codeword x is sent and the word y is received with at most n errors. Then d(x, y) ≤ n. If z is any codeword other than x, then 2n + 1 ≤ d(x, z) ≤ d(x, y) + d(y, z) ≤ n + d(y, z). Hence, d(y, z) ≥ n + 1 and y will be correctly decoded as x. Now suppose that x is transmitted and y is received and that at least one error has occurred, but not more than 2n errors. Then 1 ≤ d(x, y) ≤ 2n. Since the minimum distance between codewords is 2n+1, y cannot be a codeword. Consequently, the code can detect between 1 and 2n errors. Example 8.14. In Table 8.15, the codewords c1 = (00000), c2 = (00111), c3 = (11100), and c4 = (11011) determine a single error-correcting code. 00000 00111 11100 11011 00000 0 3 3 4 00111 3 0 4 3 11100 3 4 0 3 11011 4 3 3 0 Table 8.15: Hamming distances for an error-correcting code Historical Note Modern coding theory began in 1948 with C. Shannon’s paper, “A Mathematical Theory of Information” [7]. This paper offered an example of an algebraic code, and Shannon’s Theorem proclaimed exactly how good codes could be expected to be. Richard Hamming began working with linear codes at Bell Labs in the late 1940s and early 1950s after becoming frustrated because the programs that he was running could not recover from simple errors generated by noise. Coding theory has grown tremendously in the past several decades. The Theory of Error-Correcting Codes, by MacWilliams and Sloane [5], published in 1977, already contained over 1500 references. Linear codes (Reed-Muller (32, 6)-block codes) were used on NASA’s Mariner space probes. More recent space probes such as Voyager have used what are called convolution codes. Currently, very active research is being done with Goppa codes, which are heavily dependent on algebraic geometry. 8.2 Linear Codes To gain more knowledge of a particular code and develop more efficient techniques of en- coding, decoding, and error detection, we need to add additional structure to our codes. One way to accomplish this is to require that the code also be a group. A group code is a code that is also a subgroup of Zn2 . To check that a code is a group code, we need only verify one thing. If we add any two elements in the code, the result must be an n-tuple that is again in the code. It is not 8.2. LINEAR CODES 91 necessary to check that the inverse of the n-tuple is in the code, since every codeword is its own inverse, nor is it necessary to check that 0 is a codeword. For instance, (11000101) + (11000101) = (00000000). Example 8.16. Suppose that we have a code that consists of the following 7-tuples: (0000000) (0001111) (0010101) (0011010) (0100110) (0101001) (0110011) (0111100) (1000011) (1001100) (1010110) (1011001) (1100101) (1101010) (1110000) (1111111). It is a straightforward though tedious task to verify that this code is also a subgroup of Z72 and, therefore, a group code. This code is a single error-detecting and single error-correcting code, but it is a long and tedious process to compute all of the distances between pairs of codewords to determine that dmin = 3. It is much easier to see that the minimum weight of all the nonzero codewords is 3. As we will soon see, this is no coincidence. However, the relationship between weights and distances in a particular code is heavily dependent on the fact that the code is a group. Lemma 8.17. Let x and y be binary n-tuples. Then w(x + y) = d(x, y). Proof. Suppose that x and y are binary n-tuples. Then the distance between x and y is exactly the number of places in which x and y differ. But x and y differ in a particular coordinate exactly when the sum in the coordinate is 1, since 1+1=0 0+0=0 1+0=1 0 + 1 = 1. Consequently, the weight of the sum must be the distance between the two codewords. Theorem 8.18. Let dmin be the minimum distance for a group code C. Then dmin is the minimum of all the nonzero weights of the nonzero codewords in C. That is, dmin = min{w(x) : x ̸= 0}. Proof. Observe that dmin = min{d(x, y) : x ̸= y} = min{d(x, y) : x + y ̸= 0} = min{w(x + y) : x + y ̸= 0} = min{w(z) : z ̸= 0}. Linear Codes From Example 8.16, it is now easy to check that the minimum nonzero weight is 3; hence, the code does indeed detect and correct all single errors. We have now reduced the problem of finding “good” codes to that of generating group codes. One easy way to generate group codes is to employ a bit of matrix theory. Define the inner product of two binary n-tuples to be x · y = x1 y1 + · · · + xn yn , 92 CHAPTER 8. ALGEBRAIC CODING THEORY where x = (x1 , x2 , . . . , xn )t and y = (y1 , y2 , . . . , yn )t are column vectors.3 For example, if x = (011001)t and y = (110101)t , then x · y = 0. We can also look at an inner product as the product of a row matrix with a column matrix; that is, x · y = xt y y1 ( ) y2 = x1 x2 · · · xn . .. yn = x1 y1 + x2 y2 + · · · + xn yn . Example 8.19. Suppose that the words to be encoded consist of all binary 3-tuples and that our encoding scheme is even-parity. To encode an arbitrary 3-tuple, we add a fourth bit to obtain an even number of 1s. Notice that an arbitrary n-tuple x = (x1 , x2 , . . . , xn )t has an even number of 1s exactly when x1 + x2 + · · · + xn = 0; hence, a 4-tuple x = (x1 , x2 , x3 , x4 )t has an even number of 1s if x1 + x2 + x3 + x4 = 0, or 1 ( ) 1 x · 1 = xt 1 = x1 x2 x3 x4 = 0. 1 1 This example leads us to hope that there is a connection between matrices and coding theory. Let Mm×n (Z2 ) denote the set of all m × n matrices with entries in Z2 . We do matrix operations as usual except that all our addition and multiplication operations occur in Z2 . Define the null space of a matrix H ∈ Mm×n (Z2 ) to be the set of all binary n-tuples x such that Hx = 0. We denote the null space of a matrix H by Null(H). Example 8.20. Suppose that 0 1 0 1 0 H = 1 1 1 1 0 . 0 0 1 1 1 For a 5-tuple x = (x1 , x2 , x3 , x4 , x5 )t to be in the null space of H, Hx = 0. Equivalently, the following system of equations must be satisfied: x2 + x4 = 0 x1 + x2 + x3 + x4 = 0 x3 + x4 + x5 = 0. The set of binary 5-tuples satisfying these equations is (00000) (11110) (10101) (01011). This code is easily determined to be a group code. Theorem 8.21. Let H be in Mm×n (Z2 ). Then the null space of H is a group code. 3 Since we will be working with matrices, we will write binary n-tuples as column vectors for the remainder of this chapter. 8.3. PARITY-CHECK AND GENERATOR MATRICES 93 Proof. Since each element of Zn2 is its own inverse, the only thing that really needs to be checked here is closure. Let x, y ∈ Null(H) for some matrix H in Mm×n (Z2 ). Then Hx = 0 and Hy = 0. So H(x + y) = Hx + Hy = 0 + 0 = 0. Hence, x + y is in the null space of H and therefore must be a codeword. A code is a linear code if it is determined by the null space of some matrix H ∈ Mm×n (Z2 ). Example 8.22. Let C be the code given by the matrix 0 0 0 1 1 1 H = 0 1 1 0 1 1 . 1 0 1 0 0 1 Suppose that the 6-tuple x = (010011)t is received. It is a simple matter of matrix multi- plication to determine whether or not x is a codeword. Since 0 Hx = 1 , 1 the received word is not a codeword. We must either attempt to correct the word or request that it be transmitted again. 8.3 Parity-Check and Generator Matrices We need to find a systematic way of generating linear codes as well as fast methods of decoding. By examining the properties of a matrix H and by carefully choosing H, it is possible to develop very efficient methods of encoding and decoding messages. To this end, we will introduce standard generator and canonical parity-check matrices. Suppose that H is an m × n matrix with entries in Z2 and n > m. If the last m columns of the matrix form the m × m identity matrix, Im , then the matrix is a canonical parity-check matrix. More specifically, H = (A | Im ), where A is the m × (n − m) matrix a11 a12 · · · a1,n−m a21 a22 · · · a2,n−m . .. . .. .. . . . . am1 am2 · · · am,n−m and Im is the m × m identity matrix 1 0 ··· 0 0 1 · · · 0 . . . .. . . . . . . . . 0 0 ··· 1 With each canonical parity-check matrix we can associate an n × (n − m) standard gen- erator matrix ( ) In−m G= . A Our goal will be to show that an x satisfying Gx = y exists if and only if Hy = 0. Given a message block x to be encoded, the matrix G will allow us to quickly encode it into a linear codeword y. 94 CHAPTER 8. ALGEBRAIC CODING THEORY Example 8.23. Suppose that we have the following eight words to be encoded: (000), (001), (010), . . . , (111). For 0 1 1 A = 1 1 0 , 1 0 1 the associated standard generator and canonical parity-check matrices are 1 0 0 0 0 1 0 0 1 G= 0 1 1 1 1 0 1 0 1 and 0 1 1 1 0 0 H = 1 1 0 0 1 0 , 1 0 1 0 0 1 respectively. Observe that the rows in H represent the parity checks on certain bit positions in a 6-tuple. The 1s in the identity matrix serve as parity checks for the 1s in the same row. If x = (x1 , x2 , x3 , x4 , x5 , x6 ), then x2 + x3 + x4 0 = Hx = x1 + x2 + x5 , x1 + x3 + x6 which yields a system of equations: x2 + x3 + x4 = 0 x1 + x2 + x5 = 0 x1 + x3 + x6 = 0. Here x4 serves as a check bit for x2 and x3 ; x5 is a check bit for x1 and x2 ; and x6 is a check bit for x1 and x3 . The identity matrix keeps x4 , x5 , and x6 from having to check on each other. Hence, x1 , x2 , and x3 can be arbitrary but x4 , x5 , and x6 must be chosen to ensure parity. The null space of H is easily computed to be (000000) (001101) (010110) (011011) (100011) (101110) (110101) (111000). An even easier way to compute the null space is with the generator matrix G (Table 8.24). 8.3. PARITY-CHECK AND GENERATOR MATRICES 95 Message Word x Codeword Gx 000 000000 001 001101 010 010110 011 011011 100 100011 101 101110 110 110101 111 111000 Table 8.24: A matrix-generated code Theorem 8.25. If H ∈ Mm×n (Z2 ) is a canonical parity-check matrix, then Null(H) con- sists of all x ∈ Zn2 whose first n − m bits are arbitrary but whose last m bits are determined by Hx = 0. Each of the last m bits serves as an even parity check bit for some of the first n − m bits. Hence, H gives rise to an (n, n − m)-block code. We leave the proof of this theorem as an exercise. In light of the theorem, the first n − m bits in x are called information bits and the last m bits are called check bits. In Example 8.23, the first three bits are the information bits and the last three are the check bits. Theorem { } that G is an n × k standard generator matrix. Then C = 8.26. Suppose y : Gx = y for x ∈ Z2 is an (n, k)-block code. More specifically, C is a group code. k Proof. Let Gx1 = y1 and Gx2 = y2 be two codewords. Then y1 + y2 is in C since G(x1 + x2 ) = Gx1 + Gx2 = y1 + y2 . We must also show that two message blocks cannot be encoded into the same codeword. That is, we must show that if Gx = Gy, then x = y. Suppose that Gx = Gy. Then Gx − Gy = G(x − y) = 0. However, the first k coordinates in G(x − y) are exactly x1 − y1 , . . . , xk − yk , since they are determined by the identity matrix, Ik , part of G. Hence, G(x − y) = 0 exactly when x = y. Before we can prove the relationship between canonical parity-check matrices and stan- dard generating matrices, we need to prove a lemma. ( ) Lemma 8.27. Let H = (A | Im ) be an m×n canonical parity-check matrix and G = In−m A be the corresponding n × (n − m) standard generator matrix. Then HG = 0. Proof. Let C = HG. The ijth entry in C is ∑ n cij = hik gkj k=1 ∑ n−m ∑ n = hik gkj + hik gkj k=1 k=n−m+1 ∑ n−m ∑n = aik δkj + δi−(m−n),k akj k=1 k=n−m+1 96 CHAPTER 8. ALGEBRAIC CODING THEORY = aij + aij = 0, where { 1, i = j δij = 0, i ̸= j is the Kronecker delta. Theorem ( )8.28. Let H = (A | Im ) be an m × n canonical parity-check matrix and let In−m G= A be the n × (n − m) standard generator matrix associated with H. Let C be the code generated by G. Then y is in C if and only if Hy = 0. In particular, C is a linear code with canonical parity-check matrix H. Proof. First suppose that y ∈ C. Then Gx = y for some x ∈ Zm 2 . By Lemma 8.27, Hy = HGx = 0. Conversely, suppose that y = (y1 , . . . , yn )t is in the null space of H. We need to find an x in Zn−m 2 such that Gxt = y. Since Hy = 0, the following set of equations must be satisfied: a11 y1 + a12 y2 + · · · + a1,n−m yn−m + yn−m+1 = 0 a21 y1 + a22 y2 + · · · + a2,n−m yn−m + yn−m+1 = 0 .. . am1 y1 + am2 y2 + · · · + am,n−m yn−m + yn−m+1 = 0. Equivalently, yn−m+1 , . . . , yn are determined by y1 , . . . , yn−m : yn−m+1 = a11 y1 + a12 y2 + · · · + a1,n−m yn−m yn−m+1 = a21 y1 + a22 y2 + · · · + a2,n−m yn−m .. . yn−m+1 = am1 y1 + am2 y2 + · · · + am,n−m yn−m . Consequently, we can let xi = yi for i = 1, . . . , n − m. It would be helpful if we could compute the minimum distance of a linear code directly from its matrix H in order to determine the error-detecting and error-correcting capabilities of the code. Suppose that e1 = (100 · · · 00)t e2 = (010 · · · 00)t .. . en = (000 · · · 01)t are the n-tuples in Zn2 of weight 1. For an m × n binary matrix H, Hei is exactly the ith column of the matrix H. Example 8.29. Observe that 0 1 1 1 1 0 0 1 1 0 0 1 0 0 = 0 . 1 1 0 0 1 0 1 0 8.3. PARITY-CHECK AND GENERATOR MATRICES 97 We state this result in the following proposition and leave the proof as an exercise. Proposition 8.30. Let ei be the binary n-tuple with a 1 in the ith coordinate and 0’s elsewhere and suppose that H ∈ Mm×n (Z2 ). Then Hei is the ith column of the matrix H. Theorem 8.31. Let H be an m × n binary matrix. Then the null space of H is a single error-detecting code if and only if no column of H consists entirely of zeros. Proof. Suppose that Null(H) is a single error-detecting code. Then the minimum dis- tance of the code must be at least 2. Since the null space is a group code, it is sufficient to require that the code contain no codewords of less than weight 2 other than the zero codeword. That is, ei must not be a codeword for i = 1, . . . , n. Since Hei is the ith column of H, the only way in which ei could be in the null space of H would be if the ith column were all zeros, which is impossible; hence, the code must have the capability to detect at least single errors. Conversely, suppose that no column of H is the zero column. By Proposition 8.30, Hei ̸= 0. Example 8.32. If we consider the matrices 1 1 1 0 0 H1 = 1 0 0 1 0 1 1 0 0 1 and 1 1 1 0 0 H2 = 1 0 0 0 0 , 1 1 0 0 1 then the null space of H1 is a single error-detecting code and the null space of H2 is not. We can even do better than Theorem 8.31. This theorem gives us conditions on a matrix H that tell us when the minimum weight of the code formed by the null space of H is 2. We can also determine when the minimum distance of a linear code is 3 by examining the corresponding matrix. Example 8.33. If we let 1 1 1 0 H = 1 0 0 1 1 1 0 0 and want to determine whether or not H is the canonical parity-check matrix for an error- correcting code, it is necessary to make certain that Null(H) does not contain any 4-tuples of weight 2. That is, (1100), (1010), (1001), (0110), (0101), and (0011) must not be in Null(H). The next theorem states that we can indeed determine that the code generated by H is error-correcting by examining the columns of H. Notice in this example that not only does H have no zero columns, but also that no two columns are the same. Theorem 8.34. Let H be a binary matrix. The null space of H is a single error-correcting code if and only if H does not contain any zero columns and no two columns of H are identical. Proof. The n-tuple ei + ej has 1s in the ith and jth entries and 0s elsewhere, and w(ei + ej ) = 2 for i ̸= j. Since 0 = H(ei + ej ) = Hei + Hej can only occur if the ith and jth columns are identical, the null space of H is a single error-correcting code. 98 CHAPTER 8. ALGEBRAIC CODING THEORY Suppose now that we have a canonical parity-check matrix H with three rows. Then we might ask how many more columns we can add to the matrix and still have a null space that is a single error-detecting and single error-correcting code. Since each column has three entries, there are 23 = 8 possible distinct columns. We cannot add the columns 0 1 0 0 0 , 0 , 1 , 0 . 0 0 0 1 So we can add as many as four columns and still maintain a minimum distance of 3. In general, if H is an m × n canonical parity-check matrix, then there are n − m informa- tion positions in each codeword. Each column has m bits, so there are 2m possible distinct columns. It is necessary that the columns 0, e1 , . . . , em be excluded, leaving 2m − (1 + m) remaining columns for information if we are still to maintain the ability not only to detect but also to correct single errors. 8.4 Efficient Decoding We are now at the stage where we are able to generate linear codes that detect and correct errors fairly easily, but it is still a time-consuming process to decode a received n-tuple and determine which is the closest codeword, because the received n-tuple must be compared to each possible codeword to determine the proper decoding. This can be a serious impediment if the code is very large. Example 8.35. Given the binary matrix 1 1 1 0 0 H = 0 1 0 1 0 1 0 0 0 1 and the 5-tuples x = (11011)t and y = (01011)t , we can compute 0 1 Hx = 0 and Hy = 0 . 0 1 Hence, x is a codeword and y is not, since x is in the null space and y is not. Notice that Hy is identical to the first column of H. In fact, this is where the error occurred. If we flip the first bit in y from 0 to 1, then we obtain x. If H is an m × n matrix and x ∈ Zn2 , then we say that the syndrome of x is Hx. The following proposition allows the quick detection and correction of errors. Proposition 8.36. Let the m × n binary matrix H determine a linear code and let x be the received n-tuple. Write x as x = c + e, where c is the transmitted codeword and e is the transmission error. Then the syndrome Hx of the received codeword x is also the syndrome of the error e. Proof. The proof follows from the fact that Hx = H(c + e) = Hc + He = 0 + He = He. 8.4. EFFICIENT DECODING 99 This proposition tells us that the syndrome of a received word depends solely on the error and not on the transmitted codeword. The proof of the following theorem follows immediately from Proposition 8.36 and from the fact that He is the ith column of the matrix H. Theorem 8.37. Let H ∈ Mm×n (Z2 ) and suppose that the linear code corresponding to H is single error-correcting. Let r be a received n-tuple that was transmitted with at most one error. If the syndrome of r is 0, then no error has occurred; otherwise, if the syndrome of r is equal to some column of H, say the ith column, then the error has occurred in the ith bit. Example 8.38. Consider the matrix 1 0 1 1 0 0 H = 0 1 1 0 1 0 1 1 1 0 0 1 and suppose that the 6-tuples x = (111110)t , y = (111111)t , and z = (010111)t have been received. Then 1 1 1 Hx = 1 , Hy = 1 , Hz = 0 . 1 0 0 Hence, x has an error in the third bit and z has an error in the fourth bit. The transmitted codewords for x and z must have been (110110) and (010011), respectively. The syndrome of y does not occur in any of the columns of the matrix H, so multiple errors must have occurred to produce y. Coset Decoding We can use group theory to obtain another way of decoding messages. A linear code C is a subgroup of Zn2 . Coset or standard decoding uses the cosets of C in Zn2 to implement maximum-likelihood decoding. Suppose that C is an (n, m)-linear code. A coset of C in Zn2 is written in the form x + C, where x ∈ Zn2 . By Lagrange’s Theorem (Theorem 6.10), there are 2n−m distinct cosets of C in Zn2 . Example 8.39. Let C be the (5, 3)-linear code given by the parity-check matrix 0 1 1 0 0 H = 1 0 0 1 0 . 1 1 0 0 1 The code consists of the codewords (00000) (01101) (10011) (11110). There are 25−2 = 23 cosets of C in Z52 , each with order 22 = 4. These cosets are listed in Table 8.40. 100 CHAPTER 8. ALGEBRAIC CODING THEORY Coset Coset Representative C (00000)(01101)(10011)(11110) (10000) + C (10000)(11101)(00011)(01110) (01000) + C (01000)(00101)(11011)(10110) (00100) + C (00100)(01001)(10111)(11010) (00010) + C (00010)(01111)(10001)(11100) (00001) + C (00001)(01100)(10010)(11111) (10100) + C (00111)(01010)(10100)(11001) (00110) + C (00110)(01011)(10101)(11000) Table 8.40: Cosets of C Our task is to find out how knowing the cosets might help us to decode a message. Suppose that x was the original codeword sent and that r is the n-tuple received. If e is the transmission error, then r = e + x or, equivalently, x = e + r. However, this is exactly the statement that r is an element in the coset e + C. In maximum-likelihood decoding we expect the error e to be as small as possible; that is, e will have the least weight. An n-tuple of least weight in a coset is called a coset leader. Once we have determined a coset leader for each coset, the decoding process becomes a task of calculating r + e to obtain x. Example 8.41. In Table 8.40, notice that we have chosen a representative of the least possible weight for each coset. These representatives are coset leaders. Now suppose that r = (01111) is the received word. To decode r, we find that it is in the coset (00010) + C; hence, the originally transmitted codeword must have been (01101) = (01111) + (00010). A potential problem with this method of decoding is that we might have to examine every coset for the received codeword. The following proposition gives a method of implementing coset decoding. It states that we can associate a syndrome with each coset; hence, we can make a table that designates a coset leader corresponding to each syndrome. Such a list is called a decoding table. Syndrome Coset Leader (000) (00000) (001) (00001) (010) (00010) (011) (10000) (100) (00100) (101) (01000) (110) (00110) (111) (10100) Table 8.42: Syndromes for each coset Proposition 8.43. Let C be an (n, k)-linear code given by the matrix H and suppose that x and y are in Zn2 . Then x and y are in the same coset of C if and only if Hx = Hy. That is, two n-tuples are in the same coset if and only if their syndromes are the same. Proof. Two n-tuples x and y are in the same coset of C exactly when x−y ∈ C; however, this is equivalent to H(x − y) = 0 or Hx = Hy. 8.5. EXERCISES 101 Example 8.44. Table 8.42 is a decoding table for the code C given in Example 8.39. If x = (01111) is received, then its syndrome can be computed to be 0 Hx = 1 . 1 Examining the decoding table, we determine that the coset leader is (00010). It is now easy to decode the received codeword. Given an (n, k)-block code, the question arises of whether or not coset decoding is a manageable scheme. A decoding table requires a list of cosets and syndromes, one for each of the 2n−k cosets of C. Suppose that we have a (32, 24)-block code. We have a huge number of codewords, 224 , yet there are only 232−24 = 28 = 256 cosets. Sage Sage has a substantial repertoire of commands for coding theory, including the ability to build many different families of codes. 8.5 Exercises 1. Why is the following encoding scheme not acceptable? Information 0 1 2 3 4 5 6 7 8 Codeword 000 001 010 011 101 110 111 000 001 2. Without doing any addition, explain why the following set of 4-tuples in Z42 cannot be a group code. (0110) (1001) (1010) (1100) 3. Compute the Hamming distances between the following pairs of n-tuples. (a) (011010), (011100) (c) (00110), (01111) (b) (11110101), (01010100) (d) (1001), (0111) 4. Compute the weights of the following n-tuples. (a) (011010) (c) (01111) (b) (11110101) (d) (1011) 5. Suppose that a linear code C has a minimum weight of 7. What are the error-detection and error-correction capabilities of C? 6. In each of the following codes, what is the minimum distance for the code? What is the best situation we might hope for in connection with error detection and error correction? (a) (011010) (011100) (110111) (110000) (b) (011100) (011011) (111011) (100011) (000000) (010101) (110100) (110011) (c) (000000) (011100) (110101) (110001) 102 CHAPTER 8. ALGEBRAIC CODING THEORY (d) (0110110) (0111100) (1110000) (1111111) (1001001) (1000011) (0001111) (0000000) 7. Compute the null space of each of the following matrices. What type of (n, k)-block codes are the null spaces? Can you find a matrix (not necessarily a standard generator matrix) that generates each code? Are your generator matrices unique? (a) (c) ( ) 0 1 0 0 0 1 0 0 1 1 1 0 1 0 1 0 1 0 1 1 1 0 0 1 0 (b) (d) 1 0 1 0 0 0 0 0 0 1 1 1 1 1 1 0 1 0 0 0 1 1 0 0 1 1 0 1 0 0 1 0 1 0 1 0 1 0 1 1 1 0 0 0 1 0 1 1 0 0 1 1 8. Construct a (5, 2)-block code. Discuss both the error-detection and error-correction capabilities of your code. 9. Let C be the code obtained from the null space of the matrix 0 1 0 0 1 H = 1 0 1 0 1 . 0 0 1 1 1 Decode the message 01111 10101 01110 00011 if possible. 10. Suppose that a 1000-bit binary message is transmitted. Assume that the probability of a single error is p and that the errors occurring in different bits are independent of one another. If p = 0.01, what is the probability of more than one error occurring? What is the probability of exactly two errors occurring? Repeat this problem for p = 0.0001. 11. Which matrices are canonical parity-check matrices? For those matrices that are canonical parity-check matrices, what are the corresponding standard generator matrices? What are the error-detection and error-correction capabilities of the code generated by each of these matrices? (a) (c) 1 1 0 0 0 ( ) 1 1 1 0 0 0 1 0 0 1 0 0 1 0 0 0 1 0 1 0 0 0 1 (d) (b) 0 1 1 0 0 0 0 0 0 1 0 0 0 1 1 0 1 0 0 0 1 1 0 1 0 0 0 1 0 0 1 0 1 0 1 0 0 1 0 1 1 0 0 0 1 0 1 1 0 0 0 1 8.5. EXERCISES 103 12. List all possible syndromes for the codes generated by each of the matrices in Exer- cise 8.5.11. 13. Let 0 1 1 1 1 H = 0 0 0 1 1 . 1 0 1 0 1 Compute the syndrome caused by each of the following transmission errors. (a) An error in the first bit. (b) An error in the third bit. (c) An error in the last bit. (d) Errors in the third and fourth bits. 14. Let C be the group code in Z32 defined by the codewords (000) and (111). Compute the cosets of C in Z32 . Why was there no need to specify right or left cosets? Give the single transmission error, if any, to which each coset corresponds. 15. For each of the following matrices, find the cosets of the corresponding code C. Give a decoding table for each code if possible. (a) (c) ( ) 0 1 0 0 0 1 0 0 1 1 1 0 1 0 1 0 1 0 1 1 1 0 0 1 0 (b) (d) 0 0 1 0 0 1 0 0 1 1 1 1 1 1 0 1 0 1 1 1 0 0 1 1 0 1 0 1 0 1 0 1 0 1 0 1 1 1 0 0 1 1 1 1 0 0 1 0 16. Let x, y, and z be binary n-tuples. Prove each of the following statements. (a) w(x) = d(x, 0) (b) d(x, y) = d(x + z, y + z) (c) d(x, y) = w(x − y) 17. A metric on a set X is a map d : X × X → R satisfying the following conditions. (a) d(x, y) ≥ 0 for all x, y ∈ X; (b) d(x, y) = 0 exactly when x = y; (c) d(x, y) = d(y, x); (d) d(x, y) ≤ d(x, z) + d(z, y). 104 CHAPTER 8. ALGEBRAIC CODING THEORY In other words, a metric is simply a generalization of the notion of distance. Prove that Hamming distance is a metric on Zn2 . Decoding a message actually reduces to deciding which is the closest codeword in terms of distance. 18. Let C be a linear code. Show that either the ith coordinates in the codewords of C are all zeros or exactly half of them are zeros. 19. Let C be a linear code. Show that either every codeword has even weight or exactly half of the codewords have even weight. 20. Show that the codewords of even weight in a linear code C are also a linear code. 21. If we are to use an error-correcting linear code to transmit the 128 ascii characters, what size matrix must be used? What size matrix must be used to transmit the extended ascii character set of 256 characters? What if we require only error detection in both cases? 22. Find the canonical parity-check matrix that gives the even parity check bit code with three information positions. What is the matrix for seven information positions? What are the corresponding standard generator matrices? 23. How many check positions are needed for a single error-correcting code with 20 information positions? With 32 information positions? 24. Let ei be the binary n-tuple with a 1 in the ith coordinate and 0’s elsewhere and suppose that H ∈ Mm×n (Z2 ). Show that Hei is the ith column of the matrix H. 25. Let C be an (n, k)-linear code. Define the dual or orthogonal code of C to be C ⊥ = {x ∈ Zn2 : x · y = 0 for all y ∈ C}. (a) Find the dual code of the linear code C where C is given by the matrix 1 1 1 0 0 0 0 1 0 1 . 1 0 0 1 0 (b) Show that C ⊥ is an (n, n − k)-linear code. (c) Find the standard generator and parity-check matrices of C and C ⊥ . What happens in general? Prove your conjecture. 26. Let H be an m × n matrix over Z2 , where the ith column is the number i written in binary with m bits. The null space of such a matrix is called a Hamming code. (a) Show that the matrix 0 0 0 1 1 1 H = 0 1 1 0 0 1 1 0 1 0 1 0 generates a Hamming code. What are the error-correcting properties of a Hamming code? (b) The column corresponding to the syndrome also marks the bit that was in error; that is, the ith column of the matrix is i written as a binary number, and the syndrome immediately tells us which bit is in error. If the received word is (101011), compute the syndrome. In which bit did the error occur in this case, and what codeword was originally transmitted? 8.6. PROGRAMMING EXERCISES 105 (c) Give a binary matrix H for the Hamming code with six information positions and four check positions. What are the check positions and what are the information positions? Encode the messages (101101) and (001001). Decode the received words (0010000101) and (0000101100). What are the possible syndromes for this code? (d) What is the number of check bits and the number of information bits in an (m, n)- block Hamming code? Give both an upper and a lower bound on the number of information bits in terms of the number of check bits. Hamming codes having the maximum possible number of information bits with k check bits are called perfect. Every possible syndrome except 0 occurs as a column. If the number of information bits is less than the maximum, then the code is called shortened. In this case, give an example showing that some syndromes can represent multiple errors. 8.6 Programming Exercises 1. Write a program to implement a (16, 12)-linear code. Your program should be able to encode and decode messages using coset decoding. Once your program is written, write a program to simulate a binary symmetric channel with transmission noise. Compare the results of your simulation with the theoretically predicted error probability. References and Suggested Readings [1] Blake, I. F. “Codes and Designs,” Mathematics Magazine 52(1979), 81–95. [2] Hill, R. A First Course in Coding Theory. Oxford University Press, Oxford, 1990. [3] Levinson, N. “Coding Theory: A Counterexample to G. H. Hardy’s Conception of Applied Mathematics,” American Mathematical Monthly 77(1970), 249–58. [4] Lidl, R. and Pilz, G. Applied Abstract Algebra. 2nd ed. Springer, New York, 1998. [5] MacWilliams, F. J. and Sloane, N. J. A. The Theory of Error-Correcting Codes. North-Holland Mathematical Library, 16, Elsevier, Amsterdam, 1983. [6] Roman, S. Coding and Information Theory. Springer-Verlag, New York, 1992. [7] Shannon, C. E. “A Mathematical Theory of Communication,” Bell System Technical Journal 27(1948), 379–423, 623–56. [8] Thompson, T. M. From Error-Correcting Codes through Sphere Packing to Simple Groups. Carus Monograph Series, No. 21. Mathematical Association of America, Washington, DC, 1983. [9] van Lint, J. H. Introduction to Coding Theory. Springer, New York, 1999. 9 Isomorphisms Many groups may appear to be different at first glance, but can be shown to be the same by a simple renaming of the group elements. For example, Z4 and the subgroup of the circle group T generated by i can be shown to be the same by demonstrating a one-to-one correspondence between the elements of the two groups and between the group operations. In such a case we say that the groups are isomorphic. 9.1 Definition and Examples Two groups (G, ·) and (H, ◦) are isomorphic if there exists a one-to-one and onto map ϕ : G → H such that the group operation is preserved; that is, ϕ(a · b) = ϕ(a) ◦ ϕ(b) for all a and b in G. If G is isomorphic to H, we write G ∼ = H. The map ϕ is called an isomorphism. Example 9.1. To show that Z4 ∼ = ⟨i⟩, define a map ϕ : Z4 → ⟨i⟩ by ϕ(n) = in . We must show that ϕ is bijective and preserves the group operation. The map ϕ is one-to-one and onto because ϕ(0) = 1 ϕ(1) = i ϕ(2) = −1 ϕ(3) = −i. Since ϕ(m + n) = im+n = im in = ϕ(m)ϕ(n), the group operation is preserved. Example 9.2. We can define an isomorphism ϕ from the additive group of real numbers (R, +) to the multiplicative group of positive real numbers (R+ , ·) with the exponential map; that is, ϕ(x + y) = ex+y = ex ey = ϕ(x)ϕ(y). Of course, we must still show that ϕ is one-to-one and onto, but this can be determined using calculus. Example 9.3. The integers are isomorphic to the subgroup of Q∗ consisting of elements of the form 2n . Define a map ϕ : Z → Q∗ by ϕ(n) = 2n . Then ϕ(m + n) = 2m+n = 2m 2n = ϕ(m)ϕ(n). 106 9.1. DEFINITION AND EXAMPLES 107 By definition the map ϕ is onto the subset {2n : n ∈ Z} of Q∗ . To show that the map is injective, assume that m ̸= n. If we can show that ϕ(m) ̸= ϕ(n), then we are done. Suppose that m > n and assume that ϕ(m) = ϕ(n). Then 2m = 2n or 2m−n = 1, which is impossible since m − n > 0. Example 9.4. The groups Z8 and Z12 cannot be isomorphic since they have different orders; however, it is true that U (8) ∼ = U (12). We know that U (8) = {1, 3, 5, 7} U (12) = {1, 5, 7, 11}. An isomorphism ϕ : U (8) → U (12) is then given by 1 7→ 1 3 7→ 5 5 7→ 7 7 7→ 11. The map ϕ is not the only possible isomorphism between these two groups. We could define another isomorphism ψ by ψ(1) = 1, ψ(3) = 11, ψ(5) = 5, ψ(7) = 7. In fact, both of these groups are isomorphic to Z2 × Z2 (see Example 3.28 in Chapter 3). Example 9.5. Even though S3 and Z6 possess the same number of elements, we would suspect that they are not isomorphic, because Z6 is abelian and S3 is nonabelian. To demonstrate that this is indeed the case, suppose that ϕ : Z6 → S3 is an isomorphism. Let a, b ∈ S3 be two elements such that ab ̸= ba. Since ϕ is an isomorphism, there exist elements m and n in Z6 such that ϕ(m) = a and ϕ(n) = b. However, ab = ϕ(m)ϕ(n) = ϕ(m + n) = ϕ(n + m) = ϕ(n)ϕ(m) = ba, which contradicts the fact that a and b do not commute. Theorem 9.6. Let ϕ : G → H be an isomorphism of two groups. Then the following statements are true. 1. ϕ−1 : H → G is an isomorphism. 2. |G| = |H|. 3. If G is abelian, then H is abelian. 4. If G is cyclic, then H is cyclic. 5. If G has a subgroup of order n, then H has a subgroup of order n. Proof. Assertions (1) and (2) follow from the fact that ϕ is a bijection. We will prove (3) here and leave the remainder of the theorem to be proved in the exercises. (3) Suppose that h1 and h2 are elements of H. Since ϕ is onto, there exist elements g1 , g2 ∈ G such that ϕ(g1 ) = h1 and ϕ(g2 ) = h2 . Therefore, h1 h2 = ϕ(g1 )ϕ(g2 ) = ϕ(g1 g2 ) = ϕ(g2 g1 ) = ϕ(g2 )ϕ(g1 ) = h2 h1 . We are now in a position to characterize all cyclic groups. 108 CHAPTER 9. ISOMORPHISMS Theorem 9.7. All cyclic groups of infinite order are isomorphic to Z. Proof. Let G be a cyclic group with infinite order and suppose that a is a generator of G. Define a map ϕ : Z → G by ϕ : n 7→ an . Then ϕ(m + n) = am+n = am an = ϕ(m)ϕ(n). To show that ϕ is injective, suppose that m and n are two elements in Z, where m ̸= n. We can assume that m > n. We must show that am ̸= an . Let us suppose the contrary; that is, am = an . In this case am−n = e, where m − n > 0, which contradicts the fact that a has infinite order. Our map is onto since any element in G can be written as an for some integer n and ϕ(n) = an . Theorem 9.8. If G is a cyclic group of order n, then G is isomorphic to Zn . Proof. Let G be a cyclic group of order n generated by a and define a map ϕ : Zn → G by ϕ : k 7→ ak , where 0 ≤ k < n. The proof that ϕ is an isomorphism is one of the end-of-chapter exercises. Corollary 9.9. If G is a group of order p, where p is a prime number, then G is isomorphic to Zp . Proof. The proof is a direct result of Corollary 6.12. The main goal in group theory is to classify all groups; however, it makes sense to consider two groups to be the same if they are isomorphic. We state this result in the following theorem, whose proof is left as an exercise. Theorem 9.10. The isomorphism of groups determines an equivalence relation on the class of all groups. Hence, we can modify our goal of classifying all groups to classifying all groups up to isomorphism; that is, we will consider two groups to be the same if they are isomorphic. Cayley’s Theorem Cayley proved that if G is a group, it is isomorphic to a group of permutations on some set; hence, every group is a permutation group. Cayley’s Theorem is what we call a represen- tation theorem. The aim of representation theory is to find an isomorphism of some group G that we wish to study into a group that we know a great deal about, such as a group of permutations or matrices. Example 9.11. Consider the group Z3 . The Cayley table for Z3 is as follows. + 0 1 2 0 0 1 2 1 1 2 0 2 2 0 1 The addition table of Z3 suggests that it is the same as the permutation group G = {(0), (012), (021)}. The isomorphism here is ( ) 0 1 2 0 7→ = (0) 0 1 2 9.1. DEFINITION AND EXAMPLES 109 ( ) 0 1 2 1 7→ = (012) 1 2 0 ( ) 0 1 2 2 7→ = (021). 2 0 1 Theorem 9.12 Cayley. Every group is isomorphic to a group of permutations. Proof. Let G be a group. We must find a group of permutations G that is isomorphic to G. For any g ∈ G, define a function λg : G → G by λg (a) = ga. We claim that λg is a permutation of G. To show that λg is one-to-one, suppose that λg (a) = λg (b). Then ga = λg (a) = λg (b) = gb. Hence, a = b. To show that λg is onto, we must prove that for each a ∈ G, there is a b such that λg (b) = a. Let b = g −1 a. Now we are ready to define our group G. Let G = {λg : g ∈ G}. We must show that G is a group under composition of functions and find an isomorphism between G and G. We have closure under composition of functions since (λg ◦ λh )(a) = λg (ha) = gha = λgh (a). Also, λe (a) = ea = a and (λg−1 ◦ λg )(a) = λg−1 (ga) = g −1 ga = a = λe (a). We can define an isomorphism from G to G by ϕ : g 7→ λg . The group operation is preserved since ϕ(gh) = λgh = λg λh = ϕ(g)ϕ(h). It is also one-to-one, because if ϕ(g)(a) = ϕ(h)(a), then ga = λg a = λh a = ha. Hence, g = h. That ϕ is onto follows from the fact that ϕ(g) = λg for any λg ∈ G. The isomorphism g 7→ λg is known as the left regular representation of G. Historical Note Arthur Cayley was born in England in 1821, though he spent much of the first part of his life in Russia, where his father was a merchant. Cayley was educated at Cambridge, where he took the first Smith’s Prize in mathematics. A lawyer for much of his adult life, he wrote several papers in his early twenties before entering the legal profession at the age of 25. While practicing law he continued his mathematical research, writing more than 300 papers during this period of his life. These included some of his best work. In 1863 he left law to become a professor at Cambridge. Cayley wrote more than 900 papers in fields such as group theory, geometry, and linear algebra. His legal knowledge was very valuable to Cambridge; he participated in the writing of many of the university’s statutes. Cayley was also one of the people responsible for the admission of women to Cambridge. 110 CHAPTER 9. ISOMORPHISMS 9.2 Direct Products Given two groups G and H, it is possible to construct a new group from the Cartesian product of G and H, G × H. Conversely, given a large group, it is sometimes possible to decompose the group; that is, a group is sometimes isomorphic to the direct product of two smaller groups. Rather than studying a large group G, it is often easier to study the component groups of G. External Direct Products If (G, ·) and (H, ◦) are groups, then we can make the Cartesian product of G and H into a new group. As a set, our group is just the ordered pairs (g, h) ∈ G × H where g ∈ G and h ∈ H. We can define a binary operation on G × H by (g1 , h1 )(g2 , h2 ) = (g1 · g2 , h1 ◦ h2 ); that is, we just multiply elements in the first coordinate as we do in G and elements in the second coordinate as we do in H. We have specified the particular operations · and ◦ in each group here for the sake of clarity; we usually just write (g1 , h1 )(g2 , h2 ) = (g1 g2 , h1 h2 ). Proposition 9.13. Let G and H be groups. The set G × H is a group under the operation (g1 , h1 )(g2 , h2 ) = (g1 g2 , h1 h2 ) where g1 , g2 ∈ G and h1 , h2 ∈ H. Proof. Clearly the binary operation defined above is closed. If eG and eH are the identities of the groups G and H respectively, then (eG , eH ) is the identity of G × H. The inverse of (g, h) ∈ G × H is (g −1 , h−1 ). The fact that the operation is associative follows directly from the associativity of G and H. Example 9.14. Let R be the group of real numbers under addition. The Cartesian product of R with itself, R × R = R2 , is also a group, in which the group operation is just addition in each coordinate; that is, (a, b) + (c, d) = (a + c, b + d). The identity is (0, 0) and the inverse of (a, b) is (−a, −b). Example 9.15. Consider Z2 × Z2 = {(0, 0), (0, 1), (1, 0), (1, 1)}. Although Z2 × Z2 and Z4 both contain four elements, they are not isomorphic. Every element (a, b) in Z2 × Z2 has order 2, since (a, b) + (a, b) = (0, 0); however, Z4 is cyclic. The group G × H is called the external direct product of G and H. Notice that there is nothing special about the fact that we have used only two groups to build a new group. The direct product ∏n Gi = G1 × G2 × · · · × Gn i=1 of the groups G1 , G2 , . . . , Gn is defined in exactly the same manner. If G = G1 = G2 = · · · = Gn , we often write Gn instead of G1 × G2 × · · · × Gn . Example 9.16. The group Zn2 , considered as a set, is just the set of all binary n-tuples. The group operation is the “exclusive or” of two binary n-tuples. For example, (01011101) + (01001011) = (00010110). This group is important in coding theory, in cryptography, and in many areas of computer science. 9.2. DIRECT PRODUCTS 111 Theorem 9.17. Let (g, h) ∈ G × H. If g and h have finite orders r and s respectively, then the order of (g, h) in G × H is the least common multiple of r and s. Proof. Suppose that m is the least common multiple of r and s and let n = |(g, h)|. Then (g, h)m = (g m , hm ) = (eG , eH ) (g n , hn ) = (g, h)n = (eG , eH ). Hence, n must divide m, and n ≤ m. However, by the second equation, both r and s must divide n; therefore, n is a common multiple of r and s. Since m is the least common multiple of r and s, m ≤ n. Consequently, m must be equal to n. ∏ Corollary 9.18. ∏ Let (g1 , . . . , gn ) ∈ Gi . If gi has finite order ri in Gi , then the order of (g1 , . . . , gn ) in Gi is the least common multiple of r1 , . . . , rn . Example 9.19. Let (8, 56) ∈ Z12 × Z60 . Since gcd(8, 12) = 4, the order of 8 is 12/4 = 3 in Z12 . Similarly, the order of 56 in Z60 is 15. The least common multiple of 3 and 15 is 15; hence, (8, 56) has order 15 in Z12 × Z60 . Example 9.20. The group Z2 × Z3 consists of the pairs (0, 0), (0, 1), (0, 2), (1, 0), (1, 1), (1, 2). In this case, unlike that of Z2 × Z2 and Z4 , it is true that Z2 × Z3 ∼ = Z6 . We need only show that Z2 × Z3 is cyclic. It is easy to see that (1, 1) is a generator for Z2 × Z3 . The next theorem tells us exactly when the direct product of two cyclic groups is cyclic. Theorem 9.21. The group Zm × Zn is isomorphic to Zmn if and only if gcd(m, n) = 1. Proof. We will first show that if Zm × Zn ∼ = Zmn , then gcd(m, n) = 1. We will prove the contrapositive; that is, we will show that if gcd(m, n) = d > 1, then Zm ×Zn cannot be cyclic. Notice that mn/d is divisible by both m and n; hence, for any element (a, b) ∈ Zm × Zn , (a, b) + (a, b) + · · · + (a, b) = (0, 0). | {z } mn/d times Therefore, no (a, b) can generate all of Zm × Zn . The converse follows directly from Theorem 9.17 since lcm(m, n) = mn if and only if gcd(m, n) = 1. Corollary 9.22. Let n1 , . . . , nk be positive integers. Then ∏ k Zni ∼ = Zn1 ···nk i=1 if and only if gcd(ni , nj ) = 1 for i ̸= j. Corollary 9.23. If m = pe11 · · · pekk , where the pi s are distinct primes, then Zm ∼ = Zpe11 × · · · × Zpek . k 112 CHAPTER 9. ISOMORPHISMS e Proof. Since the greatest common divisor of pei i and pj j is 1 for i ̸= j, the proof follows from Corollary 9.22. In Chapter 13, we will prove that all finite abelian groups are isomorphic to direct products of the form Zpe1 × · · · × Zpek 1 k where p1 , . . . , pk are (not necessarily distinct) primes. Internal Direct Products The external direct product of two groups builds a large group out of two smaller groups. We would like to be able to reverse this process and conveniently break down a group into its direct product components; that is, we would like to be able to say when a group is isomorphic to the direct product of two of its subgroups. Let G be a group with subgroups H and K satisfying the following conditions. • G = HK = {hk : h ∈ H, k ∈ K}; • H ∩ K = {e}; • hk = kh for all k ∈ K and h ∈ H. Then G is the internal direct product of H and K. Example 9.24. The group U (8) is the internal direct product of H = {1, 3} and K = {1, 5}. Example 9.25. The dihedral group D6 is an internal direct product of its two subgroups H = {id, r3 } and K = {id, r2 , r4 , s, r2 s, r4 s}. It can easily be shown that K ∼ = S3 ; consequently, D6 ∼ = Z2 × S3 . Example 9.26. Not every group can be written as the internal direct product of two of its proper subgroups. If the group S3 were an internal direct product of its proper subgroups H and K, then one of the subgroups, say H, would have to have order 3. In this case H is the subgroup {(1), (123), (132)}. The subgroup K must have order 2, but no matter which subgroup we choose for K, the condition that hk = kh will never be satisfied for h ∈ H and k ∈ K. Theorem 9.27. Let G be the internal direct product of subgroups H and K. Then G is isomorphic to H × K. Proof. Since G is an internal direct product, we can write any element g ∈ G as g = hk for some h ∈ H and some k ∈ K. Define a map ϕ : G → H × K by ϕ(g) = (h, k). The first problem that we must face is to show that ϕ is a well-defined map; that is, we must show that h and k are uniquely determined by g. Suppose that g = hk = h′ k ′ . Then h−1 h′ = k(k ′ )−1 is in both H and K, so it must be the identity. Therefore, h = h′ and k = k ′ , which proves that ϕ is, indeed, well-defined. To show that ϕ preserves the group operation, let g1 = h1 k1 and g2 = h2 k2 and observe that ϕ(g1 g2 ) = ϕ(h1 k1 h2 k2 ) = ϕ(h1 h2 k1 k2 ) 9.3. EXERCISES 113 = (h1 h2 , k1 k2 ) = (h1 , k1 )(h2 , k2 ) = ϕ(g1 )ϕ(g2 ). We will leave the proof that ϕ is one-to-one and onto as an exercise. Example 9.28. The group Z6 is an internal direct product isomorphic to {0, 2, 4} × {0, 3}. We can extend the definition of an internal direct product of G to a collection of sub- groups H1 , H2 , . . . , Hn of G, by requiring that • G = H1 H2 · · · Hn = {h1 h2 · · · hn : hi ∈ Hi }; • Hi ∩ ⟨∪j̸=i Hj ⟩ = {e}; • hi hj = hj hi for all hi ∈ Hi and hj ∈ Hj . We will leave the proof of the following theorem as an exercise. Theorem 9.29. Let G be∏the internal direct product of subgroups Hi , where i = 1, 2, . . . , n. Then G is isomorphic to i Hi . Sage Sage can quickly determine if two permutation groups are isomorphic, even though this should, in theory, be a very difficult computation. 9.3 Exercises 1. Prove that Z ∼ = nZ for n ̸= 0. ∗ 2. Prove that C is isomorphic to the subgroup of GL2 (R) consisting of matrices of the form ( ) a b . −b a 3. Prove or disprove: U (8) ∼ = Z4 . 4. Prove that U (8) is isomorphic to the group of matrices ( ) ( ) ( ) ( ) 1 0 1 0 −1 0 −1 0 , , , . 0 1 0 −1 0 1 0 −1 5. Show that U (5) is isomorphic to U (10), but U (12) is not. 6. Show that the nth roots of unity are isomorphic to Zn . 7. Show that any cyclic group of order n is isomorphic to Zn . 8. Prove that Q is not isomorphic to Z. 9. Let G = R \ {−1} and define a binary operation on G by a ∗ b = a + b + ab. Prove that G is a group under this operation. Show that (G, ∗) is isomorphic to the multiplicative group of nonzero real numbers. 10. Show that the matrices 1 0 0 1 0 0 0 1 0 0 1 0 0 0 1 1 0 0 0 0 1 0 1 0 0 0 1 114 CHAPTER 9. ISOMORPHISMS 0 0 1 0 0 1 0 1 0 1 0 0 0 1 0 0 0 1 0 1 0 1 0 0 1 0 0 form a group. Find an isomorphism of G with a more familiar group of order 6. 11. Find five non-isomorphic groups of order 8. 12. Prove S4 is not isomorphic to D12 . 13. Let ω = cis(2π/n) be a primitive nth root of unity. Prove that the matrices ( ) ( ) ω 0 0 1 A= and B = 0 ω −1 1 0 generate a multiplicative group isomorphic to Dn . 14. Show that the set of all matrices of the form ( ) ±1 k , 0 1 is a group isomorphic to Dn , where all entries in the matrix are in Zn . 15. List all of the elements of Z4 × Z2 . 16. Find the order of each of the following elements. (a) (3, 4) in Z4 × Z6 (b) (6, 15, 4) in Z30 × Z45 × Z24 (c) (5, 10, 15) in Z25 × Z25 × Z25 (d) (8, 8, 8) in Z10 × Z24 × Z80 17. Prove that D4 cannot be the internal direct product of two of its proper subgroups. 18. Prove that the subgroup of Q∗ consisting of elements of the form 2m 3n for m, n ∈ Z is an internal direct product isomorphic to Z × Z. 19. Prove that S3 × Z2 is isomorphic to D6 . Can you make a conjecture about D2n ? Prove your conjecture. 20. Prove or disprove: Every abelian group of order divisible by 3 contains a subgroup of order 3. 21. Prove or disprove: Every nonabelian group of order divisible by 6 contains a subgroup of order 6. 22. Let G be a group of order 20. If G has subgroups H and K of orders 4 and 5 respectively such that hk = kh for all h ∈ H and k ∈ K, prove that G is the internal direct product of H and K. 23. Prove or disprove the following assertion. Let G, H, and K be groups. If G × K ∼ = H × K, then G ∼ = H. 24. Prove or disprove: There is a noncyclic abelian group of order 51. 25. Prove or disprove: There is a noncyclic abelian group of order 52. 26. Let ϕ : G → H be a group isomorphism. Show that ϕ(x) = eH if and only if x = eG , where eG and eH are the identities of G and H, respectively. 27. Let G ∼ = H. Show that if G is cyclic, then so is H. 28. Prove that any group G of order p, p prime, must be isomorphic to Zp . 9.3. EXERCISES 115 29. Show that Sn is isomorphic to a subgroup of An+2 . 30. Prove that Dn is isomorphic to a subgroup of Sn . 31. Let ϕ : G1 → G2 and ψ : G2 → G3 be isomorphisms. Show that ϕ−1 and ψ ◦ ϕ are both isomorphisms. Using these results, show that the isomorphism of groups determines an equivalence relation on the class of all groups. 32. Prove U (5) ∼ = Z4 . Can you generalize this result for U (p), where p is prime? 33. Write out the permutations associated with each element of S3 in the proof of Cayley’s Theorem. 34. An automorphism of a group G is an isomorphism with itself. Prove that complex conjugation is an automorphism of the additive group of complex numbers; that is, show that the map ϕ(a + bi) = a − bi is an isomorphism from C to C. 35. Prove that a + ib 7→ a − ib is an automorphism of C∗ . 36. Prove that A 7→ B −1 AB is an automorphism of SL2 (R) for all B in GL2 (R). 37. We will denote the set of all automorphisms of G by Aut(G). Prove that Aut(G) is a subgroup of SG , the group of permutations of G. 38. Find Aut(Z6 ). 39. Find Aut(Z). 40. Find two nonisomorphic groups G and H such that Aut(G) ∼ = Aut(H). 41. Let G be a group and g ∈ G. Define a map ig : G → G by ig (x) = gxg −1 . Prove that ig defines an automorphism of G. Such an automorphism is called an inner automorphism. The set of all inner automorphisms is denoted by Inn(G). 42. Prove that Inn(G) is a subgroup of Aut(G). 43. What are the inner automorphisms of the quaternion group Q8 ? Is Inn(G) = Aut(G) in this case? 44. Let G be a group and g ∈ G. Define maps λg : G → G and ρg : G → G by λg (x) = gx and ρg (x) = xg −1 . Show that ig = ρg ◦ λg is an automorphism of G. The isomorphism g 7→ ρg is called the right regular representation of G. 45. Let G be the internal direct product of subgroups H and K. Show that the map ϕ : G → H × K defined by ϕ(g) = (h, k) for g = hk, where h ∈ H and k ∈ K, is one-to-one and onto. 46. Let G and H be isomorphic groups. If G has a subgroup of order n, prove that H must also have a subgroup of order n. 47. If G ∼ = G and H ∼= H, show that G × H ∼ = G × H. 48. Prove that G × H is isomorphic to H × G. 49. Let n1 , . . . , nk be positive integers. Show that ∏ k Zni ∼ = Zn1 ···nk i=1 if and only if gcd(ni , nj ) = 1 for i ̸= j. 50. Prove that A × B is abelian if and only if A and B are abelian. 51. ∏ If G is the internal direct product of H1 , H2 , . . . , Hn , prove that G is isomorphic to H i i . 52. Let H1 and H2 be subgroups of G1 and G2 , respectively. Prove that H1 × H2 is a subgroup of G1 × G2 . 116 CHAPTER 9. ISOMORPHISMS 53. Let m, n ∈ Z. Prove that ⟨m, n⟩ = ⟨d⟩ if and only if d = gcd(m, n). 54. Let m, n ∈ Z. Prove that ⟨m⟩ ∩ ⟨n⟩ = ⟨l⟩ if and only if l = lcm(m, n). 55. Groups of order 2p. In this series of exercises we will classify all groups of order 2p, where p is an odd prime. (a) Assume G is a group of order 2p, where p is an odd prime. If a ∈ G, show that a must have order 1, 2, p, or 2p. (b) Suppose that G has an element of order 2p. Prove that G is isomorphic to Z2p . Hence, G is cyclic. (c) Suppose that G does not contain an element of order 2p. Show that G must contain an element of order p. Hint: Assume that G does not contain an element of order p. (d) Suppose that G does not contain an element of order 2p. Show that G must contain an element of order 2. (e) Let P be a subgroup of G with order p and y ∈ G have order 2. Show that yP = P y. (f) Suppose that G does not contain an element of order 2p and P = ⟨z⟩ is a subgroup of order p generated by z. If y is an element of order 2, then yz = z k y for some 2 ≤ k < p. (g) Suppose that G does not contain an element of order 2p. Prove that G is not abelian. (h) Suppose that G does not contain an element of order 2p and P = ⟨z⟩ is a subgroup of order p generated by z and y is an element of order 2. Show that we can list the elements of G as {z i y j | 0 ≤ i < p, 0 ≤ j < 2}. (i) Suppose that G does not contain an element of order 2p and P = ⟨z⟩ is a subgroup of order p generated by z and y is an element of order 2. Prove that the product (z i y j )(z r y s ) can be expressed as a uniquely as z m y n for some non negative integers m, n. Thus, conclude that there is only one possibility for a non-abelian group of order 2p, it must therefore be the one we have seen already, the dihedral group. 10 Normal Subgroups and Factor Groups If H is a subgroup of a group G, then right cosets are not always the same as left cosets; that is, it is not always the case that gH = Hg for all g ∈ G. The subgroups for which this property holds play a critical role in group theory—they allow for the construction of a new class of groups, called factor or quotient groups. Factor groups may be studied directly or by using homomorphisms, a generalization of isomorphisms. We will study homomorphisms in Chapter 11. 10.1 Factor Groups and Normal Subgroups Normal Subgroups A subgroup H of a group G is normal in G if gH = Hg for all g ∈ G. That is, a normal subgroup of a group G is one in which the right and left cosets are precisely the same. Example 10.1. Let G be an abelian group. Every subgroup H of G is a normal subgroup. Since gh = hg for all g ∈ G and h ∈ H, it will always be the case that gH = Hg. Example 10.2. Let H be the subgroup of S3 consisting of elements (1) and (12). Since (123)H = {(123), (13)} and H(123) = {(123), (23)}, H cannot be a normal subgroup of S3 . However, the subgroup N , consisting of the permu- tations (1), (123), and (132), is normal since the cosets of N are N = {(1), (123), (132)} (12)N = N (12) = {(12), (13), (23)}. The following theorem is fundamental to our understanding of normal subgroups. Theorem 10.3. Let G be a group and N be a subgroup of G. Then the following statements are equivalent. 1. The subgroup N is normal in G. 2. For all g ∈ G, gN g −1 ⊂ N . 3. For all g ∈ G, gN g −1 = N . 117 118 CHAPTER 10. NORMAL SUBGROUPS AND FACTOR GROUPS Proof. (1) ⇒ (2). Since N is normal in G, gN = N g for all g ∈ G. Hence, for a given g ∈ G and n ∈ N , there exists an n′ in N such that gn = n′ g. Therefore, gng −1 = n′ ∈ N or gN g −1 ⊂ N . (2) ⇒ (3). Let g ∈ G. Since gN g −1 ⊂ N , we need only show N ⊂ gN g −1 . For n ∈ N , g ng = g −1 n(g −1 )−1 ∈ N . Hence, g −1 ng = n′ for some n′ ∈ N . Therefore, n = gn′ g −1 is −1 in gN g −1 . (3) ⇒ (1). Suppose that gN g −1 = N for all g ∈ G. Then for any n ∈ N there exists an n′ ∈ N such that gng −1 = n′ . Consequently, gn = n′ g or gN ⊂ N g. Similarly, N g ⊂ gN . Factor Groups If N is a normal subgroup of a group G, then the cosets of N in G form a group G/N under the operation (aN )(bN ) = abN . This group is called the factor or quotient group of G and N . Our first task is to prove that G/N is indeed a group. Theorem 10.4. Let N be a normal subgroup of a group G. The cosets of N in G form a group G/N of order [G : N ]. Proof. The group operation on G/N is (aN )(bN ) = abN . This operation must be shown to be well-defined; that is, group multiplication must be independent of the choice of coset representative. Let aN = bN and cN = dN . We must show that (aN )(cN ) = acN = bdN = (bN )(dN ). Then a = bn1 and c = dn2 for some n1 and n2 in N . Hence, acN = bn1 dn2 N = bn1 dN = bn1 N d = bN d = bdN. The remainder of the theorem is easy: eN = N is the identity and g −1 N is the inverse of gN . The order of G/N is, of course, the number of cosets of N in G. It is very important to remember that the elements in a factor group are sets of elements in the original group. Example 10.5. Consider the normal subgroup of S3 , N = {(1), (123), (132)}. The cosets of N in S3 are N and (12)N . The factor group S3 /N has the following multiplication table. N (12)N N N (12)N (12)N (12)N N This group is isomorphic to Z2 . At first, multiplying cosets seems both complicated and strange; however, notice that S3 /N is a smaller group. The factor group displays a certain amount of information about S3 . Actually, N = A3 , the group of even permutations, and (12)N = {(12), (13), (23)} is the set of odd permutations. The information captured in G/N is parity; that is, multiplying two even or two odd permutations results in an even permutation, whereas multiplying an odd permutation by an even permutation yields an odd permutation. 10.2. THE SIMPLICITY OF THE ALTERNATING GROUP 119 Example 10.6. Consider the normal subgroup 3Z of Z. The cosets of 3Z in Z are 0 + 3Z = {. . . , −3, 0, 3, 6, . . .} 1 + 3Z = {. . . , −2, 1, 4, 7, . . .} 2 + 3Z = {. . . , −1, 2, 5, 8, . . .}. The group Z/3Z is given by the multiplication table below. + 0 + 3Z 1 + 3Z 2 + 3Z 0 + 3Z 0 + 3Z 1 + 3Z 2 + 3Z 1 + 3Z 1 + 3Z 2 + 3Z 0 + 3Z 2 + 3Z 2 + 3Z 0 + 3Z 1 + 3Z In general, the subgroup nZ of Z is normal. The cosets of Z/nZ are nZ 1 + nZ 2 + nZ .. . (n − 1) + nZ. The sum of the cosets k + Z and l + Z is k + l + Z. Notice that we have written our cosets additively, because the group operation is integer addition. Example 10.7. Consider the dihedral group Dn , generated by the two elements r and s, satisfying the relations rn = id s2 = id srs = r−1 . The element r actually generates the cyclic subgroup of rotations, Rn , of Dn . Since srs−1 = srs = r−1 ∈ Rn , the group of rotations is a normal subgroup of Dn ; therefore, Dn /Rn is a group. Since there are exactly two elements in this group, it must be isomorphic to Z2 . 10.2 The Simplicity of the Alternating Group Of special interest are groups with no nontrivial normal subgroups. Such groups are called simple groups. Of course, we already have a whole class of examples of simple groups, Zp , where p is prime. These groups are trivially simple since they have no proper subgroups other than the subgroup consisting solely of the identity. Other examples of simple groups are not so easily found. We can, however, show that the alternating group, An , is simple for n ≥ 5. The proof of this result requires several lemmas. Lemma 10.8. The alternating group An is generated by 3-cycles for n ≥ 3. Proof. To show that the 3-cycles generate An , we need only show that any pair of transpositions can be written as the product of 3-cycles. Since (ab) = (ba), every pair of transpositions must be one of the following: (ab)(ab) = id 120 CHAPTER 10. NORMAL SUBGROUPS AND FACTOR GROUPS (ab)(cd) = (acb)(acd) (ab)(ac) = (acb). Lemma 10.9. Let N be a normal subgroup of An , where n ≥ 3. If N contains a 3-cycle, then N = An . Proof. We will first show that An is generated by 3-cycles of the specific form (ijk), where i and j are fixed in {1, 2, . . . , n} and we let k vary. Every 3-cycle is the product of 3-cycles of this form, since (iaj) = (ija)2 (iab) = (ijb)(ija)2 (jab) = (ijb)2 (ija) (abc) = (ija)2 (ijc)(ijb)2 (ija). Now suppose that N is a nontrivial normal subgroup of An for n ≥ 3 such that N contains a 3-cycle of the form (ija). Using the normality of N , we see that [(ij)(ak)](ija)2 [(ij)(ak)]−1 = (ijk) is in N . Hence, N must contain all of the 3-cycles (ijk) for 1 ≤ k ≤ n. By Lemma 10.8, these 3-cycles generate An ; hence, N = An . Lemma 10.10. For n ≥ 5, every nontrivial normal subgroup N of An contains a 3-cycle. Proof. Let σ be an arbitrary element in a normal subgroup N . There are several possible cycle structures for σ. • σ is a 3-cycle. • σ is the product of disjoint cycles, σ = τ (a1 a2 · · · ar ) ∈ N , where r > 3. • σ is the product of disjoint cycles, σ = τ (a1 a2 a3 )(a4 a5 a6 ). • σ = τ (a1 a2 a3 ), where τ is the product of disjoint 2-cycles. • σ = τ (a1 a2 )(a3 a4 ), where τ is the product of an even number of disjoint 2-cycles. If σ is a 3-cycle, then we are done. If N contains a product of disjoint cycles, σ, and at least one of these cycles has length greater than 3, say σ = τ (a1 a2 · · · ar ), then (a1 a2 a3 )σ(a1 a2 a3 )−1 is in N since N is normal; hence, σ −1 (a1 a2 a3 )σ(a1 a2 a3 )−1 is also in N . Since σ −1 (a1 a2 a3 )σ(a1 a2 a3 )−1 = σ −1 (a1 a2 a3 )σ(a1 a3 a2 ) = (a1 a2 · · · ar )−1 τ −1 (a1 a2 a3 )τ (a1 a2 · · · ar )(a1 a3 a2 ) = (a1 ar ar−1 · · · a2 )(a1 a2 a3 )(a1 a2 · · · ar )(a1 a3 a2 ) = (a1 a3 ar ), 10.2. THE SIMPLICITY OF THE ALTERNATING GROUP 121 N must contain a 3-cycle; hence, N = An . Now suppose that N contains a disjoint product of the form σ = τ (a1 a2 a3 )(a4 a5 a6 ). Then σ −1 (a1 a2 a4 )σ(a1 a2 a4 )−1 ∈ N since (a1 a2 a4 )σ(a1 a2 a4 )−1 ∈ N. So σ −1 (a1 a2 a4 )σ(a1 a2 a4 )−1 = [τ (a1 a2 a3 )(a4 a5 a6 )]−1 (a1 a2 a4 )τ (a1 a2 a3 )(a4 a5 a6 )(a1 a2 a4 )−1 = (a4 a6 a5 )(a1 a3 a2 )τ −1 (a1 a2 a4 )τ (a1 a2 a3 )(a4 a5 a6 )(a1 a4 a2 ) = (a4 a6 a5 )(a1 a3 a2 )(a1 a2 a4 )(a1 a2 a3 )(a4 a5 a6 )(a1 a4 a2 ) = (a1 a4 a2 a6 a3 ). So N contains a disjoint cycle of length greater than 3, and we can apply the previous case. Suppose N contains a disjoint product of the form σ = τ (a1 a2 a3 ), where τ is the product of disjoint 2-cycles. Since σ ∈ N , σ 2 ∈ N , and σ 2 = τ (a1 a2 a3 )τ (a1 a2 a3 ) = (a1 a3 a2 ). So N contains a 3-cycle. The only remaining possible case is a disjoint product of the form σ = τ (a1 a2 )(a3 a4 ), where τ is the product of an even number of disjoint 2-cycles. But σ −1 (a1 a2 a3 )σ(a1 a2 a3 )−1 is in N since (a1 a2 a3 )σ(a1 a2 a3 )−1 is in N ; and so σ −1 (a1 a2 a3 )σ(a1 a2 a3 )−1 = τ −1 (a1 a2 )(a3 a4 )(a1 a2 a3 )τ (a1 a2 )(a3 a4 )(a1 a2 a3 )−1 = (a1 a3 )(a2 a4 ). Since n ≥ 5, we can find b ∈ {1, 2, . . . , n} such that b ̸= a1 , a2 , a3 , a4 . Let µ = (a1 a3 b). Then µ−1 (a1 a3 )(a2 a4 )µ(a1 a3 )(a2 a4 ) ∈ N and µ−1 (a1 a3 )(a2 a4 )µ(a1 a3 )(a2 a4 ) = (a1 ba3 )(a1 a3 )(a2 a4 )(a1 a3 b)(a1 a3 )(a2 a4 ) = (a1 a3 b). Therefore, N contains a 3-cycle. This completes the proof of the lemma. Theorem 10.11. The alternating group, An , is simple for n ≥ 5. Proof. Let N be a normal subgroup of An . By Lemma 10.10, N contains a 3-cycle. By Lemma 10.9, N = An ; therefore, An contains no proper nontrivial normal subgroups for n ≥ 5. 122 CHAPTER 10. NORMAL SUBGROUPS AND FACTOR GROUPS Sage Sage can easily determine if a subgroup is normal or not. If so, it can create the quotient group. However, the construction creates a new permuation group, isomorphic to the quotient group, so its utility is limited. Historical Note One of the foremost problems of group theory has been to classify all simple finite groups. This problem is over a century old and has been solved only in the last few decades of the twentieth century. In a sense, finite simple groups are the building blocks of all finite groups. The first nonabelian simple groups to be discovered were the alternating groups. Galois was the first to prove that A5 was simple. Later, mathematicians such as C. Jordan and L. E. Dickson found several infinite families of matrix groups that were simple. Other families of simple groups were discovered in the 1950s. At the turn of the century, William Burnside conjectured that all nonabelian simple groups must have even order. In 1963, W. Feit and J. Thompson proved Burnside’s conjecture and published their results in the paper “Solvability of Groups of Odd Order,” which appeared in the Pacific Journal of Mathematics. Their proof, running over 250 pages, gave impetus to a program in the 1960s and 1970s to classify all finite simple groups. Daniel Gorenstein was the organizer of this remarkable effort. One of the last simple groups was the “Monster,” discovered by R. Greiss. The Monster, a 196,833 × 196,833 matrix group, is one of the 26 sporadic, or special, simple groups. These sporadic simple groups are groups that fit into no infinite family of simple groups. Some of the sporadic groups play an important role in physics. 10.3 Exercises 1. For each of the following groups G, determine whether H is a normal subgroup of G. If H is a normal subgroup, write out a Cayley table for the factor group G/H. (a) G = S4 and H = A4 (b) G = A5 and H = {(1), (123), (132)} (c) G = S4 and H = D4 (d) G = Q8 and H = {1, −1, I, −I} (e) G = Z and H = 5Z 2. Find all the subgroups of D4 . Which subgroups are normal? What are all the factor groups of D4 up to isomorphism? 3. Find all the subgroups of the quaternion group, Q8 . Which subgroups are normal? What are all the factor groups of Q8 up to isomorphism? 4. Let T be the group of nonsingular upper triangular 2 × 2 matrices with entries in R; that is, matrices of the form ( ) a b , 0 c where a, b, c ∈ R and ac ̸= 0. Let U consist of matrices of the form ( ) 1 x , 0 1 where x ∈ R. 10.3. EXERCISES 123 (a) Show that U is a subgroup of T . (b) Prove that U is abelian. (c) Prove that U is normal in T . (d) Show that T /U is abelian. (e) Is T normal in GL2 (R)? 5. Show that the intersection of two normal subgroups is a normal subgroup. 6. If G is abelian, prove that G/H must also be abelian. 7. Prove or disprove: If H is a normal subgroup of G such that H and G/H are abelian, then G is abelian. 8. If G is cyclic, prove that G/H must also be cyclic. 9. Prove or disprove: If H and G/H are cyclic, then G is cyclic. 10. Let H be a subgroup of index 2 of a group G. Prove that H must be a normal subgroup of G. Conclude that Sn is not simple for n ≥ 3. 11. If a group G has exactly one subgroup H of order k, prove that H is normal in G. 12. Define the centralizer of an element g in a group G to be the set C(g) = {x ∈ G : xg = gx}. Show that C(g) is a subgroup of G. If g generates a normal subgroup of G, prove that C(g) is normal in G. 13. Recall that the center of a group G is the set Z(G) = {x ∈ G : xg = gx for all g ∈ G}. (a) Calculate the center of S3 . (b) Calculate the center of GL2 (R). (c) Show that the center of any group G is a normal subgroup of G. (d) If G/Z(G) is cyclic, show that G is abelian. 14. Let G be a group and let G′ = ⟨aba−1 b−1 ⟩; that is, G′ is the subgroup of all finite products of elements in G of the form aba−1 b−1 . The subgroup G′ is called the commutator subgroup of G. (a) Show that G′ is a normal subgroup of G. (b) Let N be a normal subgroup of G. Prove that G/N is abelian if and only if N contains the commutator subgroup of G. 11 Homomorphisms One of the basic ideas of algebra is the concept of a homomorphism, a natural generalization of an isomorphism. If we relax the requirement that an isomorphism of groups be bijective, we have a homomorphism. 11.1 Group Homomorphisms A homomorphism between groups (G, ·) and (H, ◦) is a map ϕ : G → H such that ϕ(g1 · g2 ) = ϕ(g1 ) ◦ ϕ(g2 ) for g1 , g2 ∈ G. The range of ϕ in H is called the homomorphic image of ϕ. Two groups are related in the strongest possible way if they are isomorphic; however, a weaker relationship may exist between two groups. For example, the symmetric group Sn and the group Z2 are related by the fact that Sn can be divided into even and odd permu- tations that exhibit a group structure like that Z2 , as shown in the following multiplication table. even odd even even odd odd odd even We use homomorphisms to study relationships such as the one we have just described. Example 11.1. Let G be a group and g ∈ G. Define a map ϕ : Z → G by ϕ(n) = g n . Then ϕ is a group homomorphism, since ϕ(m + n) = g m+n = g m g n = ϕ(m)ϕ(n). This homomorphism maps Z onto the cyclic subgroup of G generated by g. Example 11.2. Let G = GL2 (R). If ( ) a b A= c d is in G, then the determinant is nonzero; that is, det(A) = ad − bc ̸= 0. Also, for any two elements A and B in G, det(AB) = det(A) det(B). Using the determinant, we can define a homomorphism ϕ : GL2 (R) → R∗ by A 7→ det(A). 124 11.1. GROUP HOMOMORPHISMS 125 Example 11.3. Recall that the circle group T consists of all complex numbers z such that |z| = 1. We can define a homomorphism ϕ from the additive group of real numbers R to T by ϕ : θ 7→ cos θ + i sin θ. Indeed, ϕ(α + β) = cos(α + β) + i sin(α + β) = (cos α cos β − sin α sin β) + i(sin α cos β + cos α sin β) = (cos α + i sin α)(cos β + i sin β) = ϕ(α)ϕ(β). Geometrically, we are simply wrapping the real line around the circle in a group-theoretic fashion. The following proposition lists some basic properties of group homomorphisms. Proposition 11.4. Let ϕ : G1 → G2 be a homomorphism of groups. Then 1. If e is the identity of G1 , then ϕ(e) is the identity of G2 ; 2. For any element g ∈ G1 , ϕ(g −1 ) = [ϕ(g)]−1 ; 3. If H1 is a subgroup of G1 , then ϕ(H1 ) is a subgroup of G2 ; 4. If H2 is a subgroup of G2 , then ϕ−1 (H2 ) = {g ∈ G1 : ϕ(g) ∈ H2 } is a subgroup of G1 . Furthermore, if H2 is normal in G2 , then ϕ−1 (H2 ) is normal in G1 . Proof. (1) Suppose that e and e′ are the identities of G1 and G2 , respectively; then e′ ϕ(e) = ϕ(e) = ϕ(ee) = ϕ(e)ϕ(e). By cancellation, ϕ(e) = e′ . (2) This statement follows from the fact that ϕ(g −1 )ϕ(g) = ϕ(g −1 g) = ϕ(e) = e′ . (3) The set ϕ(H1 ) is nonempty since the identity of G2 is in ϕ(H1 ). Suppose that H1 is a subgroup of G1 and let x and y be in ϕ(H1 ). There exist elements a, b ∈ H1 such that ϕ(a) = x and ϕ(b) = y. Since xy −1 = ϕ(a)[ϕ(b)]−1 = ϕ(ab−1 ) ∈ ϕ(H1 ), ϕ(H1 ) is a subgroup of G2 by Proposition 3.31. (4) Let H2 be a subgroup of G2 and define H1 to be ϕ−1 (H2 ); that is, H1 is the set of all g ∈ G1 such that ϕ(g) ∈ H2 . The identity is in H1 since ϕ(e) = e′ . If a and b are in H1 , then ϕ(ab−1 ) = ϕ(a)[ϕ(b)]−1 is in H2 since H2 is a subgroup of G2 . Therefore, ab−1 ∈ H1 and H1 is a subgroup of G1 . If H2 is normal in G2 , we must show that g −1 hg ∈ H1 for h ∈ H1 and g ∈ G1 . But ϕ(g −1 hg) = [ϕ(g)]−1 ϕ(h)ϕ(g) ∈ H2 , since H2 is a normal subgroup of G2 . Therefore, g −1 hg ∈ H1 . Let ϕ : G → H be a group homomorphism and suppose that e is the identity of H. By Proposition 11.4, ϕ−1 ({e}) is a subgroup of G. This subgroup is called the kernel of ϕ and will be denoted by ker ϕ. In fact, this subgroup is a normal subgroup of G since the trivial subgroup is normal in H. We state this result in the following theorem, which says that with every homomorphism of groups we can naturally associate a normal subgroup. 126 CHAPTER 11. HOMOMORPHISMS Theorem 11.5. Let ϕ : G → H be a group homomorphism. Then the kernel of ϕ is a normal subgroup of G. Example 11.6. Let us examine the homomorphism ϕ : GL2 (R) → R∗ defined by A 7→ det(A). Since 1 is the identity of R∗ , the kernel of this homomorphism is all 2 × 2 matrices having determinant one. That is, ker ϕ = SL2 (R). Example 11.7. The kernel of the group homomorphism ϕ : R → C∗ defined by ϕ(θ) = cos θ + i sin θ is {2πn : n ∈ Z}. Notice that ker ϕ ∼ = Z. Example 11.8. Suppose that we wish to determine all possible homomorphisms ϕ from Z7 to Z12 . Since the kernel of ϕ must be a subgroup of Z7 , there are only two possible kernels, {0} and all of Z7 . The image of a subgroup of Z7 must be a subgroup of Z12 . Hence, there is no injective homomorphism; otherwise, Z12 would have a subgroup of order 7, which is impossible. Consequently, the only possible homomorphism from Z7 to Z12 is the one mapping all elements to zero. Example 11.9. Let G be a group. Suppose that g ∈ G and ϕ is the homomorphism from Z to G given by ϕ(n) = g n . If the order of g is infinite, then the kernel of this homomorphism is {0} since ϕ maps Z onto the cyclic subgroup of G generated by g. However, if the order of g is finite, say n, then the kernel of ϕ is nZ. 11.2 The Isomorphism Theorems Although it is not evident at first, factor groups correspond exactly to homomorphic images, and we can use factor groups to study homomorphisms. We already know that with every group homomorphism ϕ : G → H we can associate a normal subgroup of G, ker ϕ. The con- verse is also true; that is, every normal subgroup of a group G gives rise to homomorphism of groups. Let H be a normal subgroup of G. Define the natural or canonical homomorphism ϕ : G → G/H by ϕ(g) = gH. This is indeed a homomorphism, since ϕ(g1 g2 ) = g1 g2 H = g1 Hg2 H = ϕ(g1 )ϕ(g2 ). The kernel of this homomorphism is H. The following theorems describe the relationships between group homomorphisms, normal subgroups, and factor groups. Theorem 11.10 First Isomorphism Theorem. If ψ : G → H is a group homomorphism with K = ker ψ, then K is normal in G. Let ϕ : G → G/K be the canonical homomorphism. Then there exists a unique isomorphism η : G/K → ψ(G) such that ψ = ηϕ. Proof. We already know that K is normal in G. Define η : G/K → ψ(G) by η(gK) = ψ(g). We first show that η is a well-defined map. If g1 K = g2 K, then for some k ∈ K, g1 k = g2 ; consequently, η(g1 K) = ψ(g1 ) = ψ(g1 )ψ(k) = ψ(g1 k) = ψ(g2 ) = η(g2 K). 11.2. THE ISOMORPHISM THEOREMS 127 Thus, η does not depend on the choice of coset representatives and the map η : G/K → ψ(G) is uniquely defined since ψ = ηϕ. We must also show that η is a homomorphism, but η(g1 Kg2 K) = η(g1 g2 K) = ψ(g1 g2 ) = ψ(g1 )ψ(g2 ) = η(g1 K)η(g2 K). Clearly, η is onto ψ(G). To show that η is one-to-one, suppose that η(g1 K) = η(g2 K). Then ψ(g1 ) = ψ(g2 ). This implies that ψ(g1−1 g2 ) = e, or g1−1 g2 is in the kernel of ψ; hence, g1−1 g2 K = K; that is, g1 K = g2 K. Mathematicians often use diagrams called commutative diagrams to describe such theorems. The following diagram “commutes” since ψ = ηϕ. ψ G H ϕ η G/K Example 11.11. Let G be a cyclic group with generator g. Define a map ϕ : Z → G by n 7→ g n . This map is a surjective homomorphism since ϕ(m + n) = g m+n = g m g n = ϕ(m)ϕ(n). Clearly ϕ is onto. If |g| = m, then g m = e. Hence, ker ϕ = mZ and Z/ ker ϕ = Z/mZ ∼ = G. On the other hand, if the order of g is infinite, then ker ϕ = 0 and ϕ is an isomorphism of G and Z. Hence, two cyclic groups are isomorphic exactly when they have the same order. Up to isomorphism, the only cyclic groups are Z and Zn . Theorem 11.12 Second Isomorphism Theorem. Let H be a subgroup of a group G (not necessarily normal in G) and N a normal subgroup of G. Then HN is a subgroup of G, H ∩ N is a normal subgroup of H, and H/H ∩ N ∼ = HN /N. Proof. We will first show that HN = {hn : h ∈ H, n ∈ N } is a subgroup of G. Suppose that h1 n1 , h2 n2 ∈ HN . Since N is normal, (h2 )−1 n1 h2 ∈ N . So (h1 n1 )(h2 n2 ) = h1 h2 ((h2 )−1 n1 h2 )n2 is in HN . The inverse of hn ∈ HN is in HN since (hn)−1 = n−1 h−1 = h−1 (hn−1 h−1 ). 128 CHAPTER 11. HOMOMORPHISMS Next, we prove that H ∩ N is normal in H. Let h ∈ H and n ∈ H ∩ N . Then h−1 nh ∈ H since each element is in H. Also, h−1 nh ∈ N since N is normal in G; therefore, h−1 nh ∈ H ∩ N . Now define a map ϕ from H to HN /N by h 7→ hN . The map ϕ is onto, since any coset hnN = hN is the image of h in H. We also know that ϕ is a homomorphism because ϕ(hh′ ) = hh′ N = hN h′ N = ϕ(h)ϕ(h′ ). By the First Isomorphism Theorem, the image of ϕ is isomorphic to H/ ker ϕ; that is, HN /N = ϕ(H) ∼ = H/ ker ϕ. Since ker ϕ = {h ∈ H : h ∈ N } = H ∩ N, HN /N = ϕ(H) ∼ = H/H ∩ N . Theorem 11.13 Correspondence Theorem. Let N be a normal subgroup of a group G. Then H 7→ H/N is a one-to-one correspondence between the set of subgroups H containing N and the set of subgroups of G/N . Furthermore, the normal subgroups of G containing N correspond to normal subgroups of G/N . Proof. Let H be a subgroup of G containing N . Since N is normal in H, H/N makes sense. Let aN and bN be elements of H/N . Then (aN )(b−1 N ) = ab−1 N ∈ H/N ; hence, H/N is a subgroup ofG/N . Let S be a subgroup of G/N . This subgroup is a set of cosets of N . If H = {g ∈ G : gN ∈ S}, then for h1 , h2 ∈ H, we have that (h1 N )(h2 N ) = h1 h2 N ∈ S and h−1 1 N ∈ S. Therefore, H must be a subgroup of G. Clearly, H contains N . Therefore, S = H/N . Consequently, the map H 7→ H/N is onto. Suppose that H1 and H2 are subgroups of G containing N such that H1 /N = H2 /N . If h1 ∈ H1 , then h1 N ∈ H1 /N . Hence, h1 N = h2 N ⊂ H2 for some h2 in H2 . However, since N is contained in H2 , we know that h1 ∈ H2 or H1 ⊂ H2 . Similarly, H2 ⊂ H1 . Since H1 = H2 , the map H 7→ H/N is one-to-one. Suppose that H is normal in G and N is a subgroup of H. Then it is easy to verify that the map G/N → G/H defined by gN 7→ gH is a homomorphism. The kernel of this homomorphism is H/N , which proves that H/N is normal in G/N . Conversely, suppose that H/N is normal in G/N . The homomorphism given by G/N G → G/N → H/N has kernel H. Hence, H must be normal in G. Notice that in the course of the proof of Theorem 11.13, we have also proved the following theorem. Theorem 11.14 Third Isomorphism Theorem. Let G be a group and N and H be normal subgroups of G with N ⊂ H. Then G/N G/H ∼ = . H/N Example 11.15. By the Third Isomorphism Theorem, Z/mZ ∼ = (Z/mnZ)/(mZ/mnZ). Since |Z/mnZ| = mn and |Z/mZ| = m, we have |mZ/mnZ| = n. 11.3. EXERCISES 129 Sage Sage can create homomorphisms between groups, which can be used directly as functions, and then queried for their kernels and images. So there is great potential for exploring the many fundamental relationships between groups, normal subgroups, quotient groups and properties of homomorphisms. 11.3 Exercises 1. Prove that det(AB) = det(A) det(B) for A, B ∈ GL2 (R). This shows that the determinant is a homomorphism from GL2 (R) to R∗ . 2. Which of the following maps are homomorphisms? If the map is a homomorphism, what is the kernel? (a) ϕ : R∗ → GL2 (R) defined by ( ) 1 0 ϕ(a) = 0 a (b) ϕ : R → GL2 (R) defined by ( ) 1 0 ϕ(a) = a 1 (c) ϕ : GL2 (R) → R defined by (( )) a b ϕ =a+d c d (d) ϕ : GL2 (R) → R∗ defined by (( )) a b ϕ = ad − bc c d (e) ϕ : M2 (R) → R defined by (( )) a b ϕ = b, c d where M2 (R) is the additive group of 2 × 2 matrices with entries in R. 3. Let A be an m × n matrix. Show that matrix multiplication, x 7→ Ax, defines a homomorphism ϕ : Rn → Rm . 4. Let ϕ : Z → Z be given by ϕ(n) = 7n. Prove that ϕ is a group homomorphism. Find the kernel and the image of ϕ. 5. Describe all of the homomorphisms from Z24 to Z18 . 6. Describe all of the homomorphisms from Z to Z12 . 7. In the group Z24 , let H = ⟨4⟩ and N = ⟨6⟩. (a) List the elements in HN (we usually write H + N for these additive groups) and H ∩ N. (b) List the cosets in HN /N , showing the elements in each coset. (c) List the cosets in H/(H ∩ N ), showing the elements in each coset. 130 CHAPTER 11. HOMOMORPHISMS (d) Give the correspondence between HN /N and H/(H ∩ N ) described in the proof of the Second Isomorphism Theorem. 8. If G is an abelian group and n ∈ N, show that ϕ : G → G defined by g 7→ g n is a group homomorphism. 9. If ϕ : G → H is a group homomorphism and G is abelian, prove that ϕ(G) is also abelian. 10. If ϕ : G → H is a group homomorphism and G is cyclic, prove that ϕ(G) is also cyclic. 11. Show that a homomorphism defined on a cyclic group is completely determined by its action on the generator of the group. 12. If a group G has exactly one subgroup H of order k, prove that H is normal in G. 13. Prove or disprove: Q/Z ∼ = Q. 14. Let G be a finite group and N a normal subgroup of G. If H is a subgroup of G/N , prove that ϕ−1 (H) is a subgroup in G of order |H|·|N |, where ϕ : G → G/N is the canonical homomorphism. 15. Let G1 and G2 be groups, and let H1 and H2 be normal subgroups of G1 and G2 respectively. Let ϕ : G1 → G2 be a homomorphism. Show that ϕ induces a natural homomorphism ϕ : (G1 /H1 ) → (G2 /H2 ) if ϕ(H1 ) ⊂ H2 . 16. If H and K are normal subgroups of G and H ∩ K = {e}, prove that G is isomorphic to a subgroup of G/H × G/K. 17. Let ϕ : G1 → G2 be a surjective group homomorphism. Let H1 be a normal subgroup of G1 and suppose that ϕ(H1 ) = H2 . Prove or disprove that G1 /H1 ∼ = G2 /H2 . 18. Let ϕ : G → H be a group homomorphism. Show that ϕ is one-to-one if and only if ϕ−1 (e) = {e}. 19. Given a homomorphism ϕ : G → H define a relation ∼ on G by a ∼ b if ϕ(a) = ϕ(b) for a, b ∈ G. Show this relation is an equivalence relation and describe the equivalence classes. 11.4 Additional Exercises: Automorphisms 1. Let Aut(G) be the set of all automorphisms of G; that is, isomorphisms from G to itself. Prove this set forms a group and is a subgroup of the group of permutations of G; that is, Aut(G) ≤ SG . 2. An inner automorphism of G, ig : G → G, is defined by the map ig (x) = gxg −1 , for g ∈ G. Show that ig ∈ Aut(G). 3. The set of all inner automorphisms is denoted by Inn(G). Show that Inn(G) is a subgroup of Aut(G). 4. Find an automorphism of a group G that is not an inner automorphism. 5. Let G be a group and ig be an inner automorphism of G, and define a map G → Aut(G) 11.4. ADDITIONAL EXERCISES: AUTOMORPHISMS 131 by g 7→ ig . Prove that this map is a homomorphism with image Inn(G) and kernel Z(G). Use this result to conclude that G/Z(G) ∼ = Inn(G). 6. Compute Aut(S3 ) and Inn(S3 ). Do the same thing for D4 . 7. Find all of the homomorphisms ϕ : Z → Z. What is Aut(Z)? 8. Find all of the automorphisms of Z8 . Prove that Aut(Z8 ) ∼ = U (8). 9. For k ∈ Zn , define a map ϕk : Zn → Zn by a 7→ ka. Prove that ϕk is a homomorphism. 10. Prove that ϕk is an isomorphism if and only if k is a generator of Zn . 11. Show that every automorphism of Zn is of the form ϕk , where k is a generator of Zn . 12. Prove that ψ : U (n) → Aut(Zn ) is an isomorphism, where ψ : k 7→ ϕk . 12 Matrix Groups and Symmetry When Felix Klein (1849–1925) accepted a chair at the University of Erlangen, he outlined in his inaugural address a program to classify different geometries. Central to Klein’s program was the theory of groups: he considered geometry to be the study of properties that are left invariant under transformation groups. Groups, especially matrix groups, have now become important in the study of symmetry and have found applications in such disciplines as chemistry and physics. In the first part of this chapter, we will examine some of the classical matrix groups, such as the general linear group, the special linear group, and the orthogonal group. We will then use these matrix groups to investigate some of the ideas behind geometric symmetry. 12.1 Matrix Groups Some Facts from Linear Algebra Before we study matrix groups, we must recall some basic facts from linear algebra. One of the most fundamental ideas of linear algebra is that of a linear transformation. A linear transformation or linear map T : Rn → Rm is a map that preserves vector addition and scalar multiplication; that is, for vectors x and y in Rn and a scalar α ∈ R, T (x + y) = T (x) + T (y) T (αy) = αT (y). An m × n matrix with entries in R represents a linear transformation from Rn to Rm . If we write vectors x = (x1 , . . . , xn )t and y = (y1 , . . . , yn )t in Rn as column matrices, then an m × n matrix a11 a12 · · · a1n a21 a22 · · · a2n A= . .. . .. .. . . . . am1 am2 · · · amn maps the vectors to Rm linearly by matrix multiplication. Observe that if α is a real number, A(x + y) = Ax + Ay and αAx = A(αx), where x1 x2 x = . . .. xn 132 12.1. MATRIX GROUPS 133 We will often abbreviate the matrix A by writing (aij ). Conversely, if T : Rn → Rm is a linear map, we can associate a matrix A with T by considering what T does to the vectors e1 = (1, 0, . . . , 0)t e2 = (0, 1, . . . , 0)t .. . en = (0, 0, . . . , 1)t . We can write any vector x = (x1 , . . . , xn )t as x1 e1 + x2 e2 + · · · + xn en . Consequently, if T (e1 ) = (a11 , a21 , . . . , am1 )t , T (e2 ) = (a12 , a22 , . . . , am2 )t , .. . T (en ) = (a1n , a2n , . . . , amn )t , then T (x) = T (x1 e1 + x2 e2 + · · · + xn en ) = x1 T (e1 ) + x2 T (e2 ) + · · · + xn T (en ) ( n )t ∑ ∑ n = a1k xk , . . . , amk xk k=1 k=1 = Ax. Example 12.1. If we let T : R2 → R2 be the map given by T (x1 , x2 ) = (2x1 + 5x2 , −4x1 + 3x2 ), the axioms that T must satisfy to be a linear transformation are easily verified. The column vectors T e1 = (2, −4)t and T e2 = (5, 3)t tell us that T is given by the matrix ( ) 2 5 A= . −4 3 Since we are interested in groups of matrices, we need to know which matrices have multiplicative inverses. Recall that an n × n matrix A is invertible exactly when there exists another matrix A−1 such that AA−1 = A−1 A = I, where 1 0 ··· 0 0 1 · · · 0 I = . . . . .. .. . . .. 0 0 ··· 1 is the n × n identity matrix. From linear algebra we know that A is invertible if and only if the determinant of A is nonzero. Sometimes an invertible matrix is said to be nonsingular. 134 CHAPTER 12. MATRIX GROUPS AND SYMMETRY Example 12.2. If A is the matrix ( ) 2 1 , 5 3 then the inverse of A is ( ) −1 3 −1 A = . −5 2 We are guaranteed that A−1 exists, since det(A) = 2 · 3 − 5 · 1 = 1 is nonzero. Some other facts about determinants will also prove useful in the course of this chapter. Let A and B be n × n matrices. From linear algebra we have the following properties of determinants. • The determinant is a homomorphism into the multiplicative group of real numbers; that is, det(AB) = (det A)(det B). • If A is an invertible matrix, then det(A−1 ) = 1/ det A. • If we define the transpose of a matrix A = (aij ) to be At = (aji ), then det(At ) = det A. • Let T be the linear transformation associated with an n × n matrix A. Then T multiplies volumes by a factor of | det A|. In the case of R2 , this means that T multiplies areas by | det A|. Linear maps, matrices, and determinants are covered in any elementary linear algebra text; however, if you have not had a course in linear algebra, it is a straightforward process to verify these properties directly for 2 × 2 matrices, the case with which we are most concerned. The General and Special Linear Groups The set of all n × n invertible matrices forms a group called the general linear group. We will denote this group by GLn (R). The general linear group has several important subgroups. The multiplicative properties of the determinant imply that the set of matrices with determinant one is a subgroup of the general linear group. Stated another way, suppose that det(A) = 1 and det(B) = 1. Then det(AB) = det(A) det(B) = 1 and det(A−1 ) = 1/ det A = 1. This subgroup is called the special linear group and is denoted by SLn (R). Example 12.3. Given a 2 × 2 matrix ( ) a b A= , c d the determinant of A is ad − bc. The group GL2 (R) consists of those matrices in which ad − bc ̸= 0. The inverse of A is ( ) −1 1 d −b A = . ad − bc −c a If A is in SL2 (R), then ( ) d −b A−1 = . −c a 12.1. MATRIX GROUPS 135 Geometrically, SL2 (R) is the group that preserves the areas of parallelograms. Let ( ) 1 1 A= 0 1 be in SL2 (R). In Figure 12.4, the unit square corresponding to the vectors x = (1, 0)t and y = (0, 1)t is taken by A to the parallelogram with sides (1, 0)t and (1, 1)t ; that is, Ax = (1, 0)t and Ay = (1, 1)t . Notice that these two parallelograms have the same area. y y (1, 1) (0, 1) (1, 0) x (1, 0) x Figure 12.4: SL2 (R) acting on the unit square The Orthogonal Group O(n) Another subgroup of GLn (R) is the orthogonal group. A matrix A is orthogonal if A−1 = At . The orthogonal group consists of the set of all orthogonal matrices. We write O(n) for the n × n orthogonal group. We leave as an exercise the proof that O(n) is a subgroup of GLn (R). Example 12.5. The following matrices are orthogonal: √ √ ( ) ( √ ) −1/ 2 0 1/ 2 3/5 −4/5 1/2 − 3/2 √ √ √ , √ , 1/ 6 −2/ 6 1/ 6 . 4/5 3/5 3/2 1/2 √ √ √ 1/ 3 1/ 3 1/ 3 There is a more geometric way of viewing the group O(n). The orthogonal matrices are exactly those matrices that preserve the length of vectors. We can define the length of a vector using the Euclidean inner product, or dot product, of two vectors. The Euclidean inner product of two vectors x = (x1 , . . . , xn )t and y = (y1 , . . . , yn )t is y1 y2 ⟨x, y⟩ = xt y = (x1 , x2 , . . . , xn ) . = x1 y1 + · · · + xn yn . .. yn We define the length of a vector x = (x1 , . . . , xn )t to be √ √ ∥x∥ = ⟨x, x⟩ = x21 + · · · + x2n . Associated with the notion of the length of a vector is the idea of the distance between two vectors. We define the distance between two vectors x and y to be ∥x − y∥. We leave as an exercise the proof of the following proposition about the properties of Euclidean inner products. 136 CHAPTER 12. MATRIX GROUPS AND SYMMETRY Proposition 12.6. Let x, y, and w be vectors in Rn and α ∈ R. Then 1. ⟨x, y⟩ = ⟨y, x⟩. 2. ⟨x, y + w⟩ = ⟨x, y⟩ + ⟨x, w⟩. 3. ⟨αx, y⟩ = ⟨x, αy⟩ = α⟨x, y⟩. 4. ⟨x, x⟩ ≥ 0 with equality exactly when x = 0. 5. If ⟨x, y⟩ = 0 for all x in Rn , then y = 0. √ Example 12.7. The vector x = (3, 4)t has length 32 + 42 = 5. We can also see that the orthogonal matrix ( ) 3/5 −4/5 A= 4/5 3/5 preserves the length of this vector. The vector Ax = (−7/5, 24/5)t also has length 5. Since det(AAt ) = det(I) = 1 and det(A) = det(At ), the determinant of any orthogonal matrix is either 1 or −1. Consider the column vectors a1j a2j aj = . .. anj of the orthogonal matrix A = (aij ). Since AAt = I, ⟨ar , as ⟩ = δrs , where { 1 r=s δrs = ̸ s 0 r= is the Kronecker delta. Accordingly, column vectors of an orthogonal matrix all have length 1; and the Euclidean inner product of distinct column vectors is zero. Any set of vectors satisfying these properties is called an orthonormal set. Conversely, given an n×n matrix A whose columns form an orthonormal set, it follows that A−1 = At . We say that a matrix A is distance-preserving, length-preserving, or inner product- preserving when ∥T x − T y∥ = ∥x − y∥, ∥T x∥ = ∥x∥, or ⟨T x, T y⟩ = ⟨x, y⟩, respectively. The following theorem, which characterizes the orthogonal group, says that these notions are the same. Theorem 12.8. Let A be an n × n matrix. The following statements are equivalent. 1. The columns of the matrix A form an orthonormal set. 2. A−1 = At . 3. For vectors x and y, ⟨Ax, Ay⟩ = ⟨x, y⟩. 4. For vectors x and y, ∥Ax − Ay∥ = ∥x − y∥. 5. For any vector x, ∥Ax∥ = ∥x∥. 12.1. MATRIX GROUPS 137 Proof. We have already shown (1) and (2) to be equivalent. (2) ⇒ (3). ⟨Ax, Ay⟩ = (Ax)t Ay = xt At Ay = xt y = ⟨x, y⟩. (3) ⇒ (2). Since ⟨x, x⟩ = ⟨Ax, Ax⟩ = xt At Ax = ⟨x, At Ax⟩, we know that ⟨x, (At A − I)x⟩ = 0 for all x. Therefore, At A − I = 0 or A−1 = At . (3) ⇒ (4). If A is inner product-preserving, then A is distance-preserving, since ∥Ax − Ay∥2 = ∥A(x − y)∥2 = ⟨A(x − y), A(x − y)⟩ = ⟨x − y, x − y⟩ = ∥x − y∥2 . (4) ⇒ (5). If A is distance-preserving, then A is length-preserving. Letting y = 0, we have ∥Ax∥ = ∥Ax − Ay∥ = ∥x − y∥ = ∥x∥. (5) ⇒ (3). We use the following identity to show that length-preserving implies inner product-preserving: 1[ ] ⟨x, y⟩ = ∥x + y∥2 − ∥x∥2 − ∥y∥2 . 2 Observe that 1[ ] ⟨Ax, Ay⟩ = ∥Ax + Ay∥2 − ∥Ax∥2 − ∥Ay∥2 2 1[ ] = ∥A(x + y)∥2 − ∥Ax∥2 − ∥Ay∥2 2 1[ ] = ∥x + y∥2 − ∥x∥2 − ∥y∥2 2 = ⟨x, y⟩. y y (sin θ, − cos θ) (a, b) (cos θ, sin θ) θ x x (a, −b) Figure 12.9: O(2) acting on R2 138 CHAPTER 12. MATRIX GROUPS AND SYMMETRY Example 12.10. Let us examine the orthogonal group on R2 a bit more closely. An element T ∈ O(2) is determined by its action on e1 = (1, 0)t and e2 = (0, 1)t . If T (e1 ) = (a, b)t , then a2 + b2 = 1 and T (e2 ) = (−b, a)t . Hence, T can be represented by ( ) ( ) a −b cos θ − sin θ A= = , b a sin θ cos θ where 0 ≤ θ < 2π. A matrix T in O(2) either reflects or rotates a vector in R2 (Figure 12.9). A reflection about the horizontal axis is given by the matrix ( ) 1 0 , 0 −1 whereas a rotation by an angle θ in a counterclockwise direction must come from a matrix of the form ( ) cos θ sin θ . sin θ − cos θ A reflection about a line ℓ is simply a reflection about the horizontal axis followed by a rotation. If det A = −1, then A gives a reflection. Two of the other matrix or matrix-related groups that we will consider are the special orthogonal group and the group of Euclidean motions. The special orthogonal group, SO(n), is just the intersection of O(n) and SLn (R); that is, those elements in O(n) with determinant one. The Euclidean group, E(n), can be written as ordered pairs (A, x), where A is in O(n) and x is in Rn . We define multiplication by (A, x)(B, y) = (AB, Ay + x). The identity of the group is (I, 0); the inverse of (A, x) is (A−1 , −A−1 x). In Exercise 12.3.6, you are asked to check that E(n) is indeed a group under this operation. y y x+y x x x Figure 12.11: Translations in R2 12.2 Symmetry An isometry or rigid motion in Rn is a distance-preserving function f from Rn to Rn . This means that f must satisfy ∥f (x) − f (y)∥ = ∥x − y∥ for all x, y ∈ Rn . It is not difficult to show that f must be a one-to-one map. By Theo- rem 12.8, any element in O(n) is an isometry on Rn ; however, O(n) does not include all 12.2. SYMMETRY 139 possible isometries on Rn . Translation by a vector x, Ty (x) = x + y is also an isometry (Figure 12.11); however, T cannot be in O(n) since it is not a linear map. We are mostly interested in isometries in R2 . In fact, the only isometries in R2 are rotations and reflections about the origin, translations, and combinations of the two. For example, a glide reflection is a translation followed by a reflection (Figure 12.12). In Rn all isometries are given in the same manner. The proof is very easy to generalize. y y x x x T (x) Figure 12.12: Glide reflections Lemma 12.13. An isometry f that fixes the origin in R2 is a linear transformation. In particular, f is given by an element in O(2). Proof. Let f be an isometry in R2 fixing the origin. We will first show that f preserves inner products. Since f (0) = 0, ∥f (x)∥ = ∥x∥; therefore, ∥x∥2 − 2⟨f (x), f (y)⟩ + ∥y∥2 = ∥f (x)∥2 − 2⟨f (x), f (y)⟩ + ∥f (y)∥2 = ⟨f (x) − f (y), f (x) − f (y)⟩ = ∥f (x) − f (y)∥2 = ∥x − y∥2 = ⟨x − y, x − y⟩ = ∥x∥2 − 2⟨x, y⟩ + ∥y∥2 . Consequently, ⟨f (x), f (y)⟩ = ⟨x, y⟩. Now let e1 and e2 be (1, 0)t and (0, 1)t , respectively. If x = (x1 , x2 ) = x1 e1 + x2 e2 , then f (x) = ⟨f (x), f (e1 )⟩f (e1 ) + ⟨f (x), f (e2 )⟩f (e2 ) = x1 f (e1 ) + x2 f (e2 ). The linearity of f easily follows. For any arbitrary isometry, f , Tx f will fix the origin for some vector x in R2 ; hence, Tx f (y) = Ay for some matrix A ∈ O(2). Consequently, f (y) = Ay+x. Given the isometries f (y) = Ay + x1 g(y) = By + x2 , 140 CHAPTER 12. MATRIX GROUPS AND SYMMETRY their composition is f (g(y)) = f (By + x2 ) = ABy + Ax2 + x1 . This last computation allows us to identify the group of isometries on R2 with E(2). Theorem 12.14. The group of isometries on R2 is the Euclidean group, E(2). A symmetry group in Rn is a subgroup of the group of isometries on Rn that fixes a set of points X ⊂ R2 . It is important to realize that the symmetry group of X depends both on Rn and on X. For example, the symmetry group of the origin in R1 is Z2 , but the symmetry group of the origin in R2 is O(2). Theorem 12.15. The only finite symmetry groups in R2 are Zn and Dn . Proof. Let G = {f1 , f2 , . . . , fn } be a finite symmetry group that fixes a set of points in X ⊂ R2 . Choose a point x ∈ X. This point may not be a fixed point—it could be moved by G to another point in X. Define a set S = {y1 , y2 , . . . yn }, where yi = fi (x). Now, let 1∑ n z= xi . n i=1 While the point z is not necessarily in the set X, it is fixed by every element in the symetry group. Without loss of generality, we may now assume that z is the origin. Any finite symmetry group G in R2 that fixes the origin must be a finite subgroup of O(2), since translations and glide reflections have infinite order. By Example 12.10, elements in O(2) are either rotations of the form ( ) cos θ − sin θ Rθ = sin θ cos θ or reflections of the form ( )( ) ( ) cos ϕ − sin ϕ 1 0 cos ϕ sin ϕ Tϕ = = . sin ϕ cos ϕ 0 −1 sin ϕ − cos ϕ Notice that det(Rθ ) = 1, det(Tϕ ) = −1, and Tϕ2 = I. We can divide the proof up into two cases. In the first case, all of the elements in G have determinant one. In the second case, there exists at least one element in G with determinant −1. Case 1. The determinant of every element in G is one. In this case every element in G must be a rotation. Since G is finite, there is a smallest angle, say θ0 , such that the corresponding element Rθ0 is the smallest rotation in the positive direction. We claim that Rθ0 generates G. If not, then for some positive integer n there is an angle θ1 between nθ0 and (n + 1)θ0 . If so, then (n + 1)θ0 − θ1 corresponds to a rotation smaller than θ0 , which contradicts the minimality of θ0 . Case 2. The group G contains a reflection T . The kernel of the homomorphism ϕ : G → {−1, 1} given by A 7→ det(A) consists of elements whose determinant is 1. Therefore, |G/ ker ϕ| = 2. We know that the kernel is cyclic by the first case and is a subgroup of G of, say, order n. Hence, |G| = 2n. The elements of G are Rθ , . . . , Rθn−1 , T Rθ , . . . , T Rθn−1 . These elements satisfy the relation T Rθ T = Rθ−1 . Consequently, G must be isomorphic to Dn in this case. 12.2. SYMMETRY 141 The Wallpaper Groups Suppose that we wish to study wallpaper patterns in the plane or crystals in three dimen- sions. Wallpaper patterns are simply repeating patterns in the plane (Figure 12.16). The analogs of wallpaper patterns in R3 are crystals, which we can think of as repeating pat- terns of molecules in three dimensions (Figure 12.17). The mathematical equivalent of a wallpaper or crystal pattern is called a lattice. Figure 12.16: A wallpaper pattern in R2 Figure 12.17: A crystal structure in R3 Let us examine wallpaper patterns in the plane a little more closely. Suppose that x and y are linearly independent vectors in R2 ; that is, one vector cannot be a scalar multiple of the other. A lattice of x and y is the set of all linear combinations mx + ny, where m and n are integers. The vectors x and y are said to be a basis for the lattice. Notice that a lattice can have several bases. For example, the vectors (1, 1)t and (2, 0)t have the same lattice as the vectors (−1, 1)t and (−1, −1)t (Figure 12.18). However, any lattice is completely determined by a basis. Given two bases for the same lattice, say {x1 , x2 } and {y1 , y2 }, we can write y1 = α1 x1 + α2 x2 y2 = β1 x1 + β2 x2 , where α1 , α2 , β1 , and β2 are integers. The matrix corresponding to this transformation is ( ) α1 α2 U= . β1 β2 If we wish to give x1 and x2 in terms of y1 and y2 , we need only calculate U −1 ; that is, ( ) ( ) y1 x1 U −1 = . y2 x2 142 CHAPTER 12. MATRIX GROUPS AND SYMMETRY Since U has integer entries, U −1 must also have integer entries; hence the determinants of both U and U −1 must be integers. Because U U −1 = I, det(U U −1 ) = det(U ) det(U −1 ) = 1; consequently, det(U ) = ±1. A matrix with determinant ±1 and integer entries is called unimodular. For example, the matrix ( ) 3 1 5 2 is unimodular. It should be clear that there is a minimum length for vectors in a lattice. (−1, 1) (1, 1) (2, 0) (−1, −1) Figure 12.18: A lattice in R2 We can classify lattices by studying their symmetry groups. The symmetry group of a lattice is the subgroup of E(2) that maps the lattice to itself. We consider two lattices in R2 to be equivalent if they have the same symmetry group. Similarly, classification of crystals in R3 is accomplished by associating a symmetry group, called a space group, with each type of crystal. Two lattices are considered different if their space groups are not the same. The natural question that now arises is how many space groups exist. A space group is composed of two parts: a translation subgroup and a point. The translation subgroup is an infinite abelian subgroup of the space group made up of the translational symmetries of the crystal; the point group is a finite group consisting of ro- tations and reflections of the crystal about a point. More specifically, a space group is a subgroup of G ⊂ E(2) whose translations are a set of the form {(I, t) : t ∈ L}, where L is a lattice. Space groups are, of course, infinite. Using geometric arguments, we can prove the following theorem (see [5] or [6]). Theorem 12.19. Every translation group in R2 is isomorphic to Z × Z. The point group of G is G0 = {A : (A, b) ∈ G for some b}. In particular, G0 must be a subgroup of O(2). Suppose that x is a vector in a lattice L with space group G, translation group H, and point group G0 . For any element (A, y) in G, (A, y)(I, x)(A, y)−1 = (A, Ax + y)(A−1 , −A−1 y) = (AA−1 , −AA−1 y + Ax + y) = (I, Ax); hence, (I, Ax) is in the translation group of G. More specifically, Ax must be in the lattice L. It is important to note that G0 is not usually a subgroup of the space group G; however, if T is the translation subgroup of G, then G/T ∼ = G0 . The proof of the following theorem can be found in [2], [5], or [6]. 12.2. SYMMETRY 143 Theorem 12.20. The point group in the wallpaper groups is isomorphic to Zn or Dn , where n = 1, 2, 3, 4, 6. To answer the question of how the point groups and the translation groups can be combined, we must look at the different types of lattices. Lattices can be classified by the structure of a single lattice cell. The possible cell shapes are parallelogram, rectangular, square, rhombic, and hexagonal (Figure 12.21). The wallpaper groups can now be classified according to the types of reflections that occur in each group: these are ordinarily reflections, glide reflections, both, or none. Rectangular Square Rhombic Parallelogram Hexagonal Figure 12.21: Types of lattices in R2 Notation and Reflections or Space Groups Point Group Lattice Type Glide Reflections? p1 Z1 parallelogram none p2 Z2 parallelogram none p3 Z3 hexagonal none p4 Z4 square none p6 Z6 hexagonal none pm D1 rectangular reflections pg D1 rectangular glide reflections cm D1 rhombic both pmm D2 rectangular reflections pmg D2 rectangular glide reflections pgg D2 rectangular both c2mm D2 rhombic both p3m1, p31m D3 hexagonal both p4m, p4g D4 square both p6m D6 hexagonal both Table 12.22: The 17 wallpaper groups Theorem 12.23. There are exactly 17 wallpaper groups. 144 CHAPTER 12. MATRIX GROUPS AND SYMMETRY p4m p4g Figure 12.24: The wallpaper groups p4m and p4g The 17 wallpaper groups are listed in Table 12.22. The groups p3m1 and p31m can be distinguished by whether or not all of their threefold centers lie on the reflection axes: those of p3m1 must, whereas those of p31m may not. Similarly, the fourfold centers of p4m must lie on the reflection axes whereas those of p4g need not (Figure 12.24). The complete proof of this theorem can be found in several of the references at the end of this chapter, including [5], [6], [10], and [11]. Sage We have not yet included any Sage material related to this chapter. Historical Note Symmetry groups have intrigued mathematicians for a long time. Leonardo da Vinci was probably the first person to know all of the point groups. At the International Congress of Mathematicians in 1900, David Hilbert gave a now-famous address outlining 23 problems to guide mathematics in the twentieth century. Hilbert’s eighteenth problem asked whether or not crystallographic groups in n dimensions were always finite. In 1910, L. Bieberbach proved that crystallographic groups are finite in every dimension. Finding out how many of these groups there are in each dimension is another matter. In R3 there are 230 different space groups; in R4 there are 4783. No one has been able to compute the number of space groups for R5 and beyond. It is interesting to note that the crystallographic groups were found mathematically for R3 before the 230 different types of crystals were actually discovered in nature. 12.3 Exercises 1. Prove the identity 1[ ] ⟨x, y⟩ = ∥x + y∥2 − ∥x∥2 − ∥y∥2 . 2 2. Show that O(n) is a group. 3. Prove that the following matrices are orthogonal. Are any of these matrices in SO(n)? (a) (b) ( √ √ ) ( √ √ ) 1/ 2 −1/ 2 1/ 5 2/ 5 √ √ √ √ 1/ 2 1/ 2 −2/ 5 1/ 5 12.3. EXERCISES 145 (c) √ √ (d) 4/ 5 0 3/ 5 1/3 2/3 −2/3 √ √ −3/ 5 0 4/ 5 −2/3 2/3 1/3 0 −1 0 −2/3 1/3 2/3 4. Determine the symmetry group of each of the figures in Figure 12.25. (a) (c) (b) Figure 12.25 5. Let x, y, and w be vectors in Rn and α ∈ R. Prove each of the following properties of inner products. (a) ⟨x, y⟩ = ⟨y, x⟩. (b) ⟨x, y + w⟩ = ⟨x, y⟩ + ⟨x, w⟩. (c) ⟨αx, y⟩ = ⟨x, αy⟩ = α⟨x, y⟩. (d) ⟨x, x⟩ ≥ 0 with equality exactly when x = 0. (e) If ⟨x, y⟩ = 0 for all x in Rn , then y = 0. 6. Verify that E(n) = {(A, x) : A ∈ O(n) and x ∈ Rn } is a group. 7. Prove that {(2, 1), (1, 1)} and {(12, 5), (7, 3)} are bases for the same lattice. 8. Let G be a subgroup of E(2) and suppose that T is the translation subgroup of G. Prove that the point group of G is isomorphic to G/T . 9. Let A ∈ SL2 (R) and suppose that the vectors x and y form two sides of a parallelogram in R2 . Prove that the area of this parallelogram is the same as the area of the parallelogram with sides Ax and Ay. 10. Prove that SO(n) is a normal subgroup of O(n). 11. Show that any isometry f in Rn is a one-to-one map. 12. Prove or disprove: an element in E(2) of the form (A, x), where x ̸= 0, has infinite order. 13. Prove or disprove: There exists an infinite abelian subgroup of O(n). 14. Let x = (x1 , x2 ) be a point on the unit circle in R2 ; that is, x21 + x22 = 1. If A ∈ O(2), show that Ax is also a point on the unit circle. 15. Let G be a group with a subgroup H (not necessarily normal) and a normal subgroup N . Then G is a semidirect product of N by H if 146 CHAPTER 12. MATRIX GROUPS AND SYMMETRY • H ∩ N = {id}; • HN = G. Show that each of the following is true. (a) S3 is the semidirect product of A3 by H = {(1), (12)}. (b) The quaternion group, Q8 , cannot be written as a semidirect product. (c) E(2) is the semidirect product of O(2) by H, where H consists of all translations in R2 . 16. Determine which of the 17 wallpaper groups preserves the symmetry of the pattern in Figure 12.16. 17. Determine which of the 17 wallpaper groups preserves the symmetry of the pattern in Figure 12.26. Figure 12.26 18. Find the rotation group of a dodecahedron. 19. For each of the 17 wallpaper groups, draw a wallpaper pattern having that group as a symmetry group. References and Suggested Readings [1] Coxeter, H. M. and Moser, W. O. J. Generators and Relations for Discrete Groups, 3rd ed. Springer-Verlag, New York, 1972. [2] Grove, L. C. and Benson, C. T. Finite Reflection Groups. 2nd ed. Springer-Verlag, New York, 1985. [3] Hiller, H. “Crystallography and Cohomology of Groups,” American Mathematical Monthly 93 (1986), 765–79. [4] Lockwood, E. H. and Macmillan, R. H. Geometric Symmetry. Cambridge University Press, Cambridge, 1978. [5] Mackiw, G. Applications of Abstract Algebra. Wiley, New York, 1985. [6] Martin, G. Transformation Groups: An Introduction to Symmetry. Springer-Verlag, New York, 1982. [7] Milnor, J. “Hilbert’s Problem 18: On Crystallographic Groups, Fundamental Do- mains, and Sphere Packing,” t Proceedings of Symposia in Pure Mathematics 18, American Mathematical Society, 1976. 12.3. EXERCISES 147 [8] Phillips, F. C. An Introduction to Crystallography. 4th ed. Wiley, New York, 1971. [9] Rose, B. I. and Stafford, R. D. “An Elementary Course in Mathematical Symmetry,” American Mathematical Monthly 88 (1980), 54–64. [10] Schattschneider, D. “The Plane Symmetry Groups: Their Recognition and Their Notation,” American Mathematical Monthly 85(1978), 439–50. [11] Schwarzenberger, R. L. “The 17 Plane Symmetry Groups,” Mathematical Gazette 58(1974), 123–31. [12] Weyl, H. Symmetry. Princeton University Press, Princeton, NJ, 1952. 13 The Structure of Groups The ultimate goal of group theory is to classify all groups up to isomorphism; that is, given a particular group, we should be able to match it up with a known group via an isomorphism. For example, we have already proved that any finite cyclic group of order n is isomorphic to Zn ; hence, we “know” all finite cyclic groups. It is probably not reasonable to expect that we will ever know all groups; however, we can often classify certain types of groups or distinguish between groups in special cases. In this chapter we will characterize all finite abelian groups. We shall also investigate groups with sequences of subgroups. If a group has a sequence of subgroups, say G = Hn ⊃ Hn−1 ⊃ · · · ⊃ H1 ⊃ H0 = {e}, where each subgroup Hi is normal in Hi+1 and each of the factor groups Hi+1 /Hi is abelian, then G is a solvable group. In addition to allowing us to distinguish between certain classes of groups, solvable groups turn out to be central to the study of solutions to polynomial equations. 13.1 Finite Abelian Groups In our investigation of cyclic groups we found that every group of prime order was isomorphic to Zp , where p was a prime number. We also determined that Zmn ∼ = Zm × Zn when gcd(m, n) = 1. In fact, much more is true. Every finite abelian group is isomorphic to a direct product of cyclic groups of prime power order; that is, every finite abelian group is isomorphic to a group of the type Zpα1 × · · · × Zpαnn , 1 where each pk is prime (not necessarily distinct). First, let us examine a slight generalization of finite abelian groups. Suppose that G is a group and let {gi } be a set of elements in G, where i is in some index set I (not necessarily finite). The smallest subgroup of G containing all of the gi ’s is the subgroup of G generated by the gi ’s. If this subgroup of G is in fact all of G, then G is generated by the set {gi : i ∈ I}. In this case the gi ’s are said to be the generators of G. If there is a finite set {gi : i ∈ I} that generates G, then G is finitely generated. Example 13.1. Obviously, all finite groups are finitely generated. For example, the group S3 is generated by the permutations (12) and (123). The group Z × Zn is an infinite group but is finitely generated by {(1, 0), (0, 1)}. Example 13.2. Not all groups are finitely generated. Consider the rational numbers Q under the operation of addition. Suppose that Q is finitely generated with generators 148 13.1. FINITE ABELIAN GROUPS 149 p1 /q1 , . . . , pn /qn , where each pi /qi is a fraction expressed in its lowest terms. Let p be some prime that does not divide any of the denominators q1 , . . . , qn . We claim that 1/p cannot be in the subgroup of Q that is generated by p1 /q1 , . . . , pn /qn , since p does not divide the denominator of any element in this subgroup. This fact is easy to see since the sum of any two generators is pi /qi + pj /qj = (pi qj + pj qi )/(qi qj ). Proposition 13.3. Let H be the subgroup of a group G that is generated by {gi ∈ G : i ∈ I}. Then h ∈ H exactly when it is a product of the form h = giα11 · · · giαnn , where the gik s are not necessarily distinct. Proof. Let K be the set of all products of the form giα11 · · · giαnn , where the gik s are not necessarily distinct. Certainly K is a subset of H. We need only show that K is a subgroup of G. If this is the case, then K = H, since H is the smallest subgroup containing all the gi s. Clearly, the set K is closed under the group operation. Since gi0 = 1, the identity is in K. It remains to show that the inverse of an element g = gik11 · · · giknn in K must also be in K. However, g −1 = (gik11 · · · giknn )−1 = (gi−k n n · · · gi−k 1 1 ). The reason that powers of a fixed gi may occur several times in the product is that we may have a nonabelian group. However, if the group is abelian, then the gi s need occur only once. For example, a product such as a−3 b5 a7 in an abelian group could always be simplified (in this case, to a4 b5 ). Now let us restrict our attention to finite abelian groups. We can express any finite abelian group as a finite direct product of cyclic groups. More specifically, letting p be prime, we define a group G to be a p-group if every element in G has as its order a power of p. For example, both Z2 × Z2 and Z4 are 2-groups, whereas Z27 is a 3-group. We shall prove the Fundamental Theorem of Finite Abelian Groups which tells us that every finite abelian group is isomorphic to a direct product of cyclic p-groups. Theorem 13.4 Fundamental Theorem of Finite Abelian Groups. Every finite abelian group G is isomorphic to a direct product of cyclic groups of the form Zpα1 × Zpα2 × · · · × Zpαnn 1 2 here the pi ’s are primes (not necessarily distinct). Example 13.5. Suppose that we wish to classify all abelian groups of order 540 = 22 ·33 ·5. The Fundamental Theorem of Finite Abelian Groups tells us that we have the following six possibilities. • Z2 × Z2 × Z3 × Z3 × Z3 × Z5 ; • Z2 × Z2 × Z3 × Z9 × Z5 ; • Z2 × Z2 × Z27 × Z5 ; • Z4 × Z3 × Z3 × Z3 × Z5 ; • Z4 × Z3 × Z9 × Z5 ; 150 CHAPTER 13. THE STRUCTURE OF GROUPS • Z4 × Z27 × Z5 . The proof of the Fundamental Theorem of Finite Abelian Groups depends on several lemmas. Lemma 13.6. Let G be a finite abelian group of order n. If p is a prime that divides n, then G contains an element of order p. Proof. We will prove this lemma by induction. If n = 1, then there is nothing to show. Now suppose that the order of G is n the lemma is true for all groups of order k, where k < n. Furthermore, let p be a prime that divides n. If G has no proper nontrivial subgroups, then G = ⟨a⟩, where a is any element other than the identity. By Exercise 4.4.39, the order of G must be prime. Since p divides n, we know that p = n, and G contains p − 1 elements of order p. Now suppose that G contains a nontrivial proper subgroup H. Then 1 < |H| < n. If p | |H|, then H contains an element of order p by induction and the lemma is true. Suppose that p does not divide the order of H. Since G is abelian, it must be the case that H is a normal subgroup of G, and |G| = |H| · |G/H|. Consequently, p must divide |G/H|. Since |G/H| < |G| = n, we know that G/H contains an element aH of order p by the induction hypothesis. Thus, H = (aH)p = ap H, and ap ∈ H but a ∈ / H. If |H| = r, then p and r are relatively prime, and there exist integers s and t such that sp + tr = 1. Furthermore, the order of ap must divide r, and (ap )r = (ar )p = 1. We claim that ar has order p. We must show that ar ̸= 1. Suppose ar = 1. Then a = asp+tr = asp atr = (ap )s (ar )t = (ap )s 1 = (ap )s . Since ap ∈ H, it must be the case that a = (ap )s ∈ H, which is a contradiction. Therefore, ar ̸= 1 is an element of order p in G. Lemma 13.6 is a special case of Cauchy’s Theorem (Theorem 15.1), which states that if G be a finite group and p a prime such that p divides the order of G, then G contains a subgroup of order p. We will prove Cauchy’s Theorem in Chapter 15. Lemma 13.7. A finite abelian group is a p-group if and only if its order is a power of p. Proof. If |G| = pn then by Lagrange’s theorem, then the order of any g ∈ G must divide pn , and therefore must be a power of p. Conversely, if |G| is not a power of p, then it has some other prime divisor q, so by Lemma 13.6, G has an element of order q and thus is not a p-group. Lemma 13.8. Let G be a finite abelian group of order n = pα1 1 · · · pαk k , where where p1 , . . . , pk are distinct primes and α1 , α2 , . . . , αk are positive integers. Then G is the internal direct product of subgroups G1 , G2 , . . . , Gk , where Gi is the subgroup of G consisting of all elements of order pki for some integer k. 13.1. FINITE ABELIAN GROUPS 151 Proof. Since G is an abelian group, we are guaranteed that Gi is a subgroup of G for i = 1, . . . , n. Since the identity has order p0i = 1, we know that 1 ∈ Gi . If g ∈ Gi has order pri , then g −1 must also have order pri . Finally, if h ∈ Gi has order psi , then t t t (gh)pi = g pi hpi = 1 · 1 = 1, where t is the maximum of r and s. We must show that G = G 1 G2 · · · Gk and Gi ∩ Gj = {1} for i ̸= j. Suppose that g1 ∈ G1 is in the subgroup generated by G2 , G3 , . . . , Gk . Then g1 = g2 g3 · · · gk for gi ∈ Gi . Since gi has order pαi , we know that α2 αk αi p ···p gip = 1 for i = 2, 3, . . . , k, and g1 2 k = 1. Since the order of g1 is a power of p1 α2 αk and gcd(p1 , p2 · · · pk ) = 1, it must be the case that g1 = 1 and the intersection of G1 with any of the subgroups G2 , G3 , . . . , Gk is the identity. A similar argument shows that Gi ∩ Gj = {1} for i ̸= j. Next, we must show that it possible to write every g ∈ G as a product g1 · · · gk , where gi ∈ Gi . Since the order of g divides the order of G, we know that |g| = pβ1 1 pβ2 2 · · · pβk k for some integers β1 , . . . , βk . Letting ai = |g|/pβi i , the ai ’s are relatively prime; hence, there exist integers b1 , . . . , bk such that a1 b1 + · · · + ak bk = 1. Consequently, g = g a1 b1 +···+ak bk = g a1 b1 · · · g ak bk . Since βi g (ai bi )pi = g bi |g| = e, it follows that g ai bi must be in Gi . Let gi = g ai bi . Then g = g1 · · · gk ∈ G1 G2 · · · Gk . Therefore, G = G1 G2 · · · Gk is an internal direct product of subgroups. If remains for us to determine the possible structure of each pi -group Gi in Lemma 13.8. Lemma 13.9. Let G be a finite abelian p-group and suppose that g ∈ G has maximal order. Then G is isomorphic to ⟨g⟩ × H for some subgroup H of G. Proof. By Lemma 13.7, we may assume that the order of G is pn . We shall induct on n. If n = 1, then G is cyclic of order p and must be generated by g. Suppose now that the statement of the lemma holds for all integers k with 1 ≤ k < n and let g be of maximal m order in G, say |g| = pm . Then ap = e for all a ∈ G. Now choose h in G such that h ∈ / ⟨g⟩, where h has the smallest possible order. Certainly such an h exists; otherwise, G = ⟨g⟩ and we are done. Let H = ⟨h⟩. We claim that ⟨g⟩ ∩ H = {e}. It suffices to show that |H| = p. Since |hp | = |h|/p, the order of hp is smaller than the order of h and must be in ⟨g⟩ by the minimality of h; that is, hp = g r for some number r. Hence, m−1 m−1 m (g r )p = (hp )p = hp = e, and the order of g r must be less than or equal to pm−1 . Therefore, g r cannot generate ⟨g⟩. Notice that p must occur as a factor of r, say r = ps, and hp = g r = g ps . Define a to be g −s h. Then a cannot be in ⟨g⟩; otherwise, h would also have to be in ⟨g⟩. Also, ap = g −sp hp = g −r hp = h−p hp = e. 152 CHAPTER 13. THE STRUCTURE OF GROUPS We have now formed an element a with order p such that a ∈ / ⟨g⟩. Since h was chosen to have the smallest order of all of the elements that are not in ⟨g⟩, |H| = p. Now we will show that the order of gH in the factor group G/H must be the same as the order of g in G. If |gH| < |g| = pm , then m−1 m−1 H = (gH)p = gp H; m−1 hence, g p must be in ⟨g⟩ ∩ H = {e}, which contradicts the fact that the order of g is m p . Therefore, gH must have maximal order in G/H. By the Correspondence Theorem and our induction hypothesis, G/H ∼= ⟨gH⟩ × K/H for some subgroup K of G containing H. We claim that ⟨g⟩ ∩ K = {e}. If b ∈ ⟨g⟩ ∩ K, then bH ∈ ⟨gH⟩ ∩ K/H = {H} and b ∈ ⟨g⟩ ∩ H = {e}. It follows that G = ⟨g⟩K implies that G∼ = ⟨g⟩ × K. The proof of the Fundamental Theorem of Finite Abelian Groups follows very quickly from Lemma 13.9. Suppose that G is a finite abelian group and let g be an element of maximal order in G. If ⟨g⟩ = G, then we are done; otherwise, G ∼ = Z|g| × H for some subgroup H contained in G by the lemma. Since |H| < |G|, we can apply mathematical induction. We now state the more general theorem for all finitely generated abelian groups. The proof of this theorem can be found in any of the references at the end of this chapter. Theorem 13.10 The Fundamental Theorem of Finitely Generated Abelian Groups. Every finitely generated abelian group G is isomorphic to a direct product of cyclic groups of the form Zpα1 × Zpα2 × · · · × Zpαnn × Z × · · · × Z, 1 2 where the pi ’s are primes (not necessarily distinct). 13.2 Solvable Groups A subnormal series of a group G is a finite sequence of subgroups G = Hn ⊃ Hn−1 ⊃ · · · ⊃ H1 ⊃ H0 = {e}, where Hi is a normal subgroup of Hi+1 . If each subgroup Hi is normal in G, then the series is called a normal series. The length of a subnormal or normal series is the number of proper inclusions. Example 13.11. Any series of subgroups of an abelian group is a normal series. Consider the following series of groups: Z ⊃ 9Z ⊃ 45Z ⊃ 180Z ⊃ {0}, Z24 ⊃ ⟨2⟩ ⊃ ⟨6⟩ ⊃ ⟨12⟩ ⊃ {0}. Example 13.12. A subnormal series need not be a normal series. Consider the following subnormal series of the group D4 : D4 ⊃ {(1), (12)(34), (13)(24), (14)(23)} ⊃ {(1), (12)(34)} ⊃ {(1)}. The subgroup {(1), (12)(34)} is not normal in D4 ; consequently, this series is not a normal series. 13.2. SOLVABLE GROUPS 153 A subnormal (normal) series {Kj } is a refinement of a subnormal (normal) series {Hi } if {Hi } ⊂ {Kj }. That is, each Hi is one of the Kj . Example 13.13. The series Z ⊃ 3Z ⊃ 9Z ⊃ 45Z ⊃ 90Z ⊃ 180Z ⊃ {0} is a refinement of the series Z ⊃ 9Z ⊃ 45Z ⊃ 180Z ⊃ {0}. The best way to study a subnormal or normal series of subgroups, {Hi } of G, is actually to study the factor groups Hi+1 /Hi . We say that two subnormal (normal) series {Hi } and {Kj } of a group G are isomorphic if there is a one-to-one correspondence between the collections of factor groups {Hi+1 /Hi } and {Kj+1 /Kj }. Example 13.14. The two normal series Z60 ⊃ ⟨3⟩ ⊃ ⟨15⟩ ⊃ {0} Z60 ⊃ ⟨4⟩ ⊃ ⟨20⟩ ⊃ {0} of the group Z60 are isomorphic since Z60 /⟨3⟩ ∼ = ⟨20⟩/{0} ∼ = Z3 ∼ ⟨4⟩/⟨20⟩ = ⟨3⟩/⟨15⟩ = ∼ Z5 ⟨15⟩/{0} ∼ = Z60 /⟨4⟩ ∼ = Z4 . A subnormal series {Hi } of a group G is a composition series if all the factor groups are simple; that is, if none of the factor groups of the series contains a normal subgroup. A normal series {Hi } of G is a principal series if all the factor groups are simple. Example 13.15. The group Z60 has a composition series Z60 ⊃ ⟨3⟩ ⊃ ⟨15⟩ ⊃ ⟨30⟩ ⊃ {0} with factor groups Z60 /⟨3⟩ ∼ = Z3 ⟨3⟩/⟨15⟩ =∼ Z5 ⟨15⟩/⟨30⟩ ∼ = Z2 ⟨30⟩/{0} ∼ = Z2 . Since Z60 is an abelian group, this series is automatically a principal series. Notice that a composition series need not be unique. The series Z60 ⊃ ⟨2⟩ ⊃ ⟨4⟩ ⊃ ⟨20⟩ ⊃ {0} is also a composition series. Example 13.16. For n ≥ 5, the series Sn ⊃ An ⊃ {(1)} is a composition series for Sn since Sn /An ∼ = Z2 and An is simple. 154 CHAPTER 13. THE STRUCTURE OF GROUPS Example 13.17. Not every group has a composition series or a principal series. Suppose that {0} = H0 ⊂ H1 ⊂ · · · ⊂ Hn−1 ⊂ Hn = Z is a subnormal series for the integers under addition. Then H1 must be of the form kZ for some k ∈ N. In this case H1 /H0 ∼= kZ is an infinite cyclic group with many nontrivial proper normal subgroups. Although composition series need not be unique as in the case of Z60 , it turns out that any two composition series are related. The factor groups of the two composition series for Z60 are Z2 , Z2 , Z3 , and Z5 ; that is, the two composition series are isomorphic. The Jordan-Hölder Theorem says that this is always the case. Theorem 13.18 Jordan-Hölder. Any two composition series of G are isomorphic. Proof. We shall employ mathematical induction on the length of the composition series. If the length of a composition series is 1, then G must be a simple group. In this case any two composition series are isomorphic. Suppose now that the theorem is true for all groups having a composition series of length k, where 1 ≤ k < n. Let G = Hn ⊃ Hn−1 ⊃ · · · ⊃ H1 ⊃ H0 = {e} G = Km ⊃ Km−1 ⊃ · · · ⊃ K1 ⊃ K0 = {e} be two composition series for G. We can form two new subnormal series for G since Hi ∩ Km−1 is normal in Hi+1 ∩ Km−1 and Kj ∩ Hn−1 is normal in Kj+1 ∩ Hn−1 : G = Hn ⊃ Hn−1 ⊃ Hn−1 ∩ Km−1 ⊃ · · · ⊃ H0 ∩ Km−1 = {e} G = Km ⊃ Km−1 ⊃ Km−1 ∩ Hn−1 ⊃ · · · ⊃ K0 ∩ Hn−1 = {e}. Since Hi ∩ Km−1 is normal in Hi+1 ∩ Km−1 , the Second Isomorphism Theorem (Theo- rem 11.12) implies that (Hi+1 ∩ Km−1 )/(Hi ∩ Km−1 ) = (Hi+1 ∩ Km−1 )/(Hi ∩ (Hi+1 ∩ Km−1 )) ∼ Hi (Hi+1 ∩ Km−1 )/Hi , = where Hi is normal in Hi (Hi+1 ∩ Km−1 ). Since {Hi } is a composition series, Hi+1 /Hi must be simple; consequently, Hi (Hi+1 ∩ Km−1 )/Hi is either Hi+1 /Hi or Hi /Hi . That is, Hi (Hi+1 ∩ Km−1 ) must be either Hi or Hi+1 . Removing any nonproper inclusions from the series Hn−1 ⊃ Hn−1 ∩ Km−1 ⊃ · · · ⊃ H0 ∩ Km−1 = {e}, we have a composition series for Hn−1 . Our induction hypothesis says that this series must be equivalent to the composition series Hn−1 ⊃ · · · ⊃ H1 ⊃ H0 = {e}. Hence, the composition series G = Hn ⊃ Hn−1 ⊃ · · · ⊃ H1 ⊃ H0 = {e} and G = Hn ⊃ Hn−1 ⊃ Hn−1 ∩ Km−1 ⊃ · · · ⊃ H0 ∩ Km−1 = {e} are equivalent. If Hn−1 = Km−1 , then the composition series {Hi } and {Kj } are equivalent and we are done; otherwise, Hn−1 Km−1 is a normal subgroup of G properly containing 13.3. EXERCISES 155 Hn−1 . In this case Hn−1 Km−1 = G and we can apply the Second Isomorphism Theorem once again; that is, Km−1 /(Km−1 ∩ Hn−1 ) ∼ = (Hn−1 Km−1 )/Hn−1 = G/Hn−1 . Therefore, G = Hn ⊃ Hn−1 ⊃ Hn−1 ∩ Km−1 ⊃ · · · ⊃ H0 ∩ Km−1 = {e} and G = Km ⊃ Km−1 ⊃ Km−1 ∩ Hn−1 ⊃ · · · ⊃ K0 ∩ Hn−1 = {e} are equivalent and the proof of the theorem is complete. A group G is solvable if it has a subnormal series {Hi } such that all of the factor groups Hi+1 /Hi are abelian. Solvable groups will play a fundamental role when we study Galois theory and the solution of polynomial equations. Example 13.19. The group S4 is solvable since S4 ⊃ A4 ⊃ {(1), (12)(34), (13)(24), (14)(23)} ⊃ {(1)} has abelian factor groups; however, for n ≥ 5 the series Sn ⊃ An ⊃ {(1)} is a composition series for Sn with a nonabelian factor group. Therefore, Sn is not a solvable group for n ≥ 5. Sage Sage is able to create direct products of cyclic groups, though they are realized as permutation groups. This is a situation that should improve. However, with a classification of finite abelian groups, we can describe how to construct in Sage every group of order less than 16. 13.3 Exercises 1. Find all of the abelian groups of order less than or equal to 40 up to isomorphism. 2. Find all of the abelian groups of order 200 up to isomorphism. 3. Find all of the abelian groups of order 720 up to isomorphism. 4. Find all of the composition series for each of the following groups. (a) Z12 (e) S3 × Z4 (b) Z48 (f) S4 (c) The quaternions, Q8 (g) Sn , n ≥ 5 (d) D4 (h) Q 5. Show that the infinite direct product G = Z2 × Z2 × · · · is not finitely generated. 6. Let G be an abelian group of order m. If n divides m, prove that G has a subgroup of order n. 7. A group G is a torsion group if every element of G has finite order. Prove that a finitely generated abelian torsion group must be finite. 156 CHAPTER 13. THE STRUCTURE OF GROUPS 8. Let G, H, and K be finitely generated abelian groups. Show that if G × H ∼ = G × K, then H ∼ = K. Give a counterexample to show that this cannot be true in general. 9. Let G and H be solvable groups. Show that G × H is also solvable. 10. If G has a composition (principal) series and if N is a proper normal subgroup of G, show there exists a composition (principal) series containing N . 11. Prove or disprove: Let N be a normal subgroup of G. If N and G/N have composition series, then G must also have a composition series. 12. Let N be a normal subgroup of G. If N and G/N are solvable groups, show that G is also a solvable group. 13. Prove that G is a solvable group if and only if G has a series of subgroups G = Pn ⊃ Pn−1 ⊃ · · · ⊃ P1 ⊃ P0 = {e} where Pi is normal in Pi+1 and the order of Pi+1 /Pi is prime. 14. Let G be a solvable group. Prove that any subgroup of G is also solvable. 15. Let G be a solvable group and N a normal subgroup of G. Prove that G/N is solvable. 16. Prove that Dn is solvable for all integers n. 17. Suppose that G has a composition series. If N is a normal subgroup of G, show that N and G/N also have composition series. 18. Let G be a cyclic p-group with subgroups H and K. Prove that either H is contained in K or K is contained in H. 19. Suppose that G is a solvable group with order n ≥ 2. Show that G contains a normal nontrivial abelian subgroup. 20. Recall that the commutator subgroup G′ of a group G is defined as the subgroup of G generated by elements of the form a−1 b−1 ab for a, b ∈ G. We can define a series of subgroups of G by G(0) = G, G(1) = G′ , and G(i+1) = (G(i) )′ . (a) Prove that G(i+1) is normal in (G(i) )′ . The series of subgroups G(0) = G ⊃ G(1) ⊃ G(2) ⊃ · · · is called the derived series of G. (b) Show that G is solvable if and only if G(n) = {e} for some integer n. 21. Suppose that G is a solvable group with order n ≥ 2. Show that G contains a normal nontrivial abelian factor group. 22. Zassenhaus Lemma. Let H and K be subgroups of a group G. Suppose also that H ∗ and K ∗ are normal subgroups of H and K respectively. Then (a) H ∗ (H ∩ K ∗ ) is a normal subgroup of H ∗ (H ∩ K). (b) K ∗ (H ∗ ∩ K) is a normal subgroup of K ∗ (H ∩ K). (c) H ∗ (H ∩ K)/H ∗ (H ∩ K ∗ ) ∼ = K ∗ (H ∩ K)/K ∗ (H ∗ ∩ K) ∼ = (H ∩ K)/(H ∗ ∩ K)(H ∩ K ∗ ). 23. Schreier’s Theorem. Use the Zassenhaus Lemma to prove that two subnormal (normal) series of a group G have isomorphic refinements. 24. Use Schreier’s Theorem to prove the Jordan-Hölder Theorem. 13.4. PROGRAMMING EXERCISES 157 13.4 Programming Exercises 1. Write a program that will compute all possible abelian groups of order n. What is the largest n for which your program will work? References and Suggested Readings [1] Hungerford, T. W. Algebra. Springer, New York, 1974. [2] Lang, S. Algebra. 3rd ed. Springer, New York, 2002. [3] Rotman, J. J. An Introduction to the Theory of Groups. 4th ed. Springer, New York, 1995. 14 Group Actions Group actions generalize group multiplication. If G is a group and X is an arbitrary set, a group action of an element g ∈ G and x ∈ X is a product, gx, living in X. Many problems in algebra are best be attacked via group actions. For example, the proofs of the Sylow theorems and of Burnside’s Counting Theorem are most easily understood when they are formulated in terms of group actions. 14.1 Groups Acting on Sets Let X be a set and G be a group. A (left) action of G on X is a map G × X → X given by (g, x) 7→ gx, where 1. ex = x for all x ∈ X; 2. (g1 g2 )x = g1 (g2 x) for all x ∈ X and all g1 , g2 ∈ G. Under these considerations X is called a G-set. Notice that we are not requiring X to be related to G in any way. It is true that every group G acts on every set X by the trivial action (g, x) 7→ x; however, group actions are more interesting if the set X is somehow related to the group G. Example 14.1. Let G = GL2 (R) and X = R2 . Then G acts on X by left multiplication. If v ∈ R2 and I is the identity matrix, then Iv = v. If A and B are 2 × 2 invertible matrices, then (AB)v = A(Bv) since matrix multiplication is associative. Example 14.2. Let G = D4 be the symmetry group of a square. If X = {1, 2, 3, 4} is the set of vertices of the square, then we can consider D4 to consist of the following permutations: {(1), (13), (24), (1432), (1234), (12)(34), (14)(23), (13)(24)}. The elements of D4 act on X as functions. The permutation (13)(24) acts on vertex 1 by sending it to vertex 3, on vertex 2 by sending it to vertex 4, and so on. It is easy to see that the axioms of a group action are satisfied. In general, if X is any set and G is a subgroup of SX , the group of all permutations acting on X, then X is a G-set under the group action (σ, x) 7→ σ(x) for σ ∈ G and x ∈ X. 158 14.1. GROUPS ACTING ON SETS 159 Example 14.3. If we let X = G, then every group G acts on itself by the left regular representation; that is, (g, x) 7→ λg (x) = gx, where λg is left multiplication: e · x = λe x = ex = x (gh) · x = λgh x = λg λh x = λg (hx) = g · (h · x). If H is a subgroup of G, then G is an H-set under left multiplication by elements of H. Example 14.4. Let G be a group and suppose that X = G. If H is a subgroup of G, then G is an H-set under conjugation; that is, we can define an action of H on G, H × G → G, via (h, g) 7→ hgh−1 for h ∈ H and g ∈ G. Clearly, the first axiom for a group action holds. Observing that (h1 h2 , g) = h1 h2 g(h1 h2 )−1 = h1 (h2 gh−1 −1 2 )h1 = (h1 , (h2 , g)), we see that the second condition is also satisfied. Example 14.5. Let H be a subgroup of G and LH the set of left cosets of H. The set LH is a G-set under the action (g, xH) 7→ gxH. Again, it is easy to see that the first axiom is true. Since (gg ′ )xH = g(g ′ xH), the second axiom is also true. If G acts on a set X and x, y ∈ X, then x is said to be G-equivalent to y if there exists a g ∈ G such that gx = y. We write x ∼G y or x ∼ y if two elements are G-equivalent. Proposition 14.6. Let X be a G-set. Then G-equivalence is an equivalence relation on X. Proof. The relation ∼ is reflexive since ex = x. Suppose that x ∼ y for x, y ∈ X. Then there exists a g such that gx = y. In this case g −1 y = x; hence, y ∼ x. To show that the relation is transitive, suppose that x ∼ y and y ∼ z. Then there must exist group elements g and h such that gx = y and hy = z. So z = hy = (hg)x, and x is equivalent to z. If X is a G-set, then each partition of X associated with G-equivalence is called an orbit of X under G. We will denote the orbit that contains an element x of X by Ox . Example 14.7. Let G be the permutation group defined by G = {(1), (123), (132), (45), (123)(45), (132)(45)} and X = {1, 2, 3, 4, 5}. Then X is a G-set. The orbits are O1 = O2 = O3 = {1, 2, 3} and O4 = O5 = {4, 5}. Now suppose that G is a group acting on a set X and let g be an element of G. The fixed point set of g in X, denoted by Xg , is the set of all x ∈ X such that gx = x. We can also study the group elements g that fix a given x ∈ X. This set is more than a subset of G, it is a subgroup. This subgroup is called the stabilizer subgroup or isotropy subgroup of x. We will denote the stabilizer subgroup of x by Gx . 160 CHAPTER 14. GROUP ACTIONS Remark 14.8. It is important to remember that Xg ⊂ X and Gx ⊂ G. Example 14.9. Let X = {1, 2, 3, 4, 5, 6} and suppose that G is the permutation group given by the permutations {(1), (12)(3456), (35)(46), (12)(3654)}. Then the fixed point sets of X under the action of G are X(1) = X, X(35)(46) = {1, 2}, X(12)(3456) = X(12)(3654) = ∅, and the stabilizer subgroups are G1 = G2 = {(1), (35)(46)}, G3 = G4 = G5 = G6 = {(1)}. It is easily seen that Gx is a subgroup of G for each x ∈ X. Proposition 14.10. Let G be a group acting on a set X and x ∈ X. The stabilizer group of x, Gx , is a subgroup of G. Proof. Clearly, e ∈ Gx since the identity fixes every element in the set X. Let g, h ∈ Gx . Then gx = x and hx = x. So (gh)x = g(hx) = gx = x; hence, the product of two elements in Gx is also in Gx . Finally, if g ∈ Gx , then x = ex = (g −1 g)x = (g −1 )gx = g −1 x. So g −1 is in Gx . We will denote the number of elements in the fixed point set of an element g ∈ G by |Xg | and denote the number of elements in the orbit of x ∈ X by |Ox |. The next theorem demonstrates the relationship between orbits of an element x ∈ X and the left cosets of Gx in G. Theorem 14.11. Let G be a finite group and X a finite G-set. If x ∈ X, then |Ox | = [G : Gx ]. Proof. We know that |G|/|Gx | is the number of left cosets of Gx in G by Lagrange’s Theorem (Theorem 6.10). We will define a bijective map ϕ between the orbit Ox of X and the set of left cosets LGx of Gx in G. Let y ∈ Ox . Then there exists a g in G such that gx = y. Define ϕ by ϕ(y) = gGx . To show that ϕ is one-to-one, assume that ϕ(y1 ) = ϕ(y2 ). Then ϕ(y1 ) = g1 Gx = g2 Gx = ϕ(y2 ), where g1 x = y1 and g2 x = y2 . Since g1 Gx = g2 Gx , there exists a g ∈ Gx such that g2 = g1 g, y2 = g2 x = g1 gx = g1 x = y1 ; consequently, the map ϕ is one-to-one. Finally, we must show that the map ϕ is onto. Let gGx be a left coset. If gx = y, then ϕ(y) = gGx . 14.2. THE CLASS EQUATION 161 14.2 The Class Equation Let X be a finite G-set and XG be the set of fixed points in X; that is, XG = {x ∈ X : gx = x for all g ∈ G}. Since the orbits of the action partition X, ∑ n |X| = |XG | + |Oxi |, i=k where xk , . . . , xn are representatives from the distinct nontrivial orbits of X. Now consider the special case in which G acts on itself by conjugation, (g, x) 7→ gxg −1 . The center of G, Z(G) = {x : xg = gx for all g ∈ G}, is the set of points that are fixed by conjugation. The nontrivial orbits of the action are called the conjugacy classes of G. If x1 , . . . , xk are representatives from each of the nontrivial conjugacy classes of G and |Ox1 | = n1 , . . . , |Oxk | = nk , then |G| = |Z(G)| + n1 + · · · + nk . The stabilizer subgroups of each of the xi ’s, C(xi ) = {g ∈ G : gxi = xi g}, are called the centralizer subgroups of the xi ’s. From Theorem 14.11, we obtain the class equation: |G| = |Z(G)| + [G : C(x1 )] + · · · + [G : C(xk )]. One of the consequences of the class equation is that the order of each conjugacy class must divide the order of G. Example 14.12. It is easy to check that the conjugacy classes in S3 are the following: {(1)}, {(123), (132)}, {(12), (13), (23)}. The class equation is 6 = 1 + 2 + 3. Example 14.13. The center of D4 is {(1), (13)(24)}, and the conjugacy classes are {(13), (24)}, {(1432), (1234)}, {(12)(34), (14)(23)}. Thus, the class equation for D4 is 8 = 2 + 2 + 2 + 2. Example 14.14. For Sn it takes a bit of work to find the conjugacy classes. We begin with cycles. Suppose that σ = (a1 , . . . , ak ) is a cycle and let τ ∈ Sn . By Theorem 6.16, τ στ −1 = (τ (a1 ), . . . , τ (ak )). Consequently, any two cycles of the same length are conjugate. Now let σ = σ1 σ2 · · · σr be a cycle decomposition, where the length of each cycle σi is ri . Then σ is conjugate to every other τ ∈ Sn whose cycle decomposition has the same lengths. The number of conjugate classes in Sn is the number of ways in which n can be parti- tioned into sums of positive integers. In the case of S3 for example, we can partition the integer 3 into the following three sums: 3=1+1+1 3=1+2 162 CHAPTER 14. GROUP ACTIONS 3 = 3; therefore, there are three conjugacy classes. The problem of finding the number of such partitions for any positive integer n is what computer scientists call NP-complete. This effectively means that the problem cannot be solved for a large n because the computations would be too time-consuming for even the largest computer. Theorem 14.15. Let G be a group of order pn where p is prime. Then G has a nontrivial center. Proof. We apply the class equation |G| = |Z(G)| + n1 + · · · + nk . Since each ni > 1 and ni | |G|, it follows that p must divide each ni . Also, p | |G|; hence, p must divide |Z(G)|. Since the identity is always in the center of G, |Z(G)| ≥ 1. Therefore, |Z(G)| ≥ p, and there exists some g ∈ Z(G) such that g ̸= 1. Corollary 14.16. Let G be a group of order p2 where p is prime. Then G is abelian. Proof. By Theorem 14.15, |Z(G)| = p or p2 . If |Z(G)| = p2 , then we are done. Suppose that |Z(G)| = p. Then Z(G) and G/Z(G) both have order p and must both be cyclic groups. Choosing a generator aZ(G) for G/Z(G), we can write any element gZ(G) in the quotient group as am Z(G) for some integer m; hence, g = am x for some x in the center of G. Similarly, if hZ(G) ∈ G/Z(G), there exists a y in Z(G) such that h = an y for some integer n. Since x and y are in the center of G, they commute with all other elements of G; therefore, gh = am xan y = am+n xy = an yam x = hg, and G must be abelian. 14.3 Burnside’s Counting Theorem Suppose that we wish to color the vertices of a square with two different colors, say black and white. We might suspect that there would be 24 = 16 different colorings. However, some of these colorings are equivalent. If we color the first vertex black and the remaining vertices white, it is the same as coloring the second vertex black and the remaining ones white since we could obtain the second coloring simply by rotating the square 90◦ (Figure 14.17). B W W B W W W W W W W W B W W B Figure 14.17: Equivalent colorings of square 14.3. BURNSIDE’S COUNTING THEOREM 163 Burnside’s Counting Theorem offers a method of computing the number of distinguish- able ways in which something can be done. In addition to its geometric applications, the theorem has interesting applications to areas in switching theory and chemistry. The proof of Burnside’s Counting Theorem depends on the following lemma. Lemma 14.18. Let X be a G-set and suppose that x ∼ y. Then Gx is isomorphic to Gy . In particular, |Gx | = |Gy |. Proof. Let G act on X by (g, x) 7→ g · x. Since x ∼ y, there exists a g ∈ G such that g · x = y. Let a ∈ Gx . Since gag −1 · y = ga · g −1 y = ga · x = g · x = y, we can define a map ϕ : Gx → Gy by ϕ(a) = gag −1 . The map ϕ is a homomorphism since ϕ(ab) = gabg −1 = gag −1 gbg −1 = ϕ(a)ϕ(b). Suppose that ϕ(a) = ϕ(b). Then gag −1 = gbg −1 or a = b; hence, the map is injective. To show that ϕ is onto, let b be in Gy ; then g −1 bg is in Gx since g −1 bg · x = g −1 b · gx = g −1 b · y = g −1 · y = x; and ϕ(g −1 bg) = b. Theorem 14.19 Burnside. Let G be a finite group acting on a set X and let k denote the number of orbits of X. Then 1 ∑ k= |Xg |. |G| g∈G Proof. We look at all the fixed points x of all the elements in g ∈ G; that is, we look at all g’s and all x’s such that gx = x. If viewed in terms of fixed point sets, the number of all g’s fixing x’s is ∑ |Xg |. g∈G However, if viewed in terms of the stabilizer subgroups, this number is ∑ |Gx |; x∈X ∑ ∑ hence, g∈G |Xg | = x∈X |Gx |. By Lemma 14.18, ∑ |Gy | = |Ox | · |Gx |. y∈Ox By Theorem 14.11 and Lagrange’s Theorem, this expression is equal to |G|. Summing over all of the k distinct orbits, we conclude that ∑ ∑ |Xg | = |Gx | = k · |G|. g∈G x∈X Example 14.20. Let X = {1, 2, 3, 4, 5} and suppose that G is the permutation group G = {(1), (13), (13)(25), (25)}. The orbits of X are {1, 3}, {2, 5}, and {4}. The fixed point sets are X(1) = X 164 CHAPTER 14. GROUP ACTIONS X(13) = {2, 4, 5} X(13)(25) = {4} X(25) = {1, 3, 4}. Burnside’s Theorem says that 1 ∑ 1 k= |Xg | = (5 + 3 + 1 + 3) = 3. |G| 4 g∈G A Geometric Example Before we apply Burnside’s Theorem to switching-theory problems, let us examine the number of ways in which the vertices of a square can be colored black or white. Notice that we can sometimes obtain equivalent colorings by simply applying a rigid motion to the square. For instance, as we have pointed out, if we color one of the vertices black and the remaining three white, it does not matter which vertex was colored black since a rotation will give an equivalent coloring. The symmetry group of a square, D4 , is given by the following permutations: (1) (13) (24) (1432) (1234) (12)(34) (14)(23) (13)(24) The group G acts on the set of vertices {1, 2, 3, 4} in the usual manner. We can describe the different colorings by mappings from X into Y = {B, W } where B and W represent the colors black and white, respectively. Each map f : X → Y describes a way to color the corners of the square. Every σ ∈ D4 induces a permutation σ e of the possible colorings given by σe(f ) = f ◦ σ for f : X → Y . For example, suppose that f is defined by f (1) = B f (2) = W f (3) = W f (4) = W and σ = (12)(34). Then σ e(f ) = f ◦ σ sends vertex 2 to B and the remaining vertices to e is a permutation group G W . The set of all such σ e on the set of possible colorings. Let Xe e denote the set of all possible colorings; that is, X is the set of all possible maps from X to e Y . Now we must compute the number of G-equivalence classes. e(1) = X 1. X e since the identity fixes every possible coloring. |X| e = 24 = 16. 2. Xe(1234) consists of all f ∈ X e such that f is unchanged by the permutation (1234). In this case f (1) = f (2) = f (3) = f (4), so that all values of f must be the same; that is, either f (x) = B or f (x) = W for every vertex x of the square. So |X e(1234) | = 2. e(1432) | = 2. 3. |X e(13)(24) , f (1) = f (3) and f (2) = f (4). Thus, |X 4. For X e(13)(24) | = 22 = 4. e(12)(34) | = 4. 5. |X e(14)(23) | = 4. 6. |X 14.3. BURNSIDE’S COUNTING THEOREM 165 e(13) , f (1) = f (3) and the other corners can be of any color; hence, |X 7. For X e(13) | = 3 2 = 8. e(24) | = 8. 8. |X By Burnside’s Theorem, we can conclude that there are exactly 1 4 (2 + 21 + 22 + 21 + 22 + 22 + 23 + 23 ) = 6 8 ways to color the vertices of the square. Proposition 14.21. Let G be a permutation group of X and X e the set of functions from e e X to Y . Then there exists a permutation group G acting on X, where σ e∈G e is defined by e(f ) = f ◦ σ for σ ∈ G and f ∈ X. σ e Furthermore, if n is the number of cycles in the cycle e decomposition of σ, then |Xσ | = |Y |n . Proof. Let σ ∈ G and f ∈ X. e Clearly, f ◦ σ is also in X. e Suppose that g is another e(f ) = σ function from X to Y such that σ e(g). Then for each x ∈ X, e(f )(x) = σ f (σ(x)) = σ e(g)(x) = g(σ(x)). Since σ is a permutation of X, every element x′ in X is the image of some x in X under σ; hence, f and g agree on all elements of X. Therefore, f = g and σ e is injective. The map σ 7→ σ e is onto, since the two sets are the same size. Suppose that σ is a permutation of X with cycle decomposition σ = σ1 σ2 · · · σn . Any f in Xeσ must have the same value on each cycle of σ. Since there are n cycles and |Y | eσ | = |Y |n . possible values for each cycle, |X Example 14.22. Let X = {1, 2, . . . , 7} and suppose that Y = {A, B, C}. If g is the permutation of X given by (13)(245) = (13)(245)(6)(7), then n = 4. Any f ∈ X eg must have the same value on each cycle in g. There are |Y | = 3 such choices for any value, so eg | = 34 = 81. |X Example 14.23. Suppose that we wish to color the vertices of a square using four different colors. By Proposition 14.21, we can immediately decide that there are 1 4 (4 + 41 + 42 + 41 + 42 + 42 + 43 + 43 ) = 55 8 possible ways. Switching Functions In switching theory we are concerned with the design of electronic circuits with binary inputs and outputs. The simplest of these circuits is a switching function that has n inputs and a single output (Figure 14.24). Large electronic circuits can often be constructed by combining smaller modules of this kind. The inherent problem here is that even for a simple circuit a large number of different switching functions can be constructed. With only four inputs and a single output, we can construct 65,536 different switching functions. However, we can often replace one switching function with another merely by permuting the input leads to the circuit (Figure 14.25). 166 CHAPTER 14. GROUP ACTIONS x1 x2 .. f f (x1 , x2 , . . . , xn ) . xn Figure 14.24: A switching function of n variables We define a switching or Boolean function of n variables to be a function from Zn2 to Z2 . Since any switching function can have two possible values for each binary n-tuple n and there are 2n binary n-tuples, 22 switching functions are possible for n variables. In general, allowing permutations of the inputs greatly reduces the number of different kinds of modules that are needed to build a large circuit. a a f f (a, b) f f (b, a) = g(a, b) b b Figure 14.25: A switching function of two variables The possible switching functions with two input variables a and b are listed in Ta- ble 14.26. Two switching functions f and g are equivalent if g can be obtained from f by a permutation of the input variables. For example, g(a, b, c) = f (b, c, a). In this case g ∼ f via the permutation (acb). In the case of switching functions of two variables, the permutation (ab) reduces 16 possible switching functions to 12 equivalent functions since f2 ∼ f4 f3 ∼ f5 f10 ∼ f12 f11 ∼ f13 . Inputs Outputs f0 f1 f2 f3 f4 f5 f6 f7 0 0 0 0 0 0 0 0 0 0 0 1 0 0 0 0 1 1 1 1 1 0 0 0 1 1 0 0 1 1 1 1 0 1 0 1 0 1 0 1 Inputs Outputs f8 f9 f10 f11 f12 f13 f14 f15 0 0 1 1 1 1 1 1 1 1 0 1 0 0 0 0 1 1 1 1 1 0 0 0 1 1 0 0 1 1 1 1 0 1 0 1 0 1 0 1 Table 14.26: Switching functions in two variables 3 For three input variables there are 22 = 256 possible switching functions; in the case 4 of four variables there are 22 = 65,536. The number of equivalence classes is too large to 14.3. BURNSIDE’S COUNTING THEOREM 167 reasonably calculate directly. It is necessary to employ Burnside’s Theorem. Consider a switching function with three possible inputs, a, b, and c. As we have mentioned, two switching functions f and g are equivalent if a permutation of the input variables of f gives g. It is important to notice that a permutation of the switching functions is not simply a permutation of the input values {a, b, c}. A switching function is a set of output values for the inputs a, b, and c, so when we consider equivalent switching functions, we are permuting 23 possible outputs, not just three input values. For example, each binary triple (a, b, c) has a specific output associated with it. The permutation (acb) changes outputs as follows: (0, 0, 0) 7→ (0, 0, 0) (0, 0, 1) 7→ (0, 1, 0) (0, 1, 0) 7→ (1, 0, 0) .. . (1, 1, 0) 7→ (1, 0, 1) (1, 1, 1) 7→ (1, 1, 1). Let X be the set of output values for a switching function in n variables. Then |X| = 2n . We can enumerate these values as follows: (0, . . . , 0, 1) 7→ 0 (0, . . . , 1, 0) 7→ 1 (0, . . . , 1, 1) 7→ 2 .. . (1, . . . , 1, 1) 7→ 2n − 1. Now let us consider a circuit with four input variables and a single output. Suppose that we can permute the leads of any circuit according to the following permutation group: (a), (ac), (bd), (adcb), (abcd), (ab)(cd), (ad)(bc), (ac)(bd). The permutations of the four possible input variables induce the permutations of the output values in Table 14.27. Hence, there are 1 16 (2 + 2 · 212 + 2 · 26 + 3 · 210 ) = 9616 8 possible switching functions of four variables under this group of permutations. This number will be even smaller if we consider the full symmetric group on four letters. 168 CHAPTER 14. GROUP ACTIONS Group Number Permutation Switching Function Permutation of Cycles (a) (0) 16 (ac) (2, 8)(3, 9)(6, 12)(7, 13) 12 (bd) (1, 4)(3, 6)(9, 12)(11, 14) 12 (adcb) (1, 2, 4, 8)(3, 6.12, 9)(5, 10)(7, 14, 13, 11) 6 (abcd) (1, 8, 4, 2)(3, 9, 12, 6)(5, 10)(7, 11, 13, 14) 6 (ab)(cd) (1, 2)(4, 8)(5, 10)(6, 9)(7, 11)(13, 14) 10 (ad)(bc) (1, 8)(2, 4)(3, 12)(5, 10)(7, 14)(11, 13) 10 (ac)(bd) (1, 4)(2, 8)(3, 12)(6, 9)(7, 13)(11, 14) 10 Table 14.27: Permutations of switching functions in four variables Sage Sage has many commands related to conjugacy, which is a group action. It also has commands for orbits and stabilizers of permutation groups. In the supplement, we illustrate the automorphism group of a (combinatorial) graph as another example of a group action on the vertex set of the graph. Historical Note William Burnside was born in London in 1852. He attended Cambridge University from 1871 to 1875 and won the Smith’s Prize in his last year. After his graduation he lectured at Cambridge. He was made a member of the Royal Society in 1893. Burnside wrote approximately 150 papers on topics in applied mathematics, differential geometry, and probability, but his most famous contributions were in group theory. Several of Burnside’s conjectures have stimulated research to this day. One such conjecture was that every group of odd order is solvable; that is, for a group G of odd order, there exists a sequence of subgroups G = Hn ⊃ Hn−1 ⊃ · · · ⊃ H1 ⊃ H0 = {e} such that Hi is normal in Hi+1 and Hi+1 /Hi is abelian. This conjecture was finally proven by W. Feit and J. Thompson in 1963. Burnside’s The Theory of Groups of Finite Order, published in 1897, was one of the first books to treat groups in a modern context as opposed to permutation groups. The second edition, published in 1911, is still a classic. 14.4 Exercises 1. Examples 14.1–14.5 in the first section each describe an action of a group G on a set X, which will give rise to the equivalence relation defined by G-equivalence. For each example, compute the equivalence classes of the equivalence relation, the G-equivalence classes. 2. Compute all Xg and all Gx for each of the following permutation groups. (a) X = {1, 2, 3}, G = S3 = {(1), (12), (13), (23), (123), (132)} (b) X = {1, 2, 3, 4, 5, 6}, G = {(1), (12), (345), (354), (12)(345), (12)(354)} 3. Compute the G-equivalence classes of X for each of the G-sets in Exercise 14.4.2. For each x ∈ X verify that |G| = |Ox | · |Gx |. 14.4. EXERCISES 169 4. Let G be the additive group of real numbers. Let the action of θ ∈ G on the real plane R2 be given by rotating the plane counterclockwise about the origin through θ radians. Let P be a point on the plane other than the origin. (a) Show that R2 is a G-set. (b) Describe geometrically the orbit containing P . (c) Find the group GP . 5. Let G = A4 and suppose that G acts on itself by conjugation; that is, (g, h) 7→ ghg −1 . (a) Determine the conjugacy classes (orbits) of each element of G. (b) Determine all of the isotropy subgroups for each element of G. 6. Find the conjugacy classes and the class equation for each of the following groups. (a) S4 (b) D5 (c) Z9 (d) Q8 7. Write the class equation for S5 and for A5 . 8. If a square remains fixed in the plane, how many different ways can the corners of the square be colored if three colors are used? 9. How many ways can the vertices of an equilateral triangle be colored using three different colors? 10. Find the number of ways a six-sided die can be constructed if each side is marked differently with 1, . . . , 6 dots. 11. Up to a rotation, how many ways can the faces of a cube be colored with three different colors? 12. Consider 12 straight wires of equal lengths with their ends soldered together to form the edges of a cube. Either silver or copper wire can be used for each edge. How many different ways can the cube be constructed? 13. Suppose that we color each of the eight corners of a cube. Using three different colors, how many ways can the corners be colored up to a rotation of the cube? 14. Each of the faces of a regular tetrahedron can be painted either red or white. Up to a rotation, how many different ways can the tetrahedron be painted? 15. Suppose that the vertices of a regular hexagon are to be colored either red or white. How many ways can this be done up to a symmetry of the hexagon? 16. A molecule of benzene is made up of six carbon atoms and six hydrogen atoms, linked together in a hexagonal shape as in Figure 14.28. (a) How many different compounds can be formed by replacing one or more of the hy- drogen atoms with a chlorine atom? (b) Find the number of different chemical compounds that can be formed by replacing three of the six hydrogen atoms in a benzene ring with a CH3 radical. 170 CHAPTER 14. GROUP ACTIONS H H H H H H Figure 14.28: A benzene ring 17. How many equivalence classes of switching functions are there if the input variables x1 , x2 , and x3 can be permuted by any permutation in S3 ? What if the input variables x1 , x2 , x3 , and x4 can be permuted by any permutation in S4 ? 18. How many equivalence classes of switching functions are there if the input variables x1 , x2 , x3 , and x4 can be permuted by any permutation in the subgroup of S4 generated by the permutation (x1 x2 x3 x4 )? 19. A striped necktie has 12 bands of color. Each band can be colored by one of four possible colors. How many possible different-colored neckties are there? 20. A group acts faithfully on a G-set X if the identity is the only element of G that leaves every element of X fixed. Show that G acts faithfully on X if and only if no two distinct elements of G have the same action on each element of X. 21. Let p be prime. Show that the number of different abelian groups of order pn (up to isomorphism) is the same as the number of conjugacy classes in Sn . 22. Let a ∈ G. Show that for any g ∈ G, gC(a)g −1 = C(gag −1 ). 23. Let |G| = pn be a nonabelian group for p prime. Prove that |Z(G)| < pn−1 . 24. Let G be a group with order pn where p is prime and X a finite G-set. If XG = {x ∈ X : gx = x for all g ∈ G} is the set of elements in X fixed by the group action, then prove that |X| ≡ |XG | (mod p). 25. If G is a group of order pn , where p is prime and n ≥ 2, show that G must have a proper subgroup of order p. If n ≥ 3, is it true that G will have a proper subgroup of order p2 ? 14.5 Programming Exercise 1. Write a program to compute the number of conjugacy classes in Sn . What is the largest n for which your program will work? References and Suggested Reading [1] De Bruijin, N. G. “Pólya’s Theory of Counting,” in Applied Combinatorial Mathemat- ics, Beckenbach, E. F., ed. Wiley, New York, 1964. 14.5. PROGRAMMING EXERCISE 171 [2] Eidswick, J. A. “Cubelike Puzzles—What Are They and How Do You Solve Them?” American Mathematical Monthly 93(1986), 157–76. [3] Harary, F., Palmer, E. M., and Robinson, R. W. “Pólya’s Contributions to Chem- ical Enumeration,” in Chemical Applications of Graph Theory, Balaban, A. T., ed. Academic Press, London, 1976. [4] Gårding, L. and Tambour, T. Algebra for Computer Science. Springer-Verlag, New York, 1988. [5] Laufer, H. B. Discrete Mathematics and Applied Modern Algebra. PWS-Kent, Boston, 1984. [6] Pólya, G. and Read, R. C. Combinatorial Enumeration of Groups, Graphs, and Chem- ical Compounds. Springer-Verlag, New York, 1985. [7] Shapiro, L. W. “Finite Groups Acting on Sets with Applications,” Mathematics Mag- azine, May–June 1973, 136–47. 15 The Sylow Theorems We already know that the converse of Lagrange’s Theorem is false. If G is a group of order m and n divides m, then G does not necessarily possess a subgroup of order n. For example, A4 has order 12 but does not possess a subgroup of order 6. However, the Sylow Theorems do provide a partial converse for Lagrange’s Theorem—in certain cases they guarantee us subgroups of specific orders. These theorems yield a powerful set of tools for the classification of all finite nonabelian groups. 15.1 The Sylow Theorems We will use what we have learned about group actions to prove the Sylow Theorems. Recall for a moment what it means for G to act on itself by conjugation and how conjugacy classes are distributed in the group according to the class equation, discussed in Chapter 14. A group G acts on itself by conjugation via the map (g, x) 7→ gxg −1 . Let x1 , . . . , xk be representatives from each of the distinct conjugacy classes of G that consist of more than one element. Then the class equation can be written as |G| = |Z(G)| + [G : C(x1 )] + · · · + [G : C(xk )], where Z(G) = {g ∈ G : gx = xg for all x ∈ G} is the center of G and C(xi ) = {g ∈ G : gxi = xi g} is the centralizer subgroup of xi . We begin our investigation of the Sylow Theorems by examining subgroups of order p, where p is prime. A group G is a p-group if every element in G has as its order a power of p, where p is a prime number. A subgroup of a group G is a p-subgroup if it is a p-group. Theorem 15.1 Cauchy. Let G be a finite group and p a prime such that p divides the order of G. Then G contains a subgroup of order p. Proof. We will use induction on the order of G. If |G| = p, then clearly G itself is the required subgroup. We now assume that every group of order k, where p ≤ k < n and p divides k, has an element of order p. Assume that |G| = n and p | n and consider the class equation of G: |G| = |Z(G)| + [G : C(x1 )] + · · · + [G : C(xk )]. We have two cases. Case 1. Suppose the order of one of the centralizer subgroups, C(xi ), is divisible by p for some i, i = 1, . . . , k. In this case, by our induction hypothesis, we are done. Since C(xi ) is a proper subgroup of G and p divides |C(xi )|, C(xi ) must contain an element of order p. Hence, G must contain an element of order p. Case 2. Suppose the order of no centralizer subgroup is divisible by p. Then p divides [G : C(xi )], the order of each conjugacy class in the class equation; hence, p must divide 172 15.1. THE SYLOW THEOREMS 173 the center of G, Z(G). Since Z(G) is abelian, it must have a subgroup of order p by the Fundamental Theorem of Finite Abelian Groups. Therefore, the center of G contains an element of order p. Corollary 15.2. Let G be a finite group. Then G is a p-group if and only if |G| = pn . Example 15.3. Let us consider the group A5 . We know that |A5 | = 60 = 22 · 3 · 5. By Cauchy’s Theorem, we are guaranteed that A5 has subgroups of orders 2, 3 and 5. The Sylow Theorems will give us even more information about the possible subgroups of A5 . We are now ready to state and prove the first of the Sylow Theorems. The proof is very similar to the proof of Cauchy’s Theorem. Theorem 15.4 First Sylow Theorem. Let G be a finite group and p a prime such that pr divides |G|. Then G contains a subgroup of order pr . Proof. We induct on the order of G once again. If |G| = p, then we are done. Now suppose that the order of G is n with n > p and that the theorem is true for all groups of order less than n, where p divides n. We shall apply the class equation once again: |G| = |Z(G)| + [G : C(x1 )] + · · · + [G : C(xk )]. First suppose that p does not divide [G : C(xi )] for some i. Then pr | |C(xi )|, since pr divides |G| = |C(xi )| · [G : C(xi )]. Now we can apply the induction hypothesis to C(xi ). Hence, we may assume that p divides [G : C(xi )] for all i. Since p divides |G|, the class equation says that p must divide |Z(G)|; hence, by Cauchy’s Theorem, Z(G) has an element of order p, say g. Let N be the group generated by g. Clearly, N is a normal subgroup of Z(G) since Z(G) is abelian; therefore, N is normal in G since every element in Z(G) commutes with every element in G. Now consider the factor group G/N of order |G|/p. By the induction hypothesis, G/N contains a subgroup H of order pr−1 . The inverse image of H under the canonical homomorphism ϕ : G → G/N is a subgroup of order pr in G. A Sylow p-subgroup P of a group G is a maximal p-subgroup of G. To prove the other two Sylow Theorems, we need to consider conjugate subgroups as opposed to conjugate elements in a group. For a group G, let S be the collection of all subgroups of G. For any subgroup H, S is a H-set, where H acts on S by conjugation. That is, we have an action H ×S →S defined by h · K 7→ hKh−1 for K in S. The set N (H) = {g ∈ G : gHg −1 = H} is a subgroup of G called the the normalizer of H in G. Notice that H is a normal subgroup of N (H). In fact, N (H) is the largest subgroup of G in which H is normal. Lemma 15.5. Let P be a Sylow p-subgroup of a finite group G and let x have as its order a power of p. If x−1 P x = P , then x ∈ P . Proof. Certainly x ∈ N (P ), and the cyclic subgroup, ⟨xP ⟩ ⊂ N (P )/P , has as its order a power of p. By the Correspondence Theorem there exists a subgroup H of N (P ) containing P such that H/P = ⟨xP ⟩. Since |H| = |P | · |⟨xP ⟩|, the order of H must be a power of p. However, P is a Sylow p-subgroup contained in H. Since the order of P is the largest power of p dividing |G|, H = P . Therefore, H/P is the trivial subgroup and xP = P , or x ∈ P. 174 CHAPTER 15. THE SYLOW THEOREMS Lemma 15.6. Let H and K be subgroups of G. The number of distinct H-conjugates of K is [H : N (K) ∩ H]. Proof. We define a bijection between the conjugacy classes of K and the right cosets of N (K) ∩ H by h−1 Kh 7→ (N (K) ∩ H)h. To show that this map is a bijection, let h1 , h2 ∈ H and suppose that (N (K) ∩ H)h1 = (N (K) ∩ H)h2 . Then h2 h−1 1 ∈ N (K). Therefore, −1 −1 −1 −1 K = h2 h1 Kh1 h2 or h1 Kh1 = h2 Kh2 , and the map is an injection. It is easy to see that this map is surjective; hence, we have a one-to-one and onto map between the H-conjugates of K and the right cosets of N (K) ∩ H in H. Theorem 15.7 Second Sylow Theorem. Let G be a finite group and p a prime dividing |G|. Then all Sylow p-subgroups of G are conjugate. That is, if P1 and P2 are two Sylow p-subgroups, there exists a g ∈ G such that gP1 g −1 = P2 . Proof. Let P be a Sylow p-subgroup of G and suppose that |G| = pr m with |P | = pr . Let S = {P = P1 , P2 , . . . , Pk } consist of the distinct conjugates of P in G. By Lemma 15.6, k = [G : N (P )]. Notice that |G| = pr m = |N (P )| · [G : N (P )] = |N (P )| · k. Since pr divides |N (P )|, p cannot divide k. Given any other Sylow p-subgroup Q, we must show that Q ∈ S. Consider the Q- conjugacy classes of each Pi . Clearly, these conjugacy classes partition S. The size of the partition containing Pi is [Q : N (Pi ) ∩ Q] by Lemma 15.6, and Lagrange’s Theorem tells us that |Q| = [Q : N (Pi ) ∩ Q]|N (Pi ) ∩ Q|. Thus, [Q : N (Pi ) ∩ Q] must be a divisor of |Q| = pr . Hence, the number of conjugates in every equivalence class of the partition is a power of p. However, since p does not divide k, one of these equivalence classes must contain only a single Sylow p-subgroup, say Pj . In this case, x−1 Pj x = Pj for all x ∈ Q. By Lemma 15.5, Pj = Q. Theorem 15.8 Third Sylow Theorem. Let G be a finite group and let p be a prime dividing the order of G. Then the number of Sylow p-subgroups is congruent to 1 (mod p) and divides |G|. Proof. Let P be a Sylow p-subgroup acting on the set of Sylow p-subgroups, S = {P = P1 , P2 , . . . , Pk }, by conjugation. From the proof of the Second Sylow Theorem, the only P -conjugate of P is itself and the order of the other P -conjugacy classes is a power of p. Each P -conjugacy class contributes a positive power of p toward |S| except the equivalence class {P }. Since |S| is the sum of positive powers of p and 1, |S| ≡ 1 (mod p). Now suppose that G acts on S by conjugation. Since all Sylow p-subgroups are conju- gate, there can be only one orbit under this action. For P ∈ S, |S| = |orbit of P | = [G : N (P )] by Lemma 15.6. But [G : N (P )] is a divisor of |G|; consequently, the number of Sylow p-subgroups of a finite group must divide the order of the group. 15.2. EXAMPLES AND APPLICATIONS 175 Historical Note Peter Ludvig Mejdell Sylow was born in 1832 in Christiania, Norway (now Oslo). After attending Christiania University, Sylow taught high school. In 1862 he obtained a temporary appointment at Christiania University. Even though his appointment was relatively brief, he influenced students such as Sophus Lie (1842–1899). Sylow had a chance at a permanent chair in 1869, but failed to obtain the appointment. In 1872, he published a 10-page paper presenting the theorems that now bear his name. Later Lie and Sylow collaborated on a new edition of Abel’s works. In 1898, a chair at Christiania University was finally created for Sylow through the efforts of his student and colleague Lie. Sylow died in 1918. 15.2 Examples and Applications Example 15.9. Using the Sylow Theorems, we can determine that A5 has subgroups of orders 2, 3, 4, and 5. The Sylow p-subgroups of A5 have orders 3, 4, and 5. The Third Sylow Theorem tells us exactly how many Sylow p-subgroups A5 has. Since the number of Sylow 5-subgroups must divide 60 and also be congruent to 1 (mod 5), there are either one or six Sylow 5-subgroups in A5 . All Sylow 5-subgroups are conjugate. If there were only a single Sylow 5-subgroup, it would be conjugate to itself; that is, it would be a normal subgroup of A5 . Since A5 has no normal subgroups, this is impossible; hence, we have determined that there are exactly six distinct Sylow 5-subgroups of A5 . The Sylow Theorems allow us to prove many useful results about finite groups. By using them, we can often conclude a great deal about groups of a particular order if certain hypotheses are satisfied. Theorem 15.10. If p and q are distinct primes with p < q, then every group G of order pq has a single subgroup of order q and this subgroup is normal in G. Hence, G cannot be simple. Furthermore, if q ̸≡ 1 (mod p), then G is cyclic. Proof. We know that G contains a subgroup H of order q. The number of conjugates of H divides pq and is equal to 1 + kq for k = 0, 1, . . .. However, 1 + q is already too large to divide the order of the group; hence, H can only be conjugate to itself. That is, H must be normal in G. The group G also has a Sylow p-subgroup, say K. The number of conjugates of K must divide q and be equal to 1 + kp for k = 0, 1, . . .. Since q is prime, either 1 + kp = q or 1 + kp = 1. If 1 + kp = 1, then K is normal in G. In this case, we can easily show that G satisfies the criteria, given in Chapter 9, for the internal direct product of H and K. Since H is isomorphic to Zq and K is isomorphic to Zp , G ∼ = Zp × Zq ∼= Zpq by Theorem 9.21. Example 15.11. Every group of order 15 is cyclic. This is true because 15 = 5 · 3 and 5 ̸≡ 1 (mod 3). Example 15.12. Let us classify all of the groups of order 99 = 32 · 11 up to isomorphism. First we will show that every group G of order 99 is abelian. By the Third Sylow Theorem, there are 1+3k Sylow 3-subgroups, each of order 9, for some k = 0, 1, 2, . . .. Also, 1+3k must divide 11; hence, there can only be a single normal Sylow 3-subgroup H in G. Similarly, there are 1+11k Sylow 11-subgroups and 1+11k must divide 9. Consequently, there is only one Sylow 11-subgroup K in G. By Corollary 14.16, any group of order p2 is abelian for p prime; hence, H is isomorphic either to Z3 × Z3 or to Z9 . Since K has order 11, it must be isomorphic to Z11 . Therefore, the only possible groups of order 99 are Z3 × Z3 × Z11 or Z9 × Z11 up to isomorphism. 176 CHAPTER 15. THE SYLOW THEOREMS To determine all of the groups of order 5 · 7 · 47 = 1645, we need the following theorem. Theorem 15.13. Let G′ = ⟨aba−1 b−1 : a, b ∈ G⟩ be the subgroup consisting of all finite products of elements of the form aba−1 b−1 in a group G. Then G′ is a normal subgroup of G and G/G′ is abelian. The subgroup G′ of G is called the commutator subgroup of G. We leave the proof of this theorem as an exercise (Exercise 10.3.14 in Chapter 10). Example 15.14. We will now show that every group of order 5 · 7 · 47 = 1645 is abelian, and cyclic by Corollary 9.21. By the Third Sylow Theorem, G has only one subgroup H1 of order 47. So G/H1 has order 35 and must be abelian by Theorem 15.10. Hence, the commutator subgroup of G is contained in H which tells us that |G′ | is either 1 or 47. If |G′ | = 1, we are done. Suppose that |G′ | = 47. The Third Sylow Theorem tells us that G has only one subgroup of order 5 and one subgroup of order 7. So there exist normal subgroups H2 and H3 in G, where |H2 | = 5 and |H3 | = 7. In either case the quotient group is abelian; hence, G′ must be a subgroup of Hi , i = 1, 2. Therefore, the order of G′ is 1, 5, or 7. However, we already have determined that |G′ | = 1 or 47. So the commutator subgroup of G is trivial, and consequently G is abelian. Finite Simple Groups Given a finite group, one can ask whether or not that group has any normal subgroups. Recall that a simple group is one with no proper nontrivial normal subgroups. As in the case of A5 , proving a group to be simple can be a very difficult task; however, the Sylow Theorems are useful tools for proving that a group is not simple. Usually, some sort of counting argument is involved. Example 15.15. Let us show that no group G of order 20 can be simple. By the Third Sylow Theorem, G contains one or more Sylow 5-subgroups. The number of such subgroups is congruent to 1 (mod 5) and must also divide 20. The only possible such number is 1. Since there is only a single Sylow 5-subgroup and all Sylow 5-subgroups are conjugate, this subgroup must be normal. Example 15.16. Let G be a finite group of order pn , n > 1 and p prime. By Theorem 14.15, G has a nontrivial center. Since the center of any group G is a normal subgroup, G cannot be a simple group. Therefore, groups of orders 4, 8, 9, 16, 25, 27, 32, 49, 64, and 81 are not simple. In fact, the groups of order 4, 9, 25, and 49 are abelian by Corollary 14.16. Example 15.17. No group of order 56 = 23 · 7 is simple. We have seen that if we can show that there is only one Sylow p-subgroup for some prime p dividing 56, then this must be a normal subgroup and we are done. By the Third Sylow Theorem, there are either one or eight Sylow 7-subgroups. If there is only a single Sylow 7-subgroup, then it must be normal. On the other hand, suppose that there are eight Sylow 7-subgroups. Then each of these subgroups must be cyclic; hence, the intersection of any two of these subgroups contains only the identity of the group. This leaves 8 · 6 = 48 distinct elements in the group, each of order 7. Now let us count Sylow 2-subgroups. There are either one or seven Sylow 2-subgroups. Any element of a Sylow 2-subgroup other than the identity must have as its order a power of 2; and therefore cannot be one of the 48 elements of order 7 in the Sylow 7-subgroups. Since a Sylow 2-subgroup has order 8, there is only enough room for a single Sylow 2-subgroup in a group of order 56. If there is only one Sylow 2-subgroup, it must be normal. 15.2. EXAMPLES AND APPLICATIONS 177 For other groups G, it is more difficult to prove that G is not simple. Suppose G has order 48. In this case the technique that we employed in the last example will not work. We need the following lemma to prove that no group of order 48 is simple. Lemma 15.18. Let H and K be finite subgroups of a group G. Then |H| · |K| |HK| = . |H ∩ K| Proof. Recall that HK = {hk : h ∈ H, k ∈ K}. Certainly, |HK| ≤ |H| · |K| since some element in HK could be written as the product of different elements in H and K. It is quite possible that h1 k1 = h2 k2 for h1 , h2 ∈ H and k1 , k2 ∈ K. If this is the case, let a = (h1 )−1 h2 = k1 (k2 )−1 . Notice that a ∈ H ∩ K, since (h1 )−1 h2 is in H and k2 (k1 )−1 is in K; consequently, h2 = h1 a−1 k2 = ak1 . Conversely, let h = h1 b−1 and k = bk1 for b ∈ H ∩ K. Then hk = h1 k1 , where h ∈ H and k ∈ K. Hence, any element hk ∈ HK can be written in the form hi ki for hi ∈ H and ki ∈ K, as many times as there are elements in H ∩ K; that is, |H ∩ K| times. Therefore, |HK| = (|H| · |K|)/|H ∩ K|. Example 15.19. To demonstrate that a group G of order 48 is not simple, we will show that G contains either a normal subgroup of order 8 or a normal subgroup of order 16. By the Third Sylow Theorem, G has either one or three Sylow 2-subgroups of order 16. If there is only one subgroup, then it must be a normal subgroup. Suppose that the other case is true, and two of the three Sylow 2-subgroups are H and K. We claim that |H ∩ K| = 8. If |H ∩ K| ≤ 4, then by Lemma 15.18, 16 · 16 |HK| = = 64, 4 which is impossible. Notice that H ∩ K has index two in both of H and K, so is normal in both, and thus H and K are each in the normalizer of H ∩ K. Because H is a subgroup of N (H ∩ K) and because N (H ∩ K) has strictly more than 16 elements, |N (H ∩ K)| must be a multiple of 16 greater than 1, as well as dividing 48. The only possibility is that |N (H ∩ K)| = 48. Hence, N (H ∩ K) = G. The following famous conjecture of Burnside was proved in a long and difficult paper by Feit and Thompson [2]. Theorem 15.20 Odd Order Theorem. Every finite simple group of nonprime order must be of even order. The proof of this theorem laid the groundwork for a program in the 1960s and 1970s that classified all finite simple groups. The success of this program is one of the outstanding achievements of modern mathematics. Sage Sage will compute a single Sylow p-subgroup for each prime divisor p of the order of the group. Then, with conjugacy, all of the Sylow p-subgroups can be enumerated. It is also possible to compute the normalizer of a subgroup. 178 CHAPTER 15. THE SYLOW THEOREMS 15.3 Exercises 1. What are the orders of all Sylow p-subgroups where G has order 18, 24, 54, 72, and 80? 2. Find all the Sylow 3-subgroups of S4 and show that they are all conjugate. 3. Show that every group of order 45 has a normal subgroup of order 9. 4. Let H be a Sylow p-subgroup of G. Prove that H is the only Sylow p-subgroup of G contained in N (H). 5. Prove that no group of order 96 is simple. 6. Prove that no group of order 160 is simple. 7. If H is a normal subgroup of a finite group G and |H| = pk for some prime p, show that H is contained in every Sylow p-subgroup of G. 8. Let G be a group of order p2 q 2 , where p and q are distinct primes such that q ∤ p2 − 1 and p ∤ q 2 − 1. Prove that G must be abelian. Find a pair of primes for which this is true. 9. Show that a group of order 33 has only one Sylow 3-subgroup. 10. Let H be a subgroup of a group G. Prove or disprove that the normalizer of H is normal in G. 11. Let G be a finite group divisible by a prime p. Prove that if there is only one Sylow p-subgroup in G, it must be a normal subgroup of G. 12. Let G be a group of order pr , p prime. Prove that G contains a normal subgroup of order pr−1 . 13. Suppose that G is a finite group of order pn k, where k < p. Show that G must contain a normal subgroup. 14. Let H be a subgroup of a finite group G. Prove that gN (H)g −1 = N (gHg −1 ) for any g ∈ G. 15. Prove that a group of order 108 must have a normal subgroup. 16. Classify all the groups of order 175 up to isomorphism. 17. Show that every group of order 255 is cyclic. 18. Let G have order pe11 · · · penn and suppose that G has n Sylow p-subgroups P1 , . . . , Pn where |Pi | = pei i . Prove that G is isomorphic to P1 × · · · × Pn . 19. Let P be a normal Sylow p-subgroup of G. Prove that every inner automorphism of G fixes P . 20. What is the smallest possible order of a group G such that G is nonabelian and |G| is odd? Can you find such a group? 21. The Frattini Lemma. If H is a normal subgroup of a finite group G and P is a Sylow p-subgroup of H, for each g ∈ G show that there is an h in H such that gP g −1 = hP h−1 . Also, show that if N is the normalizer of P , then G = HN . 22. Show that if the order of G is pn q, where p and q are primes and p > q, then G contains a normal subgroup. 23. Prove that the number of distinct conjugates of a subgroup H of a finite group G is [G : N (H)]. 24. Prove that a Sylow 2-subgroup of S5 is isomorphic to D4 . 25. Another Proof of the Sylow Theorems. (a) Suppose p is prime and p does not divide m. Show that ( k ) p m p∤ . pk 15.4. A PROJECT 179 (b) Let S denote the set of all pk element subsets of G. Show that p does not divide |S|. (c) Define an action of G on S by left multiplication, aT = {at : t ∈ T } for a ∈ G and T ∈ S. Prove that this is a group action. (d) Prove p ∤ |OT | for some T ∈ S. (e) Let {T1 , . . . , Tu } be an orbit such that p ∤ u and H = {g ∈ G : gT1 = T1 }. Prove that H is a subgroup of G and show that |G| = u|H|. (f) Show that pk divides |H| and pk ≤ |H|. (g) Show that |H| = |OT | ≤ pk ; conclude that therefore pk = |H|. 26. Let G be a group. Prove that G′ = ⟨aba−1 b−1 : a, b ∈ G⟩ is a normal subgroup of G and G/G′ is abelian. Find an example to show that {aba−1 b−1 : a, b ∈ G} is not necessarily a group. 15.4 A Project The main objective of finite group theory is to classify all possible finite groups up to isomorphism. This problem is very difficult even if we try to classify the groups of order less than or equal to 60. However, we can break the problem down into several intermediate problems. This is a challenging project that requires a working knowledge of the group theory you have learned up to this point. Even if you do not complete it, it will teach you a great deal about finite groups. You can use Table 15.21 as a guide. Order Number Order Number Order Number Order Number 1 ? 16 14 31 1 46 2 2 ? 17 1 32 51 47 1 3 ? 18 ? 33 1 48 52 4 ? 19 ? 34 ? 49 ? 5 ? 20 5 35 1 50 5 6 ? 21 ? 36 14 51 ? 7 ? 22 2 37 1 52 ? 8 ? 23 1 38 ? 53 ? 9 ? 24 ? 39 2 54 15 10 ? 25 2 40 14 55 2 11 ? 26 2 41 1 56 ? 12 5 27 5 42 ? 57 2 13 ? 28 ? 43 1 58 ? 14 ? 29 1 44 4 59 1 15 1 30 4 45 ? 60 13 Table 15.21: Numbers of distinct groups G, |G| ≤ 60 1. Find all simple groups G ( |G| ≤ 60). Do not use the Odd Order Theorem unless you are prepared to prove it. 2. Find the number of distinct groups G, where the order of G is n for n = 1, . . . , 60. 3. Find the actual groups (up to isomorphism) for each n. 180 CHAPTER 15. THE SYLOW THEOREMS References and Suggested Readings [1] Edwards, H. “A Short History of the Fields Medal,” Mathematical Intelligencer 1(1978), 127–29. [2] Feit, W. and Thompson, J. G. “Solvability of Groups of Odd Order,” Pacific Journal of Mathematics 13(1963), 775–1029. [3] Gallian, J. A. “The Search for Finite Simple Groups,” Mathematics Magazine 49(1976), 163–79. [4] Gorenstein, D. “Classifying the Finite Simple Groups,” Bulletin of the American Mathematical Society 14(1986), 1–98. [5] Gorenstein, D. Finite Groups. AMS Chelsea Publishing, Providence RI, 1968. [6] Gorenstein, D., Lyons, R., and Solomon, R. The Classification of Finite Simple Groups. American Mathematical Society, Providence RI, 1994. 16 Rings Up to this point we have studied sets with a single binary operation satisfying certain ax- ioms, but we are often more interested in working with sets that have two binary operations. For example, one of the most natural algebraic structures to study is the integers with the operations of addition and multiplication. These operations are related to one another by the distributive property. If we consider a set with two such related binary operations sat- isfying certain axioms, we have an algebraic structure called a ring. In a ring we add and multiply elements such as real numbers, complex numbers, matrices, and functions. 16.1 Rings A nonempty set R is a ring if it has two closed binary operations, addition and multipli- cation, satisfying the following conditions. 1. a + b = b + a for a, b ∈ R. 2. (a + b) + c = a + (b + c) for a, b, c ∈ R. 3. There is an element 0 in R such that a + 0 = a for all a ∈ R. 4. For every element a ∈ R, there exists an element −a in R such that a + (−a) = 0. 5. (ab)c = a(bc) for a, b, c ∈ R. 6. For a, b, c ∈ R, a(b + c) = ab + ac (a + b)c = ac + bc. This last condition, the distributive axiom, relates the binary operations of addition and multiplication. Notice that the first four axioms simply require that a ring be an abelian group under addition, so we could also have defined a ring to be an abelian group (R, +) together with a second binary operation satisfying the fifth and sixth conditions given above. If there is an element 1 ∈ R such that 1 ̸= 0 and 1a = a1 = a for each element a ∈ R, we say that R is a ring with unity or identity. A ring R for which ab = ba for all a, b in R is called a commutative ring. A commutative ring R with identity is called an integral domain if, for every a, b ∈ R such that ab = 0, either a = 0 or b = 0. A division ring is a ring R, with an identity, in which every nonzero element in R is a unit; that is, for each a ∈ R with a ̸= 0, there exists a unique element a−1 such that a−1 a = aa−1 = 1. A commutative division ring is called a field. The relationship among rings, integral domains, division rings, and fields is shown in Figure 16.1. 181 182 CHAPTER 16. RINGS Rings Commutative Rings with Rings Identity Integral Division Domains Rings Fields Figure 16.1: Types of rings Example 16.2. As we have mentioned previously, the integers form a ring. In fact, Z is an integral domain. Certainly if ab = 0 for two integers a and b, either a = 0 or b = 0. However, Z is not a field. There is no integer that is the multiplicative inverse of 2, since 1/2 is not an integer. The only integers with multiplicative inverses are 1 and −1. Example 16.3. Under the ordinary operations of addition and multiplication, all of the familiar number systems are rings: the rationals, Q; the real numbers, R; and the complex numbers, C. Each of these rings is a field. Example 16.4. We can define the product of two elements a and b in Zn by ab (mod n). For instance, in Z12 , 5 · 7 ≡ 11 (mod 12). This product makes the abelian group Zn into a ring. Certainly Zn is a commutative ring; however, it may fail to be an integral domain. If we consider 3 · 4 ≡ 0 (mod 12) in Z12 , it is easy to see that a product of two nonzero elements in the ring can be equal to zero. A nonzero element a in a ring R is called a zero divisor if there is a nonzero element b in R such that ab = 0. In the previous example, 3 and 4 are zero divisors in Z12 . Example 16.5. In calculus the continuous real-valued functions on an interval [a, b] form a commutative ring. We add or multiply two functions by adding or multiplying the values of the functions. If f (x) = x2 and g(x) = cos x, then (f + g)(x) = f (x) + g(x) = x2 + cos x and (f g)(x) = f (x)g(x) = x2 cos x. Example 16.6. The 2×2 matrices with entries in R form a ring under the usual operations of matrix addition and multiplication. This ring is noncommutative, since it is usually the case that AB ̸= BA. Also, notice that we can have AB = 0 when neither A nor B is zero. Example 16.7. For an example of a noncommutative division ring, let ( ) ( ) ( ) ( ) 1 0 0 1 0 i i 0 1= , i= , j= , k= , 0 1 −1 0 i 0 0 −i where i2 = −1. These elements satisfy the following relations: i2 = j2 = k2 = −1 ij = k jk = i ki = j ji = −k 16.1. RINGS 183 kj = −i ik = −j. Let H consist of elements of the form a + bi + cj + dk, where a, b, c, d are real numbers. Equivalently, H can be considered to be the set of all 2 × 2 matrices of the form ( ) α β , −β α where α = a + di and β = b + ci are complex numbers. We can define addition and multiplication on H either by the usual matrix operations or in terms of the generators 1, i, j, and k: (a1 + b1 i + c1 j + d1 k) + (a2 + b2 i + c2 j + d2 k) = (a1 + a2 ) + (b1 + b2 )i + (c1 + c2 )j + (d1 + d2 )k and (a1 + b1 i + c1 j + d1 k)(a2 + b2 i + c2 j + d2 k) = α + βi + γj + δk, where α = a1 a2 − b1 b2 − c1 c2 − d1 d2 β = a1 b2 + a2 b1 + c1 d2 − d1 c2 γ = a1 c2 − b1 d2 + c1 a2 + d1 b2 δ = a1 d2 + b1 c2 − c1 b2 + d1 a2 . Though multiplication looks complicated, it is actually a straightforward computation if we remember that we just add and multiply elements in H like polynomials and keep in mind the relationships between the generators i, j, and k. The ring H is called the ring of quaternions. To show that the quaternions are a division ring, we must be able to find an inverse for each nonzero element. Notice that (a + bi + cj + dk)(a − bi − cj − dk) = a2 + b2 + c2 + d2 . This element can be zero only if a, b, c, and d are all zero. So if a + bi + cj + dk ̸= 0, ( ) a − bi − cj − dk (a + bi + cj + dk) = 1. a2 + b2 + c2 + d2 Proposition 16.8. Let R be a ring with a, b ∈ R. Then 1. a0 = 0a = 0; 2. a(−b) = (−a)b = −ab; 3. (−a)(−b) = ab. Proof. To prove (1), observe that a0 = a(0 + 0) = a0 + a0; hence, a0 = 0. Similarly, 0a = 0. For (2), we have ab + a(−b) = a(b − b) = a0 = 0; consequently, −ab = a(−b). Similarly, −ab = (−a)b. Part (3) follows directly from (2) since (−a)(−b) = −(a(−b)) = −(−ab) = ab. 184 CHAPTER 16. RINGS Just as we have subgroups of groups, we have an analogous class of substructures for rings. A subring S of a ring R is a subset S of R such that S is also a ring under the inherited operations from R. Example 16.9. The ring nZ is a subring of Z. Notice that even though the original ring may have an identity, we do not require that its subring have an identity. We have the following chain of subrings: Z ⊂ Q ⊂ R ⊂ C. The following proposition gives us some easy criteria for determining whether or not a subset of a ring is indeed a subring. (We will leave the proof of this proposition as an exercise.) Proposition 16.10. Let R be a ring and S a subset of R. Then S is a subring of R if and only if the following conditions are satisfied. 1. S ̸= ∅. 2. rs ∈ S for all r, s ∈ S. 3. r − s ∈ S for all r, s ∈ S. Example 16.11. Let R = M2 (R) be the ring of 2 × 2 matrices with entries in R. If T is the set of upper triangular matrices in R; i.e., {( ) } a b T = : a, b, c ∈ R , 0 c then T is a subring of R. If ( ) ( ′ ′) a b a b A= and B= 0 c 0 c′ are in T , then clearly A − B is also in T . Also, ( ′ ) aa ab′ + bc′ AB = 0 cc′ is in T . 16.2 Integral Domains and Fields Let us briefly recall some definitions. If R is a ring and r is a nonzero element in R, then r is said to be a zero divisor if there is some nonzero element s ∈ R such that rs = 0. A commutative ring with identity is said to be an integral domain if it has no zero divisors. If an element a in a ring R with identity has a multiplicative inverse, we say that a is a unit. If every nonzero element in a ring R is a unit, then R is called a division ring. A commutative division ring is called a field. Example 16.12. If i2 = −1, then the set Z[i] = {m + ni : m, n ∈ Z} forms a ring known as the Gaussian integers. It is easily seen that the Gaussian integers are a subring of the complex numbers since they are closed under addition and multiplication. Let α = a + bi be a unit in Z[i]. Then α = a − bi is also a unit since if αβ = 1, then αβ = 1. If β = c + di, then 1 = αβαβ = (a2 + b2 )(c2 + d2 ). Therefore, a2 + b2 must either be 1 or −1; or, equivalently, a + bi = ±1 or a + bi = ±i. Therefore, units of this ring are ±1 and ±i; hence, the Gaussian integers are not a field. We will leave it as an exercise to prove that the Gaussian integers are an integral domain. 16.2. INTEGRAL DOMAINS AND FIELDS 185 Example 16.13. The set of matrices {( ) ( ) ( ) ( )} 1 0 1 1 0 1 0 0 F = , , , 0 1 1 0 1 1 0 0 with entries in Z2 forms a field. √ √ Example 16.14.√ The√set Q( 2 ) = {a + b 2 : a, b ∈ Q} is a field. The inverse of an element a + b 2 in Q( 2 ) is a −b √ + 2 2. a2 − 2b2 a − 2b2 We have the following alternative characterization of integral domains. Proposition 16.15 Cancellation Law. Let D be a commutative ring with identity. Then D is an integral domain if and only if for all nonzero elements a ∈ D with ab = ac, we have b = c. Proof. Let D be an integral domain. Then D has no zero divisors. Let ab = ac with a ̸= 0. Then a(b − c) = 0. Hence, b − c = 0 and b = c. Conversely, let us suppose that cancellation is possible in D. That is, suppose that ab = ac implies b = c. Let ab = 0. If a ̸= 0, then ab = a0 or b = 0. Therefore, a cannot be a zero divisor. The following surprising theorem is due to Wedderburn. Theorem 16.16. Every finite integral domain is a field. Proof. Let D be a finite integral domain and D∗ be the set of nonzero elements of D. We must show that every element in D∗ has an inverse. For each a ∈ D∗ we can define a map λa : D∗ → D∗ by λa (d) = ad. This map makes sense, because if a ̸= 0 and d ̸= 0, then ad ̸= 0. The map λa is one-to-one, since for d1 , d2 ∈ D∗ , ad1 = λa (d1 ) = λa (d2 ) = ad2 implies d1 = d2 by left cancellation. Since D∗ is a finite set, the map λa must also be onto; hence, for some d ∈ D∗ , λa (d) = ad = 1. Therefore, a has a left inverse. Since D is commutative, d must also be a right inverse for a. Consequently, D is a field. For any nonnegative integer n and any element r in a ring R we write r + · · · + r (n times) as nr. We define the characteristic of a ring R to be the least positive integer n such that nr = 0 for all r ∈ R. If no such integer exists, then the characteristic of R is defined to be 0. We will denote the characteristic of R by char R. Example 16.17. For every prime p, Zp is a field of characteristic p. By Proposition 3.4, every nonzero element in Zp has an inverse; hence, Zp is a field. If a is any nonzero element in the field, then pa = 0, since the order of any nonzero element in the abelian group Zp is p. Lemma 16.18. Let R be a ring with identity. If 1 has order n, then the characteristic of R is n. Proof. If 1 has order n, then n is the least positive integer such that n1 = 0. Thus, for all r ∈ R, nr = n(1r) = (n1)r = 0r = 0. On the other hand, if no positive n exists such that n1 = 0, then the characteristic of R is zero. 186 CHAPTER 16. RINGS Theorem 16.19. The characteristic of an integral domain is either prime or zero. Proof. Let D be an integral domain and suppose that the characteristic of D is n with n ̸= 0. If n is not prime, then n = ab, where 1 < a < n and 1 < b < n. By Lemma 16.18, we need only consider the case n1 = 0. Since 0 = n1 = (ab)1 = (a1)(b1) and there are no zero divisors in D, either a1 = 0 or b1 = 0. Hence, the characteristic of D must be less than n, which is a contradiction. Therefore, n must be prime. 16.3 Ring Homomorphisms and Ideals In the study of groups, a homomorphism is a map that preserves the operation of the group. Similarly, a homomorphism between rings preserves the operations of addition and multi- plication in the ring. More specifically, if R and S are rings, then a ring homomorphism is a map ϕ : R → S satisfying ϕ(a + b) = ϕ(a) + ϕ(b) ϕ(ab) = ϕ(a)ϕ(b) for all a, b ∈ R. If ϕ : R → S is a one-to-one and onto homomorphism, then ϕ is called an isomorphism of rings. The set of elements that a ring homomorphism maps to 0 plays a fundamental role in the theory of rings. For any ring homomorphism ϕ : R → S, we define the kernel of a ring homomorphism to be the set ker ϕ = {r ∈ R : ϕ(r) = 0}. Example 16.20. For any integer n we can define a ring homomorphism ϕ : Z → Zn by a 7→ a (mod n). This is indeed a ring homomorphism, since ϕ(a + b) = (a + b) (mod n) = a (mod n) + b (mod n) = ϕ(a) + ϕ(b) and ϕ(ab) = ab (mod n) = a (mod n) · b (mod n) = ϕ(a)ϕ(b). The kernel of the homomorphism ϕ is nZ. Example 16.21. Let C[a, b] be the ring of continuous real-valued functions on an interval [a, b] as in Example 16.5. For a fixed α ∈ [a, b], we can define a ring homomorphism ϕα : C[a, b] → R by ϕα (f ) = f (α). This is a ring homomorphism since ϕα (f + g) = (f + g)(α) = f (α) + g(α) = ϕα (f ) + ϕα (g) ϕα (f g) = (f g)(α) = f (α)g(α) = ϕα (f )ϕα (g). Ring homomorphisms of the type ϕα are called evaluation homomorphisms. In the next proposition we will examine some fundamental properties of ring homomor- phisms. The proof of the proposition is left as an exercise. 16.3. RING HOMOMORPHISMS AND IDEALS 187 Proposition 16.22. Let ϕ : R → S be a ring homomorphism. 1. If R is a commutative ring, then ϕ(R) is a commutative ring. 2. ϕ(0) = 0. 3. Let 1R and 1S be the identities for R and S, respectively. If ϕ is onto, then ϕ(1R ) = 1S . 4. If R is a field and ϕ(R) ̸= {0}, then ϕ(R) is a field. In group theory we found that normal subgroups play a special role. These subgroups have nice characteristics that make them more interesting to study than arbitrary subgroups. In ring theory the objects corresponding to normal subgroups are a special class of subrings called ideals. An ideal in a ring R is a subring I of R such that if a is in I and r is in R, then both ar and ra are in I; that is, rI ⊂ I and Ir ⊂ I for all r ∈ R. Example 16.23. Every ring R has at least two ideals, {0} and R. These ideals are called the trivial ideals. Let R be a ring with identity and suppose that I is an ideal in R such that 1 is in I. Since for any r ∈ R, r1 = r ∈ I by the definition of an ideal, I = R. Example 16.24. If a is any element in a commutative ring R with identity, then the set ⟨a⟩ = {ar : r ∈ R} is an ideal in R. Certainly, ⟨a⟩ is nonempty since both 0 = a0 and a = a1 are in ⟨a⟩. The sum of two elements in ⟨a⟩ is again in ⟨a⟩ since ar + ar′ = a(r + r′ ). The inverse of ar is −ar = a(−r) ∈ ⟨a⟩. Finally, if we multiply an element ar ∈ ⟨a⟩ by an arbitrary element s ∈ R, we have s(ar) = a(sr). Therefore, ⟨a⟩ satisfies the definition of an ideal. If R is a commutative ring with identity, then an ideal of the form ⟨a⟩ = {ar : r ∈ R} is called a principal ideal. Theorem 16.25. Every ideal in the ring of integers Z is a principal ideal. Proof. The zero ideal {0} is a principal ideal since ⟨0⟩ = {0}. If I is any nonzero ideal in Z, then I must contain some positive integer m. There exists a least positive integer n in I by the Principle of Well-Ordering. Now let a be any element in I. Using the division algorithm, we know that there exist integers q and r such that a = nq + r where 0 ≤ r < n. This equation tells us that r = a − nq ∈ I, but r must be 0 since n is the least positive element in I. Therefore, a = nq and I = ⟨n⟩. Example 16.26. The set nZ is ideal in the ring of integers. If na is in nZ and b is in Z, then nab is in nZ as required. In fact, by Theorem 16.25, these are the only ideals of Z. Proposition 16.27. The kernel of any ring homomorphism ϕ : R → S is an ideal in R. Proof. We know from group theory that ker ϕ is an additive subgroup of R. Suppose that r ∈ R and a ∈ ker ϕ. Then we must show that ar and ra are in ker ϕ. However, ϕ(ar) = ϕ(a)ϕ(r) = 0ϕ(r) = 0 and ϕ(ra) = ϕ(r)ϕ(a) = ϕ(r)0 = 0. 188 CHAPTER 16. RINGS Remark 16.28. In our definition of an ideal we have required that rI ⊂ I and Ir ⊂ I for all r ∈ R. Such ideals are sometimes referred to as two-sided ideals. We can also consider one-sided ideals; that is, we may require only that either rI ⊂ I or Ir ⊂ I for r ∈ R hold but not both. Such ideals are called left ideals and right ideals, respectively. Of course, in a commutative ring any ideal must be two-sided. In this text we will concentrate on two-sided ideals. Theorem 16.29. Let I be an ideal of R. The factor group R/I is a ring with multiplication defined by (r + I)(s + I) = rs + I. Proof. We already know that R/I is an abelian group under addition. Let r + I and s + I be in R/I. We must show that the product (r + I)(s + I) = rs + I is independent of the choice of coset; that is, if r′ ∈ r + I and s′ ∈ s + I, then r′ s′ must be in rs + I. Since r′ ∈ r + I, there exists an element a in I such that r′ = r + a. Similarly, there exists a b ∈ I such that s′ = s + b. Notice that r′ s′ = (r + a)(s + b) = rs + as + rb + ab and as + rb + ab ∈ I since I is an ideal; consequently, r′ s′ ∈ rs + I. We will leave as an exercise the verification of the associative law for multiplication and the distributive laws. The ring R/I in Theorem 16.29 is called the factor or quotient ring. Just as with group homomorphisms and normal subgroups, there is a relationship between ring homo- morphisms and ideals. Theorem 16.30. Let I be an ideal of R. The map ϕ : R → R/I defined by ϕ(r) = r + I is a ring homomorphism of R onto R/I with kernel I. Proof. Certainly ϕ : R → R/I is a surjective abelian group homomorphism. It remains to show that ϕ works correctly under ring multiplication. Let r and s be in R. Then ϕ(r)ϕ(s) = (r + I)(s + I) = rs + I = ϕ(rs), which completes the proof of the theorem. The map ϕ : R → R/I is often called the natural or canonical homomorphism. In ring theory we have isomorphism theorems relating ideals and ring homomorphisms similar to the isomorphism theorems for groups that relate normal subgroups and homomorphisms in Chapter 11. We will prove only the First Isomorphism Theorem for rings in this chapter and leave the proofs of the other two theorems as exercises. All of the proofs are similar to the proofs of the isomorphism theorems for groups. Theorem 16.31 First Isomorphism Theorem. Let ψ : R → S be a ring homomorphism. Then ker ψ is an ideal of R. If ϕ : R → R/ ker ψ is the canonical homomorphism, then there exists a unique isomorphism η : R/ ker ψ → ψ(R) such that ψ = ηϕ. Proof. Let K = ker ψ. By the First Isomorphism Theorem for groups, there exists a well-defined group homomorphism η : R/K → ψ(R) defined by η(r + K) = ψ(r) for the additive abelian groups R and R/K. To show that this is a ring homomorphism, we need only show that η((r + K)(s + K)) = η(r + K)η(s + K); but η((r + K)(s + K)) = η(rs + K) = ψ(rs) = ψ(r)ψ(s) = η(r + K)η(s + K). 16.4. MAXIMAL AND PRIME IDEALS 189 Theorem 16.32 Second Isomorphism Theorem. Let I be a subring of a ring R and J an ideal of R. Then I ∩ J is an ideal of I and I/I ∩ J ∼ = (I + J)/J. Theorem 16.33 Third Isomorphism Theorem. Let R be a ring and I and J be ideals of R where J ⊂ I. Then R/J R/I ∼ = . I/J Theorem 16.34 Correspondence Theorem. Let I be an ideal of a ring R. Then S 7→ S/I is a one-to-one correspondence between the set of subrings S containing I and the set of subrings of R/I. Furthermore, the ideals of R containing I correspond to ideals of R/I. 16.4 Maximal and Prime Ideals In this particular section we are especially interested in certain ideals of commutative rings. These ideals give us special types of factor rings. More specifically, we would like to char- acterize those ideals I of a commutative ring R such that R/I is an integral domain or a field. A proper ideal M of a ring R is a maximal ideal of R if the ideal M is not a proper subset of any ideal of R except R itself. That is, M is a maximal ideal if for any ideal I properly containing M , I = R. The following theorem completely characterizes maximal ideals for commutative rings with identity in terms of their corresponding factor rings. Theorem 16.35. Let R be a commutative ring with identity and M an ideal in R. Then M is a maximal ideal of R if and only if R/M is a field. Proof. Let M be a maximal ideal in R. If R is a commutative ring, then R/M must also be a commutative ring. Clearly, 1 + M acts as an identity for R/M . We must also show that every nonzero element in R/M has an inverse. If a + M is a nonzero element in R/M , then a ∈ / M . Define I to be the set {ra + m : r ∈ R and m ∈ M }. We will show that I is an ideal in R. The set I is nonempty since 0a + 0 = 0 is in I. If r1 a + m1 and r2 a + m2 are two elements in I, then (r1 a + m1 ) − (r2 a + m2 ) = (r1 − r2 )a + (m1 − m2 ) is in I. Also, for any r ∈ R it is true that rI ⊂ I; hence, I is closed under multiplication and satisfies the necessary conditions to be an ideal. Therefore, by Proposition 16.10 and the definition of an ideal, I is an ideal properly containing M . Since M is a maximal ideal, I = R; consequently, by the definition of I there must be an m in M and an element b in R such that 1 = ab + m. Therefore, 1 + M = ab + M = ba + M = (a + M )(b + M ). Conversely, suppose that M is an ideal and R/M is a field. Since R/M is a field, it must contain at least two elements: 0 + M = M and 1 + M . Hence, M is a proper ideal of R. Let I be any ideal properly containing M . We need to show that I = R. Choose a in I but not in M . Since a + M is a nonzero element in a field, there exists an element b + M in R/M such that (a + M )(b + M ) = ab + M = 1 + M . Consequently, there exists an element m ∈ M such that ab + m = 1 and 1 is in I. Therefore, r1 = r ∈ I for all r ∈ R. Consequently, I = R. 190 CHAPTER 16. RINGS Example 16.36. Let pZ be an ideal in Z, where p is prime. Then pZ is a maximal ideal since Z/pZ ∼ = Zp is a field. A proper ideal P in a commutative ring R is called a prime ideal if whenever ab ∈ P , then either a ∈ P or b ∈ P .1 Example 16.37. It is easy to check that the set P = {0, 2, 4, 6, 8, 10} is an ideal in Z12 . This ideal is prime. In fact, it is a maximal ideal. Proposition 16.38. Let R be a commutative ring with identity 1, where 1 ̸= 0. Then P is a prime ideal in R if and only if R/P is an integral domain. Proof. First let us assume that P is an ideal in R and R/P is an integral domain. Suppose that ab ∈ P . If a+P and b+P are two elements of R/P such that (a+P )(b+P ) = 0+P = P , then either a + P = P or b + P = P . This means that either a is in P or b is in P , which shows that P must be prime. Conversely, suppose that P is prime and (a + P )(b + P ) = ab + P = 0 + P = P. Then ab ∈ P . If a ∈ / P , then b must be in P by the definition of a prime ideal; hence, b + P = 0 + P and R/P is an integral domain. Example 16.39. Every ideal in Z is of the form nZ. The factor ring Z/nZ ∼ = Zn is an integral domain only when n is prime. It is actually a field. Hence, the nonzero prime ideals in Z are the ideals pZ, where p is prime. This example really justifies the use of the word “prime” in our definition of prime ideals. Since every field is an integral domain, we have the following corollary. Corollary 16.40. Every maximal ideal in a commutative ring with identity is also a prime ideal. Historical Note Amalie Emmy Noether, one of the outstanding mathematicians of the twentieth century, was born in Erlangen, Germany in 1882. She was the daughter of Max Noether (1844– 1921), a distinguished mathematician at the University of Erlangen. Together with Paul Gordon (1837–1912), Emmy Noether’s father strongly influenced her early education. She entered the University of Erlangen at the age of 18. Although women had been admitted to universities in England, France, and Italy for decades, there was great resistance to their presence at universities in Germany. Noether was one of only two women among the university’s 986 students. After completing her doctorate under Gordon in 1907, she continued to do research at Erlangen, occasionally lecturing when her father was ill. Noether went to Göttingen to study in 1916. David Hilbert and Felix Klein tried un- successfully to secure her an appointment at Göttingen. Some of the faculty objected to women lecturers, saying, “What will our soldiers think when they return to the university and are expected to learn at the feet of a woman?” Hilbert, annoyed at the question, re- sponded, “Meine Herren, I do not see that the sex of a candidate is an argument against her admission as a Privatdozent. After all, the Senate is not a bathhouse.” At the end of World War I, attitudes changed and conditions greatly improved for women. After Noether 1 It is possible to define prime ideals in a noncommutative ring. See [1] or [3]. 16.5. AN APPLICATION TO SOFTWARE DESIGN 191 passed her habilitation examination in 1919, she was given a title and was paid a small sum for her lectures. In 1922, Noether became a Privatdozent at Göttingen. Over the next 11 years she used axiomatic methods to develop an abstract theory of rings and ideals. Though she was not good at lecturing, Noether was an inspiring teacher. One of her many students was B. L. van der Waerden, author of the first text treating abstract algebra from a modern point of view. Some of the other mathematicians Noether influenced or closely worked with were Alexandroff, Artin, Brauer, Courant, Hasse, Hopf, Pontryagin, von Neumann, and Weyl. One of the high points of her career was an invitation to address the International Congress of Mathematicians in Zurich in 1932. In spite of all the recognition she received from her colleagues, Noether’s abilities were never recognized as they should have been during her lifetime. She was never promoted to full professor by the Prussian academic bureaucracy. In 1933, Noether, a Jew, was banned from participation in all academic activities in Germany. She emigrated to the United States, took a position at Bryn Mawr College, and became a member of the Institute for Advanced Study at Princeton. Noether died suddenly on April 14, 1935. After her death she was eulogized by such notable scientists as Albert Einstein. 16.5 An Application to Software Design The Chinese Remainder Theorem is a result from elementary number theory about the solution of systems of simultaneous congruences. The Chinese mathematician Sun-tsï wrote about the theorem in the first century A.D. This theorem has some interesting consequences in the design of software for parallel processors. Lemma 16.41. Let m and n be positive integers such that gcd(m, n) = 1. Then for a, b ∈ Z the system x ≡ a (mod m) x ≡ b (mod n) has a solution. If x1 and x2 are two solutions of the system, then x1 ≡ x2 (mod mn). Proof. The equation x ≡ a (mod m) has a solution since a + km satisfies the equation for all k ∈ Z. We must show that there exists an integer k1 such that a + k1 m ≡ b (mod n). This is equivalent to showing that k1 m ≡ (b − a) (mod n) has a solution for k1 . Since m and n are relatively prime, there exist integers s and t such that ms + nt = 1. Consequently, (b − a)ms = (b − a) − (b − a)nt, or [(b − a)s]m ≡ (b − a) (mod n). Now let k1 = (b − a)s. To show that any two solutions are congruent modulo mn, let c1 and c2 be two solutions of the system. That is, ci ≡ a (mod m) 192 CHAPTER 16. RINGS ci ≡ b (mod n) for i = 1, 2. Then c2 ≡ c1 (mod m) c2 ≡ c1 (mod n). Therefore, both m and n divide c1 − c2 . Consequently, c2 ≡ c1 (mod mn). Example 16.42. Let us solve the system x ≡ 3 (mod 4) x ≡ 4 (mod 5). Using the Euclidean algorithm, we can find integers s and t such that 4s + 5t = 1. Two such integers are s = 4 and t = −3. Consequently, x = a + k1 m = 3 + 4k1 = 3 + 4[(5 − 4)4] = 19. Theorem 16.43 Chinese Remainder Theorem. Let n1 , n2 , . . . , nk be positive integers such that gcd(ni , nj ) = 1 for i ̸= j. Then for any integers a1 , . . . , ak , the system x ≡ a1 (mod n1 ) x ≡ a2 (mod n2 ) .. . x ≡ ak (mod nk ) has a solution. Furthermore, any two solutions of the system are congruent modulo n1 n2 · · · nk . Proof. We will use mathematical induction on the number of equations in the system. If there are k = 2 equations, then the theorem is true by Lemma 16.41. Now suppose that the result is true for a system of k equations or less and that we wish to find a solution of x ≡ a1 (mod n1 ) x ≡ a2 (mod n2 ) .. . x ≡ ak+1 (mod nk+1 ). Considering the first k equations, there exists a solution that is unique modulo n1 · · · nk , say a. Since n1 · · · nk and nk+1 are relatively prime, the system x≡a (mod n1 · · · nk ) x ≡ ak+1 (mod nk+1 ) has a solution that is unique modulo n1 . . . nk+1 by the lemma. Example 16.44. Let us solve the system x ≡ 3 (mod 4) x ≡ 4 (mod 5) x ≡ 1 (mod 9) 16.5. AN APPLICATION TO SOFTWARE DESIGN 193 x ≡ 5 (mod 7). From Example 16.42 we know that 19 is a solution of the first two congruences and any other solution of the system is congruent to 19 (mod 20). Hence, we can reduce the system to a system of three congruences: x ≡ 19 (mod 20) x≡1 (mod 9) x≡5 (mod 7). Solving the next two equations, we can reduce the system to x ≡ 19 (mod 180) x ≡ 5 (mod 7). Solving this last system, we find that 19 is a solution for the system that is unique up to modulo 1260. One interesting application of the Chinese Remainder Theorem in the design of computer software is that the theorem allows us to break up a calculation involving large integers into several less formidable calculations. A computer will handle integer calculations only up to a certain size due to the size of its processor chip, which is usually a 32 or 64-bit processor chip. For example, the largest integer available on a computer with a 64-bit processor chip is 263 − 1 = 9,223,372,036,854,775,807. Larger processors such as 128 or 256-bit have been proposed or are under development. There is even talk of a 512-bit processor chip. The largest integer that such a chip could store with be 2511 − 1, which would be a 154 digit number. However, we would need to deal with much larger numbers to break sophisticated encryption schemes. Special software is required for calculations involving larger integers which cannot be added directly by the machine. By using the Chinese Remainder Theorem we can break down large integer additions and multiplications into calculations that the computer can handle directly. This is especially useful on parallel processing computers which have the ability to run several programs concurrently. Most computers have a single central processing unit (CPU) containing one processor chip and can only add two numbers at a time. To add a list of ten numbers, the CPU must do nine additions in sequence. However, a parallel processing computer has more than one CPU. A computer with 10 CPUs, for example, can perform 10 different additions at the same time. If we can take a large integer and break it down into parts, sending each part to a different CPU, then by performing several additions or multiplications simultaneously on those parts, we can work with an integer that the computer would not be able to handle as a whole. Example 16.45. Suppose that we wish to multiply 2134 by 1531. We will use the integers 95, 97, 98, and 99 because they are relatively prime. We can break down each integer into four parts: 2134 ≡ 44 (mod 95) 2134 ≡ 0 (mod 97) 2134 ≡ 76 (mod 98) 2134 ≡ 55 (mod 99) 194 CHAPTER 16. RINGS and 1531 ≡ 11 (mod 95) 1531 ≡ 76 (mod 97) 1531 ≡ 61 (mod 98) 1531 ≡ 46 (mod 99). Multiplying the corresponding equations, we obtain 2134 · 1531 ≡ 44 · 11 ≡ 9 (mod 95) 2134 · 1531 ≡ 0 · 76 ≡ 0 (mod 97) 2134 · 1531 ≡ 76 · 61 ≡ 30 (mod 98) 2134 · 1531 ≡ 55 · 46 ≡ 55 (mod 99). Each of these four computations can be sent to a different processor if our computer has several CPUs. By the above calculation, we know that 2134·1531 is a solution of the system x ≡ 9 (mod 95) x ≡ 0 (mod 97) x ≡ 30 (mod 98) x ≡ 55 (mod 99). The Chinese Remainder Theorem tells us that solutions are unique up to modulo 95 · 97 · 98 · 99 = 89,403,930. Solving this system of congruences for x tells us that 2134 · 1531 = 3,267,154. The conversion of the computation into the four subcomputations will take some com- puting time. In addition, solving the system of congruences can also take considerable time. However, if we have many computations to be performed on a particular set of numbers, it makes sense to transform the problem as we have done above and to perform the necessary calculations simultaneously. Sage Rings are at the heart of Sage’s design, so you will find a wide range of possibilities for computing with rings and fields. Ideals, quotients, and homomorphisms are all available. 16.6 Exercises 1. Which of the following sets are rings with respect to the usual operations of addition and multiplication? If the set is a ring, is it also a field? (a) 7Z (b) Z18 √ √ (c) Q( 2 ) = {a + b 2 : a, b ∈ Q} √ √ √ √ √ (d) Q( 2, 3 ) = {a + b 2 + c 3 + d 6 : a, b, c, d ∈ Q} √ √ (e) Z[ 3 ] = {a + b 3 : a, b ∈ Z} √ (f) R = {a + b 3 3 : a, b ∈ Q} (g) Z[i] = {a + bi : a, b ∈ Z and i2 = −1} 16.6. EXERCISES 195 √ √ √ (h) Q( 3 3 ) = {a + b 3 3 + c 3 9 : a, b, c ∈ Q} 2. Let R be the ring of 2 × 2 matrices of the form ( ) a b , 0 0 where a, b ∈ R. Show that although R is a ring that has no identity, we can find a subring S of R with an identity. 3. List or characterize all of the units in each of the following rings. (a) Z10 (b) Z12 (c) Z7 (d) M2 (Z), the 2 × 2 matrices with entries in Z (e) M2 (Z2 ), the 2 × 2 matrices with entries in Z2 4. Find all of the ideals in each of the following rings. Which of these ideals are maximal and which are prime? (a) Z18 (b) Z25 (c) M2 (R), the 2 × 2 matrices with entries in R (d) M2 (Z), the 2 × 2 matrices with entries in Z (e) Q 5. For each of the following rings R with ideal I, give an addition table and a multipli- cation table for R/I. (a) R = Z and I = 6Z (b) R = Z12 and I = {0, 3, 6, 9} 6. Find all homomorphisms ϕ : Z/6Z → Z/15Z. 7. Prove that R is not isomorphic to C. √ √ 8. √ Prove or disprove: √ The ring Q( 2 ) = {a + b 2 : a, b ∈ Q} is isomorphic to the ring Q( 3 ) = {a + b 3 : a, b ∈ Q}. 9. What is the characteristic of the field formed by the set of matrices {( ) ( ) ( ) ( )} 1 0 1 1 0 1 0 0 F = , , , 0 1 1 0 1 1 0 0 with entries in Z2 ? 10. Define a map ϕ : C → M2 (R) by ( ) a b ϕ(a + bi) = . −b a Show that ϕ is an isomorphism of C with its image in M2 (R). 11. Prove that the Gaussian integers, Z[i], are an integral domain. √ √ 12. Prove that Z[ 3 i] = {a + b 3 i : a, b ∈ Z} is an integral domain. 13. Solve each of the following systems of congruences. 196 CHAPTER 16. RINGS (a) x ≡ 4 (mod 7) x≡2 (mod 5) x ≡ 7 (mod 9) x≡6 (mod 11) x ≡ 5 (mod 11) (b) x≡3 (mod 7) (d) x≡0 (mod 8) x≡5 (mod 15) x ≡ 3 (mod 5) x ≡ 0 (mod 8) (c) x ≡ 1 (mod 11) x≡2 (mod 4) x ≡ 5 (mod 13) 14. Use the method of parallel computation outlined in the text to calculate 2234 + 4121 by dividing the calculation into four separate additions modulo 95, 97, 98, and 99. 15. Explain why the method of parallel computation outlined in the text fails for 2134 · 1531 if we attempt to break the calculation down into two smaller calculations modulo 98 and 99. 16. If R is a field, show that the only two ideals of R are {0} and R itself. 17. Let a be any element in a ring R with identity. Show that (−1)a = −a. 18. Let ϕ : R → S be a ring homomorphism. Prove each of the following statements. (a) If R is a commutative ring, then ϕ(R) is a commutative ring. (b) ϕ(0) = 0. (c) Let 1R and 1S be the identities for R and S, respectively. If ϕ is onto, then ϕ(1R ) = 1S . (d) If R is a field and ϕ(R) ̸= 0, then ϕ(R) is a field. 19. Prove that the associative law for multiplication and the distributive laws hold in R/I. 20. Prove the Second Isomorphism Theorem for rings: Let I be a subring of a ring R and J an ideal in R. Then I ∩ J is an ideal in I and I/I ∩ J ∼ = I + J/J. 21. Prove the Third Isomorphism Theorem for rings: Let R be a ring and I and J be ideals of R, where J ⊂ I. Then R/J R/I ∼ = . I/J 22. Prove the Correspondence Theorem: Let I be an ideal of a ring R. Then S → S/I is a one-to-one correspondence between the set of subrings S containing I and the set of subrings of R/I. Furthermore, the ideals of R correspond to ideals of R/I. 23. Let R be a ring and S a subset of R. Show that S is a subring of R if and only if each of the following conditions is satisfied. (a) S ̸= ∅. (b) rs ∈ S for all r, s ∈ S. 16.6. EXERCISES 197 (c) r − s ∈ S for all r, s ∈ S. ∩ 24. Let R be a ring with a collection of subrings {Rα }. Prove that Rα is a subring of R. Give an example to show that the union of two subrings is not necessarily a subring. ∩ 25. Let {Iα }α∈A be a collection of ideals in a ring R. Prove that α∈A Iα is also an ideal in R. Give an example to show that if I1 and I2 are ideals in R, then I1 ∪ I2 may not be an ideal. 26. Let R be an integral domain. Show that if the only ideals in R are {0} and R itself, R must be a field. 27. Let R be a commutative ring. An element a in R is nilpotent if an = 0 for some positive integer n. Show that the set of all nilpotent elements forms an ideal in R. 28. A ring R is a Boolean ring if for every a ∈ R, a2 = a. Show that every Boolean ring is a commutative ring. 29. Let R be a ring, where a3 = a for all a ∈ R. Prove that R must be a commutative ring. 30. Let R be a ring with identity 1R and S a subring of R with identity 1S . Prove or disprove that 1R = 1S . 31. If we do not require the identity of a ring to be distinct from 0, we will not have a very interesting mathematical structure. Let R be a ring such that 1 = 0. Prove that R = {0}. 32. Let S be a nonempty subset of a ring R. Prove that there is a subring R′ of R that contains S. 33. Let R be a ring. Define the center of R to be Z(R) = {a ∈ R : ar = ra for all r ∈ R}. Prove that Z(R) is a commutative subring of R. 34. Let p be prime. Prove that Z(p) = {a/b : a, b ∈ Z and gcd(b, p) = 1} is a ring. The ring Z(p) is called the ring of integers localized at p. 35. Prove or disprove: Every finite integral domain is isomorphic to Zp . 36. Let R be a ring with identity. (a) Let u be a unit in R. Define a map iu : R → R by r 7→ uru−1 . Prove that iu is an automorphism of R. Such an automorphism of R is called an inner automorphism of R. Denote the set of all inner automorphisms of R by Inn(R). (b) Denote the set of all automorphisms of R by Aut(R). Prove that Inn(R) is a normal subgroup of Aut(R). (c) Let U (R) be the group of units in R. Prove that the map ϕ : U (R) → Inn(R) defined by u 7→ iu is a homomorphism. Determine the kernel of ϕ. (d) Compute Aut(Z), Inn(Z), and U (Z). 37. Let R and S be arbitrary rings. Show that their Cartesian product is a ring if we define addition and multiplication in R × S by 198 CHAPTER 16. RINGS (a) (r, s) + (r′ , s′ ) = (r + r′ , s + s′ ) (b) (r, s)(r′ , s′ ) = (rr′ , ss′ ) 38. An element x in a ring is called an idempotent if x2 = x. Prove that the only idempotents in an integral domain are 0 and 1. Find a ring with a idempotent x not equal to 0 or 1. 39. Let gcd(a, n) = d and gcd(b, d) ̸= 1. Prove that ax ≡ b (mod n) does not have a solution. 40. The Chinese Remainder Theorem for Rings. Let R be a ring and I and J be ideals in R such that I + J = R. (a) Show that for any r and s in R, the system of equations x≡r (mod I) x ≡ s (mod J) has a solution. (b) In addition, prove that any two solutions of the system are congruent modulo I ∩ J. (c) Let I and J be ideals in a ring R such that I + J = R. Show that there exists a ring isomorphism R/(I ∩ J) ∼ = R/I × R/J. 16.7 Programming Exercise 1. Write a computer program implementing fast addition and multiplication using the Chinese Remainder Theorem and the method outlined in the text. References and Suggested Readings [1] Anderson, F. W. and Fuller, K. R. Rings and Categories of Modules. 2nd ed. Springer, New York, 1992. [2] Atiyah, M. F. and MacDonald, I. G. Introduction to Commutative Algebra. Westview Press, Boulder, CO, 1994. [3] Herstein, I. N. Noncommutative Rings. Mathematical Association of America, Wash- ington, DC, 1994. [4] Kaplansky, I. Commutative Rings. Revised edition. University of Chicago Press, Chicago, 1974. [5] Knuth, D. E. The Art of Computer Programming: Semi-Numerical Algorithms, vol. 2. 3rd ed. Addison-Wesley Professional, Boston, 1997. [6] Lidl, R. and Pilz, G. Applied Abstract Algebra. 2nd ed. Springer, New York, 1998. A good source for applications. [7] Mackiw, G. Applications of Abstract Algebra. Wiley, New York, 1985. 16.7. PROGRAMMING EXERCISE 199 [8] McCoy, N. H. Rings and Ideals. Carus Monograph Series, No. 8. Mathematical Association of America, Washington, DC, 1968. [9] McCoy, N. H. The Theory of Rings. Chelsea, New York, 1972. [10] Zariski, O. and Samuel, P. Commutative Algebra, vols. I and II. Springer, New York, 1975, 1960. 17 Polynomials Most people are fairly familiar with polynomials by the time they begin to study abstract algebra. When we examine polynomial expressions such as p(x) = x3 − 3x + 2 q(x) = 3x2 − 6x + 5, we have a pretty good idea of what p(x) + q(x) and p(x)q(x) mean. We just add and multiply polynomials as functions; that is, (p + q)(x) = p(x) + q(x) = (x3 − 3x + 2) + (3x2 − 6x + 5) = x3 + 3x2 − 9x + 7 and (pq)(x) = p(x)q(x) = (x3 − 3x + 2)(3x2 − 6x + 5) = 3x5 − 6x4 − 4x3 + 24x2 − 27x + 10. It is probably no surprise that polynomials form a ring. In this chapter we shall emphasize the algebraic structure of polynomials by studying polynomial rings. We can prove many results for polynomial rings that are similar to the theorems we proved for the integers. Analogs of prime numbers, the division algorithm, and the Euclidean algorithm exist for polynomials. 17.1 Polynomial Rings Throughout this chapter we shall assume that R is a commutative ring with identity. Any expression of the form ∑ n f (x) = ai xi = a0 + a1 x + a2 x2 + · · · + an xn , i=0 where ai ∈ R and an ̸= 0, is called a polynomial over R with indeterminate x. The elements a0 , a1 , . . . , an are called the coefficients of f . The coefficient an is called the leading coefficient. A polynomial is called monic if the leading coefficient is 1. If n is the largest nonnegative number for which an ̸= 0, we say that the degree of f is n and write deg f (x) = n. If no such n exists—that is, if f = 0 is the zero polynomial—then the degree 200 17.1. POLYNOMIAL RINGS 201 of f is defined to be −∞. We will denote the set of all polynomials with coefficients in a ring R by R[x]. Two polynomials are equal exactly when their corresponding coefficients are equal; that is, if we let p(x) = a0 + a1 x + · · · + an xn q(x) = b0 + b1 x + · · · + bm xm , then p(x) = q(x) if and only if ai = bi for all i ≥ 0. To show that the set of all polynomials forms a ring, we must first define addition and multiplication. We define the sum of two polynomials as follows. Let p(x) = a0 + a1 x + · · · + an xn q(x) = b0 + b1 x + · · · + bm xm . Then the sum of p(x) and q(x) is p(x) + q(x) = c0 + c1 x + · · · + ck xk , where ci = ai + bi for each i. We define the product of p(x) and q(x) to be p(x)q(x) = c0 + c1 x + · · · + cm+n xm+n , where ∑ i ci = ak bi−k = a0 bi + a1 bi−1 + · · · + ai−1 b1 + ai b0 k=0 for each i. Notice that in each case some of the coefficients may be zero. Example 17.1. Suppose that p(x) = 3 + 0x + 0x2 + 2x3 + 0x4 and q(x) = 2 + 0x − x2 + 0x3 + 4x4 are polynomials in Z[x]. If the coefficient of some term in a polynomial is zero, then we usually just omit that term. In this case we would write p(x) = 3 + 2x3 and q(x) = 2 − x2 + 4x4 . The sum of these two polynomials is p(x) + q(x) = 5 − x2 + 2x3 + 4x4 . The product, p(x)q(x) = (3 + 2x3 )(2 − x2 + 4x4 ) = 6 − 3x2 + 4x3 + 12x4 − 2x5 + 8x7 , can be calculated either by determining the ci s in the definition or by simply multiplying polynomials in the same way as we have always done. Example 17.2. Let p(x) = 3 + 3x3 and q(x) = 4 + 4x2 + 4x4 be polynomials in Z12 [x]. The sum of p(x) and q(x) is 7 + 4x2 + 3x3 + 4x4 . The product of the two polynomials is the zero polynomial. This example tells us that we can not expect R[x] to be an integral domain if R is not an integral domain. 202 CHAPTER 17. POLYNOMIALS Theorem 17.3. Let R be a commutative ring with identity. Then R[x] is a commutative ring with identity. Proof. Our first task is to show that R[x] is an abelian group under polynomial addi- tion. ∑n Thei zero polynomial, f (x) = 0, is the additive identity. ∑ Given a polynomial∑np(x) = n a i=0 i x , the inverse of p(x) is easily verified to be −p(x) = i=0 (−ai )x i =− i i=0 ai x . Commutativity and associativity follow immediately from the definition of polynomial ad- dition and from the fact that addition in R is both commutative and associative. To show that polynomial multiplication is associative, let ∑ m p(x) = ai xi , i=0 ∑ n q(x) = bi xi , i=0 ∑ p r(x) = ci xi . i=0 Then [( m )( )] ( ) ∑ ∑ n ∑ p [p(x)q(x)]r(x) = ai xi bi xi ci xi i=0 i=0 i=0 ( ) ∑ ∑ m+n i ∑ p = aj bi−j xi ci xi i=0 j=0 i=0 ( j ) ∑ ∑ m+n+p i ∑ = ak bj−k ci−j xi i=0 j=0 k=0 ∑ m+n+p ∑ = aj bk cl xi i=0 j+k+l=i ( i−j ) ∑ ∑ m+n+p i ∑ = aj bk ci−j−k xi i=0 j=0 k=0 (m ) n+p i ∑ ∑ ∑ = ai xi bj ci−j xi i=0 i=0 j=0 (m ) [( )( )] ∑ ∑ n ∑ p i i i = ai x bi x ci x i=0 i=0 i=0 = p(x)[q(x)r(x)] The commutativity and distribution properties of polynomial multiplication are proved in a similar manner. We shall leave the proofs of these properties as an exercise. Proposition 17.4. Let p(x) and q(x) be polynomials in R[x], where R is an integral domain. Then deg p(x) + deg q(x) = deg(p(x)q(x)). Furthermore, R[x] is an integral domain. Proof. Suppose that we have two nonzero polynomials p(x) = am xm + · · · + a1 x + a0 17.2. THE DIVISION ALGORITHM 203 and q(x) = bn xn + · · · + b1 x + b0 with am ̸= 0 and bn ̸= 0. The degrees of p(x) and q(x) are m and n, respectively. The leading term of p(x)q(x) is am bn xm+n , which cannot be zero since R is an integral domain; hence, the degree of p(x)q(x) is m + n, and p(x)q(x) ̸= 0. Since p(x) ̸= 0 and q(x) ̸= 0 imply that p(x)q(x) ̸= 0, we know that R[x] must also be an integral domain. We also want to consider polynomials in two or more variables, such as x2 − 3xy + 2y 3 . Let R be a ring and suppose that we are given two indeterminates x and y. Certainly we can form the ring (R[x])[y]. It is straightforward but perhaps tedious to show that (R[x])[y] ∼ = R([y])[x]. We shall identify these two rings by this isomorphism and simply write R[x, y]. The ring R[x, y] is called the ring of polynomials in two indeterminates x and y with coefficients in R. We can define the ring of polynomials in n indeterminates with coefficients in R similarly. We shall denote this ring by R[x1 , x2 , . . . , xn ]. Theorem 17.5. Let R be a commutative ring with identity and α ∈ R. Then we have a ring homomorphism ϕα : R[x] → R defined by ϕα (p(x)) = p(α) = an αn + · · · + a1 α + a0 , where p(x) = an xn + · · · + a1 x + a0 . ∑ ∑ Proof. Let p(x) = ni=0 ai xi and q(x) = m i i=0 bi x . It is easy to show that ϕα (p(x) + q(x)) = ϕα (p(x)) + ϕα (q(x)). To show that multiplication is preserved under the map ϕα , observe that ϕα (p(x))ϕα (q(x)) = p(α)q(α) ( n )( m ) ∑ ∑ = ai α i bi αi i=0 i=0 ( i ) ∑ ∑ m+n = ak bi−k αi i=0 k=0 = ϕα (p(x)q(x)). The map ϕα : R[x] → R is called the evaluation homomorphism at α. 17.2 The Division Algorithm Recall that the division algorithm for integers (Theorem 2.9) says that if a and b are integers with b > 0, then there exist unique integers q and r such that a = bq + r, where 0 ≤ r < b. The algorithm by which q and r are found is just long division. A similar theorem exists for polynomials. The division algorithm for polynomials has several important consequences. Since its proof is very similar to the corresponding proof for integers, it is worthwhile to review Theorem 2.9 at this point. Theorem 17.6 Division Algorithm. Let f (x) and g(x) be polynomials in F [x], where F is a field and g(x) is a nonzero polynomial. Then there exist unique polynomials q(x), r(x) ∈ F [x] such that f (x) = g(x)q(x) + r(x), where either deg r(x) < deg g(x) or r(x) is the zero polynomial. 204 CHAPTER 17. POLYNOMIALS Proof. We will first consider the existence of q(x) and r(x). If f (x) is the zero polynomial, then 0 = 0 · g(x) + 0; hence, both q and r must also be the zero polynomial. Now suppose that f (x) is not the zero polynomial and that deg f (x) = n and deg g(x) = m. If m > n, then we can let q(x) = 0 and r(x) = f (x). Hence, we may assume that m ≤ n and proceed by induction on n. If f (x) = an xn + an−1 xn−1 + · · · + a1 x + a0 g(x) = bm xm + bm−1 xm−1 + · · · + b1 x + b0 the polynomial an n−m f ′ (x) = f (x) − x g(x) bm has degree less than n or is the zero polynomial. By induction, there exist polynomials q ′ (x) and r(x) such that f ′ (x) = q ′ (x)g(x) + r(x), where r(x) = 0 or the degree of r(x) is less than the degree of g(x). Now let an n−m q(x) = q ′ (x) + x . bm Then f (x) = g(x)q(x) + r(x), with r(x) the zero polynomial or deg r(x) < deg g(x). To show that q(x) and r(x) are unique, suppose that there exist two other polynomials q1 (x) and r1 (x) such that f (x) = g(x)q1 (x) + r1 (x) with deg r1 (x) < deg g(x) or r1 (x) = 0, so that f (x) = g(x)q(x) + r(x) = g(x)q1 (x) + r1 (x), and g(x)[q(x) − q1 (x)] = r1 (x) − r(x). If q(x) − q1 (x) is not the zero polynomial, then deg(g(x)[q(x) − q1 (x)]) = deg(r1 (x) − r(x)) ≥ deg g(x). However, the degrees of both r(x) and r1 (x) are strictly less than the degree of g(x); therefore, r(x) = r1 (x) and q(x) = q1 (x). Example 17.7. The division algorithm merely formalizes long division of polynomials, a task we have been familiar with since high school. For example, suppose that we divide x3 − x2 + 2x − 3 by x − 2. x2 + x + 4 x − 2 x3 − x2 + 2x − 3 x3 − 2x2 x2 + 2x − 3 x2 − 2x 4x − 3 4x − 8 5 Hence, x3 − x2 + 2x − 3 = (x − 2)(x2 + x + 4) + 5. 17.2. THE DIVISION ALGORITHM 205 Let p(x) be a polynomial in F [x] and α ∈ F . We say that α is a zero or root of p(x) if p(x) is in the kernel of the evaluation homomorphism ϕα . All we are really saying here is that α is a zero of p(x) if p(α) = 0. Corollary 17.8. Let F be a field. An element α ∈ F is a zero of p(x) ∈ F [x] if and only if x − α is a factor of p(x) in F [x]. Proof. Suppose that α ∈ F and p(α) = 0. By the division algorithm, there exist polynomials q(x) and r(x) such that p(x) = (x − α)q(x) + r(x) and the degree of r(x) must be less than the degree of x − α. Since the degree of r(x) is less than 1, r(x) = a for a ∈ F ; therefore, p(x) = (x − α)q(x) + a. But 0 = p(α) = 0 · q(α) + a = a; consequently, p(x) = (x − α)q(x), and x − α is a factor of p(x). Conversely, suppose that x − α is a factor of p(x); say p(x) = (x − α)q(x). Then p(α) = 0 · q(α) = 0. Corollary 17.9. Let F be a field. A nonzero polynomial p(x) of degree n in F [x] can have at most n distinct zeros in F . Proof. We will use induction on the degree of p(x). If deg p(x) = 0, then p(x) is a constant polynomial and has no zeros. Let deg p(x) = 1. Then p(x) = ax + b for some a and b in F . If α1 and α2 are zeros of p(x), then aα1 + b = aα2 + b or α1 = α2 . Now assume that deg p(x) > 1. If p(x) does not have a zero in F , then we are done. On the other hand, if α is a zero of p(x), then p(x) = (x − α)q(x) for some q(x) ∈ F [x] by Corollary 17.8. The degree of q(x) is n − 1 by Proposition 17.4. Let β be some other zero of p(x) that is distinct from α. Then p(β) = (β − α)q(β) = 0. Since α ̸= β and F is a field, q(β) = 0. By our induction hypothesis, q(x) can have at most n − 1 zeros in F that are distinct from α. Therefore, p(x) has at most n distinct zeros in F . Let F be a field. A monic polynomial d(x) is a greatest common divisor of poly- nomials p(x), q(x) ∈ F [x] if d(x) evenly divides both p(x) and q(x); and, if for any other polynomial d′ (x) dividing both p(x) and q(x), d′ (x) | d(x). We write d(x) = gcd(p(x), q(x)). Two polynomials p(x) and q(x) are relatively prime if gcd(p(x), q(x)) = 1. Proposition 17.10. Let F be a field and suppose that d(x) is a greatest common divisor of two polynomials p(x) and q(x) in F [x]. Then there exist polynomials r(x) and s(x) such that d(x) = r(x)p(x) + s(x)q(x). Furthermore, the greatest common divisor of two polynomials is unique. Proof. Let d(x) be the monic polynomial of smallest degree in the set S = {f (x)p(x) + g(x)q(x) : f (x), g(x) ∈ F [x]}. We can write d(x) = r(x)p(x) + s(x)q(x) for two polynomials r(x) and s(x) in F [x]. We need to show that d(x) divides both p(x) and q(x). We shall first show that d(x) divides 206 CHAPTER 17. POLYNOMIALS p(x). By the division algorithm, there exist polynomials a(x) and b(x) such that p(x) = a(x)d(x) + b(x), where b(x) is either the zero polynomial or deg b(x) < deg d(x). Therefore, b(x) = p(x) − a(x)d(x) = p(x) − a(x)(r(x)p(x) + s(x)q(x)) = p(x) − a(x)r(x)p(x) − a(x)s(x)q(x) = p(x)(1 − a(x)r(x)) + q(x)(−a(x)s(x)) is a linear combination of p(x) and q(x) and therefore must be in S. However, b(x) must be the zero polynomial since d(x) was chosen to be of smallest degree; consequently, d(x) divides p(x). A symmetric argument shows that d(x) must also divide q(x); hence, d(x) is a common divisor of p(x) and q(x). To show that d(x) is a greatest common divisor of p(x) and q(x), suppose that d′ (x) is another common divisor of p(x) and q(x). We will show that d′ (x) | d(x). Since d′ (x) is a common divisor of p(x) and q(x), there exist polynomials u(x) and v(x) such that p(x) = u(x)d′ (x) and q(x) = v(x)d′ (x). Therefore, d(x) = r(x)p(x) + s(x)q(x) = r(x)u(x)d′ (x) + s(x)v(x)d′ (x) = d′ (x)[r(x)u(x) + s(x)v(x)]. Since d′ (x) | d(x), d(x) is a greatest common divisor of p(x) and q(x). Finally, we must show that the greatest common divisor of p(x) and q(x) is unique. Suppose that d′ (x) is another greatest common divisor of p(x) and q(x). We have just shown that there exist polynomials u(x) and v(x) in F [x] such that d(x) = d′ (x)[r(x)u(x) + s(x)v(x)]. Since deg d(x) = deg d′ (x) + deg[r(x)u(x) + s(x)v(x)] and d(x) and d′ (x) are both greatest common divisors, deg d(x) = deg d′ (x). Since d(x) and d′ (x) are both monic polynomials of the same degree, it must be the case that d(x) = d′ (x). Notice the similarity between the proof of Proposition 17.10 and the proof of Theo- rem 2.10. 17.3 Irreducible Polynomials A nonconstant polynomial f (x) ∈ F [x] is irreducible over a field F if f (x) cannot be expressed as a product of two polynomials g(x) and h(x) in F [x], where the degrees of g(x) and h(x) are both smaller than the degree of f (x). Irreducible polynomials function as the “prime numbers” of polynomial rings. Example 17.11. The polynomial x2 − 2 ∈ Q[x] is irreducible since it cannot be factored any further over the rational numbers. Similarly, x2 + 1 is irreducible over the real numbers. Example 17.12. The polynomial p(x) = x3 + x2 + 2 is irreducible over Z3 [x]. Suppose that this polynomial was reducible over Z3 [x]. By the division algorithm there would have to be a factor of the form x − a, where a is some element in Z3 [x]. Hence, it would have to be true that p(a) = 0. However, p(0) = 2 p(1) = 1 17.3. IRREDUCIBLE POLYNOMIALS 207 p(2) = 2. Therefore, p(x) has no zeros in Z3 and must be irreducible. Lemma 17.13. Let p(x) ∈ Q[x]. Then r p(x) = (a0 + a1 x + · · · + an xn ), s where r, s, a0 , . . . , an are integers, the ai ’s are relatively prime, and r and s are relatively prime. Proof. Suppose that b0 b1 bn p(x) = + x + · · · + xn , c0 c1 cn where the bi ’s and the ci ’s are integers. We can rewrite p(x) as 1 p(x) = (d0 + d1 x + · · · + dn xn ), c0 · · · cn where d0 , . . . , dn are integers. Let d be the greatest common divisor of d0 , . . . , dn . Then d p(x) = (a0 + a1 x + · · · + an xn ), c0 · · · cn where di = dai and the ai ’s are relatively prime. Reducing d/(c0 · · · cn ) to its lowest terms, we can write r p(x) = (a0 + a1 x + · · · + an xn ), s where gcd(r, s) = 1. Theorem 17.14 Gauss’s Lemma. Let p(x) ∈ Z[x] be a monic polynomial such that p(x) factors into a product of two polynomials α(x) and β(x) in Q[x], where the degrees of both α(x) and β(x) are less than the degree of p(x). Then p(x) = a(x)b(x), where a(x) and b(x) are monic polynomials in Z[x] with deg α(x) = deg a(x) and deg β(x) = deg b(x). Proof. By Lemma 17.13, we can assume that c1 c1 α(x) = (a0 + a1 x + · · · + am xm ) = α1 (x) d1 d1 c2 c2 β(x) = (b0 + b1 x + · · · + bn x ) = β1 (x), n d2 d2 where the ai ’s are relatively prime and the bi ’s are relatively prime. Consequently, c1 c2 c p(x) = α(x)β(x) = α1 (x)β1 (x) = α1 (x)β1 (x), d1 d2 d where c/d is the product of c1 /d1 and c2 /d2 expressed in lowest terms. Hence, dp(x) = cα1 (x)β1 (x). If d = 1, then cam bn = 1 since p(x) is a monic polynomial. Hence, either c = 1 or c = −1. If c = 1, then either am = bn = 1 or am = bn = −1. In the first case p(x) = α1 (x)β1 (x), where α1 (x) and β1 (x) are monic polynomials with deg α(x) = deg α1 (x) and deg β(x) = deg β1 (x). In the second case a(x) = −α1 (x) and b(x) = −β1 (x) are the correct monic polynomials since p(x) = (−α1 (x))(−β1 (x)) = a(x)b(x). The case in which c = −1 can be handled similarly. Now suppose that d ̸= 1. Since gcd(c, d) = 1, there exists a prime p such that p | d and p ∤ c. Also, since the coefficients of α1 (x) are relatively prime, there exists a coefficient ai 208 CHAPTER 17. POLYNOMIALS such that p ∤ ai . Similarly, there exists a coefficient bj of β1 (x) such that p ∤ bj . Let α1′ (x) and β1′ (x) be the polynomials in Zp [x] obtained by reducing the coefficients of α1 (x) and β1 (x) modulo p. Since p | d, α1′ (x)β1′ (x) = 0 in Zp [x]. However, this is impossible since neither α1′ (x) nor β1′ (x) is the zero polynomial and Zp [x] is an integral domain. Therefore, d = 1 and the theorem is proven. Corollary 17.15. Let p(x) = xn + an−1 xn−1 + · · · + a0 be a polynomial with coefficients in Z and a0 ̸= 0. If p(x) has a zero in Q, then p(x) also has a zero α in Z. Furthermore, α divides a0 . Proof. Let p(x) have a zero a ∈ Q. Then p(x) must have a linear factor x − a. By Gauss’s Lemma, p(x) has a factorization with a linear factor in Z[x]. Hence, for some α ∈ Z p(x) = (x − α)(xn−1 + · · · − a0 /α). Thus a0 /α ∈ Z and so α | a0 . Example 17.16. Let p(x) = x4 − 2x3 + x + 1. We shall show that p(x) is irreducible over Q[x]. Assume that p(x) is reducible. Then either p(x) has a linear factor, say p(x) = (x − α)q(x), where q(x) is a polynomial of degree three, or p(x) has two quadratic factors. If p(x) has a linear factor in Q[x], then it has a zero in Z. By Corollary 17.15, any zero must divide 1 and therefore must be ±1; however, p(1) = 1 and p(−1) = 3. Consequently, we have eliminated the possibility that p(x) has any linear factors. Therefore, if p(x) is reducible it must factor into two quadratic polynomials, say p(x) = (x2 + ax + b)(x2 + cx + d) = x4 + (a + c)x3 + (ac + b + d)x2 + (ad + bc)x + bd, where each factor is in Z[x] by Gauss’s Lemma. Hence, a + c = −2 ac + b + d = 0 ad + bc = 1 bd = 1. Since bd = 1, either b = d = 1 or b = d = −1. In either case b = d and so ad + bc = b(a + c) = 1. Since a + c = −2, we know that −2b = 1. This is impossible since b is an integer. Therefore, p(x) must be irreducible over Q. Theorem 17.17 Eisenstein’s Criterion. Let p be a prime and suppose that f (x) = an xn + · · · + a0 ∈ Z[x]. If p | ai for i = 0, 1, . . . , n − 1, but p ∤ an and p2 ∤ a0 , then f (x) is irreducible over Q. Proof. By Gauss’s Lemma, we need only show that f (x) does not factor into polynomials of lower degree in Z[x]. Let f (x) = (br xr + · · · + b0 )(cs xs + · · · + c0 ) be a factorization in Z[x], with br and cs not equal to zero and r, s < n. Since p2 does not divide a0 = b0 c0 , either b0 or c0 is not divisible by p. Suppose that p ∤ b0 and p | c0 . Since 17.3. IRREDUCIBLE POLYNOMIALS 209 p ∤ an and an = br cs , neither br nor cs is divisible by p. Let m be the smallest value of k such that p ∤ ck . Then am = b0 cm + b1 cm−1 + · · · + bm c0 is not divisible by p, since each term on the right-hand side of the equation is divisible by p except for b0 cm . Therefore, m = n since ai is divisible by p for m < n. Hence, f (x) cannot be factored into polynomials of lower degree and therefore must be irreducible. Example 17.18. The polynomial f (x) = 16x5 − 9x4 + 3x2 + 6x − 21 is easily seen to be irreducible over Q by Eisenstein’s Criterion if we let p = 3. Eisenstein’s Criterion is more useful in constructing irreducible polynomials of a certain degree over Q than in determining the irreducibility of an arbitrary polynomial in Q[x]: given an arbitrary polynomial, it is not very likely that we can apply Eisenstein’s Crite- rion. The real value of Theorem 17.17 is that we now have an easy method of generating irreducible polynomials of any degree. Ideals in F [x] Let F be a field. Recall that a principal ideal in F [x] is an ideal ⟨p(x)⟩ generated by some polynomial p(x); that is, ⟨p(x)⟩ = {p(x)q(x) : q(x) ∈ F [x]}. Example 17.19. The polynomial x2 in F [x] generates the ideal ⟨x2 ⟩ consisting of all polynomials with no constant term or term of degree 1. Theorem 17.20. If F is a field, then every ideal in F [x] is a principal ideal. Proof. Let I be an ideal of F [x]. If I is the zero ideal, the theorem is easily true. Suppose that I is a nontrivial ideal in F [x], and let p(x) ∈ I be a nonzero element of minimal degree. If deg p(x) = 0, then p(x) is a nonzero constant and 1 must be in I. Since 1 generates all of F [x], ⟨1⟩ = I = F [x] and I is again a principal ideal. Now assume that deg p(x) ≥ 1 and let f (x) be any element in I. By the division algorithm there exist q(x) and r(x) in F [x] such that f (x) = p(x)q(x) + r(x) and deg r(x) < deg p(x). Since f (x), p(x) ∈ I and I is an ideal, r(x) = f (x)−p(x)q(x) is also in I. However, since we chose p(x) to be of minimal degree, r(x) must be the zero polynomial. Since we can write any element f (x) in I as p(x)q(x) for some q(x) ∈ F [x], it must be the case that I = ⟨p(x)⟩. Example 17.21. It is not the case that every ideal in the ring F [x, y] is a principal ideal. Consider the ideal of F [x, y] generated by the polynomials x and y. This is the ideal of F [x, y] consisting of all polynomials with no constant term. Since both x and y are in the ideal, no single polynomial can generate the entire ideal. Theorem 17.22. Let F be a field and suppose that p(x) ∈ F [x]. Then the ideal generated by p(x) is maximal if and only if p(x) is irreducible. Proof. Suppose that p(x) generates a maximal ideal of F [x]. Then ⟨p(x)⟩ is also a prime ideal of F [x]. Since a maximal ideal must be properly contained inside F [x], p(x) cannot be a constant polynomial. Let us assume that p(x) factors into two polynomials of lesser degree, say p(x) = f (x)g(x). Since ⟨p(x)⟩ is a prime ideal one of these factors, say f (x), is 210 CHAPTER 17. POLYNOMIALS in ⟨p(x)⟩ and therefore be a multiple of p(x). But this would imply that ⟨p(x)⟩ ⊂ ⟨f (x)⟩, which is impossible since ⟨p(x)⟩ is maximal. Conversely, suppose that p(x) is irreducible over F [x]. Let I be an ideal in F [x] contain- ing ⟨p(x)⟩. By Theorem 17.20, I is a principal ideal; hence, I = ⟨f (x)⟩ for some f (x) ∈ F [x]. Since p(x) ∈ I, it must be the case that p(x) = f (x)g(x) for some g(x) ∈ F [x]. However, p(x) is irreducible; hence, either f (x) or g(x) is a constant polynomial. If f (x) is constant, then I = F [x] and we are done. If g(x) is constant, then f (x) is a constant multiple of I and I = ⟨p(x)⟩. Thus, there are no proper ideals of F [x] that properly contain ⟨p(x)⟩. Sage Polynomial rings are very important for computational approaches to algebra, and so Sage makes it very easy to compute with polynomials, over rings, or over fields. And it is trivial to check if a polynomial is irreducible. Historical Note Throughout history, the solution of polynomial equations has been a challenging prob- lem. The Babylonians knew how to solve the equation ax2 + bx + c = 0. Omar Khayyam (1048–1131) devised methods of solving cubic equations through the use of geometric constructions and conic sections. The algebraic solution of the general cubic equation ax3 + bx2 + cx + d = 0 was not discovered until the sixteenth century. An Italian mathe- matician, Luca Pacioli (ca. 1445–1509), wrote in Summa de Arithmetica that the solution of the cubic was impossible. This was taken as a challenge by the rest of the mathematical community. Scipione del Ferro (1465–1526), of the University of Bologna, solved the “depressed cubic,” ax3 + cx + d = 0. He kept his solution an absolute secret. This may seem surprising today, when mathe- maticians are usually very eager to publish their results, but in the days of the Italian Renaissance secrecy was customary. Academic appointments were not easy to secure and depended on the ability to prevail in public contests. Such challenges could be issued at any time. Consequently, any major new discovery was a valuable weapon in such a contest. If an opponent presented a list of problems to be solved, del Ferro could in turn present a list of depressed cubics. He kept the secret of his discovery throughout his life, passing it on only on his deathbed to his student Antonio Fior (ca. 1506–?). Although Fior was not the equal of his teacher, he immediately issued a challenge to Niccolo Fontana (1499–1557). Fontana was known as Tartaglia (the Stammerer). As a youth he had suffered a blow from the sword of a French soldier during an attack on his village. He survived the savage wound, but his speech was permanently impaired. Tartaglia sent Fior a list of 30 various mathematical problems; Fior countered by sending Tartaglia a list of 30 depressed cubics. Tartaglia would either solve all 30 of the problems or absolutely fail. After much effort Tartaglia finally succeeded in solving the depressed cubic and defeated Fior, who faded into obscurity. At this point another mathematician, Gerolamo Cardano (1501–1576), entered the story. Cardano wrote to Tartaglia, begging him for the solution to the depressed cubic. Tartaglia refused several of his requests, then finally revealed the solution to Cardano after the latter swore an oath not to publish the secret or to pass it on to anyone else. Using the knowledge that he had obtained from Tartaglia, Cardano eventually solved the general cubic ax3 + bx2 + cx + d = 0. 17.4. EXERCISES 211 Cardano shared the secret with his student, Ludovico Ferrari (1522–1565), who solved the general quartic equation, ax4 + bx3 + cx2 + dx + e = 0. In 1543, Cardano and Ferrari examined del Ferro’s papers and discovered that he had also solved the depressed cubic. Cardano felt that this relieved him of his obligation to Tartaglia, so he proceeded to publish the solutions in Ars Magna (1545), in which he gave credit to del Ferro for solving the special case of the cubic. This resulted in a bitter dispute between Cardano and Tartaglia, who published the story of the oath a year later. 17.4 Exercises 1. List all of the polynomials of degree 3 or less in Z2 [x]. 2. Compute each of the following. (a) (5x2 + 3x − 4) + (4x2 − x + 9) in Z12 (b) (5x2 + 3x − 4)(4x2 − x + 9) in Z12 (c) (7x3 + 3x2 − x) + (6x2 − 8x + 4) in Z9 (d) (3x2 + 2x − 4) + (4x2 + 2) in Z5 (e) (3x2 + 2x − 4)(4x2 + 2) in Z5 (f) (5x2 + 3x − 2)2 in Z12 3. Use the division algorithm to find q(x) and r(x) such that a(x) = q(x)b(x) + r(x) with deg r(x) < deg b(x) for each of the following pairs of polynomials. (a) a(x) = 5x3 + 6x2 − 3x + 4 and b(x) = x − 2 in Z7 [x] (b) a(x) = 6x4 − 2x3 + x2 − 3x + 1 and b(x) = x2 + x − 2 in Z7 [x] (c) a(x) = 4x5 − x3 + x2 + 4 and b(x) = x3 − 2 in Z5 [x] (d) a(x) = x5 + x3 − x2 − x and b(x) = x3 + x in Z2 [x] 4. Find the greatest common divisor of each of the following pairs p(x) and q(x) of polynomials. If d(x) = gcd(p(x), q(x)), find two polynomials a(x) and b(x) such that a(x)p(x) + b(x)q(x) = d(x). (a) p(x) = x3 − 6x2 + 14x − 15 and q(x) = x3 − 8x2 + 21x − 18, where p(x), q(x) ∈ Q[x] (b) p(x) = x3 + x2 − x + 1 and q(x) = x3 + x − 1, where p(x), q(x) ∈ Z2 [x] (c) p(x) = x3 + x2 − 4x + 4 and q(x) = x3 + 3x − 2, where p(x), q(x) ∈ Z5 [x] (d) p(x) = x3 − 2x + 4 and q(x) = 4x3 + x + 3, where p(x), q(x) ∈ Q[x] 5. Find all of the zeros for each of the following polynomials. (a) 5x3 + 4x2 − x + 9 in Z12 (c) 5x4 + 2x2 − 3 in Z7 (b) 3x3 − 4x2 − x + 4 in Z5 (d) x3 + x + 1 in Z2 212 CHAPTER 17. POLYNOMIALS 6. Find all of the units in Z[x]. 7. Find a unit p(x) in Z4 [x] such that deg p(x) > 1. 8. Which of the following polynomials are irreducible over Q[x]? (a) x4 − 2x3 + 2x2 + x + 4 (c) 3x5 − 4x3 − 6x2 + 6 (b) x4 − 5x3 + 3x − 2 (d) 5x5 − 6x4 − 3x2 + 9x − 15 9. Find all of the irreducible polynomials of degrees 2 and 3 in Z2 [x]. 10. Give two different factorizations of x2 + x + 8 in Z10 [x]. 11. Prove or disprove: There exists a polynomial p(x) in Z6 [x] of degree n with more than n distinct zeros. 12. If F is a field, show that F [x1 , . . . , xn ] is an integral domain. 13. Show that the division algorithm does not hold for Z[x]. Why does it fail? 14. Prove or disprove: xp + a is irreducible for any a ∈ Zp , where p is prime. 15. Let f (x) be irreducible in F [x], where F is a field. If f (x) | p(x)q(x), prove that either f (x) | p(x) or f (x) | q(x). 16. Suppose that R and S are isomorphic rings. Prove that R[x] ∼ = S[x]. 17. Let F be a field and a ∈ F . If p(x) ∈ F [x], show that p(a) is the remainder obtained when p(x) is divided by x − a. 18. The Rational Root Theorem. Let p(x) = an xn + an−1 xn−1 + · · · + a0 ∈ Z[x], where an ̸= 0. Prove that if p(r/s) = 0, where gcd(r, s) = 1, then r | a0 and s | an . 19. Let Q∗ be the multiplicative group of positive rational numbers. Prove that Q∗ is isomorphic to (Z[x], +). 20. Cyclotomic Polynomials. The polynomial xn − 1 Φn (x) = = xn−1 + xn−2 + · · · + x + 1 x−1 is called the cyclotomic polynomial. Show that Φp (x) is irreducible over Q for any prime p. 21. If F is a field, show that there are infinitely many irreducible polynomials in F [x]. 22. Let R be a commutative ring with identity. Prove that multiplication is commutative in R[x]. 23. Let R be a commutative ring with identity. Prove that multiplication is distributive in R[x]. 24. Show that xp − x has p distinct zeros in Zp , for any prime p. Conclude that xp − x = x(x − 1)(x − 2) · · · (x − (p − 1)). 25. Let F be a field and f (x) = a0 + a1 x + · · · + an xn be in F [x]. Define f ′ (x) = a1 + 2a2 x + · · · + nan xn−1 to be the derivative of f (x). (a) Prove that (f + g)′ (x) = f ′ (x) + g ′ (x). Conclude that we can define a homomorphism of abelian groups D : F [x] → F [x] by D(f (x)) = f ′ (x). 17.5. ADDITIONAL EXERCISES: SOLVING THE CUBIC AND QUARTIC EQUATIONS213 (b) Calculate the kernel of D if char F = 0. (c) Calculate the kernel of D if char F = p. (d) Prove that (f g)′ (x) = f ′ (x)g(x) + f (x)g ′ (x). (e) Suppose that we can factor a polynomial f (x) ∈ F [x] into linear factors, say f (x) = a(x − a1 )(x − a2 ) · · · (x − an ). Prove that f (x) has no repeated factors if and only if f (x) and f ′ (x) are relatively prime. 26. Let F be a field. Show that F [x] is never a field. 27. Let R be an integral domain. Prove that R[x1 , . . . , xn ] is an integral domain. 28. Let R be a commutative ring with identity. Show that R[x] has a subring R′ isomorphic to R. 29. Let p(x) and q(x) be polynomials in R[x], where R is a commutative ring with identity. Prove that deg(p(x) + q(x)) ≤ max(deg p(x), deg q(x)). 17.5 Additional Exercises: Solving the Cubic and Quartic Equations 1. Solve the general quadratic equation ax2 + bx + c = 0 to obtain √ −b ± b2 − 4ac x= . 2a The discriminant of the quadratic equation ∆ = b2 − 4ac determines the nature of the solutions of the equation. If ∆ > 0, the equation has two distinct real solutions. If ∆ = 0, the equation has a single repeated real root. If ∆ < 0, there are two distinct imaginary solutions. 2. Show that any cubic equation of the form x3 + bx2 + cx + d = 0 can be reduced to the form y 3 + py + q = 0 by making the substitution x = y − b/3. 3. Prove that the cube roots of 1 are given by √ −1 + i 3 ω= 2 √ −1 − i 3 ω2 = 2 ω 3 = 1. 4. Make the substitution p y=z− 3z 214 CHAPTER 17. POLYNOMIALS for y in the equation y 3 + py + q = 0 and obtain two solutions A and B for z 3 . 5. √ Show that the product of the solutions obtained in (4) is −p3 /27, deducing that 3 AB = −p/3. 6. Prove that the possible solutions for z in (4) are given by √ 3 √3 √3 √3 √3 √ 3 A, ω A, ω 2 A, B, ω B, ω 2 B and use this result to show that the three possible solutions for y are √ √ √ √ q p 3 q 2 q p3 q2 i 3 2i 3 ω − + + +ω − − + , 2 27 4 2 27 4 where i = 0, 1, 2. 7. The discriminant of the cubic equation is p3 q2 ∆= + . 27 4 Show that y 3 + py + q = 0 (a) has three real roots, at least two of which are equal, if ∆ = 0. (b) has one real root and two conjugate imaginary roots if ∆ > 0. (c) has three distinct real roots if ∆ < 0. 8. Solve the following cubic equations. (a) x3 − 4x2 + 11x + 30 = 0 (b) x3 − 3x + 5 = 0 (c) x3 − 3x + 2 = 0 (d) x3 + x + 3 = 0 9. Show that the general quartic equation x4 + ax3 + bx2 + cx + d = 0 can be reduced to y 4 + py 2 + qy + r = 0 by using the substitution x = y − a/4. 10. Show that ( ) ( ) 1 2 1 2 y 2 + z = (z − p)y 2 − qy + z −r . 2 4 11. Show that the right-hand side of Exercise 17.5.10 can be put in the form (my + k)2 if and only if ( ) 1 2 q − 4(z − p) 2 z − r = 0. 4 12. From Exercise 17.5.11 obtain the resolvent cubic equation z 3 − pz 2 − 4rz + (4pr − q 2 ) = 0. 17.5. ADDITIONAL EXERCISES: SOLVING THE CUBIC AND QUARTIC EQUATIONS215 Solving the resolvent cubic equation, put the equation found in Exercise 17.5.10 in the form ( ) 1 2 y + z = (my + k)2 2 2 to obtain the solution of the quartic equation. 13. Use this method to solve the following quartic equations. (a) x4 − x2 − 3x + 2 = 0 (b) x4 + x3 − 7x2 − x + 6 = 0 (c) x4 − 2x2 + 4x − 3 = 0 (d) x4 − 4x3 + 3x2 − 5x + 2 = 0 18 Integral Domains One of the most important rings we study is the ring of integers. It was our first example of an algebraic structure: the first polynomial ring that we examined was Z[x]. We also know that the integers sit naturally inside the field of rational numbers, Q. The ring of integers is the model for all integral domains. In this chapter we will examine integral domains in general, answering questions about the ideal structure of integral domains, polynomial rings over integral domains, and whether or not an integral domain can be embedded in a field. 18.1 Fields of Fractions Every field is also an integral domain; however, there are many integral domains that are not fields. For example, the integers Z form an integral domain but not a field. A question that naturally arises is how we might associate an integral domain with a field. There is a natural way to construct the rationals Q from the integers: the rationals can be represented as formal quotients of two integers. The rational numbers are certainly a field. In fact, it can be shown that the rationals are the smallest field that contains the integers. Given an integral domain D, our question now becomes how to construct a smallest field F containing D. We will do this in the same way as we constructed the rationals from the integers. An element p/q ∈ Q is the quotient of two integers p and q; however, different pairs of integers can represent the same rational number. For instance, 1/2 = 2/4 = 3/6. We know that a c = b d if and only if ad = bc. A more formal way of considering this problem is to examine fractions in terms of equivalence relations. We can think of elements in Q as ordered pairs in Z × Z. A quotient p/q can be written as (p, q). For instance, (3, 7) would represent the fraction 3/7. However, there are problems if we consider all possible pairs in Z × Z. There is no fraction 5/0 corresponding to the pair (5, 0). Also, the pairs (3, 6) and (2, 4) both represent the fraction 1/2. The first problem is easily solved if we require the second coordinate to be nonzero. The second problem is solved by considering two pairs (a, b) and (c, d) to be equivalent if ad = bc. If we use the approach of ordered pairs instead of fractions, then we can study integral domains in general. Let D be any integral domain and let S = {(a, b) : a, b ∈ D and b ̸= 0}. Define a relation on S by (a, b) ∼ (c, d) if ad = bc. Lemma 18.1. The relation ∼ between elements of S is an equivalence relation. 216 18.1. FIELDS OF FRACTIONS 217 Proof. Since D is commutative, ab = ba; hence, ∼ is reflexive on D. Now suppose that (a, b) ∼ (c, d). Then ad = bc or cb = da. Therefore, (c, d) ∼ (a, b) and the relation is symmetric. Finally, to show that the relation is transitive, let (a, b) ∼ (c, d) and (c, d) ∼ (e, f ). In this case ad = bc and cf = de. Multiplying both sides of ad = bc by f yields af d = adf = bcf = bde = bed. Since D is an integral domain, we can deduce that af = be or (a, b) ∼ (e, f ). We will denote the set of equivalence classes on S by FD . We now need to define the operations of addition and multiplication on FD . Recall how fractions are added and multiplied in Q: a c ad + bc + = ; b d bd a c ac · = . b d bd It seems reasonable to define the operations of addition and multiplication on FD in a similar manner. If we denote the equivalence class of (a, b) ∈ S by [a, b], then we are led to define the operations of addition and multiplication on FD by [a, b] + [c, d] = [ad + bc, bd] and [a, b] · [c, d] = [ac, bd], respectively. The next lemma demonstrates that these operations are independent of the choice of representatives from each equivalence class. Lemma 18.2. The operations of addition and multiplication on FD are well-defined. Proof. We will prove that the operation of addition is well-defined. The proof that multiplication is well-defined is left as an exercise. Let [a1 , b1 ] = [a2 , b2 ] and [c1 , d1 ] = [c2 , d2 ]. We must show that [a1 d1 + b1 c1 , b1 d1 ] = [a2 d2 + b2 c2 , b2 d2 ] or, equivalently, that (a1 d1 + b1 c1 )(b2 d2 ) = (b1 d1 )(a2 d2 + b2 c2 ). Since [a1 , b1 ] = [a2 , b2 ] and [c1 , d1 ] = [c2 , d2 ], we know that a1 b2 = b1 a2 and c1 d2 = d1 c2 . Therefore, (a1 d1 + b1 c1 )(b2 d2 ) = a1 d1 b2 d2 + b1 c1 b2 d2 = a1 b2 d1 d2 + b1 b2 c1 d2 = b1 a2 d1 d2 + b1 b2 d1 c2 = (b1 d1 )(a2 d2 + b2 c2 ). Lemma 18.3. The set of equivalence classes of S, FD , under the equivalence relation ∼, together with the operations of addition and multiplication defined by [a, b] + [c, d] = [ad + bc, bd] [a, b] · [c, d] = [ac, bd], is a field. 218 CHAPTER 18. INTEGRAL DOMAINS Proof. The additive and multiplicative identities are [0, 1] and [1, 1], respectively. To show that [0, 1] is the additive identity, observe that [a, b] + [0, 1] = [a1 + b0, b1] = [a, b]. It is easy to show that [1, 1] is the multiplicative identity. Let [a, b] ∈ FD such that a ̸= 0. Then [b, a] is also in FD and [a, b] · [b, a] = [1, 1]; hence, [b, a] is the multiplicative inverse for [a, b]. Similarly, [−a, b] is the additive inverse of [a, b]. We leave as exercises the verification of the associative and commutative properties of multiplication in FD . We also leave it to the reader to show that FD is an abelian group under addition. It remains to show that the distributive property holds in FD ; however, [a, b][e, f ] + [c, d][e, f ] = [ae, bf ] + [ce, df ] = [aedf + bf ce, bdf 2 ] = [aed + bce, bdf ] = [ade + bce, bdf ] = ([a, b] + [c, d])[e, f ] and the lemma is proved. The field FD in Lemma 18.3 is called the field of fractions or field of quotients of the integral domain D. Theorem 18.4. Let D be an integral domain. Then D can be embedded in a field of fractions FD , where any element in FD can be expressed as the quotient of two elements in D. Furthermore, the field of fractions FD is unique in the sense that if E is any field containing D, then there exists a map ψ : FD → E giving an isomorphism with a subfield of E such that ψ(a) = a for all elements a ∈ D, where we identify a with its image in FD . Proof. We will first demonstrate that D can be embedded in the field FD . Define a map ϕ : D → FD by ϕ(a) = [a, 1]. Then for a and b in D, ϕ(a + b) = [a + b, 1] = [a, 1] + [b, 1] = ϕ(a) + ϕ(b) and ϕ(ab) = [ab, 1] = [a, 1][b, 1] = ϕ(a)ϕ(b); hence, ϕ is a homomorphism. To show that ϕ is one-to-one, suppose that ϕ(a) = ϕ(b). Then [a, 1] = [b, 1], or a = a1 = 1b = b. Finally, any element of FD can be expressed as the quotient of two elements in D, since ϕ(a)[ϕ(b)]−1 = [a, 1][b, 1]−1 = [a, 1] · [1, b] = [a, b]. Now let E be a field containing D and define a map ψ : FD → E by ψ([a, b]) = ab−1 . To show that ψ is well-defined, let [a1 , b1 ] = [a2 , b2 ]. Then a1 b2 = b1 a2 . Therefore, a1 b−1 1 = −1 a2 b2 and ψ([a1 , b1 ]) = ψ([a2 , b2 ]). If [a, b] and [c, d] are in FD , then ψ([a, b] + [c, d]) = ψ([ad + bc, bd]) = (ad + bc)(bd)−1 = ab−1 + cd−1 = ψ([a, b]) + ψ([c, d]) 18.2. FACTORIZATION IN INTEGRAL DOMAINS 219 and ψ([a, b] · [c, d]) = ψ([ac, bd]) = (ac)(bd)−1 = ab−1 cd−1 = ψ([a, b])ψ([c, d]). Therefore, ψ is a homomorphism. To complete the proof of the theorem, we need to show that ψ is one-to-one. Suppose that ψ([a, b]) = ab−1 = 0. Then a = 0b = 0 and [a, b] = [0, b]. Therefore, the kernel of ψ is the zero element [0, b] in FD , and ψ is injective. Example 18.5. Since Q is a field, Q[x] is an integral domain. The field of fractions of Q[x] is the set of all rational expressions p(x)/q(x), where p(x) and q(x) are polynomials over the rationals and q(x) is not the zero polynomial. We will denote this field by Q(x). We will leave the proofs of the following corollaries of Theorem 18.4 as exercises. Corollary 18.6. Let F be a field of characteristic zero. Then F contains a subfield iso- morphic to Q. Corollary 18.7. Let F be a field of characteristic p. Then F contains a subfield isomorphic to Zp . 18.2 Factorization in Integral Domains The building blocks of the integers are the prime numbers. If F is a field, then irreducible polynomials in F [x] play a role that is very similar to that of the prime numbers in the ring of integers. Given an arbitrary integral domain, we are led to the following series of definitions. Let R be a commutative ring with identity, and let a and b be elements in R. We say that a divides b, and write a | b, if there exists an element c ∈ R such that b = ac. A unit in R is an element that has a multiplicative inverse. Two elements a and b in R are said to be associates if there exists a unit u in R such that a = ub. Let D be an integral domain. A nonzero element p ∈ D that is not a unit is said to be irreducible provided that whenever p = ab, either a or b is a unit. Furthermore, p is prime if whenever p | ab either p | a or p | b. Example 18.8. It is important to notice that prime and irreducible elements do not always coincide. Let R be the subring (with identity) of Q[x, y] generated by x2 , y 2 , and xy. Each of these elements is irreducible in R; however, xy is not prime, since xy divides x2 y 2 but does not divide either x2 or y 2 . The Fundamental Theorem of Arithmetic states that every positive integer n > 1 can be factored into a product of prime numbers p1 · · · pk , where the pi ’s are not necessarily distinct. We also know that such factorizations are unique up to the order of the pi ’s. We can easily extend this result to the integers. The question arises of whether or not such factorizations are possible in other rings. Generalizing this definition, we say an integral domain D is a unique factorization domain, or ufd, if D satisfies the following criteria. 1. Let a ∈ D such that a ̸= 0 and a is not a unit. Then a can be written as the product of irreducible elements in D. 220 CHAPTER 18. INTEGRAL DOMAINS 2. Let a = p1 · · · pr = q1 · · · qs , where the pi ’s and the qi ’s are irreducible. Then r = s and there is a π ∈ Sr such that pi and qπ(j) are associates for j = 1, . . . , r. Example 18.9. The integers are a unique factorization domain by the Fundamental The- orem of Arithmetic. Example √ 18.10.√Not every integral domain is a unique factorization domain. The subring Z[ 3 i] = {a + b 3 i} of the √ complex numbers√is an integral domain (Exercise 16.6.12, Chapter 16). Let z = a + b 3 i and define ν : Z[ 3 i] → N ∪ {0} by ν(z) = |z| = a2 + 3b2 . 2 It is clear that ν(z) ≥ 0 with equality when z = 0. Also, from our knowledge of complex numbers we know that ν(zw) = ν(z)ν(w). √ It is easy to show that if ν(z) = 1, then z is a unit, and that the only units of Z[ 3 i] are 1 and −1. We claim that 4 has two distinct factorizations into irreducible elements: √ √ 4 = 2 · 2 = (1 − 3 i)(1 + 3 i). √ We must show that each of these factors is an irreducible √ element in Z[ 3 i]. If 2 is not irreducible, then 2 = zw for elements z, w√in Z[ 3 i] where ν(z) = ν(w) = 2. However, there does not exist an element in z in Z[ 3 i] such that ν(z) = 2 because the equation a2 + 3b2 = 2 has no integer √ solutions. √ Therefore, 2 must be irreducible. A similar argument shows√ that both√1 − 3 i and 1 + 3 i are irreducible. Since 2 is not a unit multiple of either 1 − 3 i or 1 + 3 i, 4 has at least two distinct factorizations into irreducible elements. Principal Ideal Domains Let R be a commutative ring with identity. Recall that a principal ideal generated by a ∈ R is an ideal of the form ⟨a⟩ = {ra : r ∈ R}. An integral domain in which every ideal is principal is called a principal ideal domain, or pid. Lemma 18.11. Let D be an integral domain and let a, b ∈ D. Then 1. a | b if and only if ⟨b⟩ ⊂ ⟨a⟩. 2. a and b are associates if and only if ⟨b⟩ = ⟨a⟩. 3. a is a unit in D if and only if ⟨a⟩ = D. Proof. (1) Suppose that a | b. Then b = ax for some x ∈ D. Hence, for every r in D, br = (ax)r = a(xr) and ⟨b⟩ ⊂ ⟨a⟩. Conversely, suppose that ⟨b⟩ ⊂ ⟨a⟩. Then b ∈ ⟨a⟩. Consequently, b = ax for some x ∈ D. Thus, a | b. (2) Since a and b are associates, there exists a unit u such that a = ub. Therefore, b | a and ⟨a⟩ ⊂ ⟨b⟩. Similarly, ⟨b⟩ ⊂ ⟨a⟩. It follows that ⟨a⟩ = ⟨b⟩. Conversely, suppose that ⟨a⟩ = ⟨b⟩. By part (1), a | b and b | a. Then a = bx and b = ay for some x, y ∈ D. Therefore, a = bx = ayx. Since D is an integral domain, xy = 1; that is, x and y are units and a and b are associates. (3) An element a ∈ D is a unit if and only if a is an associate of 1. However, a is an associate of 1 if and only if ⟨a⟩ = ⟨1⟩ = D. Theorem 18.12. Let D be a pid and ⟨p⟩ be a nonzero ideal in D. Then ⟨p⟩ is a maximal ideal if and only if p is irreducible. Proof. Suppose that ⟨p⟩ is a maximal ideal. If some element a in D divides p, then ⟨p⟩ ⊂ ⟨a⟩. Since ⟨p⟩ is maximal, either D = ⟨a⟩ or ⟨p⟩ = ⟨a⟩. Consequently, either a and p are associates or a is a unit. Therefore, p is irreducible. Conversely, let p be irreducible. If ⟨a⟩ is an ideal in D such that ⟨p⟩ ⊂ ⟨a⟩ ⊂ D, then a | p. Since p is irreducible, either a must be a unit or a and p are associates. Therefore, either D = ⟨a⟩ or ⟨p⟩ = ⟨a⟩. Thus, ⟨p⟩ is a maximal ideal. 18.2. FACTORIZATION IN INTEGRAL DOMAINS 221 Corollary 18.13. Let D be a pid. If p is irreducible, then p is prime. Proof. Let p be irreducible and suppose that p | ab. Then ⟨ab⟩ ⊂ ⟨p⟩. By Corollary 16.40, since ⟨p⟩ is a maximal ideal, ⟨p⟩ must also be a prime ideal. Thus, either a ∈ ⟨p⟩ or b ∈ ⟨p⟩. Hence, either p | a or p | b. Lemma 18.14. Let D be a pid. Let I1 , I2 , . . . be a set of ideals such that I1 ⊂ I2 ⊂ · · ·. Then there exists an integer N such that In = IN for all n ≥ N . ∪ Proof. We claim that I = ∞ i=1 Ii is an ideal of D. Certainly I is not empty, since I1 ⊂ I and 0 ∈ I. If a, b ∈ I, then a ∈ Ii and b ∈ Ij for some i and j in N. Without loss of generality we can assume that i ≤ j. Hence, a and b are both in Ij and so a − b is also in Ij . Now let r ∈ D and a ∈ I. Again, we note that a ∈ Ii for some positive integer i. Since Ii is an ideal, ra ∈ Ii and hence must be in I. Therefore, we have shown that I is an ideal in D. Since D is a principal ideal domain, there exists an element a ∈ D that generates I. Since a is in IN for some N ∈ N, we know that IN = I = ⟨a⟩. Consequently, In = IN for n ≥ N. Any commutative ring satisfying the condition in Lemma 18.14 is said to satisfy the ascending chain condition, or ACC. Such rings are called Noetherian rings, after Emmy Noether. Theorem 18.15. Every pid is a ufd. Proof. Existence of a factorization. Let D be a pid and a be a nonzero element in D that is not a unit. If a is irreducible, then we are done. If not, then there exists a factorization a = a1 b1 , where neither a1 nor b1 is a unit. Hence, ⟨a⟩ ⊂ ⟨a1 ⟩. By Lemma 18.11, we know that ⟨a⟩ ̸= ⟨a1 ⟩; otherwise, a and a1 would be associates and b1 would be a unit, which would contradict our assumption. Now suppose that a1 = a2 b2 , where neither a2 nor b2 is a unit. By the same argument as before, ⟨a1 ⟩ ⊂ ⟨a2 ⟩. We can continue with this construction to obtain an ascending chain of ideals ⟨a⟩ ⊂ ⟨a1 ⟩ ⊂ ⟨a2 ⟩ ⊂ · · · . By Lemma 18.14, there exists a positive integer N such that ⟨an ⟩ = ⟨aN ⟩ for all n ≥ N . Consequently, aN must be irreducible. We have now shown that a is the product of two elements, one of which must be irreducible. Now suppose that a = c1 p1 , where p1 is irreducible. If c1 is not a unit, we can repeat the preceding argument to conclude that ⟨a⟩ ⊂ ⟨c1 ⟩. Either c1 is irreducible or c1 = c2 p2 , where p2 is irreducible and c2 is not a unit. Continuing in this manner, we obtain another chain of ideals ⟨a⟩ ⊂ ⟨c1 ⟩ ⊂ ⟨c2 ⟩ ⊂ · · · . This chain must satisfy the ascending chain condition; therefore, a = p1 p2 · · · pr for irreducible elements p1 , . . . , pr . Uniqueness of the factorization. To show uniqueness, let a = p1 p2 · · · pr = q1 q2 · · · qs , 222 CHAPTER 18. INTEGRAL DOMAINS where each pi and each qi is irreducible. Without loss of generality, we can assume that r < s. Since p1 divides q1 q2 · · · qs , by Corollary 18.13 it must divide some qi . By rearranging the qi ’s, we can assume that p1 | q1 ; hence, q1 = u1 p1 for some unit u1 in D. Therefore, a = p1 p2 · · · pr = u1 p1 q2 · · · qs or p2 · · · pr = u1 q2 · · · qs . Continuing in this manner, we can arrange the qi ’s such that p2 = q2 , p3 = q3 , . . . , pr = qr , to obtain u1 u2 · · · ur qr+1 · · · qs = 1. In this case qr+1 · · · qs is a unit, which contradicts the fact that qr+1 , . . . , qs are irreducibles. Therefore, r = s and the factorization of a is unique. Corollary 18.16. Let F be a field. Then F [x] is a ufd. Example 18.17. Every pid is a ufd, but it is not the case that every ufd is a pid. In Corollary 18.31, we will prove that Z[x] is a ufd. However, Z[x] is not a pid. Let I = {5f (x) + xg(x) : f (x), g(x) ∈ Z[x]}. We can easily show that I is an ideal of Z[x]. Suppose that I = ⟨p(x)⟩. Since 5 ∈ I, 5 = f (x)p(x). In this case p(x) = p must be a constant. Since x ∈ I, x = pg(x); consequently, p = ±1. However, it follows from this fact that ⟨p(x)⟩ = Z[x]. But this would mean that 3 is in I. Therefore, we can write 3 = 5f (x) + xg(x) for some f (x) and g(x) in Z[x]. Examining the constant term of this polynomial, we see that 3 = 5f (x), which is impossible. Euclidean Domains We have repeatedly used the division algorithm when proving results about either Z or F [x], where F is a field. We should now ask when a division algorithm is available for an integral domain. Let D be an integral domain such that for each a ∈ D there is a nonnegative integer ν(a) satisfying the following conditions. 1. If a and b are nonzero elements in D, then ν(a) ≤ ν(ab). 2. Let a, b ∈ D and suppose that b ̸= 0. Then there exist elements q, r ∈ D such that a = bq + r and either r = 0 or ν(r) < ν(b). Then D is called a Euclidean domain and ν is called a Euclidean valuation. Example 18.18. Absolute value on Z is a Euclidean valuation. Example 18.19. Let F be a field. Then the degree of a polynomial in F [x] is a Euclidean valuation. Example 18.20. Recall that the Gaussian integers in Example 16.12 of Chapter 16 are defined by Z[i] = {a + bi : a, b ∈ Z}. √ usually measure√the size of a complex number a + bi by its absolute value, |a + bi| = We a2 + b2 ; however, a2 + b2 may not be an integer. For our valuation we will let ν(a+bi) = a + b2 to ensure that we have an integer. 2 We claim that ν(a + bi) = a2 + b2 is a Euclidean valuation on Z[i]. Let z, w ∈ Z[i]. Then ν(zw) = |zw|2 = |z|2 |w|2 = ν(z)ν(w). Since ν(z) ≥ 1 for every nonzero z ∈ Z[i], ν(z) ≤ ν(z)ν(w). Next, we must show that for any z = a + bi and w = c + di in Z[i] with w ̸= 0, there exist elements q and r in Z[i] such that z = qw + r with either r = 0 or ν(r) < ν(w). We 18.2. FACTORIZATION IN INTEGRAL DOMAINS 223 can view z and w as elements in Q(i) = {p + qi : p, q ∈ Q}, the field of fractions of Z[i]. Observe that c − di zw−1 = (a + bi) c2 + d2 ac + bd bc − ad = 2 + 2 i c + d2 ( c +)d2 ( ) n1 n2 = m1 + 2 + m2 + 2 i c + d2 c + d2 ( ) n1 n2 = (m1 + m2 i) + + i c2 + d2 c2 + d2 = (m1 + m2 i) + (s + ti) in Q(i). In the last steps we are writing the real and imaginary parts as an integer plus a proper fraction. That is, we take the closest integer mi such that the fractional part satisfies |ni /(a2 + b2 )| ≤ 1/2. For example, we write 9 1 =1+ 8 8 15 1 =2− . 8 8 Thus, s and t are the “fractional parts” of zw−1 = (m1 + m2 i) + (s + ti). We also know that s2 + t2 ≤ 1/4 + 1/4 = 1/2. Multiplying by w, we have z = zw−1 w = w(m1 + m2 i) + w(s + ti) = qw + r, where q = m1 + m2 i and r = w(s + ti). Since z and qw are in Z[i], r must be in Z[i]. Finally, we need to show that either r = 0 or ν(r) < ν(w). However, 1 ν(r) = ν(w)ν(s + ti) ≤ ν(w) < ν(w). 2 Theorem 18.21. Every Euclidean domain is a principal ideal domain. Proof. Let D be a Euclidean domain and let ν be a Euclidean valuation on D. Suppose I is a nontrivial ideal in D and choose a nonzero element b ∈ I such that ν(b) is minimal for all a ∈ I. Since D is a Euclidean domain, there exist elements q and r in D such that a = bq + r and either r = 0 or ν(r) < ν(b). But r = a − bq is in I since I is an ideal; therefore, r = 0 by the minimality of b. It follows that a = bq and I = ⟨b⟩. Corollary 18.22. Every Euclidean domain is a unique factorization domain. Factorization in D[x] One of the most important polynomial rings is Z[x]. One of the first questions that come to mind about Z[x] is whether or not it is a ufd. We will prove a more general statement here. Our first task is to obtain a more general version of Gauss’s Lemma (Theorem 17.14). Let D be a unique factorization domain and suppose that p(x) = an xn + · · · + a1 x + a0 in D[x]. Then the content of p(x) is the greatest common divisor of a0 , . . . , an . We say that p(x) is primitive if gcd(a0 , . . . , an ) = 1. 224 CHAPTER 18. INTEGRAL DOMAINS Example 18.23. In Z[x] the polynomial p(x) = 5x4 − 3x3 + x − 4 is a primitive polynomial since the greatest common divisor of the coefficients is 1; however, the polynomial q(x) = 4x2 − 6x + 8 is not primitive since the content of q(x) is 2. Theorem 18.24 Gauss’s Lemma. Let D be a ufd and let f (x) and g(x) be primitive polynomials in D[x]. Then f (x)g(x) is primitive. ∑ ∑n Proof. Let f (x) = m i i=0 ai x and g(x) = i i=0 bi x . Suppose that p is a prime dividing the coefficients of f (x)g(x). Let r be the smallest integer such that p ∤ ar and s be the smallest integer such that p ∤ bs . The coefficient of xr+s in f (x)g(x) is cr+s = a0 br+s + a1 br+s−1 + · · · + ar+s−1 b1 + ar+s b0 . Since p divides a0 , . . . , ar−1 and b0 , . . . , bs−1 , p divides every term of cr+s except for the term ar bs . However, since p | cr+s , either p divides ar or p divides bs . But this is impossible. Lemma 18.25. Let D be a ufd, and let p(x) and q(x) be in D[x]. Then the content of p(x)q(x) is equal to the product of the contents of p(x) and q(x). Proof. Let p(x) = cp1 (x) and q(x) = dq1 (x), where c and d are the contents of p(x) and q(x), respectively. Then p1 (x) and q1 (x) are primitive. We can now write p(x)q(x) = cdp1 (x)q1 (x). Since p1 (x)q1 (x) is primitive, the content of p(x)q(x) must be cd. Lemma 18.26. Let D be a ufd and F its field of fractions. Suppose that p(x) ∈ D[x] and p(x) = f (x)g(x), where f (x) and g(x) are in F [x]. Then p(x) = f1 (x)g1 (x), where f1 (x) and g1 (x) are in D[x]. Furthermore, deg f (x) = deg f1 (x) and deg g(x) = deg g1 (x). Proof. Let a and b be nonzero elements of D such that af (x), bg(x) are in D[x]. We can find a1 , b2 ∈ D such that af (x) = a1 f1 (x) and bg(x) = b1 g1 (x), where f1 (x) and g1 (x) are primitive polynomials in D[x]. Therefore, abp(x) = (a1 f1 (x))(b1 g1 (x)). Since f1 (x) and g1 (x) are primitive polynomials, it must be the case that ab | a1 b1 by Gauss’s Lemma. Thus there exists a c ∈ D such that p(x) = cf1 (x)g1 (x). Clearly, deg f (x) = deg f1 (x) and deg g(x) = deg g1 (x). The following corollaries are direct consequences of Lemma 18.26. Corollary 18.27. Let D be a ufd and F its field of fractions. A primitive polynomial p(x) in D[x] is irreducible in F [x] if and only if it is irreducible in D[x]. Corollary 18.28. Let D be a ufd and F its field of fractions. If p(x) is a monic polynomial in D[x] with p(x) = f (x)g(x) in F [x], then p(x) = f1 (x)g1 (x), where f1 (x) and g1 (x) are in D[x]. Furthermore, deg f (x) = deg f1 (x) and deg g(x) = deg g1 (x). Theorem 18.29. If D is a ufd, then D[x] is a ufd. Proof. Let p(x) be a nonzero polynomial in D[x]. If p(x) is a constant polynomial, then it must have a unique factorization since D is a ufd. Now suppose that p(x) is a polynomial of positive degree in D[x]. Let F be the field of fractions of D, and let p(x) = f1 (x)f2 (x) · · · fn (x) by a factorization of p(x), where each fi (x) is irreducible. Choose ai ∈ D such that ai fi (x) is in D[x]. There exist b1 , . . . , bn ∈ D such that ai fi (x) = bi gi (x), where gi (x) is a primitive polynomial in D[x]. By Corollary 18.27, each gi (x) is irreducible in D[x]. Consequently, we can write a1 · · · an p(x) = b1 · · · bn g1 (x) · · · gn (x). 18.2. FACTORIZATION IN INTEGRAL DOMAINS 225 Let b = b1 · · · bn . Since g1 (x) · · · gn (x) is primitive, a1 · · · an divides b. Therefore, p(x) = ag1 (x) · · · gn (x), where a ∈ D. Since D is a ufd, we can factor a as uc1 · · · ck , where u is a unit and each of the ci ’s is irreducible in D. We will now show the uniqueness of this factorization. Let p(x) = a1 · · · am f1 (x) · · · fn (x) = b1 · · · br g1 (x) · · · gs (x) be two factorizations of p(x), where all of the factors are irreducible in D[x]. By Corol- lary 18.27, each of the fi ’s and gi ’s is irreducible in F [x]. The ai ’s and the bi ’s are units in F . Since F [x] is a pid, it is a ufd; therefore, n = s. Now rearrange the gi (x)’s so that fi (x) and gi (x) are associates for i = 1, . . . , n. Then there exist c1 , . . . , cn and d1 , . . . , dn in D such that (ci /di )fi (x) = gi (x) or ci fi (x) = di gi (x). The polynomials fi (x) and gi (x) are primitive; hence, ci and di are associates in D. Thus, a1 · · · am = ub1 · · · br in D, where u is a unit in D. Since D is a unique factorization domain, m = s. Finally, we can reorder the bi ’s so that ai and bi are associates for each i. This completes the uniqueness part of the proof. The theorem that we have just proven has several obvious but important corollaries. Corollary 18.30. Let F be a field. Then F [x] is a ufd. Corollary 18.31. The ring of polynomials over the integers, Z[x], is a ufd. Corollary 18.32. Let D be a ufd. Then D[x1 , . . . , xn ] is a ufd. Remark 18.33. It is important to notice that every Euclidean domain is a pid and every pid is a ufd. However, as demonstrated by our examples, the converse of each of these statements fails. There are principal ideal domains that are not Euclidean domains, and there are unique factorization domains that are not principal ideal domains (Z[x]). Sage Sage supports distinctions between “plain” rings, domains, principal ideal domains and fields. Support is often very good for constructions and computations with PID’s, but sometimes problems get significantly harder (computationally) when a ring has less structure that that of a PID. So be aware when using Sage that some questions may go unanswered for rings with less structure. Historical Note Karl Friedrich Gauss, born in Brunswick, Germany on April 30, 1777, is considered to be one of the greatest mathematicians who ever lived. Gauss was truly a child prodigy. At the age of three he was able to detect errors in the books of his father’s business. Gauss entered college at the age of 15. Before the age of 20, Gauss was able to construct a regular 17-sided polygon with a ruler and compass. This was the first new construction of a regular n-sided polygon since the time of the ancient Greeks. Gauss succeeded in showing that if n N = 22 + 1 was prime, then it was possible to construct a regular N -sided polygon. Gauss obtained his Ph.D. in 1799 under the direction of Pfaff at the University of Helmstedt. In his dissertation he gave the first complete proof of the Fundamental Theorem of Algebra, which states that every polynomial with real coefficients can be factored into linear factors over the complex numbers. The acceptance of complex numbers √ was brought about by Gauss, who was the first person to use the notation of i for −1. Gauss then turned his attention toward number theory; in 1801, he published his fa- mous book on number theory, Disquisitiones Arithmeticae. Throughout his life Gauss was 226 CHAPTER 18. INTEGRAL DOMAINS intrigued with this branch of mathematics. He once wrote, “Mathematics is the queen of the sciences, and the theory of numbers is the queen of mathematics.” In 1807, Gauss was appointed director of the Observatory at the University of Göttingen, a position he held until his death. This position required him to study applications of math- ematics to the sciences. He succeeded in making contributions to fields such as astronomy, mechanics, optics, geodesy, and magnetism. Along with Wilhelm Weber, he coinvented the first practical electric telegraph some years before a better version was invented by Samuel F. B. Morse. Gauss was clearly the most prominent mathematician in the world in the early nineteenth century. His status naturally made his discoveries subject to intense scrutiny. Gauss’s cold and distant personality many times led him to ignore the work of his contemporaries, mak- ing him many enemies. He did not enjoy teaching very much, and young mathematicians who sought him out for encouragement were often rebuffed. Nevertheless, he had many outstanding students, including Eisenstein, Riemann, Kummer, Dirichlet, and Dedekind. Gauss also offered a great deal of encouragement to Sophie Germain (1776–1831), who overcame the many obstacles facing women in her day to become a very prominent mathe- matician. Gauss died at the age of 78 in Göttingen on February 23, 1855. 18.3 Exercises √ √ √ in Z[ 3 i]. If a + 3b = 1, show that z must be a unit. Show 1. Let z = a + b 3 i be 2 2 that the only units of Z[ 3 i] are 1 and −1. 2. The Gaussian integers, Z[i], are a ufd. Factor each of the following elements in Z[i] into a product of irreducibles. (a) 5 (c) 6 + 8i (b) 1 + 3i (d) 2 3. Let D be an integral domain. (a) Prove that FD is an abelian group under the operation of addition. (b) Show that the operation of multiplication is well-defined in the field of fractions, FD . (c) Verify the associative and commutative properties for multiplication in FD . 4. Prove or disprove: Any subring of a field F containing 1 is an integral domain. 5. Prove or disprove: If D is an integral domain, then every prime element in D is also irreducible in D. 6. Let F be a field of characteristic zero. Prove that F contains a subfield isomorphic to Q. 7. Let F be a field. (a) Prove that the field of fractions of F [x], denoted by F (x), is isomorphic to the set all rational expressions p(x)/q(x), where q(x) is not the zero polynomial. (b) Let p(x1 , . . . , xn ) and q(x1 , . . . , xn ) be polynomials in F [x1 , . . . , xn ]. Show that the set of all rational expressions p(x1 , . . . , xn )/q(x1 , . . . , xn ) is isomorphic to the field of fractions of F [x1 , . . . , xn ]. We denote the field of fractions of F [x1 , . . . , xn ] by F (x1 , . . . , xn ). 18.3. EXERCISES 227 8. Let p be prime and denote the field of fractions of Zp [x] by Zp (x). Prove that Zp (x) is an infinite field of characteristic p. 9. Prove that the field of fractions of the Gaussian integers, Z[i], is Q(i) = {p + qi : p, q ∈ Q}. 10. A field F is called a prime field if it has no proper subfields. If E is a subfield of F and E is a prime field, then E is a prime subfield of F . (a) Prove that every field contains a unique prime subfield. (b) If F is a field of characteristic 0, prove that the prime subfield of F is isomorphic to the field of rational numbers, Q. (c) If F is a field of characteristic p, prove that the prime subfield of F is isomorphic to Zp . √ √ 11. Let Z[ 2 ] = {a + b 2 : a, b ∈ Z}. √ (a) Prove that Z[ 2 ] is an integral domain. √ (b) Find all of the units in Z[ 2 ]. √ (c) Determine the field of fractions of Z[ 2 ]. √ √ (d) Prove that Z[ 2i] is a Euclidean domain under the Euclidean valuation ν(a+b 2 i) = a2 + 2b2 . 12. Let D be a ufd. An element d ∈ D is a greatest common divisor of a and b in D if d | a and d | b and d is divisible by any other element dividing both a and b. (a) If D is a pid and a and b are both nonzero elements of D, prove there exists a unique greatest common divisor of a and b up to associates. That is, if d and d′ are both greatest common divisors of a and b, then d and d′ are associates. We write gcd(a, b) for the greatest common divisor of a and b. (b) Let D be a pid and a and b be nonzero elements of D. Prove that there exist elements s and t in D such that gcd(a, b) = as + bt. 13. Let D be an integral domain. Define a relation on D by a ∼ b if a and b are associates in D. Prove that ∼ is an equivalence relation on D. 14. Let D be a Euclidean domain with Euclidean valuation ν. If u is a unit in D, show that ν(u) = ν(1). 15. Let D be a Euclidean domain with Euclidean valuation ν. If a and b are associates in D, prove that ν(a) = ν(b). √ 16. Show that Z[ 5 i] is not a unique factorization domain. 17. Prove or disprove: Every subdomain of a ufd is also a ufd. 18. An ideal of a commutative ring R is said to be finitely generated if there exist elements a1 , . . . , an in R such that every element r ∈ R can be written as a1 r1 + · · · + an rn for some r1 , . . . , rn in R. Prove that R satisfies the ascending chain condition if and only if every ideal of R is finitely generated. 19. Let D be an integral domain with a descending chain of ideals I1 ⊃ I2 ⊃ I3 ⊃ · · ·. Suppose that there exists an N such that Ik = IN for all k ≥ N . A ring satisfying this 228 CHAPTER 18. INTEGRAL DOMAINS condition is said to satisfy the descending chain condition, or DCC. Rings satisfying the DCC are called Artinian rings, after Emil Artin. Show that if D satisfies the descending chain condition, it must satisfy the ascending chain condition. 20. Let R be a commutative ring with identity. We define a multiplicative subset of R to be a subset S such that 1 ∈ S and ab ∈ S if a, b ∈ S. (a) Define a relation ∼ on R × S by (a, s) ∼ (a′ , s′ ) if there exists an s∗ ∈ S such that s∗ (s′ a − sa′ ) = 0. Show that ∼ is an equivalence relation on R × S. (b) Let a/s denote the equivalence class of (a, s) ∈ R × S and let S −1 R be the set of all equivalence classes with respect to ∼. Define the operations of addition and multiplication on S −1 R by a b at + bs + = s t st ab ab = , st st respectively. Prove that these operations are well-defined on S −1 R and that S −1 R is a ring with identity under these operations. The ring S −1 R is called the ring of quotients of R with respect to S. (c) Show that the map ψ : R → S −1 R defined by ψ(a) = a/1 is a ring homomorphism. (d) If R has no zero divisors and 0 ∈ / S, show that ψ is one-to-one. (e) Prove that P is a prime ideal of R if and only if S = R \ P is a multiplicative subset of R. (f) If P is a prime ideal of R and S = R \ P , show that the ring of quotients S −1 R has a unique maximal ideal. Any ring that has a unique maximal ideal is called a local ring. References and Suggested Readings [1] Atiyah, M. F. and MacDonald, I. G. Introduction to Commutative Algebra. Westview Press, Boulder, CO, 1994. [2] Zariski, O. and Samuel, P. Commutative Algebra, vols. I and II. Springer, New York, 1975, 1960. 19 Lattices and Boolean Algebras The axioms of a ring give structure to the operations of addition and multiplication on a set. However, we can construct algebraic structures, known as lattices and Boolean algebras, that generalize other types of operations. For example, the important operations on sets are inclusion, union, and intersection. Lattices are generalizations of order relations on algebraic spaces, such as set inclusion in set theory and inequality in the familiar number systems N, Z, Q, and R. Boolean algebras generalize the operations of intersection and union. Lattices and Boolean algebras have found applications in logic, circuit theory, and probability. 19.1 Lattices Partially Ordered Sets We begin the study of lattices and Boolean algebras by generalizing the idea of inequality. Recall that a relation on a set X is a subset of X × X. A relation P on X is called a partial order of X if it satisfies the following axioms. 1. The relation is reflexive: (a, a) ∈ P for all a ∈ X. 2. The relation is antisymmetric: if (a, b) ∈ P and (b, a) ∈ P , then a = b. 3. The relation is transitive: if (a, b) ∈ P and (b, c) ∈ P , then (a, c) ∈ P . We will usually write a ⪯ b to mean (a, b) ∈ P unless some symbol is naturally associated with a particular partial order, such as a ≤ b with integers a and b, or A ⊂ B with sets A and B. A set X together with a partial order ⪯ is called a partially ordered set, or poset. Example 19.1. The set of integers (or rationals or reals) is a poset where a ≤ b has the usual meaning for two integers a and b in Z. Example 19.2. Let X be any set. We will define the power set of X to be the set of all subsets of X. We denote the power set of X by P(X). For example, let X = {a, b, c}. Then P(X) is the set of all subsets of the set {a, b, c}: ∅ {a} {b} {c} {a, b} {a, c} {b, c} {a, b, c}. On any power set of a set X, set inclusion, ⊂, is a partial order. We can represent the order on {a, b, c} schematically by a diagram such as the one in Figure 19.3. 229 230 CHAPTER 19. LATTICES AND BOOLEAN ALGEBRAS {a, b, c} {a, b} {a, c} {b, c} {a} {b} {c} ∅ Figure 19.3: Partial order on P({a, b, c}) Example 19.4. Let G be a group. The set of subgroups of G is a poset, where the partial order is set inclusion. Example 19.5. There can be more than one partial order on a particular set. We can form a partial order on N by a ⪯ b if a | b. The relation is certainly reflexive since a | a for all a ∈ N. If m | n and n | m, then m = n; hence, the relation is also antisymmetric. The relation is transitive, because if m | n and n | p, then m | p. Example 19.6. Let X = {1, 2, 3, 4, 6, 8, 12, 24} be the set of divisors of 24 with the partial order defined in Example 19.5. Figure 19.7 shows the partial order on X. 24 8 12 4 6 2 3 1 Figure 19.7: A partial order on the divisors of 24 Let Y be a subset of a poset X. An element u in X is an upper bound of Y if a ⪯ u for every element a ∈ Y . If u is an upper bound of Y such that u ⪯ v for every other upper bound v of Y , then u is called a least upper bound or supremum of Y . An element l in X is said to be a lower bound of Y if l ⪯ a for all a ∈ Y . If l is a lower bound of Y such that k ⪯ l for every other lower bound k of Y , then l is called a greatest lower bound or infimum of Y . Example 19.8. Let Y = {2, 3, 4, 6} be contained in the set X of Example 19.6. Then Y has upper bounds 12 and 24, with 12 as a least upper bound. The only lower bound is 1; hence, it must be a greatest lower bound. As it turns out, least upper bounds and greatest lower bounds are unique if they exist. Theorem 19.9. Let Y be a nonempty subset of a poset X. If Y has a least upper bound, then Y has a unique least upper bound. If Y has a greatest lower bound, then Y has a unique greatest lower bound. 19.1. LATTICES 231 Proof. Let u1 and u2 be least upper bounds for Y . By the definition of the least upper bound, u1 ⪯ u for all upper bounds u of Y . In particular, u1 ⪯ u2 . Similarly, u2 ⪯ u1 . Therefore, u1 = u2 by antisymmetry. A similar argument show that the greatest lower bound is unique. On many posets it is possible to define binary operations by using the greatest lower bound and the least upper bound of two elements. A lattice is a poset L such that every pair of elements in L has a least upper bound and a greatest lower bound. The least upper bound of a, b ∈ L is called the join of a and b and is denoted by a ∨ b. The greatest lower bound of a, b ∈ L is called the meet of a and b and is denoted by a ∧ b. Example 19.10. Let X be a set. Then the power set of X, P(X), is a lattice. For two sets A and B in P(X), the least upper bound of A and B is A ∪ B. Certainly A ∪ B is an upper bound of A and B, since A ⊂ A ∪ B and B ⊂ A ∪ B. If C is some other set containing both A and B, then C must contain A ∪ B; hence, A ∪ B is the least upper bound of A and B. Similarly, the greatest lower bound of A and B is A ∩ B. Example 19.11. Let G be a group and suppose that X is the set of subgroups of G. Then X is a poset ordered by set-theoretic inclusion, ⊂. The set of subgroups of G is also a lattice. If H and K are subgroups of G, the greatest lower bound of H and K is H ∩ K. The set H ∪ K may not be a subgroup of G. We leave it as an exercise to show that the least upper bound of H and K is the subgroup generated by H ∪ K. In set theory we have certain duality conditions. For example, by De Morgan’s laws, any statement about sets that is true about (A ∪ B)′ must also be true about A′ ∩ B ′ . We also have a duality principle for lattices. Axiom 19.12 Principle of Duality. Any statement that is true for all lattices remains true when ⪯ is replaced by ⪰ and ∨ and ∧ are interchanged throughout the statement. The following theorem tells us that a lattice is an algebraic structure with two binary operations that satisfy certain axioms. Theorem 19.13. If L is a lattice, then the binary operations ∨ and ∧ satisfy the following properties for a, b, c ∈ L. 1. Commutative laws: a ∨ b = b ∨ a and a ∧ b = b ∧ a. 2. Associative laws: a ∨ (b ∨ c) = (a ∨ b) ∨ c and a ∧ (b ∧ c) = (a ∧ b) ∧ c. 3. Idempotent laws: a ∨ a = a and a ∧ a = a. 4. Absorption laws: a ∨ (a ∧ b) = a and a ∧ (a ∨ b) = a. Proof. By the Principle of Duality, we need only prove the first statement in each part. (1) By definition a ∨ b is the least upper bound of {a, b}, and b ∨ a is the least upper bound of {b, a}; however, {a, b} = {b, a}. (2) We will show that a ∨ (b ∨ c) and (a ∨ b) ∨ c are both least upper bounds of {a, b, c}. Let d = a ∨ b. Then c ⪯ d ∨ c = (a ∨ b) ∨ c. We also know that a ⪯ a ∨ b = d ⪯ d ∨ c = (a ∨ b) ∨ c. A similar argument demonstrates that b ⪯ (a ∨ b) ∨ c. Therefore, (a ∨ b) ∨ c is an upper bound of {a, b, c}. We now need to show that (a ∨ b) ∨ c is the least upper bound of {a, b, c}. Let u be some other upper bound of {a, b, c}. Then a ⪯ u and b ⪯ u; hence, d = a ∨ b ⪯ u. 232 CHAPTER 19. LATTICES AND BOOLEAN ALGEBRAS Since c ⪯ u, it follows that (a ∨ b) ∨ c = d ∨ c ⪯ u. Therefore, (a ∨ b) ∨ c must be the least upper bound of {a, b, c}. The argument that shows a ∨ (b ∨ c) is the least upper bound of {a, b, c} is the same. Consequently, a ∨ (b ∨ c) = (a ∨ b) ∨ c. (3) The join of a and a is the least upper bound of {a}; hence, a ∨ a = a. (4) Let d = a ∧ b. Then a ⪯ a ∨ d. On the other hand, d = a ∧ b ⪯ a, and so a ∨ d ⪯ a. Therefore, a ∨ (a ∧ b) = a. Given any arbitrary set L with operations ∨ and ∧, satisfying the conditions of the previous theorem, it is natural to ask whether or not this set comes from some lattice. The following theorem says that this is always the case. Theorem 19.14. Let L be a nonempty set with two binary operations ∨ and ∧ satisfying the commutative, associative, idempotent, and absorption laws. We can define a partial order on L by a ⪯ b if a ∨ b = b. Furthermore, L is a lattice with respect to ⪯ if for all a, b ∈ L, we define the least upper bound and greatest lower bound of a and b by a ∨ b and a ∧ b, respectively. Proof. We first show that L is a poset under ⪯. Since a ∨ a = a, a ⪯ a and ⪯ is reflexive. To show that ⪯ is antisymmetric, let a ⪯ b and b ⪯ a. Then a ∨ b = b and b ∨ a = a.By the commutative law, b = a ∨ b = b ∨ a = a. Finally, we must show that ⪯ is transitive. Let a ⪯ b and b ⪯ c. Then a ∨ b = b and b ∨ c = c. Thus, a ∨ c = a ∨ (b ∨ c) = (a ∨ b) ∨ c = b ∨ c = c, or a ⪯ c. To show that L is a lattice, we must prove that a ∨ b and a ∧ b are, respectively, the least upper and greatest lower bounds of a and b. Since a = (a ∨ b) ∧ a = a ∧ (a ∨ b), it follows that a ⪯ a ∨ b. Similarly, b ⪯ a ∨ b. Therefore, a ∨ b is an upper bound for a and b. Let u be any other upper bound of both a and b. Then a ⪯ u and b ⪯ u. But a ∨ b ⪯ u since (a ∨ b) ∨ u = a ∨ (b ∨ u) = a ∨ u = u. The proof that a ∧ b is the greatest lower bound of a and b is left as an exercise. 19.2 Boolean Algebras Let us investigate the example of the power set, P(X), of a set X more closely. The power set is a lattice that is ordered by inclusion. By the definition of the power set, the largest element in P(X) is X itself and the smallest element is ∅, the empty set. For any set A in P(X), we know that A ∩ X = A and A ∪ ∅ = A. This suggests the following definition for lattices. An element I in a poset X is a largest element if a ⪯ I for all a ∈ X. An element O is a smallest element of X if O ⪯ a for all a ∈ X. Let A be in P(X). Recall that the complement of A is A′ = X \ A = {x : x ∈ X and x ∈ / A}. We know that A ∪ A′ = X and A ∩ A′ = ∅. We can generalize this example for lattices. A lattice L with a largest element I and a smallest element O is complemented if for each a ∈ L, there exists an a′ such that a ∨ a′ = I and a ∧ a′ = O. In a lattice L, the binary operations ∨ and ∧ satisfy commutative and associative laws; however, they need not satisfy the distributive law a ∧ (b ∨ c) = (a ∧ b) ∨ (a ∧ c); 19.2. BOOLEAN ALGEBRAS 233 however, in P(X) the distributive law is satisfied since A ∩ (B ∪ C) = (A ∩ B) ∪ (A ∩ C) for A, B, C ∈ P(X). We will say that a lattice L is distributive if the following distributive law holds: a ∧ (b ∨ c) = (a ∧ b) ∨ (a ∧ c) for all a, b, c ∈ L. Theorem 19.15. A lattice L is distributive if and only if a ∨ (b ∧ c) = (a ∨ b) ∧ (a ∨ c) for all a, b, c ∈ L. Proof. Let us assume that L is a distributive lattice. a ∨ (b ∧ c) = [a ∨ (a ∧ c)] ∨ (b ∧ c) = a ∨ [(a ∧ c) ∨ (b ∧ c)] = a ∨ [(c ∧ a) ∨ (c ∧ b)] = a ∨ [c ∧ (a ∨ b)] = a ∨ [(a ∨ b) ∧ c] = [(a ∨ b) ∧ a] ∨ [(a ∨ b) ∧ c] = (a ∨ b) ∧ (a ∨ c). The converse follows directly from the Duality Principle. A Boolean algebra is a lattice B with a greatest element I and a smallest element O such that B is both distributive and complemented. The power set of X, P(X), is our prototype for a Boolean algebra. As it turns out, it is also one of the most important Boolean algebras. The following theorem allows us to characterize Boolean algebras in terms of the binary relations ∨ and ∧ without mention of the fact that a Boolean algebra is a poset. Theorem 19.16. A set B is a Boolean algebra if and only if there exist binary operations ∨ and ∧ on B satisfying the following axioms. 1. a ∨ b = b ∨ a and a ∧ b = b ∧ a for a, b ∈ B. 2. a ∨ (b ∨ c) = (a ∨ b) ∨ c and a ∧ (b ∧ c) = (a ∧ b) ∧ c for a, b, c ∈ B. 3. a ∧ (b ∨ c) = (a ∧ b) ∨ (a ∧ c) and a ∨ (b ∧ c) = (a ∨ b) ∧ (a ∨ c) for a, b, c ∈ B. 4. There exist elements I and O such that a ∨ O = a and a ∧ I = a for all a ∈ B. 5. For every a ∈ B there exists an a′ ∈ B such that a ∨ a′ = I and a ∧ a′ = O. Proof. Let B be a set satisfying (1)–(5) in the theorem. One of the idempotent laws is satisfied since a=a∨O = a ∨ (a ∧ a′ ) = (a ∨ a) ∧ (a ∨ a′ ) 234 CHAPTER 19. LATTICES AND BOOLEAN ALGEBRAS = (a ∨ a) ∧ I = a ∨ a. Observe that I ∨ b = (b ∨ b′ ) ∨ b = (b′ ∨ b) ∨ b = b′ ∨ (b ∨ b) = b′ ∨ b = I. Consequently, the first of the two absorption laws holds, since a ∨ (a ∧ b) = (a ∧ I) ∨ (a ∧ b) = a ∧ (I ∨ b) =a∧I = a. The other idempotent and absorption laws are proven similarly. Since B also satisfies (1)– (3), the conditions of Theorem 19.14 are met; therefore, B must be a lattice. Condition (4) tells us that B is a distributive lattice. For a ∈ B, O ∨ a = a; hence, O ⪯ a and O is the smallest element in B. To show that I is the largest element in B, we will first show that a ∨ b = b is equivalent to a ∧ b = a. Since a ∨ I = a for all a ∈ B, using the absorption laws we can determine that a ∨ I = (a ∧ I) ∨ I = I ∨ (I ∧ a) = I or a ⪯ I for all a in B. Finally, since we know that B is complemented by (5), B must be a Boolean algebra. Conversely, suppose that B is a Boolean algebra. Let I and O be the greatest and least elements in B, respectively. If we define a ∨ b and a ∧ b as least upper and greatest lower bounds of {a, b}, then B is a Boolean algebra by Theorem 19.14, Theorem 19.15, and our hypothesis. Many other identities hold in Boolean algebras. Some of these identities are listed in the following theorem. Theorem 19.17. Let B be a Boolean algebra. Then 1. a ∨ I = I and a ∧ O = O for all a ∈ B. 2. If a ∨ b = a ∨ c and a ∧ b = a ∧ c for a, b, c ∈ B, then b = c. 3. If a ∨ b = I and a ∧ b = O, then b = a′ . 4. (a′ )′ = a for all a ∈ B. 5. I ′ = O and O′ = I. 6. (a ∨ b)′ = a′ ∧ b′ and (a ∧ b)′ = a′ ∨ b′ (De Morgan’s Laws). Proof. We will prove only (2). The rest of the identities are left as exercises. For a ∨ b = a ∨ c and a ∧ b = a ∧ c, we have b = b ∨ (b ∧ a) = b ∨ (a ∧ b) = b ∨ (a ∧ c) = (b ∨ a) ∧ (b ∨ c) 19.2. BOOLEAN ALGEBRAS 235 = (a ∨ b) ∧ (b ∨ c) = (a ∨ c) ∧ (b ∨ c) = (c ∨ a) ∧ (c ∨ b) = c ∨ (a ∧ b) = c ∨ (a ∧ c) = c ∨ (c ∧ a) = c. Finite Boolean Algebras A Boolean algebra is a finite Boolean algebra if it contains a finite number of elements as a set. Finite Boolean algebras are particularly nice since we can classify them up to isomorphism. Let B and C be Boolean algebras. A bijective map ϕ : B → C is an isomorphism of Boolean algebras if ϕ(a ∨ b) = ϕ(a) ∨ ϕ(b) ϕ(a ∧ b) = ϕ(a) ∧ ϕ(b) for all a and b in B. We will show that any finite Boolean algebra is isomorphic to the Boolean algebra obtained by taking the power set of some finite set X. We will need a few lemmas and definitions before we prove this result. Let B be a finite Boolean algebra. An element a ∈ B is an atom of B if a ̸= O and a ∧ b = a for all nonzero b ∈ B. Equivalently, a is an atom of B if there is no nonzero b ∈ B distinct from a such that O ⪯ b ⪯ a. Lemma 19.18. Let B be a finite Boolean algebra. If b is a nonzero element of B, then there is an atom a in B such that a ⪯ b. Proof. If b is an atom, let a = b. Otherwise, choose an element b1 , not equal to O or b, such that b1 ⪯ b. We are guaranteed that this is possible since b is not an atom. If b1 is an atom, then we are done. If not, choose b2 , not equal to O or b1 , such that b2 ⪯ b1 . Again, if b2 is an atom, let a = b2 . Continuing this process, we can obtain a chain O ⪯ · · · ⪯ b3 ⪯ b2 ⪯ b1 ⪯ b. Since B is a finite Boolean algebra, this chain must be finite. That is, for some k, bk is an atom. Let a = bk . Lemma 19.19. Let a and b be atoms in a finite Boolean algebra B such that a ̸= b. Then a ∧ b = O. Proof. Since a ∧ b is the greatest lower bound of a and b, we know that a ∧ b ⪯ a. Hence, either a ∧ b = a or a ∧ b = O. However, if a ∧ b = a, then either a ⪯ b or a = O. In either case we have a contradiction because a and b are both atoms; therefore, a ∧ b = O. Lemma 19.20. Let B be a Boolean algebra and a, b ∈ B. The following statements are equivalent. 1. a ⪯ b. 2. a ∧ b′ = O. 236 CHAPTER 19. LATTICES AND BOOLEAN ALGEBRAS 3. a′ ∨ b = I. Proof. (1) ⇒ (2). If a ⪯ b, then a ∨ b = b. Therefore, a ∧ b′ = a ∧ (a ∨ b)′ = a ∧ (a′ ∧ b′ ) = (a ∧ a′ ) ∧ b′ = O ∧ b′ = O. (2) ⇒ (3). If a ∧ b′ = O, then a′ ∨ b = (a ∧ b′ )′ = O′ = I. (3) ⇒ (1). If a′ ∨ b = I, then a = a ∧ (a′ ∨ b) = (a ∧ a′ ) ∨ (a ∧ b) = O ∨ (a ∧ b) = a ∧ b. Thus, a ⪯ b. Lemma 19.21. Let B be a Boolean algebra and b and c be elements in B such that b ̸⪯ c. Then there exists an atom a ∈ B such that a ⪯ b and a ̸⪯ c. Proof. By Lemma 19.20, b ∧ c′ = ̸ O. Hence, there exists an atom a such that a ⪯ b ∧ c′ . Consequently, a ⪯ b and a ̸⪯ c. Lemma 19.22. Let b ∈ B and a1 , . . . , an be the atoms of B such that ai ⪯ b. Then b = a1 ∨ · · · ∨ an . Furthermore, if a, a1 , . . . , an are atoms of B such that a ⪯ b, ai ⪯ b, and b = a ∨ a1 ∨ · · · ∨ an , then a = ai for some i = 1, . . . , n. Proof. Let b1 = a1 ∨ · · · ∨ an . Since ai ⪯ b for each i, we know that b1 ⪯ b. If we can show that b ⪯ b1 , then the lemma is true by antisymmetry. Assume b ̸⪯ b1 . Then there exists an atom a such that a ⪯ b and a ̸⪯ b1 . Since a is an atom and a ⪯ b, we can deduce that a = ai for some ai . However, this is impossible since a ⪯ b1 . Therefore, b ⪯ b1 . Now suppose that b = a1 ∨ · · · ∨ an . If a is an atom less than b, a = a ∧ b = a ∧ (a1 ∨ · · · ∨ an ) = (a ∧ a1 ) ∨ · · · ∨ (a ∧ an ). But each term is O or a with a ∧ ai occurring for only one ai . Hence, by Lemma 19.19, a = ai for some i. Theorem 19.23. Let B be a finite Boolean algebra. Then there exists a set X such that B is isomorphic to P(X). Proof. We will show that B is isomorphic to P(X), where X is the set of atoms of B. Let a ∈ B. By Lemma 19.22, we can write a uniquely as a = a1 ∨· · ·∨an for a1 , . . . , an ∈ X. Consequently, we can define a map ϕ : B → P(X) by ϕ(a) = ϕ(a1 ∨ · · · ∨ an ) = {a1 , . . . , an }. Clearly, ϕ is onto. Now let a = a1 ∨ · · · ∨ an and b = b1 ∨ · · · ∨ bm be elements in B, where each ai and each bi is an atom. If ϕ(a) = ϕ(b), then {a1 , . . . , an } = {b1 , . . . , bm } and a = b. Consequently, ϕ is injective. The join of a and b is preserved by ϕ since ϕ(a ∨ b) = ϕ(a1 ∨ · · · ∨ an ∨ b1 ∨ · · · ∨ bm ) 19.3. THE ALGEBRA OF ELECTRICAL CIRCUITS 237 = {a1 , . . . , an , b1 , . . . , bm } = {a1 , . . . , an } ∪ {b1 , . . . , bm } = ϕ(a1 ∨ · · · ∨ an ) ∪ ϕ(b1 ∧ · · · ∨ bm ) = ϕ(a) ∪ ϕ(b). Similarly, ϕ(a ∧ b) = ϕ(a) ∩ ϕ(b). We leave the proof of the following corollary as an exercise. Corollary 19.24. The order of any finite Boolean algebra must be 2n for some positive integer n. 19.3 The Algebra of Electrical Circuits The usefulness of Boolean algebras has become increasingly apparent over the past several decades with the development of the modern computer. The circuit design of computer chips can be expressed in terms of Boolean algebras. In this section we will develop the Boolean algebra of electrical circuits and switches; however, these results can easily be generalized to the design of integrated computer circuitry. A switch is a device, located at some point in an electrical circuit, that controls the flow of current through the circuit. Each switch has two possible states: it can be open, and not allow the passage of current through the circuit, or a it can be closed, and allow the passage of current. These states are mutually exclusive. We require that every switch be in one state or the other—a switch cannot be open and closed at the same time. Also, if one switch is always in the same state as another, we will denote both by the same letter; that is, two switches that are both labeled with the same letter a will always be open at the same time and closed at the same time. Given two switches, we can construct two fundamental types of circuits. Two switches a and b are in series if they make up a circuit of the type that is illustrated in Figure 19.25. Current can pass between the terminals A and B in a series circuit only if both of the switches a and b are closed. We will denote this combination of switches by a ∧ b. Two switches a and b are in parallel if they form a circuit of the type that appears in Fig- ure 19.26. In the case of a parallel circuit, current can pass between A and B if either one of the switches is closed. We denote a parallel combination of circuits a and b by a ∨ b. A a b B Figure 19.25: a ∧ b a A B b Figure 19.26: a ∨ b We can build more complicated electrical circuits out of series and parallel circuits by replacing any switch in the circuit with one of these two fundamental types of circuits. Circuits constructed in this manner are called series-parallel circuits. We will consider two circuits equivalent if they act the same. That is, if we set the switches in equivalent circuits exactly the same we will obtain the same result. For example, 238 CHAPTER 19. LATTICES AND BOOLEAN ALGEBRAS in a series circuit a∧b is exactly the same as b∧a. Notice that this is exactly the commutative law for Boolean algebras. In fact, the set of all series-parallel circuits forms a Boolean algebra under the operations of ∨ and ∧. We can use diagrams to verify the different axioms of a Boolean algebra. The distributive law, a ∧ (b ∨ c) = (a ∧ b) ∨ (a ∧ c), is illustrated in Figure 19.27. If a is a switch, then a′ is the switch that is always open when a is closed and always closed when a is open. A circuit that is always closed is I in our algebra; a circuit that is always open is O. The laws for a ∧ a′ = O and a ∨ a′ = I are shown in Figure 19.28. b a b a c a c Figure 19.27: a ∧ (b ∨ c) = (a ∧ b) ∨ (a ∧ c) a a a′ a′ Figure 19.28: a ∧ a′ = O and a ∨ a′ = I Example 19.29. Every Boolean expression represents a switching circuit. For example, given the expression (a ∨ b) ∧ (a ∨ b′ ) ∧ (a ∨ b), we can construct the circuit in Figure 19.32. Theorem 19.30. The set of all circuits is a Boolean algebra. We leave as an exercise the proof of this theorem for the Boolean algebra axioms not yet verified. We can now apply the techniques of Boolean algebras to switching theory. Example 19.31. Given a complex circuit, we can now apply the techniques of Boolean algebra to reduce it to a simpler one. Consider the circuit in Figure 19.32. Since (a ∨ b) ∧ (a ∨ b′ ) ∧ (a ∨ b) = (a ∨ b) ∧ (a ∨ b) ∧ (a ∨ b′ ) = (a ∨ b) ∧ (a ∨ b′ ) = a ∨ (b ∧ b′ ) =a∨O = a, we can replace the more complicated circuit with a circuit containing the single switch a and achieve the same function. a a a b b′ b Figure 19.32: (a ∨ b) ∧ (a ∨ b′ ) ∧ (a ∨ b) 19.4. EXERCISES 239 Sage Sage has a full suite of functionality for both posets and lattices, all as part of its ex- cellent support for combinatorics. There is little in this chapter that cannot be investigated with Sage. Historical Note George Boole (1815–1864) was the first person to study lattices. In 1847, he published The Investigation of the Laws of Thought, a book in which he used lattices to formalize logic and the calculus of propositions. Boole believed that mathematics was the study of form rather than of content; that is, he was not so much concerned with what he was calculating as with how he was calculating it. Boole’s work was carried on by his friend Augustus De Morgan (1806–1871). De Morgan observed that the principle of duality often held in set theory, as is illustrated by De Morgan’s laws for set theory. He believed, as did Boole, that mathematics was the study of symbols and abstract operations. Set theory and logic were further advanced by such mathematicians as Alfred North Whitehead (1861–1947), Bertrand Russell (1872–1970), and David Hilbert (1862–1943). In Principia Mathematica, Whitehead and Russell attempted to show the connection between mathematics and logic by the deduction of the natural number system from the rules of formal logic. If the natural numbers could be determined from logic itself, then so could much of the rest of existing mathematics. Hilbert attempted to build up mathematics by using symbolic logic in a way that would prove the consistency of mathematics. His approach was dealt a mortal blow by Kurt Gödel (1906–1978), who proved that there will always be “undecidable” problems in any sufficiently rich axiomatic system; that is, that in any mathematical system of any consequence, there will always be statements that can never be proven either true or false. As often occurs, this basic research in pure mathematics later became indispensable in a wide variety of applications. Boolean algebras and logic have become essential in the design of the large-scale integrated circuitry found on today’s computer chips. Sociologists have used lattices and Boolean algebras to model social hierarchies; biologists have used them to describe biosystems. 19.4 Exercises 1. Draw the lattice diagram for the power set of X = {a, b, c, d} with the set inclusion relation, ⊂. 2. Draw the diagram for the set of positive integers that are divisors of 30. Is this poset a Boolean algebra? 3. Draw a diagram of the lattice of subgroups of Z12 . 4. Let B be the set of positive integers that are divisors of 36. Define an order on B by a ⪯ b if a | b. Prove that B is a Boolean algebra. Find a set X such that B is isomorphic to P(X). 5. Prove or disprove: Z is a poset under the relation a ⪯ b if a | b. 6. Draw the switching circuit for each of the following Boolean expressions. (a) (a ∨ b ∨ a′ ) ∧ a (c) a ∨ (a ∧ b) (b) (a ∨ b)′ ∧ (a ∨ b) (d) (c ∨ a ∨ b) ∧ c′ ∧ (a ∨ b)′ 7. Draw a circuit that will be closed exactly when only one of three switches a, b, and c are closed. 240 CHAPTER 19. LATTICES AND BOOLEAN ALGEBRAS 8. Prove or disprove that the two circuits shown are equivalent. a b c a b a′ b a c′ a c′ 9. Let X be a finite set containing n elements. Prove that P(X) = 2n . Conclude that the order of any finite Boolean algebra must be 2n for some n ∈ N. 10. For each of the following circuits, write a Boolean expression. If the circuit can be replaced by one with fewer switches, give the Boolean expression and draw a diagram for the new circuit. a b′ a′ b a a b a′ b a′ b a b c a′ b′ c a b′ c′ 11. Prove or disprove: The set of all nonzero integers is a lattice, where a ⪯ b is defined by a | b. 12. Let L be a nonempty set with two binary operations ∨ and ∧ satisfying the commu- tative, associative, idempotent, and absorption laws. We can define a partial order on L, as in Theorem 19.14, by a ⪯ b if a ∨ b = b. Prove that the greatest lower bound of a and b is a ∧ b. 13. Let G be a group and X be the set of subgroups of G ordered by set-theoretic inclusion. If H and K are subgroups of G, show that the least upper bound of H and K is the subgroup generated by H ∪ K. 14. Let R be a ring and suppose that X is the set of ideals of R. Show that X is a poset ordered by set-theoretic inclusion, ⊂. Define the meet of two ideals I and J in X by I ∩ J and the join of I and J by I + J. Prove that the set of ideals of R is a lattice under these operations. 19.5. PROGRAMMING EXERCISES 241 15. Let B be a Boolean algebra. Prove each of the following identities. (a) a ∨ I = I and a ∧ O = O for all a ∈ B. (b) If a ∨ b = I and a ∧ b = O, then b = a′ . (c) (a′ )′ = a for all a ∈ B. (d) I ′ = O and O′ = I. (e) (a ∨ b)′ = a′ ∧ b′ and (a ∧ b)′ = a′ ∨ b′ (De Morgan’s laws). 16. By drawing the appropriate diagrams, complete the proof of Theorem 19.30 to show that the switching functions form a Boolean algebra. 17. Let B be a Boolean algebra. Define binary operations + and · on B by a + b = (a ∧ b′ ) ∨ (a′ ∧ b) a · b = a ∧ b. Prove that B is a commutative ring under these operations satisfying a2 = a for all a ∈ B. 18. Let X be a poset such that for every a and b in X, either a ⪯ b or b ⪯ a. Then X is said to be a totally ordered set. (a) Is a | b a total order on N? (b) Prove that N, Z, Q, and R are totally ordered sets under the usual ordering ≤. 19. Let X and Y be posets. A map ϕ : X → Y is order-preserving if a ⪯ b implies that ϕ(a) ⪯ ϕ(b). Let L and M be lattices. A map ψ : L → M is a lattice homomorphism if ψ(a ∨ b) = ψ(a) ∨ ψ(b) and ψ(a ∧ b) = ψ(a) ∧ ψ(b). Show that every lattice homomorphism is order-preserving, but that it is not the case that every order-preserving homomorphism is a lattice homomorphism. 20. Let B be a Boolean algebra. Prove that a = b if and only if (a ∧ b′ ) ∨ (a′ ∧ b) = O for a, b ∈ B. 21. Let B be a Boolean algebra. Prove that a = O if and only if (a ∧ b′ ) ∨ (a′ ∧ b) = b for all b ∈ B. 22. Let L and M be lattices. Define an order relation on L × M by (a, b) ⪯ (c, d) if a ⪯ c and b ⪯ d. Show that L × M is a lattice under this partial order. 19.5 Programming Exercises 1. A Boolean or switching function on n variables is a map f : {O, I}n → {0, I}. A Boolean polynomial is a special type of Boolean function: it is any type of Boolean expression formed from a finite combination of variables x1 , . . . , xn together with O and I, using the operations ∨, ∧, and ′ . The values of the functions are defined in Table 19.33. Write a program to evaluate Boolean polynomials. x y x′ x∨y x∧y 0 0 1 0 0 0 1 1 1 0 1 0 0 1 0 1 1 0 1 1 Table 19.33: Boolean polynomials 242 CHAPTER 19. LATTICES AND BOOLEAN ALGEBRAS References and Suggested Readings [1] Donnellan, T. Lattice Theory. Pergamon Press, Oxford, 1968. [2] Halmos, P. R. “The Basic Concepts of Algebraic Logic,” American Mathematical Monthly 53(1956), 363–87. [3] Hohn, F. “Some Mathematical Aspects of Switching,” American Mathematical Monthly 62(1955), 75–90. [4] Hohn, F. Applied Boolean Algebra. 2nd ed. Macmillan, New York, 1966. [5] Lidl, R. and Pilz, G. Applied Abstract Algebra. 2nd ed. Springer, New York, 1998. [6] Whitesitt, J. Boolean Algebra and Its Applications. Dover, Mineola, NY, 2010. 20 Vector Spaces In a physical system a quantity can often be described with a single number. For example, we need to know only a single number to describe temperature, mass, or volume. However, for some quantities, such as location, we need several numbers. To give the location of a point in space, we need x, y, and z coordinates. Temperature distribution over a solid object requires four numbers: three to identify each point within the object and a fourth to describe the temperature at that point. Often n-tuples of numbers, or vectors, also have certain algebraic properties, such as addition or scalar multiplication. In this chapter we will examine mathematical structures called vector spaces. As with groups and rings, it is desirable to give a simple list of axioms that must be satisfied to make a set of vectors a structure worth studying. 20.1 Definitions and Examples A vector space V over a field F is an abelian group with a scalar product α · v or αv defined for all α ∈ F and all v ∈ V satisfying the following axioms. • α(βv) = (αβ)v; • (α + β)v = αv + βv; • α(u + v) = αu + αv; • 1v = v; where α, β ∈ F and u, v ∈ V . The elements of V are called vectors; the elements of F are called scalars. It is important to notice that in most cases two vectors cannot be multiplied. In general, it is only possible to multiply a vector with a scalar. To differentiate between the scalar zero and the vector zero, we will write them as 0 and 0, respectively. Let us examine several examples of vector spaces. Some of them will be quite familiar; others will seem less so. Example 20.1. The n-tuples of real numbers, denoted by Rn , form a vector space over R. Given vectors u = (u1 , . . . , un ) and v = (v1 , . . . , vn ) in Rn and α in R, we can define vector addition by u + v = (u1 , . . . , un ) + (v1 , . . . , vn ) = (u1 + v1 , . . . , un + vn ) and scalar multiplication by αu = α(u1 , . . . , un ) = (αu1 , . . . , αun ). 243 244 CHAPTER 20. VECTOR SPACES Example 20.2. If F is a field, then F [x] is a vector space over F . The vectors in F [x] are simply polynomials, and vector addition is just polynomial addition. If α ∈ F and p(x) ∈ F [x], then scalar multiplication is defined by αp(x). Example 20.3. The set of all continuous real-valued functions on a closed interval [a, b] is a vector space over R. If f (x) and g(x) are continuous on [a, b], then (f + g)(x) is defined to be f (x) + g(x). Scalar multiplication is defined by (αf )(x) = αf (x) for α ∈ R. For example, if f (x) = sin x and g(x) = x2 , then (2f + 5g)(x) = 2 sin x + 5x2 . √ √ Example 20.4. √ Let V = Q( 2√ ) = {a + b 2 : a, b ∈ Q}. Then V√is a vector space over Q. If u = a + b 2 and v = c + d 2, then u + v = (a + c) + (b + d) 2 is again in V . Also, for α ∈ Q, αv is in V . We will leave it as an exercise to verify that all of the vector space axioms hold for V . Proposition 20.5. Let V be a vector space over F . Then each of the following statements is true. 1. 0v = 0 for all v ∈ V . 2. α0 = 0 for all α ∈ F . 3. If αv = 0, then either α = 0 or v = 0. 4. (−1)v = −v for all v ∈ V . 5. −(αv) = (−α)v = α(−v) for all α ∈ F and all v ∈ V . Proof. To prove (1), observe that 0v = (0 + 0)v = 0v + 0v; consequently, 0 + 0v = 0v + 0v. Since V is an abelian group, 0 = 0v. The proof of (2) is almost identical to the proof of (1). For (3), we are done if α = 0. Suppose that α ̸= 0. Multiplying both sides of αv = 0 by 1/α, we have v = 0. To show (4), observe that v + (−1)v = 1v + (−1)v = (1 − 1)v = 0v = 0, and so −v = (−1)v. We will leave the proof of (5) as an exercise. 20.2 Subspaces Just as groups have subgroups and rings have subrings, vector spaces also have substruc- tures. Let V be a vector space over a field F , and W a subset of V . Then W is a subspace of V if it is closed under vector addition and scalar multiplication; that is, if u, v ∈ W and α ∈ F , it will always be the case that u + v and αv are also in W . Example 20.6. Let W be the subspace of R3 defined by W = {(x1 , 2x1 + x2 , x1 − x2 ) : x1 , x2 ∈ R}. We claim that W is a subspace of R3 . Since α(x1 , 2x1 + x2 , x1 − x2 ) = (αx1 , α(2x1 + x2 ), α(x1 − x2 )) = (αx1 , 2(αx1 ) + αx2 , αx1 − αx2 ), W is closed under scalar multiplication. To show that W is closed under vector addition, let u = (x1 , 2x1 + x2 , x1 − x2 ) and v = (y1 , 2y1 + y2 , y1 − y2 ) be vectors in W . Then u + v = (x1 + y1 , 2(x1 + y1 ) + (x2 + y2 ), (x1 + y1 ) − (x2 + y2 )). 20.3. LINEAR INDEPENDENCE 245 Example 20.7. Let W be the subset of polynomials of F [x] with no odd-power terms. If p(x) and q(x) have no odd-power terms, then neither will p(x) + q(x). Also, αp(x) ∈ W for α ∈ F and p(x) ∈ W . Let V be any vector space over a field F and suppose that v1 , v2 , . . . , vn are vectors in V and α1 , α2 , . . . , αn are scalars in F . Any vector w in V of the form ∑ n w= αi vi = α1 v1 + α2 v2 + · · · + αn vn i=1 is called a linear combination of the vectors v1 , v2 , . . . , vn . The spanning set of vec- tors v1 , v2 , . . . , vn is the set of vectors obtained from all possible linear combinations of v1 , v2 , . . . , vn . If W is the spanning set of v1 , v2 , . . . , vn , then we say that W is spanned by v1 , v 2 , . . . , v n . Proposition 20.8. Let S = {v1 , v2 , . . . , vn } be vectors in a vector space V . Then the span of S is a subspace of V . Proof. Let u and v be in S. We can write both of these vectors as linear combinations of the vi ’s: u = α1 v1 + α2 v2 + · · · + αn vn v = β1 v1 + β2 v2 + · · · + βn vn . Then u + v = (α1 + β1 )v1 + (α2 + β2 )v2 + · · · + (αn + βn )vn is a linear combination of the vi ’s. For α ∈ F , αu = (αα1 )v1 + (αα2 )v2 + · · · + (ααn )vn is in the span of S. 20.3 Linear Independence Let S = {v1 , v2 , . . . , vn } be a set of vectors in a vector space V . If there exist scalars α1 , α2 . . . αn ∈ F such that not all of the αi ’s are zero and α1 v1 + α2 v2 + · · · + αn vn = 0, then S is said to be linearly dependent. If the set S is not linearly dependent, then it is said to be linearly independent. More specifically, S is a linearly independent set if α1 v1 + α2 v2 + · · · + αn vn = 0 implies that α1 = α2 = · · · = αn = 0 for any set of scalars {α1 , α2 . . . αn }. Proposition 20.9. Let {v1 , v2 , . . . , vn } be a set of linearly independent vectors in a vector space. Suppose that v = α1 v1 + α2 v2 + · · · + αn vn = β1 v1 + β2 v2 + · · · + βn vn . Then α1 = β1 , α2 = β2 , . . . , αn = βn . 246 CHAPTER 20. VECTOR SPACES Proof. If v = α1 v1 + α2 v2 + · · · + αn vn = β1 v1 + β2 v2 + · · · + βn vn , then (α1 − β1 )v1 + (α2 − β2 )v2 + · · · + (αn − βn )vn = 0. Since v1 , . . . , vn are linearly independent, αi − βi = 0 for i = 1, . . . , n. The definition of linear dependence makes more sense if we consider the following propo- sition. Proposition 20.10. A set {v1 , v2 , . . . , vn } of vectors in a vector space V is linearly depen- dent if and only if one of the vi ’s is a linear combination of the rest. Proof. Suppose that {v1 , v2 , . . . , vn } is a set of linearly dependent vectors. Then there exist scalars α1 , . . . , αn such that α1 v1 + α2 v2 + · · · + αn vn = 0, with at least one of the αi ’s not equal to zero. Suppose that αk ̸= 0. Then α1 αk−1 αk+1 αn vk = − v1 − · · · − vk−1 − vk+1 − · · · − vn . αk αk αk αk Conversely, suppose that vk = β1 v1 + · · · + βk−1 vk−1 + βk+1 vk+1 + · · · + βn vn . Then β1 v1 + · · · + βk−1 vk−1 − vk + βk+1 vk+1 + · · · + βn vn = 0. The following proposition is a consequence of the fact that any system of homogeneous linear equations with more unknowns than equations will have a nontrivial solution. We leave the details of the proof for the end-of-chapter exercises. Proposition 20.11. Suppose that a vector space V is spanned by n vectors. If m > n, then any set of m vectors in V must be linearly dependent. A set {e1 , e2 , . . . , en } of vectors in a vector space V is called a basis for V if {e1 , e2 , . . . , en } is a linearly independent set that spans V . Example 20.12. The vectors e1 = (1, 0, 0), e2 = (0, 1, 0), and e3 = (0, 0, 1) form a basis for R3 . The set certainly spans R3 , since any arbitrary vector (x1 , x2 , x3 ) in R3 can be written as x1 e1 + x2 e2 + x3 e3 . Also, none of the vectors e1 , e2 , e3 can be written as a linear combination of the other two; hence, they are linearly independent. The vectors e1 , e2 , e3 are not the only basis of R3 : the set {(3, 2, 1), (3, 2, 0), (1, 1, 1)} is also a basis for R3 . √ √ √ √ √ Example 20.13. Let √Q( 2 ) = {a+b 2 : a, b ∈ Q}. The sets {1, 2 } and {1+ 2, 1− 2 } are both bases of Q( 2 ). From the last two examples it should be clear that a given vector space has several bases. In fact, there are an infinite number of bases for both of these examples. In general, there is no unique basis for a vector√space. However, every basis of R3 consists of exactly three vectors, and every basis of Q( 2 ) consists of exactly two vectors. This is a consequence of the next proposition. Proposition 20.14. Let {e1 , e2 , . . . , em } and {f1 , f2 , . . . , fn } be two bases for a vector space V . Then m = n. 20.4. EXERCISES 247 Proof. Since {e1 , e2 , . . . , em } is a basis, it is a linearly independent set. By Proposi- tion 20.11, n ≤ m. Similarly, {f1 , f2 , . . . , fn } is a linearly independent set, and the last proposition implies that m ≤ n. Consequently, m = n. If {e1 , e2 , . . . , en } is a basis for a vector space V , then we say that the dimension of V is n and we write dim V = n. We will leave the proof of the following theorem as an exercise. Theorem 20.15. Let V be a vector space of dimension n. 1. If S = {v1 , . . . , vn } is a set of linearly independent vectors for V , then S is a basis for V. 2. If S = {v1 , . . . , vn } spans V , then S is a basis for V . 3. If S = {v1 , . . . , vk } is a set of linearly independent vectors for V with k < n, then there exist vectors vk+1 , . . . , vn such that {v1 , . . . , vk , vk+1 , . . . , vn } is a basis for V . Sage Many of Sage’s computations, in a wide variety of algebraic settings, come from solving problems in linear algebra. So you will find a wealth of linear algebra functionality. Further, you can use structures such as finite fields to find vector spaces in new settings. 20.4 Exercises 1. If F is a field, show that F [x] is a vector space over F , where the vectors in F [x] are polynomials. Vector addition is polynomial addition, and scalar multiplication is defined by αp(x) for α ∈ F . √ 2. Prove that Q( 2 ) is a vector space. √ √ √ √ √ 3. Let Q( 2, 3 ) be the field generated √ by√ elements of the form a + b 2 + c 3 + d 6, √ Q.√ Prove that Q( 2, 3 ) is a vector space of dimension 4 over Q. where a, b, c, d are in Find a basis for Q( 2, 3 ). 4. Prove that the complex numbers are a vector space of dimension 2 over R. 5. Prove that the set Pn of all polynomials of degree less than n form a subspace of the vector space F [x]. Find a basis for Pn and compute the dimension of Pn . 6. Let F be a field and denote the set of n-tuples of F by F n . Given vectors u = (u1 , . . . , un ) and v = (v1 , . . . , vn ) in F n and α in F , define vector addition by u + v = (u1 , . . . , un ) + (v1 , . . . , vn ) = (u1 + v1 , . . . , un + vn ) and scalar multiplication by αu = α(u1 , . . . , un ) = (αu1 , . . . , αun ). Prove that F n is a vector space of dimension n under these operations. 7. Which of the following sets are subspaces of R3 ? If the set is indeed a subspace, find a basis for the subspace and compute its dimension. (a) {(x1 , x2 , x3 ) : 3x1 − 2x2 + x3 = 0} 248 CHAPTER 20. VECTOR SPACES (b) {(x1 , x2 , x3 ) : 3x1 + 4x3 = 0, 2x1 − x2 + x3 = 0} (c) {(x1 , x2 , x3 ) : x1 − 2x2 + 2x3 = 2} (d) {(x1 , x2 , x3 ) : 3x1 − 2x22 = 0} 8. Show that the set of all possible solutions (x, y, z) ∈ R3 of the equations Ax + By + Cz = 0 Dx + Ey + Cz = 0 form a subspace of R3 . 9. Let W be the subset of continuous functions on [0, 1] such that f (0) = 0. Prove that W is a subspace of C[0, 1]. 10. Let V be a vector space over F . Prove that −(αv) = (−α)v = α(−v) for all α ∈ F and all v ∈ V . 11. Let V be a vector space of dimension n. Prove each of the following statements. (a) If S = {v1 , . . . , vn } is a set of linearly independent vectors for V , then S is a basis for V. (b) If S = {v1 , . . . , vn } spans V , then S is a basis for V . (c) If S = {v1 , . . . , vk } is a set of linearly independent vectors for V with k < n, then there exist vectors vk+1 , . . . , vn such that {v1 , . . . , vk , vk+1 , . . . , vn } is a basis for V . 12. Prove that any set of vectors containing 0 is linearly dependent. 13. Let V be a vector space. Show that {0} is a subspace of V of dimension zero. 14. If a vector space V is spanned by n vectors, show that any set of m vectors in V must be linearly dependent for m > n. 15. Linear Transformations. Let V and W be vector spaces over a field F , of dimen- sions m and n, respectively. If T : V → W is a map satisfying T (u + v) = T (u) + T (v) T (αv) = αT (v) for all α ∈ F and all u, v ∈ V , then T is called a linear transformation from V into W . (a) Prove that the kernel of T , ker(T ) = {v ∈ V : T (v) = 0}, is a subspace of V . The kernel of T is sometimes called the null space of T . (b) Prove that the range or range space of T , R(V ) = {w ∈ W : T (v) = w for some v ∈ V }, is a subspace of W . (c) Show that T : V → W is injective if and only if ker(T ) = {0}. (d) Let {v1 , . . . , vk } be a basis for the null space of T . We can extend this basis to be a basis {v1 , . . . , vk , vk+1 , . . . , vm } of V . Why? Prove that {T (vk+1 ), . . . , T (vm )} is a basis for the range of T . Conclude that the range of T has dimension m − k. 20.4. EXERCISES 249 (e) Let dim V = dim W . Show that a linear transformation T : V → W is injective if and only if it is surjective. 16. Let V and W be finite dimensional vector spaces of dimension n over a field F . Suppose that T : V → W is a vector space isomorphism. If {v1 , . . . , vn } is a basis of V , show that {T (v1 ), . . . , T (vn )} is a basis of W . Conclude that any vector space over a field F of dimension n is isomorphic to F n . 17. Direct Sums. Let U and V be subspaces of a vector space W . The sum of U and V , denoted U + V , is defined to be the set of all vectors of the form u + v, where u ∈ U and v ∈ V . (a) Prove that U + V and U ∩ V are subspaces of W . (b) If U + V = W and U ∩ V = 0, then W is said to be the direct sum. In this case, we write W = U ⊕ V . Show that every element w ∈ W can be written uniquely as w = u + v, where u ∈ U and v ∈ V . (c) Let U be a subspace of dimension k of a vector space W of dimension n. Prove that there exists a subspace V of dimension n − k such that W = U ⊕ V . Is the subspace V unique? (d) If U and V are arbitrary subspaces of a vector space W , show that dim(U + V ) = dim U + dim V − dim(U ∩ V ). 18. Dual Spaces. Let V and W be finite dimensional vector spaces over a field F . (a) Show that the set of all linear transformations from V into W , denoted by Hom(V, W ), is a vector space over F , where we define vector addition as follows: (S + T )(v) = S(v) + T (v) (αS)(v) = αS(v), where S, T ∈ Hom(V, W ), α ∈ F , and v ∈ V . (b) Let V be an F -vector space. Define the dual space of V to be V ∗ = Hom(V, F ). Elements in the dual space of V are called linear functionals. Let v1 , . . . , vn be an ordered basis for V . If v = α1 v1 + · · · + αn vn is any vector in V , define a linear functional ϕi : V → F by ϕi (v) = αi . Show that the ϕi ’s form a basis for V ∗ . This basis is called the dual basis of v1 , . . . , vn (or simply the dual basis if the context makes the meaning clear). (c) Consider the basis {(3, 1), (2, −2)} for R2 . What is the dual basis for (R2 )∗ ? (d) Let V be a vector space of dimension n over a field F and let V ∗∗ be the dual space of V ∗ . Show that each element v ∈ V gives rise to an element λv in V ∗∗ and that the map v 7→ λv is an isomorphism of V with V ∗∗ . 250 CHAPTER 20. VECTOR SPACES References and Suggested Readings [1] Beezer, R. A First Course in Linear Algebra. Available online at http://linear.ups. edu/. 2004–2014. [2] Bretscher, O. Linear Algebra with Applications. 4th ed. Pearson, Upper Saddle River, NJ, 2009. [3] Curtis, C. W. Linear Algebra: An Introductory Approach. 4th ed. Springer, New York, 1984. [4] Hoffman, K. and Kunze, R. Linear Algebra. 2nd ed. Prentice-Hall, Englewood Cliffs, NJ, 1971. [5] Johnson, L. W., Riess, R. D., and Arnold, J. T. Introduction to Linear Algebra. 6th ed. Pearson, Upper Saddle River, NJ, 2011. [6] Leon, S. J. Linear Algebra with Applications. 8th ed. Pearson, Upper Saddle River, NJ, 2010. 21 Fields It is natural to ask whether or not some field F is contained in a larger field. We think of the rational numbers, which reside inside the real numbers, while in turn, the real numbers live inside the complex numbers. We can also study the fields between Q and R and inquire as to the nature of these fields. More specifically if we are given a field F and a polynomial p(x) ∈ F [x], we can ask whether or not we can find a field E containing F such that p(x) factors into linear factors over E[x]. For example, if we consider the polynomial p(x) = x4 − 5x2 + 6 in Q[x], then p(x) factors as (x2 − 2)(x2 − 3). However, both of these factors are irreducible in Q[x]. If we wish to find a zero of p(x), we must go to a larger field. Certainly the field of real numbers will work, since √ √ √ √ p(x) = (x − 2)(x + 2)(x − 3)(x + 3). It is possible to find a smaller field in which p(x) has a zero, namely √ √ Q( 2) = {a + b 2 : a, b ∈ Q}. We wish to be able to compute and study such fields for arbitrary polynomials over a field F. 21.1 Extension Fields A field E is an extension field of a field F if F is a subfield of E. The field F is called the base field. We write F ⊂ E. Example 21.1. For example, let √ √ F = Q( 2 ) = {a + b 2 : a, b ∈ Q} √ √ √ √ and let E = Q( 2 + 3 ) be the smallest field containing both Q and 2 + 3. Both E and F are extension fields of the rational numbers. √ We claim that √ E is an √ extension field√ of F√. To see √ this, √ we need only show that 2 is in E. Since 2 +√ 3 is√ in E, 1/( √ 2 √+ 3 ) = 3 − √ 2 must also √ be in E. Taking linear combinations of 2 + 3 and 3 − 2, we find that 2 and 3 must both be in E. Example 21.2. Let p(x) = x2 + x + 1 ∈ Z2 [x]. Since neither 0 nor 1 is a root of this polynomial, we know that p(x) is irreducible over Z2 . We will construct a field extension of Z2 containing an element α such that p(α) = 0. By Theorem 17.22, the ideal ⟨p(x)⟩ 251 252 CHAPTER 21. FIELDS generated by p(x) is maximal; hence, Z2 [x]/⟨p(x)⟩ is a field. Let f (x) + ⟨p(x)⟩ be an arbitrary element of Z2 [x]/⟨p(x)⟩. By the division algorithm, f (x) = (x2 + x + 1)q(x) + r(x), where the degree of r(x) is less than the degree of x2 + x + 1. Therefore, f (x) + ⟨x2 + x + 1⟩ = r(x) + ⟨x2 + x + 1⟩. The only possibilities for r(x) are then 0, 1, x, and 1+x. Consequently, E = Z2 [x]/⟨x2 +x+1⟩ is a field with four elements and must be a field extension of Z2 , containing a zero α of p(x). The field Z2 (α) consists of elements 0 + 0α = 0 1 + 0α = 1 0 + 1α = α 1 + 1α = 1 + α. Notice that α2 + α + 1 = 0; hence, if we compute (1 + α)2 , (1 + α)(1 + α) = 1 + α + α + (α)2 = α. Other calculations are accomplished in a similar manner. We summarize these computations in the following tables, which tell us how to add and multiply elements in E. + 0 1 α 1+α 0 0 1 α 1+α 1 1 0 1+α α α α 1+α 0 1 1+α 1+α α 1 0 Table 21.3: Addition Table for Z2 (α) · 0 1 α 1+α 0 0 0 0 0 1 0 1 α 1+α α 0 α 1+α 1 1+α 0 1+α 1 α Table 21.4: Multiplication Table for Z2 (α) The following theorem, due to Kronecker, is so important and so basic to our under- standing of fields that it is often known as the Fundamental Theorem of Field Theory. Theorem 21.5. Let F be a field and let p(x) be a nonconstant polynomial in F [x]. Then there exists an extension field E of F and an element α ∈ E such that p(α) = 0. 21.1. EXTENSION FIELDS 253 Proof. To prove this theorem, we will employ the method that we used to construct Example 21.2. Clearly, we can assume that p(x) is an irreducible polynomial. We wish to find an extension field E of F containing an element α such that p(α) = 0. The ideal ⟨p(x)⟩ generated by p(x) is a maximal ideal in F [x] by Theorem 17.22; hence, F [x]/⟨p(x)⟩ is a field. We claim that E = F [x]/⟨p(x)⟩ is the desired field. We first show that E is a field extension of F . We can define a homomorphism of commutative rings by the map ψ : F → F [x]/⟨p(x)⟩, where ψ(a) = a + ⟨p(x)⟩ for a ∈ F . It is easy to check that ψ is indeed a ring homomorphism. Observe that ψ(a) + ψ(b) = (a + ⟨p(x)⟩) + (b + ⟨p(x)⟩) = (a + b) + ⟨p(x)⟩ = ψ(a + b) and ψ(a)ψ(b) = (a + ⟨p(x)⟩)(b + ⟨p(x)⟩) = ab + ⟨p(x)⟩ = ψ(ab). To prove that ψ is one-to-one, assume that a + ⟨p(x)⟩ = ψ(a) = ψ(b) = b + ⟨p(x)⟩. Then a − b is a multiple of p(x), since it lives in the ideal ⟨p(x)⟩. Since p(x) is a nonconstant polynomial, the only possibility is that a − b = 0. Consequently, a = b and ψ is injective. Since ψ is one-to-one, we can identify F with the subfield {a + ⟨p(x)⟩ : a ∈ F } of E and view E as an extension field of F . It remains for us to prove that p(x) has a zero α ∈ E. Set α = x + ⟨p(x)⟩. Then α is in E. If p(x) = a0 + a1 x + · · · + an xn , then p(α) = a0 + a1 (x + ⟨p(x)⟩) + · · · + an (x + ⟨p(x)⟩)n = a0 + (a1 x + ⟨p(x)⟩) + · · · + (an xn + ⟨p(x)⟩) = a0 + a1 x + · · · + an xn + ⟨p(x)⟩ = 0 + ⟨p(x)⟩. Therefore, we have found an element α ∈ E = F [x]/⟨p(x)⟩ such that α is a zero of p(x). Example 21.6. Let p(x) = x5 + x4 + 1 ∈ Z2 [x]. Then p(x) has irreducible factors x2 + x + 1 and x3 + x + 1. For a field extension E of Z2 such that p(x) has a root in E, we can let E be either Z2 [x]/⟨x2 + x + 1⟩ or Z2 [x]/⟨x3 + x + 1⟩. We will leave it as an exercise to show that Z2 [x]/⟨x3 + x + 1⟩ is a field with 23 = 8 elements. Algebraic Elements An element α in an extension field E over F is algebraic over F if f (α) = 0 for some nonzero polynomial f (x) ∈ F [x]. An element in E that is not algebraic over F is transcendental over F . An extension field E of a field F is an algebraic extension of F if every element in E is algebraic over F . If E is a field extension of F and α1 , . . . , αn are contained in E, we denote the smallest field containing F and α1 , . . . , αn by F (α1 , . . . , αn ). If E = F (α) for some α ∈ E, then E is a simple extension of F . √ Example 21.7. Both 2 and i are algebraic over Q since they are zeros of the polynomials x2 −2 and x2 +1, respectively. Clearly π and e are algebraic over the real numbers; however, it is a nontrivial fact that they are transcendental over Q. Numbers in R that are algebraic over Q are in fact quite rare. Almost all real numbers are transcendental over Q.1 (In many cases we do not know whether or not a particular number is transcendental; for example, it is still not known whether π + e is transcendental or algebraic.) 1 The probability that a real number chosen at random from the interval [0, 1] will be transcendental over the rational numbers is one. 254 CHAPTER 21. FIELDS A complex number that is algebraic over Q is an algebraic number. A transcendental number is an element of C that is transcendental over Q. √ √ √ √ Example√21.8. We will show √ that 2 + 3 is algebraic over Q. If α = 2 + 3, then α2 = 2 + 3. Hence, α2 − 2 = 3 and (α2 − 2)2 = 3. Since α4 − 4α2 + 1 = 0, it must be true that α is a zero of the polynomial x4 − 4x2 + 1 ∈ Q[x]. It is very easy to give an example of an extension field E over a field F , where E contains an element transcendental over F . The following theorem characterizes transcendental extensions. Theorem 21.9. Let E be an extension field of F and α ∈ E. Then α is transcendental over F if and only if F (α) is isomorphic to F (x), the field of fractions of F [x]. Proof. Let ϕα : F [x] → E be the evaluation homomorphism for α. Then α is tran- scendental over F if and only if ϕα (p(x)) = p(α) ̸= 0 for all nonconstant polynomials p(x) ∈ F [x]. This is true if and only if ker ϕα = {0}; that is, it is true exactly when ϕα is one-to-one. Hence, E must contain a copy of F [x]. The smallest field containing F [x] is the field of fractions F (x). By Theorem 18.4, E must contain a copy of this field. We have a more interesting situation in the case of algebraic extensions. Theorem 21.10. Let E be an extension field of a field F and α ∈ E with α algebraic over F . Then there is a unique irreducible monic polynomial p(x) ∈ F [x] of smallest degree such that p(α) = 0. If f (x) is another polynomial in F [x] such that f (α) = 0, then p(x) divides f (x). Proof. Let ϕα : F [x] → E be the evaluation homomorphism. The kernel of ϕα is a principal ideal generated by some p(x) ∈ F [x] with deg p(x) ≥ 1. We know that such a polynomial exists, since F [x] is a principal ideal domain and α is algebraic. The ideal ⟨p(x)⟩ consists exactly of those elements of F [x] having α as a zero. If f (α) = 0 and f (x) is not the zero polynomial, then f (x) ∈ ⟨p(x)⟩ and p(x) divides f (x). So p(x) is a polynomial of minimal degree having α as a zero. Any other polynomial of the same degree having α as a zero must have the form βp(x) for some β ∈ F . Suppose now that p(x) = r(x)s(x) is a factorization of p(x) into polynomials of lower degree. Since p(α) = 0, r(α)s(α) = 0; consequently, either r(α) = 0 or s(α) = 0, which contradicts the fact that p is of minimal degree. Therefore, p(x) must be irreducible. Let E be an extension field of F and α ∈ E be algebraic over F . The unique monic polynomial p(x) of the last theorem is called the minimal polynomial for α over F . The degree of p(x) is the degree of α over F . − 2 and g(x) = x4 − 4x2 + 1. These polynomials are the Example 21.11. Let f (x) = x2√ √ √ minimal polynomials of 2 and 2 + 3, respectively. Proposition 21.12. Let E be a field extension of F and α ∈ E be algebraic over F . Then F (α) ∼ = F [x]/⟨p(x)⟩, where p(x) is the minimal polynomial of α over F . Proof. Let ϕα : F [x] → E be the evaluation homomorphism. The kernel of this map is ⟨p(x)⟩, where p(x) is the minimal polynomial of α. By the First Isomorphism Theorem for rings, the image of ϕα in E is isomorphic to F (α) since it contains both F and α. Theorem 21.13. Let E = F (α) be a simple extension of F , where α ∈ E is algebraic over F . Suppose that the degree of α over F is n. Then every element β ∈ E can be expressed uniquely in the form β = b0 + b1 α + · · · + bn−1 αn−1 for bi ∈ F . 21.1. EXTENSION FIELDS 255 Proof. Since ϕα (F [x]) ∼= F (α), every element in E = F (α) must be of the form ϕα (f (x)) = f (α), where f (α) is a polynomial in α with coefficients in F . Let p(x) = xn + an−1 xn−1 + · · · + a0 be the minimal polynomial of α. Then p(α) = 0; hence, αn = −an−1 αn−1 − · · · − a0 . Similarly, αn+1 = ααn = −an−1 αn − an−2 αn−1 − · · · − a0 α = −an−1 (−an−1 αn−1 − · · · − a0 ) − an−2 αn−1 − · · · − a0 α. Continuing in this manner, we can express every monomial αm , m ≥ n, as a linear combi- nation of powers of α that are less than n. Hence, any β ∈ F (α) can be written as β = b0 + b1 α + · · · + bn−1 αn−1 . To show uniqueness, suppose that β = b0 + b1 α + · · · + bn−1 αn−1 = c0 + c1 α + · · · + cn−1 αn−1 for bi and ci in F . Then g(x) = (b0 − c0 ) + (b1 − c1 )x + · · · + (bn−1 − cn−1 )xn−1 is in F [x] and g(α) = 0. Since the degree of g(x) is less than the degree of p(x), the irreducible polynomial of α, g(x) must be the zero polynomial. Consequently, b0 − c0 = b1 − c1 = · · · = bn−1 − cn−1 = 0, or bi = ci for i = 0, 1, . . . , n − 1. Therefore, we have shown uniqueness. Example 21.14. Since x2 + 1 is irreducible over R, ⟨x2 + 1⟩ is a maximal ideal in R[x]. So E = R[x]/⟨x2 +1⟩ is a field extension of R that contains a root of x2 +1. Let α = x+⟨x2 +1⟩. We can identify E with the complex numbers. By Proposition 21.12, E is isomorphic to R(α) = {a + bα : a, b ∈ R}. We know that α2 = −1 in E, since α2 + 1 = (x + ⟨x2 + 1⟩)2 + (1 + ⟨x2 + 1⟩) = (x2 + 1) + ⟨x2 + 1⟩ = 0. Hence, we have an isomorphism of R(α) with C defined by the map that takes a + bα to a + bi. Let E be a field extension of a field F . If we regard E as a vector space over F , then we can bring the machinery of linear algebra to bear on the problems that we will encounter in our study of fields. The elements in the field E are vectors; the elements in the field F are scalars. We can think of addition in E as adding vectors. When we multiply an element in E by an element of F , we are multiplying a vector by a scalar. This view of field extensions is especially fruitful if a field extension E of F is a finite dimensional vector space over F , 256 CHAPTER 21. FIELDS and Theorem 21.13 states that E = F (α) is finite dimensional vector space over F with basis {1, α, α2 , . . . , αn−1 }. If an extension field E of a field F is a finite dimensional vector space over F of dimension n, then we say that E is a finite extension of degree n over F . We write [E : F ] = n. to indicate the dimension of E over F . Theorem 21.15. Every finite extension field E of a field F is an algebraic extension. Proof. Let α ∈ E. Since [E : F ] = n, the elements 1, α, . . . , αn cannot be linearly independent. Hence, there exist ai ∈ F , not all zero, such that an αn + an−1 αn−1 + · · · + a1 α + a0 = 0. Therefore, p(x) = an xn + · · · + a0 ∈ F [x] is a nonzero polynomial with p(α) = 0. Remark 21.16. Theorem 21.15 says that every finite extension of a field F is an algebraic extension. The converse is false, however. We will leave it as an exercise to show that the set of all elements in R that are algebraic over Q forms an infinite field extension of Q. The next theorem is a counting theorem, similar to Lagrange’s Theorem in group theory. Theorem 21.17 will prove to be an extremely useful tool in our investigation of finite field extensions. Theorem 21.17. If E is a finite extension of F and K is a finite extension of E, then K is a finite extension of F and [K : F ] = [K : E][E : F ]. Proof. Let {α1 , . . . , αn } be a basis for E as a vector space over F and {β1 , . . . , βm } be a basis for K as a vector space over E. We claim that {αi βj } ∑ is a basis for K over ∑ F . We will first show that these vectors span K. Let u ∈ K. Then u = m b j=1 j j β and bj = n i=1 aij αi , where bj ∈ E and aij ∈ F . Then ( n ) ∑m ∑ ∑ u= aij αi βj = aij (αi βj ). j=1 i=1 i,j So the mn vectors αi βj must span K over F . We must show that {αi βj } are linearly independent. Recall that a set of vectors v1 , v2 , . . . , vn in a vector space V are linearly independent if c1 v1 + c2 v2 + · · · + cn vn = 0 implies that c1 = c2 = · · · = cn = 0. Let ∑ u= cij (αi βj ) = 0 i,j 21.1. EXTENSION FIELDS 257 for cij ∈ F . We need to prove that all of the cij ’s are zero. We can rewrite u as ( n ) ∑m ∑ cij αi βj = 0, j=1 i=1 ∑ where i cij αi ∈ E. Since the βj ’s are linearly independent over E, it must be the case that ∑ n cij αi = 0 i=1 for all j. However, the αj are also linearly independent over F . Therefore, cij = 0 for all i and j, which completes the proof. The following corollary is easily proved using mathematical induction. Corollary 21.18. If Fi is a field for i = 1, . . . , k and Fi+1 is a finite extension of Fi , then Fk is a finite extension of F1 and [Fk : F1 ] = [Fk : Fk−1 ] · · · [F2 : F1 ]. Corollary 21.19. Let E be an extension field of F . If α ∈ E is algebraic over F with minimal polynomial p(x) and β ∈ F (α) with minimal polynomial q(x), then deg q(x) divides deg p(x). Proof. We know that deg p(x) = [F (α) : F ] and deg q(x) = [F (β) : F ]. Since F ⊂ F (β) ⊂ F (α), [F (α) : F ] = [F (α) : F (β)][F (β) : F ]. √ √ Example 21.20. Let us determine an extension √ field √ of Q4containing 3 + 5. It is easy to determine that the minimal polynomial of 3 + 5 is x − 16x2 + 4. It follows that √ √ [Q( 3 + 5 ) : Q] = 4. √ √ √ √ We√know that {1, 3 } is √ a basis for Q( 3 ) √ over Q. Hence, 3 + 5√ cannot be in Q( 3 ).√ √ It follows that √ 5 √ cannot be √in Q( 3 ) either. √ √ √ √ Therefore, √ {1, 5 } is a basis for√Q( √3, 5 ) = √ (Q( 3√))( 5 ) over Q( 3 ) and {1, 3, 5, 3 5 = 15 } is a basis for Q( 3, 5 ) = Q( 3 + 5 ) over Q. This example shows that it is possible that some extension F (α1 , . . . , αn ) is actually a simple extension of F even though n > 1. √ √ √ Example 21.21. √ Let us compute a basis for Q( 3 5, 5 i), where √ 5√is the positive square root of 5 and 3 5 is the real cube root of 5. We know that 5 i ∈ / Q( 3 5 ), so √ √ √ [Q( 5, 5 i) : Q( 5 )] = 2. 3 3 √ √ √ √ It is easy√to determine √ that {1, 5i } √is a basis for Q( 3 5, 5 i) over Q( 3 √5 ).√We also know that {1, 3 5, ( 3 5 )2 } is a basis for Q( 3 5 ) over Q. Hence, a basis for Q( 3 5, 5 i) over Q is √ √ √ √ √ √ √ {1, 5 i, 5, ( 5 )2 , ( 5 )5 i, ( 5 )7 i = 5 5 i or 5 i}. 3 3 6 6 6 6 √ Notice that 6 5 i is a zero of x6 + 5. We can show that this polynomial is irreducible over Q using Eisenstein’s Criterion, where we let p = 5. Consequently, √ √ √ Q ⊂ Q( 5 i) ⊂ Q( 5, 5 i). 6 3 √ √ √ But it must be the case that Q( 6 5 i) = Q( 3 5, 5 i), since the degree of both of these extensions is 6. 258 CHAPTER 21. FIELDS Theorem 21.22. Let E be a field extension of F . Then the following statements are equivalent. 1. E is a finite extension of F . 2. There exists a finite number of algebraic elements α1 , . . . , αn ∈ E such that E = F (α1 , . . . , αn ). 3. There exists a sequence of fields E = F (α1 , . . . , αn ) ⊃ F (α1 , . . . , αn−1 ) ⊃ · · · ⊃ F (α1 ) ⊃ F, where each field F (α1 , . . . , αi ) is algebraic over F (α1 , . . . , αi−1 ). Proof. (1) ⇒ (2). Let E be a finite algebraic extension of F . Then E is a finite dimensional vector space over F and there exists a basis consisting of elements α1 , . . . , αn in E such that E = F (α1 , . . . , αn ). Each αi is algebraic over F by Theorem 21.15. (2) ⇒ (3). Suppose that E = F (α1 , . . . , αn ), where every αi is algebraic over F . Then E = F (α1 , . . . , αn ) ⊃ F (α1 , . . . , αn−1 ) ⊃ · · · ⊃ F (α1 ) ⊃ F, where each field F (α1 , . . . , αi ) is algebraic over F (α1 , . . . , αi−1 ). (3) ⇒ (1). Let E = F (α1 , . . . , αn ) ⊃ F (α1 , . . . , αn−1 ) ⊃ · · · ⊃ F (α1 ) ⊃ F, where each field F (α1 , . . . , αi ) is algebraic over F (α1 , . . . , αi−1 ). Since F (α1 , . . . , αi ) = F (α1 , . . . , αi−1 )(αi ) is simple extension and αi is algebraic over F (α1 , . . . , αi−1 ), it follows that [F (α1 , . . . , αi ) : F (α1 , . . . , αi−1 )] is finite for each i. Therefore, [E : F ] is finite. Algebraic Closure Given a field F , the question arises as to whether or not we can find a field E such that every polynomial p(x) has a root in E. This leads us to the following theorem. Theorem 21.23. Let E be an extension field of F . The set of elements in E that are algebraic over F form a field. Proof. Let α, β ∈ E be algebraic over F . Then F (α, β) is a finite extension of F . Since every element of F (α, β) is algebraic over F , α ± β, αβ, and α/β (β ̸= 0) are all algebraic over F . Consequently, the set of elements in E that are algebraic over F form a field. Corollary 21.24. The set of all algebraic numbers forms a field; that is, the set of all complex numbers that are algebraic over Q makes up a field. Let E be a field extension of a field F . We define the algebraic closure of a field F in E to be the field consisting of all elements in E that are algebraic over F . A field F is algebraically closed if every nonconstant polynomial in F [x] has a root in F . Theorem 21.25. A field F is algebraically closed if and only if every nonconstant polyno- mial in F [x] factors into linear factors over F [x]. 21.2. SPLITTING FIELDS 259 Proof. Let F be an algebraically closed field. If p(x) ∈ F [x] is a nonconstant polynomial, then p(x) has a zero in F , say α. Therefore, x − α must be a factor of p(x) and so p(x) = (x − α)q1 (x), where deg q1 (x) = deg p(x) − 1. Continue this process with q1 (x) to find a factorization p(x) = (x − α)(x − β)q2 (x), where deg q2 (x) = deg p(x) − 2. The process must eventually stop since the degree of p(x) is finite. Conversely, suppose that every nonconstant polynomial p(x) in F [x] factors into linear factors. Let ax − b be such a factor. Then p(b/a) = 0. Consequently, F is algebraically closed. Corollary 21.26. An algebraically closed field F has no proper algebraic extension E. Proof. Let E be an algebraic extension of F ; then F ⊂ E. For α ∈ E, the minimal polynomial of α is x − α. Therefore, α ∈ F and F = E. Theorem 21.27. Every field F has a unique algebraic closure. It is a nontrivial fact that every field has a unique algebraic closure. The proof is not extremely difficult, but requires some rather sophisticated set theory. We refer the reader to [3], [4], or [8] for a proof of this result. We now state the Fundamental Theorem of Algebra, first proven by Gauss at the age of 22 in his doctoral thesis. This theorem states that every polynomial with coefficients in the complex numbers has a root in the complex numbers. The proof of this theorem will be given in Chapter 23. Theorem 21.28 Fundamental Theorem of Algebra. The field of complex numbers is algebraically closed. 21.2 Splitting Fields Let F be a field and p(x) be a nonconstant polynomial in F [x]. We already know that we can find a field extension of F that contains a root of p(x). However, we would like to know whether an extension E of F containing all of the roots of p(x) exists. In other words, can we find a field extension of F such that p(x) factors into a product of linear polynomials? What is the “smallest” extension containing all the roots of p(x)? Let F be a field and p(x) = a0 + a1 x + · · · + an xn be a nonconstant polynomial in F [x]. An extension field E of F is a splitting field of p(x) if there exist elements α1 , . . . , αn in E such that E = F (α1 , . . . , αn ) and p(x) = (x − α1 )(x − α2 ) · · · (x − αn ). A polynomial p(x) ∈ F [x] splits in E if it is the product of linear factors in E[x]. Example 21.29. Let p(x) = x4 + 2x2 −√ 8 be in Q[x]. Then p(x) has irreducible factors x − 2 and x + 4. Therefore, the field Q( 2, i) is a splitting field for p(x). 2 2 √ Example 21.30. Let p(x) = x3 − 3 be in Q[x]. Then p(x) has a root in the field Q( 3 3 ). However, this field is not a splitting field for p(x) since the complex cube roots of 3, √ √ − 3 3 ± ( 6 3 )5 i , 2 √ are not in Q( 3 3 ). 260 CHAPTER 21. FIELDS Theorem 21.31. Let p(x) ∈ F [x] be a nonconstant polynomial. Then there exists a splitting field E for p(x). Proof. We will use mathematical induction on the degree of p(x). If deg p(x) = 1, then p(x) is a linear polynomial and E = F . Assume that the theorem is true for all polynomials of degree k with 1 ≤ k < n and let deg p(x) = n. We can assume that p(x) is irreducible; otherwise, by our induction hypothesis, we are done. By Theorem 21.5, there exists a field K such that p(x) has a zero α1 in K. Hence, p(x) = (x − α1 )q(x), where q(x) ∈ K[x]. Since deg q(x) = n − 1, there exists a splitting field E ⊃ K of q(x) that contains the zeros α2 , . . . , αn of p(x) by our induction hypothesis. Consequently, E = K(α2 , . . . , αn ) = F (α1 , . . . , αn ) is a splitting field of p(x). The question of uniqueness now arises for splitting fields. This question is answered in the affirmative. Given two splitting fields K and L of a polynomial p(x) ∈ F [x], there exists a field isomorphism ϕ : K → L that preserves F . In order to prove this result, we must first prove a lemma. Lemma 21.32. Let ϕ : E → F be an isomorphism of fields. Let K be an extension field of E and α ∈ K be algebraic over E with minimal polynomial p(x). Suppose that L is an extension field of F such that β is root of the polynomial in F [x] obtained from p(x) under the image of ϕ. Then ϕ extends to a unique isomorphism ϕ : E(α) → F (β) such that ϕ(α) = β and ϕ agrees with ϕ on E. Proof. If p(x) has degree n, then by Theorem 21.13 we can write any element in E(α) as a linear combination of 1, α, . . . , αn−1 . Therefore, the isomorphism that we are seeking must be ϕ(a0 + a1 α + · · · + an−1 αn−1 ) = ϕ(a0 ) + ϕ(a1 )β + · · · + ϕ(an−1 )β n−1 , where a0 + a1 α + · · · + an−1 αn−1 is an element in E(α). The fact that ϕ is an isomorphism could be checked by direct computation; however, it is easier to observe that ϕ is a composition of maps that we already know to be isomorphisms. We can extend ϕ to be an isomorphism from E[x] to F [x], which we will also denote by ϕ, by letting ϕ(a0 + a1 x + · · · + an xn ) = ϕ(a0 ) + ϕ(a1 )x + · · · + ϕ(an )xn . This extension agrees with the original isomorphism ϕ : E → F , since constant polynomials get mapped to constant polynomials. By assumption, ϕ(p(x)) = q(x); hence, ϕ maps ⟨p(x)⟩ onto ⟨q(x)⟩. Consequently, we have an isomorphism ψ : E[x]/⟨p(x)⟩ → F [x]/⟨q(x)⟩. By Proposition 21.12, we have isomorphisms σ : E[x]/⟨p(x)⟩ → E(α) and τ : F [x]/⟨q(x)⟩ → F (β), defined by evaluation at α and β, respectively. Therefore, ϕ = τ ψσ −1 is the required isomorphism. 21.2. SPLITTING FIELDS 261 ψ E[x]/⟨p(x)⟩ F [x]/⟨q(x)⟩ σ τ ϕ E(α) F (β) ϕ E F We leave the proof of uniqueness as a exercise. Theorem 21.33. Let ϕ : E → F be an isomorphism of fields and let p(x) be a nonconstant polynomial in E[x] and q(x) the corresponding polynomial in F [x] under the isomorphism. If K is a splitting field of p(x) and L is a splitting field of q(x), then ϕ extends to an isomorphism ψ : K → L. Proof. We will use mathematical induction on the degree of p(x). We can assume that p(x) is irreducible over E. Therefore, q(x) is also irreducible over F . If deg p(x) = 1, then by the definition of a splitting field, K = E and L = F and there is nothing to prove. Assume that the theorem holds for all polynomials of degree less than n. Since K is a splitting field of p(x), all of the roots of p(x) are in K. Choose one of these roots, say α, such that E ⊂ E(α) ⊂ K. Similarly, we can find a root β of q(x) in L such that F ⊂ F (β) ⊂ L. By Lemma 21.32, there exists an isomorphism ϕ : E(α) → F (β) such that ϕ(α) = β and ϕ agrees with ϕ on E. ψ K L ϕ E(α) F (β) ϕ E F Now write p(x) = (x − α)f (x) and q(x) = (x − β)g(x), where the degrees of f (x) and g(x) are less than the degrees of p(x) and q(x), respectively. The field extension K is a 262 CHAPTER 21. FIELDS splitting field for f (x) over E(α), and L is a splitting field for g(x) over F (β). By our induction hypothesis there exists an isomorphism ψ : K → L such that ψ agrees with ϕ on E(α). Hence, there exists an isomorphism ψ : K → L such that ψ agrees with ϕ on E. Corollary 21.34. Let p(x) be a polynomial in F [x]. Then there exists a splitting field K of p(x) that is unique up to isomorphism. 21.3 Geometric Constructions In ancient Greece, three classic problems were posed. These problems are geometric in nature and involve straightedge-and-compass constructions from what is now high school geometry; that is, we are allowed to use only a straightedge and compass to solve them. The problems can be stated as follows. 1. Given an arbitrary angle, can one trisect the angle into three equal subangles using only a straightedge and compass? 2. Given an arbitrary circle, can one construct a square with the same area using only a straightedge and compass? 3. Given a cube, can one construct the edge of another cube having twice the volume of the original? Again, we are only allowed to use a straightedge and compass to do the construction. After puzzling mathematicians for over two thousand years, each of these constructions was finally shown to be impossible. We will use the theory of fields to provide a proof that the solutions do not exist. It is quite remarkable that the long-sought solution to each of these three geometric problems came from abstract algebra. First, let us determine more specifically what we mean by a straightedge and compass, and also examine the nature of these problems in a bit more depth. To begin with, a straightedge is not a ruler. We cannot measure arbitrary lengths with a straightedge. It is merely a tool for drawing a line through two points. The statement that the trisection of an arbitrary angle is impossible means that there is at least one angle that is impossible to trisect with a straightedge-and-compass construction. Certainly it is possible to trisect an angle in special cases. We can construct a 30◦ angle; hence, it is possible to trisect a 90◦ angle. However, we will show that it is impossible to construct a 20◦ angle. Therefore, we cannot trisect a 60◦ angle. Constructible Numbers A real number α is constructible if we can construct a line segment of length |α| in a finite number of steps from a segment of unit length by using a straightedge and compass. Theorem 21.35. The set of all constructible real numbers forms a subfield F of the field of real numbers. Proof. Let α and β be constructible numbers. We must show that α + β, α − β, αβ, and α/β (β ̸= 0) are also constructible numbers. We can assume that both α and β are positive with α > β. It is quite obvious how to construct α + β and α − β. To find a line segment with length αβ, we assume that β > 1 and construct the triangle in Figure 21.36 such that triangles △ABC and △ADE are similar. Since α/1 = x/β, the line segment x has length αβ. A similar construction can be made if β < 1. We will leave it as an exercise to show that the same triangle can be used to construct α/β for β ̸= 0. 21.3. GEOMETRIC CONSTRUCTIONS 263 D β B 1 α C A E x Figure 21.36: Construction of products √ Lemma 21.37. If α is a constructible number, then α is a constructible number. Proof. In Figure 21.38 the triangles △ABD, △BCD, and △ABC are similar; hence, 1/x = x/α, or x2 = α. B x 1 α A D C Figure 21.38: Construction of roots By Theorem 21.35, we can locate in the plane any point P = (p, q) that has rational coordinates p and q. We need to know what other points can be constructed with a compass and straightedge from points with rational coordinates. Lemma 21.39. Let F be a subfield of R. 1. If a line contains two points in F , then it has the equation ax + by + c = 0, where a, b, and c are in F . 2. If a circle has a center at a point with coordinates in F and a radius that is also in F , then it has the equation x2 + y 2 + dx + ey + f = 0, where d, e, and f are in F . Proof. Let (x1 , y1 ) and (x2 , y2 ) be points on a line whose coordinates are in F . If x1 = x2 , then the equation of the line through the two points is x − x1 = 0, which has the form ax + by + c = 0. If x1 ̸= x2 , then the equation of the line through the two points is given by ( ) y2 − y1 y − y1 = (x − x1 ), x2 − x1 which can also be put into the proper form. To prove the second part of the lemma, suppose that (x1 , y1 ) is the center of a circle of radius r. Then the circle has the equation (x − x1 )2 + (y − y1 )2 − r2 = 0. This equation can easily be put into the appropriate form. 264 CHAPTER 21. FIELDS Starting with a field of constructible numbers F , we have three possible ways of con- structing additional points in R with a compass and straightedge. 1. To find possible new points in R, we can take the intersection of two lines, each of which passes through two known points with coordinates in F . 2. The intersection of a line that passes through two points that have coordinates in F and a circle whose center has coordinates in F with radius of a length in F will give new points in R. 3. We can obtain new points in R by intersecting two circles whose centers have coordi- nates in F and whose radii are of lengths in F . The first case gives no new points in R, since the solution of two equations of the form ax + by + c = 0 having coefficients in F will always be in F . The third case can be reduced to the second case. Let x2 + y 2 + d1 x + e1 y + f1 = 0 x2 + y 2 + d2 x + e2 y + f2 = 0 be the equations of two circles, where di , ei , and fi are in F for i = 1, 2. These circles have the same intersection as the circle x2 + y 2 + d1 x + e1 x + f1 = 0 and the line (d1 − d2 )x + b(e2 − e1 )y + (f2 − f1 ) = 0. The last equation is that of the chord passing through the intersection points of the two circles. Hence, the intersection of two circles can be reduced to the case of an intersection of a line with a circle. Considering the case of the intersection of a line and a circle, we must determine the nature of the solutions of the equations ax + by + c = 0 2 2 x + y + dx + ey + f = 0. If we eliminate y from these equations, we obtain an equation of the form Ax2 +Bx+C = 0, where A, B, and C are in F . The x coordinate of the intersection points is given by √ −B ± B 2 − 4AC x= 2A √ and is in F ( α ), where α = B 2 − 4AC > 0. We have proven the following lemma. Lemma 21.40. Let F be a field of constructible numbers. Then the points determined by √ the intersections of lines and circles in F lie in the field F ( α ) for some α in F . Theorem 21.41. A real number α is a constructible number if and only if there exists a sequence of fields Q = F0 ⊂ F1 ⊂ · · · ⊂ Fk √ such that Fi = Fi−1 ( αi ) with αi ∈ Fi and α ∈ Fk . In particular, there exists an integer k > 0 such that [Q(α) : Q] = 2k . 21.3. GEOMETRIC CONSTRUCTIONS 265 Proof. The existence of the Fi ’s and the αi ’s is a direct consequence of Lemma 21.40 and of the fact that [Fk : Q] = [Fk : Fk−1 ][Fk−1 : Fk−2 ] · · · [F1 : Q] = 2k . Corollary 21.42. The field of all constructible numbers is an algebraic extension of Q. As we can see by the field of constructible numbers, not every algebraic extension of a field is a finite extension. Doubling the Cube and Squaring the Circle We are now ready to investigate the classical problems of doubling the cube and squaring the circle. We can use the field of constructible numbers to show exactly when a particular geometric construction can be accomplished. Doubling the cube is impossible Given the edge of the cube, it is impossible to con- struct with a straightedge and compass the edge of the cube that has twice the volume of the original cube. Let the original cube have an edge of length 1 and, therefore, a volume of 1. If we could construct √ a cube√ having a volume of 2, then this new cube would have an edge of length 2. However, 2 is a zero of the irreducible polynomial x3 − 2 over Q; 3 3 hence, √ [Q( 2 ) : Q] = 3 3 This is impossible, since 3 is not a power of 2. Squaring the circle Suppose that we have a circle of radius 1. The area of the circle √ is π; therefore, we must be able to construct a square with side π. This is impossible √ since π and consequently π are both transcendental. Therefore, using a straightedge and compass, it is not possible to construct a square with the same area as the circle. Trisecting an Angle Trisecting an arbitrary angle is impossible. We will show that it is impossible to construct a 20◦ angle. Consequently, a 60◦ angle cannot be trisected. We first need to calculate the triple-angle formula for the cosine: cos 3θ = cos(2θ + θ) = cos 2θ cos θ − sin 2θ sin θ = (2 cos2 θ − 1) cos θ − 2 sin2 θ cos θ = (2 cos2 θ − 1) cos θ − 2(1 − cos2 θ) cos θ = 4 cos3 θ − 3 cos θ. The angle θ can be constructed if and only if α = cos θ is constructible. Let θ = 20◦ . Then cos 3θ = cos 60◦ = 1/2. By the triple-angle formula for the cosine, 1 4α3 − 3α = . 2 Therefore, α is a zero of 8x3 − 6x − 1. This polynomial has no factors in Z[x], and hence is irreducible over Q[x]. Thus, [Q(α) : Q] = 3. Consequently, α cannot be a constructible number. 266 CHAPTER 21. FIELDS Sage Extensions of the field of rational numbers are a central object of study in number theory, so with Sage’s roots in this discipline, it is no surprise that there is extensive support for fields and for extensions of the rationals. Sage also contains an implementation of the entire field of algebraic numbers, with exact representations. Historical Note Algebraic number theory uses the tools of algebra to solve problems in number theory. Modern algebraic number theory began with Pierre de Fermat (1601–1665). Certainly we can find many positive integers that satisfy the equation x2 + y 2 = z 2 ; Fermat conjectured that the equation xn + y n = z n has no positive integer solutions for n ≥ 3. He stated in the margin of his copy of the Latin translation of Diophantus’ Arithmetica that he had found a marvelous proof of this theorem, but that the margin of the book was too narrow to contain it. Building on work of other mathematicians, it was Andrew Wiles who finally succeeded in proving Fermat’s Last Theorem in the 1990s. Wiles’s achievement was reported on the front page of the New York Times. Attempts to prove Fermat’s Last Theorem have led to important contributions to al- gebraic number theory by such notable mathematicians as Leonhard Euler (1707–1783). Significant advances in the understanding of Fermat’s Last Theorem were made by Ernst Kummer (1810–1893). Kummer’s student, Leopold Kronecker (1823–1891), became one of the leading algebraists of the nineteenth century. Kronecker’s theory of ideals and his study of algebraic number theory added much to the understanding of fields. David Hilbert (1862–1943) and Hermann Minkowski (1864–1909) were among the math- ematicians who led the way in this subject at the beginning of the twentieth century. Hilbert and Minkowski were both mathematicians at Göttingen University in Germany. Göttingen was truly one the most important centers of mathematical research during the last two cen- turies. The large number of exceptional mathematicians who studied there included Gauss, Dirichlet, Riemann, Dedekind, Noether, and Weyl. André Weil answered questions in number theory using algebraic geometry, a field of mathematics that studies geometry by studying commutative rings. From about 1955 to 1970, Alexander Grothendieck dominated the field of algebraic geometry. Pierre Deligne, a student of Grothendieck, solved several of Weil’s number-theoretic conjectures. One of the most recent contributions to algebra and number theory is Gerd Falting’s proof of the Mordell-Weil conjecture. This conjecture of Mordell and Weil essentially says that certain polynomials p(x, y) in Z[x, y] have only a finite number of integral solutions. 21.4 Exercises 1. Show that each of the following numbers is algebraic over Q by finding the minimal polynomial of the number over Q. √ √ (a) 1/3 + 7 √ √ 3 (b) 3+ 5 √ √ (c) 3+ 2i (d) cos θ + i sin θ for θ = 2π/n with n ∈ N √√ (e) 3 2−i 21.4. EXERCISES 267 2. Find a basis for each of the following field extensions. What is the degree of each extension? √ √ (a) Q( 3, 6 ) over Q √ √ (b) Q( 3 2, 3 3 ) over Q √ (c) Q( 2, i) over Q √ √ √ (d) Q( 3, 5, 7 ) over Q √ √ (e) Q( 2, 3 2 ) over Q √ √ (f) Q( 8 ) over Q( 2 ) √ √ (g) Q(i, 2 + i, 3 + i) over Q √ √ √ (h) Q( 2 + 5 ) over Q( 5 ) √ √ √ √ √ (i) Q( 2, 6 + 10 ) over Q( 3 + 5 ) 3. Find the splitting field for each of the following polynomials. (a) x4 − 10x2 + 21 over Q (c) x3 + 2x + 2 over Z3 (b) x4 + 1 over Q (d) x3 − 3 over Q √ 4. Consider the field extension Q( 4 3, i) over Q. √ √ (a) Find a basis for the field extension Q( 4 3, i) over Q. Conclude that [Q( 4 3, i) : Q] = 8. √ (b) Find all subfields F of Q( 4 3, i) such that [F : Q] = 2. √ (c) Find all subfields F of Q( 4 3, i) such that [F : Q] = 4. 5. Show that Z2 [x]/⟨x3 + x + 1⟩ is a field with eight elements. Construct a multiplication table for the multiplicative group of the field. 6. Show that the regular 9-gon is not constructible with a straightedge and compass, but that the regular 20-gon is constructible. 7. Prove that the cosine of one degree (cos 1◦ ) is algebraic over Q but not constructible. 8. Can a cube be constructed with three times the volume of a given cube? √ √ √ 9. Prove that Q( 3, 4 3, 8 3, . . .) is an algebraic extension of Q but not a finite extension. 10. Prove or disprove: π is algebraic over Q(π 3 ). 11. Let p(x) be a nonconstant polynomial of degree n in F [x]. Prove that there exists a splitting field E for p(x) such that [E : F ] ≤ n!. √ √ 12. Prove or disprove: Q( 2 ) ∼ = Q( 3 ). √ √ 13. Prove that the fields Q( 4 3 ) and Q( 4 3 i) are isomorphic but not equal. 14. Let K be an algebraic extension of E, and E an algebraic extension of F . Prove that K is algebraic over F . [Caution: Do not assume that the extensions are finite.] 15. Prove or disprove: Z[x]/⟨x3 − 2⟩ is a field. 16. Let F be a field of characteristic p. Prove that p(x) = xp − a either is irreducible over F or splits in F . 268 CHAPTER 21. FIELDS 17. Let E be the algebraic closure of a field F . Prove that every polynomial p(x) in F [x] splits in E. 18. If every irreducible polynomial p(x) in F [x] is linear, show that F is an algebraically closed field. 19. Prove that if α and β are constructible numbers such that β ̸= 0, then so is α/β. 20. Show that the set of all elements in R that are algebraic over Q form a field extension of Q that is not finite. 21. Let E be an algebraic extension of a field F , and let σ be an automorphism of E leaving F fixed. Let α ∈ E. Show that σ induces a permutation of the set of all zeros of the minimal polynomial of α that are in E. √ √ √ √ √ √ 22. Show√ that Q( 3, 7 ) = Q( 3 + 7 ). Extend your proof to show that Q( a, b ) = √ Q( a + b ), where gcd(a, b) = 1. 23. Let E be a finite extension of a field F . If [E : F ] = 2, show that E is a splitting field of F for some polynomial f (x) ∈ F [x]. 24. Prove or disprove: Given a polynomial p(x) in Z6 [x], it is possible to construct a ring R such that p(x) has a root in R. 25. Let E be a field extension of F and α ∈ E. Determine [F (α) : F (α3 )]. 26. Let α, β be transcendental over Q. Prove that either αβ or α+β is also transcendental. 27. Let E be an extension field of F and α ∈ E be transcendental over F . Prove that every element in F (α) that is not in F is also transcendental over F . 28. Let α be a root of an irreducible monic polynomial p(x) ∈ F [x], with deg p = n. Prove that [F (α) : F ] = n. References and Suggested Readings [1] Dean, R. A. Elements of Abstract Algebra. Wiley, New York, 1966. [2] Dudley, U. A Budget of Trisections. Springer-Verlag, New York, 1987. An interesting and entertaining account of how not to trisect an angle. [3] Fraleigh, J. B. A First Course in Abstract Algebra. 7th ed. Pearson, Upper Saddle River, NJ, 2003. [4] Kaplansky, I. Fields and Rings, 2nd ed. University of Chicago Press, Chicago, 1972. [5] Klein, F. Famous Problems of Elementary Geometry. Chelsea, New York, 1955. [6] Martin, G. Geometric Constructions. Springer, New York, 1998. [7] H. Pollard and H. G. Diamond. Theory of Algebraic Numbers, Dover, Mineola, NY, 2010. [8] Walker, E. A. Introduction to Abstract Algebra. Random House, New York, 1987. This work contains a proof showing that every field has an algebraic closure. 22 Finite Fields Finite fields appear in many applications of algebra, including coding theory and cryptog- raphy. We already know one finite field, Zp , where p is prime. In this chapter we will show that a unique finite field of order pn exists for every prime p, where n is a positive integer. Finite fields are also called Galois fields in honor of Évariste Galois, who was one of the first mathematicians to investigate them. 22.1 Structure of a Finite Field Recall that a field F has characteristic p if p is the smallest positive integer such that for every nonzero element α in F , we have pα = 0. If no such integer exists, then F has characteristic 0. From Theorem 16.19 we know that p must be prime. Suppose that F is a finite field with n elements. Then nα = 0 for all α in F . Consequently, the characteristic of F must be p, where p is a prime dividing n. This discussion is summarized in the following proposition. Proposition 22.1. If F is a finite field, then the characteristic of F is p, where p is prime. Throughout this chapter we will assume that p is a prime number unless otherwise stated. Proposition 22.2. If F is a finite field of characteristic p, then the order of F is pn for some n ∈ N. Proof. Let ϕ : Z → F be the ring homomorphism defined by ϕ(n) = n · 1. Since the characteristic of F is p, the kernel of ϕ must be pZ and the image of ϕ must be a subfield of F isomorphic to Zp . We will denote this subfield by K. Since F is a finite field, it must be a finite extension of K and, therefore, an algebraic extension of K. Suppose that [F : K] = n is the dimension of F , where F is a K vector space. There must exist elements α1 , . . . , αn ∈ F such that any element α in F can be written uniquely in the form α = a1 α1 + · · · + an αn , where the ai ’s are in K. Since there are p elements in K, there are pn possible linear combinations of the αi ’s. Therefore, the order of F must be pn . Lemma 22.3 Freshman’s Dream. Let p be prime and D be an integral domain of char- acteristic p. Then n n n ap + bp = (a + b)p for all positive integers n. 269 270 CHAPTER 22. FINITE FIELDS Proof. We will prove this lemma using mathematical induction on n. We can use the binomial formula (see Chapter 2, Example 2.4) to verify the case for n = 1; that is, ∑p ( ) p p k p−k (a + b) = a b . k k=0 If 0 < k < p, then ( ) p p! = k k!(p − k)! must be divisible by p, since p cannot divide k!(p − k)!. Note that D is an integral domain of characteristic p, so all but the first and last terms in the sum must be zero. Therefore, (a + b)p = ap + bp . Now suppose that the result holds for all k, where 1 ≤ k ≤ n. By the induction hypothesis, n+1 n n n n n+1 n+1 (a + b)p = ((a + b)p )p = (ap + bp )p = (ap )p + (bp )p = ap + bp . Therefore, the lemma is true for n + 1 and the proof is complete. Let F be a field. A polynomial f (x) ∈ F [x] of degree n is separable if it has n distinct roots in the splitting field of f (x); that is, f (x) is separable when it factors into distinct linear factors over the splitting field of f . An extension E of F is a separable extension of F if every element in E is the root of a separable polynomial in F [x]. √ √ polynomial x − 2 is separable over Q since it factors as (x − 2 )(x + Example 22.4. The 2 √ √ 2√). In fact, Q( 2 ) is a separable extension of Q. Let α = a + b 2 be any element in Q( 2 ). If b = 0, then α is a root of x − a. If b ̸= 0, then α is the root of the separable polynomial √ √ x2 − 2ax + a2 − 2b2 = (x − (a + b 2 ))(x − (a − b 2 )). Fortunately, we have an easy test to determine the separability of any polynomial. Let f (x) = a0 + a1 x + · · · + an xn be any polynomial in F [x]. Define the derivative of f (x) to be f ′ (x) = a1 + 2a2 x + · · · + nan xn−1 . Lemma 22.5. Let F be a field and f (x) ∈ F [x]. Then f (x) is separable if and only if f (x) and f ′ (x) are relatively prime. Proof. Let f (x) be separable. Then f (x) factors over some extension field of F as f (x) = (x − α1 )(x − α2 ) · · · (x − αn ), where αi ̸= αj for i ̸= j. Taking the derivative of f (x), we see that f ′ (x) = (x − α2 ) · · · (x − αn ) + (x − α1 )(x − α3 ) · · · (x − αn ) + · · · + (x − α1 ) · · · (x − αn−1 ). Hence, f (x) and f ′ (x) can have no common factors. To prove the converse, we will show that the contrapositive of the statement is true. Suppose that f (x) = (x − α)k g(x), where k > 1. Differentiating, we have f ′ (x) = k(x − α)k−1 g(x) + (x − α)k g ′ (x). Therefore, f (x) and f ′ (x) have a common factor. 22.1. STRUCTURE OF A FINITE FIELD 271 Theorem 22.6. For every prime p and every positive integer n, there exists a finite field F with pn elements. Furthermore, any field of order pn is isomorphic to the splitting field n of xp − x over Zp . n Proof. Let f (x) = xp − x and let F be the splitting field of f (x). Then by Lemma 22.5, f (x) has pn distinct zeros in F , since f ′ (x) = pn xp −1 − 1 = −1 is relatively prime to n f (x). We claim that the roots of f (x) form a subfield of F . Certainly 0 and 1 are zeros of f (x). If α and β are zeros of f (x), then α + β and αβ are also zeros of f (x), since n n n n n n αp + β p = (α + β)p and αp β p = (αβ)p . We also need to show that the additive inverse and the multiplicative inverse of each root of f (x) are roots of f (x). For any zero α of f (x), we know that −α is also a zero of f (x), since n n n f (−α) = (−α)p − (−α) = −αp + α = −(αp − α) = 0, provided p is odd. If p = 2, then n f (−α) = (−α)2 − (−α) = α + α = 0. If α ̸= 0, then (α−1 )p = (αp )−1 = α−1 . Since the zeros of f (x) form a subfield of F and n n f (x) splits in this subfield, the subfield must be all of F . Let E be any other field of order pn . To show that E is isomorphic to F , we must show that every element in E is a root of f (x). Certainly 0 is a root of f (x). Let α be a nonzero element of E. The order of the multiplicative group of nonzero elements of E is pn − 1; hence, αp −1 = 1 or αp − α = 0. Since E contains pn elements, E must be a splitting field n n of f (x); however, by Corollary 21.34, the splitting field of any polynomial is unique up to isomorphism. The unique finite field with pn elements is called the Galois field of order pn . We will denote this field by GF(pn ). Theorem 22.7. Every subfield of the Galois field GF(pn ) has pm elements, where m divides n. Conversely, if m | n for m > 0, then there exists a unique subfield of GF(pn ) isomorphic to GF(pm ). Proof. Let F be a subfield of E = GF(pn ). Then F must be a field extension of K that contains pm elements, where K is isomorphic to Zp . Then m | n, since [E : K] = [E : F ][F : K]. To prove the converse, suppose that m | n for some m > 0. Then pm − 1 divides pn − 1. Consequently, xp −1 − 1 divides xp −1 − 1. Therefore, xp − x must divide xp − x, and m n m n m n every zero of xp − x is also a zero of xp − x. Thus, GF(pn ) contains, as a subfield, a m splitting field of xp − x, which must be isomorphic to GF(pm ). Example 22.8. The lattice of subfields of GF(p24 ) is given in Figure 22.9. 272 CHAPTER 22. FINITE FIELDS GF(p24 ) GF(p8 ) GF(p12 ) GF(p4 ) GF(p6 ) GF(p2 ) GF(p3 ) GF(p) Figure 22.9: Subfields of GF(p24 ) With each field F we have a multiplicative group of nonzero elements of F which we will denote by F ∗ . The multiplicative group of any finite field is cyclic. This result follows from the more general result that we will prove in the next theorem. Theorem 22.10. If G is a finite subgroup of F ∗ , the multiplicative group of nonzero elements of a field F , then G is cyclic. Proof. Let G be a finite subgroup of F ∗ of order n. By the Fundamental Theorem of Finite Abelian Groups (Theorem 13.4), ∼ Z e1 × · · · × Z ek , G= p 1 p k where n = pe11 · · · pekk and the p1 , . . . , pk are (not necessarily distinct) primes. Let m be the least common multiple of pe11 , . . . , pekk . Then G contains an element of order m. Since every α in G satisfies xr − 1 for some r dividing m, α must also be a root of xm − 1. Since xm − 1 has at most m roots in F , n ≤ m. On the other hand, we know that m ≤ |G|; therefore, m = n. Thus, G contains an element of order n and must be cyclic. Corollary 22.11. The multiplicative group of all nonzero elements of a finite field is cyclic. Corollary 22.12. Every finite extension E of a finite field F is a simple extension of F . Proof. Let α be a generator for the cyclic group E ∗ of nonzero elements of E. Then E = F (α). Example 22.13. The finite field GF(24 ) is isomorphic to the field Z2 /⟨1 + x + x4 ⟩. There- fore, the elements of GF(24 ) can be taken to be {a0 + a1 α + a2 α2 + a3 α3 : ai ∈ Z2 and 1 + α + α4 = 0}. Remembering that 1 + α + α4 = 0, we add and multiply elements of GF(24 ) exactly as we add and multiply polynomials. The multiplicative group of GF(24 ) is isomorphic to Z15 with generator α: α1 = α α6 = α2 + α3 α11 = α + α2 + α3 α2 = α2 α7 = 1 + α + α3 α12 = 1 + α + α2 + α3 α3 = α3 α8 = 1 + α2 α13 = 1 + α2 + α3 α4 = 1 + α α9 = α + α3 α14 = 1 + α3 α5 = α + α2 α10 = 1 + α + α2 α15 = 1. 22.2. POLYNOMIAL CODES 273 22.2 Polynomial Codes With knowledge of polynomial rings and finite fields, it is now possible to derive more sophisticated codes than those of Chapter 8. First let us recall that an (n, k)-block code consists of a one-to-one encoding function E : Zk2 → Zn2 and a decoding function D : Zn2 → Zk2 . The code is error-correcting if D is onto. A code is a linear code if it is the null space of a matrix H ∈ Mk×n (Z2 ). We are interested in a class of codes known as cyclic codes. Let ϕ : Zk2 → Zn2 be a binary (n, k)-block code. Then ϕ is a cyclic code if for every codeword (a1 , a2 , . . . , an ), the cyclically shifted n-tuple (an , a1 , a2 , . . . , an−1 ) is also a codeword. Cyclic codes are particularly easy to implement on a computer using shift registers [2, 3]. Example 22.14. Consider the (6, 3)-linear codes generated by the two matrices 1 0 0 1 0 0 0 0 1 0 1 1 0 0 1 1 1 1 G1 = and G2 = . 1 0 0 1 1 1 0 1 0 0 1 1 0 0 1 0 0 1 Messages in the first code are encoded as follows: (000) 7→ (000000) (100) 7→ (100100) (001) 7 → (001001) (101) 7 → (101101) (010) 7 → (010010) (110) 7 → (110110) (011) 7 → (011011) (111) 7 → (111111). It is easy to see that the codewords form a cyclic code. In the second code, 3-tuples are encoded in the following manner: (000) 7→ (000000) (100) 7→ (111100) (001) 7 → (001111) (101) 7 → (110011) (010) 7 → (011110) (110) 7 → (100010) (011) 7 → (010001) (111) 7 → (101101). This code cannot be cyclic, since (101101) is a codeword but (011011) is not a codeword. Polynomial Codes We would like to find an easy method of obtaining cyclic linear codes. To accomplish this, we can use our knowledge of finite fields and polynomial rings over Z2 . Any binary n-tuple can be interpreted as a polynomial in Z2 [x]. Stated another way, the n-tuple (a0 , a1 , . . . , an−1 ) corresponds to the polynomial f (x) = a0 + a1 x + · · · + an−1 xn−1 , where the degree of f (x) is at most n − 1. For example, the polynomial corresponding to the 5-tuple (10011) is 1 + 0x + 0x2 + 1x3 + 1x4 = 1 + x3 + x4 . 274 CHAPTER 22. FINITE FIELDS Conversely, with any polynomial f (x) ∈ Z2 [x] with deg f (x) < n we can associate a binary n-tuple. The polynomial x + x2 + x4 corresponds to the 5-tuple (01101). Let us fix a nonconstant polynomial g(x) in Z2 [x] of degree n − k. We can define an (n, k)-code C in the following manner. If (a0 , . . . , ak−1 ) is a k-tuple to be encoded, then f (x) = a0 + a1 x + · · · + ak−1 xk−1 is the corresponding polynomial in Z2 [x]. To encode f (x), we multiply by g(x). The codewords in C are all those polynomials in Z2 [x] of degree less than n that are divisible by g(x). Codes obtained in this manner are called polynomial codes. Example 22.15. If we let g(x) = 1+x3 , we can define a (6, 3)-code C as follows. To encode a 3-tuple (a0 , a1 , a2 ), we multiply the corresponding polynomial f (x) = a0 + a1 x + a2 x2 by 1 + x3 . We are defining a map ϕ : Z32 → Z62 by ϕ : f (x) 7→ g(x)f (x). It is easy to check that this map is a group homomorphism. In fact, if we regard Zn2 as a vector space over Z2 , ϕ is a linear transformation of vector spaces (see Exercise 20.4.15, Chapter 20). Let us compute the kernel of ϕ. Observe that ϕ(a0 , a1 , a2 ) = (000000) exactly when 0 + 0x + 0x2 + 0x3 + 0x4 + 0x5 = (1 + x3 )(a0 + a1 x + a2 x2 ) = a0 + a1 x + a2 x2 + a0 x3 + a1 x4 + a2 x5 . Since the polynomials over a field form an integral domain, a0 + a1 x + a2 x2 must be the zero polynomial. Therefore, ker ϕ = {(000)} and ϕ is one-to-one. To calculate a generator matrix for C, we merely need to examine the way the polyno- mials 1, x, and x2 are encoded: (1 + x3 ) · 1 = 1 + x3 (1 + x3 )x = x + x4 (1 + x3 )x2 = x2 + x5 . We obtain the code corresponding to the generator matrix G1 in Example 22.14. The parity-check matrix for this code is 1 0 0 1 0 0 H = 0 1 0 0 1 0 . 0 0 1 0 0 1 Since the smallest weight of any nonzero codeword is 2, this code has the ability to detect all single errors. Rings of polynomials have a great deal of structure; therefore, our immediate goal is to establish a link between polynomial codes and ring theory. Recall that xn − 1 = (x − 1)(xn−1 + · · · + x + 1). The factor ring Rn = Z2 [x]/⟨xn − 1⟩ can be considered to be the ring of polynomials of the form f (t) = a0 + a1 t + · · · + an−1 tn−1 that satisfy the condition tn = 1. It is an easy exercise to show that Zn2 and Rn are isomor- phic as vector spaces. We will often identify elements in Zn2 with elements in Z[x]/⟨xn − 1⟩. In this manner we can interpret a linear code as a subset of Z[x]/⟨xn − 1⟩. The additional ring structure on polynomial codes is very powerful in describing cyclic codes. A cyclic shift of an n-tuple can be described by polynomial multiplication. If f (t) = a0 + a1 t + · · · + an−1 tn−1 is a code polynomial in Rn , then tf (t) = an−1 + a0 t + · · · + an−2 tn−1 22.2. POLYNOMIAL CODES 275 is the cyclically shifted word obtained from multiplying f (t) by t. The following theorem gives a beautiful classification of cyclic codes in terms of the ideals of Rn . Theorem 22.16. A linear code C in Zn2 is cyclic if and only if it is an ideal in Rn = Z[x]/⟨xn − 1⟩. Proof. Let C be a linear cyclic code and suppose that f (t) is in C. Then tf (t) must also be in C. Consequently, tk f (t) is in C for all k ∈ N. Since C is a linear code, any linear combination of the codewords f (t), tf (t), t2 f (t), . . . , tn−1 f (t) is also a codeword; therefore, for every polynomial p(t), p(t)f (t) is in C. Hence, C is an ideal. Conversely, let C be an ideal in Z2 [x]/⟨xn + 1⟩. Suppose that f (t) = a0 + a1 t + · · · + an−1 tn−1 is a codeword in C. Then tf (t) is a codeword in C; that is, (a1 , . . . , an−1 , a0 ) is in C. Theorem 22.16 tells us that knowing the ideals of Rn is equivalent to knowing the linear cyclic codes in Zn2 . Fortunately, the ideals in Rn are easy to describe. The natural ring homomorphism ϕ : Z2 [x] → Rn defined by ϕ[f (x)] = f (t) is a surjective homomorphism. The kernel of ϕ is the ideal generated by xn − 1. By Theorem 16.34, every ideal C in Rn is of the form ϕ(I), where I is an ideal in Z2 [x] that contains ⟨xn − 1⟩. By Theorem 17.20, we know that every ideal I in Z2 [x] is a principal ideal, since Z2 is a field. Therefore, I = ⟨g(x)⟩ for some unique monic polynomial in Z2 [x]. Since ⟨xn − 1⟩ is contained in I, it must be the case that g(x) divides xn − 1. Consequently, every ideal C in Rn is of the form C = ⟨g(t)⟩ = {f (t)g(t) : f (t) ∈ Rn and g(x) | (xn − 1) in Z2 [x]}. The unique monic polynomial of the smallest degree that generates C is called the minimal generator polynomial of C. Example 22.17. If we factor x7 − 1 into irreducible components, we have x7 − 1 = (1 + x)(1 + x + x3 )(1 + x2 + x3 ). We see that g(t) = (1 + t + t3 ) generates an ideal C in R7 . This code is a (7, 4)-block code. As in Example 22.15, it is easy to calculate a generator matrix by examining what g(t) does to the polynomials 1, t, t2 , and t3 . A generator matrix for C is 1 0 0 0 1 1 0 0 0 1 1 0 G = 1 0 1 1 . 0 1 0 1 0 0 1 0 0 0 0 1 In general, we can determine a generator matrix for an (n, k)-code C by the manner in which the elements tk are encoded. Let xn − 1 = g(x)h(x) in Z2 [x]. If g(x) = g0 + g1 x + · · · + gn−k xn−k and h(x) = h0 + h1 x + · · · + hk xk , then the n × k matrix g0 0 ··· 0 g1 g0 ··· 0 . .. .. .. .. . . . G = gn−k gn−k−1 · · · g0 0 gn−k · · · g1 .. .. .. .. . . . . 0 0 · · · gn−k 276 CHAPTER 22. FINITE FIELDS is a generator matrix for the code C with generator polynomial g(t). The parity-check matrix for C is the (n − k) × n matrix 0 ··· 0 0 hk · · · h0 0 · · · 0 hk · · · h0 0 H= . · · · · · · · · · · · · · · · · · · · · · hk · · · h0 0 0 ··· 0 We will leave the details of the proof of the following proposition as an exercise. Proposition 22.18. Let C = ⟨g(t)⟩ be a cyclic code in Rn and suppose that xn − 1 = g(x)h(x). Then G and H are generator and parity-check matrices for C, respectively. Furthermore, HG = 0. Example 22.19. In Example 22.17, x7 − 1 = g(x)h(x) = (1 + x + x3 )(1 + x + x2 + x4 ). Therefore, a parity-check matrix for this code is 0 0 1 0 1 1 1 H = 0 1 0 1 1 1 0 . 1 0 1 1 1 0 0 To determine the error-detecting and error-correcting capabilities of a cyclic code, we need to know something about determinants. If α1 , . . . , αn are elements in a field F , then the n × n matrix 1 1 ··· 1 α1 α2 · · · αn 2 α1 α22 · · · αn2 .. .. .. .. . . . . α1n−1 α2n−1 · · · αnn−1 is called the Vandermonde matrix. The determinant of this matrix is called the Van- dermonde determinant. We will need the following lemma in our investigation of cyclic codes. Lemma 22.20. Let α1 , . . . , αn be elements in a field F with n ≥ 2. Then 1 1 ··· 1 α1 α2 · · · αn 2 ∏ det 1 α α22 · · · αn2 = (αi − αj ). .. .. .. .. 1≤j<i≤n . . . . α1n−1 n−1 α2 · · · αnn−1 In particular, if the αi ’s are distinct, then the determinant is nonzero. Proof. We will induct on n. If n = 2, then the determinant is α2 − α1 . Let us assume the result for n − 1 and consider the polynomial p(x) defined by 1 1 ··· 1 1 α1 α2 · · · αn−1 x 2 p(x) = det α22 · · · αn−1 x2 . α 2 1 .. .. .. .. .. . . . . . α1n−1 α2n−1 · · · αn−1 n−1 xn−1 22.2. POLYNOMIAL CODES 277 Expanding this determinant by cofactors on the last column, we see that p(x) is a polynomial of at most degree n − 1. Moreover, the roots of p(x) are α1 , . . . , αn−1 , since the substitution of any one of these elements in the last column will produce a column identical to the last column in the matrix. Remember that the determinant of a matrix is zero if it has two identical columns. Therefore, p(x) = (x − α1 )(x − α2 ) · · · (x − αn−1 )β, where 1 1 ··· 1 α1 α2 · · · αn−1 det α12 α22 · · · αn−1 . n+n 2 β = (−1) .. .. .. .. . . . . α1n−2 α2n−2 · · · αn−1 n−2 By our induction hypothesis, ∏ β = (−1)n+n (αi − αj ). 1≤j<i≤n−1 If we let x = αn , the result now follows immediately. The following theorem gives us an estimate on the error detection and correction capa- bilities for a particular generator polynomial. Theorem 22.21. Let C = ⟨g(t)⟩ be a cyclic code in Rn and suppose that ω is a primitive nth root of unity over Z2 . If s consecutive powers of ω are roots of g(x), then the minimum distance of C is at least s + 1. Proof. Suppose that g(ω r ) = g(ω r+1 ) = · · · = g(ω r+s−1 ) = 0. Let f (x) be some polynomial in C with s or fewer nonzero coefficients. We can assume that f (x) = ai0 xi0 + ai1 xi1 + · · · + ais−1 xis−1 be some polynomial in C. It will suffice to show that all of the ai ’s must be 0. Since g(ω r ) = g(ω r+1 ) = · · · = g(ω r+s−1 ) = 0 and g(x) divides f (x), f (ω r ) = f (ω r+1 ) = · · · = f (ω r+s−1 ) = 0. Equivalently, we have the following system of equations: ai0 (ω r )i0 + ai1 (ω r )i1 + · · · + ais−1 (ω r )is−1 = 0 ai0 (ω r+1 )i0 + ai1 (ω r+1 )i2 + · · · + ais−1 (ω r+1 )is−1 = 0 .. . ai0 (ω r+s−1 )i0 + ai1 (ω r+s−1 )i1 + · · · + ais−1 (ω r+s−1 )is−1 = 0. Therefore, (ai0 , ai1 , . . . , ais−1 ) is a solution to the homogeneous system of linear equations (ω i0 )r x0 + (ω i1 )r x1 + · · · + (ω is−1 )r xn−1 = 0 278 CHAPTER 22. FINITE FIELDS (ω i0 )r+1 x0 + (ω i1 )r+1 x1 + · · · + (ω is−1 )r+1 xn−1 = 0 .. . (ω i0 )r+s−1 x0 + (ω i1 )r+s−1 x1 + · · · + (ω is−1 )r+s−1 xn−1 = 0. However, this system has a unique solution, since the determinant of the matrix (ω i0 )r (ω i1 )r ··· (ω is−1 )r (ω i0 )r+1 (ω i1 )r+1 ··· (ω is−1 )r+1 .. .. .. .. . . . . (ω i0 )r+s−1 (ω i1 )r+s−1 · · · (ω is−1 )r+s−1 can be shown to be nonzero using Lemma 22.20 and the basic properties of determinants (Exercise). Therefore, this solution must be ai0 = ai1 = · · · = ais−1 = 0. BCH Codes Some of the most important codes, discovered independently by A. Hocquenghem in 1959 and by R. C. Bose and D. V. Ray-Chaudhuri in 1960, are bch codes. The European and transatlantic communication systems both use bch codes. Information words to be encoded are of length 231, and a polynomial of degree 24 is used to generate the code. Since 231 + 24 = 255 = 28 − 1, we are dealing with a (255, 231)-block code. This bch code will detect six errors and has a failure rate of 1 in 16 million. One advantage of bch codes is that efficient error correction algorithms exist for them. The idea behind bch codes is to choose a generator polynomial of smallest degree that has the largest error detection and error correction capabilities. Let d = 2r + 1 for some r ≥ 0. Suppose that ω is a primitive nth root of unity over Z2 , and let mi (x) be the minimal polynomial over Z2 of ω i . If g(x) = lcm[m1 (x), m2 (x), . . . , m2r (x)], then the cyclic code ⟨g(t)⟩ in Rn is called the bch code of length n and distance d. By Theorem 22.21, the minimum distance of C is at least d. Theorem 22.22. Let C = ⟨g(t)⟩ be a cyclic code in Rn . The following statements are equivalent. 1. The code C is a bch code whose minimum distance is at least d. 2. A code polynomial f (t) is in C if and only if f (ω i ) = 0 for 1 ≤ i < d. 3. The matrix 1 ω ω2 ··· ω n−1 1 ω2 ω4 ··· ω (n−1)(2) H= 1 ω3 ω6 ··· ω (n−1)(3) .. .. .. .. .. . . . . . 1 ω 2r ω 4r · · · ω (n−1)(2r) is a parity-check matrix for C. Proof. (1) ⇒ (2). If f (t) is in C, then g(x) | f (x) in Z2 [x]. Hence, for i = 1, . . . , 2r, f (ω i ) = 0 since g(ω i ) = 0. Conversely, suppose that f (ω i ) = 0 for 1 ≤ i ≤ d. Then f (x) is 22.3. EXERCISES 279 divisible by each mi (x), since mi (x) is the minimal polynomial of ω i . Therefore, g(x) | f (x) by the definition of g(x). Consequently, f (x) is a codeword. (2) ⇒ (3). Let f (t) = a0 + a1 t + · · · + an−1 vtn−1 be in Rn . The corresponding n-tuple in Zn2 is x = (a0 a1 · · · an−1 )t . By (2), a0 + a1 ω + · · · + an−1 ω n−1 f (ω) a0 + a1 ω 2 + · · · + an−1 (ω 2 )n−1 f (ω 2 ) Hx = .. = . =0 . .. a0 + a1 ω 2r + · · · + an−1 (ω 2r )n−1 f (ω 2r ) exactly when f (t) is in C. Thus, H is a parity-check matrix for C. (3) ⇒ (1). By (3), a code polynomial f (t) = a0 +a1 t+· · ·+an−1 tn−1 is in C exactly when f (ω i ) = 0 for i = 1, . . . , 2r. The smallest such polynomial is g(t) = lcm[m1 (t), . . . , m2r (t)]. Therefore, C = ⟨g(t)⟩. Example 22.23. It is easy to verify that x15 − 1 ∈ Z2 [x] has a factorization x15 − 1 = (x + 1)(x2 + x + 1)(x4 + x + 1)(x4 + x3 + 1)(x4 + x3 + x2 + x + 1), where each of the factors is an irreducible polynomial. Let ω be a root of 1 + x + x4 . The Galois field GF(24 ) is {a0 + a1 ω + a2 ω 2 + a3 ω 3 : ai ∈ Z2 and 1 + ω + ω 4 = 0}. By Example 22.8, ω is a primitive 15th root of unity. The minimal polynomial of ω is m1 (x) = 1 + x + x4 . It is easy to see that ω 2 and ω 4 are also roots of m1 (x). The minimal polynomial of ω 3 is m2 (x) = 1 + x + x2 + x3 + x4 . Therefore, g(x) = m1 (x)m2 (x) = 1 + x4 + x6 + x7 + x8 has roots ω, ω 2 , ω 3 , ω 4 . Since both m1 (x) and m2 (x) divide x15 − 1, the bch code is a (15, 7)-code. If x15 − 1 = g(x)h(x), then h(x) = 1 + x4 + x6 + x7 ; therefore, a parity-check matrix for this code is 0 0 0 0 0 0 0 1 1 0 1 0 0 0 1 0 0 0 0 0 0 1 1 0 1 0 0 0 1 0 0 0 0 0 0 1 1 0 1 0 0 0 1 0 0 0 0 0 0 1 1 0 1 0 0 0 1 0 0 0 . 0 0 0 1 1 0 1 0 0 0 1 0 0 0 0 0 0 1 1 0 1 0 0 0 1 0 0 0 0 0 0 1 1 0 1 0 0 0 1 0 0 0 0 0 0 1 1 0 1 0 0 0 1 0 0 0 0 0 0 0 Sage Finite fields are important in a variety of applied disciplines, such as cryptography and coding theory (see introductions to these topics in other chapters). Sage has excellent support for finite fields allowing for a wide variety of computations. 22.3 Exercises 1. Calculate each of the following. 280 CHAPTER 22. FINITE FIELDS (a) [GF(36 ) : GF(33 )] (c) [GF(625) : GF(25)] (b) [GF(128) : GF(16)] (d) [GF(p12 ) : GF(p2 )] 2. Calculate [GF(pm ) : GF(pn )], where n | m. 3. What is the lattice of subfields for GF(p30 )? 4. Let α be a zero of x3 + x2 + 1 over Z2 . Construct a finite field of order 8. Show that x3 + x2 + 1 splits in Z2 (α). 5. Construct a finite field of order 27. 6. Prove or disprove: Q∗ is cyclic. 7. Factor each of the following polynomials in Z2 [x]. (a) x5 − 1 (c) x9 − 1 (b) x6 + x5 + x4 + x3 + x2 + x + 1 (d) x4 + x3 + x2 + x + 1 8. Prove or disprove: Z2 [x]/⟨x3 + x + 1⟩ ∼ = Z2 [x]/⟨x3 + x2 + 1⟩. 9. Determine the number of cyclic codes of length n for n = 6, 7, 8, 10. 10. Prove that the ideal ⟨t + 1⟩ in Rn is the code in Zn2 consisting of all words of even parity. 11. Construct all bch codes of (a) length 7. (b) length 15. 12. Prove or disprove: There exists a finite field that is algebraically closed. 13. Let p be prime. Prove that the field of rational functions Zp (x) is an infinite field of characteristic p. n n n 14. Let D be an integral domain of characteristic p. Prove that (a − b)p = ap − bp for all a, b ∈ D. 15. Show that every element in a finite field can be written as the sum of two squares. 16. Let E and F be subfields of a finite field K. If E is isomorphic to F , show that E = F. 17. Let F ⊂ E ⊂ K be fields. If K is a separable extension of F , show that K is also separable extension of E. 18. Let E be an extension of a finite field F , where F has q elements. Let α ∈ E be algebraic over F of degree n. Prove that F (α) has q n elements. 19. Show that every finite extension of a finite field F is simple; that is, if E is a finite extension of a finite field F , prove that there exists an α ∈ E such that E = F (α). 20. Show that for every n there exists an irreducible polynomial of degree n in Zp [x]. 21. Prove that the Frobenius map Φ : GF(pn ) → GF(pn ) given by Φ : α 7→ αp is an automorphism of order n. 22. Show that every element in GF(pn ) can be written in the form ap for some unique a ∈ GF(pn ). 23. Let E and F be subfields of GF(pn ). If |E| = pr and |F | = ps , what is the order of E ∩ F? 24. Wilson’s Theorem. Let p be prime. Prove that (p − 1)! ≡ −1 (mod p). 22.4. ADDITIONAL EXERCISES: ERROR CORRECTION FOR BCH CODES 281 25. If g(t) is the minimal generator polynomial for a cyclic code C in Rn , prove that the constant term of g(x) is 1. 26. Often it is conceivable that a burst of errors might occur during transmission, as in the case of a power surge. Such a momentary burst of interference might alter several consecutive bits in a codeword. Cyclic codes permit the detection of such error bursts. Let C be an (n, k)-cyclic code. Prove that any error burst up to n − k digits can be detected. 27. Prove that the rings Rn and Zn2 are isomorphic as vector spaces. 28. Let C be a code in Rn that is generated by g(t). If ⟨f (t)⟩ is another code in Rn , show that ⟨g(t)⟩ ⊂ ⟨f (t)⟩ if and only if f (x) divides g(x) in Z2 [x]. 29. Let C = ⟨g(t)⟩ be a cyclic code in Rn and suppose that xn − 1 = g(x)h(x), where g(x) = g0 + g1 x + · · · + gn−k xn−k and h(x) = h0 + h1 x + · · · + hk xk . Define G to be the n × k matrix g0 0 ··· 0 g1 g0 ··· 0 . .. .. .. .. . . . G = gn−k gn−k−1 · · · g0 0 gn−k · · · g1 .. .. .. .. . . . . 0 0 · · · gn−k and H to be the (n − k) × n matrix 0 ··· 0 0 hk · · · h0 0 · · · 0 hk · · · h0 0 H= . · · · · · · · · · · · · · · · · · · · · · hk · · · h0 0 0 ··· 0 (a) Prove that G is a generator matrix for C. (b) Prove that H is a parity-check matrix for C. (c) Show that HG = 0. 22.4 Additional Exercises: Error Correction for BCH Codes bch codes have very attractive error correction algorithms. Let C be a bch code in Rn , and suppose that a code polynomial c(t) = c0 + c1 t + · · · + cn−1 tn−1 is transmitted. Let w(t) = w0 + w1 t + · · · wn−1 tn−1 be the polynomial in Rn that is received. If errors have occurred in bits a1 , . . . , ak , then w(t) = c(t) + e(t), where e(t) = ta1 + ta2 + · · · + tak is the error polynomial. The decoder must determine the integers ai and then recover c(t) from w(t) by flipping the ai th bit. From w(t) we can compute w(ω i ) = si for i = 1, . . . , 2r, where ω is a primitive nth root of unity over Z2 . We say the syndrome of w(t) is s1 , . . . , s2r .1. Show that w(t) is a code polynomial if and only if si = 0 for all i. 2. Show that si = w(ω i ) = e(ω i ) = ω ia1 + ω ia2 + · · · + ω iak for i = 1, . . . , 2r. The error-locator polynomial is defined to be s(x) = (x + ω a1 )(x + ω a2 ) · · · (x + ω ak ). 282 CHAPTER 22. FINITE FIELDS 3. Recall the (15, 7)-block bch code in Example 22.19. By Theorem 8.13, this code is capable of correcting two errors. Suppose that these errors occur in bits a1 and a2 . The error-locator polynomial is s(x) = (x + ω a1 )(x + ω a2 ). Show that ( ) 2 2 s3 s(x) = x + s1 x + s1 + . s1 4. Let w(t) = 1 + t2 + t4 + t5 + t7 + t12 + t13 . Determine what the originally transmitted code polynomial was. References and Suggested Readings [1] Childs, L. A Concrete Introduction to Higher Algebra. 2nd ed. Springer-Verlag, New York, 1995. [2] Gåding, L. and Tambour, T. Algebra for Computer Science. Springer-Verlag, New York, 1988. [3] Lidl, R. and Pilz, G. Applied Abstract Algebra. 2nd ed. Springer, New York, 1998. An excellent presentation of finite fields and their applications. [4] Mackiw, G. Applications of Abstract Algebra. Wiley, New York, 1985. [5] Roman, S. Coding and Information Theory. Springer-Verlag, New York, 1992. [6] van Lint, J. H. Introduction to Coding Theory. Springer, New York, 1999. 23 Galois Theory A classic problem of algebra is to find the solutions of a polynomial equation. The solution to the quadratic equation was known in antiquity. Italian mathematicians found general solutions to the general cubic and quartic equations in the sixteenth century; however, attempts to solve the general fifth-degree, or quintic, polynomial were repulsed for the next three hundred years. Certainly, equations such as x5 − 1 = 0 or x6 − x3 − 6 = 0 could be solved, but no solution like the quadratic formula was found for the general quintic, ax5 + bx4 + cx3 + dx2 + ex + f = 0. Finally, at the beginning of the nineteenth century, Ruffini and Abel both found quintics that could not be solved with any formula. It was Galois, however, who provided the full explanation by showing which polynomials could and could not be solved by formulas. He discovered the connection between groups and field extensions. Galois theory demonstrates the strong interdependence of group and field theory, and has had far-reaching implications beyond its original purpose. In this chapter we will prove the Fundamental Theorem of Galois Theory. This result will be used to establish the insolvability of the quintic and to prove the Fundamental Theorem of Algebra. 23.1 Field Automorphisms Our first task is to establish a link between group theory and field theory by examining automorphisms of fields. Proposition 23.1. The set of all automorphisms of a field F is a group under composition of functions. Proof. If σ and τ are automorphisms of F , then so are στ and σ −1 . The identity is certainly an automorphism; hence, the set of all automorphisms of a field F is indeed a group. Proposition 23.2. Let E be a field extension of F . Then the set of all automorphisms of E that fix F elementwise is a group; that is, the set of all automorphisms σ : E → E such that σ(α) = α for all α ∈ F is a group. Proof. We need only show that the set of automorphisms of E that fix F elementwise is a subgroup of the group of all automorphisms of E. Let σ and τ be two automorphisms of E such that σ(α) = α and τ (α) = α for all α ∈ F . Then στ (α) = σ(α) = α and σ −1 (α) = α. Since the identity fixes every element of E, the set of automorphisms of E that leave elements of F fixed is a subgroup of the entire group of automorphisms of E. 283 284 CHAPTER 23. GALOIS THEORY Let E be a field extension of F . We will denote the full group of automorphisms of E by Aut(E). We define the Galois group of E over F to be the group of automorphisms of E that fix F elementwise; that is, G(E/F ) = {σ ∈ Aut(E) : σ(α) = α for all α ∈ F }. If f (x) is a polynomial in F [x] and E is the splitting field of f (x) over F , then we define the Galois group of f (x) to be G(E/F ). Example 23.3. Complex conjugation, defined by σ : a + bi 7→ a − bi, is an automorphism of the complex numbers. Since σ(a) = σ(a + 0i) = a − 0i = a, the automorphism defined by complex conjugation must be in G(C/R). √ √ √ √ Example 23.4. Consider the fields Q ⊂ Q( 5 ) ⊂ Q( 3, 5 ). Then for a, b ∈ Q( 5 ), √ √ σ(a + b 3 ) = a − b 3 √ √ √ is an automorphism of Q( 3, 5 ) leaving Q( 5 ) fixed. Similarly, √ √ τ (a + b 5 ) = a − b 5 √ √ √ is an automorphism √ √ of Q( 3, 5 ) leaving Q( 3 ) fixed. The automorphism µ = στ √ moves √ both 3 and 5. It will soon be clear that {id, σ, τ, µ} is the Galois group of Q( 3, 5 ) over Q. The following table shows that this group is isomorphic to Z2 × Z2 . id σ τ µ id id σ τ µ σ σ id µ τ τ τ µ id σ µ µ τ σ id √ √ √ √ √ We may also regard the field Q( √3, √5 ) as a vector √ √ over Q that has basis {1, 3, 5, 15 }. space It is no coincidence that |G(Q( 3, 5 )/Q)| = [Q( 3, 5 ) : Q)] = 4. Proposition 23.5. Let E be a field extension of F and f (x) be a polynomial in F [x]. Then any automorphism in G(E/F ) defines a permutation of the roots of f (x) that lie in E. Proof. Let f (x) = a0 + a1 x + a2 x2 + · · · + an xn and suppose that α ∈ E is a zero of f (x). Then for σ ∈ G(E/F ), 0 = σ(0) = σ(f (α)) = σ(a0 + a1 α + a2 α2 + · · · + an αn ) = a0 + a1 σ(α) + a2 [σ(α)]2 + · · · + an [σ(α)]n ; therefore, σ(α) is also a zero of f (x). Let E be an algebraic extension of a field F . Two elements α, β ∈ E are√conjugate over √ the same minimal polynomial. For example, in the field Q( 2 ) the elements √ if they have F 2 and − 2 are conjugate over Q since they are both roots of the irreducible polynomial x2 − 2. A converse of the last proposition exists. The proof follows directly from Lemma 21.32. 23.1. FIELD AUTOMORPHISMS 285 Proposition 23.6. If α and β are conjugate over F , there exists an isomorphism σ : F (α) → F (β) such that σ is the identity when restricted to F . Theorem 23.7. Let f (x) be a polynomial in F [x] and suppose that E is the splitting field for f (x) over F . If f (x) has no repeated roots, then |G(E/F )| = [E : F ]. Proof. We will use mathematical induction on the degree of f (x). If the degree of f (x) is 0 or 1, then E = F and there is nothing to show. Assume that the result holds for all polynomials of degree k with 0 ≤ k < n. Suppose that the degree of f (x) is n. Let p(x) be an irreducible factor of f (x) of degree r. Since all of the roots of p(x) are in E, we can choose one of these roots, say α, so that F ⊂ F (α) ⊂ E. Then [E : F (α)] = n/r and [F (α) : F ] = r. If β is any other root of p(x), then F ⊂ F (β) ⊂ E. By Lemma 21.32, there exists a unique isomorphism σ : F (α) → F (β) for each such β that fixes F elementwise. Since E is a splitting field of p(x), there are exactly r such isomorphisms. For each of these automorphisms, we can use our induction hypothesis on [E : F (α)] = n/r < n to conclude that |G(E/F (α))| = [E : F (α)]. Consequently, there are [E : F ] = [E : F (α)][F (α) : F ] = n possible automorphisms of E that fix F , or |G(E/F )| = [E : F ]. Corollary 23.8. Let F be a finite field with a finite extension E such that [E : F ] = k. Then G(E/F ) is cyclic of order k. Proof. Let p be the characteristic of E and F and assume that the orders of E and F are pm and pn , respectively. Then nk = m. We can also assume that E is the splitting m field of xp − x over a subfield of order p. Therefore, E must also be the splitting field of m xp − x over F . Applying Theorem 23.7, we find that |G(E/F )| = k. To prove that G(E/F ) is cyclic, we must find a generator for G(E/F ). Let σ : E → E n be defined by σ(α) = αp . We claim that σ is the element in G(E/F ) that we are seeking. We first need to show that σ is in Aut(E). If α and β are in E, n n n σ(α + β) = (α + β)p = αp + β p = σ(α) + σ(β) by Lemma 22.3. Also, it is easy to show that σ(αβ) = σ(α)σ(β). Since σ is a nonzero homomorphism of fields, it must be injective. It must also be onto, since E is a finite field. n We know that σ must be in G(E/F ), since F is the splitting field of xp − x over the base field of order p. This means that σ leaves every element in F fixed. Finally, we must show that the order of σ is k. By Theorem 23.7, we know that nk m σ k (α) = αp = αp = α is the identity of G(E/F ). However, σ r cannot be the identity for 1 ≤ r < k; otherwise, nr xp − x would have pm roots, which is impossible. √ √ Example 23.9. We can now confirm that the Galois group of Q( 3, 5 ) over Q in Exam- ple 23.4 √ is indeed √ isomorphic to Z2 × Z2 . Certainly the√ √ H = {id, σ, τ, µ} is a subgroup group of G(Q( 3, 5 )/Q); however, H must be all of G(Q( 3, 5 )/Q), since √ √ √ √ |H| = [Q( 3, 5 ) : Q] = |G(Q( 3, 5 )/Q)| = 4. 286 CHAPTER 23. GALOIS THEORY Example 23.10. Let us compute the Galois group of f (x) = x4 + x3 + x2 + x + 1 over Q. We know that f (x) is irreducible by Exercise 17.4.20 in Chapter 17. Furthermore, since (x − 1)f (x) = x5 − 1, we can use DeMoivre’s Theorem to determine that the roots of f (x) are ω i , where i = 1, . . . , 4 and ω = cos(2π/5) + i sin(2π/5). Hence, the splitting field of f (x) must be Q(ω). We can define automorphisms σi of Q(ω) by σi (ω) = ω i for i = 1, . . . , 4. It is easy to check that these are indeed distinct automorphisms in G(Q(ω)/Q). Since [Q(ω) : Q] = |G(Q(ω)/Q)| = 4, the σi ’s must be all of G(Q(ω)/Q). Therefore, G(Q(ω)/Q) ∼ = Z4 since ω is a generator for the Galois group. Separable Extensions Many of the results that we have just proven depend on the fact that a polynomial f (x) in F [x] has no repeated roots in its splitting field. It is evident that we need to know exactly when a polynomial factors into distinct linear factors in its splitting field. Let E be the splitting field of a polynomial f (x) in F [x]. Suppose that f (x) factors over E as ∏ r f (x) = (x − α1 )n1 (x − α2 )n2 · · · (x − αr )nr = (x − αi )ni . i=1 We define the multiplicity of a root αi of f (x) to be ni . A root with multiplicity 1 is called a simple root. Recall that a polynomial f (x) ∈ F [x] of degree n is separable if it has n distinct roots in its splitting field E. Equivalently, f (x) is separable if it factors into distinct linear factors over E[x]. An extension E of F is a separable extension of F if every element in E is the root of a separable polynomial in F [x]. Also recall that f (x) is separable if and only if gcd(f (x), f ′ (x)) = 1 (Lemma 22.5). Proposition 23.11. Let f (x) be an irreducible polynomial over F . If the characteristic of F is 0, then f (x) is separable. If the characteristic of F is p and f (x) ̸= g(xp ) for some g(x) in F [x], then f (x) is also separable. Proof. First assume that char F = 0. Since deg f ′ (x) < deg f (x) and f (x) is irreducible, the only way gcd(f (x), f ′ (x)) ̸= 1 is if f ′ (x) is the zero polynomial; however, this is impos- sible in a field of characteristic zero. If char F = p, then f ′ (x) can be the zero polynomial if every coefficient of f ′ (x) is a multiple of p. This can happen only if we have a polynomial of the form f (x) = a0 + a1 xp + a2 x2p + · · · + an xnp . Certainly extensions of a field F of the form F (α) are some of the easiest to study and understand. Given a field extension E of F , the obvious question to ask is when it is possible to find an element α ∈ E such that E = F (α). In this case, α is called a primitive element. We already know that primitive elements exist for certain extensions. For example, √ √ √ √ Q( 3, 5 ) = Q( 3 + 5 ) and √ √ √ Q( 5, 5 i) = Q( 5 i). 3 6 Corollary 22.12 tells us that there exists a primitive element for any finite extension of a finite field. The next theorem tells us that we can often find a primitive element. 23.2. THE FUNDAMENTAL THEOREM 287 Theorem 23.12 Primitive Element Theorem. Let E be a finite separable extension of a field F . Then there exists an α ∈ E such that E = F (α). Proof. We already know that there is no problem if F is a finite field. Suppose that E is a finite extension of an infinite field. We will prove the result for F (α, β). The general case easily follows when we use mathematical induction. Let f (x) and g(x) be the minimal polynomials of α and β, respectively. Let K be the field in which both f (x) and g(x) split. Suppose that f (x) has zeros α = α1 , . . . , αn in K and g(x) has zeros β = β1 , . . . , βm in K. All of these zeros have multiplicity 1, since E is separable over F . Since F is infinite, we can find an a in F such that αi − α a ̸= β − βj for all i and j with j ̸= 1. Therefore, a(β − βj ) ̸= αi − α. Let γ = α + aβ. Then γ = α + aβ ̸= αi + aβj ; hence, γ − aβj ̸= αi for all i, j with j ̸= 1. Define h(x) ∈ F (γ)[x] by h(x) = f (γ − ax). Then h(β) = f (α) = 0. However, h(βj ) ̸= 0 for j ̸= 1. Hence, h(x) and g(x) have a single common factor in F (γ)[x]; that is, the minimal polynomial of β over F (γ) must be linear, since β is the only zero common to both g(x) and h(x). So β ∈ F (γ) and α = γ − aβ is in F (γ). Hence, F (α, β) = F (γ). 23.2 The Fundamental Theorem The goal of this section is to prove the Fundamental Theorem of Galois Theory. This theorem explains the connection between the subgroups of G(E/F ) and the intermediate fields between E and F . Proposition 23.13. Let {σi : i ∈ I} be a collection of automorphisms of a field F . Then F{σi } = {a ∈ F : σi (a) = a for all σi } is a subfield of F . Proof. Let σi (a) = a and σi (b) = b. Then σi (a ± b) = σi (a) ± σi (b) = a ± b and σi (ab) = σi (a)σi (b) = ab. If a ̸= 0, then σi (a−1 ) = [σi (a)]−1 = a−1 . Finally, σi (0) = 0 and σi (1) = 1 since σi is an automorphism. Corollary 23.14. Let F be a field and let G be a subgroup of Aut(F ). Then FG = {α ∈ F : σ(α) = α for all σ ∈ G} is a subfield of F . The subfield F{σi } of F is called the fixed field of {σi }. The field fixed by a subgroup G of Aut(F ) will be denoted by FG . √ √ √ √ √ Example √ 23.15. √Let σ : Q( 3, 5 ) → Q( √ √3, 5 ) be the automorphism that maps 3 to − 3. Then Q( 5 ) is the subfield of Q( 3, 5 ) left fixed by σ. 288 CHAPTER 23. GALOIS THEORY Proposition 23.16. Let E be a splitting field over F of a separable polynomial. Then EG(E/F ) = F . Proof. Let G = G(E/F ). Clearly, F ⊂ EG ⊂ E. Also, E must be a splitting field of EG and G(E/F ) = G(E/EG ). By Theorem 23.7, |G| = [E : EG ] = [E : F ]. Therefore, [EG : F ] = 1. Consequently, EG = F . A large number of mathematicians first learned Galois theory from Emil Artin’s mono- graph on the subject [1]. The very clever proof of the following lemma is due to Artin. Lemma 23.17. Let G be a finite group of automorphisms of E and let F = EG . Then [E : F ] ≤ |G|. Proof. Let |G| = n. We must show that any set of n + 1 elements α1 , . . . , αn+1 in E is linearly dependent over F ; that is, we need to find elements ai ∈ F , not all zero, such that a1 α1 + a2 α2 + · · · + an+1 αn+1 = 0. Suppose that σ1 = id, σ2 , . . . , σn are the automorphisms in G. The homogeneous system of linear equations σ1 (α1 )x1 + σ1 (α2 )x2 + · · · + σ1 (αn+1 )xn+1 = 0 σ2 (α1 )x1 + σ2 (α2 )x2 + · · · + σ2 (αn+1 )xn+1 = 0 .. . σn (α1 )x1 + σn (α2 )x2 + · · · + σn (αn+1 )xn+1 = 0 has more unknowns than equations. From linear algebra we know that this system has a nontrivial solution, say xi = ai for i = 1, 2, . . . , n + 1. Since σ1 is the identity, the first equation translates to a1 α1 + a2 α2 + · · · + an+1 αn+1 = 0. The problem is that some of the ai ’s may be in E but not in F . We must show that this is impossible. Suppose that at least one of the ai ’s is in E but not in F . By rearranging the αi ’s we may assume that a1 is nonzero. Since any nonzero multiple of a solution is also a solution, we can also assume that a1 = 1. Of all possible solutions fitting this description, we choose the one with the smallest number of nonzero terms. Again, by rearranging α2 , . . . , αn+1 if necessary, we can assume that a2 is in E but not in F . Since F is the subfield of E that is fixed elementwise by G, there exists a σi in G such that σi (a2 ) ̸= a2 . Applying σi to each equation in the system, we end up with the same homogeneous system, since G is a group. Therefore, x1 = σi (a1 ) = 1, x2 = σi (a2 ), . . ., xn+1 = σi (an+1 ) is also a solution of the original system. We know that a linear combination of two solutions of a homogeneous system is also a solution; consequently, x1 = 1 − 1 = 0 x2 = a2 − σi (a2 ) .. . xn+1 = an+1 − σi (an+1 ) 23.2. THE FUNDAMENTAL THEOREM 289 must be another solution of the system. This is a nontrivial solution because σi (a2 ) ̸= a2 , and has fewer nonzero entries than our original solution. This is a contradiction, since the number of nonzero solutions to our original solution was assumed to be minimal. We can therefore conclude that a1 , . . . , an+1 ∈ F . Let E be an algebraic extension of F . If every irreducible polynomial in F [x] with a root in E has all of its roots in E, then E is called a normal extension of F ; that is, every irreducible polynomial in F [x] containing a root in E is the product of linear factors in E[x]. Theorem 23.18. Let E be a field extension of F . Then the following statements are equivalent. 1. E is a finite, normal, separable extension of F . 2. E is a splitting field over F of a separable polynomial. 3. F = EG for some finite group G of automorphisms of E. Proof. (1) ⇒ (2). Let E be a finite, normal, separable extension of F . By the Primitive Element Theorem, we can find an α in E such that E = F (α). Let f (x) be the minimal polynomial of α over F . The field E must contain all of the roots of f (x) since it is a normal extension F ; hence, E is a splitting field for f (x). (2) ⇒ (3). Let E be the splitting field over F of a separable polynomial. By Proposi- tion 23.16, EG(E/F ) = F . Since |G(E/F )| = [E : F ], this is a finite group. (3) ⇒ (1). Let F = EG for some finite group of automorphisms G of E. Since [E : F ] ≤ |G|, E is a finite extension of F . To show that E is a finite, normal extension of F , let f (x) ∈ F [x] be an irreducible monic polynomial that has a root α in E. We must show that f (x) is the product of distinct linear factors in E[x]. By Proposition 23.5, automorphisms in G permute the roots of f (x) lying in E. Hence, ∏n if we let G act on α, we can obtain distinct roots α1 = α, α2 , . . . , αn in E. Let g(x) = i=1 (x − αi ). Then g(x) is separable over F and g(α) = 0. Any automorphism σ in G permutes the factors of g(x) since it permutes these roots; hence, when σ acts on g(x), it must fix the coefficients of g(x). Therefore, the coefficients of g(x) must be in F . Since deg g(x) ≤ deg f (x) and f (x) is the minimal polynomial of α, f (x) = g(x). Corollary 23.19. Let K be a field extension of F such that F = KG for some finite group of automorphisms G of K. Then G = G(K/F ). Proof. Since F = KG , G is a subgroup of G(K/F ). Hence, [K : F ] ≤ |G| ≤ |G(K/F )| = [K : F ]. It follows that G = G(K/F ), since they must have the same order. Before we determine the exact correspondence between field extensions and automor- phisms of fields, let us return to a familiar example. √ √ Example 23.20. In Example 23.4 we examined the automorphisms of Q( 3, 5 ) fixing Q. Figure √ compares the lattice of field extensions of Q with the lattice of subgroups √ 23.21 of G(Q( 3, 5 )/Q). The Fundamental Theorem of Galois Theory tells us what the rela- tionship is between the two lattices. 290 CHAPTER 23. GALOIS THEORY √ √ {id, σ, τ, µ} Q( 3, 5 ) √ √ √ {id, σ} {id, τ } {id, µ} Q( 3 ) Q( 5 ) Q( 15 ) {id} Q √ √ Figure 23.21: G(Q( 3, 5 )/Q) We are now ready to state and prove the Fundamental Theorem of Galois Theory. Theorem 23.22 Fundamental Theorem of Galois Theory. Let F be a finite field or a field of characteristic zero. If E is a finite normal extension of F with Galois group G(E/F ), then the following statements are true. 1. The map K 7→ G(E/K) is a bijection of subfields K of E containing F with the subgroups of G(E/F ). 2. If F ⊂ K ⊂ E, then [E : K] = |G(E/K)| and [K : F ] = [G(E/F ) : G(E/K)]. 3. F ⊂ K ⊂ L ⊂ E if and only if {id} ⊂ G(E/L) ⊂ G(E/K) ⊂ G(E/F ). 4. K is a normal extension of F if and only if G(E/K) is a normal subgroup of G(E/F ). In this case G(K/F ) ∼= G(E/F )/G(E/K). Proof. (1) Suppose that G(E/K) = G(E/L) = G. Both K and L are fixed fields of G; hence, K = L and the map defined by K 7→ G(E/K) is one-to-one. To show that the map is onto, let G be a subgroup of G(E/F ) and K be the field fixed by G. Then F ⊂ K ⊂ E; consequently, E is a normal extension of K. Thus, G(E/K) = G and the map K 7→ G(E/K) is a bijection. (2) By Theorem 23.7, |G(E/K)| = [E : K]; therefore, |G(E/F )| = [G(E/F ) : G(E/K)] · |G(E/K)| = [E : F ] = [E : K][K : F ]. Thus, [K : F ] = [G(E/F ) : G(E/K)]. Statement (3) is illustrated in Figure 23.23. We leave the proof of this property as an exercise. (4) This part takes a little more work. Let K be a normal extension of F . If σ is in G(E/F ) and τ is in G(E/K), we need to show that σ −1 τ σ is in G(E/K); that is, we need to show that σ −1 τ σ(α) = α for all α ∈ K. Suppose that f (x) is the minimal polynomial of α over F . Then σ(α) is also a root of f (x) lying in K, since K is a normal extension of F . Hence, τ (σ(α)) = σ(α) or σ −1 τ σ(α) = α. Conversely, let G(E/K) be a normal subgroup of G(E/F ). We need to show that F = KG(K/F ) . Let τ ∈ G(E/K). For all σ ∈ G(E/F ) there exists a τ ∈ G(E/K) such that τ σ = στ . Consequently, for all α ∈ K τ (σ(α)) = σ(τ (α)) = σ(α); 23.2. THE FUNDAMENTAL THEOREM 291 hence, σ(α) must be in the fixed field of G(E/K). Let σ be the restriction of σ to K. Then σ is an automorphism of K fixing F , since σ(α) ∈ K for all α ∈ K; hence, σ ∈ G(K/F ). Next, we will show that the fixed field of G(K/F ) is F . Let β be an element in K that is fixed by all automorphisms in G(K/F ). In particular, σ(β) = β for all σ ∈ G(E/F ). Therefore, β belongs to the fixed field F of G(E/F ). Finally, we must show that when K is a normal extension of F , G(K/F ) ∼ = G(E/F )/G(E/K). For σ ∈ G(E/F ), let σK be the automorphism of K obtained by restricting σ to K. Since K is a normal extension, the argument in the preceding paragraph shows that σK ∈ G(K/F ). Consequently, we have a map ϕ : G(E/F ) → G(K/F ) defined by σ 7→ σK . This map is a group homomorphism since ϕ(στ ) = (στ )K = σK τK = ϕ(σ)ϕ(τ ). The kernel of ϕ is G(E/K). By (2), |G(E/F )|/|G(E/K)| = [K : F ] = |G(K/F )|. Hence, the image of ϕ is G(K/F ) and ϕ is onto. Applying the First Isomorphism Theorem, we have G(K/F ) ∼= G(E/F )/G(E/K). E {id} L G(E/L) K G(E/K) F G(E/F ) Figure 23.23: Subgroups of G(E/F ) and subfields of E Example 23.24. In this example we will illustrate the Fundamental Theorem of Galois Theory by determining the lattice of subgroups of the Galois group of f (x) = x4 − 2. We will compare this lattice to the lattice of field extensions √ of Q that are contained in the splitting field of x −√2. The splitting 4 √ field of f (x) is Q( 2, i). To 4 √ see this,√ notice that f (x) factors as (x 2 + 2 )(x2 − 2 ); hence, the roots of f (x) are ± 4 2 and ± 4 2 i. We first √ √ adjoin the root 4 2√to Q and then √ adjoin the root i of x 2 + 1 to Q( 4 2 ). The splitting field of f (x) is then √ Q( 4 2 )(i) = Q( 4 2, i). √ √ Since [Q( 4 2 ) : Q] =√4 and i is not in Q( 4 2 ), it must be the case that [Q( 4 2, i) : √ Q( 4 2 )] = 2. Hence, [Q( 4 2, i) : Q] = 8. The set √ √ √ √ √ √ {1, 2, ( 2 )2 , ( 2 )3 , i, i 2, i( 2 )2 , i( 2 )3 } 4 4 4 4 4 4 √ √ is a basis of Q( 4 2, i) over Q. The lattice of field extensions of Q contained in Q( 4 2, i) is illustrated in Figure 23.25(a). √The Galois √ group G of f (x) must be of order 8. Let σ be the automorphism defined by σ( 4 2 ) = i 4 2 and σ(i) = i, and τ be the automorphism defined by complex conjugation; 292 CHAPTER 23. GALOIS THEORY that is, τ (i) = −i. Then G has an element of order 4 and an element of order 2. It is easy to verify by direct computation that the elements of G are {id, σ, σ 2 , σ 3 , τ, στ, σ 2 τ, σ 3 τ } and that the relations τ 2 = id, σ 4 = id, and τ στ = σ −1 are satisfied; hence, G must be isomorphic to D4 . The lattice of subgroups of G is illustrated in Figure 23.25(b). √ Q( 4 2, i) √ √ √ √ √ Q( 4 2 ) Q( 4 2 i) Q( 2, i) Q((1 + i) 4 2 ) Q((1 − i) 4 2 ) √ √ Q( 2 ) Q(i) Q( 2 i) Q (a) D4 {id, σ 2 , τ, σ 2 τ } {id, σ, σ 2 , σ 3 }{id, σ 2 , στ, σ 3 τ } {id, τ } {id, σ 2 τ } {id, σ 2 } {id, στ } {id, σ 3 τ } {id} (b) Figure 23.25: Galois group of x4 − 2 Historical Note Solutions for the cubic and quartic equations were discovered in the 1500s. Attempts to find solutions for the quintic equations puzzled some of history’s best mathematicians. In 1798, P. Ruffini submitted a paper that claimed no such solution could be found; however, the paper was not well received. In 1826, Niels Henrik Abel (1802–1829) finally offered the first correct proof that quintics are not always solvable by radicals. Abel inspired the work of Évariste Galois. Born in 1811, Galois began to display ex- traordinary mathematical talent at the age of 14. He applied for entrance to the École Polytechnique several times; however, he had great difficulty meeting the formal entrance requirements, and the examiners failed to recognize his mathematical genius. He was finally accepted at the École Normale in 1829. Galois worked to develop a theory of solvability for polynomials. In 1829, at the age of 17, Galois presented two papers on the solution of algebraic equations to the Académie des Sciences de Paris. These papers were sent to Cauchy, who subsequently lost them. A third paper was submitted to Fourier, who died before he could read the paper. Another paper 23.3. APPLICATIONS 293 was presented, but was not published until 1846. Galois’ democratic sympathies led him into the Revolution of 1830. He was expelled from school and sent to prison for his part in the turmoil. After his release in 1832, he was drawn into a duel possibly over a love affair. Certain that he would be killed, he spent the evening before his death outlining his work and his basic ideas for research in a long letter to his friend Chevalier. He was indeed dead the next day, at the age of 20. 23.3 Applications Solvability by Radicals Throughout this section we shall assume that all fields have characteristic zero to ensure that irreducible polynomials do not have multiple roots. The immediate goal of this section is to determine when the roots of a polynomial f (x) can be computed with a finite number of operations on the coefficients of f (x). The allowable operations are addition, subtraction, multiplication, division, and the extraction of nth roots. Certainly the solution to the quadratic equation, ax2 + bx + c = 0, illustrates this process: √ −b ± b2 − 4ac x= . 2a The only one of these operations that might demand a larger field is the taking of nth roots. We are led to the following definition. An extension field E of a field F is an extension by radicals if there exists a chain of subfields F = F0 ⊂ F1 ⊂ F2 ⊂ · · · ⊂ Fr = E such for i = 1, 2, . . . , r, we have Fi = Fi−1 (αi ) and αini ∈ Fi−1 for some positive integer ni . A polynomial f (x) is solvable by radicals over F if the splitting field K of f (x) over F is contained in an extension of F by radicals. Our goal is to arrive at criteria that will tell us whether or not a polynomial f (x) is solvable by radicals by examining the Galois group f (x). The easiest polynomial to solve by radicals is one of the form xn − a. As we discussed in Chapter 4, the roots of xn − 1 are called the nth roots of unity. These roots are a finite subgroup of the splitting field of xn − 1. By Corollary 22.11, the nth roots of unity form a cyclic group. Any generator of this group is called a primitive nth root of unity. Example 23.26. The polynomial xn − 1 is solvable by radicals over Q. The roots of this polynomial are 1, ω, ω 2 , . . . , ω n−1 , where ( ) ( ) 2π 2π ω = cos + i sin . n n The splitting field of xn − 1 over Q is Q(ω). We shall prove that a polynomial is solvable by radicals if its Galois group is solvable. Recall that a subnormal series of a group G is a finite sequence of subgroups G = Hn ⊃ Hn−1 ⊃ · · · ⊃ H1 ⊃ H0 = {e}, where Hi is normal in Hi+1 . A group G is solvable if it has a subnormal series {Hi } such that all of the factor groups Hi+1 /Hi are abelian. For example, if we examine the series {id} ⊂ A3 ⊂ S3 , we see that S3 is solvable. On the other hand, S5 is not solvable, by Theorem 10.11. 294 CHAPTER 23. GALOIS THEORY Lemma 23.27. Let F be a field of characteristic zero and E be the splitting field of xn − a over F with a ∈ F . Then G(E/F ) is a solvable group. √ √ √ Proof. The roots of xn − a are n a, ω n a, . . . , ω n−1 n a, where ω is a primitive nth root of unity. Suppose that F contains all of its nth roots of unity. If ζ is one of the roots of xn − a, then distinct roots of xn − a are ζ, ωζ, . . . , ω n−1 ζ, and E = F (ζ). Since G(E/F ) permutes the roots xn − a, the elements in G(E/F ) must be determined by their action on these roots. Let σ and τ be in G(E/F ) and suppose that σ(ζ) = ω i ζ and τ (ζ) = ω j ζ. If F contains the roots of unity, then στ (ζ) = σ(ω j ζ) = ω j σ(ζ) = ω i+j ζ = ω i τ (ζ) = τ (ω i ζ) = τ σ(ζ). Therefore, στ = τ σ and G(E/F ) is abelian, and G(E/F ) must be solvable. Now suppose that F does not contain a primitive nth root of unity. Let ω be a generator of the cyclic group of the nth roots of unity. Let α be a zero of xn − a. Since α and ωα are both in the splitting field of xn − a, ω = (ωα)/α is also in E. Let K = F (ω). Then F ⊂ K ⊂ E. Since K is the splitting field of xn − 1, K is a normal extension of F . Therefore, any automorphism σ in G(F (ω)/F ) is determined by σ(ω). It must be the case that σ(ω) = ω i for some integer i since all of the zeros of xn −1 are powers of ω. If τ (ω) = ω j is in G(F (ω)/F ), then στ (ω) = σ(ω j ) = [σ(ω)]j = ω ij = [τ (ω)]i = τ (ω i ) = τ σ(ω). Therefore, G(F (ω)/F ) is abelian. By the Fundamental Theorem of Galois Theory the series {id} ⊂ G(E/F (ω)) ⊂ G(E/F ) is a normal series. By our previous argument, G(E/F (ω)) is abelian. Since G(E/F )/G(E/F (ω)) ∼ = G(F (ω)/F ) is also abelian, G(E/F ) is solvable. Lemma 23.28. Let F be a field of characteristic zero and let F = F0 ⊂ F1 ⊂ F2 ⊂ · · · ⊂ Fr = E a radical extension of F . Then there exists a normal radical extension F = K0 ⊂ K1 ⊂ K2 ⊂ · · · ⊂ Kr = K such that K that contains E and Ki is a normal extension of Ki−1 . Proof. Since E is a radical extension of F , there exists a chain of subfields F = F0 ⊂ F1 ⊂ F2 ⊂ · · · ⊂ Fr = E such for i = 1, 2, . . . , r, we have Fi = Fi−1 (αi ) and αini ∈ Fi−1 for some positive integer ni . We will build a normal radical extension of F , F = K0 ⊂ K1 ⊂ K2 ⊂ · · · ⊂ Kr = K such that K ⊇ E. Define K1 for be the splitting field of xn1 − α1n1 . The roots of this polynomial are α1 , α1 ω, α1 ω 2 , . . . , α1 ω n1 −1 , where ω is a primitive n1 th root of unity. If F contains all of its n1 roots of unity, then K1 = F (α! ). On the other hand, suppose that F does not contain a primitive n1 th root of unity. If β is a root of xn1 − α1n1 , then all of 23.3. APPLICATIONS 295 the roots of xn1 − α1n1 must be β, ωβ, . . . , ω n1 −1 , where ω is a primitive n1 th root of unity. In this case, K1 = F (ωβ). Thus, K1 is a normal radical extension of F containing F1 . Continuing in this manner, we obtain F = K0 ⊂ K1 ⊂ K2 ⊂ · · · ⊂ Kr = K such that Ki is a normal extension of Ki−1 and Ki ⊇ Fi for i = 1, 2, . . . , r. We will now prove the main theorem about solvability by radicals. Theorem 23.29. Let f (x) be in F [x], where char F = 0. If f (x) is solvable by radicals, then the Galois group of f (x) over F is solvable. Proof. Since f (x) is solvable by radicals there exists an extension E of F by radicals F = F0 ⊂ F1 ⊂ · · · ⊂ Fn = E. By Lemma 23.28, we can assume that E is a splitting field f (x) and Fi is normal over Fi−1 . By the Fundamental Theorem of Galois Theory, G(E/Fi ) is a normal subgroup of G(E/Fi−1 ). Therefore, we have a subnormal series of subgroups of G(E/F ): {id} ⊂ G(E/Fn−1 ) ⊂ · · · ⊂ G(E/F1 ) ⊂ G(E/F ). Again by the Fundamental Theorem of Galois Theory, we know that G(E/Fi−1 )/G(E/Fi ) ∼ = G(Fi /Fi−1 ). By Lemma 23.27, G(Fi /Fi−1 ) is solvable; hence, G(E/F ) is also solvable. The converse of Theorem 23.29 is also true. For a proof, see any of the references at the end of this chapter. Insolvability of the Quintic We are now in a position to find a fifth-degree polynomial that is not solvable by radicals. We merely need to find a polynomial whose Galois group is S5 . We begin by proving a lemma. Lemma 23.30. If p is prime, then any subgroup of Sp that contains a transposition and a cycle of length p must be all of Sp . Proof. Let G be a subgroup of Sp that contains a transposition σ and τ a cycle of length p. We may assume that σ = (12). The order of τ is p and τ n must be a cycle of length p for 1 ≤ n < p. Therefore, we may assume that µ = τ n = (12i3 . . . ip ) for some n, where 1 ≤ n < p (see Exercise 5.3.13 in Chapter 5). Noting that (12)(12i3 . . . ip ) = (2i3 . . . ip ) and (2i3 . . . ip )k (12)(2i3 . . . ip )−k = (1ik ), we can obtain all the transpositions of the form (1n) for 1 ≤ n < p. However, these transpositions generate all transpositions in Sp , since (1j)(1i)(1j) = (ij). The transpositions generate Sp . 296 CHAPTER 23. GALOIS THEORY y 60 f(x) = x5 −6x3 −27x−3 40 20 x -3 -2 -1 1 2 3 -20 -40 -60 Figure 23.31: The graph of f (x) = x5 − 6x3 − 27x − 3 Example 23.32. We will show that f (x) = x5 − 6x3 − 27x − 3 ∈ Q[x] is not solvable. We claim that the Galois group of f (x) over Q is S5 . By Eisenstein’s Criterion, f (x) is irreducible and, therefore, must be separable. The derivative of f (x) is f ′ (x) = 5x4 −18x2 − 27; hence, setting f ′ (x) = 0 and solving, we find that the only real roots of f ′ (x) are √ √ 6 6+9 x=± . 5 Therefore, f (x) can have at most one maximum and one minimum. It is easy to show that f (x) changes sign between −3 and −2, between −2 and 0, and once again between 0 and 4 (Figure 23.31). Therefore, f (x) has exactly three distinct real roots. The remaining two roots of f (x) must be complex conjugates. Let K be the splitting field of f (x). Since f (x) has five distinct roots in K and every automorphism of K fixing Q is determined by the way it permutes the roots of f (x), we know that G(K/Q) is a subgroup of S5 . Since f is irreducible, there is an element in σ ∈ G(K/Q) such that σ(a) = b for two roots a and b of f (x). The automorphism of C that takes a + bi 7→ a − bi leaves the real roots fixed and interchanges the complex roots; consequently, G(K/Q) contains a transpostion. If α is one of the real roots of f (x), then [Q(α) : Q] = 5 by Exercise 21.4.28. Since Q(α) is a subfield of K, it must be the case the [K : Q] is divisible by 5. Since [K : Q] = |G(K/Q)| and G(K/Q) ⊂ S5 , we know that G(K/Q) contains a cycle of length 5. By Lemma 23.30, S5 is generated by a transposition and an element of order 5; therefore, G(K/Q) must be all of 23.4. EXERCISES 297 S5 . By Theorem 10.11, S5 is not solvable. Consequently, f (x) cannot be solved by radicals. The Fundamental Theorem of Algebra It seems fitting that the last theorem that we will state and prove is the Fundamental Theorem of Algebra. This theorem was first proven by Gauss in his doctoral thesis. Prior to Gauss’s proof, mathematicians suspected that there might exist polynomials over the real and complex numbers having no solutions. The Fundamental Theorem of Algebra states that every polynomial over the complex numbers factors into distinct linear factors. Theorem 23.33 Fundamental Theorem of Algebra. The field of complex numbers is algebraically closed; that is, every polynomial in C[x] has a root in C. Proof. Suppose that E is a proper finite field extension of the complex numbers. Since any finite extension of a field of characteristic zero is a simple extension, there exists an α ∈ E such that E = C(α) with α the root of an irreducible polynomial f (x) in C[x]. The splitting field L of f (x) is a finite normal separable extension of C that contains E. We must show that it is impossible for L to be a proper extension of C. Suppose that L is a proper extension of C. Since L is the splitting field of f (x)(x2 + 1) over R, L is a finite normal separable extension of R. Let K be the fixed field of a Sylow 2-subgroup G of G(L/R). Then L ⊃ K ⊃ R and |G(L/K)| = [L : K]. Since [L : R] = [L : K][K : R], we know that [K : R] must be odd. Consequently, K = R(β) with β having a minimal polynomial f (x) of odd degree. Therefore, K = R. We now know that G(L/R) must be a 2-group. It follows that G(L/C) is a 2-group. We have assumed that L ̸= C; therefore, |G(L/C)| ≥ 2. By the first Sylow Theorem and the Fundamental Theorem of Galois Theory, there exists a subgroup G of G(L/C) of index 2 and a field E fixed elementwise by G. Then [E : C] = 2 and there exists an element √ γ∈E with minimal polynomial x + bx + c in C[x]. This polynomial has roots (−b ± b − 4c )/2 2 2 that are in C, since b2 − 4c is in C. This is impossible; hence, L = C. Although our proof was strictly algebraic, we were forced to rely on results from cal- culus. It is necessary to assume the completeness axiom from analysis to show that every polynomial of odd degree has a real root and that every positive real number has a square root. It seems that there is no possible way to avoid this difficulty and formulate a purely algebraic argument. It is somewhat amazing that there are several elegant proofs of the Fundamental Theorem of Algebra that use complex analysis. It is also interesting to note that we can obtain a proof of such an important theorem from two very different fields of mathematics. Sage Fields, field extensions, roots of polynomials, and group theory — Sage has it all, and so it is possible to carefully study very complicated examples from Galois Theory with Sage. 23.4 Exercises 1. Compute each of the following Galois groups. Which of these field extensions are normal field extensions? If the extension is not normal, find a normal extension of Q in which the extension field is contained. 298 CHAPTER 23. GALOIS THEORY √ √ √ (a) G(Q( 30 )/Q) (d) G(Q( 2, 3 2, i)/Q) √ (b) G(Q( 4 5 )/Q) √ √ √ √ (c) G(Q( 2, 3, 5 )/Q) (e) G(Q( 6, i)/Q) 2. Determine the separability of each of the following polynomials. (a) x3 + 2x2 − x − 2 over Q (c) x4 + x2 + 1 over Z3 (b) x4 + 2x2 + 1 over Q (d) x3 + x2 + 1 over Z2 3. Give the order and describe a generator of the Galois group of GF(729) over GF(9). 4. Determine the Galois groups of each of the following polynomials in Q[x]; hence, determine the solvability by radicals of each of the polynomials. (a) x5 − 12x2 + 2 (f) (x2 − 2)(x2 + 2) (b) x5 − 4x4 + 2x + 2 (g) x8 − 1 (c) x3 −5 (h) x8 + 1 (d) x4 − x2 − 6 (e) x5 + 1 (i) x4 − 3x2 − 10 5. Find a primitive element in the splitting field of each of the following polynomials in Q[x]. (a) x4 − 1 (c) x4 − 2x2 − 15 (b) x4 − 8x2 + 15 (d) x3 − 2 6. Prove that the Galois group of an irreducible quadratic polynomial is isomorphic to Z2 . 7. Prove that the Galois group of an irreducible cubic polynomial is isomorphic to S3 or Z3 . 8. Let F ⊂ K ⊂ E be fields. If E is a normal extension of F , show that E must also be a normal extension of K. 9. Let G be the Galois group of a polynomial of degree n. Prove that |G| divides n!. 10. Let F ⊂ E. If f (x) is solvable over F , show that f (x) is also solvable over E. 11. Construct a polynomial f (x) in Q[x] of degree 7 that is not solvable by radicals. 12. Let p be prime. Prove that there exists a polynomial f (x) ∈ Q[x] of degree p with Galois group isomorphic to Sp . Conclude that for each prime p with p ≥ 5 there exists a polynomial of degree p that is not solvable by radicals. 13. Let p be a prime and Zp (t) be the field of rational functions over Zp . Prove that f (x) = xp − t is an irreducible polynomial in Zp (t)[x]. Show that f (x) is not separable. 14. Let E be an extension field of F . Suppose that K and L are two intermediate fields. If there exists an element σ ∈ G(E/F ) such that σ(K) = L, then K and L are said to be conjugate fields. Prove that K and L are conjugate if and only if G(E/K) and G(E/L) are conjugate subgroups of G(E/F ). 15. Let σ ∈ Aut(R). If a is a positive real number, show that σ(a) > 0. 23.4. EXERCISES 299 16. Let K be the splitting field of x3 + x2 + 1 ∈ Z2 [x]. Prove or disprove that K is an extension by radicals. 17. Let F be a field such that char(F ) ̸= 2. Prove that the splitting field of f (x) = √ ax + bx + c is F ( α ), where α = b2 − 4ac. 2 18. Prove or disprove: Two different subgroups of a Galois group will have different fixed fields. 19. Let K be the splitting field of a polynomial over F . If E is a field extension of F contained in K and [E : F ] = 2, then E is the splitting field of some polynomial in F [x]. 20. We know that the cyclotomic polynomial xp − 1 Φp (x) = = xp−1 + xp−2 + · · · + x + 1 x−1 is irreducible over Q for every prime p. Let ω be a zero of Φp (x), and consider the field Q(ω). (a) Show that ω, ω 2 , . . . , ω p−1 are distinct zeros of Φp (x), and conclude that they are all the zeros of Φp (x). (b) Show that G(Q(ω)/Q) is abelian of order p − 1. (c) Show that the fixed field of G(Q(ω)/Q) is Q. 21. Let F be a finite field or a field of characteristic zero. Let E be a finite normal extension of F with Galois group G(E/F ). Prove that F ⊂ K ⊂ L ⊂ E if and only if {id} ⊂ G(E/L) ⊂ G(E/K) ⊂ G(E/F ). 22. Let F be a field of characteristic zero and let f (x) ∈ F [x] be a separable polynomial of degree ∏ n. If E is the splitting field of f (x), let α1 , . . . , αn be the2 roots of f (x) in E. Let ∆ = i<j (αi − αj ). We define the discriminant of f (x) to be ∆ . (a) If f (x) = x2 + bx + c, show that ∆2 = b2 − 4c. (b) If f (x) = x3 + px + q, show that ∆2 = −4p3 − 27q 2 . (c) Prove that ∆2 is in F . (d) If σ ∈ G(E/F ) is a transposition of two roots of f (x), show that σ(∆) = −∆. (e) If σ ∈ G(E/F ) is an even permutation of the roots of f (x), show that σ(∆) = ∆. (f) Prove that G(E/F ) is isomorphic to a subgroup of An if and only if ∆ ∈ F . (g) Determine the Galois groups of x3 + 2x − 4 and x3 + x − 3. References and Suggested Readings [1] Artin, E. Theory: Lectures Delivered at the University of Notre Dame (Notre Dame Mathematical Lectures, Number 2). Dover, Mineola, NY, 1997. [2] Edwards, H. M. Galois Theory. Springer-Verlag, New York, 1984. [3] Fraleigh, J. B. A First Course in Abstract Algebra. 7th ed. Pearson, Upper Saddle River, NJ, 2003. 300 CHAPTER 23. GALOIS THEORY [4] Gaal, L. Classical Galois Theory with Examples. American Mathematical Society, Providence, 1979. [5] Garling, D. J. H. A Course in Galois Theory. Cambridge University Press, Cambridge, 1986. [6] Kaplansky, I. Fields and Rings. 2nd ed. University of Chicago Press, Chicago, 1972. [7] Rothman, T. “The Short Life of Évariste Galois,” Scientific American, April 1982, 136–49. A GNU Free Documentation License Version 1.3, 3 November 2008 Copyright © 2000, 2001, 2002, 2007, 2008 Free Software Foundation, Inc. <http://www. fsf.org/> Everyone is permitted to copy and distribute verbatim copies of this license document, but changing it is not allowed. 0. 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If you have Invariant Sections, Front-Cover Texts and Back-Cover Texts, replace the “with… Texts.” line with this: with the Invariant Sections being LIST THEIR TITLES, with the Front-Cover Texts being LIST, and with the Back-Cover Texts being LIST. If you have Invariant Sections without Cover Texts, or some other combination of the three, merge those two alternatives to suit the situation. If your document contains nontrivial examples of program code, we recommend releasing these examples in parallel under your choice of free software license, such as the GNU General Public License, to permit their use in free software. B Hints and Solutions to Selected Exercises 1 Preliminaries 1.3 Exercises 1.3.1. Hint. (a) A ∩ B = {2}; (b) B ∩ C = {5}. 1.3.2. Hint. (a) A × B = {(a, 1), (a, 2), (a, 3), (b, 1), (b, 2), (b, 3), (c, 1), (c, 2), (c, 3)}; (d) A × D = ∅. 1.3.6. Hint. If x ∈ A ∪ (B ∩ C), then either x ∈ A or x ∈ B ∩ C. Thus, x ∈ A ∪ B and A ∪ C. Hence, x ∈ (A ∪ B) ∩ (A ∪ C). Therefore, A ∪ (B ∩ C) ⊂ (A ∪ B) ∩ (A ∪ C). Conversely, if x ∈ (A ∪ B) ∩ (A ∪ C), then x ∈ A ∪ B and A ∪ C. Thus, x ∈ A or x is in both B and C. So x ∈ A ∪ (B ∩ C) and therefore (A ∪ B) ∩ (A ∪ C) ⊂ A ∪ (B ∩ C). Hence, A ∪ (B ∩ C) = (A ∪ B) ∩ (A ∪ C). 1.3.10. Hint. (A ∩ B) ∪ (A \ B) ∪ (B \ A) = (A ∩ B) ∪ (A ∩ B ′ ) ∪ (B ∩ A′ ) = [A ∩ (B ∪ B ′ )] ∪ (B ∩ A′ ) = A ∪ (B ∩ A′ ) = (A ∪ B) ∩ (A ∪ A′ ) = A ∪ B. 1.3.14. Hint. A \ (B ∪ C) = A ∩ (B ∪ C)′ = (A ∩ A) ∩ (B ′ ∩ C ′ ) = (A ∩ B ′ ) ∩ (A ∩ C ′ ) = (A \ B) ∩ (A \ C). 1.3.17. Hint. (a) Not a map since f (2/3) is undefined; (b) this is a map; (c) not a map, since f (1/2) = 3/4 but f (2/4) = 3/8; (d) this is a map. 1.3.18. Hint. (a) f is one-to-one but not onto. f (R) = {x ∈ R : x > 0}. (c) f is neither one-to-one nor onto. f (R) = {x : −1 ≤ x ≤ 1}. 1.3.20. Hint. (a) f (n) = n + 1. 1.3.22. Hint. (a) Let x, y ∈ A. Then g(f (x)) = (g ◦f )(x) = (g ◦f )(y) = g(f (y)). Thus, f (x) = f (y) and x = y, so g ◦ f is one-to-one. (b) Let c ∈ C, then c = (g ◦ f )(x) = g(f (x)) for some x ∈ A. Since f (x) ∈ B, g is onto. 1.3.23. Hint. f −1 (x) = (x + 1)/(x − 1). 1.3.24. Hint. (a) Let y ∈ f (A1 ∪ A2 ). Then there exists an x ∈ A1 ∪ A2 such that f (x) = y. Hence, y ∈ f (A1 ) or f (A2 ). Therefore, y ∈ f (A1 ) ∪ f (A2 ). Consequently, f (A1 ∪ A2 ) ⊂ f (A1 ) ∪ f (A2 ). Conversely, if y ∈ f (A1 ) ∪ f (A2 ), then y ∈ f (A1 ) or f (A2 ). Hence, there exists an x in A1 or A2 such that f (x) = y. Thus, there exists an x ∈ A1 ∪ A2 such that f (x) = y. Therefore, f (A1 )∪f (A2 ) ⊂ f (A1 ∪A2 ), and f (A1 ∪A2 ) = f (A1 )∪f (A2 ). 1.3.25. Hint. (a) The relation fails to be symmetric. (b) The relation is not reflexive, since 0 is not equivalent to itself. (c) The relation is not transitive. √ 1.3.28. Hint. Let X = N ∪ { 2 } and define x ∼ y if x + y ∈ N. 308 309 2 The Integers 2.3 Exercises 2.3.1. Hint. The base case, S(1) : [1(1 + 1)(2(1) + 1)]/6 = 1 = 12 is true. Assume that S(k) : 12 + 22 + · · · + k 2 = [k(k + 1)(2k + 1)]/6 is true. Then 12 + 22 + · · · + k 2 + (k + 1)2 = [k(k + 1)(2k + 1)]/6 + (k + 1)2 = [(k + 1)((k + 1) + 1)(2(k + 1) + 1)]/6, and so S(k + 1) is true. Thus, S(n) is true for all positive integers n. 2.3.3. Hint. The base case, S(4) : 4! = 24 > 16 = 24 is true. Assume S(k) : k! > 2k is true. Then (k + 1)! = k!(k + 1) > 2k · 2 = 2k+1 , so S(k + 1) is true. Thus, S(n) is true for all positive integers n. 2.3.8. Hint. Follow the proof in Example 2.4. 2.3.11. Hint. The base case, S(0) : (1 + x)0 − 1 = 0 ≥ 0 = 0 · x is true. Assume S(k) : (1 + x)k − 1 ≥ kx is true. Then (1 + x)k+1 − 1 = (1 + x)(1 + x)k − 1 = (1 + x)k + x(1 + x)k − 1 ≥ kx + x(1 + x)k ≥ kx + x = (k + 1)x, so S(k + 1) is true. Therefore, S(n) is true for all positive integers n. 2.3.17. Fibonacci Numbers. Hint. For (a) and (b) use mathematical induction. (c) Show that f1 = 1, f2 = 1, and fn+2 = fn+1 + fn . (d) Use part (c). (e) Use part (b) and Exercise 2.3.16. 2.3.19. Hint. Use the Fundamental Theorem of Arithmetic. 2.3.23. Hint. Use the Principle of Well-Ordering and the division algorithm. 2.3.27. Hint. Since gcd(a, b) = 1, there exist integers r and s such that ar + bs = 1. Thus, acr + bcs = c. 2.3.29. Hint. Every prime must be of the form 2, 3, 6n + 1, or 6n + 5. Suppose there are only finitely many primes of the form 6k + 5. 3 Groups 3.4 Exercises 3.4.1. Hint. (a) 3 + 7Z = {. . . , −4, 3, 10, . . .}; (c) 18 + 26Z; (e) 5 + 6Z. 3.4.2. Hint. (a) Not a group; (c) a group. 3.4.6. Hint. · 1 5 7 11 1 1 5 7 11 5 5 1 11 7 7 7 11 1 5 11 11 7 5 1 310 APPENDIX B. HINTS AND SOLUTIONS TO SELECTED EXERCISES 3.4.8. Hint. Pick two matrices. Almost any pair will work. 3.4.15. Hint. There is a nonabelian group containing six elements. 3.4.16. Hint. Look at the symmetry group of an equilateral triangle or a square. 3.4.17. Hint. The are five different groups of order 8. 3.4.18. Hint. Let ( ) 1 2 ··· n σ= a1 a2 · · · an be in Sn . All of the ai s must be distinct. There are n ways to choose a1 , n − 1 ways to choose a2 , . . ., 2 ways to choose an−1 , and only one way to choose an . Therefore, we can form σ in n(n − 1) · · · 2 · 1 = n! ways. 3.4.25. Hint. (aba−1 )n = (aba−1 )(aba−1 ) · · · (aba−1 ) = ab(aa−1 )b(aa−1 )b · · · b(aa−1 )ba−1 = abn a−1 . 3.4.31. Hint. Since abab = (ab)2 = e = a2 b2 = aabb, we know that ba = ab. 3.4.35. Hint. H1 = {id}, H2 = {id, ρ1 , ρ2 }, H3 = {id, µ1 }, H4 = {id, µ2 }, H5 = {id, µ3 }, S3 . √ √ √ 3.4.41. Hint.√ The identity of G is 1 = 1 + 0 2. Since (a + b 2 √ −1 )(c + d 2 ) = (ac + 2bd) + (ad + bc) 2, G is closed under multiplication. Finally, (a + b 2 ) = a/(a 2 − 2b2 ) − √ b 2/(a − 2b ). 2 2 3.4.46. Hint. Look at S3 . 3.4.49. Hint. ba = a4 b = a3 ab = ab 4 Cyclic Groups 4.4 Exercises 4.4.1. Hint. (a) False; (c) false; (e) true. 4.4.2. Hint. (a) 12; (c) infinite; (e) 10. 4.4.3. Hint. (a) 7Z = {. . . , −7, 0, 7, 14, . . .}; (b) {0, 3, 6, 9, 12, 15, 18, 21}; (c) {0}, {0, 6}, {0, 4, 8}, {0, 3, 6, 9}, {0, 2, 4, 6, 8, 10}; (g) {1, 3, 7, 9}; (j) {1, −1, i, −i}. 4.4.4. Hint. (a) ( ) ( ) ( ) ( ) 1 0 −1 0 0 −1 0 1 , , , . 0 1 0 −1 1 0 −1 0 (c) ( ) ( ) ( ) ( ) ( ) ( ) 1 0 1 −1 −1 1 0 1 0 −1 −1 0 , , , , , . 0 1 1 0 −1 0 −1 1 1 −1 0 −1 4.4.10. Hint. (a) 0; (b) 1, −1. 4.4.11. Hint. 1, 2, 3, 4, 6, 8, 12, 24. 4.4.15. Hint. (a) −3 + 3i; (c) 43 − 18i; (e) i √ 4.4.16. Hint. (a) 3 + i; (c) −3. 311 √ √ 4.4.17. Hint. (a) 2 cis(7π/4); (c) 2 2 cis(π/4); (e) 3 cis(3π/2). √ 4.4.18. Hint. (a) (1 − i)/2; (c) 16(i − 3 ); (e) −1/4. 4.4.22. Hint. (a) 292; (c) 1523. 4.4.27. Hint. |⟨g⟩ ∩ ⟨h⟩| = 1. 4.4.31. Hint. The identity element in any group has finite order. Let g, h ∈ G have orders m and n, respectively. Since (g −1 )m = e and (gh)mn = e, the elements of finite order in G form a subgroup of G. 4.4.37. Hint. If g is an element distinct from the identity in G, g must generate G; otherwise, ⟨g⟩ is a nontrivial proper subgroup of G. 5 Permutation Groups 5.3 Exercises 5.3.1. Hint. (a) (12453); (c) (13)(25). 5.3.2. Hint. (a) (135)(24); (c) (14)(23); (e) (1324); (g) (134)(25); (n) (17352). 5.3.3. Hint. (a) (16)(15)(13)(14); (c) (16)(14)(12). 5.3.4. Hint. (a1 , a2 , . . . , an )−1 = (a1 , an , an−1 , . . . , a2 ) 5.3.5. Hint. (a) {(13), (13)(24), (132), (134), (1324), (1342)} is not a subgroup. 5.3.8. Hint. (12345)(678). 5.3.11. Hint. Permutations of the form (1), (a1 , a2 )(a3 , a4 ), (a1 , a2 , a3 ), (a1 , a2 , a3 , a4 , a5 ) are possible for A5 . 5.3.17. Hint. Calculate (123)(12) and (12)(123). 5.3.25. Hint. Consider the cases (ab)(bc) and (ab)(cd). 5.3.30. Hint. For (a), show that στ σ −1 (σ(ai )) = σ(ai+1 ). 6 Cosets and Lagrange’s Theorem 6.4 Exercises 6.4.1. Hint. The order of g and the order h must both divide the order of G. 6.4.2. Hint. The possible orders must divide 60. 6.4.3. Hint. This is true for every proper nontrivial subgroup. 6.4.4. Hint. False. 6.4.5. Hint. (a) ⟨8⟩, 1 + ⟨8⟩, 2 + ⟨8⟩, 3 + ⟨8⟩, 4 + ⟨8⟩, 5 + ⟨8⟩, 6 + ⟨8⟩, and 7 + ⟨8⟩; (c) 3Z, 1 + 3Z, and 2 + 3Z. 6.4.7. Hint. 4ϕ(15) ≡ 48 ≡ 1 (mod 15). 6.4.12. Hint. Let g1 ∈ gH. Show that g1 ∈ Hg and thus gH ⊂ Hg. 6.4.19. Hint. Show that g(H ∩ K) = gH ∩ gK. 6.4.22. Hint. If gcd(m, n) = 1, then ϕ(mn) = ϕ(m)ϕ(n) (Exercise 2.3.26 in Chapter 2). 312 APPENDIX B. HINTS AND SOLUTIONS TO SELECTED EXERCISES 7 Introduction to Cryptography 7.3 Exercises 7.3.1. Hint. LAORYHAPDWK 7.3.3. Hint. Hint: V = E, E = X (also used for spaces and punctuation), K = R. 7.3.4. Hint. 26! − 1 7.3.7. Hint. (a) 2791; (c) 11213525032442. 7.3.9. Hint. (a) 31 (c) 14. 7.3.10. Hint. (a) n = 11 · 41; (c) n = 8779 · 4327. 8 Algebraic Coding Theory 8.5 Exercises 8.5.2. Hint. This cannot be a group code since (0000) ∈ / C. 8.5.3. Hint. (a) 2; (c) 2. 8.5.4. Hint. (a) 3; (c) 4. 8.5.6. Hint. (a) dmin = 2; (c) dmin = 1. 8.5.7. Hint. (a) (00000), (00101), (10011), (10110) 0 1 0 0 G = 1 0 0 1 1 1 (b) (000000), (010111), (101101), (111010) 1 0 0 1 1 0 G= 1 1 0 1 1 1 8.5.9. Hint. Multiple errors occur in one of the received words. 8.5.11. Hint. (a) A canonical parity-check matrix with standard generator matrix 1 1 G = 0 . 0 1 313 (c) A canonical parity-check matrix with standard generator matrix 1 0 0 1 G= . 1 1 1 0 8.5.12. Hint. (a) All possible syndromes occur. 8.5.15. Hint. (a) C, (10000) + C, (01000) + C, (00100) + C, (00010) + C, (11000) + C, (01100) + C, (01010) + C. A decoding table does not exist for C since this is only a single error-detecting code. 8.5.19. Hint. Let x ∈ C have odd weight and define a map from the set of odd codewords to the set of even codewords by y 7→ x + y. Show that this map is a bijection. 8.5.23. Hint. For 20 information positions, at least 6 check bits are needed to ensure an error-correcting code. 9 Isomorphisms 9.3 Exercises 9.3.1. Hint. Every infinite cyclic group is isomorphic to Z by Theorem 9.7. 9.3.2. Hint. Define ϕ : C∗ → GL2 (R) by ( ) a b ϕ(a + bi) = . −b a 9.3.3. Hint. False. 9.3.6. Hint. Define a map from Zn into the nth roots of unity by k 7→ cis(2kπ/n). 9.3.8. Hint. Assume that Q is cyclic and try to find a generator. 9.3.11. Hint. There are two nonabelian and three abelian groups that are not isomor- phic. 9.3.16. Hint. (a) 12; (c) 5. 9.3.19. Hint. Draw the picture. 9.3.20. Hint. True. 9.3.25. Hint. True. 9.3.27. Hint. Let a be a generator for G. If ϕ : G → H is an isomorphism, show that ϕ(a) is a generator for H. 9.3.38. Hint. Any automorphism of Z6 must send 1 to another generator of Z6 . 9.3.45. Hint. To show that ϕ is one-to-one, let g1 = h1 k1 and g2 = h2 k2 and consider ϕ(g1 ) = ϕ(g2 ). 314 APPENDIX B. HINTS AND SOLUTIONS TO SELECTED EXERCISES 10 Normal Subgroups and Factor Groups 10.3 Exercises 10.3.1. Hint. (a) A4 (12)A4 A4 A4 (12)A4 (12)A4 (12)A4 A4 (c) D4 is not normal in S4 . 10.3.8. Hint. If a ∈ G is a generator for G, then aH is a generator for G/H. 10.3.11. Hint. For any g ∈ G, show that the map ig : G → G defined by ig : x 7→ gxg −1 is an isomorphism of G with itself. Then consider ig (H). 10.3.12. Hint. Suppose that ⟨g⟩ is normal in G and let y be an arbitrary element of G. If x ∈ C(g), we must show that yxy −1 is also in C(g). Show that (yxy −1 )g = g(yxy −1 ). 10.3.14. Hint. (a) Let g ∈ G and h ∈ G′ . If h = aba−1 b−1 , then ghg −1 = gaba−1 b−1 g −1 = (gag −1 )(gbg −1 )(ga−1 g −1 )(gb−1 g −1 ) = (gag −1 )(gbg −1 )(gag −1 )−1 (gbg −1 )−1 . We also need to show that if h = h1 · · · hn with hi = ai bi a−1 −1 i bi , then ghg −1 is a product of elements of the same type. However, ghg −1 = gh1 · · · hn g −1 = (gh1 g −1 )(gh2 g −1 ) · · · (ghn g −1 ). 11 Homomorphisms 11.3 Exercises 11.3.2. Hint. (a) is a homomorphism with kernel {1}; (c) is not a homomorphism. 11.3.4. Hint. Since ϕ(m + n) = 7(m + n) = 7m + 7n = ϕ(m) + ϕ(n), ϕ is a homomor- phism. 11.3.5. Hint. For any homomorphism ϕ : Z24 → Z18 , the kernel of ϕ must be a subgroup of Z24 and the image of ϕ must be a subgroup of Z18 . Now use the fact that a generator must map to a generator. 11.3.9. Hint. Let a, b ∈ G. Then ϕ(a)ϕ(b) = ϕ(ab) = ϕ(ba) = ϕ(b)ϕ(a). 11.3.17. Hint. Find a counterexample. 12 Matrix Groups and Symmetry 12.3 Exercises 12.3.1. Hint. 1[ ] 1[ ] ∥x + y∥2 + ∥x∥2 − ∥y∥2 = ⟨x + y, x + y⟩ − ∥x∥2 − ∥y∥2 2 2 1[ ] = ∥x∥2 + 2⟨x, y⟩ + ∥y∥2 − ∥x∥2 − ∥y∥2 2 = ⟨x, y⟩. 315 12.3.3. Hint. (a) is in SO(2); (c) is not in O(3). 12.3.5. Hint. (a) ⟨x, y⟩ = ⟨y, x⟩. 12.3.7. Hint. Use the unimodular matrix ( ) 5 2 . 2 1 12.3.10. Hint. Show that the kernel of the map det : O(n) → R∗ is SO(n). 12.3.13. Hint. True. 12.3.17. Hint. p6m 13 The Structure of Groups 13.3 Exercises 13.3.1. Hint. There are three possible groups. 13.3.4. Hint. (a) {0} ⊂ ⟨6⟩ ⊂ ⟨3⟩ ⊂ Z12 ; (e) {(1)} × {0} ⊂ {(1), (123), (132)} × {0} ⊂ S3 × {0} ⊂ S3 × ⟨2⟩ ⊂ S3 × Z4 . 13.3.7. Hint. Use the Fundamental Theorem of Finitely Generated Abelian Groups. 13.3.12. Hint. If N and G/N are solvable, then they have solvable series N = Nn ⊃ Nn−1 ⊃ · · · ⊃ N1 ⊃ N0 = {e} G/N = Gn /N ⊃ Gn−1 /N ⊃ · · · G1 /N ⊃ G0 /N = {N }. 13.3.16. Hint. Use the fact that Dn has a cyclic subgroup of index 2. 13.3.21. Hint. G/G′ is abelian. 14 Group Actions 14.4 Exercises 14.4.1. Hint. Example 14.1: 0, R2 \ {0}. Example 14.2: X = {1, 2, 3, 4}. 14.4.2. Hint. (a) X(1) = {1, 2, 3}, X(12) = {3}, X(13) = {2}, X(23) = {1}, X(123) = X(132) = ∅. G1 = {(1), (23)}, G2 = {(1), (13)}, G3 = {(1), (12)}. 14.4.3. Hint. (a) O1 = O2 = O3 = {1, 2, 3}. 14.4.6. Hint. The conjugacy classes for S4 are O(1) = {(1)}, O(12) = {(12), (13), (14), (23), (24), (34)}, O(12)(34) = {(12)(34), (13)(24), (14)(23)}, O(123) = {(123), (132), (124), (142), (134), (143), (234), (243)}, O(1234) = {(1234), (1243), (1324), (1342), (1423), (1432)}. The class equation is 1 + 3 + 6 + 6 + 8 = 24. 14.4.8. Hint. (34 + 31 + 32 + 31 + 32 + 32 + 33 + 33 )/8 = 21. 316 APPENDIX B. HINTS AND SOLUTIONS TO SELECTED EXERCISES 14.4.11. Hint. The group of rigid motions of the cube can be described by the allowable permutations of the six faces and is isomorphic to S4 . There are the identity cycle, 6 permutations with the structure (abcd) that correspond to the quarter turns, 3 permutations with the structure (ab)(cd) that correspond to the half turns, 6 permutations with the structure (ab)(cd)(ef ) that correspond to rotating the cube about the centers of opposite edges, and 8 permutations with the structure (abc)(def ) that correspond to rotating the cube about opposite vertices. 14.4.15. Hint. (1 · 26 + 3 · 24 + 4 · 23 + 2 · 22 + 2 · 21 )/12 = 13. 14.4.17. Hint. (1 · 28 + 3 · 26 + 2 · 24 )/6 = 80. 14.4.22. Hint. Use the fact that x ∈ gC(a)g −1 if and only if g −1 xg ∈ C(a). 15 The Sylow Theorems 15.3 Exercises 15.3.1. Hint. If |G| = 18 = 2 · 32 , then the order of a Sylow 2-subgroup is 2, and the order of a Sylow 3-subgroup is 9. 15.3.2. Hint. The four Sylow 3-subgroups of S4 are P1 = {(1), (123), (132)}, P2 = {(1), (124), (142)}, P3 = {(1), (134), (143)}, P4 = {(1), (234), (243)}. 15.3.5. Hint. Since |G| = 96 = 25 · 3, G has either one or three Sylow 2-subgroups by the Third Sylow Theorem. If there is only one subgroup, we are done. If there are three Sylow 2-subgroups, let H and K be two of them. Therefore, |H ∩ K| ≥ 16; otherwise, HK would have (32 · 32)/8 = 128 elements, which is impossible. Thus, H ∩ K is normal in both H and K since it has index 2 in both groups. 15.3.8. Hint. Show that G has a normal Sylow p-subgroup of order p2 and a normal Sylow q-subgroup of order q 2 . 15.3.10. Hint. False. 15.3.17. Hint. If G is abelian, then G is cyclic, since |G| = 3 · 5 · 17. Now look at Example 15.14. 15.3.23. Hint. Define a mapping between the right cosets of N (H) in G and the conjugates of H in G by N (H)g 7→ g −1 Hg. Prove that this map is a bijection. 15.3.26. Hint. Let aG′ , bG′ ∈ G/G′ . Then (aG′ )(bG′ ) = abG′ = ab(b−1 a−1 ba)G′ = (abb−1 a−1 )baG′ = baG′ . 16 Rings 16.6 Exercises √ 16.6.1. Hint. (a) 7Z is a ring but not a field; (c) Q( 2 ) is a field; (f) R is not a ring. 16.6.3. Hint. (a) {1, 3, 7, 9}; (c) {1, 2, 3, 4, 5, 6}; (e) {( ) ( ) ( ) ( ) ( ) ( ) } 1 0 1 1 1 0 0 1 1 1 0 1 , , , , , , . 0 1 0 1 1 1 1 0 1 0 1 1 16.6.4. Hint. (a) {0}, {0, 9}, {0, 6, 12}, {0, 3, 6, 9, 12, 15}, {0, 2, 4, 6, 8, 10, 12, 14, 16}; (c) there are no nontrivial ideals. 16.6.7. Hint. Assume there is an isomorphism ϕ : C → R with ϕ(i) = a. 317 √ √ 16.6.8. √ Hint. False. Assume there is an isomorphism ϕ : Q( 2 ) → Q( 3 ) such that ϕ( 2 ) = a. 16.6.13. Hint. (a) x ≡ 17 (mod 55); (c) x ≡ 214 (mod 2772). 16.6.16. Hint. If I ̸= {0}, show that 1 ∈ I. 16.6.18. Hint. (a) ϕ(a)ϕ(b) = ϕ(ab) = ϕ(ba) = ϕ(b)ϕ(a). 16.6.26. Hint. Let a ∈ R with a ̸= 0. Then the principal ideal generated by a is R. Thus, there exists a b ∈ R such that ab = 1. 16.6.28. Hint. Compute (a + b)2 and (−ab)2 . 16.6.34. Hint. Let a/b, c/d ∈ Z(p) . Then a/b + c/d = (ad + bc)/bd and (a/b) · (c/d) = (ac)/(bd) are both in Z(p) , since gcd(bd, p) = 1. 16.6.38. Hint. Suppose that x2 = x and x ̸= 0. Since R is an integral domain, x = 1. To find a nontrivial idempotent, look in M2 (R). 17 Polynomials 17.4 Exercises 17.4.2. Hint. (a) 9x2 + 2x + 5; (b) 8x4 + 7x3 + 2x2 + 7x. 17.4.3. Hint. (a) 5x3 + 6x2 − 3x + 4 = (5x2 + 2x + 1)(x − 2) + 6; (c) 4x5 − x3 + x2 + 4 = (4x2 + 4)(x3 + 3) + 4x2 + 2. 17.4.5. Hint. (a) No zeros in Z12 ; (c) 3, 4. 17.4.7. Hint. Look at (2x + 1). 17.4.8. Hint. (a) Reducible; (c) irreducible. 17.4.10. Hint. One factorization is x2 + x + 8 = (x + 2)(x + 9). 17.4.13. Hint. The integers Z do not form a field. 17.4.14. Hint. False. 17.4.16. Hint. Let ϕ : R → S be an isomorphism. Define ϕ : R[x] → S[x] by ϕ(a0 + a1 x + · · · + an xn ) = ϕ(a0 ) + ϕ(a1 )x + · · · + ϕ(an )xn . 17.4.20. Cyclotomic Polynomials. Hint. The polynomial xn − 1 Φn (x) = = xn−1 + xn−2 + · · · + x + 1 x−1 is called the cyclotomic polynomial. Show that Φp (x) is irreducible over Q for any prime p. 17.4.26. Hint. Find a nontrivial proper ideal in F [x]. 18 Integral Domains 18.3 Exercises √ √ √ 18.3.1. Hint. Note that z −1 = 1/(a + b 3 i) = (a − b 3 i)/(a2 + 3b2 ) is in Z[ 3 i] if and only if a2 + 3b2 = 1. The only integer solutions to the equation are a = ±1, b = 0. 18.3.2. Hint. (a) 5 = −i(1 + 2i)(2 + i); (c) 6 + 8i = −i(1 + i)2 (2 + i)2 . 18.3.4. Hint. True. 18.3.9. Hint. Let z = a + bi and w = c + di ̸= 0 be in Z[i]. Prove that z/w ∈ Q(i). 318 APPENDIX B. HINTS AND SOLUTIONS TO SELECTED EXERCISES 18.3.15. Hint. Let a = ub with u a unit. Then ν(b) ≤ ν(ub) ≤ ν(a). Similarly, ν(a) ≤ ν(b). 18.3.16. Hint. Show that 21 can be factored in two different ways. 19 Lattices and Boolean Algebras 19.4 Exercises 19.4.2. Hint. 30 10 15 2 5 3 1 19.4.5. Hint. False. 19.4.6. Hint. (a) (a ∨ b ∨ a′ ) ∧ a a b a a′ (c) a ∨ (a ∧ b) a b a 19.4.8. Hint. Not equivalent. 19.4.10. Hint. (a) a′ ∧ [(a ∧ b′ ) ∨ b] = a ∧ (a ∨ b). 319 19.4.14. Hint. Let I, J be ideals in R. We need to show that I + J = {r + s : r ∈ I and s ∈ J} is the smallest ideal in R containing both I and J. If r1 , r2 ∈ I and s1 , s2 ∈ J, then (r1 + s1 ) + (r2 + s2 ) = (r1 + r2 ) + (s1 + s2 ) is in I + J. For a ∈ R, a(r1 + s1 ) = ar1 + as1 ∈ I + J; hence, I + J is an ideal in R. 19.4.18. Hint. (a) No. 19.4.20. Hint. (⇒). a = b ⇒ (a ∧ b′ ) ∨ (a′ ∧ b) = (a ∧ a′ ) ∨ (a′ ∧ a) = O ∨ O = O. (⇐). (a ∧ b′ ) ∨ (a′ ∧ b) = O ⇒ a ∨ b = (a ∨ a) ∨ b = a ∨ (a ∨ b) = a ∨ [I ∧ (a ∨ b)] = a ∨ [(a ∨ a′ ) ∧ (a ∨ b)] = [a ∨ (a ∧ b′ )] ∨ [a ∨ (a′ ∧ b)] = a ∨ [(a ∧ b′ ) ∨ (a′ ∧ b)] = a ∨ 0 = a. A symmetric argument shows that a ∨ b = b. 20 Vector Spaces 20.4 Exercises √ √ √ √ √ 20.4.3. Hint. Q( 2, 3 ) has basis {1, 2, 3, 6 } over Q. 20.4.5. Hint. The set {1, x, x2 , . . . , xn−1 } is a basis for Pn . 20.4.7. Hint. (a) Subspace of dimension 2 with basis {(1, 0, −3), (0, 1, 2)}; (d) not a subspace 20.4.10. Hint. Since 0 = α0 = α(−v + v) = α(−v) + αv, it follows that −αv = α(−v). 20.4.12. Hint. Let v0 = 0, v1 , . . . , vn ∈ V and α0 ̸= 0, α1 , . . . , αn ∈ F . Then α0 v0 + · · · + αn vn = 0. 20.4.15. Linear Transformations. Hint. (a) Let u, v ∈ ker(T ) and α ∈ F . Then T (u + v) = T (u) + T (v) = 0 T (αv) = αT (v) = α0 = 0. Hence, u + v, αv ∈ ker(T ), and ker(T ) is a subspace of V . (c) The statement that T (u) = T (v) is equivalent to T (u − v) = T (u) − T (v) = 0, which is true if and only if u − v = 0 or u = v. 20.4.17. Direct Sums. Hint. (a) Let u, u′ ∈ U and v, v ′ ∈ V . Then (u + v) + (u′ + v ′ ) = (u + u′ ) + (v + v ′ ) ∈ U + V α(u + v) = αu + αv ∈ U + V. 21 Fields 21.4 Exercises 21.4.1. Hint. (a) x4 − (2/3)x2 − 62/9; (c) x4 − 2x2 + 25. √ √ √ √ √ 21.4.2. Hint. (a) {1, 2, 3, 6 }; (c) {1, i, 2, 2 i}; (e) {1, 21/6 , 21/3 , 21/2 , 22/3 , 25/6 }. √ √ 21.4.3. Hint. (a) Q( 3, 7 ). 21.4.5. Hint. Use the fact that the elements of Z2 [x]/⟨x3 + x + 1⟩ are 0, 1, α, 1 + α, α , 1 + α , α + α2 , 1 + α + α2 and the fact that α3 + α + 1 = 0. 2 2 21.4.8. Hint. False. 21.4.14. Hint. Suppose that E is algebraic over F and K is algebraic over E. Let α ∈ K. It suffices to show that α is algebraic over some finite extension of F . Since α is 320 APPENDIX B. HINTS AND SOLUTIONS TO SELECTED EXERCISES algebraic over E, it must be the zero of some polynomial p(x) = β0 + β1 x + · · · + βn xn in E[x]. Hence α is algebraic over F (β0 , . . . , βn ). √ √ √ √ √ √ √ 21.4.22. √ √ Hint. Since {1, √ √ 3, 7, 21 } is √a basis √ for Q( 3, 7 ) over Q, Q( 3, 7 ) ⊃ Q( 3 + 7 ). Since [Q( 3,√ 7 ) :√Q] = 4, [Q( √ 3√+ 7 ) : Q] √ = 2√or 4. Since the degree of the minimal polynomial of 3 + 7 is 4, Q( 3, 7 ) = Q( 3 + 7 ). 21.4.27. Hint. Let β ∈ F (α) not in F . Then β = p(α)/q(α), where p and q are polynomials in α with q(α) ̸= 0 and coefficients in F . If β is algebraic over F , then there exists a polynomial f (x) ∈ F [x] such that f (β) = 0. Let f (x) = a0 + a1 x + · · · + an xn . Then ( ) ( ) ( ) p(α) p(α) p(α) n 0 = f (β) = f = a0 + a1 + · · · + an . q(α) q(α) q(α) Now multiply both sides by q(α)n to show that there is a polynomial in F [x] that has α as a zero. 21.4.28. Hint. See the comments following Theorem 21.13. 22 Finite Fields 22.3 Exercises 22.3.1. Hint. Make sure that you have a field extension. 22.3.4. Hint. There are eight elements in Z2 (α). Exhibit two more zeros of x3 + x2 + 1 other than α in these eight elements. 22.3.5. Hint. Find an irreducible polynomial p(x) in Z3 [x] of degree 3 and show that Z3 [x]/⟨p(x)⟩ has 27 elements. 22.3.7. Hint. (a) x5 − 1 = (x + 1)(x4 + x3 + x2 + x + 1); (c) x9 − 1 = (x + 1)(x2 + x + 1)(x6 + x3 + 1). 22.3.8. Hint. True. 22.3.11. Hint. (a) Use the fact that x7 − 1 = (x + 1)(x3 + x + 1)(x3 + x2 + 1). 22.3.12. Hint. False. 22.3.17. Hint. If p(x) ∈ F [x], then p(x) ∈ E[x]. 22.3.18. Hint. Since α is algebraic over F of degree n, we can write any element β ∈ F (α) uniquely as β = a0 + a1 α + · · · + an−1 αn−1 with ai ∈ F . There are q n possible n-tuples (a0 , a1 , . . . , an−1 ). 22.3.24. Wilson’s Theorem. Hint. Factor xp−1 − 1 over Zp . 23 Galois Theory 23.4 Exercises 23.4.1. Hint. (a) Z2 ; (c) Z2 × Z2 × Z2 . 23.4.2. Hint. (a) Separable over Q since x3 + 2x2 − x − 2 = (x − 1)(x + 1)(x + 2); (c) not separable over Z3 since x4 + x2 + 1 = (x + 1)2 (x + 2)2 . 23.4.3. Hint. If [GF(729) : GF(9)] = [GF(729) : GF(3)]/[GF(9) : GF(3)] = 6/2 = 3, 321 then G(GF(729)/ GF(9)) ∼ = Z3 . A generator for G(GF(729)/ GF(9)) is σ, where σ36 (α) = 6 α3 = α729 for α ∈ GF(729). 23.4.4. Hint. (a) S5 ; (c) S3 ; (g) see Example 23.10. 23.4.5. Hint. (a) Q(i) 23.4.7. Hint. Let E be the splitting field of a cubic polynomial in F [x]. Show that [E : F ] is less than or equal to 6 and is divisible by 3. Since G(E/F ) is a subgroup of S3 whose order is divisible by 3, conclude that this group must be isomorphic to Z3 or S3 . 23.4.9. Hint. G is a subgroup of Sn . 23.4.16. Hint. True. 23.4.20. Hint. (a) Clearly ω, ω 2 , . . . , ω p−1 are distinct since ω ̸= 1 or 0. To show that ω i is a zero of Φp , calculate Φp (ω i ). (b) The conjugates of ω are ω, ω 2 , . . . , ω p−1 . Define a map ϕi : Q(ω) → Q(ω i ) by ϕi (a0 + a1 ω + · · · + ap−2 ω p−2 ) = a0 + a1 ω i + · · · + cp−2 (ω i )p−2 , where ai ∈ Q. Prove that ϕi is an isomorphism of fields. Show that ϕ2 generates G(Q(ω)/Q). (c) Show that {ω, ω 2 , . . . , ω p−1 } is a basis for Q(ω) over Q, and consider which linear combinations of ω, ω 2 , . . . , ω p−1 are left fixed by all elements of G(Q(ω)/Q). C Notation The following table defines the notation used in this book. Page numbers or references refer to the first appearance of each symbol. Symbol Description Page a∈A a is in the set A 3 N the natural numbers 4 Z the integers 4 Q the rational numbers 4 R the real numbers 4 C the complex numbers 4 A⊂B A is a subset of B 4 ∅ the empty set 4 A∪B the union of sets A and B 4 A∩B the intersection of sets A and B 4 A′ complement of the set A 4 A\B difference between sets A and B 4 A×B Cartesian product of sets A and B 6 An A × · · · × A (n times) 6 id identity mapping 9 f −1 inverse of the function f 9 a ≡ b (mod n) a is congruent to b modulo n 12 n! n factorial 18 (n) k binomial coefficient n!/(k!(n − k)!) 18 a|b a divides b 20 gcd(a, b) greatest common divisor of a and b 20 P(X) power set of X 24 lcm(m, n) the least common multiple of m and n 25 Zn the integers modulo n 27 U (n) group of units in Zn 32 Mn (R) the n × n matrices with entries in R 33 det A the determinant of A 33 GLn (R) the general linear group 33 Q8 the group of quaternions 33 C∗ the multiplicative group of complex numbers 33 |G| the order of a group 34 (Continued on next page) 322 323 Symbol Description Page R∗ the multiplicative group of real numbers 36 Q∗ the multiplicative group of rational numbers 36 SLn (R) the special linear group 36 Z(G) the center of a group 41 ⟨a⟩ cyclic group generated by a 44 |a| the order of an element a 44 cis θ cos θ + i sin θ 48 T the circle group 49 Sn the symmetric group on n letters 56 (a1 , a2 , . . . , ak ) cycle of length k 58 An the alternating group on n letters 61 Dn the dihedral group 62 [G : H] index of a subgroup H in a group G 70 LH the set of left cosets of a subgroup H in a group G 71 RH the set of right cosets of a subgroup H in a group G 71 a∤b a does not divide b 73 d(x, y) Hamming distance between x and y 88 dmin the minimum distance of a code 88 w(x) the weight of x 88 Mm×n (Z2 ) the set of m × n matrices with entries in Z2 92 Null(H) null space of a matrix H 92 δij Kronecker delta 96 G∼ =H G is isomorphic to a group H 106 Aut(G) automorphism group of a group G 115 ig ig (x) = gxg −1 115 Inn(G) inner automorphism group of a group G 115 ρg right regular representation 115 G/N factor group of G mod N 118 G′ commutator subgroup of G 123 ker ϕ kernel of ϕ 125 (aij ) matrix 133 O(n) orthogonal group 135 ∥x∥ length of a vector x 135 SO(n) special orthogonal group 138 E(n) Euclidean group 138 Ox orbit of x 159 Xg fixed point set of g 159 Gx isotropy subgroup of x 159 N (H) normalizer of s subgroup H 173 H the ring of quaternions 183 Z[i] the Gaussian integers 184 char R characteristic of a ring R 185 Z(p) ring of integers localized at p 197 deg f (x) degree of a polynomial 200 (Continued on next page) 324 APPENDIX C. NOTATION Symbol Description Page R[x] ring of polynomials over a ring R 201 R[x1 , x2 , . . . , xn ] ring of polynomials in n indeterminants 203 ϕα evaluation homomorphism at α 203 Q(x) field of rational functions over Q 219 ν(a) Euclidean valuation of a 222 F (x) field of rational functions in x 226 F (x1 , . . . , xn ) field of rational functions in x1 , . . . , xn 226 a⪯b a is less than b 229 a∨b join of a and b 231 a∧b meet of a and b 231 I largest element in a lattice 232 O smallest element in a lattice 232 a′ complement of a in a lattice 232 dim V dimension of a vector space V 247 U ⊕V direct sum of vector spaces U and V 249 Hom(V, W ) set of all linear transformations from U into V 249 V∗ dual of a vector space V 249 F (α1 , . . . , αn ) smallest field containing F and α1 , . . . , αn 253 [E : F ] dimension of a field extension of E over F 256 GF(pn ) Galois field of order pn 271 F∗ multiplicative group of a field F 272 G(E/F ) Galois group of E over F 284 F{σi } field fixed by the automorphism σi 287 FG field fixed by the automorphism group G 287 ∆2 discriminant of a polynomial 299 Index G-equivalent, 159 Cauchy’s Theorem, 172 G-set, 158 Cauchy, Augustin-Louis, 62 nth root of unity, 49, 293 Cayley table, 32 rsa cryptosystem, 78 Cayley’s Theorem, 109 Cayley, Arthur, 109 Abel, Niels Henrik, 292 Centralizer Abelian group, 31 of a subgroup, 161 Adleman, L., 78 Characteristic of a ring, 185 Algebraic closure, 258 Chinese Remainder Theorem Algebraic extension, 253 for integers, 192 Algebraic number, 254 Cipher, 75 Algorithm Ciphertext, 75 division, 203 Circuit Euclidean, 22 parallel, 237 Ascending chain condition, 221 series, 237 Associate elements, 219 series-parallel, 237 Atom, 235 Class equation, 161 Automorphism Code inner, 130 bch, 278 Basis of a lattice, 141 cyclic, 273 Bieberbach, L., 144 group, 90 Binary operation, 31 linear, 93 Binary symmetric channel, 87 minimum distance of, 88 Boole, George, 239 polynomial, 274 Boolean algebra Commutative diagrams, 127 atom in a, 235 Commutative rings, 181 definition of, 233 Composite integer, 22 finite, 235 Composition series, 153 isomorphism, 235 Congruence modulo n, 12 Boolean function, 166, 241 Conjugacy classes, 161 Burnside’s Counting Theorem, 163 Conjugate elements, 284 Burnside, William, 35, 122, 168 Conjugate, complex, 47 Conjugation, 159 Cancellation law Constructible number, 262 for groups, 35 Correspondence Theorem for integral domains, 185 for groups, 128 Cardano, Gerolamo, 210 for rings, 189 Carmichael numbers, 83 Coset 325 326 INDEX leader, 100 irreducible, 219 left, 69 order of, 44 representative, 69 prime, 219 right, 69 primitive, 286 Coset decoding, 99 transcendental, 253 Cryptanalysis, 76 Equivalence class, 12 Cryptosystem Equivalence relation, 11 rsa, 78 Euclidean algorithm, 22 affine, 77 Euclidean domain, 222 definition of, 75 Euclidean group, 138 monoalphabetic, 76 Euclidean inner product, 135 polyalphabetic, 77 Euclidean valuation, 222 private key, 75 Euler ϕ-function, 72 public key, 75 Euler, Leonhard, 73, 266 single key, 75 Extension Cycle algebraic, 253 definition of, 57 field, 251 disjoint, 58 finite, 256 normal, 289 De Morgan’s laws radical, 293 for Boolean algebras, 234 separable, 270, 286 for sets, 5 simple, 253 De Morgan, Augustus, 239 External direct product, 110 Decoding table, 100 Deligne, Pierre, 266 Faltings, Gerd, 266 DeMoivre’s Theorem, 49 Feit, W., 122, 168 Derivative, 270 Fermat’s factorizationalgorithm, 82 Determinant, Vandermonde, 276 Fermat’s Little Theorem, 73 Dickson, L. E., 122 Fermat, Pierre de, 73, 266 Diffie, W., 77 Ferrari, Ludovico, 211 Direct product of groups Ferro, Scipione del, 210 external, 110 Field, 181 internal, 112 algebraically closed, 258 Discriminant base, 251 of the cubic equation, 214 extension, 251 of the quadratic equation, 213 fixed, 287 Division algorithm Galois, 271 for integers, 20 of fractions, 218 for polynomials, 203 of quotients, 218 Division ring, 181 splitting, 259 Domain Finitely generated group, 148 Euclidean, 222 Fior, Antonio, 210 principal ideal, 220 First Isomorphism Theorem unique factorization, 219 for groups, 126 Doubling the cube, 265 for rings, 188 Fixed point set, 159 Eisenstein’s Criterion, 208 Freshman’s Dream, 269 Element Function associate, 219 bijective, 7 identity, 31 Boolean, 166, 241 inverse, 31 composition of, 7 INDEX 327 definition of, 6 homomorphism of, 124 domain of, 6 infinite, 34 identity, 9 isomorphic, 106 injective, 7 isomorphism of, 106 invertible, 9 nonabelian, 31 one-to-one, 7 noncommutative, 31 onto, 7 of units, 32 range of, 6 order of, 34 surjective, 7 orthogonal, 135 switching, 166, 241 permutation, 57 Fundamental Theorem point, 142 of Algebra, 259, 297 quaternion, 33 of Arithmetic, 22 quotient, 118 of Finite Abelian Groups, 149 simple, 119, 122 Fundamental Theorem of Galois Theory, solvable, 155 290 space, 142 special linear, 36, 134 Galois field, 271 special orthogonal, 138 Galois group, 284 symmetric, 56 Galois, Évariste, 35, 292 symmetry, 140 Gauss’s Lemma, 224 Groupp-group, 149 Gauss, Karl Friedrich, 225 Gödel, Kurt, 239 Gaussian integers, 184 Generator of a cyclic subgroup, 44 Hamming distance, 88 Generators for a group, 148 Hamming, R., 90 Glide reflection, 139 Hellman, M., 77 Gorenstein, Daniel, 122 Hilbert, David, 144, 190, 239, 266 Greatest common divisor Homomorphic image, 124 of two integers, 20 Homomorphism of two polynomials, 205 canonical, 126, 188 Greatest lower bound, 230 evaluation, 186, 203 Greiss, R., 122 kernel of a group, 125 Grothendieck, Alexander, 266 kernel of a ring, 186 Group natural, 126, 188 p-group, 172 of groups, 124 abelian, 31 ring, 186 action, 158 alternating, 61 Ideal center of, 161 definition of, 187 circle, 49 maximal, 189 commutative, 31 one-sided, 188 cyclic, 44 prime, 190 definition of, 31 principal, 187 dihedral, 62 trivial, 187 Euclidean, 138 two-sided, 188 factor, 118 Indeterminate, 200 finite, 34 Index of a subgroup, 70 finitely generated, 148 Induction Galois, 284 first principle of, 17 general linear, 33, 134 second principle of, 19 generators of, 148 Infimum, 230 328 INDEX Inner product, 91 generator, 93 Integral domain, 181 inner product-preserving, 136 Internal direct product, 112 invertible, 133 International standard book number, 42 length-preserving, 136 Irreducible element, 219 nonsingular, 133 Irreducible polynomial, 206 null space of, 92 Isometry, 138 orthogonal, 135 Isomorphism parity-check, 93 of Boolean algebras, 235 similar, 12 of groups, 106 unimodular, 142 ring, 186 Matrix, Vandermonde, 276 Maximal ideal, 189 Join, 231 Maximum-likelihood decoding, 87 Jordan, C., 122 Meet, 231 Jordan-Hölder Theorem, 154 Minimal generator polynomial, 275 Kernel Minimal polynomial, 254 of a group homomorphism, 125 Minkowski, Hermann, 266 of a ring homomorphism, 186 Monic polynomial, 200 Key Mordell-Weil conjecture, 266 definition of, 75 Multiplicity of a root, 286 private, 75 Noether, A. Emmy, 190 public, 75 Noether, Max, 190 single, 75 Normal extension, 289 Klein, Felix, 35, 132, 190 Normal series of a group, 152 Kronecker delta, 96, 136 Normal subgroup, 117 Kronecker, Leopold, 266 Kummer, Ernst, 266 Normalizer, 173 Null space Lagrange’s Theorem, 71 of a matrix, 92 Lagrange, Joseph-Louis, 35, 62, 73 Laplace, Pierre-Simon, 62 Odd Order Theorem, 177 Lattice Orbit, 159 completed, 232 Orthogonal group, 135 definition of, 231 Orthogonal matrix, 135 distributive, 233 Orthonormal set, 136 Lattice of points, 141 Lattices, Principle of Duality for, 231 Partial order, 229 Least upper bound, 230 Partially ordered set, 229 Left regular representation, 109 Partitions, 12 Lie, Sophus, 35, 175 Permutation Linear combination, 245 definition of, 9, 56 Linear dependence, 245 even, 61 Linear independence, 245 odd, 61 Linear map, 132 Permutation group, 57 Linear transformation Plaintext, 75 definition of, 8, 132 Polynomial Lower bound, 230 code, 274 content of, 223 Mapping, see Function definition of, 200 Matrix degree of, 200 distance-preserving, 136 error, 281 INDEX 329 error-locator, 281 Second Isomorphism Theorem greatest common divisor of, 205 for groups, 127 in n indeterminates, 203 for rings, 189 irreducible, 206 Shamir, A., 78 leading coefficient of, 200 Shannon, C., 90 minimal, 254 Simple extension, 253 minimal generator, 275 Simple group, 119 monic, 200 Simple root, 286 primitive, 223 Solvability by radicals, 293 root of, 205 Spanning set, 245 separable, 286 Splitting field, 259 zero of, 205 Squaring the circle is impossible, 265 Polynomial separable, 270 Standard decoding, 99 Poset Subgroup definition of, 229 p-subgroup, 172 largest element in, 232 centralizer, 161 smallest element in, 232 commutator, 176 Power set, 229 cyclic, 44 Prime element, 219 definition of, 36 Prime ideal, 190 index of, 70 Prime integer, 22 isotropy, 159 Primitive nth root of unity, 50, 293 normal, 117 Primitive element, 286 normalizer of, 173 Primitive Element Theorem, 287 proper, 36 Primitive polynomial, 223 stabilizer, 159 Principal ideal, 187 Sylowp-subgroup, 173 Principal ideal domain (pid), 220 translation, 142 Principal series, 153 trivial, 36 Pseudoprime, 82 Subnormal series of a group, 152 Subring, 184 Quaternions, 33, 183 Supremum, 230 Switch Resolvent cubic equation, 214 closed, 237 Rigid motion, 29, 138 definition of, 237 Ring open, 237 characteristic of, 185 Switching function, 166, 241 commutative, 181 Sylow p-subgroup, 173 definition of, 181 Sylow, Ludvig, 175 division, 181 Syndrome of a code, 98, 281 factor, 188 homomorphism, 186 Tartaglia, 210 isomorphism, 186 Third Isomorphism Theorem Noetherian, 221 for groups, 128 quotient, 188 for rings, 189 with identity, 181 Thompson, J., 122, 168 with unity, 181 Transcendental element, 253 Rivest, R., 78 Transcendental number, 254 Ruffini, P., 292 Transposition, 60 Russell, Bertrand, 239 Trisection of an angle, 265 Scalar product, 243 Unique factorization domain (ufd), 219 330 INDEX Unit, 181, 219 Weight of a codeword, 88 Universal Product Code, 41 Weil, André, 266 Upper bound, 230 Well-defined map, 7 Well-ordered set, 19 Vandermonde determinant, 276 Whitehead, Alfred North, 239 Vandermonde matrix, 276 Vector space basis of, 246 Zero definition of, 243 multiplicity of, 286 dimension of, 247 of a polynomial, 205 subspace of, 244 Zero divisor, 182 This book was authored and produced with PreTeXt.