Burnside's lemma
Burnside's lemma, sometimes also called Burnside's counting theorem, the Cauchy–Frobenius lemma, or the orbit-counting theorem, is a result in group theory that is often useful in taking account of symmetry when counting mathematical objects. It was discovered by Augustin Louis Cauchy and Ferdinand Georg Frobenius, and became well known after William Burnside quoted it. The result enumerates orbits of a symmetry group acting on some objects: that is, it counts distinct objects, considering objects symmetric to each other as the same; or counting distinct objects up to a symmetry equivalence relation; or counting only objects in canonical form. For example, in describing possible organic compounds of certain type, one considers them up to spatial rotation symmetry: different rotated drawings of a given molecule are chemically identical.
Statement
Let be a finite group that acts on a set. For each in, let denote the set of elements in that are fixed by : that is, Burnside's lemma asserts the following formula for the number of orbits, denoted :Thus the number of orbits is equal to the average number of points fixed by an element of G. For an infinite group, there is still a bijection:
Examples
Necklaces
There are 8 possible bit strings of length 3, but tying together the string ends gives only four distinct 2-colored necklaces of length 3, given by the canonical forms 000, 001, 011, 111: the other strings 100 and 010 are equivalent to 001 by rotation, while 110 and 101 are equivalent to 011. That is, rotation equivalence splits the set of strings into four orbits: The Burnside formula uses the number of rotations, which is 3 including the null rotation, and the number of bit strings left unchanged by each rotation. All 8 bit vectors are unchanged by the null rotation, and two are unchanged by the other two rotations. Thus the number of orbits is:For length 4, there are 16 possible bit strings; 4 rotations; the null rotation leaves all 16 strings unchanged; the 1-rotation and 3-rotation each leave two strings unchanged ; the 2-rotation leaves 4 bit strings unchanged. The number of distinct necklaces is thus:, represented by the canonical forms 0000, 0001, 0011, 0101, 0111, 1111.
The general case of n bits and k colors is given by a necklace polynomial.
Colorings of a cube
Burnside's lemma can compute the number of rotationally distinct colourings of the faces of a cube using three colours.Let be the set of 36 possible face color combinations that can be applied to a fixed cube, and let the rotation group G of the cube act on by moving the colored faces: two colorings in belong to the same orbit precisely when one is a rotation of the other. Rotationally distinct colorings correspond to group orbits, and can be found by counting the sizes of the fixed sets for the 24 elements of G, the colorings left unchanged by each rotation:
- the identity element fixes all 36 colorings
- six 90-degree face rotations each fix 33 colorings
- three 180-degree face rotations each fix 34 colorings
- eight 120-degree vertex rotations each fix 32 colorings
- six 180-degree edge rotations each fix 33 colorings.
here.
The average fixed-set size is thus:
There are 57 rotationally distinct colourings of the faces of a cube in three colours. In general, the number of rotationally distinct colorings of the faces of a cube in n colors is:
Conjugacy Classes
Let be a finite group. Consider the group action of on itself given by the conjugation map where.The orbits are the conjugacy classes of and the set of fixed points of an element is the centralizer.
Thus by Burnside's lemma, the number of conjugacy classes of G is equal to, that is, the average size of the centralizer.
Proof
In the proof of Burnside's lemma, the first step is to re-express the sum over the group elements g ∈ G as an equivalent sum over the set of elements x ∈ X:Here is the set of points of fixed by the element of, whereas is the stabilizer subgroup of, consisting of those symmetries that fix the point.)
The orbit-stabilizer theorem says that for each there is a natural bijection between the orbit and the set of left cosets. Lagrange's theorem implies that
The sum may therefore be rewritten as
Writing as the disjoint union of its orbits in gives
Putting everything together gives the desired result:
This is similar to the proof of the conjugacy class equation, which considers the conjugation action of on itself, that is, it is the case and, so that the stabilizer of is the centralizer.