TheoremBase

Split the Gibbs score into beta times the noise score field plus the noise gradient of V. The first pairing is the Gaussian Ornstein-Uhlenbeck functional and the second is the coordinate sum of the products of the partial derivatives of V and f; together they give beta times the Gibbs Ornstein-Uhlenbeck functional. The operator formula then follows from the pointwise form of the Hamilton-Jacobi operator and the coordinate formula for the noise norm.

Proof

Each result cited is universally quantified over the data in its own statement. Elementary real-number arithmetic and the manipulation of finite sums are carried by The Real Numbers: Standing Notation and Background §background.

Throughout, the notation of Probability Measures on a Hilbert Space Transported in the Noise Norm: Standing Notation is in force by A Diagonal Gaussian Reference Measure on the Noise Wasserstein Space, Rescaled Heads and Gaussian Tails: Standing Notation §background, so Integrals of Bounded C^2 Cylindrical Functions are Noise Intrinsic Test Functions with the Noise Gradient as Gradient applies to nn, ff, φ=f∘pn\varphi=f\circ p_{n} and UφU_{\varphi}. Let dd be the head dimension of VV (Admissible Cylindrical Potentials on a Hilbert Space in the Noise Geometry §admissible), so that ∂kV=0\partial_{k}V=0 for k>dk>d by Admissible Cylindrical Potentials on a Hilbert Space in the Noise Geometry §gradient. By The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §penalty-domain and The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §score-domain, DΣ⊆D⊆Pρa\mathcal{D}_{\Sigma}\subseteq\mathcal{D}\subseteq\mathcal{P}^{a}_{\rho}, and every μ∈D\mu\in\mathcal{D} lies in P2(X)\mathcal{P}_{2}(X) with VV integrable with respect to μ\mu (Entropy and Score Relative to the Gibbs Measure Split into Their Gaussian Parts and the Potential, with a Fisher Information Bound §entropy, Entropy and Score Relative to the Gibbs Measure Split into Their Gaussian Parts and the Potential, with a Fisher Information Bound §domain).

Claim 1. Since D⊆Pρa\mathcal{D}\subseteq\mathcal{P}^{a}_{\rho}, Integrals of Bounded C^2 Cylindrical Functions are Noise Intrinsic Test Functions with the Noise Gradient as Gradient §test, applied with Q=DQ=\mathcal{D}, shows that UφU_{\varphi} is a noise intrinsic test function on D\mathcal{D}, and for μ∈D⊆Pρa\mu\in\mathcal{D}\subseteq\mathcal{P}^{a}_{\rho}, Integrals of Bounded C^2 Cylindrical Functions are Noise Intrinsic Test Functions with the Noise Gradient as Gradient §gradient gives ∇Uφ(μ)=∇aφ\nabla U_{\varphi}(\mu)=\nabla_{a}\varphi in L2(μ;Xa)L^{2}(\mu;X^{a}).

Preparation: coordinates of ∇aφ\nabla_{a}\varphi. Since f∈Cb2(Rn)f\in C^{2}_{b}(\mathbb{R}^{n}), also f∈Cb1(Rn)f\in C^{1}_{b}(\mathbb{R}^{n}), as recorded in The Noise Score Field of a Measure of Finite Weighted Fisher Information: Existence, Norm, Pairing with Noise Gradients, Head Approximation and Tangency §pairing-functional; so (n,f)(n,f) is a representation of φ∈FCb1(X)\varphi\in\mathcal{F}C^{1}_{b}(X), and by Bounded C^1 Cylindrical Functions: Linear Structure, the Gradient and the Partial Derivatives, Bounds and Integrability, and Density in the Square-Integrable Functions §partial ∂kφ=(∂kf)∘pn\partial_{k}\varphi=(\partial_{k}f)\circ p_{n} for k∈[n]k\in[n]. By The Noise Gradient of a Cylindrical Function and the Noise Tangent Space at a Probability Measure on a Hilbert Space §gradient, computed with (n,f)(n,f), the kk-th coordinate of ∇aφ(x)∈Xa\nabla_{a}\varphi(x)\in X^{a} is ak∂kf(pn(x))a_{k}\partial_{k}f(p_{n}(x)) for k≤nk\le n and 00 for k>nk>n, and

∣∇aφ(x)∣a2=∑k=1nak ∂kf(pn(x))2(x∈X).(1)|\nabla_{a}\varphi(x)|_{a}^{2}=\sum_{k=1}^{n}a_{k}\,\partial_{k}f(p_{n}(x))^{2}\qquad(x\in X).\tag{1}

Claim 2. Let μ∈DΣ\mu\in\mathcal{D}_{\Sigma}. Then μ∈D\mu\in\mathcal{D}, so ∇Uφ(μ)=∇aφ\nabla U_{\varphi}(\mu)=\nabla_{a}\varphi by claim 1, and Σ(μ)=βZμa+∇aV\Sigma(\mu)=\beta Z^{a}_{\mu}+\nabla_{a}V by The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §pair, where, by The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §score-domain, μ\mu has a relative score with respect to γc\gamma_{c} and finite Fisher information relative to γc\gamma_{c} with weights aa, ∫X∣∇aV∣a2 dμ<∞\int_{X}|\nabla_{a}V|_{a}^{2}\,d\mu<\infty, and the class of ∇aV\nabla_{a}V lies in Tμa⊆L2(μ;Xa)T^{a}_{\mu}\subseteq L^{2}(\mu;X^{a}). The inner product of the real Hilbert space L2(μ;Xa)L^{2}(\mu;X^{a}) (Probability Measures on a Hilbert Space Transported in the Noise Norm: Standing Notation §fields) is bilinear, so

⟨Σ(μ),∇aφ⟩μ=β ⟨Zμa,∇aφ⟩μ+⟨∇aV,∇aφ⟩μ.(2)\langle\Sigma(\mu),\nabla_{a}\varphi\rangle_{\mu}=\beta\,\langle Z^{a}_{\mu},\nabla_{a}\varphi\rangle_{\mu}+\langle\nabla_{a}V,\nabla_{a}\varphi\rangle_{\mu}.\tag{2}

The Gaussian term. As μ∈P2(X)\mu\in\mathcal{P}_{2}(X), the hypotheses of The Noise Score Field of a Measure of Finite Weighted Fisher Information: Existence, Norm, Pairing with Noise Gradients, Head Approximation and Tangency hold, and The Noise Score Field of a Measure of Finite Weighted Fisher Information: Existence, Norm, Pairing with Noise Gradients, Head Approximation and Tangency §pairing-functional (with the function there called gg taken to be ff) gives ⟨Zμa,∇aφ⟩μ=Lμa(f)\langle Z^{a}_{\mu},\nabla_{a}\varphi\rangle_{\mu}=L^{a}_{\mu}(f), the noise Ornstein-Uhlenbeck functional.

The potential term. By The Space of Square-Integrable Maps from a Measure Space into a Hilbert Space with an Orthonormal Basis §operations (with E=XaE=X^{a}, as fixed in Probability Measures on a Hilbert Space Transported in the Noise Norm: Standing Notation §fields), ⟨∇aV,∇aφ⟩μ=∫X⟨∇aV(x),∇aφ(x)⟩a μ(dx)\langle\nabla_{a}V,\nabla_{a}\varphi\rangle_{\mu}=\int_{X}\langle\nabla_{a}V(x),\nabla_{a}\varphi(x)\rangle_{a}\,\mu(dx). For x∈Xx\in X, Basic Properties of an Admissible Cylindrical Potential: Continuity, Growth under Noise Translations, Integrability, the Tangent Inequality and Tangency of the Noise Gradient §continuity, applied with h=∇aφ(x)∈Xah=\nabla_{a}\varphi(x)\in X^{a} and the coordinates of the preparation, gives

⟨∇aV(x),∇aφ(x)⟩a=∑k=1d∂kV(x) hk=∑k=1nak ∂kV(x) ∂kf(pn(x)),\langle\nabla_{a}V(x),\nabla_{a}\varphi(x)\rangle_{a}=\sum_{k=1}^{d}\partial_{k}V(x)\,h_{k}=\sum_{k=1}^{n}a_{k}\,\partial_{k}V(x)\,\partial_{k}f(p_{n}(x)),

since both sums equal the sum over k≤min⁡(d,n)k\le\min(d,n): in the first, hk=0h_{k}=0 for k>nk>n; in the second, ∂kV(x)=0\partial_{k}V(x)=0 for k>dk>d. For k∈[n]k\in[n] the function x↦∂kV(x)∂kf(pn(x))x\mapsto\partial_{k}V(x)\partial_{k}f(p_{n}(x)) is integrable with respect to μ\mu, as recorded in the preamble of The Gibbs Ornstein-Uhlenbeck Functional of a Probability Measure at a Bounded C^2 Function of Finitely Many Coordinates (which applies since μ∈P2(X)\mu\in\mathcal{P}_{2}(X) and VV is integrable with respect to μ\mu). By Linearity and Monotonicity of the Lebesgue Integral §integrable,

⟨∇aV,∇aφ⟩μ=∑k=1nak∫X∂kV(x) ∂kf(pn(x)) μ(dx).\langle\nabla_{a}V,\nabla_{a}\varphi\rangle_{\mu}=\sum_{k=1}^{n}a_{k}\int_{X}\partial_{k}V(x)\,\partial_{k}f(p_{n}(x))\,\mu(dx).

Assembly. In The Gibbs Ornstein-Uhlenbeck Functional of a Probability Measure at a Bounded C^2 Function of Finitely Many Coordinates §functional, read with g=fg=f, the kk-th integrand is the sum of xkck∂kf(pn(x))−∂k∂kf(pn(x))\frac{x_{k}}{c_{k}}\partial_{k}f(p_{n}(x))-\partial_{k}\partial_{k}f(p_{n}(x)) and β−1∂kV(x)∂kf(pn(x))\beta^{-1}\partial_{k}V(x)\partial_{k}f(p_{n}(x)), each integrable (as recorded there and in The Noise Ornstein-Uhlenbeck Functional of a Probability Measure at a Bounded C^2 Function of Finitely Many Coordinates); by Linearity and Monotonicity of the Lebesgue Integral §integrable and The Noise Ornstein-Uhlenbeck Functional of a Probability Measure at a Bounded C^2 Function of Finitely Many Coordinates §functional,

Lμa,V(f)=Lμa(f)+1β∑k=1nak∫X∂kV(x) ∂kf(pn(x)) μ(dx).L^{a,V}_{\mu}(f)=L^{a}_{\mu}(f)+\frac{1}{\beta}\sum_{k=1}^{n}a_{k}\int_{X}\partial_{k}V(x)\,\partial_{k}f(p_{n}(x))\,\mu(dx).

Multiplying by β\beta and comparing with (2) and the two terms computed above gives ⟨Σ(μ),∇Uφ(μ)⟩μ=β Lμa,V(f)\langle\Sigma(\mu),\nabla U_{\varphi}(\mu)\rangle_{\mu}=\beta\,L^{a,V}_{\mu}(f).

Claim 3. Let μ∈DΣ\mu\in\mathcal{D}_{\Sigma} and r∈Rr\in\mathbb{R}. By claim 1, ∇Uφ(μ)=∇aφ\nabla U_{\varphi}(\mu)=\nabla_{a}\varphi is an element of L2(μ;Xa)L^{2}(\mu;X^{a}), and μ∈DΣ⊆Pρa\mu\in\mathcal{D}_{\Sigma}\subseteq\mathcal{P}^{a}_{\rho}, so (μ,∇Uφ(μ))(\mu,\nabla U_{\varphi}(\mu)) belongs to the bundle Va(DΣ)\mathcal{V}^{a}(\mathcal{D}_{\Sigma}) of The Bundle of Noise Fields over a Set of Measures, First-Order Equation Operators on the Noise Wasserstein Space, and Their Delta-Shifts §bundle, applied with Q=DΣQ=\mathcal{D}_{\Sigma}. Then The Hamilton-Jacobi Equation with Gibbs Score Drift on a Hilbert Space §operator, applied with ν=μ\nu=\mu, the real number rr and q=∇aφq=\nabla_{a}\varphi, gives

F(μ,r,∇Uφ(μ))=λ0 r+θ2 ∥∇aφ∥μ2+β ⟨Zμa,∇aφ⟩μ+⟨∇aV,∇aφ⟩μ−g(μ),F\bigl(\mu,r,\nabla U_{\varphi}(\mu)\bigr)=\lambda_{0}\,r+\frac{\theta}{2}\,\lVert\nabla_{a}\varphi\rVert_{\mu}^{2}+\beta\,\langle Z^{a}_{\mu},\nabla_{a}\varphi\rangle_{\mu}+\langle\nabla_{a}V,\nabla_{a}\varphi\rangle_{\mu}-g(\mu),

and by (2) and claim 2 the sum of the third and fourth terms is ⟨Σ(μ),∇aφ⟩μ=β Lμa,V(f)\langle\Sigma(\mu),\nabla_{a}\varphi\rangle_{\mu}=\beta\,L^{a,V}_{\mu}(f). It remains to compute the norm. By The Space of Square-Integrable Maps from a Measure Space into a Hilbert Space with an Orthonormal Basis §operations, ∥∇aφ∥μ2=∫X∣∇aφ∣a2 dμ\lVert\nabla_{a}\varphi\rVert_{\mu}^{2}=\int_{X}|\nabla_{a}\varphi|_{a}^{2}\,d\mu, the square of the nonnegative square root of a nonnegative real number being that number. For k∈[n]k\in[n] the function ∂kφ\partial_{k}\varphi is Borel by Bounded C^1 Cylindrical Functions: Linear Structure, the Gradient and the Partial Derivatives, Bounds and Integrability, and Density in the Square-Integrable Functions §bounded-borel, so (∂kφ)2=∣∂kφ∣2(\partial_{k}\varphi)^{2}=|\partial_{k}\varphi|^{2} is measurable and nonnegative by Power-Integrable Functions and the p-Seminorm §measurable-power with p=2p=2, with finite integral, ∂kφ\partial_{k}\varphi being 22-integrable with respect to μ\mu by Bounded C^1 Cylindrical Functions: Linear Structure, the Gradient and the Partial Derivatives, Bounds and Integrability, and Density in the Square-Integrable Functions §square-integrable in the sense of Power-Integrable Functions and the p-Seminorm §space. By (1) and the additivity and positive homogeneity of the integral of nonnegative measurable functions in Linearity and Monotonicity of the Lebesgue Integral §nonnegative,

∥∇aφ∥μ2=∫X∑k=1nak ∂kf(pn(x))2 μ(dx)=∑k=1nak∫X∂kf(pn(x))2 μ(dx),\lVert\nabla_{a}\varphi\rVert_{\mu}^{2}=\int_{X}\sum_{k=1}^{n}a_{k}\,\partial_{k}f(p_{n}(x))^{2}\,\mu(dx)=\sum_{k=1}^{n}a_{k}\int_{X}\partial_{k}f(p_{n}(x))^{2}\,\mu(dx),

a finite sum of real numbers. Substituting gives the display of claim 3.

Citations

Loading…

Dependencies

Uses0

Loading…

Comments

Log in to comment.

Loading…