TheoremBase

w = UNU_N - u~_N solves the shifted Galerkin equation, which by the dictionary is the penalty-drift equation of the linear-cost representation theorem (variances c', cost g o iotaN)iota_N). w + sN/gammas_N/gamma is the pointwise solution for cost g o iotaNiota_N + sNs_N; its integral is the unique bounded solution of the dressed lifted OU equation, so equals the lifted solution minus PsiNPsi_N; the profile identity gives the integral formula. Recovery: the recovery clause for w and W2−convergenceW_2-convergence of the translated Gaussians to the Dirac mass for u~_N. Clause 3 adds Galerkin convergence.

Proof

Each result cited below is universally quantified over the data in its own statement. Fix N∈NN\in\mathbb{N}. Probability measures on Rm\mathbb{R}^{m} are written ρ\rho or η\eta; the temperature is ν2\tfrac{\nu}{2} throughout, and a letter aa with a mode as subscript is a renormalised constant, not a temperature. We use The Lifted Ornstein-Uhlenbeck Hamilton-Jacobi Equation with a Linear Running Cost: Its Viscosity Solution Is the Integral of the Pointwise Solution, Which It Determines (the representation theorem) with d=md=m, variances c′c', temperature ν2\tfrac{\nu}{2}, λ0=γ\lambda_{0}=\gamma and θ=1\theta=1; its pair is the Gaussian free-energy pair with variances c′c' and temperature ν2\tfrac{\nu}{2}, whose penalty domain is DN\mathcal{D}_{N} by Gaussian Dressing of the Wick-Square Cost: the Riccati Coefficients, the Dressed Variances, the Quadratic Profile, the Shifted Pair and the Shifted Operator §pairs, that lemma applying by The Galerkin Wick-Square Problem at a Cutoff as a Gaussian-Dressed Problem Relative to the Free-Field Gaussian: the Coupling Condition, the Riccati Coefficients, the Riccati Potential, the Profile and the Running Cost §condition. For a bounded uniformly continuous g~:Rm→R\tilde{g}:\mathbb{R}^{m}\to\mathbb{R} write Fg~F_{\tilde{g}} for its operator with running cost g~\tilde{g}; by The Penalty-Drift Hamilton-Jacobi Equation on an Open Subset of Euclidean Space §operator, with noise intensity 2⋅ν2=ν2\cdot\tfrac{\nu}{2}=\nu,

Fg~(z,r,p,X)=γr+12∥p∥2+DVc′(z)⋅p−ν2tr⁡(X)−g~(z).F_{\tilde{g}}(z,r,p,X)=\gamma r+\tfrac12\lVert p\rVert^{2}+DV_{c'}(z)\cdot p-\tfrac{\nu}{2}\operatorname{tr}(X)-\tilde{g}(z).

Step 1 (the shifted Galerkin solution). Let w=UN−u~Nw=U_{N}-\tilde{u}_{N}. By The Galerkin Solutions of the Wick-Square Problem Converge to the Renormalised Viscosity Solution for Every Bounded Lipschitz Running Cost §galerkin, UNU_{N} is a viscosity subsolution and supersolution of FN\mathcal{F}_{N} on Rm\mathbb{R}^{m} and ww is bounded. By The Riccati Shift of the Galerkin Equations of the Wick-Square Problem: a Penalty-Drift Equation with Bounded Cost, and Well-Posedness at Each Cutoff §solutions (its hypotheses hold as Cg≥0C_{g}\ge0 and ∣g∣≤Cg|g|\le C_{g}), ww is a viscosity subsolution and supersolution of the shifted Galerkin operator FN♯\mathcal{F}^{\sharp}_{N} of The Galerkin Hamilton-Jacobi-Bellman Equations of the Wick-Square Problem in the Coordinates of a Cube of Modes §shifted.

Step 2 (ww is the pointwise solution). By The Galerkin Wick-Square Problem at a Cutoff as a Gaussian-Dressed Problem Relative to the Free-Field Gaussian: the Coupling Condition, the Riccati Coefficients, the Riccati Potential, the Profile and the Running Cost §potential, Vc′(z)=ν4∣z∣c′2=ΦN(z)V_{c'}(z)=\tfrac{\nu}{4}|z|_{c'}^{2}=\Phi_{N}(z) for every zz, so DVc′=DΦNDV_{c'}=D\Phi_{N}, and comparing the display above with the formula of The Galerkin Hamilton-Jacobi-Bellman Equations of the Wick-Square Problem in the Coordinates of a Cube of Modes §shifted (the two versions of the penalty-drift equation item, The Penalty-Drift Hamilton-Jacobi Equation on an Open Subset of Euclidean Space §operator and The Penalty-Drift Hamilton-Jacobi Equation on an Open Subset of Euclidean Space §operator, give the same formula) gives Fg∘ιN=FN♯F_{g\circ\iota_{N}}=\mathcal{F}^{\sharp}_{N}; for both operators viscosity sub- and supersolutions on Rm\mathbb{R}^{m} are those of Viscosity Subsolution and Supersolution of a Second-Order Equation (The Penalty-Drift Hamilton-Jacobi Equation on an Open Subset of Euclidean Space §equation, The Galerkin Hamilton-Jacobi-Bellman Equations of the Wick-Square Problem in the Coordinates of a Cube of Modes §equation). By The Galerkin Wick-Square Problem at a Cutoff as a Gaussian-Dressed Problem Relative to the Free-Field Gaussian: the Coupling Condition, the Riccati Coefficients, the Riccati Potential, the Profile and the Running Cost §cost, g∘ιNg\circ\iota_{N} is bounded by CgC_{g} and uniformly continuous. Hence, by Step 1 and the uniqueness in The Lifted Ornstein-Uhlenbeck Hamilton-Jacobi Equation with a Linear Running Cost: Its Viscosity Solution Is the Integral of the Pointwise Solution, Which It Determines §pointwise, ww is the pointwise solution of the representation theorem for the running cost g∘ιNg\circ\iota_{N}; in particular ww is Borel and integrable with respect to every ρ∈P2(Rm)\rho\in\mathcal{P}_{2}(\mathbb{R}^{m}).

Step 3 (adding a constant). The constant function 11 on Rm\mathbb{R}^{m} is the indicator of Rm\mathbb{R}^{m}, bounded and Borel, hence integrable with respect to every ρ∈P2(Rm)\rho\in\mathcal{P}_{2}(\mathbb{R}^{m}) (Probability Measures on Euclidean Space and Random Vectors: Standing Notation §measures) with integral ρ(Rm)=1\rho(\mathbb{R}^{m})=1 (The Integral of an Indicator Function is the Measure of the Set). Let g~′=g∘ιN+sN\tilde{g}'=g\circ\iota_{N}+s_{N}. It is bounded by Cg+∣sN∣C_{g}+|s_{N}|, and g~′(z)−g~′(z′)=g(ιNz)−g(ιNz′)\tilde{g}'(z)-\tilde{g}'(z')=g(\iota_{N}z)-g(\iota_{N}z'), so by The Galerkin Wick-Square Problem at a Cutoff as a Gaussian-Dressed Problem Relative to the Free-Field Gaussian: the Coupling Condition, the Riccati Coefficients, the Riccati Potential, the Profile and the Running Cost §cost it is Lipschitz with constant ℓg\ell_{g} for the Euclidean distance, hence uniformly continuous by A Lipschitz Map is Uniformly Continuous. By Linearity of the Lebesgue Integral over a Finite Sum of Integrable Functions §linear (with the functions g∘ιNg\circ\iota_{N} and 11), the cost of the representation theorem for g~′\tilde{g}' is ρ↦∫Rmg~′ dρ=GN(ρ)+sN\rho\mapsto\int_{\mathbb{R}^{m}}\tilde{g}'\,d\rho=\mathcal{G}_{N}(\rho)+s_{N}.

Let w′=w+γ−1sNw'=w+\gamma^{-1}s_{N}, a bounded function. For all (z,r,p,X)(z,r,p,X), Fg~′(z,r+γ−1sN,p,X)=Fg∘ιN(z,r,p,X)F_{\tilde{g}'}(z,r+\gamma^{-1}s_{N},p,X)=F_{g\circ\iota_{N}}(z,r,p,X), the terms γ⋅γ−1sN\gamma\cdot\gamma^{-1}s_{N} and −sN-s_{N} cancelling. Since ww is upper and lower semicontinuous (Step 1 and Viscosity Subsolution and Supersolution of a Second-Order Equation), so is w′w', the inequalities of Upper Semicontinuous Function on a Subset of a Metric Space and Lower Semicontinuous Function on a Subset of a Metric Space being unchanged when one constant is added to both sides. If φ\varphi is of class C2C^{2} on Rm\mathbb{R}^{m} and w′−φw'-\varphi has a local maximum at zz, then so has w−φ=(w′−φ)−γ−1sNw-\varphi=(w'-\varphi)-\gamma^{-1}s_{N} (Local Maximum of a Function Relative to a Subset of a Metric Space), so by Steps 1 and 2

Fg~′(z,w′(z),Dφ(z),D2φ(z))=FN♯(z,w(z),Dφ(z),D2φ(z))≤0;F_{\tilde{g}'}\bigl(z,w'(z),D\varphi(z),D^{2}\varphi(z)\bigr)=\mathcal{F}^{\sharp}_{N}\bigl(z,w(z),D\varphi(z),D^{2}\varphi(z)\bigr)\le0 ;

likewise, if w′−φw'-\varphi has a local minimum at zz, then so has w−φ=(w′−φ)−γ−1sNw-\varphi=(w'-\varphi)-\gamma^{-1}s_{N} (Local Minimum of a Function Relative to a Subset of a Metric Space), and Steps 1 and 2 give Fg~′(z,w′(z),Dφ(z),D2φ(z))=FN♯(z,w(z),Dφ(z),D2φ(z))≥0F_{\tilde{g}'}\bigl(z,w'(z),D\varphi(z),D^{2}\varphi(z)\bigr)=\mathcal{F}^{\sharp}_{N}\bigl(z,w(z),D\varphi(z),D^{2}\varphi(z)\bigr)\ge0. Thus w′w' is a bounded viscosity subsolution and supersolution of Fg~′F_{\tilde{g}'}, hence by The Lifted Ornstein-Uhlenbeck Hamilton-Jacobi Equation with a Linear Running Cost: Its Viscosity Solution Is the Integral of the Pointwise Solution, Which It Determines §pointwise the pointwise solution for g~′\tilde{g}'. By Linearity of the Lebesgue Integral over a Finite Sum of Integrable Functions §linear, ∫Rmw′ dρ=∫Rmw dρ+γ−1sN\int_{\mathbb{R}^{m}}w'\,d\rho=\int_{\mathbb{R}^{m}}w\,d\rho+\gamma^{-1}s_{N} for ρ∈P2(Rm)\rho\in\mathcal{P}_{2}(\mathbb{R}^{m}).

Step 4 (clause 1). By The Lifted Ornstein-Uhlenbeck Hamilton-Jacobi Equation with a Linear Running Cost: Its Viscosity Solution Is the Integral of the Pointwise Solution, Which It Determines §representation for g~′\tilde{g}', every bounded viscosity solution on DN\mathcal{D}_{N} of the lifted Ornstein-Uhlenbeck equation with variances c′c', temperature ν2\tfrac{\nu}{2}, discount γ\gamma, control cost 11 and running cost ρ↦GN(ρ)+sN\rho\mapsto\mathcal{G}_{N}(\rho)+s_{N} equals ρ↦∫Rmw′ dρ\rho\mapsto\int_{\mathbb{R}^{m}}w'\,d\rho. By Well-Posedness of the Lifted Hamilton-Jacobi Equation with a Wick-Square Cost Relative to a Diagonal Gaussian Measure, by Gaussian Dressing §representation, applied with the data of the statement (its c′c', Φ0\Phi_{0} and ee being c′c', ΨN\Psi_{N} and sNs_{N}), UN−ΨN\mathcal{U}_{N}-\Psi_{N}, which is bounded, is a viscosity solution of exactly this equation. Hence UN(ρ)−ΨN(ρ)=∫Rmw′ dρ\mathcal{U}_{N}(\rho)-\Psi_{N}(\rho)=\int_{\mathbb{R}^{m}}w'\,d\rho for ρ∈DN\rho\in\mathcal{D}_{N}.

Now UN=u~N+wU_{N}=\tilde{u}_{N}+w, where u~N\tilde{u}_{N} is integrable with respect to every ρ∈P2(Rm)\rho\in\mathcal{P}_{2}(\mathbb{R}^{m}) by The Galerkin Wick-Square Problem at a Cutoff as a Gaussian-Dressed Problem Relative to the Free-Field Gaussian: the Coupling Condition, the Riccati Coefficients, the Riccati Potential, the Profile and the Running Cost §profile and ww by Step 2; so UNU_{N} is integrable by Linearity of the Lebesgue Integral over a Finite Sum of Integrable Functions §integrable. For ρ∈DN⊆P2(Rm)\rho\in\mathcal{D}_{N}\subseteq\mathcal{P}_{2}(\mathbb{R}^{m}) (The Gaussian Free-Energy Pair: Relative Entropy and Relative Score with Respect to a Diagonal Gaussian Measure §pair), by Linearity of the Lebesgue Integral over a Finite Sum of Integrable Functions §linear, the profile clause and Step 3,

∫RmUN dρ=ΨN(ρ)+γ−1sN+∫Rmw dρ=ΨN(ρ)+∫Rmw′ dρ=UN(ρ).\int_{\mathbb{R}^{m}}U_{N}\,d\rho=\Psi_{N}(\rho)+\gamma^{-1}s_{N}+\int_{\mathbb{R}^{m}}w\,d\rho=\Psi_{N}(\rho)+\int_{\mathbb{R}^{m}}w'\,d\rho=\mathcal{U}_{N}(\rho).

Step 5 (clause 2). Fix zz and (εj)(\varepsilon_{j}), and write ηj=ηz,εj∈DN\eta_{j}=\eta_{z,\varepsilon_{j}}\in\mathcal{D}_{N}. By clause 1 and Linearity of the Lebesgue Integral over a Finite Sum of Integrable Functions §linear, UN(ηj)=∫Rmu~N dηj+∫Rmw dηj\mathcal{U}_{N}(\eta_{j})=\int_{\mathbb{R}^{m}}\tilde{u}_{N}\,d\eta_{j}+\int_{\mathbb{R}^{m}}w\,d\eta_{j}. By Step 2 and The Lifted Ornstein-Uhlenbeck Hamilton-Jacobi Equation with a Linear Running Cost: Its Viscosity Solution Is the Integral of the Pointwise Solution, Which It Determines §recovery for the cost g∘ιNg\circ\iota_{N}, ∫Rmw dηj→w(z)\int_{\mathbb{R}^{m}}w\,d\eta_{j}\to w(z). Since UN(z)=u~N(z)+w(z)U_{N}(z)=\tilde{u}_{N}(z)+w(z), it remains to show ∫Rmu~N dηj→u~N(z)\int_{\mathbb{R}^{m}}\tilde{u}_{N}\,d\eta_{j}\to\tilde{u}_{N}(z).

Let T:Rm→RmT:\mathbb{R}^{m}\to\mathbb{R}^{m} be the constant map with value zz, Borel since each preimage is ∅\emptyset or Rm\mathbb{R}^{m}; then T#ηj(B)=ηj(T−1(B))T_{\#}\eta_{j}(B)=\eta_{j}(T^{-1}(B)) is 11 or 00 according as z∈Bz\in B or not, so T#ηj=δzT_{\#}\eta_{j}=\delta_{z} (Probability Measures on Euclidean Space and Random Vectors: Standing Notation §pushforward, The Dirac Measure at a Point of Euclidean Space §dirac), and δz∈P2(Rm)\delta_{z}\in\mathcal{P}_{2}(\mathbb{R}^{m}) by Dirac Measures on Euclidean Space: Probability Measure, Integrals, Push-Forwards and the Coupling of Two Dirac Measures §measure. The identity map id\mathrm{id} of Rm\mathbb{R}^{m} is Borel and id#ηj=ηj\mathrm{id}_{\#}\eta_{j}=\eta_{j}, since id−1(B)=B\mathrm{id}^{-1}(B)=B (Probability Measures on Euclidean Space and Random Vectors: Standing Notation §pushforward), and T#ηj=δzT_{\#}\eta_{j}=\delta_{z}; so Couplings on Euclidean Space: Product Coupling, Swap, Finiteness of the Cost, Push-Forward Couplings, Modifying One Marginal, Quantisation, Gluing over a Finitely Supported Measure, and the Lipschitz Bound §pushforward (with S=idS=\mathrm{id} and TT the constant map) shows that (id,T)#ηj∈Π(ηj,δz)(\mathrm{id},T)_{\#}\eta_{j}\in\Pi(\eta_{j},\delta_{z}) has quadratic cost ∫Rm∥x−z∥2 ηj(dx)\int_{\mathbb{R}^{m}}\lVert x-z\rVert^{2}\,\eta_{j}(dx), the integrand x↦∥x−z∥2x\mapsto\lVert x-z\rVert^{2} being Borel by Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets §functions (applied to the Borel maps id\mathrm{id} and TT). As ηj\eta_{j} is the image of the diagonal Gaussian measure γvj\gamma_{v_{j}} with variance vector vj=(εj,…,εj)v_{j}=(\varepsilon_{j},\dots,\varepsilon_{j}) under y↦z+yy\mapsto z+y, the change of variables of Probability Measures on Euclidean Space and Random Vectors: Standing Notation §pushforward, then Diagonal Gaussian Measures on Euclidean Space §measure with claim 3 of Image Measures, Measures with Densities, and Change of Variables, and The Diagonal Gaussian Density on Euclidean Space: Regularity, Gradient, Normalization, Second Moments and Exponential Moments of Diagonal Quadratic Forms §moments give that this cost is ∫Rm∥y∥2ρvj(y) λm(dy)=∑i=1mεj=mεj\int_{\mathbb{R}^{m}}\lVert y\rVert^{2}\rho_{v_{j}}(y)\,\lambda_{m}(dy)=\sum_{i=1}^{m}\varepsilon_{j}=m\varepsilon_{j}, the last step by claim 3 of Properties of Finite Sums (with λ=εj\lambda=\varepsilon_{j}, the sum of mm ones being mm). So W2(ηj,δz)2≤mεjW_{2}(\eta_{j},\delta_{z})^{2}\le m\varepsilon_{j} by The Quadratic Wasserstein Distance on Euclidean Space §distance; given a positive tt, mεj<t2m\varepsilon_{j}<t^{2} for all large jj, whence W2(ηj,δz)<tW_{2}(\eta_{j},\delta_{z})<t; thus W2(ηj,δz)→0W_{2}(\eta_{j},\delta_{z})\to0.

The function u~N\tilde{u}_{N} is of class C2C^{2} (The Galerkin Problems of the Wick-Square Problem: Standing Notation for Cubes of Modes, Coordinates, the Free Galerkin Quadratic and the Riccati Potential §functions), hence continuous by claim 3 of Euclidean Space is Open in Itself, and CkC^k Maps are Continuous and Borel (Probability Measures on Euclidean Space and Random Vectors: Standing Notation §borel-maps); and since qκN(i)>0q_{\kappa_{N}(i)}>0 (The Riccati Coefficients of the Wick-Square Problem: Existence, the Gaussian Profile and Summable Constants §root) and xi2≤∥x∥2x_{i}^{2}\le\lVert x\rVert^{2} (Elementary Properties of the Euclidean Norm on Rn\mathbb{R}^n §coordinate, squaring nonnegative numbers), each summand of u~N(x)\tilde{u}_{N}(x) satisfies ∣qκN(i)xi2+aκN(i)∣≤qκN(i)∥x∥2+∣aκN(i)∣≤(qκN(i)+∣aκN(i)∣)(1+∥x∥2)|q_{\kappa_{N}(i)}x_{i}^{2}+a_{\kappa_{N}(i)}|\le q_{\kappa_{N}(i)}\lVert x\rVert^{2}+|a_{\kappa_{N}(i)}|\le(q_{\kappa_{N}(i)}+|a_{\kappa_{N}(i)}|)(1+\lVert x\rVert^{2}); by claims 2 and 1 of Comparison and Absolute Value Bounds for Finite Sums of Real Numbers and claim 3 of Properties of Finite Sums, ∣u~N(x)∣≤B(1+∥x∥2)|\tilde{u}_{N}(x)|\le B(1+\lVert x\rVert^{2}) with B=∑i=1m(qκN(i)+∣aκN(i)∣)B=\sum_{i=1}^{m}(q_{\kappa_{N}(i)}+|a_{\kappa_{N}(i)}|). By Convergence in the Wasserstein Distance Implies Weak Convergence and Convergence of Integrals of Continuous Functions of Quadratic Growth §quadratic and Dirac Measures on Euclidean Space: Probability Measure, Integrals, Push-Forwards and the Coupling of Two Dirac Measures §integral, ∫Rmu~N dηj→∫Rmu~N dδz=u~N(z)\int_{\mathbb{R}^{m}}\tilde{u}_{N}\,d\eta_{j}\to\int_{\mathbb{R}^{m}}\tilde{u}_{N}\,d\delta_{z}=\tilde{u}_{N}(z). Adding the two limits by Arithmetic of Limits of Real Sequences §sums, UN(ηj)→UN(z)\mathcal{U}_{N}(\eta_{j})\to U_{N}(z).

Step 6 (clause 3). Let x∈H−1x\in H^{-1} and N∈NN\in\mathbb{N}. Since prNx∈Rm\mathrm{pr}_{N}x\in\mathbb{R}^{m} (The Galerkin Problems of the Wick-Square Problem: Standing Notation for Cubes of Modes, Coordinates, the Free Galerkin Quadratic and the Riccati Potential §coordinates), the first assertion is clause 2 with z=prNxz=\mathrm{pr}_{N}x. With uN(x)=UN(prNx)u_{N}(x)=U_{N}(\mathrm{pr}_{N}x) as in The Galerkin Solutions of the Wick-Square Problem Converge to the Renormalised Viscosity Solution for Every Bounded Lipschitz Running Cost §bounds, The Galerkin Solutions of the Wick-Square Problem Converge to the Renormalised Viscosity Solution for Every Bounded Lipschitz Running Cost §pointwise gives UN(prNx)→u(x)U_{N}(\mathrm{pr}_{N}x)\to u(x) as N→∞N\to\infty.

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