Consider the finite dimensional unitary representations α,β,γ of the given compact group G on corresponding vector spaces V1,V2,V3. Let |i>j,i=1,…,nj be an orthnormal basis of Vj where dimVj=nj. Then
{|i>1⊗|j>2⊗|k>3} forms an orthonormal basis of V=V1⊗V2⊗V3. An element g∈G acts on the tensor product space V as
|i>1⊗|j>2⊗|k>3→α(g)|i>1⊗β(g)|j>2⊗γ(g)|k>3
We can also find an orthogonal basis eμ,μ=1,…,N (where N=n1n2n3) of V relative to which all elements g∈G act as block diagonal matrices. More precisely, suppose with respect to basis {eμ}, the action of an element g∈G on V be denoted as
eμ→ρ(g)eμ
then ρ(g)νμ=<ν|ρ(g)|μ> is a block diagonal matrix where the dimensions of different blocks1 are independent of g. Let
|i>1⊗|j>2⊗|k>3=∑μϵμijkeμ
Acting with g∈G on both sides of this equation gives
α(g)|i>1⊗β(g)|j>2⊗γ(g)|k>3=∑μϵμijkρ(g)eμ
Taking the scalar product with |i′>1⊗|j′>2⊗|k′>3 and using (3) we get
α(g)i′iβ(g)j′jγ(g)k′k=∑μ,νρνμ(g)ϵ∗νi′j′k′ϵμijk
Now, according to the Peter-Weyl theorem (part 2), matrix elements of the irreducible representations of G form an orthogonal basis of the space of square integrable functions on G wrt the inner product
(A,B)=∫GdgA(g)∗B(g)
where dg is the Haar measure. So, if we integrate both sides of (5), the nonzero contribution on RHS will only come from the part of ρ which is direct sum of identity representations. In other words, let W⊆V be the subspace of V on which G acts trivially, and let {e1,…em}⊆ {e1,…em,…,eN} be the basis of W, then the integration of (5) gives
∫Gdgα(g)i′iβ(g)j′jγ(g)k′k=m∑μ,ν=1δνμϵ∗νi′j′k′ϵμijk=m∑μ=1ϵ∗μi′j′k′ϵμijk
where we have assumed that Vol(G)=∫Gdg=1
For the second part of your question, I would recommend these lecture notes. The basic idea for computing Wilson loop averages is following -
For a surface with boundary, the partition function of two dimensional Yang-Mills theory depends on the holonomy along the boundary. Let the partition function of a surface of genus h and one boundary be denoted as Zh(U,ag2) where U is the fixed holonomy along the given boundary, a is the area of the surface and g is the Yang-Mills coupling constant. Now, consider the simplest situation in which a Wilson loop W in representation RW is inserted along a contractible loop C on a closed surface of genus h, and area a. To compute the Wilson loop average, we first cut the surface along C, which gives a disc D of area (say) b and another surface S of area c=a−b, genus h and one boundary. Now the Wilson loop average is given by integrating over G the product of i) the partition functions of D ii) partition function of S and iii) the trace of the Wilson loop in representation RW -
<W>=1Zh(ag2)∫dUZh(U,(a−b)g2)χRW(U)Z0(U−1,bg2)
The case of a self-intersecting Wilson loop too is not very different.
1 The smallest blocks form irreducible representations of G; Exactly which irreducible representations show up will depend on α,β,γ; The same irreducible representations may also appear more than once
This post imported from StackExchange Physics at 2014-06-17 22:45 (UCT), posted by SE-user user10001