The one-dimensional periodic Schrödinger equation

Jordan Bell
April 23, 2016

1 Translations and convolution

For y∈ℝ, let

τy⁢f⁢(x)=f⁢(x-y).

To say that f:ℝ→ℂ is uniformly continuous means that ∥τh⁢f-f∥b→0 as h→0, where

∥g∥b=supx∈ℝ⁡|g⁢(x)|.

Let 1≤p<∞ and let ℒ⁢(Lp⁢(ℝ)) be the Banach algebra of bounded linear operators Lp⁢(ℝ)→Lp⁢(ℝ), with the strong operator topology: a net Ti converges to T in the strong operator topology if and only if for each f∈Lp⁢(ℝ), ∥Ti⁢f-T⁢f∥Lp→0.

Lemma 1.

y↦τy is continuous R→L⁢(Lp⁢(R)), using the strong operator topology.

Proof.

For y∈ℝ and f∈Lp⁢(ℝ), ∥τy+h⁢f-τy⁢f∥Lp=∥τh⁢f-f∥Lp. Take ϵ>0 and let ϕ∈Cc⁢(ℝ) with ∥f-ϕ∥Lp<∞. Say supp⁢ϕ⊂[a,b]. Let K=[a-1,b+1]. For |h|≤1, if x∉K then x-h,x∉supp⁢ϕ, and hence

∥τh⁢ϕ-ϕ∥Lpp =∫ℝ|ϕ⁢(x-h)-ϕ⁢(x)|p⁢𝑑x
=∫K|ϕ⁢(x-h)-ϕ⁢(x)|p⁢𝑑x
≤(b-a+2)⁢∥τh⁢ϕ-ϕ∥bp
=(b-a+2)⁢∥τϕ-τy⁢ϕ∥bp.

Because ϕ∈Cc⁢(ℝ), ϕ is uniformly continuous on ℝ, whence ∥τh⁢ϕ-ϕ∥Lp→0 as h→0, say ∥τh⁢ϕ-ϕ∥Lp<ϵ for |h|≤hϵ. Hence

∥τy+h⁢f-τy⁢f∥Lp =∥τh⁢f-f∥Lp
≤∥τh⁢f-τh⁢ϕ∥Lp+∥τh⁢ϕ-ϕ∥Lp+∥ϕ-f∥Lp
=2⁢∥f-ϕ∥Lp+∥τh-ϕ∥Lp
<3⁢ϵ.

∎

Define A:ℝ×ℝ→ℝ by

A⁢(x1,x2)=x1+x2.

If μ1,μ2 are finite Borel measures on ℝ, let μ1⊗μ2 be the product measure on ℝ2, and let

μ1*μ2=A*⁢(μ1⊗μ2)

be the pushforward of μ1⊗μ2 by A, called the convolution of μ1 and μ2. If f:ℝ→[0,∞] is measurable then applying the change of variables formula and then Tonelli’s theorem we obtain

∫f⁢d⁢(μ1*μ2) =∫f∘A⁢d⁢(μ1⊗μ2)
=∫(∫f∘A⁢(x1,x2)⁢𝑑μ1⁢(x1))⁢𝑑μ2⁢(x2)
=∫(∫f⁢(x1+x2)⁢𝑑μ1⁢(x1))⁢𝑑μ2⁢(x2).

If B is a Borel set in ℝ then applying the above with f=1B,

(μ1*μ2)⁢(B) =∫1B⁢d⁢(μ1*μ2)
=∫(∫1B⁢(x1+x2)⁢𝑑μ1⁢(x1))⁢𝑑μ2⁢(x2)
=∫μ1⁢(B-x2)⁢𝑑μ2⁢(x2).

2 Periodic functions

Let 𝕋=ℝ/ℤ, and let 𝒮⁢(𝕋) be the collection of C∞ functions ϕ:ℝ→ℂ satisfying ϕ⁢(x+1)=ϕ⁢(x) for all x∈𝕋. For ϕ,ψ∈𝒮⁢(𝕋), for n≥1 let

dn⁢(ϕ,ψ)=supx∈[0,1]⁡|ϕ(n)⁢(x)-ψ(n)⁢(x)|

and

d⁢(ϕ,ψ)=∑n=0∞2-n⁢dn⁢(ϕ,ψ)1+dn⁢(ϕ,ψ).

With this metric, 𝒮⁢(𝕋) is a Fréchet space.

For n∈ℤ, define

en⁢(x)=e2⁢π⁢i⁢n⁢x,x∈ℝ.

For f∈L1⁢(𝕋), define f^:ℤ→ℂ, for n∈ℤ, by

ϕ^⁢(n)=∫01ϕ⁢(x)⁢e-n⁢(x)⁢𝑑x=∫01ϕ⁢(x)⁢e-2⁢π⁢i⁢n⁢x⁢𝑑x.

Denote by 𝒮′⁢(𝕋) the dual space of 𝒮⁢(𝕋), the collection of continuous linear maps 𝒮⁢(𝕋)→ℂ. For L∈𝒮′⁢(𝕋), define L^:ℤ→ℂ by

L^⁢(n)=L⁢e-n.

For x∈ℝ, define δx:𝒮⁢(𝕋)→ℂ by

δx⁢ϕ=ϕ⁢(x).

δx belongs to 𝒮′⁢(𝕋), and

δ^x⁢(n)=δx⁢e-n=e-n⁢(x)=e-2⁢π⁢i⁢n⁢x.

For f∈L1⁢(𝕋), define Lf∈𝒮′⁢(𝕋) by

Lf⁢ϕ=∫01f⁢(x)⁢ϕ⁢(x)⁢𝑑x,ϕ∈𝒮⁢(𝕋).

For n∈ℤ,

Lf^⁢(n)=Lf⁢e-n=∫01f⁢(x)⁢e-n⁢(x)⁢𝑑x=f^⁢(n).

3 The Poisson summation formula

If f∈ℒ1⁢(ℝ),

∫01∑n∈ℤ|f⁢(x+n)|⁢d⁢x =∑n∈ℤ∫01|f⁢(x+n)|⁢𝑑x
=∑n∈ℤ∫nn+1|f⁢(x)|⁢𝑑x
=∫ℝ|f⁢(x)|⁢𝑑x.

This implies that there is a Borel set Nf in ℝ with λ⁢(Nf)=0 such that for x∈Nfc,

∑n∈ℤ|f⁢(x+n)|<∞.

We define P⁢f⁢(x)=∑n∈ℤf⁢(x+n) for x∈Nfc and P⁢f⁢(x)=0 for x∈Nf. Thus it makes sense to define P:L1⁢(ℝ)→L1⁢(ℝ) by

P⁢f⁢(x)=∑n∈ℤf⁢(x+n),

in other words,

P⁢f=∑n∈ℤτ-n⁢f.

Then

∫01P⁢f⁢(x)⁢e-2⁢π⁢i⁢m⁢x⁢𝑑x =∫01(∑n∈ℤf⁢(x+n))⁢e-2⁢π⁢i⁢m⁢x⁢𝑑x
=∑n∈ℤ∫01f⁢(x+n)⁢e-2⁢π⁢i⁢m⁢x⁢𝑑x
=∑n∈ℤ∫nn+1f⁢(x)⁢e-2⁢π⁢i⁢m⁢x⁢𝑑x
=∫ℝf⁢(x)⁢e-2⁢π⁢i⁢m⁢x⁢𝑑x
=f^⁢(m).

That is,

P⁢f^⁢(m)=f^⁢(m).

Supposing that P⁢f⁢(x)=∑n∈ℤP⁢f^⁢(n)⁢e2⁢π⁢i⁢n⁢x,

P⁢f⁢(x)=∑n∈ℤf^⁢(n)⁢e2⁢π⁢i⁢n⁢x

and supposing P⁢f⁢(x)=∑n∈ℤf⁢(x+n),

∑n∈ℤf⁢(x+n)=∑n∈ℤf^⁢(n)⁢e2⁢π⁢i⁢n⁢x,

the Poisson summation formula.

For N≥1, let

LN=1N⁢∑j=0N-1δj/N.

For n∈ℤ,

L^N⁢(n)=1N⁢∑j=0N-1δj/N⁢e-n=1N⁢∑j=0N-1e-n⁢(j/N)=1N⁢∑j=0N-1e-2⁢π⁢i⁢n⁢j/N.

If n∈N⁢ℤ then L^N⁢(n)=1 and otherwise L^N⁢(n)=0. That is,

LN=1N⁢∑j=0N-1δj/N∼∑k∈ℤL^N⁢(k)⁢ek=∑k∈ℤeN⁢k.

4 The heat kernel

For x∈ℝ and t>0 define

Ht⁢(x)=∫ℝe-4⁢π2⁢t⁢ξ2⁢e2⁢π⁢i⁢ξ⁢x⁢𝑑ξ.

Using

∫ℝexp⁡(12⁢i⁢a⁢w2+i⁢J⁢w)⁢𝑑w=2⁢π⁢ia⁢exp⁡(-i⁢J22⁢a),

for 12⁢i⁢a=-4⁢π2⁢t we get a=8⁢i⁢π2⁢t and J=2⁢π⁢x, and we calculate

Ht⁢(x) =2⁢π⁢i8⁢π2⁢i⁢t⁢exp⁡(-i16⁢π2⁢i⁢t⋅4⁢π2⁢x2)
=14⁢π⁢t⁢exp⁡(-x24⁢t).

By the Fourier inversion theorem,

Ht^⁢(ξ)=e-4⁢π2⁢t⁢ξ2.

For f∈L1⁢(ℝ),

τy⁢f^⁢(ξ)=∫ℝf⁢(x-y)⁢e-2⁢π⁢i⁢ξ⁢x⁢𝑑x=e-2⁢π⁢i⁢ξ⁢y⁢f^⁢(ξ)=e-n⁢(y)⁢f^⁢(ξ).

5 The Schrödinger equation on ℝ

Let

Γ⁢(t,x)=it⁢e-π⁢i⁢x2/t,

which satisfies

∂x⁡Γ⁢(t,x)=-2⁢π⁢i⁢xt⁢Γ⁢(t,x),∂x2⁡Γ⁢(t,x)=-4⁢π2⁢x2t2⁢Γ⁢(t,x)-2⁢π⁢it⁢Γ⁢(t,x)

and

∂t⁡Γ⁢(t,x)=-12⁢t-1⁢Γ⁢(t,x)+π⁢i⁢x2⁢t-2⁢Γ⁢(t,x).

This satisfies

∂t⁡Γ⁢(t,x) =12⁢(-1t+2⁢π⁢i⁢x2t2)⁢Γ⁢(t,x)
=14⁢π⁢i⁢(-2⁢π⁢it-4⁢π2⁢x2t2)⁢Γ⁢(t,x)
=14⁢π⁢i⁢∂x2⁡Γ⁢(t,x).

For f:ℝ→ℂ, let

ψ⁢(f)⁢(t,x)=f*Γ⁢(t,⋅)⁢(x)=∫ℝf⁢(y)⁢Γ⁢(t,x-y)⁢𝑑y.

This satisfies

∂t⁡ψ⁢(f)⁢(t,x) =∫ℝf⁢(y)⋅∂t⁡Γ⁢(t,x-y)⁢𝑑y
=∫ℝf⁢(y)⋅14⁢π⁢i⁢∂x2⁡Γ⁢(t,x-y)⁢𝑑y
=14⁢π⁢i⁢∂x2⁡ψ⁢(f)⁢(t,x).

We also calculate

ψ⁢(f)⁢(t,x) =∫ℝf⁢(y)⋅Γ⁢(t,x-y)⁢𝑑y
=∫ℝf⁢(y)⋅it⁢e-π⁢i⁢(x-y)2/t⁢𝑑y
=∫ℝf⁢(y)⋅it⁢exp⁡(-π⁢i⁢x2t+2⁢π⁢i⁢x⁢yt-π⁢i⁢y2t)⁢𝑑y
=Γ⁢(t,x)⋅∫ℝf⁢(y)⁢exp⁡(-π⁢it⁢(y2-2⁢x⁢y))⁢𝑑y.

Let

f^⁢(y)=∫ℝf⁢(x)⁢e-2⁢π⁢i⁢x⁢y⁢𝑑x.

Using

∫ℝexp⁡(12⁢i⁢a⁢w2+i⁢J⁢w)⁢𝑑w=2⁢π⁢ia⁢exp⁡(-i⁢J22⁢a),

we get, with a=2⁢π⁢t and J=2⁢π⁢u,

Γ⁢(t,x)⋅ψ⁢(f^)⁢(-1/t,-x/t)=Γ⁢(t,x)⋅∫ℝf^⁢(y)⁢Γ⁢(-1t,-xt-y)⁢𝑑y=Γ⁢(t,x)⋅∫ℝf^⁢(-xt-y)⁢Γ⁢(-1t,y)⁢𝑑y=it⁢e-π⁢i⁢x2/t⋅∫ℝ(∫ℝf⁢(u)⁢e-2⁢π⁢i⁢u⁢(-xt-y)⁢𝑑u)⋅-i⁢t⁢eπ⁢i⁢t⁢y2⁢𝑑y=e-π⁢i⁢x2/t⁢∫ℝf⁢(u)⁢e2⁢π⁢i⁢u⁢x/t⁢(∫ℝe2⁢π⁢i⁢u⁢y+π⁢i⁢t⁢y2⁢𝑑y)⁢𝑑u=e-π⁢i⁢x2/t⁢∫ℝf⁢(u)⁢e2⁢π⁢i⁢u⁢x/t⋅2⁢π⁢i2⁢π⁢t⁢exp⁡(-i4⁢π⁢t⁢(2⁢π⁢u)2)⁢𝑑u=e-π⁢i⁢x2/t⁢it⁢∫ℝf⁢(u)⁢e2⁢π⁢i⁢u⁢x/t⁢exp⁡(-π⁢i⁢u2t)⁢𝑑u=it⁢∫ℝf⁢(u)⁢exp⁡(-π⁢i⁢x2t+2⁢π⁢i⁢u⁢xt-π⁢i⁢u2t)⁢𝑑u=it⁢∫ℝf⁢(u)⁢e-π⁢i⁢(x-u)2t⁢𝑑u=∫ℝf⁢(u)⁢Γ⁢(t,x-u)⁢𝑑u=ψ⁢(f)⁢(t,x).

In other words,

ψ⁢(f)⁢(t,x) =Γ⁢(t,x)⋅ψ⁢(f^)⁢(-1/t,-x/t)
=it⁢e-π⁢i⁢x2/t⋅∫ℝf^⁢(ξ)⋅-i⁢t⁢exp⁡(π⁢i⁢t⁢(-xt-ξ)2)⁢𝑑ξ
=∫ℝf^⁢(ξ)⁢exp⁡(-π⁢i⁢x2t+π⁢i⁢x2t+2⁢π⁢i⁢x⁢ξ+π⁢i⁢t⁢ξ2)⁢𝑑ξ
=∫ℝf^⁢(ξ)⁢e2⁢π⁢i⁢x⁢ξ+π⁢i⁢t⁢ξ2⁢𝑑ξ.

6 The Schrödinger equation on 𝕋

Given t and x, let γ⁢(y)=Γ⁢(t,x-y). We calculate

γ^⁢(ξ) =∫ℝγ⁢(y)⁢e-2⁢π⁢i⁢ξ⁢y⁢𝑑y
=∫ℝit⁢e-π⁢i⁢(x-y)2/t⁢e-2⁢π⁢i⁢ξ⁢y⁢𝑑y
=∫ℝit⁢exp⁡(-π⁢i⁢x2t+2⁢π⁢i⁢x⁢yt-π⁢i⁢y2t-2⁢π⁢i⁢ξ⁢y)⁢𝑑y.

Using

∫ℝexp⁡(12⁢i⁢a⁢w2+i⁢J⁢w)⁢𝑑w=2⁢π⁢ia⁢exp⁡(-i⁢J22⁢a)

with a=-2⁢πt and J=2⁢π⁢xt-2⁢π⁢ξ, for which J2=4⁢π2⁢x2t2-8⁢π2⁢x⁢ξt+4⁢π2⁢ξ2,

γ^⁢(ξ) =it⁢exp⁡(-π⁢i⁢x2t)⋅-i⁢t⁢exp⁡(i⁢t4⁢π⁢J2)
=exp⁡(-π⁢i⁢x2t)⁢exp⁡(i⁢π⁢x2t-2⁢π⁢i⁢x⁢ξ+π⁢i⁢ξ2⁢t)
=exp⁡(-2⁢π⁢i⁢x⁢ξ+π⁢i⁢ξ2⁢t).

The Poisson summation formula tells us

∑n∈ℤγ⁢(n)=∑n∈ℤγ^⁢(n),

i.e.

∑n∈ℤΓ⁢(t,x-n)=∑n∈ℤe-2⁢π⁢i⁢n⁢x+π⁢i⁢t⁢n2=∑n∈ℤe2⁢π⁢i⁢n⁢x+π⁢i⁢t⁢n2.

Define

Θ⁢(t,x)=∑n∈ℤeπ⁢i⁢(t⁢n2+2⁢x⁢n)=∑n∈ℤeπ⁢i⁢t⁢n2⁢e2⁢π⁢i⁢x⁢n=∑n∈ℤΓ⁢(t,x-n).

For ϕ∈𝒮, namely a Schwartz function, define

Θt⁢ϕ⁢(x)=∑n∈ℤ∫ℝϕ⁢(x)⁢eπ⁢i⁢t⁢n2⁢e2⁢π⁢i⁢x⁢n⁢𝑑x,

which satisfies

Θt⁢ϕ⁢(x)=∑n∈ℤϕ^⁢(-n)⁢eπ⁢i⁢t⁢n2=∑n∈ℤϕ^⁢(n)⁢eπ⁢i⁢t⁢n2.

If f is 1-periodic, for n∈ℤ let

f^⁢(n)=∫01f⁢(y)⁢e-2⁢π⁢i⁢n⁢y⁢𝑑y.

Define

ψ⁢(f)⁢(t,x)=Θt*f⁢(x)=∫01Θ⁢(t,x-y)⁢f⁢(y)⁢𝑑y,

which satisfies

ψ⁢(f)⁢(t,x) =∫01∑n∈ℤeπ⁢i⁢t⁢n2⁢e2⁢π⁢i⁢(x-y)⁢n⁢f⁢(y)⁢d⁢y
=∑n∈ℤeπ⁢i⁢t⁢n2⁢e2⁢π⁢i⁢x⁢n⁢∫01f⁢(y)⁢e-2⁢π⁢i⁢n⁢y⁢𝑑y
=∑n∈ℤeπ⁢i⁢t⁢n2⁢e2⁢π⁢i⁢x⁢n⁢f^⁢(n).

We remind ourselves

Θ⁢(t,x)=Θt⁢(x)=∑n∈ℤeπ⁢i⁢t⁢n2⁢e2⁢π⁢i⁢x⁢n

and

Θ^t⁢(n)=eπ⁢i⁢t⁢n2.

Say t=2⁢MN. Then for k∈ℤ,

Θ^t⁢(k+N) =exp⁡(π⁢i⋅2⁢MN⋅(k+N)2)
=exp⁡(π⁢i⋅2⁢MN⋅k2).