
552 15 Lie groups
15.2.6 Peter–Weyl theorem
The volume element constructed in Section 15.2.4 has the feature that it is invariant. In
other words if we have a subset of the group manifold with volume V , then the image
set g under left multiplication has exactly the same volume. We can also construct a
volume element that is invariant under right multiplication by g, and in general these
will be different. For a group whose manifold is a compact set, however, both left- and
right-invariant volume elements coincide. The resulting measure on the group manifold
is called the Haar measure.
For a compact group, therefore, we can replace the sums over the group elements
that occur in the representation theory of finite groups, by convergent integrals over the
group elements using the invariant Haar measure, which is usually denoted by d[g].
The invariance property is expressed by d[g
1
g]=d[g] for any constant element g
1
.
This allows us to make a change-of-variables transformation, g → g
1
g, identical to that
which played such an important role in deriving the finite-group theorems. Consequently,
all the results from finite groups, such as the existence of an invariant inner product and
the orthogonality theorems, can be taken over by the simple replacement of a sum by
an integral. In particular, if we normalize the measure so that the volume of the group
manifold is unity, we have the orthogonality relation
d[g]
D
J
ij
(g)
∗
D
K
lm
(g) =
1
dim J
δ
JK
δ
il
δ
jm
. (15.81)
The Peter–Weyl theorem asserts that the representation matrices D
J
mn
(g) form a com-
plete set of orthogonal functions on the group manifold. In the case of SU(2) this tells
us that the spin J representation matrices
D
J
mn
(θ, φ, ψ) =J , m|e
−iJ
3
φ
e
−iJ
2
θ
e
−iJ
3
ψ
|J , n,
= e
−imφ
d
J
mn
(θ)e
−inψ
, (15.82)
which you will likely have seen in quantum mechanics courses,
1
are a complete set of
functions on the 3-sphere with orthogonality relation
1
16π
2
π
0
sin θdθ
2π
0
dφ
4π
0
dψ
D
J
mn
(θ, φ, ψ)
∗
D
J
m
n
(θ, φ, ψ)
=
1
2J + 1
δ
JJ
δ
mm
δ
nn
. (15.83)
Since the D
L
m0
(where L has to be an integer for n = 0 to be possible) are independent of
the third Euler angle, ψ, we can do the trivial integral over ψ to obtain the special case
1
4π
π
0
sin θdθ
2π
0
dφ
D
L
m0
(θ, φ)
∗
D
L
m
0
(θ, φ) =
1
2L + 1
δ
LL
δ
mm
. (15.84)
1
See, for example, G. Baym, Lectures on Quantum Mechanics, Chapter 17.