Weil–Brezin Map

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In mathematics, the Weil–Brezin map, named after André Weil[1] and Jonathan Brezin,[2] is a unitary transformation that maps a Schwartz function on the real line to a smooth function on the Heisenberg manifold. The Weil–Brezin map gives a geometric interpretation of the Fourier transform, the Plancherel theorem and the Poisson summation formula.[3][4][5] The image of Gaussian functions under the Weil–Brezin map are nil-theta functions, which are related to theta functions. The Weil–Brezin map is sometimes referred to as the Zak transform,[6] which is widely applied in the field of physics and signal processing; however, the Weil–Brezin Map is defined via Heisenberg group geometrically, whereas there is no direct geometric or group theoretic interpretation from the Zak transform.

Heisenberg manifold

The (continuous) Heisenberg group N is the 3-dimensional Lie group that can be represented by triples of real numbers with multiplication rule

x,y,ta,b,c=x+a,y+b,t+c+xb.

The discrete Heisenberg group Γ is the discrete subgroup of N whose elements are represented by the triples of integers. Considering Γ acts on N on the left, the quotient manifold ΓN is called the Heisenberg manifold. The Heisenberg group acts on the Heisenberg manifold on the right. The Haar measure μ=dxdydt on the Heisenberg group induces a right-translation-invariant measure on the Heisenberg manifold. The space of complex-valued square-integrable functions on the Heisenberg manifold has a right-translation-invariant orthogonal decomposition:

L2(ΓN)=nHn

where

Hn={fL2(ΓN)f(Γx,y,t+s)=exp(2πins)f(Γx,y,t)}.

Definition

The Weil–Brezin map W:L2()H1 is the unitary transformation given by

W(ψ)(Γx,y,t)=lψ(x+l)e2πilye2πit

for every Schwartz function ψ, where convergence is pointwise.

The inverse of the Weil–Brezin map W1:H1L2() is given by

(W1f)(x)=01f(Γx,y,0)dy

for every smooth function f on the Heisenberg manifold that is in H1.

Fundamental unitary representation of the Heisenberg group

For each real number λ0, the fundamental unitary representation Uλ of the Heisenberg group is an irreducible unitary representation of N on L2() defined by

(Uλ(a,b,c)ψ)(x)=e2πiλ(c+bx)ψ(x+a).

By Stone–von Neumann theorem, this is the unique irreducible representation up to unitary equivalence satisfying the canonical commutation relation

Uλ(a,0,0)Uλ(0,b,0)=e2πiλabUλ(0,b,0)Uλ(a,0,0).

The fundamental representation U=U1 of N on L2() and the right translation R of N on H1L2(ΓN) are intertwined by the Weil–Brezin map

WU(a,b,c)=R(a,b,c)W.

In other words, the fundamental representation U on L2() is unitarily equivalent to the right translation R on H1 through the Weil-Brezin map.

Relation to Fourier transform

Let J:NN be the automorphism on the Heisenberg group given by

J(x,y,t)=y,x,txy.

It naturally induces a unitary operator J*:H1H1, then the Fourier transform

=W1J*W

as a unitary operator on L2().

Plancherel theorem

The norm-preserving property of W and J*, which is easily seen, yields the norm-preserving property of the Fourier transform, which is referred to as the Plancherel theorem.

Poisson summation formula

For any Schwartz function ψ,

lψ(l)=W(ψ)(Γ0,0,0))=(J*W(ψ))(Γ0,0,0))=W(ψ^)(Γ0,0,0))=lψ^(l).

This is just the Poisson summation formula.

Relation to the finite Fourier transform

For each n0, the subspace HnL2(ΓN) can further be decomposed into right-translation-invariant orthogonal subspaces

Hn=m=0|n|1Hn,m

where

Hn,m={fHnf(Γx,y+1n,t)=e2πim/nf(Γx,y,t)}.

The left translation L(0,1/n,0) is well-defined on Hn, and Hn,0,...,Hn,|n|1 are its eigenspaces.

The left translation L(m/n,0,0) is well-defined on Hn, and the map

L(m/n,0,0):Hn,0Hn,m

is a unitary transformation.

For each n0, and m=0,...,|n|1, define the map Wn,m:L2()Hn,m by

Wn,m(ψ)(Γx,y,t)=lψ(x+l+mn)e2πi(nl+m)ye2πint

for every Schwartz function ψ, where convergence is pointwise.

Wn,m=L(m/n,0,0)Wn,0.

The inverse map Wn,m1:Hn,mL2() is given by

(Wn,m1f)(x)=01e2πimyf(Γxmn,y,0)dy

for every smooth function f on the Heisenberg manifold that is in Hn,m.

Similarly, the fundamental unitary representation Un of the Heisenberg group is unitarily equivalent to the right translation on Hn,m through Wn,m:

Wn,mUn(a,b,c)=R(a,b,c)Wn,m.

For any m,m,

(Wn,m1J*Wn,mψ)(x)=e2πimm/nψ^(nx).

For each n>0, let ϕn(x)=(2n)1/4eπnx2. Consider the finite dimensional subspace Kn of Hn generated by {𝒆n,0,...,𝒆n,n1} where

𝒆n,m=Wn,m(ϕn)Hn,m.

Then the left translations L(1/n,0,0) and L(0,1/n,0) act on Kn and give rise to the irreducible representation of the finite Heisenberg group. The map J* acts on Kn and gives rise to the finite Fourier transform

J*𝒆n,m=1nme2πimm/n𝒆n,m.

Nil-theta functions

Nil-theta functions are functions on the Heisenberg manifold that are analogous to the theta functions on the complex plane. The image of Gaussian functions under the Weil–Brezin Map are nil-theta functions. There is a model[7] of the finite Fourier transform defined with nil-theta functions, and the nice property of the model is that the finite Fourier transform is compatible with the algebra structure of the space of nil-theta functions.

Definition of nil-theta functions

Let 𝔫 be the complexified Lie algebra of the Heisenberg group N. A basis of 𝔫 is given by the left-invariant vector fields X,Y,T on N:

X(x,y,t)=x,
Y(x,y,t)=y+xt,
T(x,y,t)=t.

These vector fields are well-defined on the Heisenberg manifold ΓN.

Introduce the notation Vi=XiY. For each n>0, the vector field Vi on the Heisenberg manifold can be thought of as a differential operator on C(ΓN)Hn,m with the kernel generated by 𝒆n,m.

We call

ker(Vi:C(ΓN)HnHn)={Kn,n>0,n=0

the space of nil-theta functions of degree n.

Algebra structure of nil-theta functions

The nil-theta functions with pointwise multiplication on ΓN form a graded algebra n0Kn (here K0=).

Auslander and Tolimieri showed that this graded algebra is isomorphic to

[x1,x22,x33]/(x36+x14x22+x26),

and that the finite Fourier transform (see the preceding section #Relation to the finite Fourier transform) is an automorphism of the graded algebra.

Relation to Jacobi theta functions

Let ϑ(z;τ)=l=exp(πil2τ+2πilz) be the Jacobi theta function. Then

ϑ(n(x+iy);ni)=(2n)1/4eπny2𝒆n,0(Γy,x,0).

Higher order theta functions with characteristics

An entire function f on is called a theta function of order n, period τ (Im(τ)>0) and characteristic [ba] if it satisfies the following equations:

  1. f(z+1)=exp(πia)f(z),
  2. f(z+τ)=exp(πib)exp(πin(2z+τ))f(z).

The space of theta functions of order n, period τ and characteristic [ba] is denoted by Θn[ba](τ,A).

dimΘn[ba](τ,A)=n.

A basis of Θn[00](i,A) is

θn,m(z)=lexp[πn(l+mn)2+2πi(ln+m)z)].

These higher order theta functions are related to the nil-theta functions by

θn,m(x+iy)=(2n)1/4eπny2𝒆n,m(Γy,x,0).

See also

References

Template:Reflist

  1. Weil, André. "Sur certains groupes d'opérateurs unitaires." Acta mathematica 111.1 (1964): 143-211.
  2. Brezin, Jonathan. "Harmonic analysis on nilmanifolds." Transactions of the American Mathematical Society 150.2 (1970): 611-618.
  3. Auslander, Louis, and Richard Tolimieri. Abelian harmonic analysis, theta functions and function algebras on a nilmanifold. Springer, 1975.
  4. Auslander, Louis. "Lecture notes on nil-theta functions." Conference Board of the Mathematical Sciences, 1977.
  5. Zhang, D. "Integer Linear Canonical Transforms, Their Discretization, and Poisson Summation Formulae"
  6. Template:Cite web
  7. Auslander, L., and R. Tolimieri. "Algebraic structures for⨁Σ _ {𝑛≥ 1} 𝐿2 (𝑍/𝑛) compatible with the finite Fourier transform." Transactions of the American Mathematical Society 244 (1978): 263-272.