Chapter I
Symmetry for Differential Equations
In the 1870s the Norwegian mathematician Sophus Lie set out to do for differential equations what Galois had done for polynomials: understand when they can be solved through their symmetries. Those symmetries are continuous, like rotations by any angle, so they form smooth groups, now called Lie groups. Lie saw that such a group is governed by its "infinitesimal" transformations, which form a simpler linear object, a Lie algebra.
Which Lie algebras are possible? Wilhelm Killing, teaching at a small-town lyceum, answered in 1888–90. The simple ones fall into four infinite families and exactly five exceptions, the largest being , of dimension 248. His proofs were flawed. Élie Cartan made them rigorous in 1894. Credit went mostly to Cartan for decades, and historians now argue that Killing's paper was one of the most remarkable ever written.
Chapter II
Groups as Matrices
For finite groups the key move came from Ferdinand Georg Frobenius in 1896. Answering a question Dedekind had raised in their letters, he let a group act on a vector space, turning each element into a matrix, and invented characters, the traces of those matrices. From a small table of numbers, much of a group's structure can be read. Burnside and Schur built the theory out within a decade, and it became the main tool of group theory.
Chapter III
The Language of Physics
Quantum mechanics made the subject physics. Hermann Weyl and Eugene Wigner showed that the energy levels of atoms, the rules for which transitions emit light, and the property of spin are all dictated by how symmetry groups are represented on quantum states. Many physicists at first resented the "group pest". By 1961 Murray Gell-Mann and Yuval Ne'eman were sorting the newly found particles into representations of and predicting new ones. The Standard Model is built on Lie groups.
Chapter IV
A Closer Look: The Character Table of a Triangle
The six symmetries of an equilateral triangle form the group : the identity, two rotations (by and ), and three flips. Symmetries that are "the same kind", such as the three flips, are grouped into classes. Here there are three classes, of sizes 1, 3 and 2.
A representation assigns each symmetry a matrix. has exactly three irreducible representations:
- trivial: every symmetry becomes the matrix ;
- sign: rotations become and flips become , recording whether the triangle has been turned over;
- standard: each symmetry becomes the matrix that actually rotates or reflects the plane.
The character of a representation records the trace of each matrix, one number per class:
| identity (1) | flips (3) | rotations (2) | |
|---|---|---|---|
| trivial | 1 | 1 | 1 |
| sign | 1 | 1 | |
| standard | 2 | 0 |
This small table obeys striking laws. The squares of the dimensions (first column) add up to the size of the group: . Any two different rows are orthogonal once each column is weighted by its class size. For example, trivial and standard give . These laws hold for every finite group, and they let mathematicians pin down groups, including the Monster, through character tables alone.
In quantum mechanics the same table is physics. A molecule with threefold symmetry, such as ammonia, a pyramid on a triangular base, has this symmetry group, and its vibrations and electron orbitals sort themselves into these three types. The table predicts which vibrations can absorb infrared light, before anyone looks at a spectrum.
Chapter V
Moonshine
The strangest chapter came from a coincidence. In 1978 John McKay noticed that , a coefficient in the -function of number theory, is one more than , the smallest dimension in which the newly predicted Monster group can act. John Conway and Simon Norton called the web of such coincidences "monstrous moonshine". In 1992 Richard Borcherds proved it, using the vertex algebras of string theory. The largest sporadic symmetry group, a modular function and a physical theory turned out to be one structure. Why that should be so is still not fully understood.