Gaussian integrals

Jordan Bell
August 29, 2015

1 One dimensional Gaussian integrals

For p∈ℂ, let11 1 Eberhard Zeidler, Quantum Field Theory I: Basics in Mathematics and Physics, p. 493, Problem 7.1.

h⁢(p)=∫ℝe-x2/2⁢e-i⁢p⁢x⁢𝑑x.

Then we check that

h′⁢(p)=-i⁢∫ℝx⁢e-x2/2⁢e-i⁢p⁢x⁢𝑑x=i⁢∫ℝdd⁢x⁢(e-x2/2)⁢e-i⁢p⁢x⁢𝑑x.

Integrating by parts yields

h′⁢(p)=-p⁢∫ℝe-x2/2⁢e-i⁢p⁢x⁢𝑑x=-p⁢h⁢(p).

Since h′⁢(p)=-p⁢h⁢(p),22 2 cf. Einar Hille, Ordinary Differential Equations in the Complex Domain.

h⁢(p)=h⁢(0)⁢e-p2/2.

Now, using Fubini’s theorem and then polar coordinates,

h⁢(0)2 =∫ℝ(∫ℝe-x2/2⁢𝑑x)⁢e-y2/2⁢𝑑y
=∫ℝ2e-(x2+y2)/2⁢𝑑x⁢𝑑y
=∫0∞(∫S1e-r2/2⁢e-r2/2⁢𝑑σ⁢(θ))⁢r⁢𝑑r
=2⁢π⁢∫0∞r⁢e-r2/2⁢𝑑r
=2⁢π,

so

h⁢(p)=(2⁢π)1/2⁢e-p2/2.

For a>0 and p∈ℂ, doing the change of variable y=a1/2⁢x,

(2⁢π)-1/2⁢∫ℝe-a⁢x2/2⁢e-i⁢p⁢x⁢𝑑x =(2⁢π)-1/2⁢a-1/2⁢∫ℝe-y2/2⁢e-i⁢p⁢a-1/2⁢y⁢𝑑y
=(2⁢π)-1/2⁢a-1/2⁢h⁢(p⁢a-1/2)
=a-1/2⁢e-a-1⁢p2/2.

For t>0 and m∈ℝ, doing the change of variable y=x-m, and using the above with a=t-2 and p=0,

(2⁢π⁢t2)-1/2⁢∫ℝexp⁡(-(x-m)22⁢t2)⁢𝑑x =(2⁢π)-1/2⁢t-1⁢∫ℝe-a⁢y2/2⁢𝑑x
=t-1⋅a-1/2
=1.
Theorem 1.

For a>0 and p∈ℂ,

(2⁢π)-1/2⁢∫ℝe-a⁢x2/2⁢e-i⁢p⁢x⁢𝑑x=a-1/2⁢e-a-1⁢p2/2.

For t>0 and m∈ℝ,

(2⁢π⁢t2)-1/2⁢∫ℝexp⁡(-(x-m)22⁢t2)⁢𝑑x=1.

For t>0 and x∈ℝ, let

pt⁢(x)=(2⁢π⁢t2)-1/2⁢exp⁡(-x22⁢t2).

For ϕ∈𝒮⁢(ℝ), doing the change of variable x=t⁢y,

∫ℝϕ⁢(x)⁢pt⁢(x)⁢𝑑x=(2⁢π)-1/2⁢∫ℝϕ⁢(t⁢y)⁢e-y2/2⁢𝑑y=∫ℝϕ⁢(t⁢x)⁢p1⁢(x)⁢𝑑x.

Then as t↓0, using the dominated convergence theorem,

∫ℝϕ⁢(x)⁢pt⁢(x)⁢𝑑x→∫ℝϕ⁢(0)⁢p1⁢(x)⁢𝑑x=ϕ⁢(0).

For ϕ∈L1⁢(ℝN), let

ϕ^⁢(ξ)=(2⁢π)-N/2⁢∫ℝNe-i⁢⟨ξ,x⟩⁢ϕ⁢(x)⁢𝑑x,ξ∈ℝN.

By Theorem 1, with a=t-2,

p^t⁢(ξ) =(2⁢π⁢t2)-1/2⋅(2⁢π)-1/2⁢∫ℝe-a⁢x2/2⁢e-i⁢ξ⁢x⁢𝑑x
=(2⁢π⁢t2)-1/2⁢a-1/2⁢e-a-1⁢ξ2/2
=(2⁢π)-1/2⁢e-t2⁢ξ2/2.

2 Moments

For a>0, define for Z∈ℂ,

Z⁢(J)=a1/2⁢(2⁢π)-1/2⁢∫ℝe-a⁢x2/2⁢ei⁢J⁢x⁢𝑑x.

By Theorem 1,

Z⁢(J)=e-a-1⁢J2/2. (1)

By the dominated convergence theorem,

Z(n)⁢(J)=a1/2⁢(2⁢π)-1/2⁢in⁢∫ℝxn⁢e-a⁢x2/2⁢ei⁢J⁢x⁢𝑑x,

and so

a1/2⁢(2⁢π)-1/2⁢∫ℝxn⁢e-a⁢x2/2⁢𝑑x=i-n⁢d⁢Zd⁢J⁢(0).

From (1) we calculate

Z′⁢(J)=-a-1⁢J⁢Z⁢(J),Z′′⁢(J)=-a-1⁢Z⁢(J)+a-2⁢J2⁢Z⁢(J),

so Z′′⁢(0)=-a-1⁢Z⁢(0)=-a-1, and thus for t>0 and a=t-1,

(2⁢π⁢t)-1/2⁢∫ℝx2⁢e-t-2⁢x2/2⁢𝑑x=t,

i.e.

∫ℝx2⁢pt⁢(x)⁢𝑑x=t.

3 N-dimensional Gaussian integrals

Let S⁢(x)=⟨x,x⟩2 for x∈ℝN. For χ∈𝒟⁢(ℝN) and t>0, Laplace’s method tells us that

∫ℝNe-t⁢S⁢(x)⁢χ⁢(x)⁢𝑑x=(2⁢π⁢t-1)N/2⁢(det⁡Hess⁢S⁢(0))-1/2⁢e-t⁢S⁢(0)⁢χ⁢(0)⁢(1+O⁢(t-1))

as t→∞. Here, Hess⁢S⁢(x)=I for all x and S⁢(0)=0, so

∫ℝNe-t⁢⟨x,x⟩2⁢χ⁢(x)⁢𝑑x=(2⁢π⁢t-1)N/2⁢χ⁢(0)⁢(1+O⁢(t-1))

as t→∞.

For A an N×N matrix, we write A>0 if A is symmetric and has positive eigenvalues. It is proved that

∫ℝNexp⁡(-12⁢⟨A⁢x,x⟩-i⁢⟨ξ,x⟩)⁢𝑑x=(det⁡A)-1/2⁢(2⁢π)N/2⁢exp⁡(-12⁢⟨A-1⁢ξ,ξ⟩)

for all ξ∈ℝN, and

∫ℝNexp⁡(-12⁢⟨A⁢x,x⟩+⟨b,x⟩)⁢𝑑x=(det⁡A)-1/2⁢(2⁢π)N/2⁢exp⁡(12⁢⟨A-1⁢b,b⟩).

for all b∈ℝN. Let

ZA=∫ℝNe-12⁢⟨A⁢x,x⟩⁢𝑑x=(det⁡A)-1/2⁢(2⁢π)N/2.

Let λN be Lebesgue measure on ℝN and let μA be the following Borel probability measure on ℝN:

d⁢μA⁢(x)=1ZA⁢e-12⁢⟨A⁢x,x⟩⁢d⁢λN⁢(x)=(det⁡A)1/2⁢(2⁢π)-N/2⁢e-12⁢⟨A⁢x,x⟩⁢d⁢λN⁢(x).

For ξ∈ℝN,

∫ℝNe-i⁢⟨ξ,x⟩⁢𝑑μA⁢(x) =(det⁡A)1/2⁢(2⁢π)-N/2⁢∫ℝNe-12⁢⟨A⁢x,x⟩⁢e-i⁢⟨ξ,x⟩⁢𝑑λN⁢(x)
=(det⁡A)1/2⁢(2⁢π)-N/2⋅(det⁡A)-1/2⁢(2⁢π)N/2⁢e-12⁢⟨A-1⁢ξ,ξ⟩
=e-12⁢⟨A-1⁢ξ,ξ⟩,

and for b∈ℝN,

∫ℝNe⟨b,x⟩⁢𝑑μA⁢(x) =(det⁡A)1/2⁢(2⁢π)-N/2⁢∫ℝNe⟨b,x⟩⁢e-12⁢⟨A⁢x,x⟩⁢𝑑λN⁢(x)
=(det⁡A)1/2⁢(2⁢π)-N/2⋅(det⁡A)-1/2⁢(2⁢π)N/2⁢e12⁢⟨A-1⁢b,b⟩
=e12⁢⟨A-1⁢b,b⟩.
Theorem 2.

For ξ∈ℝN,

∫ℝNe-i⁢⟨ξ,x⟩⁢𝑑μA⁢(x)=e-12⁢⟨A-1⁢ξ,ξ⟩,

and for b∈ℝN,

∫ℝNe⟨b,x⟩⁢𝑑μA⁢(x)=e12⁢⟨A-1⁢b,b⟩.

Let33 3 See http://www.math.ucsd.edu/~bdriver/247A-Winter2012/

L=LA=∑j,k=1NAj,k-1⁢∂j⁡∂k.

We work out the semigroup whose infinitesimal generator is L/2.

Theorem 3.

For f∈C1⁢(ℝN) that is μA-integrable and for t>0,

(et⁢L/2⁢f)⁢(x)=∫ℝNf⁢(x-t1/2⁢y)⁢𝑑μA⁢(y),x∈ℝN.
Proof.

For ξ∈ℝN define f⁢(x)=e⟨ξ,x⟩=eξ1⁢x1+⋯+ξN⁢xN. On the one hand,

L⁢f=∑j,k=1nAj,k-1⁢ξj⁢ξk⁢f=⟨A-1⁢ξ,ξ⟩⁢f.

Then

exp⁡(t⁢L/2)⁢f=exp⁡(12⁢t⁢⟨A-1⁢ξ,ξ⟩)⁢f.

On the other hand, for x∈ℝN, applying Theorem 2,

∫ℝNf⁢(x-t1/2⁢y)⁢𝑑μA⁢(y) =∫ℝNe⟨ξ,x-t1/2⁢y⟩⁢𝑑μA⁢(y)
=e⟨λ,x⟩⁢∫ℝNe⟨-t1/2⁢ξ,y⟩⁢𝑑μA⁢(y)
=e⟨λ,x⟩⁢e12⁢⟨A-1⁢(-t1/2⁢ξ),(-t1/2⁢ξ)⟩
=e12⁢t⁢⟨A-1⁢ξ,ξ⟩⁢f.

Therefore

∫ℝNf⁢(x-t1/2⁢y)⁢𝑑μA⁢(y)=et⁢L/2⁢f.

∎

4 Concentration of measure

Let γN be the Borel probability measure on ℝN defined by

d⁢γN⁢(x)=(2⁢π)-N/2⁢e-12⁢⟨x,x⟩⁢d⁢λN⁢(x).

We estimate the mass γN assigns to a spherical shell about the sphere of radius N1/2.44 4 Alexander Barvinok, Measure Concentration, http://www.math.lsa.umich.edu/~barvinok/total710.pdf, p. 5, Proposition 2.2.

Theorem 4.

For δ≥0,

γN⁢{x∈ℝN:∥x∥2≥N+δ}≤(NN+δ)-N/2⁢e-δ/2,

and for 0<δ≤N,

γN⁢{x∈ℝN:∥x∥2≤N-δ}≤(NN-δ)-N/2⁢eδ/2.
Proof.

For 0<λ<1, if ∥x∥2≥N+δ then λ⁢∥x∥2/2≥λ⁢(N+δ)/2 and then eλ⁢∥x∥2/2≥eλ⁢(N+δ)/2. Hence

γN⁢{x∈ℝN:∥x∥2≥N+δ} =e-λ⁢(N+δ)/2⁢∫∥x∥2≥N+δeλ⁢(N+δ)/2⁢𝑑γN⁢(x)
≤e-λ⁢(N+δ)/2⁢∫∥x∥2≥N+δeλ⁢∥x∥2/2⁢𝑑γN⁢(x)
≤e-λ⁢(N+δ)/2⁢∫ℝNeλ⁢∥x∥2/2⁢𝑑γN⁢(x)
=e-λ⁢(N+δ)/2⋅(2⁢π)-N/2⁢∫ℝNeλ⁢∥x∥2/2⁢e-12⁢∥x∥2⁢𝑑λN⁢(x)
=e-λ⁢(N+δ)/2⋅∏k=1N(2⁢π)-1/2⁢∫ℝe(λ-1)⁢u2/2⁢𝑑u.

For a=-λ+1>0, we have by Theorem 1

(2⁢π)-1/2⁢∫ℝe-a⁢u2/2⁢𝑑u=a-1/2,

so

γN⁢{x∈ℝN:∥x∥2≥N+δ}≤e-λ⁢(N+δ)/2⁢a-N/2=e-λ⁢(N+δ)/2⁢(1-λ)-N/2.

For λ=δN+δ this is

γN⁢{x∈ℝN:∥x∥2≥N+δ}≤e-δ/2⁢(NN+δ)-N/2.

∎

Let ΣN={x∈ℝN:∥x∥=N1/2}, and let μN be the unique S⁢O⁢(N)-invariant Borel probability measure on SN-1 (any Borel probability measure on a metric space is regular so we need not explicitly demand this to ensure uniqueness). Let πN:ΣN→ℝ be the projection

πN⁢(x)=πN⁢(x1,…,xN)=x1,

and let νN=(πN)*⁢μN, the pushforward measure which is itself a Borel probability measure on ℝ. The following theorem states that the measures νN converges strongly to the standard Gaussian measure γ1.55 5 Alexander Barvinok, Measure Concentration, http://www.math.lsa.umich.edu/~barvinok/total710.pdf, p. 54, Theorem 13.2.

Theorem 5.

For A a Borel set in ℝ,

νN⁢(A)→γ1⁢(A)

as N→∞.

5 Zeta functions

Let A>0, with eigenvalues λ1,…,λN, counted according to multiplicity. For s∈ℂ, define66 6 Eberhard Zeidler, Quantum Field Theory I: Basics in Mathematics and Physics, p. 434, §7.23.3.

ζA⁢(s)=∑k=1Nλk-s=∑k=1Ne-s⁢log⁡λk.

The derivative of ζA is

ζA′⁢(s)=∑k=1N-log⁡λk⋅λk-s,

so

ζA′⁢(0)=-∑k=1Nlog⁡λk,

hence

e-ζA′⁢(0)=∏k=1Nλk=det⁡A.
Theorem 6.

For ξ∈ℝN,

(2⁢π)-N/2⁢∫ℝNexp⁡(-12⁢⟨A⁢x,x⟩-i⁢⟨ξ,x⟩)⁢𝑑x=eζA′⁢(0)/2⁢exp⁡(-12⁢⟨A-1⁢ξ,ξ⟩).

Let λk>0, k≥1, and let A⁢ek=λk⁢ek, and if it makes sense let

det⁡A=∏k=1∞λk.

For those complex s for which the expression makes sense, let

ζA⁢(s)=∑k=1∞λk-s=∑k=1∞e-s⁢log⁡λk.

Then, if the above makes sense in a neighborhood of s=0,

ζA′⁢(0)=-∑k=1∞log⁡λk,

so

e-ζA′⁢(0)=det⁡A.

We calculate, doing the change of variables t=λk⁢u,

Γ⁢(s)⁢ζA⁢(s) =∫0∞ts-1⁢e-t⁢𝑑t⋅∑k=1∞λk-s
=∑k=1∞λk-s⁢∫0∞ts-1⁢e-t⁢𝑑t
=∑k=1∞λk-s⁢∫0∞(λk⁢u)s-1⁢e-λk⁢u⁢λk⁢𝑑u
=∑k=1∞∫0∞us-1⁢e-λk⁢u⁢𝑑u.

Thus

ζA⁢(s)=1Γ⁢(s)⁢∫0∞us-1⁢∑k=1∞e-λk⁢u⁢d⁢u.

For γ>0, the eigenvalues of γ⁢A are γ⁢λk, and doing the change of variables v=γ⁢u,

ζγ⁢A⁢(s) =1Γ⁢(s)⁢∫0∞us-1⁢∑k=1∞e-γ⁢λk⁢u⁢d⁢u
=1Γ⁢(s)⁢∫0∞γ-s⁢vs-1⁢∑k=1∞e-λk⁢v⁢d⁢v
=γ-s⁢ζA⁢(s).

Taking the derivative,

ζγ⁢A′⁢(s)=-log⁡γ⋅γ-s⋅ζA⁢(s)+γ-s⁢γA′⁢(s),

and then

ζγ⁢A′⁢(0)=-log⁡γ⋅ζA⁢(0)+ζA′⁢(0).

Then

det⁡(γ⁢A)=e-ζγ⁢A′⁢(0)=elog⁡γ⋅ζA⁢(0)-ζA′⁢(0)=γζA⁢(0)⁢det⁡A.