TheoremBase

The Gibbs score splits into the Gaussian score plus the noise gradient of the potential; the Fisher information bound makes both parts uniformly bounded, the Gaussian closed-score lemma handles the first part, and a truncation and density argument along the couplings handles the second.

Proof

Each result cited is universally quantified over the data in its own statement.

Real order and arithmetic, square roots, the Archimedean property, limits of real sequences with their limit laws and order properties, and claim 2 of Uniqueness of Limits and Boundedness of Convergent Real Sequences (convergent real sequences are bounded) are used through The Real Numbers: Standing Notation and Background §background, without further mention.

Reduction. Let dd be the head dimension and vv the profile of V=v∘pdV=v\circ p_{d}, with the noise gradient ∇aV\nabla_{a}V and the functions ∂kV\partial_{k}V of Admissible Cylindrical Potentials on a Hilbert Space in the Noise Geometry §gradient, and write (D,DΣ,E,Σ)(\mathcal{D},\mathcal{D}_{\Sigma},\mathcal{E},\Sigma) for the Gibbs entropy pair of the statement. By Noise Penalty Pairs with Closed Score Along Noise Couplings §closed, with sequences of couplings of vanishing noise cost and weak convergence along them those of Strong and Weak Convergence of Noise Fields Along Couplings of Vanishing Noise Cost §couplings and Strong and Weak Convergence of Noise Fields Along Couplings of Vanishing Noise Cost §weak, as fixed by First-Order Equations on the Noise Wasserstein Space Relative to a Noise Penalty Pair: Standing Notation §couplings, we must show the following. Let R∈RR\in\mathbb{R} be nonnegative, let (νn)n∈N(\nu_{n})_{n\in\mathbb{N}} be a sequence in DΣ\mathcal{D}_{\Sigma} with ∥Σ(νn)∥νn≤R\lVert\Sigma(\nu_{n})\rVert_{\nu_{n}}\le R for every n∈Nn\in\mathbb{N}, let ν∈D\nu\in\mathcal{D}, and let (πn)n∈N(\pi_{n})_{n\in\mathbb{N}} satisfy πn∈Πa(νn,ν)\pi_{n}\in\Pi^{a}(\nu_{n},\nu) for every nn and lim⁡n→∞Ia(πn)=0\lim_{n\to\infty}I^{a}(\pi_{n})=0. Then ν∈DΣ\nu\in\mathcal{D}_{\Sigma}, and lim⁡n→∞Ka(Σ(νn),η,πn)=⟨Σ(ν),η⟩ν\lim_{n\to\infty}\mathcal{K}^{a}(\Sigma(\nu_{n}),\eta,\pi_{n})=\langle\Sigma(\nu),\eta\rangle_{\nu} for every η∈L2(ν;Xa)\eta\in L^{2}(\nu;X^{a}). We fix RR, (νn)n∈N(\nu_{n})_{n\in\mathbb{N}}, ν\nu and (πn)n∈N(\pi_{n})_{n\in\mathbb{N}}. As in Probability Measures on a Hilbert Space Transported in the Noise Norm: Standing Notation §background, a point z∈X×Xz\in X\times X is written z=(x,y)z=(x,y) with x=π1(z)x=\pi_{1}(z) and y=π2(z)y=\pi_{2}(z); aˉ\bar{a} is the real bound ak≤aˉa_{k}\le\bar{a} (k∈Nk\in\mathbb{N}) on the noise weights fixed by the setting, and (ek)k∈N(e_{k})_{k\in\mathbb{N}}, (fk)k∈N(f_{k})_{k\in\mathbb{N}} and the coordinates xk=⟨x,ek⟩x_{k}=\langle x,e_{k}\rangle are those of the setting. Limits are taken as n→∞n\to\infty.

Step 0 (membership). By The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §score-domain and The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §penalty-domain, ν\nu and every νn\nu_{n} lie in D⊆Pρa\mathcal{D}\subseteq\mathcal{P}^{a}_{\rho} and have finite relative entropy with respect to γβV\gamma^{V}_{\beta}. By Entropy and Score Relative to the Gibbs Measure Split into Their Gaussian Parts and the Potential, with a Fisher Information Bound §entropy, each of them has finite relative entropy with respect to γc\gamma_{c} and VV is integrable with respect to it; by Entropy and Score Relative to the Gibbs Measure Split into Their Gaussian Parts and the Potential, with a Fisher Information Bound §domain, each of them lies in P2(X)\mathcal{P}_{2}(X). By The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §score-domain, each νn\nu_{n} has a relative score with respect to γβV\gamma^{V}_{\beta} and finite Fisher information relative to γβV\gamma^{V}_{\beta} with weights aa, and also a relative score with respect to γc\gamma_{c}, finite Fisher information relative to γc\gamma_{c} with weights aa, and ∫X∣∇aV∣a2 dνn<∞\int_{X}|\nabla_{a}V|_{a}^{2}\,d\nu_{n}<\infty. Let Zn=Zνna∈L2(νn;Xa)Z_{n}=Z^{a}_{\nu_{n}}\in L^{2}(\nu_{n};X^{a}) be the noise score field of νn\nu_{n}, so that ∥Zn∥νn2=Ia(νn ∣ γc)\lVert Z_{n}\rVert_{\nu_{n}}^{2}=\mathcal{I}_{a}(\nu_{n}\,|\,\gamma_{c}) by The Noise Score Field of a Measure of Finite Weighted Fisher Information: Existence, Norm, Pairing with Noise Gradients, Head Approximation and Tangency §field. By Basic Properties of an Admissible Cylindrical Potential: Continuity, Growth under Noise Translations, Integrability, the Tangent Inequality and Tangency of the Noise Gradient §tangent the class of ∇aV\nabla_{a}V lies in L2(νn;Xa)L^{2}(\nu_{n};X^{a}), and by The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §pair, Σ(νn)=βZn+∇aV\Sigma(\nu_{n})=\beta Z_{n}+\nabla_{a}V.

Step 1 (integrals of functions of quadratic growth). We show: if h:X→Rh:X\to\mathbb{R} is continuous and there is A′∈RA'\in\mathbb{R} with ∣h(x)∣≤A′(1+∣x∣2)|h(x)|\le A'(1+|x|^{2}) for every x∈Xx\in X, then hh is integrable with respect to ν\nu and every νn\nu_{n}, and lim⁡∫Xh dνn=∫Xh dν\lim\int_{X}h\,d\nu_{n}=\int_{X}h\,d\nu. Since πn∈Πa(νn,ν)\pi_{n}\in\Pi^{a}(\nu_{n},\nu), the pair (νn,ν)(\nu_{n},\nu) is noise-connected by Couplings of Finite Noise Cost and Their Noise Cost §connected, and Wa(νn,ν)2≤Ia(πn)W_{a}(\nu_{n},\nu)^{2}\le I^{a}(\pi_{n}) by The Noise Wasserstein Distance §distance. As νn,ν∈Pρa\nu_{n},\nu\in\mathcal{P}^{a}_{\rho} by Step 0, The Noise Wasserstein Distance is a Metric on the Measures Noise-Connected to the Reference Measure: Existence of Noise-Optimal Couplings, Comparison with the Quadratic Wasserstein Distance and Lower Semicontinuity §comparison gives W2(νn,ν)≤aˉ Wa(νn,ν)W_{2}(\nu_{n},\nu)\le\sqrt{\bar{a}}\,W_{a}(\nu_{n},\nu), hence 0≤W2(νn,ν)2≤aˉ Ia(πn)0\le W_{2}(\nu_{n},\nu)^{2}\le\bar{a}\,I^{a}(\pi_{n}). Given a positive ε∈R\varepsilon\in\mathbb{R}, aˉ Ia(πn)<ε2\bar{a}\,I^{a}(\pi_{n})<\varepsilon^{2} for all large nn, and then W2(νn,ν)<εW_{2}(\nu_{n},\nu)<\varepsilon; so lim⁡W2(νn,ν)=0\lim W_{2}(\nu_{n},\nu)=0, and since νn,ν∈P2(X)\nu_{n},\nu\in\mathcal{P}_{2}(X) by Step 0, the claim is Wasserstein Convergence on a Hilbert Space: Weak Convergence, Integrals of Continuous Functions of Quadratic Growth, Convergence from Weak Convergence with Uniformly Integrable Second Moments, and Compactness §quadratic.

We shall use repeatedly that finite sums and products of continuous real functions on XX are continuous: if u1,u2:X→Ru_{1},u_{2}:X\to\mathbb{R} are continuous, every sequence converging to a point xx of XX is carried by u1u_{1} and u2u_{2} to sequences converging to u1(x)u_{1}(x) and u2(x)u_{2}(x) by Continuity Between Metric Spaces is Equivalent to Sequential Continuity §sequential, so by the limit laws the same holds for u1+u2u_{1}+u_{2} and u1u2u_{1}u_{2}, which are therefore continuous by Continuity Between Metric Spaces is Equivalent to Sequential Continuity §on-subset; the same criterion shows that constant functions are continuous, as they carry every sequence to a constant sequence. Continuous real functions on XX are Borel by claim 3 of Borel Measurability and Bounded Integration on a Metric Space.

Step 2 (uniform bounds). Let n∈Nn\in\mathbb{N}. By Step 0, νn\nu_{n} satisfies the hypotheses of Entropy and Score Relative to the Gibbs Measure Split into Their Gaussian Parts and the Potential, with a Fisher Information Bound §field, which gives ∥Σ(νn)∥νn2=∥βZn+∇aV∥νn2=β2 Ia(νn ∣ γβV)\lVert\Sigma(\nu_{n})\rVert_{\nu_{n}}^{2}=\lVert\beta Z_{n}+\nabla_{a}V\rVert_{\nu_{n}}^{2}=\beta^{2}\,\mathcal{I}_{a}(\nu_{n}\,|\,\gamma^{V}_{\beta}); hence 0≤β2 Ia(νn ∣ γβV)≤R20\le\beta^{2}\,\mathcal{I}_{a}(\nu_{n}\,|\,\gamma^{V}_{\beta})\le R^{2}.

Let h0:X→Rh_{0}:X\to\mathbb{R}, h0(x)=∑k=1dxk2h_{0}(x)=\sum_{k=1}^{d}x_{k}^{2}. Each coordinate function x↦xkx\mapsto x_{k} is Lipschitz by Borel Sets of a Hilbert Space with an Orthonormal Basis: Coordinates, Determination by Finite-Dimensional Projections, and Pairs §continuity, hence continuous by A Lipschitz Map is Uniformly Continuous and Continuous, so h0h_{0} is continuous. By Elementary Properties of the Euclidean Norm on Rn\mathbb{R}^n §square, h0(x)=∥pd(x)∥2h_{0}(x)=\lVert p_{d}(x)\rVert^{2}; since all coordinates of 0X0_{X} vanish, pd(0X)p_{d}(0_{X}) is the origin of Rd\mathbb{R}^{d}, and Borel Sets of a Hilbert Space with an Orthonormal Basis: Coordinates, Determination by Finite-Dimensional Projections, and Pairs §continuity gives ∥pd(x)∥≤∣x∣\lVert p_{d}(x)\rVert\le|x|. So 0≤h0(x)≤∣x∣2≤1+∣x∣20\le h_{0}(x)\le|x|^{2}\le1+|x|^{2}, and by Step 1 the sequence of the real numbers mn=∫Xh0 dνnm_{n}=\int_{X}h_{0}\,d\nu_{n} converges to ∫Xh0 dν\int_{X}h_{0}\,d\nu. A convergent real sequence being bounded, there is a nonnegative M∈RM\in\mathbb{R} with mn≤Mm_{n}\le M for every n∈Nn\in\mathbb{N}.

Let C∗∈RC_{*}\in\mathbb{R} be the constant of Entropy and Score Relative to the Gibbs Measure Split into Their Gaussian Parts and the Potential, with a Fisher Information Bound §fisher-bound, which depends only on VV, β\beta, aa and cc, and put A=∣C∗∣ (1+R2+M)A=|C_{*}|\,(1+R^{2}+M), a nonnegative real number. By Step 0 each νn\nu_{n} lies in P2(X)\mathcal{P}_{2}(X), VV is integrable with respect to it, and it has a relative score with respect to γβV\gamma^{V}_{\beta} and finite Fisher information relative to γβV\gamma^{V}_{\beta} with weights aa; so that clause gives

β2 Ia(νn ∣ γc)+∫X∣∇aV∣a2 dνn≤C∗(1+β2 Ia(νn ∣ γβV)+mn)≤∣C∗∣ (1+R2+M)=A,\beta^{2}\,\mathcal{I}_{a}(\nu_{n}\,|\,\gamma_{c})+\int_{X}|\nabla_{a}V|_{a}^{2}\,d\nu_{n}\le C_{*}\bigl(1+\beta^{2}\,\mathcal{I}_{a}(\nu_{n}\,|\,\gamma^{V}_{\beta})+m_{n}\bigr)\le|C_{*}|\,(1+R^{2}+M)=A,

the bracket lying between 00 and 1+R2+M1+R^{2}+M by the previous two paragraphs. Both summands on the left are nonnegative, the first being β2∥Zn∥νn2\beta^{2}\lVert Z_{n}\rVert_{\nu_{n}}^{2} by Step 0 and the second the integral of a nonnegative function. Since ∥⋅∥νn\lVert\cdot\rVert_{\nu_{n}} is the norm of The Space of Square-Integrable Maps from a Measure Space into a Hilbert Space with an Orthonormal Basis §operations, we obtain for every n∈Nn\in\mathbb{N}

(2a)∥βZn∥νn2≤A,(2b)∥∇aV∥νn2=∫X∣∇aV∣a2 dνn≤A.\textup{(2a)}\quad\lVert\beta Z_{n}\rVert_{\nu_{n}}^{2}\le A,\qquad\qquad\textup{(2b)}\quad\lVert\nabla_{a}V\rVert_{\nu_{n}}^{2}=\int_{X}|\nabla_{a}V|_{a}^{2}\,d\nu_{n}\le A .

Step 3 (the Gaussian part). Let (DG,DΣG,EG,ΣG)(\mathcal{D}^{G},\mathcal{D}^{G}_{\Sigma},\mathcal{E}^{G},\Sigma^{G}) be the Gaussian entropy pair with temperature β\beta of The Gaussian Entropy Pair on the Noise Wasserstein Space: Relative Entropy and the Noise Score Field §pair, whose hypothesis The Gaussian Entropy Pair on the Noise Wasserstein Space: Relative Entropy and the Noise Score Field §hypothesis holds with the κ\kappa of the statement. By Step 0 and The Gaussian Entropy Pair on the Noise Wasserstein Space: Relative Entropy and the Noise Score Field §penalty-domain, ν\nu and every νn\nu_{n} lie in DG\mathcal{D}^{G}; by Step 0 and The Gaussian Entropy Pair on the Noise Wasserstein Space: Relative Entropy and the Noise Score Field §score-domain, every νn\nu_{n} lies in DΣG\mathcal{D}^{G}_{\Sigma}; and by The Gaussian Entropy Pair on the Noise Wasserstein Space: Relative Entropy and the Noise Score Field §pair, ΣG(νn)=βZn\Sigma^{G}(\nu_{n})=\beta Z_{n}, so ∥ΣG(νn)∥νn≤A1/2\lVert\Sigma^{G}(\nu_{n})\rVert_{\nu_{n}}\le A^{1/2} by (2a). The sequence (πn)n∈N(\pi_{n})_{n\in\mathbb{N}} is a sequence of couplings of vanishing noise cost from (νn)n∈N(\nu_{n})_{n\in\mathbb{N}} to ν\nu in the sense of Strong and Weak Convergence of Noise Fields Along Couplings of Vanishing Noise Cost §couplings. Hence The Gaussian Entropy Pair Has Closed Score Along Noise Couplings §closed, read through Noise Penalty Pairs with Closed Score Along Noise Couplings §closed with A1/2A^{1/2} in place of its RR, shows that ν∈DΣG\nu\in\mathcal{D}^{G}_{\Sigma} and that (ΣG(νn))n∈N(\Sigma^{G}(\nu_{n}))_{n\in\mathbb{N}} converges weakly to ΣG(ν)\Sigma^{G}(\nu) along (πn)n∈N(\pi_{n})_{n\in\mathbb{N}}. By The Gaussian Entropy Pair on the Noise Wasserstein Space: Relative Entropy and the Noise Score Field §score-domain, ν\nu has a relative score with respect to γc\gamma_{c} and finite Fisher information relative to γc\gamma_{c} with weights aa; let Z=ZνaZ=Z^{a}_{\nu} be its noise score field, so that ΣG(ν)=βZ\Sigma^{G}(\nu)=\beta Z by The Gaussian Entropy Pair on the Noise Wasserstein Space: Relative Entropy and the Noise Score Field §pair. By Strong and Weak Convergence of Noise Fields Along Couplings of Vanishing Noise Cost §weak,

lim⁡Ka(βZn,η,πn)=⟨βZ,η⟩νfor every η∈L2(ν;Xa).\lim\mathcal{K}^{a}(\beta Z_{n},\eta,\pi_{n})=\langle\beta Z,\eta\rangle_{\nu}\qquad\text{for every }\eta\in L^{2}(\nu;X^{a}).

Step 4 (∫X∣∇aV∣a2 dν≤A\int_{X}|\nabla_{a}V|_{a}^{2}\,d\nu\le A). Let g0=∣∇aV∣a2:X→Rg_{0}=|\nabla_{a}V|_{a}^{2}:X\to\mathbb{R}. By Basic Properties of an Admissible Cylindrical Potential: Continuity, Growth under Noise Translations, Integrability, the Tangent Inequality and Tangency of the Noise Gradient §continuity, g0(x)=∑k=1dak ∂kV(x)2g_{0}(x)=\sum_{k=1}^{d}a_{k}\,\partial_{k}V(x)^{2} with each ∂kV\partial_{k}V continuous, so g0g_{0} is continuous and nonnegative. For M′∈NM'\in\mathbb{N} let uM′=min⁡{g0,M′}u_{M'}=\min\{g_{0},M'\}, the pointwise minimum with the constant function M′M'; it is continuous by claim 4 of Continuity of the Absolute Value, Maximum and Minimum of Real-Valued Functions on a Metric Space, hence Borel, and 0≤uM′≤M′≤M′(1+∣x∣2)0\le u_{M'}\le M'\le M'(1+|x|^{2}) by claims 1 and 3 of Elementary Properties of the Minimum of Two Elements. By Step 1, ∫XuM′ dν=lim⁡∫XuM′ dνn\int_{X}u_{M'}\,d\nu=\lim\int_{X}u_{M'}\,d\nu_{n}; and by claim 6(c) of Borel Measurability and Bounded Integration on a Metric Space, for σ=ν\sigma=\nu and for each σ=νn\sigma=\nu_{n} the integral of uM′u_{M'} with respect to σ\sigma is also its integral as a nonnegative function. For each nn, uM′≤g0u_{M'}\le g_{0} (claim 1 of Elementary Properties of the Minimum of Two Elements), so the monotonicity of Linearity and Monotonicity of the Lebesgue Integral §nonnegative and (2b) give ∫XuM′ dνn≤A\int_{X}u_{M'}\,d\nu_{n}\le A, and hence ∫XuM′ dν≤A\int_{X}u_{M'}\,d\nu\le A by the order of limits. By claims 1 and 3 of Elementary Properties of the Minimum of Two Elements, uM′≤uM′+1u_{M'}\le u_{M'+1}, and uM′(x)=g0(x)u_{M'}(x)=g_{0}(x) whenever g0(x)≤M′g_{0}(x)\le M'; for each x∈Xx\in X there is such an M′M' by the Archimedean property, so sup⁡M′uM′(x)=g0(x)\sup_{M'}u_{M'}(x)=g_{0}(x). By Monotone Convergence Theorem on (X,B(X),ν)(X,\mathcal{B}(X),\nu),

∫X∣∇aV∣a2 dν=sup⁡M′∈N∫XuM′ dν≤A<∞.\int_{X}|\nabla_{a}V|_{a}^{2}\,d\nu=\sup_{M'\in\mathbb{N}}\int_{X}u_{M'}\,d\nu\le A<\infty .

By Basic Properties of an Admissible Cylindrical Potential: Continuity, Growth under Noise Translations, Integrability, the Tangent Inequality and Tangency of the Noise Gradient §tangent the class of ∇aV\nabla_{a}V lies in L2(ν;Xa)L^{2}(\nu;X^{a}), and ∥∇aV∥ν2≤A\lVert\nabla_{a}V\rVert_{\nu}^{2}\le A by the norm of The Space of Square-Integrable Maps from a Measure Space into a Hilbert Space with an Orthonormal Basis §operations.

Step 5 (ν∈DΣ\nu\in\mathcal{D}_{\Sigma}). By Step 0, ν∈P2(X)\nu\in\mathcal{P}_{2}(X) and VV is integrable with respect to ν\nu; by Step 3, ν\nu has a relative score with respect to γc\gamma_{c} and finite Fisher information relative to γc\gamma_{c} with weights aa; by Step 4, ∫X∣∇aV∣a2 dν<∞\int_{X}|\nabla_{a}V|_{a}^{2}\,d\nu<\infty. So the ``if'' direction of Entropy and Score Relative to the Gibbs Measure Split into Their Gaussian Parts and the Potential, with a Fisher Information Bound §splitting shows that ν\nu has a relative score with respect to γβV\gamma^{V}_{\beta} and finite Fisher information relative to γβV\gamma^{V}_{\beta} with weights aa. As ν∈D\nu\in\mathcal{D}, The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §score-domain gives ν∈DΣ\nu\in\mathcal{D}_{\Sigma}, and by The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §pair, Σ(ν)=βZνa+∇aV=βZ+∇aV\Sigma(\nu)=\beta Z^{a}_{\nu}+\nabla_{a}V=\beta Z+\nabla_{a}V, with ZZ the noise score field of Step 3.

Step 6 (cylindrical test fields). Let φ∈FCb1(X)\varphi\in\mathcal{F}C^{1}_{b}(X), the set of Bounded C^1 Cylindrical Functions on a Hilbert Space with an Orthonormal Basis §cylindrical, with a representation (m,ψ)(m,\psi) in the sense of Bounded C^1 Cylindrical Functions on a Hilbert Space with an Orthonormal Basis §representation, and let k∈Nk\in\mathbb{N}.

(a) Lipschitz bound. By Bounded Continuously Differentiable Functions with Bounded Partial Derivatives on Euclidean Space §bounded, ψ\psi is of class C1C^{1} on Rm\mathbb{R}^{m} and there are nonnegative reals B,B1,…,BmB,B_{1},\dots,B_{m} with ∣ψ∣≤B|\psi|\le B and ∣∂iψ∣≤Bi|\partial_{i}\psi|\le B_{i} on Rm\mathbb{R}^{m} for i∈[m]i\in[m]; put L=∑i=1mBiL=\sum_{i=1}^{m}B_{i}. Let u,w∈Rmu,w\in\mathbb{R}^{m} and h=u−wh=u-w. The set Rm\mathbb{R}^{m} is open by claim 1 of Euclidean Space is Open in Itself, and CkC^k Maps are Continuous, so claims 2 and 3 of Derivatives Along a Segment for C^1 Functions on a Euclidean Open Set, applied with Rm\mathbb{R}^{m}, ψ\psi, the point ww, the increment hh and the interval [0,1][0,1], show that F(τ)=ψ(w+τh)F(\tau)=\psi(w+\tau h) is continuous on [0,1][0,1] and differentiable at every τ∈(0,1)\tau\in(0,1) with F′(τ)=∑i=1m∂iψ(w+τh) hiF'(\tau)=\sum_{i=1}^{m}\partial_{i}\psi(w+\tau h)\,h_{i}. By Mean Value Theorem on a Closed Real Interval there is τ0∈(0,1)\tau_{0}\in(0,1) with ψ(u)−ψ(w)=F(1)−F(0)=F′(τ0)\psi(u)-\psi(w)=F(1)-F(0)=F'(\tau_{0}), so, by the coordinate bound ∣hi∣≤∥h∥|h_{i}|\le\lVert h\rVert of Elementary Properties of the Euclidean Norm on Rn\mathbb{R}^n §coordinate, ∣ψ(u)−ψ(w)∣≤∑i=1mBi∣hi∣≤L ∥u−w∥|\psi(u)-\psi(w)|\le\sum_{i=1}^{m}B_{i}|h_{i}|\le L\,\lVert u-w\rVert. Taking u=pm(x)u=p_{m}(x) and w=pm(y)w=p_{m}(y) and using ∥pm(x)−pm(y)∥≤∣x−y∣\lVert p_{m}(x)-p_{m}(y)\rVert\le|x-y| from Borel Sets of a Hilbert Space with an Orthonormal Basis: Coordinates, Determination by Finite-Dimensional Projections, and Pairs §continuity, we get ∣φ(x)−φ(y)∣≤L ∣x−y∣|\varphi(x)-\varphi(y)|\le L\,|x-y| for all x,y∈Xx,y\in X. Thus φ\varphi is Lipschitz, hence continuous by A Lipschitz Map is Uniformly Continuous and Continuous, and ∣φ∣≤B|\varphi|\le B.

(b) The field φfk\varphi f_{k}. The map φfk:X→Xa\varphi f_{k}:X\to X^{a}, y↦φ(y)fky\mapsto\varphi(y)f_{k}, takes values in XaX^{a}, a linear subspace of XX containing fk=ak1/2ekf_{k}=a_{k}^{1/2}e_{k} by The Noise Space is a Real Hilbert Space: Orthonormal Basis, Continuous Embedding, Partial Sums, Closed Balls and Borel Measurability §hilbert and The Noise Space is a Real Hilbert Space: Orthonormal Basis, Continuous Embedding, Partial Sums, Closed Balls and Borel Measurability §basis. Its coordinate along eie_{i} is ⟨φ(y)fk,ei⟩=ak1/2φ(y)⟨ek,ei⟩\langle\varphi(y)f_{k},e_{i}\rangle=a_{k}^{1/2}\varphi(y)\langle e_{k},e_{i}\rangle, which is ak1/2φ(y)a_{k}^{1/2}\varphi(y) for i=ki=k and 00 otherwise, a Borel function of yy 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 φfk\varphi f_{k} is measurable into XaX^{a} by The Noise Space is a Real Hilbert Space: Orthonormal Basis, Continuous Embedding, Partial Sums, Closed Balls and Borel Measurability §measurable. By orthonormality of (fi)i∈N(f_{i})_{i\in\mathbb{N}} in XaX^{a} (The Noise Space is a Real Hilbert Space: Orthonormal Basis, Continuous Embedding, Partial Sums, Closed Balls and Borel Measurability §basis), ⟨φ(y)fk,fi⟩a\langle\varphi(y)f_{k},f_{i}\rangle_{a} is φ(y)\varphi(y) for i=ki=k and 00 otherwise, and ∣φ(y)fk∣a2=φ(y)2≤B2|\varphi(y)f_{k}|_{a}^{2}=\varphi(y)^{2}\le B^{2}. Hence, by the monotonicity of Linearity and Monotonicity of the Lebesgue Integral §nonnegative, φfk\varphi f_{k} is square-integrable with respect to every σ∈P(X)\sigma\in\mathcal{P}(X); its class in L2(σ;Xa)L^{2}(\sigma;X^{a}), again written φfk\varphi f_{k}, has coordinates (φfk)k=φ(\varphi f_{k})_{k}=\varphi and (φfk)i=0(\varphi f_{k})_{i}=0 for i≠ki\ne k, in the sense of The Space of Square-Integrable Hilbert-Valued Maps is a Real Hilbert Space: Coordinates and Synthesis §coordinates.

(c) Discrepancy bound. Let n∈Nn\in\mathbb{N}. Since πn∈Πa(νn,ν)⊆Π(νn,ν)\pi_{n}\in\Pi^{a}(\nu_{n},\nu)\subseteq\Pi(\nu_{n},\nu), Noise Displacement and Cross Pairings Along Couplings: Bounds, Linearity, Displacement Couplings, Polarisation and a Vanishing Criterion §discrepancy, applied with νn\nu_{n} and ν\nu in place of its ν\nu and μ\mu and with φfk\varphi f_{k} in both slots, shows that the function z↦∣φ(x)fk−φ(y)fk∣a2=(φ(x)−φ(y))2z\mapsto|\varphi(x)f_{k}-\varphi(y)f_{k}|_{a}^{2}=(\varphi(x)-\varphi(y))^{2} is Borel, nonnegative and integrable with respect to πn\pi_{n}. By (a) it is at most L2∣x−y∣2L^{2}|x-y|^{2}, so by the monotonicity of Linearity and Monotonicity of the Lebesgue Integral §nonnegative, the quadratic cost I(πn)I(\pi_{n}) and the support bound I(πn)≤aˉ Ia(πn)I(\pi_{n})\le\bar{a}\,I^{a}(\pi_{n}) of Couplings of Finite Noise Cost: the Support Bound, Swap, Displacement Couplings and Lower Semicontinuity of the Noise Cost §support-bound,

Dn(φ):=∫X×X(φ(x)−φ(y))2 πn(dz)≤L2 I(πn)≤L2 aˉ Ia(πn).D_{n}(\varphi):=\int_{X\times X}(\varphi(x)-\varphi(y))^{2}\,\pi_{n}(dz)\le L^{2}\,I(\pi_{n})\le L^{2}\,\bar{a}\,I^{a}(\pi_{n}) .

Step 7 (the potential part on the fields φfk\varphi f_{k}). Let φ∈FCb1(X)\varphi\in\mathcal{F}C^{1}_{b}(X) and k∈Nk\in\mathbb{N}, with BB and LL as in Step 6(a). We show lim⁡Ka(∇aV,φfk,πn)=⟨∇aV,φfk⟩ν\lim\mathcal{K}^{a}(\nabla_{a}V,\varphi f_{k},\pi_{n})=\langle\nabla_{a}V,\varphi f_{k}\rangle_{\nu}, the class of ∇aV\nabla_{a}V being taken in L2(νn;Xa)L^{2}(\nu_{n};X^{a}) (Step 0) in the first slot and in L2(ν;Xa)L^{2}(\nu;X^{a}) (Step 4) in the second. Let g:X→Rg:X\to\mathbb{R}, g(x)=∂kV(x) φ(x)g(x)=\partial_{k}V(x)\,\varphi(x).

(a) A pointwise identity. By The Noise Space is a Real Hilbert Space: Orthonormal Basis, Continuous Embedding, Partial Sums, Closed Balls and Borel Measurability §basis, fk=ak1/2ek∈Xaf_{k}=a_{k}^{1/2}e_{k}\in X^{a}, whose coordinates ⟨fk,ej⟩\langle f_{k},e_{j}\rangle are ak1/2a_{k}^{1/2} for j=kj=k and 00 otherwise. So Basic Properties of an Admissible Cylindrical Potential: Continuity, Growth under Noise Translations, Integrability, the Tangent Inequality and Tangency of the Noise Gradient §continuity gives ⟨∇aV(x),fk⟩a=∑j=1d∂jV(x)⟨fk,ej⟩\langle\nabla_{a}V(x),f_{k}\rangle_{a}=\sum_{j=1}^{d}\partial_{j}V(x)\langle f_{k},e_{j}\rangle, which is ak1/2∂kV(x)a_{k}^{1/2}\partial_{k}V(x) if k≤dk\le d, and 0=ak1/2∂kV(x)0=a_{k}^{1/2}\partial_{k}V(x) if k>dk>d, as then ∂kV=0\partial_{k}V=0 by Admissible Cylindrical Potentials on a Hilbert Space in the Noise Geometry §gradient. By bilinearity of ⟨⋅,⋅⟩a\langle\cdot,\cdot\rangle_{a}, for all x,y∈Xx,y\in X,

⟨∇aV(x),φ(y)fk⟩a=ak1/2 ∂kV(x) φ(y).\langle\nabla_{a}V(x),\varphi(y)f_{k}\rangle_{a}=a_{k}^{1/2}\,\partial_{k}V(x)\,\varphi(y).

(b) Bounds on gg. By Basic Properties of an Admissible Cylindrical Potential: Continuity, Growth under Noise Translations, Integrability, the Tangent Inequality and Tangency of the Noise Gradient §continuity and Step 6(a), ∂kV\partial_{k}V and φ\varphi are continuous, so gg is continuous, hence Borel. If k≤dk\le d, ak∂kV(x)2a_{k}\partial_{k}V(x)^{2} is one of the nonnegative summands of g0(x)g_{0}(x) in Step 4; if k>dk>d it is 00; so g(x)2≤B2∂kV(x)2≤(B2/ak) g0(x)g(x)^{2}\le B^{2}\partial_{k}V(x)^{2}\le(B^{2}/a_{k})\,g_{0}(x), aka_{k} being positive. With (2b), Step 4 and the monotonicity of Linearity and Monotonicity of the Lebesgue Integral §nonnegative,

∫Xg2 dσ≤B2Aakfor σ=ν and for σ=νn, n∈N.\int_{X}g^{2}\,d\sigma\le\frac{B^{2}A}{a_{k}}\qquad\text{for }\sigma=\nu\text{ and for }\sigma=\nu_{n},\ n\in\mathbb{N}.

Since 2∣g∣≤1+g22|g|\le1+g^{2}, the same monotonicity and claim 6(a) of Borel Measurability and Bounded Integration on a Metric Space show that ∫X∣g∣ dσ<∞\int_{X}|g|\,d\sigma<\infty, so gg is integrable with respect to each such σ\sigma.

(c) Convergence of ∫Xg dνn\int_{X}g\,d\nu_{n}. Let ε∈R\varepsilon\in\mathbb{R} be positive. First choose, by the Archimedean property, a positive M′′∈RM''\in\mathbb{R} with B2A/(akM′′)<ε/3B^{2}A/(a_{k}M'')<\varepsilon/3. Let gM′′=max⁡{−M′′,min⁡{g,M′′}}g_{M''}=\max\{-M'',\min\{g,M''\}\}, pointwise with the constant functions ±M′′\pm M'', with the maximum and minimum of Maximum of Two Elements of a Totally Ordered Set and Minimum of Two Elements of a Totally Ordered Set; it is continuous by claim 4 of Continuity of the Absolute Value, Maximum and Minimum of Real-Valued Functions on a Metric Space, applied twice, and ∣gM′′∣≤M′′≤M′′(1+∣x∣2)|g_{M''}|\le M''\le M''(1+|x|^{2}). We claim ∣g(x)−gM′′(x)∣≤g(x)2/M′′|g(x)-g_{M''}(x)|\le g(x)^{2}/M'' for every x∈Xx\in X: if ∣g(x)∣≤M′′|g(x)|\le M'', then gM′′(x)=g(x)g_{M''}(x)=g(x); if g(x)>M′′g(x)>M'', then gM′′(x)=M′′g_{M''}(x)=M'' and 0<g(x)−M′′<g(x)<g(x)2/M′′0<g(x)-M''<g(x)<g(x)^{2}/M'', since g(x)/M′′>1g(x)/M''>1; if g(x)<−M′′g(x)<-M'', then gM′′(x)=−M′′g_{M''}(x)=-M'' and 0<−M′′−g(x)<∣g(x)∣<g(x)2/M′′0<-M''-g(x)<|g(x)|<g(x)^{2}/M''. Hence, by Linearity and Monotonicity of the Lebesgue Integral §integrable (linearity, ∣∫f∣≤∫∣f∣|\int f|\le\int|f| and monotonicity) and (b), for σ=ν\sigma=\nu and σ=νn\sigma=\nu_{n},

∣∫Xg dσ−∫XgM′′ dσ∣≤1M′′∫Xg2 dσ≤B2AakM′′<ε3.\Bigl|\int_{X}g\,d\sigma-\int_{X}g_{M''}\,d\sigma\Bigr|\le\frac{1}{M''}\int_{X}g^{2}\,d\sigma\le\frac{B^{2}A}{a_{k}M''}<\frac{\varepsilon}{3}.

Then, for this M′′M'', choose by Step 1, applied to gM′′g_{M''} with A′=M′′A'=M'', an n0∈Nn_{0}\in\mathbb{N} with ∣∫XgM′′ dνn−∫XgM′′ dν∣<ε/3|\int_{X}g_{M''}\,d\nu_{n}-\int_{X}g_{M''}\,d\nu|<\varepsilon/3 for every n≥n0n\ge n_{0}. For n≥n0n\ge n_{0} the triangle inequality gives ∣∫Xg dνn−∫Xg dν∣<ε|\int_{X}g\,d\nu_{n}-\int_{X}g\,d\nu|<\varepsilon. So lim⁡∫Xg dνn=∫Xg dν\lim\int_{X}g\,d\nu_{n}=\int_{X}g\,d\nu.

(d) The cross pairing. Fix nn, and on (X×X,B(X×X),πn)(X\times X,\mathcal{B}(X\times X),\pi_{n}) consider the maps Γ(z)=∇aV(x)\Gamma(z)=\nabla_{a}V(x) and Θ(z)=(φ(y)−φ(x))fk\Theta(z)=(\varphi(y)-\varphi(x))f_{k} into XaX^{a}. They are measurable: Γ=∇aV∘π1\Gamma=\nabla_{a}V\circ\pi_{1}, with ∇aV\nabla_{a}V measurable into XaX^{a} by Basic Properties of an Admissible Cylindrical Potential: Continuity, Growth under Noise Translations, Integrability, the Tangent Inequality and Tangency of the Noise Gradient §continuity and π1,π2\pi_{1},\pi_{2} Borel by Borel Sets of a Hilbert Space with an Orthonormal Basis: Coordinates, Determination by Finite-Dimensional Projections, and Pairs §product-sigma, so claim 4 of Borel Measurability and Bounded Integration on a Metric Space applies; and Θ=(φfk)∘π2−(φfk)∘π1\Theta=(\varphi f_{k})\circ\pi_{2}-(\varphi f_{k})\circ\pi_{1}, measurable by Step 6(b), the same claim and Measurable Maps into a Hilbert Space with an Orthonormal Basis: Norms, Inner Products and Linear Combinations, Synthesis from Coordinates, Square-Integrability, and Almost-Everywhere Equality §operations. Since (π1)#πn=νn(\pi_{1})_{\#}\pi_{n}=\nu_{n} by Couplings of Two Borel Probability Measures on a Hilbert Space and Their Quadratic Cost §coupling, claim 2 of Image Measures, Measures with Densities, and Change of Variables and (2b) give ∫∣Γ∣a2 dπn=∫X∣∇aV∣a2 dνn≤A\int|\Gamma|_{a}^{2}\,d\pi_{n}=\int_{X}|\nabla_{a}V|_{a}^{2}\,d\nu_{n}\le A, and, by (a) and (b), that claim also shows that z↦⟨∇aV(x),φ(x)fk⟩a=ak1/2g(x)z\mapsto\langle\nabla_{a}V(x),\varphi(x)f_{k}\rangle_{a}=a_{k}^{1/2}g(x) is integrable with respect to πn\pi_{n} with integral ak1/2∫Xg dνna_{k}^{1/2}\int_{X}g\,d\nu_{n}. Moreover ∣Θ(z)∣a2=(φ(y)−φ(x))2|\Theta(z)|_{a}^{2}=(\varphi(y)-\varphi(x))^{2} by Step 6(b), so ∫∣Θ∣a2 dπn=Dn(φ)\int|\Theta|_{a}^{2}\,d\pi_{n}=D_{n}(\varphi). By Measurable Maps into a Hilbert Space with an Orthonormal Basis: Norms, Inner Products and Linear Combinations, Synthesis from Coordinates, Square-Integrability, and Almost-Everywhere Equality §square-integrable, ⟨Γ,Θ⟩a\langle\Gamma,\Theta\rangle_{a} is integrable with respect to πn\pi_{n} and, by Step 6(c),

∣Δn∣≤A1/2Dn(φ)1/2≤A1/2L (aˉ Ia(πn))1/2,Δn:=∫X×X⟨Γ,Θ⟩a dπn.|\Delta_{n}|\le A^{1/2}D_{n}(\varphi)^{1/2}\le A^{1/2}L\,\bigl(\bar{a}\,I^{a}(\pi_{n})\bigr)^{1/2},\qquad\Delta_{n}:=\int_{X\times X}\langle\Gamma,\Theta\rangle_{a}\,d\pi_{n}.

Now ⟨Γ(z),Θ(z)⟩a=⟨∇aV(x),φ(y)fk⟩a−⟨∇aV(x),φ(x)fk⟩a\langle\Gamma(z),\Theta(z)\rangle_{a}=\langle\nabla_{a}V(x),\varphi(y)f_{k}\rangle_{a}-\langle\nabla_{a}V(x),\varphi(x)f_{k}\rangle_{a}, and the first term is integrable with respect to πn\pi_{n} with integral Ka(∇aV,φfk,πn)\mathcal{K}^{a}(\nabla_{a}V,\varphi f_{k},\pi_{n}) by Noise Displacement and Cross Pairings Along Couplings: Bounds, Linearity, Displacement Couplings, Polarisation and a Vanishing Criterion §cross, applied with νn\nu_{n} and ν\nu in place of its ν\nu and μ\mu, ∇aV\nabla_{a}V and φfk\varphi f_{k} being representatives of the classes involved. So by Linearity and Monotonicity of the Lebesgue Integral §integrable,

Ka(∇aV,φfk,πn)=ak1/2∫Xg dνn+Δn.\mathcal{K}^{a}(\nabla_{a}V,\varphi f_{k},\pi_{n})=a_{k}^{1/2}\int_{X}g\,d\nu_{n}+\Delta_{n}.

(e) The limit. lim⁡Δn=0\lim\Delta_{n}=0, because Δn2≤A L2 aˉ Ia(πn)\Delta_{n}^{2}\le A\,L^{2}\,\bar{a}\,I^{a}(\pi_{n}) and lim⁡Ia(πn)=0\lim I^{a}(\pi_{n})=0. With (c), lim⁡Ka(∇aV,φfk,πn)=ak1/2∫Xg dν\lim\mathcal{K}^{a}(\nabla_{a}V,\varphi f_{k},\pi_{n})=a_{k}^{1/2}\int_{X}g\,d\nu. On the other hand, the inner product of The Space of Square-Integrable Maps from a Measure Space into a Hilbert Space with an Orthonormal Basis §operations and (a) with x=yx=y give ⟨∇aV,φfk⟩ν=∫X⟨∇aV(y),φ(y)fk⟩a ν(dy)=ak1/2∫Xg dν\langle\nabla_{a}V,\varphi f_{k}\rangle_{\nu}=\int_{X}\langle\nabla_{a}V(y),\varphi(y)f_{k}\rangle_{a}\,\nu(dy)=a_{k}^{1/2}\int_{X}g\,d\nu. This proves the claim of Step 7.

Step 8 (approximation by finite sums). Let S\mathcal{S} be the set of the elements ξ=∑i=1Nφifi\xi=\sum_{i=1}^{N}\varphi_{i}f_{i} of L2(ν;Xa)L^{2}(\nu;X^{a}) with N∈NN\in\mathbb{N} and φ1,…,φN∈FCb1(X)\varphi_{1},\dots,\varphi_{N}\in\mathcal{F}C^{1}_{b}(X), each φifi\varphi_{i}f_{i} being the class of Step 6(b). We show: for every η∈L2(ν;Xa)\eta\in L^{2}(\nu;X^{a}) and every positive ε∈R\varepsilon\in\mathbb{R} there is ξ∈S\xi\in\mathcal{S} with ∥η−ξ∥ν<ε\lVert\eta-\xi\rVert_{\nu}<\varepsilon. By The Space of Square-Integrable Hilbert-Valued Maps is a Real Hilbert Space: Coordinates and Synthesis §coordinates the series ∑i=1∞∥ηi∥L2(ν)2\sum_{i=1}^{\infty}\lVert\eta_{i}\rVert_{L^{2}(\nu)}^{2} converges with sum ∥η∥ν2\lVert\eta\rVert_{\nu}^{2}; with sM′s_{M'} its partial sums, Series of Real Numbers §convergent gives N∈NN\in\mathbb{N} with ∥η∥ν2−sN<ε2/2\lVert\eta\rVert_{\nu}^{2}-s_{N}<\varepsilon^{2}/2. For i∈[N]i\in[N], the classes of the members of FCb1(X)\mathcal{F}C^{1}_{b}(X) are dense in L2(ν)L^{2}(\nu) by Bounded C^1 Cylindrical Functions: Linear Structure, the Gradient and the Partial Derivatives, Bounds and Integrability, and Density in the Square-Integrable Functions §density, so by the meaning of density and claim 3 of Characterization of the Closure in a Metric Space by Open Balls there is φi∈FCb1(X)\varphi_{i}\in\mathcal{F}C^{1}_{b}(X) with ∥ηi−φi∥L2(ν)2<ε2/(2N)\lVert\eta_{i}-\varphi_{i}\rVert_{L^{2}(\nu)}^{2}<\varepsilon^{2}/(2N). Let ξ=∑i=1Nφifi∈S\xi=\sum_{i=1}^{N}\varphi_{i}f_{i}\in\mathcal{S}. By Step 6(b) and the linearity of coordinates in The Space of Square-Integrable Hilbert-Valued Maps is a Real Hilbert Space: Coordinates and Synthesis §coordinates, (η−ξ)l=ηl−φl(\eta-\xi)_{l}=\eta_{l}-\varphi_{l} for l≤Nl\le N and (η−ξ)l=ηl(\eta-\xi)_{l}=\eta_{l} for l>Nl>N. So for M′≥NM'\ge N the M′M'-th partial sum of the series ∑l∥(η−ξ)l∥L2(ν)2\sum_{l}\lVert(\eta-\xi)_{l}\rVert_{L^{2}(\nu)}^{2} equals ∑l=1N∥ηl−φl∥L2(ν)2+sM′−sN\sum_{l=1}^{N}\lVert\eta_{l}-\varphi_{l}\rVert_{L^{2}(\nu)}^{2}+s_{M'}-s_{N}, and letting M′→∞M'\to\infty, The Space of Square-Integrable Hilbert-Valued Maps is a Real Hilbert Space: Coordinates and Synthesis §coordinates gives

∥η−ξ∥ν2=∑l=1N∥ηl−φl∥L2(ν)2+∥η∥ν2−sN<ε22+ε22=ε2.\lVert\eta-\xi\rVert_{\nu}^{2}=\sum_{l=1}^{N}\lVert\eta_{l}-\varphi_{l}\rVert_{L^{2}(\nu)}^{2}+\lVert\eta\rVert_{\nu}^{2}-s_{N}<\frac{\varepsilon^{2}}{2}+\frac{\varepsilon^{2}}{2}=\varepsilon^{2}.

Step 9 (weak convergence of the potential part). For n∈Nn\in\mathbb{N} the cross pairing Ka(⋅,⋅,πn)\mathcal{K}^{a}(\cdot,\cdot,\pi_{n}) is linear in each slot, on L2(νn;Xa)L^{2}(\nu_{n};X^{a}) and on L2(ν;Xa)L^{2}(\nu;X^{a}) respectively: representatives of sums and real multiples may be taken pointwise by The Space of Square-Integrable Maps from a Measure Space into a Hilbert Space with an Orthonormal Basis §operations, ⟨⋅,⋅⟩a\langle\cdot,\cdot\rangle_{a} is bilinear, all integrands are integrable by Noise Displacement and Cross Pairings Along Couplings: Bounds, Linearity, Displacement Couplings, Polarisation and a Vanishing Criterion §cross, and the integral is linear by Linearity and Monotonicity of the Lebesgue Integral §integrable. Hence for ξ=∑i=1Nφifi∈S\xi=\sum_{i=1}^{N}\varphi_{i}f_{i}\in\mathcal{S}, Step 7, the limit laws and the linearity of ⟨∇aV,⋅⟩ν\langle\nabla_{a}V,\cdot\rangle_{\nu} give lim⁡Ka(∇aV,ξ,πn)=∑i=1N⟨∇aV,φifi⟩ν=⟨∇aV,ξ⟩ν\lim\mathcal{K}^{a}(\nabla_{a}V,\xi,\pi_{n})=\sum_{i=1}^{N}\langle\nabla_{a}V,\varphi_{i}f_{i}\rangle_{\nu}=\langle\nabla_{a}V,\xi\rangle_{\nu}.

Now let η∈L2(ν;Xa)\eta\in L^{2}(\nu;X^{a}) and let ε∈R\varepsilon\in\mathbb{R} be positive. First choose, by Step 8, ξ∈S\xi\in\mathcal{S} with ∥η−ξ∥ν<ε/(3(A1/2+1))\lVert\eta-\xi\rVert_{\nu}<\varepsilon/(3(A^{1/2}+1)); then, for this ξ\xi, choose n1∈Nn_{1}\in\mathbb{N} with ∣Ka(∇aV,ξ,πn)−⟨∇aV,ξ⟩ν∣<ε/3|\mathcal{K}^{a}(\nabla_{a}V,\xi,\pi_{n})-\langle\nabla_{a}V,\xi\rangle_{\nu}|<\varepsilon/3 for every n≥n1n\ge n_{1}. For n≥n1n\ge n_{1}, linearity in the second slot, the choice of n1n_{1} for the middle term, the bound Noise Displacement and Cross Pairings Along Couplings: Bounds, Linearity, Displacement Couplings, Polarisation and a Vanishing Criterion §cross-bound with ∥∇aV∥νn≤A1/2\lVert\nabla_{a}V\rVert_{\nu_{n}}\le A^{1/2} from (2b), and The Cauchy-Schwarz Inequality in a Real Inner Product Space in L2(ν;Xa)L^{2}(\nu;X^{a}) with ∥∇aV∥ν≤A1/2\lVert\nabla_{a}V\rVert_{\nu}\le A^{1/2} from Step 4 give

∣Ka(∇aV,η,πn)−⟨∇aV,η⟩ν∣≤∣Ka(∇aV,η−ξ,πn)∣+∣Ka(∇aV,ξ,πn)−⟨∇aV,ξ⟩ν∣+∣⟨∇aV,ξ−η⟩ν∣≤A1/2 ε3(A1/2+1)+ε3+A1/2 ε3(A1/2+1)<ε.\begin{aligned} \bigl|\mathcal{K}^{a}(\nabla_{a}V,\eta,\pi_{n})-\langle\nabla_{a}V,\eta\rangle_{\nu}\bigr|&\le\bigl|\mathcal{K}^{a}(\nabla_{a}V,\eta-\xi,\pi_{n})\bigr|+\bigl|\mathcal{K}^{a}(\nabla_{a}V,\xi,\pi_{n})-\langle\nabla_{a}V,\xi\rangle_{\nu}\bigr|+\bigl|\langle\nabla_{a}V,\xi-\eta\rangle_{\nu}\bigr|\\ &\le\frac{A^{1/2}\,\varepsilon}{3(A^{1/2}+1)}+\frac{\varepsilon}{3}+\frac{A^{1/2}\,\varepsilon}{3(A^{1/2}+1)}<\varepsilon . \end{aligned}

Hence lim⁡Ka(∇aV,η,πn)=⟨∇aV,η⟩ν\lim\mathcal{K}^{a}(\nabla_{a}V,\eta,\pi_{n})=\langle\nabla_{a}V,\eta\rangle_{\nu} for every η∈L2(ν;Xa)\eta\in L^{2}(\nu;X^{a}).

Step 10 (conclusion). Let η∈L2(ν;Xa)\eta\in L^{2}(\nu;X^{a}). By Step 0, Σ(νn)=βZn+∇aV\Sigma(\nu_{n})=\beta Z_{n}+\nabla_{a}V in L2(νn;Xa)L^{2}(\nu_{n};X^{a}), so by the linearity of Ka(⋅,η,πn)\mathcal{K}^{a}(\cdot,\eta,\pi_{n}) in the first slot (Step 9), Step 3, Step 9, the limit laws, the linearity of the inner product of L2(ν;Xa)L^{2}(\nu;X^{a}) and Step 5,

lim⁡Ka(Σ(νn),η,πn)=lim⁡(Ka(βZn,η,πn)+Ka(∇aV,η,πn))=⟨βZ,η⟩ν+⟨∇aV,η⟩ν=⟨Σ(ν),η⟩ν.\lim\mathcal{K}^{a}(\Sigma(\nu_{n}),\eta,\pi_{n})=\lim\bigl(\mathcal{K}^{a}(\beta Z_{n},\eta,\pi_{n})+\mathcal{K}^{a}(\nabla_{a}V,\eta,\pi_{n})\bigr)=\langle\beta Z,\eta\rangle_{\nu}+\langle\nabla_{a}V,\eta\rangle_{\nu}=\langle\Sigma(\nu),\eta\rangle_{\nu}.

So, by Strong and Weak Convergence of Noise Fields Along Couplings of Vanishing Noise Cost §weak, (Σ(νn))n∈N(\Sigma(\nu_{n}))_{n\in\mathbb{N}} converges weakly to Σ(ν)\Sigma(\nu) along (πn)n∈N(\pi_{n})_{n\in\mathbb{N}}. Together with ν∈DΣ\nu\in\mathcal{D}_{\Sigma} from Step 5, this is the closed-score property of Noise Penalty Pairs with Closed Score Along Noise Couplings §closed.

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