TheoremBase

Clauses 1-2 compare with the Euclidean smoothing (unwrapping an optimal torus coupling and smoothing both marginals with a common Gaussian increment), clause 3 writes the density as a probability average of a periodised Gaussian kernel defined as a Lebesgue integral over the integer-part map and shown C2C^2 by differentiation under the integral, and clauses 4-5 follow from a supporting-line Jensen argument and periodic integration by parts with a mollified approximation of log p.

Proof

Each result cited below is universally quantified over the data in its own statement and is applied to the data named where it is used; The Gaussian Kernels on Euclidean Space: Scaling, Derivatives up to Order Three, the Convolution Identity, Moments and Tails, Gaussian Smoothing of a Probability Measure on Euclidean Space: Regularity, Mass, Duality, Approximation of a Bounded Function with a Modulus of Continuity, and the Pairing Identity and The Convolution of a Bounded Continuous Function with a Probability Measure on Euclidean Space: Continuity, Boundedness and Differentiation Under the Integral are read with q=dq=d, and The Gaussian Smoothing Weight: Normalization, Derivatives, Exponential Tilting, Moments, and First-Order Remainder with m=dm=d.

Conventions. The number ss with 0<s≤120<s\le\tfrac12 is fixed. Integrals ∫f(y) dy\int f(y)\,dy are over Rd\mathbb{R}^{d} with respect to λd\lambda_{d}. Let cs>0c_{s}>0 be the constant of The Gaussian Kernels on Euclidean Space: Scaling, Derivatives up to Order Three, the Convolution Identity, Moments and Tails, so that gs(z)=csexp⁡(−∥z∥2/(2s))g_{s}(z)=c_{s}\exp(-\lVert z\rVert^{2}/(2s)). As recorded there, gsg_{s} is the Gaussian smoothing weight of claim 1 of The Gaussian Smoothing Weight: Normalization, Derivatives, Exponential Tilting, Moments, and First-Order Remainder with η=s\eta=s; by that claim gsg_{s} is Borel, 0<gs(z)0<g_{s}(z) and gs(−z)=gs(z)g_{s}(-z)=g_{s}(z) for every zz, and ∫gs(z−a) dz=1\int g_{s}(z-a)\,dz=1 for every a∈Rda\in\mathbb{R}^{d}. For κ∈P(Rd)\kappa\in\mathcal{P}(\mathbb{R}^{d}) let gs∗κg_{s}*\kappa be the Gaussian smoothing of κ\kappa at scale ss, nonnegative, Borel and of integral 11 by Gaussian Smoothing of a Probability Measure on Euclidean Space: Regularity, Mass, Duality, Approximation of a Bounded Function with a Modulus of Continuity, and the Pairing Identity §duality, and let κs∈P(Rd)\kappa_{s}\in\mathcal{P}(\mathbb{R}^{d}) be the measure with density gs∗κg_{s}*\kappa with respect to λd\lambda_{d} (claim 3 of Image Measures, Measures with Densities, and Change of Variables), exactly as in The Heat Semigroup on the Probability Measures on the Torus; thus Ssκ=π#κsS_{s}\kappa=\pi_{\#}\kappa_{s} for κ∈P(Td)\kappa\in\mathcal{P}(\mathbb{T}^{d}) by The Heat Semigroup on the Probability Measures on the Torus §heat. Densities are those of The Radon-Nikodym Theorem for a Finite Measure and a Sigma-Finite Measure, and Uniqueness of Densities, as in The Entropy of a Probability Measure on Euclidean Space §entropy, and ϕ\phi is the function of The Function slog⁡ss\log s: Continuity, Young's Inequality and Lower Bounds, with the Elementary Bounds for the Exponential and the Logarithm (ϕ(0)=0\phi(0)=0, ϕ(t)=tlog⁡t\phi(t)=t\log t for t>0t>0) used there.

The result Gaussian Smoothing of a Measure with Finite Second Moment: Positive Density, Finite Entropy, a Tangent Score, Non-Increasing Fisher Information and Exponential Integrability is stated in the setting of Wasserstein Spaces, Random Vectors, Vector Fields and Symmetric Matrices in Every Dimension: Standing Notation, whose dimension is the dd fixed by The Wasserstein Space and Its Lift to Square-Integrable Random Vectors: Standing Notation §data; that dd is an arbitrary natural number with 1≤d1\le d, the result holding for each such choice, and we take it to be the dimension dd of the torus. By Wasserstein Spaces, Random Vectors, Vector Fields and Symmetric Matrices in Every Dimension: Standing Notation §dimensions, the set P2(Rd)\mathcal{P}_{2}(\mathbb{R}^{d}) and the distance W2W_{2} named there are those of The Second Moment of a Probability Measure on Euclidean Space and the Probability Measures with Finite Second Moment §space and The Quadratic Wasserstein Distance on Euclidean Space §distance, which are also those of The Torus Wasserstein Distance: Comparison with the Euclidean Distance, Wrapping, and Integrals of Periodic Functions; and for κ∈P2(Rd)\kappa\in\mathcal{P}_{2}(\mathbb{R}^{d}) in place of its μ\mu, its ρs\rho_{s} and μs\mu_{s} are gs∗κg_{s}*\kappa and κs\kappa_{s}. So Gaussian Smoothing of a Measure with Finite Second Moment: Positive Density, Finite Entropy, a Tangent Score, Non-Increasing Fisher Information and Exponential Integrability §density gives:

κ∈P2(Rd) ⟹ κs∈P2(Rd)  and  W2(κs,κ)2≤d s.(G)\kappa\in\mathcal{P}_{2}(\mathbb{R}^{d})\ \Longrightarrow\ \kappa_{s}\in\mathcal{P}_{2}(\mathbb{R}^{d})\ \text{ and }\ W_{2}(\kappa_{s},\kappa)^{2}\le d\,s. \qquad(\mathrm{G})

Step 0 (Preliminaries).

(a) Measures on the torus. Let κ∈P(Td)\kappa\in\mathcal{P}(\mathbb{T}^{d}). As κ(Q)=1\kappa(Q)=1 (Probability Measures on the Flat Torus, the Torus Cost of a Coupling, the Torus Wasserstein Distance and Optimal Couplings §measures), claim 3 of Basic Properties of a Measure gives κ(Rd∖Q)=0\kappa(\mathbb{R}^{d}\setminus Q)=0, and for Borel AA finite additivity and monotonicity (claims 1 and 2 there), applied to A∩QA\cap Q and A∖Q⊆Rd∖QA\setminus Q\subseteq\mathbb{R}^{d}\setminus Q, give κ(A)=κ(A∩Q)\kappa(A)=\kappa(A\cap Q). The wrapping map π\pi is Borel and π(x)=x\pi(x)=x for x∈Qx\in Q (The Half-Open Unit Cell Tiles Euclidean Space §wrap), so π−1(A)∩Q=A∩Q\pi^{-1}(A)\cap Q=A\cap Q and π#κ(A)=κ(π−1(A)∩Q)=κ(A∩Q)=κ(A)\pi_{\#}\kappa(A)=\kappa(\pi^{-1}(A)\cap Q)=\kappa(A\cap Q)=\kappa(A); that is, π#κ=κ\pi_{\#}\kappa=\kappa. Also κ∈P2(Rd)\kappa\in\mathcal{P}_{2}(\mathbb{R}^{d}) by The Torus Wasserstein Distance: Comparison with the Euclidean Distance, Wrapping, and Integrals of Periodic Functions §inclusion. Finally, for x∈Qx\in Q one has 0≤xi<10\le x_{i}<1, so xi2≤1x_{i}^{2}\le1, for each i∈[d]i\in[d], whence ∥x∥2=∑i=1dxi2≤d\lVert x\rVert^{2}=\sum_{i=1}^{d}x_{i}^{2}\le d (claim 1 of Elementary Properties of the Euclidean Norm on Rn\mathbb{R}^n) and ∥x∥≤d\lVert x\rVert\le\sqrt{d} (claim 2 of Monotonicity of Squaring on the Nonnegative Elements of an Ordered Field).

(b) Iterated integrals. Let ι:Rd×Rd→Rd+d\iota:\mathbb{R}^{d}\times\mathbb{R}^{d}\to\mathbb{R}^{d+d} be the concatenation map of Probability Measures on Euclidean Space and Random Vectors: Standing Notation §pairs. If F^:Rd+d→[0,∞]\hat F:\mathbb{R}^{d+d}\to[0,\infty] is Borel, then (x,y)↦F^(ι(x,y))(x,y)\mapsto\hat F(\iota(x,y)) is measurable for B(Rd)⊗B(Rd)\mathcal{B}(\mathbb{R}^{d})\otimes\mathcal{B}(\mathbb{R}^{d}), since ι\iota is measurable for that σ\sigma-algebra and B(Rd+d)\mathcal{B}(\mathbb{R}^{d+d}) by Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets §product and a composite of measurable maps is measurable; and F^(ι(x,y))\hat F(\iota(x,y)) is obtained by substituting x,yx,y for pr1(z),pr2(z)\mathrm{pr}_{1}(z),\mathrm{pr}_{2}(z) in any formula for F^(z)\hat F(z), by Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets §projections. Lebesgue measure is σ\sigma-finite by Lebesgue Measure on Euclidean Space is Sigma-Finite §sigma-finite, and every member of P(Rd)\mathcal{P}(\mathbb{R}^{d}) is finite, hence σ\sigma-finite. So the Tonelli clause of Tonelli and Fubini Theorems applies to such integrands for any two of these measures: the iterated integrals exist in either order, are equal, and the partial integrals are measurable functions of the remaining variable. Every integrand to which this is applied below has this form, F^\hat F being built from pr1\mathrm{pr}_{1}, pr2\mathrm{pr}_{2}, π\pi, gsg_{s}, continuous functions, Borel densities and indicators of Borel sets by composition, sums and products, and hence Borel by Probability Measures on Euclidean Space and Random Vectors: Standing Notation §borel-maps.

(c) The integer part. For y∈Rdy\in\mathbb{R}^{d} put n(y)=y−π(y)n(y)=y-\pi(y). By The Half-Open Unit Cell Tiles Euclidean Space §wrap, n(y)n(y) is the unique m∈Zdm\in\mathbb{Z}^{d} with y−m∈Qy-m\in Q provided by The Half-Open Unit Cell Tiles Euclidean Space §tiling; nn is Borel, being the composite of the Borel pairing (id,π)(\mathrm{id},\pi) (Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets §pairing) with the continuous map z↦pr1(z)−pr2(z)z\mapsto\mathrm{pr}_{1}(z)-\mathrm{pr}_{2}(z); and n(y+k)=y+k−π(y)=n(y)+kn(y+k)=y+k-\pi(y)=n(y)+k for k∈Zdk\in\mathbb{Z}^{d}, as π(y+k)=π(y)\pi(y+k)=\pi(y) by the same clause. We record three facts.

(c1) For k∈Zdk\in\mathbb{Z}^{d}: n(y)=kn(y)=k if and only if y−k∈Qy-k\in Q. Indeed, if n(y)=kn(y)=k then y−k=π(y)∈Qy-k=\pi(y)\in Q; conversely, if y−k∈Qy-k\in Q then kk is the unique m∈Zdm\in\mathbb{Z}^{d} with y−m∈Qy-m\in Q (The Half-Open Unit Cell Tiles Euclidean Space §tiling), which is n(y)n(y). Hence {y:n(y)=k}=Q+k\{y:n(y)=k\}=Q+k, a Borel set with λd(Q+k)=λd(Q)=1\lambda_{d}(Q+k)=\lambda_{d}(Q)=1 by claim 1 of Translation and Reflection Invariance of Lebesgue Measure on Rn\mathbb{R}^n and The Half-Open Unit Cell Tiles Euclidean Space §cell.

(c2) For z∈Rdz\in\mathbb{R}^{d} and Borel B⊆QB\subseteq Q:

∫1B(z−n(y)) dy=1B(π(z)).\int\mathbf{1}_{B}\bigl(z-n(y)\bigr)\,dy=\mathbf{1}_{B}\bigl(\pi(z)\bigr).

Indeed, n(y)∈Zdn(y)\in\mathbb{Z}^{d}, so by (c1) applied to zz and k=n(y)k=n(y), z−n(y)∈Qz-n(y)\in Q holds exactly when n(y)=n(z)n(y)=n(z), and then z−n(y)=π(z)z-n(y)=\pi(z). As B⊆QB\subseteq Q, the set {y:z−n(y)∈B}\{y:z-n(y)\in B\} is {y:n(y)=n(z)}=Q+n(z)\{y:n(y)=n(z)\}=Q+n(z) if π(z)∈B\pi(z)\in B and is empty otherwise; its indicator is the integrand, whose integral is its λd\lambda_{d}-measure (Measure Spaces and the Lebesgue Integral: Standing Notation §integral), namely 11 or 00 by (c1).

(c3) For z∈Rdz\in\mathbb{R}^{d}: ∫1Q(z+n(y)) dy=1\int\mathbf{1}_{Q}(z+n(y))\,dy=1. Indeed −n(y)∈Zd-n(y)\in\mathbb{Z}^{d}, so by (c1) z+n(y)=z−(−n(y))∈Qz+n(y)=z-(-n(y))\in Q exactly when −n(y)=n(z)-n(y)=n(z), that is, n(y)=−n(z)n(y)=-n(z); the set of such yy is Q−n(z)Q-n(z), of measure 11 by (c1).

(d) Representation of κs\kappa_{s}. Let κ∈P(Rd)\kappa\in\mathcal{P}(\mathbb{R}^{d}) and let h:Rd→[0,∞)h:\mathbb{R}^{d}\to[0,\infty) be Borel. Then x↦∫h(x+z)gs(z) dzx\mapsto\int h(x+z)g_{s}(z)\,dz is Borel and

∫h dκs=∫(∫h(x+z) gs(z) dz)κ(dx).(R)\int h\,d\kappa_{s}=\int\Bigl(\int h(x+z)\,g_{s}(z)\,dz\Bigr)\kappa(dx). \qquad(\mathrm{R})

By claim 3 of Image Measures, Measures with Densities, and Change of Variables and the definition of gs∗κg_{s}*\kappa, ∫h dκs=∫h(y)(∫gs(y−x) κ(dx))dy=∫(∫h(y)gs(y−x) κ(dx))dy\int h\,d\kappa_{s}=\int h(y)\bigl(\int g_{s}(y-x)\,\kappa(dx)\bigr)dy=\int\bigl(\int h(y)g_{s}(y-x)\,\kappa(dx)\bigr)dy, the constant h(y)h(y) being taken inside by claim 1 of Linearity and Monotonicity of the Lebesgue Integral. By (b) with the measures λd\lambda_{d} and κ\kappa this equals ∫(∫h(y)gs(y−x) dy)κ(dx)\int\bigl(\int h(y)g_{s}(y-x)\,dy\bigr)\kappa(dx), and the inner integral equals ∫h(x+z)gs(z) dz\int h(x+z)g_{s}(z)\,dz by claim 2 of Translation and Reflection Invariance of Lebesgue Measure on Rn\mathbb{R}^n with a=xa=x, applied to y↦h(y)gs(y−x)y\mapsto h(y)g_{s}(y-x). Measurability of the partial integral is part of (b).

Step 1 (Clause 1). By Step 0(a), μ∈P2(Rd)\mu\in\mathcal{P}_{2}(\mathbb{R}^{d}) and π#μ=μ\pi_{\#}\mu=\mu; by (G), μs∈P2(Rd)\mu_{s}\in\mathcal{P}_{2}(\mathbb{R}^{d}) and W2(μs,μ)2≤dsW_{2}(\mu_{s},\mu)^{2}\le ds. The final assertion of The Torus Wasserstein Distance: Comparison with the Euclidean Distance, Wrapping, and Integrals of Periodic Functions §wrap gives

WT(Ssμ,μ)=WT(π#μs,π#μ)≤W2(μs,μ),W_{\mathbb{T}}(S_{s}\mu,\mu)=W_{\mathbb{T}}(\pi_{\#}\mu_{s},\pi_{\#}\mu)\le W_{2}(\mu_{s},\mu),

both sides being nonnegative, so WT(Ssμ,μ)2≤W2(μs,μ)2≤dsW_{\mathbb{T}}(S_{s}\mu,\mu)^{2}\le W_{2}(\mu_{s},\mu)^{2}\le ds by claim 2 of Monotonicity of Squaring on the Nonnegative Elements of an Ordered Field.

Step 2 (Clause 2). By The Torus Wasserstein Space is a Sequentially Compact Metric Space in which Optimal Couplings Exist §optimal choose an optimal coupling γ∈Π(μ,ν)\gamma\in\Pi(\mu,\nu), so that IT(γ)=WT(μ,ν)2I_{\mathbb{T}}(\gamma)=W_{\mathbb{T}}(\mu,\nu)^{2} (Probability Measures on the Flat Torus, the Torus Cost of a Coupling, the Torus Wasserstein Distance and Optimal Couplings §optimal).

(2a) Unwrapping the second marginal. Let T:Rd+d→RdT:\mathbb{R}^{d+d}\to\mathbb{R}^{d} be T(w)=pr1(w)+ϖ(pr2(w)−pr1(w))T(w)=\mathrm{pr}_{1}(w)+\varpi(\mathrm{pr}_{2}(w)-\mathrm{pr}_{1}(w)), with the wrapped displacement ϖ\varpi, which is Borel by The Flat Torus Distance: Minimality of the Wrapped Displacement, Periodicity, the Metric on the Unit Cell and the Lipschitz Bound §lipschitz; TT is Borel as a composite of Borel maps with continuous vector operations (Probability Measures on Euclidean Space and Random Vectors: Standing Notation §borel-maps). Put ν~=T#γ∈P(Rd)\tilde\nu=T_{\#}\gamma\in\mathcal{P}(\mathbb{R}^{d}) and γ~=(pr1,T)#γ∈P(Rd+d)\tilde\gamma=(\mathrm{pr}_{1},T)_{\#}\gamma\in\mathcal{P}(\mathbb{R}^{d+d}), the pairing being Borel by Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets §pairing. Since pr1∘(pr1,T)=pr1\mathrm{pr}_{1}\circ(\mathrm{pr}_{1},T)=\mathrm{pr}_{1} and pr2∘(pr1,T)=T\mathrm{pr}_{2}\circ(\mathrm{pr}_{1},T)=T (Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets §projections) and a push-forward of a push-forward is the push-forward by the composite (as (S∘S′)−1(B)=S′−1(S−1(B))(S\circ S')^{-1}(B)=S'^{-1}(S^{-1}(B))), γ~\tilde\gamma has marginals pr1#γ=μ\mathrm{pr}_{1\#}\gamma=\mu and T#γ=ν~T_{\#}\gamma=\tilde\nu, so γ~∈Π(μ,ν~)\tilde\gamma\in\Pi(\mu,\tilde\nu) (Couplings of Two Probability Measures on Euclidean Space and Their Quadratic Cost §coupling). By the change of variables of Probability Measures on Euclidean Space and Random Vectors: Standing Notation §pushforward and The Wrapped Displacement and the Flat Torus Distance §distance,

I(γ~)=∫∥pr1(w)−T(w)∥2 γ(dw)=∫∥ϖ(pr2(w)−pr1(w))∥2 γ(dw)=∫dT(pr1(w),pr2(w))2 γ(dw)=IT(γ)=WT(μ,ν)2,I(\tilde\gamma)=\int\lVert\mathrm{pr}_{1}(w)-T(w)\rVert^{2}\,\gamma(dw)=\int\bigl\lVert\varpi\bigl(\mathrm{pr}_{2}(w)-\mathrm{pr}_{1}(w)\bigr)\bigr\rVert^{2}\,\gamma(dw)=\int d_{\mathbb{T}}\bigl(\mathrm{pr}_{1}(w),\mathrm{pr}_{2}(w)\bigr)^{2}\,\gamma(dw)=I_{\mathbb{T}}(\gamma)=W_{\mathbb{T}}(\mu,\nu)^{2},

using ∥−a∥=∥a∥\lVert-a\rVert=\lVert a\rVert (claim 5 of Elementary Properties of the Euclidean Norm on Rn\mathbb{R}^n) and Probability Measures on the Flat Torus, the Torus Cost of a Coupling, the Torus Wasserstein Distance and Optimal Couplings §cost. As μ∈P2(Rd)\mu\in\mathcal{P}_{2}(\mathbb{R}^{d}) (Step 0(a)) and I(γ~)<∞I(\tilde\gamma)<\infty, the second assertion of 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 §cost-finite gives ν~∈P2(Rd)\tilde\nu\in\mathcal{P}_{2}(\mathbb{R}^{d}). Finally, for every ww, with v=pr2(w)−pr1(w)v=\mathrm{pr}_{2}(w)-\mathrm{pr}_{1}(w),

T(w)−pr2(w)=−(v−ϖ(v))∈Zd,T(w)-\mathrm{pr}_{2}(w)=-\bigl(v-\varpi(v)\bigr)\in\mathbb{Z}^{d},

because v−ϖ(v)∈Zdv-\varpi(v)\in\mathbb{Z}^{d} by The Flat Torus Distance: Minimality of the Wrapped Displacement, Periodicity, the Metric on the Unit Cell and the Lipschitz Bound §range and the negative of an integer vector is an integer vector (Lattice-Periodic Functions and the Periodic Function Classes §lattice).

(2b) Wrapping back: π#ν~s=Ssν\pi_{\#}\tilde\nu_{s}=S_{s}\nu. Let B∈B(Rd)B\in\mathcal{B}(\mathbb{R}^{d}), put φB=1B∘π\varphi_{B}=\mathbf{1}_{B}\circ\pi, a Borel function with values in {0,1}\{0,1\}, and let hB=gs∗φBh_{B}=g_{s}*\varphi_{B} be as in Gaussian Smoothing of a Probability Measure on Euclidean Space: Regularity, Mass, Duality, Approximation of a Bounded Function with a Modulus of Continuity, and the Pairing Identity §smoothing; by Gaussian Smoothing of a Probability Measure on Euclidean Space: Regularity, Mass, Duality, Approximation of a Bounded Function with a Modulus of Continuity, and the Pairing Identity §duality (with M=1M=1) hBh_{B} is Borel with ∣hB∣≤1|h_{B}|\le1. It is Zd\mathbb{Z}^{d}-periodic: for x∈Rdx\in\mathbb{R}^{d} and k∈Zdk\in\mathbb{Z}^{d}, apply claim 2 of Translation and Reflection Invariance of Lebesgue Measure on Rn\mathbb{R}^n with a=ka=k to the nonnegative Borel function f(y)=gs(x+k−y)φB(y)f(y)=g_{s}(x+k-y)\varphi_{B}(y); since φB(y+k)=1B(π(y+k))=φB(y)\varphi_{B}(y+k)=\mathbf{1}_{B}(\pi(y+k))=\varphi_{B}(y) (The Half-Open Unit Cell Tiles Euclidean Space §wrap), f(y+k)=gs(x−y)φB(y)f(y+k)=g_{s}(x-y)\varphi_{B}(y), so

hB(x+k)=∫f(y) dy=∫f(y+k) dy=∫gs(x−y)φB(y) dy=hB(x).h_{B}(x+k)=\int f(y)\,dy=\int f(y+k)\,dy=\int g_{s}(x-y)\varphi_{B}(y)\,dy=h_{B}(x).

For every κ∈P(Rd)\kappa\in\mathcal{P}(\mathbb{R}^{d}), claim 3 of Image Measures, Measures with Densities, and Change of Variables and Gaussian Smoothing of a Probability Measure on Euclidean Space: Regularity, Mass, Duality, Approximation of a Bounded Function with a Modulus of Continuity, and the Pairing Identity §duality give

π#κs(B)=κs(π−1(B))=∫φB (gs∗κ) dλd=∫hB dκ.(W)\pi_{\#}\kappa_{s}(B)=\kappa_{s}\bigl(\pi^{-1}(B)\bigr)=\int\varphi_{B}\,(g_{s}*\kappa)\,d\lambda_{d}=\int h_{B}\,d\kappa. \qquad(\mathrm{W})

By (2a), hB(T(w))=hB(pr2(w))h_{B}(T(w))=h_{B}(\mathrm{pr}_{2}(w)) for every ww, T(w)T(w) and pr2(w)\mathrm{pr}_{2}(w) differing by an integer vector. Hence, using (W) twice and the change of variables of Probability Measures on Euclidean Space and Random Vectors: Standing Notation §pushforward for the bounded Borel function hBh_{B},

π#ν~s(B)=∫hB dν~=∫hB∘T dγ=∫hB∘pr2 dγ=∫hB dν=π#νs(B)=Ssν(B).\pi_{\#}\tilde\nu_{s}(B)=\int h_{B}\,d\tilde\nu=\int h_{B}\circ T\,d\gamma=\int h_{B}\circ\mathrm{pr}_{2}\,d\gamma=\int h_{B}\,d\nu=\pi_{\#}\nu_{s}(B)=S_{s}\nu(B).

As BB was arbitrary, π#ν~s=Ssν\pi_{\#}\tilde\nu_{s}=S_{s}\nu.

(2c) Smoothing with a common Gaussian increment. Let Ns∈P(Rd)N_{s}\in\mathcal{P}(\mathbb{R}^{d}) be the measure with density gsg_{s} with respect to λd\lambda_{d} (claim 3 of Image Measures, Measures with Densities, and Change of Variables; ∫gs dz=1\int g_{s}\,dz=1). Let Γ0=γ~⊠Ns∈P(R(d+d)+d)\Gamma_{0}=\tilde\gamma\boxtimes N_{s}\in\mathcal{P}(\mathbb{R}^{(d+d)+d}) be the product measure of Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets §product, read with q=d+dq=d+d and p=dp=d, with concatenation ι′\iota' and projections P1=pr1d+d,dP_{1}=\mathrm{pr}^{d+d,d}_{1}, P2=pr2d+d,dP_{2}=\mathrm{pr}^{d+d,d}_{2}. For Borel F^:R(d+d)+d→[0,∞]\hat F:\mathbb{R}^{(d+d)+d}\to[0,\infty], that clause, the Tonelli clause of Tonelli and Fubini Theorems and claim 3 of Image Measures, Measures with Densities, and Change of Variables give

∫F^ dΓ0=∫(∫F^(ι′(w,z)) gs(z) dz)γ~(dw).(P)\int\hat F\,d\Gamma_{0}=\int\Bigl(\int\hat F\bigl(\iota'(w,z)\bigr)\,g_{s}(z)\,dz\Bigr)\tilde\gamma(dw). \qquad(\mathrm{P})

Let F:R(d+d)+d→Rd+dF:\mathbb{R}^{(d+d)+d}\to\mathbb{R}^{d+d} send ζ\zeta to ι(pr1(P1ζ)+P2ζ, pr2(P1ζ)+P2ζ)\iota\bigl(\mathrm{pr}_{1}(P_{1}\zeta)+P_{2}\zeta,\ \mathrm{pr}_{2}(P_{1}\zeta)+P_{2}\zeta\bigr), a Borel map by Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets §pairing, and put Γ=F#Γ0∈P(Rd+d)\Gamma=F_{\#}\Gamma_{0}\in\mathcal{P}(\mathbb{R}^{d+d}). By Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets §projections, pr1(F(ι′(w,z)))=pr1(w)+z\mathrm{pr}_{1}(F(\iota'(w,z)))=\mathrm{pr}_{1}(w)+z and pr2(F(ι′(w,z)))=pr2(w)+z\mathrm{pr}_{2}(F(\iota'(w,z)))=\mathrm{pr}_{2}(w)+z. For A∈B(Rd)A\in\mathcal{B}(\mathbb{R}^{d}), the change of variables, (P), the change of variables for pr1#γ~=μ\mathrm{pr}_{1\#}\tilde\gamma=\mu applied to the Borel function x↦∫1A(x+z)gs(z) dzx\mapsto\int\mathbf{1}_{A}(x+z)g_{s}(z)\,dz of Step 0(d), and (R) with h=1Ah=\mathbf{1}_{A} give

Γ(pr1−1(A))=∫(∫1A(pr1(w)+z)gs(z) dz)γ~(dw)=∫(∫1A(x+z)gs(z) dz)μ(dx)=μs(A),\Gamma\bigl(\mathrm{pr}_{1}^{-1}(A)\bigr)=\int\Bigl(\int\mathbf{1}_{A}\bigl(\mathrm{pr}_{1}(w)+z\bigr)g_{s}(z)\,dz\Bigr)\tilde\gamma(dw)=\int\Bigl(\int\mathbf{1}_{A}(x+z)g_{s}(z)\,dz\Bigr)\mu(dx)=\mu_{s}(A),

and in the same way, with pr2\mathrm{pr}_{2} and pr2#γ~=ν~\mathrm{pr}_{2\#}\tilde\gamma=\tilde\nu, Γ(pr2−1(A))=ν~s(A)\Gamma(\mathrm{pr}_{2}^{-1}(A))=\tilde\nu_{s}(A). So Γ∈Π(μs,ν~s)\Gamma\in\Pi(\mu_{s},\tilde\nu_{s}). Its cost is, by the change of variables and (P),

I(Γ)=∫(∫∥(pr1(w)+z)−(pr2(w)+z)∥2gs(z) dz)γ~(dw)=∫∥pr1(w)−pr2(w)∥2 γ~(dw)=I(γ~),I(\Gamma)=\int\Bigl(\int\bigl\lVert(\mathrm{pr}_{1}(w)+z)-(\mathrm{pr}_{2}(w)+z)\bigr\rVert^{2}g_{s}(z)\,dz\Bigr)\tilde\gamma(dw)=\int\lVert\mathrm{pr}_{1}(w)-\mathrm{pr}_{2}(w)\rVert^{2}\,\tilde\gamma(dw)=I(\tilde\gamma),

the inner integrand being the constant ∥pr1(w)−pr2(w)∥2\lVert\mathrm{pr}_{1}(w)-\mathrm{pr}_{2}(w)\rVert^{2} times gsg_{s}, of integral 11 (claim 1 of Linearity and Monotonicity of the Lebesgue Integral).

(2d) Conclusion. By (G) applied to μ\mu and to ν~\tilde\nu, both in P2(Rd)\mathcal{P}_{2}(\mathbb{R}^{d}), we have μs,ν~s∈P2(Rd)\mu_{s},\tilde\nu_{s}\in\mathcal{P}_{2}(\mathbb{R}^{d}), so The Quadratic Wasserstein Distance on Euclidean Space §distance gives W2(μs,ν~s)2≤I(Γ)=I(γ~)=WT(μ,ν)2W_{2}(\mu_{s},\tilde\nu_{s})^{2}\le I(\Gamma)=I(\tilde\gamma)=W_{\mathbb{T}}(\mu,\nu)^{2}, hence W2(μs,ν~s)≤WT(μ,ν)W_{2}(\mu_{s},\tilde\nu_{s})\le W_{\mathbb{T}}(\mu,\nu) by claim 2 of Monotonicity of Squaring on the Nonnegative Elements of an Ordered Field. By (2b) and the final assertion of The Torus Wasserstein Distance: Comparison with the Euclidean Distance, Wrapping, and Integrals of Periodic Functions §wrap,

WT(Ssμ,Ssν)=WT(π#μs,π#ν~s)≤W2(μs,ν~s)≤WT(μ,ν).W_{\mathbb{T}}(S_{s}\mu,S_{s}\nu)=W_{\mathbb{T}}(\pi_{\#}\mu_{s},\pi_{\#}\tilde\nu_{s})\le W_{2}(\mu_{s},\tilde\nu_{s})\le W_{\mathbb{T}}(\mu,\nu).

Step 3 (A periodised Gaussian kernel). Let h0=gsh_{0}=g_{s} and, for i,j∈[d]i,j\in[d], hi=∂igsh_{i}=\partial_{i}g_{s} and hij=∂j∂igsh_{ij}=\partial_{j}\partial_{i}g_{s}; we call these 1+d+d21+d+d^{2} functions the kernels. By The Gaussian Kernels on Euclidean Space: Scaling, Derivatives up to Order Three, the Convolution Identity, Moments and Tails §derivatives, gsg_{s} is smooth, hence of class C3C^{3} (Smooth Map on a Euclidean Open Set); by clause 2 of C^k Maps on a Euclidean Open Set each hih_{i} is of class C2C^{2} and each hijh_{ij} exists and is of class C1C^{1}, so every kernel is continuous (claim 3 of Euclidean Space is Open in Itself, and CkC^k Maps are Continuous), hence Borel, and ∂ih0=hi\partial_{i}h_{0}=h_{i}, ∂jhi=hij\partial_{j}h_{i}=h_{ij} everywhere. By the same clause of The Gaussian Kernels on Euclidean Space: Scaling, Derivatives up to Order Three, the Convolution Identity, Moments and Tails, hi(u)=−s−1ui gs(u)h_{i}(u)=-s^{-1}u_{i}\,g_{s}(u) and hij(u)=(s−2uiuj−s−1δij) gs(u)h_{ij}(u)=(s^{-2}u_{i}u_{j}-s^{-1}\delta_{ij})\,g_{s}(u).

(3a) A Gaussian bound. Let e(y)=exp⁡(−∥y∥2/2)e(y)=\exp(-\lVert y\rVert^{2}/2); this is the function ψ1\psi_{1} of The Gaussian Smoothing Weight: Normalization, Derivatives, Exponential Tilting, Moments, and First-Order Remainder (η=1\eta=1), so by claim 1 there it is Borel and positive with ∫e dy<∞\int e\,dy<\infty, that is, integrable. Put Ks=s−1+s−2K_{s}=s^{-1}+s^{-2}, so Ks≥1K_{s}\ge1 as s−1≥2s^{-1}\ge2, and for real R≥0R\ge0 put aR=R+da_{R}=R+\sqrt{d} and MR=5Kscsexp⁡(32aR2)M_{R}=5K_{s}c_{s}\exp(\tfrac32a_{R}^{2}). We claim: for every kernel hh, every vv with ∥v∥≤R\lVert v\rVert\le R and every yy,

∣h(v+n(y))∣≤MR e(y).(D)\bigl|h\bigl(v+n(y)\bigr)\bigr|\le M_{R}\,e(y). \qquad(\mathrm{D})

Put u=v+n(y)u=v+n(y). First, ∣h(u)∣≤Ks(1+∥u∥2)gs(u)|h(u)|\le K_{s}(1+\lVert u\rVert^{2})g_{s}(u): for h0h_{0} because Ks≥1K_{s}\ge1; for hih_{i} because ∣ui∣≤∥u∥≤1+∥u∥2|u_{i}|\le\lVert u\rVert\le1+\lVert u\rVert^{2} (claim 4 of Elementary Properties of the Euclidean Norm on Rn\mathbb{R}^n, and 0≤(1−∥u∥)20\le(1-\lVert u\rVert)^{2}) and s−1≤Kss^{-1}\le K_{s}; for hijh_{ij} because ∣s−2uiuj−s−1δij∣≤s−2∥u∥2+s−1≤Ks(1+∥u∥2)|s^{-2}u_{i}u_{j}-s^{-1}\delta_{ij}|\le s^{-2}\lVert u\rVert^{2}+s^{-1}\le K_{s}(1+\lVert u\rVert^{2}). Next let t=∥u∥2/(8s)≥0t=\lVert u\rVert^{2}/(8s)\ge0. By claim 4 of Basic Properties of the Exponential Function, exp⁡(t)≥1+t\exp(t)\ge1+t, so 1≤exp⁡(t)1\le\exp(t) and ∥u∥2=8st≤8sexp⁡(t)\lVert u\rVert^{2}=8st\le8s\exp(t), whence 1+∥u∥2≤(1+8s)exp⁡(t)≤5exp⁡(t)1+\lVert u\rVert^{2}\le(1+8s)\exp(t)\le5\exp(t). By claims 1 and 2 there, gs(u)=csexp⁡(−t)exp⁡(−3t)g_{s}(u)=c_{s}\exp(-t)\exp(-3t) and exp⁡(−t)=exp⁡(t)−1\exp(-t)=\exp(t)^{-1}, so

∣h(u)∣≤5Kscsexp⁡(−3∥u∥28s)≤5Kscsexp⁡(−3∥u∥24),|h(u)|\le5K_{s}c_{s}\exp\Bigl(-\frac{3\lVert u\rVert^{2}}{8s}\Bigr)\le5K_{s}c_{s}\exp\Bigl(-\frac{3\lVert u\rVert^{2}}{4}\Bigr),

the last step because 38s≥34\frac{3}{8s}\ge\frac34 and exp⁡\exp is increasing (claim 4 there). Now y=n(y)+π(y)=u−v+π(y)y=n(y)+\pi(y)=u-v+\pi(y) with ∥π(y)∥≤d\lVert\pi(y)\rVert\le\sqrt{d} (Step 0(a), as π(y)∈Q\pi(y)\in Q), so ∥y∥≤∥u∥+aR\lVert y\rVert\le\lVert u\rVert+a_{R} by the triangle inequality (claim 6 of Elementary Properties of the Euclidean Norm on Rn\mathbb{R}^n). Since 2∥u∥aR≤12∥u∥2+2aR22\lVert u\rVert a_{R}\le\tfrac12\lVert u\rVert^{2}+2a_{R}^{2} (expand 0≤(12∥u∥−2aR)20\le(\tfrac{1}{\sqrt2}\lVert u\rVert-\sqrt2a_{R})^{2}) and squaring is monotone on nonnegative numbers (claim 2 of Monotonicity of Squaring on the Nonnegative Elements of an Ordered Field), ∥y∥2≤(∥u∥+aR)2≤32∥u∥2+3aR2\lVert y\rVert^{2}\le(\lVert u\rVert+a_{R})^{2}\le\tfrac32\lVert u\rVert^{2}+3a_{R}^{2}, that is, 34∥u∥2≥12∥y∥2−32aR2\tfrac34\lVert u\rVert^{2}\ge\tfrac12\lVert y\rVert^{2}-\tfrac32a_{R}^{2}. Using once more that exp⁡\exp is increasing and multiplicative, exp⁡(−34∥u∥2)≤exp⁡(32aR2) e(y)\exp(-\tfrac34\lVert u\rVert^{2})\le\exp(\tfrac32a_{R}^{2})\,e(y), which proves (D).

(3b) Definition, periodicity and continuity. For a kernel hh and v∈Rdv\in\mathbb{R}^{d}, the function y↦h(v+n(y))y\mapsto h(v+n(y)) is Borel (a continuous function of the Borel map y↦v+n(y)y\mapsto v+n(y), Step 0(c)) and dominated by M∥v∥eM_{\lVert v\rVert}e by (D), hence integrable; put

Hh(v)=∫h(v+n(y)) dy∈R,Θ=Hh0,Θi=Hhi,Θij=Hhij.H_{h}(v)=\int h\bigl(v+n(y)\bigr)\,dy\in\mathbb{R},\qquad \Theta=H_{h_{0}},\quad \Theta_{i}=H_{h_{i}},\quad \Theta_{ij}=H_{h_{ij}} .

Periodicity. For k∈Zdk\in\mathbb{Z}^{d}, h(v+k+n(y))=h(v+n(y+k))h(v+k+n(y))=h(v+n(y+k)) by Step 0(c), and claim 3 of Translation and Reflection Invariance of Lebesgue Measure on Rn\mathbb{R}^n with a=ka=k, applied to the integrable function y↦h(v+n(y))y\mapsto h(v+n(y)), gives Hh(v+k)=∫h(v+n(y+k)) dy=Hh(v)H_{h}(v+k)=\int h(v+n(y+k))\,dy=H_{h}(v). Continuity. Let (vj)j∈N(v_{j})_{j\in\mathbb{N}} converge to vv in (Rd,dE)(\mathbb{R}^{d},d_{E}). Choose J∈NJ\in\mathbb{N} with ∥vj−v∥<1\lVert v_{j}-v\rVert<1 for all j≥Jj\ge J (Convergent Sequence in a Metric Space, with dE(vj,v)=∥vj−v∥d_{E}(v_{j},v)=\lVert v_{j}-v\rVert by claim 2 of Elementary Properties of the Euclidean Norm on Rn\mathbb{R}^n), put R=∥v∥+1R=\lVert v\rVert+1 and wj=vJ+jw_{j}=v_{J+j}, so that ∥wj∥≤R\lVert w_{j}\rVert\le R. For each yy, dE(wj+n(y),v+n(y))=∥wj−v∥d_{E}(w_{j}+n(y),v+n(y))=\lVert w_{j}-v\rVert, so wj+n(y)→v+n(y)w_{j}+n(y)\to v+n(y) and h(wj+n(y))→h(v+n(y))h(w_{j}+n(y))\to h(v+n(y)) by claim 1 of Continuity Between Metric Spaces is Equivalent to Sequential Continuity. By (D) the functions y↦h(wj+n(y))y\mapsto h(w_{j}+n(y)) are all dominated by the integrable MReM_{R}e, so Dominated Convergence Theorem gives Hh(wj)→Hh(v)H_{h}(w_{j})\to H_{h}(v); given ε>0\varepsilon>0 and LL with ∣Hh(wj)−Hh(v)∣<ε|H_{h}(w_{j})-H_{h}(v)|<\varepsilon for j≥Lj\ge L, we get ∣Hh(vj)−Hh(v)∣<ε|H_{h}(v_{j})-H_{h}(v)|<\varepsilon for j≥J+Lj\ge J+L. By claim 3 of Continuity Between Metric Spaces is Equivalent to Sequential Continuity, HhH_{h} is continuous on Rd\mathbb{R}^{d}; this is also continuity at every point in the sense of Continuity at a Point for Maps Between Euclidean Spaces, whose conditions ∑i(xi−ai)2<δ2\sum_{i}(x_{i}-a_{i})^{2}<\delta^{2} and (f(x)−f(a))2<ε2(f(x)-f(a))^{2}<\varepsilon^{2} read ∥x−a∥<δ\lVert x-a\rVert<\delta and ∣f(x)−f(a)∣<ε|f(x)-f(a)|<\varepsilon by claim 1 of Elementary Properties of the Euclidean Norm on Rn\mathbb{R}^n and claim 1 of Monotonicity of Squaring on the Nonnegative Elements of an Ordered Field. Thus every HhH_{h} belongs to CperC_{\mathrm{per}}.

(3c) Derivatives. Let hh be a kernel and m∈[d]m\in[d] such that ∂mh\partial_{m}h is again a kernel (namely h=h0h=h_{0}, ∂mh=hm\partial_{m}h=h_{m}, or h=hih=h_{i}, ∂mh=him\partial_{m}h=h_{im}). We show that ∂mHh(v)\partial_{m}H_{h}(v) exists and equals H∂mh(v)H_{\partial_{m}h}(v) for every vv. Fix vv; for real tt let v[t]v[t] be the point with mmth coordinate tt and the other coordinates those of vv, as in Slice Function and the Partial Derivative, and let UU be the open interval with endpoints vm−1v_{m}-1 and vm+1v_{m}+1. For t∈Ut\in U, v[t]−vv[t]-v has the single nonzero coordinate t−vmt-v_{m}, so ∥v[t]∥≤∥v∥+1=:R\lVert v[t]\rVert\le\lVert v\rVert+1=:R (claims 1 and 6 of Elementary Properties of the Euclidean Norm on Rn\mathbb{R}^n). Apply Differentiation under the Integral Sign to (Rd,B(Rd),λd)(\mathbb{R}^{d},\mathcal{B}(\mathbb{R}^{d}),\lambda_{d}) and f(t,y)=h(v[t]+n(y))f(t,y)=h(v[t]+n(y)) on U×RdU\times\mathbb{R}^{d}. Condition (i) holds by (3b). For (ii), fix yy and t0∈Ut_{0}\in U and put b=v[t0]+n(y)b=v[t_{0}]+n(y); for real η≠0\eta\ne0 the point v[t0+η]+n(y)v[t_{0}+\eta]+n(y) is bb with its mmth coordinate bmb_{m} replaced by bm+ηb_{m}+\eta, so (f(t0+η,y)−f(t0,y))/η(f(t_{0}+\eta,y)-f(t_{0},y))/\eta is exactly the difference quotient of Partial Derivative on a Euclidean Open Set for hh at bb in the mmth variable; as hh is of class C1C^{1}, that definition's condition with value ∂mh(b)\partial_{m}h(b) holds, and it is word for word the condition that t↦f(t,y)t\mapsto f(t,y) be differentiable at t0t_{0} with derivative ∂mh(b)\partial_{m}h(b) (Derivative at an Interior Point). For (iii), ∣∂mh(v[t]+n(y))∣≤MRe(y)|\partial_{m}h(v[t]+n(y))|\le M_{R}e(y) for t∈Ut\in U by (D), ∂mh\partial_{m}h being a kernel. The theorem shows that F(t)=Hh(v[t])F(t)=H_{h}(v[t]) is differentiable on UU with F′(t)=H∂mh(v[t])F'(t)=H_{\partial_{m}h}(v[t]). Since the domain is all of Rd\mathbb{R}^{d}, the radius 11 is admissible in claim 1 of Slice Function and the Partial Derivative, FF is the slice function of HhH_{h} at vv in the mmth variable, and claim 2 there gives ∂mHh(v)=F′(vm)=H∂mh(v)\partial_{m}H_{h}(v)=F'(v_{m})=H_{\partial_{m}h}(v).

Consequently: Θ\Theta is continuous with partial derivatives ∂iΘ=Θi\partial_{i}\Theta=\Theta_{i} that exist everywhere and are continuous, so Θ\Theta is of class C1C^{1} (clause 1 of C^k Maps on a Euclidean Open Set); likewise each Θi\Theta_{i} is of class C1C^{1} with ∂jΘi=Θij\partial_{j}\Theta_{i}=\Theta_{ij}; hence Θ\Theta is of class C2C^{2} with ∂j∂iΘ=Θij\partial_{j}\partial_{i}\Theta=\Theta_{ij} (clause 2 there, with k=1k=1). By (3b) and Elementary Properties of Lattice-Periodic Functions §bounded each of the finitely many functions Θ\Theta, Θi\Theta_{i}, Θij\Theta_{ij} lies in CperC_{\mathrm{per}} and is bounded; let CΘ≥0C_{\Theta}\ge0 be a common bound (the largest of the individual bounds).

(3d) Positivity. Let v∈Rdv\in\mathbb{R}^{d}. The integrand y↦gs(v+n(y))y\mapsto g_{s}(v+n(y)) is positive everywhere. If Θ(v)=0\Theta(v)=0, then by The Lebesgue Integral and Null Sets: Almost-Everywhere Comparison, Markov's Inequality, and Dominated Convergence Almost Everywhere §vanishing it vanishes λd\lambda_{d}-almost everywhere, so Rd\mathbb{R}^{d} is λd\lambda_{d}-null, contradicting λd(Q)=1\lambda_{d}(Q)=1 and monotonicity. As Θ(v)≥0\Theta(v)\ge0 by monotonicity of the integral, Θ(v)>0\Theta(v)>0.

(3e) Cell identities. For w∈Rdw\in\mathbb{R}^{d} and Borel B⊆QB\subseteq Q, and for x∈Rdx\in\mathbb{R}^{d},

∫1B(x) Θ(x−w) dx=∫1B(π(z)) gs(z−w) dz,∫1Q(x) Θ(x−w) dx=1,∫1Q(w) Θ(x−w) dw=1.\int\mathbf{1}_{B}(x)\,\Theta(x-w)\,dx=\int\mathbf{1}_{B}\bigl(\pi(z)\bigr)\,g_{s}(z-w)\,dz,\qquad \int\mathbf{1}_{Q}(x)\,\Theta(x-w)\,dx=1,\qquad \int\mathbf{1}_{Q}(w)\,\Theta(x-w)\,dw=1 .

First identity. By Step 0(b) with λd\lambda_{d} twice, the left side is ∫(∫1B(x)gs(x+n(y)−w) dx)dy\int\bigl(\int\mathbf{1}_{B}(x)g_{s}(x+n(y)-w)\,dx\bigr)dy. For fixed yy, claim 2 of Translation and Reflection Invariance of Lebesgue Measure on Rn\mathbb{R}^n with a=n(y)a=n(y), applied to the nonnegative Borel function fy(z)=1B(z−n(y))gs(z−w)f_{y}(z)=\mathbf{1}_{B}(z-n(y))g_{s}(z-w), for which fy(x+n(y))=1B(x)gs(x+n(y)−w)f_{y}(x+n(y))=\mathbf{1}_{B}(x)g_{s}(x+n(y)-w), shows that the inner integral is ∫1B(z−n(y))gs(z−w) dz\int\mathbf{1}_{B}(z-n(y))g_{s}(z-w)\,dz. Exchanging the order again by Step 0(b), taking the factor gs(z−w)g_{s}(z-w) out of the inner integral (claim 1 of Linearity and Monotonicity of the Lebesgue Integral) and using Step 0(c2), the left side equals ∫(∫1B(z−n(y)) dy)gs(z−w) dz=∫1B(π(z))gs(z−w) dz\int\bigl(\int\mathbf{1}_{B}(z-n(y))\,dy\bigr)g_{s}(z-w)\,dz=\int\mathbf{1}_{B}(\pi(z))g_{s}(z-w)\,dz. Second identity. Take B=QB=Q: π(z)∈Q\pi(z)\in Q for every zz (The Half-Open Unit Cell Tiles Euclidean Space §wrap), so the right side is ∫gs(z−w) dz=1\int g_{s}(z-w)\,dz=1 (Conventions). Third identity. By Step 0(b) the left side is ∫(∫1Q(w)gs(x+n(y)−w) dw)dy\int\bigl(\int\mathbf{1}_{Q}(w)g_{s}(x+n(y)-w)\,dw\bigr)dy. For fixed yy put a=x+n(y)a=x+n(y); claim 2 of Translation and Reflection Invariance of Lebesgue Measure on Rn\mathbb{R}^n, applied to f(u)=1Q(a−u)gs(u)f(u)=\mathbf{1}_{Q}(a-u)g_{s}(u), for which f(a−w)=1Q(w)gs(a−w)f(a-w)=\mathbf{1}_{Q}(w)g_{s}(a-w), shows that the inner integral is ∫1Q(x−u+n(y))gs(u) du\int\mathbf{1}_{Q}(x-u+n(y))g_{s}(u)\,du. Exchanging the order by Step 0(b) and using Step 0(c3) with z=x−uz=x-u, the left side is ∫(∫1Q(x−u+n(y)) dy)gs(u) du=∫gs(u) du=1\int\bigl(\int\mathbf{1}_{Q}(x-u+n(y))\,dy\bigr)g_{s}(u)\,du=\int g_{s}(u)\,du=1.

Step 4 (Clause 3). Define p:Rd→Rp:\mathbb{R}^{d}\to\mathbb{R} by

p(x)=∫Θ(x−w) μ(dw),p(x)=\int\Theta(x-w)\,\mu(dw),

which is Θ∗μ\Theta*\mu in the notation of The Convolution of a Bounded Continuous Function with a Probability Measure on Euclidean Space: Continuity, Boundedness and Differentiation Under the Integral §continuous, Θ\Theta being continuous and bounded by CΘC_{\Theta}.

(4a) Regularity. By The Convolution of a Bounded Continuous Function with a Probability Measure on Euclidean Space: Continuity, Boundedness and Differentiation Under the Integral §derivative with G=ΘG=\Theta and C=CΘC=C_{\Theta} (legitimate by (3c)), pp is of class C1C^{1} with ∂ip=Θi∗μ\partial_{i}p=\Theta_{i}*\mu. By the same clause with G=ΘiG=\Theta_{i}, which is of class C1C^{1} with ∣Θi∣≤CΘ|\Theta_{i}|\le C_{\Theta} and ∣∂jΘi∣=∣Θij∣≤CΘ|\partial_{j}\Theta_{i}|=|\Theta_{ij}|\le C_{\Theta}, the function ∂ip\partial_{i}p is of class C1C^{1} with ∂j∂ip=Θij∗μ\partial_{j}\partial_{i}p=\Theta_{ij}*\mu. By clause 2 of C^k Maps on a Euclidean Open Set with k=1k=1, pp is of class C2C^{2} on Rd\mathbb{R}^{d}.

(4b) Periodicity, positivity and a bound. For k∈Zdk\in\mathbb{Z}^{d}, p(x+k)=∫Θ(x−w+k) μ(dw)=p(x)p(x+k)=\int\Theta(x-w+k)\,\mu(dw)=p(x) by the periodicity of Θ\Theta (3b). Also 0≤p(x)≤CΘ0\le p(x)\le C_{\Theta} by monotonicity of the integral. If p(x)=0p(x)=0, then The Lebesgue Integral and Null Sets: Almost-Everywhere Comparison, Markov's Inequality, and Dominated Convergence Almost Everywhere §vanishing, applied in (Rd,B(Rd),μ)(\mathbb{R}^{d},\mathcal{B}(\mathbb{R}^{d}),\mu) to the nonnegative Borel function w↦Θ(x−w)w\mapsto\Theta(x-w), which is positive everywhere by (3d), would make Rd\mathbb{R}^{d} a μ\mu-null set, contradicting μ(Rd)=1\mu(\mathbb{R}^{d})=1. Hence p(x)>0p(x)>0 for every xx, and p∈Cper2p\in C^{2}_{\mathrm{per}}.

(4c) The density. Let B∈B(Rd)B\in\mathcal{B}(\mathbb{R}^{d}) with B⊆QB\subseteq Q. Taking the constant 1B(x)\mathbf{1}_{B}(x) inside the integral defining p(x)p(x) (claim 1 of Linearity and Monotonicity of the Lebesgue Integral), using Step 0(b) with the measures λd\lambda_{d} and μ\mu, and then (3e),

∫1B p dλd=∫(∫1B(x)Θ(x−w) dx)μ(dw)=∫(∫1B(π(z))gs(z−w) dz)μ(dw).\int\mathbf{1}_{B}\,p\,d\lambda_{d}=\int\Bigl(\int\mathbf{1}_{B}(x)\Theta(x-w)\,dx\Bigr)\mu(dw)=\int\Bigl(\int\mathbf{1}_{B}\bigl(\pi(z)\bigr)g_{s}(z-w)\,dz\Bigr)\mu(dw).

With φB=1B∘π\varphi_{B}=\mathbf{1}_{B}\circ\pi as in (2b), the evenness of gsg_{s} gives ∫1B(π(z))gs(z−w) dz=∫gs(w−z)φB(z) dz=(gs∗φB)(w)\int\mathbf{1}_{B}(\pi(z))g_{s}(z-w)\,dz=\int g_{s}(w-z)\varphi_{B}(z)\,dz=(g_{s}*\varphi_{B})(w), so by (W) of (2b), with κ=μ\kappa=\mu,

∫1B p dλd=∫gs∗φB dμ=π#μs(B)=Ssμ(B).\int\mathbf{1}_{B}\,p\,d\lambda_{d}=\int g_{s}*\varphi_{B}\,d\mu=\pi_{\#}\mu_{s}(B)=S_{s}\mu(B).

Now let A∈B(Rd)A\in\mathcal{B}(\mathbb{R}^{d}) be arbitrary. As Ssμ∈P(Td)S_{s}\mu\in\mathcal{P}(\mathbb{T}^{d}) (The Heat Semigroup on the Probability Measures on the Torus §heat), Step 0(a) and the case B=A∩QB=A\cap Q give

Ssμ(A)=Ssμ(A∩Q)=∫1A∩Q p dλd=∫1A (1Qp) dλd.S_{s}\mu(A)=S_{s}\mu(A\cap Q)=\int\mathbf{1}_{A\cap Q}\,p\,d\lambda_{d}=\int\mathbf{1}_{A}\,(\mathbf{1}_{Q}p)\,d\lambda_{d}.

The function 1Qp\mathbf{1}_{Q}p is Borel (a product of Borel functions, pp being continuous) and nonnegative, so it is a density of SsμS_{s}\mu with respect to λd\lambda_{d} (The Radon-Nikodym Theorem for a Finite Measure and a Sigma-Finite Measure, and Uniqueness of Densities). Together with (4a) and (4b) this proves clause 3.

Step 5 (Clause 4).

(5a) The logarithm of the density. The set V=(0,∞)V=(0,\infty) is open in R1\mathbb{R}^{1}, pp takes values in VV by (4b), and log⁡\log is smooth on VV with log⁡′(t)=t−1\log'(t)=t^{-1} (The Natural Logarithm), hence of class C2C^{2} (Smooth Map on a Euclidean Open Set), with ∂1log⁡(t)=t−1\partial_{1}\log(t)=t^{-1} by claim 2 of One-Dimensional Derivatives, Partial Derivatives, and Smoothness on the Real Line. By claim 2 of A Composition of CkC^k Maps Between Euclidean Open Sets is of Class CkC^k, ℓ=log⁡∘p\ell=\log\circ p is of class C2C^{2} on Rd\mathbb{R}^{d}; it is Zd\mathbb{Z}^{d}-periodic because pp is, so ℓ∈Cper2\ell\in C^{2}_{\mathrm{per}}; and by claim 1 there

∂iℓ(x)=p(x)−1 ∂ip(x)(x∈Rd, i∈[d]).(L)\partial_{i}\ell(x)=p(x)^{-1}\,\partial_{i}p(x)\qquad(x\in\mathbb{R}^{d},\ i\in[d]). \qquad(\mathrm{L})

By claim 3 of Constants, Coordinate Functions, Sums and Products of CkC^k Functions on a Euclidean Open Set and Elementary Properties of Lattice-Periodic Functions §algebra, p ℓ∈Cper2p\,\ell\in C^{2}_{\mathrm{per}}; it is continuous (claim 3 of Euclidean Space is Open in Itself, and CkC^k Maps are Continuous), hence bounded by some Mϕ≥0M_{\phi}\ge0 (Elementary Properties of Lattice-Periodic Functions §bounded), and p(x)ℓ(x)=ϕ(p(x))p(x)\ell(x)=\phi(p(x)) for every xx.

(5b) Finite entropy. By clause 3, 1Qp\mathbf{1}_{Q}p is a density of SsμS_{s}\mu. Since ϕ(0)=0\phi(0)=0, ϕ∘(1Qp)=1Q (p ℓ)\phi\circ(\mathbf{1}_{Q}p)=\mathbf{1}_{Q}\,(p\,\ell), a Borel function with ∣ϕ∘(1Qp)∣≤Mϕ1Q|\phi\circ(\mathbf{1}_{Q}p)|\le M_{\phi}\mathbf{1}_{Q}, whose integral is Mϕλd(Q)=Mϕ<∞M_{\phi}\lambda_{d}(Q)=M_{\phi}<\infty (claim 1 of Linearity and Monotonicity of the Lebesgue Integral). So ϕ∘(1Qp)\phi\circ(\mathbf{1}_{Q}p) is integrable, SsμS_{s}\mu has finite entropy by The Entropy of a Probability Measure on Euclidean Space §entropy, and Ent(Ssμ)=∫1Q ϕ∘p dλd\mathrm{Ent}(S_{s}\mu)=\int\mathbf{1}_{Q}\,\phi\circ p\,d\lambda_{d}.

(5c) A supporting line. For real t>0t>0 and r≥0r\ge0,

ϕ(r)≥ϕ(t)+(1+log⁡t)(r−t).(S)\phi(r)\ge\phi(t)+(1+\log t)(r-t). \qquad(\mathrm{S})

If r=0r=0 the difference of the two sides is 0−tlog⁡t+(1+log⁡t)t=t≥00-t\log t+(1+\log t)t=t\ge0. If r>0r>0, then log⁡r=log⁡(r/t)+log⁡t\log r=\log(r/t)+\log t (The Natural Logarithm), and the difference is rlog⁡r−tlog⁡t−(1+log⁡t)(r−t)=rlog⁡(r/t)−r+t≥r(1−t/r)−r+t=0r\log r-t\log t-(1+\log t)(r-t)=r\log(r/t)-r+t\ge r(1-t/r)-r+t=0, by The Function slog⁡ss\log s: Continuity, Young's Inequality and Lower Bounds, with the Elementary Bounds for the Exponential and the Logarithm §log applied to r/tr/t and r>0r>0.

(5d) Monotonicity. Suppose μ\mu has finite entropy and choose, by The Entropy of a Probability Measure on Euclidean Space §entropy, a density ρ\rho of μ\mu with ϕ∘ρ\phi\circ\rho integrable. Put ρQ=1Qρ\rho_{Q}=\mathbf{1}_{Q}\rho. For Borel AA, Step 0(a) gives μ(A)=μ(A∩Q)=∫1AρQ dλd\mu(A)=\mu(A\cap Q)=\int\mathbf{1}_{A}\rho_{Q}\,d\lambda_{d}, so ρQ\rho_{Q} is a density of μ\mu; and ϕ∘ρQ=1Q(ϕ∘ρ)\phi\circ\rho_{Q}=\mathbf{1}_{Q}(\phi\circ\rho) (as ϕ(0)=0\phi(0)=0), Borel by The Function slog⁡ss\log s: Continuity, Young's Inequality and Lower Bounds, with the Elementary Bounds for the Exponential and the Logarithm §continuous with ∣ϕ∘ρQ∣≤∣ϕ∘ρ∣|\phi\circ\rho_{Q}|\le|\phi\circ\rho|, so it is integrable and Ent(μ)=∫ϕ∘ρQ dλd\mathrm{Ent}(\mu)=\int\phi\circ\rho_{Q}\,d\lambda_{d}, the entropy not depending on the density (The Entropy of a Probability Measure on Euclidean Space §entropy).

Fix x∈Rdx\in\mathbb{R}^{d} and put Kx(w)=1Q(w)Θ(x−w)K_{x}(w)=\mathbf{1}_{Q}(w)\Theta(x-w), a Borel function with 0≤Kx≤CΘ1Q0\le K_{x}\le C_{\Theta}\mathbf{1}_{Q} and ∫Kx dw=1\int K_{x}\,dw=1 by (3e). Since w↦Θ(x−w)w\mapsto\Theta(x-w) is bounded and Borel, claim 3 of Image Measures, Measures with Densities, and Change of Variables (integrable case) and 1QρQ=ρQ\mathbf{1}_{Q}\rho_{Q}=\rho_{Q} give

p(x)=∫Θ(x−w)ρQ(w) dw=∫Kx ρQ dw.p(x)=\int\Theta(x-w)\rho_{Q}(w)\,dw=\int K_{x}\,\rho_{Q}\,dw .

Apply (S) with t=p(x)>0t=p(x)>0 and r=ρQ(w)r=\rho_{Q}(w) and multiply by Kx(w)≥0K_{x}(w)\ge0:

Kx(w) ϕ(ρQ(w))≥ϕ(p(x)) Kx(w)+(1+log⁡p(x))(Kx(w)ρQ(w)−p(x)Kx(w))(w∈Rd).K_{x}(w)\,\phi(\rho_{Q}(w))\ge\phi(p(x))\,K_{x}(w)+\bigl(1+\log p(x)\bigr)\bigl(K_{x}(w)\rho_{Q}(w)-p(x)K_{x}(w)\bigr)\qquad(w\in\mathbb{R}^{d}).

All functions of ww here are integrable: Kx≤CΘ1QK_{x}\le C_{\Theta}\mathbf{1}_{Q}, KxρQ≤CΘρQK_{x}\rho_{Q}\le C_{\Theta}\rho_{Q} and ∣Kx ϕ∘ρQ∣≤CΘ∣ϕ∘ρQ∣|K_{x}\,\phi\circ\rho_{Q}|\le C_{\Theta}|\phi\circ\rho_{Q}|. Integrating in ww (claim 2 of Linearity and Monotonicity of the Lebesgue Integral) and using ∫Kx=1\int K_{x}=1 and ∫KxρQ=p(x)\int K_{x}\rho_{Q}=p(x),

∫Kx ϕ∘ρQ dw≥ϕ(p(x)).(J)\int K_{x}\,\phi\circ\rho_{Q}\,dw\ge\phi(p(x)). \qquad(\mathrm{J})

Let Ψ(x,w)=1Q(x)1Q(w)Θ(x−w) ϕ(ρQ(w))\Psi(x,w)=\mathbf{1}_{Q}(x)\mathbf{1}_{Q}(w)\Theta(x-w)\,\phi(\rho_{Q}(w)) and let Ψ+\Psi^{+}, Ψ−\Psi^{-} be its positive and negative parts, Ψ±(x,w)=1Q(x)1Q(w)Θ(x−w) (ϕ∘ρQ)±(w)\Psi^{\pm}(x,w)=\mathbf{1}_{Q}(x)\mathbf{1}_{Q}(w)\Theta(x-w)\,(\phi\circ\rho_{Q})^{\pm}(w), both of the form of Step 0(b). By that step, taking (ϕ∘ρQ)±(w)(\phi\circ\rho_{Q})^{\pm}(w) out of the inner integral and using (3e),

∫(∫Ψ±(x,w) dw)dx=∫(ϕ∘ρQ)±(w) 1Q(w)(∫1Q(x)Θ(x−w) dx)dw=∫(ϕ∘ρQ)± dλd<∞,\int\Bigl(\int\Psi^{\pm}(x,w)\,dw\Bigr)dx=\int(\phi\circ\rho_{Q})^{\pm}(w)\,\mathbf{1}_{Q}(w)\Bigl(\int\mathbf{1}_{Q}(x)\Theta(x-w)\,dx\Bigr)dw=\int(\phi\circ\rho_{Q})^{\pm}\,d\lambda_{d}<\infty,

where 1Q(ϕ∘ρQ)±=(ϕ∘ρQ)±\mathbf{1}_{Q}(\phi\circ\rho_{Q})^{\pm}=(\phi\circ\rho_{Q})^{\pm} because ϕ∘ρQ\phi\circ\rho_{Q} vanishes off QQ. The functions G±(x)=∫Ψ±(x,w) dwG^{\pm}(x)=\int\Psi^{\pm}(x,w)\,dw are measurable by Step 0(b), finite at every xx (each is at most CΘ∫∣ϕ∘ρQ∣ dλdC_{\Theta}\int|\phi\circ\rho_{Q}|\,d\lambda_{d}), and have finite integrals by the display; hence they are integrable, and G+(x)−G−(x)=1Q(x)∫Kx ϕ∘ρQ dwG^{+}(x)-G^{-}(x)=\mathbf{1}_{Q}(x)\int K_{x}\,\phi\circ\rho_{Q}\,dw. By (J), 1Q(x) ϕ(p(x))≤G+(x)−G−(x)\mathbf{1}_{Q}(x)\,\phi(p(x))\le G^{+}(x)-G^{-}(x) for every xx (both sides are 00 off QQ). Monotonicity and linearity of the integral (claim 2 of Linearity and Monotonicity of the Lebesgue Integral), (5b) and the display give

Ent(Ssμ)=∫1Q ϕ∘p dλd≤∫G+ dλd−∫G− dλd=∫(ϕ∘ρQ)+ dλd−∫(ϕ∘ρQ)− dλd=Ent(μ).\mathrm{Ent}(S_{s}\mu)=\int\mathbf{1}_{Q}\,\phi\circ p\,d\lambda_{d}\le\int G^{+}\,d\lambda_{d}-\int G^{-}\,d\lambda_{d}=\int(\phi\circ\rho_{Q})^{+}\,d\lambda_{d}-\int(\phi\circ\rho_{Q})^{-}\,d\lambda_{d}=\mathrm{Ent}(\mu).

Step 6 (Clause 5). Let ℓ=log⁡∘p∈Cper2\ell=\log\circ p\in C^{2}_{\mathrm{per}} be as in (5a), and let r:Rd→Rdr:\mathbb{R}^{d}\to\mathbb{R}^{d} be the map x↦p(x)−1∇p(x)x\mapsto p(x)^{-1}\nabla p(x); by (L), r=∇ℓr=\nabla\ell. Since ℓ\ell is of class C2C^{2}, it is of class C1C^{1} (claim 2 of Euclidean Space is Open in Itself, and CkC^k Maps are Continuous), so ℓ∈Cper1\ell\in C^{1}_{\mathrm{per}} and, by Optimal Transport on the Flat Torus: Standing Notation §calculus, rr is Borel with bounded components in CperC_{\mathrm{per}} and its class belongs to L2(Ssμ;Rd)L^{2}(S_{s}\mu;\mathbb{R}^{d}). Write σ=Ssμ\sigma=S_{s}\mu.

(6a) The integration-by-parts identity. Let f∈Cper∞f\in C^{\infty}_{\mathrm{per}}. For i∈[d]i\in[d], ∂if∈Cper∞\partial_{i}f\in C^{\infty}_{\mathrm{per}} and ∂i∂if∈Cper\partial_{i}\partial_{i}f\in C_{\mathrm{per}} (Elementary Properties of Lattice-Periodic Functions §derivative), and p∈Cper1p\in C^{1}_{\mathrm{per}} (claim 2 of Euclidean Space is Open in Itself, and CkC^k Maps are Continuous); the products (∂i∂if) p(\partial_{i}\partial_{i}f)\,p and (∂if)(∂iℓ) p(\partial_{i}f)(\partial_{i}\ell)\,p lie in CperC_{\mathrm{per}} (Elementary Properties of Lattice-Periodic Functions §algebra). For every u∈Cperu\in C_{\mathrm{per}}, Continuous Periodic Functions are Power-Integrable and Dense on the Torus §integral gives that 1Qu\mathbf{1}_{Q}u is integrable with ∫Tdu∣Q dx=∫1Qu dλd\int_{\mathbb{T}^{d}}u|_{Q}\,dx=\int\mathbf{1}_{Q}u\,d\lambda_{d}, and, if u=vpu=vp with vv bounded Borel, claim 3 of Image Measures, Measures with Densities, and Change of Variables (the density being 1Qp\mathbf{1}_{Q}p by clause 3) gives ∫1Qu dλd=∫v dσ\int\mathbf{1}_{Q}u\,d\lambda_{d}=\int v\,d\sigma. Now Δf=∑i=1d∂i∂if\Delta f=\sum_{i=1}^{d}\partial_{i}\partial_{i}f (The Laplacian of a Twice Continuously Differentiable Function §laplacian) is bounded and Borel (Optimal Transport on the Flat Torus: Standing Notation §calculus). Using linearity of the integral, Vanishing Mean of a Derivative and Integration by Parts on the Torus §parts with g=∂ifg=\partial_{i}f and h=ph=p, and ∂ip=p ∂iℓ\partial_{i}p=p\,\partial_{i}\ell from (L),

∫Δf dσ=∑i=1d∫Td(∂i∂if) p dx=−∑i=1d∫Td(∂if)(∂ip) dx=−∑i=1d∫Td(∂if)(∂iℓ) p dx=−∫∇f⋅r dσ=−⟨r,∇f⟩σ.\int\Delta f\,d\sigma=\sum_{i=1}^{d}\int_{\mathbb{T}^{d}}(\partial_{i}\partial_{i}f)\,p\,dx=-\sum_{i=1}^{d}\int_{\mathbb{T}^{d}}(\partial_{i}f)(\partial_{i}p)\,dx=-\sum_{i=1}^{d}\int_{\mathbb{T}^{d}}(\partial_{i}f)(\partial_{i}\ell)\,p\,dx=-\int\nabla f\cdot r\,d\sigma=-\langle r,\nabla f\rangle_{\sigma}.

(6b) Finite torus Fisher information. By (6a) and the Cauchy--Schwarz inequality in the real Hilbert space L2(σ;Rd)L^{2}(\sigma;\mathbb{R}^{d}) (Optimal Transport on the Flat Torus: Standing Notation §fields, The Cauchy-Schwarz Inequality in a Real Inner Product Space), ∣∫Δf dσ∣≤∥r∥σ∥∇f∥σ|\int\Delta f\,d\sigma|\le\lVert r\rVert_{\sigma}\lVert\nabla f\rVert_{\sigma} for every f∈Cper∞f\in C^{\infty}_{\mathrm{per}}. With the real number C=∥r∥σ≥0C=\lVert r\rVert_{\sigma}\ge0, Finite Torus Fisher Information, the Torus Score and the Torus Fisher Information of a Probability Measure on the Torus §finite gives σ∈PI(Td)\sigma\in\mathcal{P}^{\mathcal{I}}(\mathbb{T}^{d}).

(6c) The class of rr is tangent. By Existence of Mollifier Kernels of Every Radius choose a mollifier kernel ϱ\varrho of radius 11 on Rd\mathbb{R}^{d}, and for ε>0\varepsilon>0 let ϱε\varrho_{\varepsilon} be its rescaling (Rescaling a Mollifier Kernel), a mollifier kernel of radius ε\varepsilon. By Mollifier Kernel of Radius δ\delta on Rn\mathbb{R}^n it is smooth and vanishes outside the ball of radius ε\varepsilon, and ℓ∣Q∈L1(Td)\ell|_{Q}\in\mathcal{L}^{1}(\mathbb{T}^{d}) by Continuous Periodic Functions are Power-Integrable and Dense on the Torus §member; so fε=ϱε⋆(ℓ∣Q)f_{\varepsilon}=\varrho_{\varepsilon}\star(\ell|_{Q}) belongs to Cper∞C^{\infty}_{\mathrm{per}} by Properties of Periodic Convolution on the Torus §smooth. For k∈Nk\in\mathbb{N} let tkt_{k} be the image of kk in R\mathbb{R} (The Canonical Map from the Natural Numbers to a Field) and ηk=tk−1d−1>0\eta_{k}=t_{k}^{-1}d^{-1}>0. By Transfer of a Partial Derivative in Periodic Convolution §uniform-c1, applied to φ=ℓ∈Cper1\varphi=\ell\in C^{1}_{\mathrm{per}} and η=ηk\eta=\eta_{k}, there is ε0>0\varepsilon_{0}>0 with ∣∂ifε(x)−∂iℓ(x)∣≤ηk|\partial_{i}f_{\varepsilon}(x)-\partial_{i}\ell(x)|\le\eta_{k} for all xx, all ii and all 0<ε<ε00<\varepsilon<\varepsilon_{0}; choose such an ε\varepsilon, say ε=ε0/2\varepsilon=\varepsilon_{0}/2, and put Fk=fεF_{k}=f_{\varepsilon}. Then ∥∇Fk(x)−r(x)∥2≤d ηk2=tk−2d−1≤tk−2\lVert\nabla F_{k}(x)-r(x)\rVert^{2}\le d\,\eta_{k}^{2}=t_{k}^{-2}d^{-1}\le t_{k}^{-2} for every xx, so, σ\sigma being a probability measure, ∥∇Fk−r∥σ≤tk−1\lVert\nabla F_{k}-r\rVert_{\sigma}\le t_{k}^{-1} (monotonicity of the integral and claim 2 of Monotonicity of Squaring on the Nonnegative Elements of an Ordered Field). As (tk−1)k∈N(t_{k}^{-1})_{k\in\mathbb{N}} converges to 00 (claim 3 of The Archimedean Property of the Real Numbers), the classes of ∇Fk\nabla F_{k}, which belong to GσG_{\sigma} (The Tangent Space of the Torus Wasserstein Space at a Probability Measure §gradients), converge to the class of rr in L2(σ;Rd)L^{2}(\sigma;\mathbb{R}^{d}) with the distance of its norm. By Sequential Characterization of the Closure in a Metric Space, the class of rr lies in the closure of GσG_{\sigma}, which is TσT_{\sigma} (The Tangent Space of the Torus Wasserstein Space at a Probability Measure §tangent).

(6d) Identification of the score. By (6c) the class of rr belongs to TσT_{\sigma} and by (6a) it satisfies ⟨r,∇f⟩σ=−∫Δf dσ\langle r,\nabla f\rangle_{\sigma}=-\int\Delta f\,d\sigma for every f∈Cper∞f\in C^{\infty}_{\mathrm{per}}. By Finite Torus Fisher Information, the Torus Score and the Torus Fisher Information of a Probability Measure on the Torus §score the score ξσ\xi_{\sigma} is the unique member of TσT_{\sigma} with this property, so ξSsμ\xi_{S_{s}\mu} is the class of x↦p(x)−1∇p(x)x\mapsto p(x)^{-1}\nabla p(x). ■\blacksquare

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