Theta representation

In mathematics, the theta representation is a particular representation of the Heisenberg group of quantum mechanics. It gains its name from the fact that the Jacobi theta function is invariant under the action of a discrete subgroup of the Heisenberg group. The representation was popularized by David Mumford.

Construction

The theta representation is a representation of the continuous Heisenberg group H 3 ( R ) {\displaystyle H_{3}(\mathbb {R} )} over the field of the real numbers. In this representation, the group elements act on a particular Hilbert space. The construction below proceeds first by defining operators that correspond to the Heisenberg group generators. Next, the Hilbert space on which these act is defined, followed by a demonstration of the isomorphism to the usual representations.

Group generators

Let f(z) be a holomorphic function, let a and b be real numbers, and let τ {\displaystyle \tau } be an arbitrary fixed complex number in the upper half-plane; that is, so that the imaginary part of τ {\displaystyle \tau } is positive. Define the operators Sa and Tb such that they act on holomorphic functions as

( S a f ) ( z ) = f ( z + a ) = exp ( a z ) f ( z ) {\displaystyle (S_{a}f)(z)=f(z+a)=\exp(a\partial _{z})f(z)}

and

( T b f ) ( z ) = exp ( i π b 2 τ + 2 π i b z ) f ( z + b τ ) = exp ( i π b 2 τ + 2 π i b z + b τ z ) f ( z ) . {\displaystyle (T_{b}f)(z)=\exp(i\pi b^{2}\tau +2\pi ibz)f(z+b\tau )=\exp(i\pi b^{2}\tau +2\pi ibz+b\tau \partial _{z})f(z).}

It can be seen that each operator generates a one-parameter subgroup:

S a 1 ( S a 2 f ) = ( S a 1 S a 2 ) f = S a 1 + a 2 f {\displaystyle S_{a_{1}}\left(S_{a_{2}}f\right)=\left(S_{a_{1}}\circ S_{a_{2}}\right)f=S_{a_{1}+a_{2}}f}

and

T b 1 ( T b 2 f ) = ( T b 1 T b 2 ) f = T b 1 + b 2 f . {\displaystyle T_{b_{1}}\left(T_{b_{2}}f\right)=\left(T_{b_{1}}\circ T_{b_{2}}\right)f=T_{b_{1}+b_{2}}f.}

However, S and T do not commute:

S a T b = exp ( 2 π i a b ) T b S a . {\displaystyle S_{a}\circ T_{b}=\exp(2\pi iab)T_{b}\circ S_{a}.}

Thus we see that S and T together with a unitary phase form a nilpotent Lie group, the (continuous real) Heisenberg group, parametrizable as H = U ( 1 ) × R × R {\displaystyle H=U(1)\times \mathbb {R} \times \mathbb {R} } where U(1) is the unitary group.

A general group element U τ ( λ , a , b ) H {\displaystyle U_{\tau }(\lambda ,a,b)\in H} then acts on a holomorphic function f(z) as

U τ ( λ , a , b ) f ( z ) = λ ( S a T b f ) ( z ) = λ exp ( i π b 2 τ + 2 π i b z ) f ( z + a + b τ ) {\displaystyle U_{\tau }(\lambda ,a,b)f(z)=\lambda (S_{a}\circ T_{b}f)(z)=\lambda \exp(i\pi b^{2}\tau +2\pi ibz)f(z+a+b\tau )}

where λ U ( 1 ) . {\displaystyle \lambda \in U(1).} U ( 1 ) = Z ( H ) {\displaystyle U(1)=Z(H)} is the center of H, the commutator subgroup [ H , H ] {\displaystyle [H,H]} . The parameter τ {\displaystyle \tau } on U τ ( λ , a , b ) {\displaystyle U_{\tau }(\lambda ,a,b)} serves only to remind that every different value of τ {\displaystyle \tau } gives rise to a different representation of the action of the group.

Hilbert space

The action of the group elements U τ ( λ , a , b ) {\displaystyle U_{\tau }(\lambda ,a,b)} is unitary and irreducible on a certain Hilbert space of functions. For a fixed value of τ, define a norm on entire functions of the complex plane as

f τ 2 = C exp ( π y 2 τ ) | f ( x + i y ) | 2   d x   d y . {\displaystyle \Vert f\Vert _{\tau }^{2}=\int _{\mathbb {C} }\exp \left({\frac {-\pi y^{2}}{\Im \tau }}\right)|f(x+iy)|^{2}\ dx\ dy.}

Here, τ {\displaystyle \Im \tau } is the imaginary part of τ {\displaystyle \tau } and the domain of integration is the entire complex plane.


Mumford sets the norm as C exp ( 2 π y 2 τ ) | f ( x + i y ) | 2   d x   d y {\displaystyle \int _{\mathbb {C} }\exp \left({\frac {-2\pi y^{2}}{\Im \tau }}\right)|f(x+iy)|^{2}\ dx\ dy} , but in this way T b {\displaystyle T_{b}} is not unitary.

Let H τ {\displaystyle {\mathcal {H}}_{\tau }} be the set of entire functions f with finite norm. The subscript τ {\displaystyle \tau } is used only to indicate that the space depends on the choice of parameter τ {\displaystyle \tau } . This H τ {\displaystyle {\mathcal {H}}_{\tau }} forms a Hilbert space. The action of U τ ( λ , a , b ) {\displaystyle U_{\tau }(\lambda ,a,b)} given above is unitary on H τ {\displaystyle {\mathcal {H}}_{\tau }} , that is, U τ ( λ , a , b ) {\displaystyle U_{\tau }(\lambda ,a,b)} preserves the norm on this space. Finally, the action of U τ ( λ , a , b ) {\displaystyle U_{\tau }(\lambda ,a,b)} on H τ {\displaystyle {\mathcal {H}}_{\tau }} is irreducible.

This norm is closely related to that used to define Segal–Bargmann space[citation needed].

Isomorphism

The above theta representation of the Heisenberg group is isomorphic to the canonical Weyl representation of the Heisenberg group. In particular, this implies that H τ {\displaystyle {\mathcal {H}}_{\tau }} and L 2 ( R ) {\displaystyle L^{2}(\mathbb {R} )} are isomorphic as H-modules. Let

M ( a , b , c ) = [ 1 a c 0 1 b 0 0 1 ] {\displaystyle M(a,b,c)={\begin{bmatrix}1&a&c\\0&1&b\\0&0&1\end{bmatrix}}}

stand for a general group element of H 3 ( R ) . {\displaystyle H_{3}(\mathbb {R} ).} In the canonical Weyl representation, for every real number h, there is a representation ρ h {\displaystyle \rho _{h}} acting on L 2 ( R ) {\displaystyle L^{2}(\mathbb {R} )} as

ρ h ( M ( a , b , c ) ) ψ ( x ) = exp ( i b x + i h c ) ψ ( x + h a ) {\displaystyle \rho _{h}(M(a,b,c))\psi (x)=\exp(ibx+ihc)\psi (x+ha)}

for x R {\displaystyle x\in \mathbb {R} } and ψ L 2 ( R ) . {\displaystyle \psi \in L^{2}(\mathbb {R} ).}

Here, h is Planck's constant. Each such representation is unitarily inequivalent. The corresponding theta representation is:

M ( a , 0 , 0 ) S a h {\displaystyle M(a,0,0)\to S_{ah}}
M ( 0 , b , 0 ) T b / 2 π {\displaystyle M(0,b,0)\to T_{b/2\pi }}
M ( 0 , 0 , c ) e i h c {\displaystyle M(0,0,c)\to e^{ihc}}

Discrete subgroup

Define the subgroup Γ τ H τ {\displaystyle \Gamma _{\tau }\subset H_{\tau }} as

Γ τ = { U τ ( 1 , a , b ) H τ : a , b Z } . {\displaystyle \Gamma _{\tau }=\{U_{\tau }(1,a,b)\in H_{\tau }:a,b\in \mathbb {Z} \}.}

The Jacobi theta function is defined as

ϑ ( z ; τ ) = n = exp ( π i n 2 τ + 2 π i n z ) . {\displaystyle \vartheta (z;\tau )=\sum _{n=-\infty }^{\infty }\exp(\pi in^{2}\tau +2\pi inz).}

It is an entire function of z that is invariant under Γ τ . {\displaystyle \Gamma _{\tau }.} This follows from the properties of the theta function:

ϑ ( z + 1 ; τ ) = ϑ ( z ; τ ) {\displaystyle \vartheta (z+1;\tau )=\vartheta (z;\tau )}

and

ϑ ( z + a + b τ ; τ ) = exp ( π i b 2 τ 2 π i b z ) ϑ ( z ; τ ) {\displaystyle \vartheta (z+a+b\tau ;\tau )=\exp(-\pi ib^{2}\tau -2\pi ibz)\vartheta (z;\tau )}

when a and b are integers. It can be shown that the Jacobi theta is the unique such function.

See also

References

  • David Mumford, Tata Lectures on Theta I (1983), Birkhäuser, Boston ISBN 3-7643-3109-7