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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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References

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  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. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  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.