TheoremBase

Take the Brenier optimal map T from the diagonal Gaussian to mu for the Euclidean cost and apply McCann's tangent inequality at the Gaussian, whose score is minus the scaling map. Writing relative entropy as entropy plus half the weighted second moment and expanding the weighted square of T turns this inequality into the weighted Talagrand bound.

Proof

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

Throughout, dd, cc, γc\gamma_{c} and μ\mu are as in the statement. Let ρc\rho_{c} be the diagonal Gaussian density with variances cc, ZcZ_{c} its normalizing constant, ScS_{c} the scaling map and ∣x∣c2=x⋅Sc(x)=∑k=1dxk2/ck|x|_{c}^{2}=x\cdot S_{c}(x)=\sum_{k=1}^{d}x_{k}^{2}/c_{k} the weighted square of x∈Rdx\in\mathbb{R}^{d}; let id\mathrm{id} be the identity map of Rd\mathbb{R}^{d}, and let λd\lambda_{d} be Lebesgue measure on B(Rd)\mathcal{B}(\mathbb{R}^{d}). The entropy Ent\mathrm{Ent}, the set P2Ent(Rd)\mathcal{P}_{2}^{\mathrm{Ent}}(\mathbb{R}^{d}), the score ξν\xi_{\nu}, the tangent spaces TνT_{\nu} and the spaces L2(ν;Rd)L^{2}(\nu;\mathbb{R}^{d}) with inner product ⟨⋅,⋅⟩ν\langle\cdot,\cdot\rangle_{\nu} are those named in Relative Entropy and Relative Score with Respect to a Diagonal Gaussian Measure: Comparison with the Entropy, the Score and the Relative Free Energy of a Quadratic Potential. The proof runs McCann's tangent inequality at the source γc\gamma_{c} along the Brenier map from γc\gamma_{c} to μ\mu for the ordinary Euclidean cost; the weighted cost appears only through the weighted squares in the comparison of relative entropy and entropy, so no rescaling of the variances is needed.

Step 1 (γc\gamma_{c} relative to itself). The constant function 1\mathbf{1} on Rd\mathbb{R}^{d} with value 11 is Borel and nonnegative, and for every B∈B(Rd)B\in\mathcal{B}(\mathbb{R}^{d}) one has ∫Rd1B⋅1 dγc=∫Rd1B dγc=γc(B)\int_{\mathbb{R}^{d}}\mathbf{1}_{B}\cdot1\,d\gamma_{c}=\int_{\mathbb{R}^{d}}\mathbf{1}_{B}\,d\gamma_{c}=\gamma_{c}(B) by The Integral of an Indicator Function is the Measure of the Set; so the constant 11 is a density of γc\gamma_{c} with respect to γc\gamma_{c} in the sense of The Radon-Nikodym Theorem for a Finite Measure and a Sigma-Finite Measure, and Uniqueness of Densities. For the function ϕ\phi of The Function slog⁡ss\log s: Continuity, Young's Inequality and Lower Bounds, with the Elementary Bounds for the Exponential and the Logarithm one has ϕ(1)=1⋅log⁡1=0\phi(1)=1\cdot\log1=0, because 0=1−1−1≤log⁡1≤1−1=00=1-1^{-1}\le\log1\le1-1=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. Hence ϕ∘1\phi\circ\mathbf{1} is the zero function, which is integrable with respect to γc\gamma_{c} with integral 0⋅γc(Rd)=00\cdot\gamma_{c}(\mathbb{R}^{d})=0 by claim 6(a) of Borel Measurability and Bounded Integration on a Metric Space (γc\gamma_{c} being a Borel measure on (Rd,dE)(\mathbb{R}^{d},d_{E}) by Probability Measures on Euclidean Space and Random Vectors: Standing Notation §measures). By Relative Entropy of Probability Measures §relative-entropy, γc\gamma_{c} has finite relative entropy with respect to γc\gamma_{c} and H(γc ∣ γc)=0H(\gamma_{c}\,|\,\gamma_{c})=0.

Step 2 (Second moments, entropies and absolute continuity). By The Entropy Inequality for Nonnegative Functions, and Quadratic Moments Bounded by the Relative Entropy with Respect to a Diagonal Gaussian Measure §second-moment, applied to μ\mu and, by Step 1, to γc\gamma_{c}, both μ\mu and γc\gamma_{c} belong to P2(Rd)\mathcal{P}_{2}(\mathbb{R}^{d}). By Relative Entropy and Relative Score with Respect to a Diagonal Gaussian Measure: Comparison with the Entropy, the Score and the Relative Free Energy of a Quadratic Potential §integrable, applied to each of them, the function x↦∣x∣c2x\mapsto|x|_{c}^{2} is integrable (in particular Borel) with respect to μ\mu and with respect to γc\gamma_{c}. By Relative Entropy and Relative Score with Respect to a Diagonal Gaussian Measure: Comparison with the Entropy, the Score and the Relative Free Energy of a Quadratic Potential §entropy, applied to μ\mu and to γc\gamma_{c}, both have finite entropy, so both belong to P2Ent(Rd)\mathcal{P}_{2}^{\mathrm{Ent}}(\mathbb{R}^{d}), and, using Step 1 for the second identity,

H(μ ∣ γc)=Ent(μ)+12∫Rd∣y∣c2 μ(dy)+Zc,0=Ent(γc)+12∫Rd∣x∣c2 γc(dx)+Zc.(1)H(\mu\,|\,\gamma_{c})=\mathrm{Ent}(\mu)+\tfrac12\int_{\mathbb{R}^{d}}|y|_{c}^{2}\,\mu(dy)+Z_{c},\qquad 0=\mathrm{Ent}(\gamma_{c})+\tfrac12\int_{\mathbb{R}^{d}}|x|_{c}^{2}\,\gamma_{c}(dx)+Z_{c}.\tag{1}

Since γc\gamma_{c} has finite entropy, it is absolutely continuous by Basic Properties of the Entropy on the Wasserstein Space: Comparison with the Gaussian Relative Entropy, Lower Bound, Translation Invariance, Absolute Continuity, Closed Sublevel Sets and Lower Semicontinuity §absolutely-continuous.

Step 3 (The score of γc\gamma_{c}). We apply The Score of a Measure with a Positive Continuously Differentiable Density with m=ρcm=\rho_{c}. By The Diagonal Gaussian Density on Euclidean Space: Regularity, Gradient, Normalization, Second Moments and Exponential Moments of Diagonal Quadratic Forms §regularity, ρc\rho_{c} is smooth and positive on Rd\mathbb{R}^{d}, in particular of class C1C^{1} there (Smooth Map on a Euclidean Open Set, with k=1k=1); γc\gamma_{c} is the measure with density ρc\rho_{c} with respect to λd\lambda_{d} by Diagonal Gaussian Measures on Euclidean Space §measure, and it belongs to P2(Rd)\mathcal{P}_{2}(\mathbb{R}^{d}) by Step 2. By The Diagonal Gaussian Density on Euclidean Space: Regularity, Gradient, Normalization, Second Moments and Exponential Moments of Diagonal Quadratic Forms §gradient, Dρc(x)=−ρc(x) Sc(x)D\rho_{c}(x)=-\rho_{c}(x)\,S_{c}(x), so the map η\eta of The Score of a Measure with a Positive Continuously Differentiable Density is η(x)=ρc(x)−1Dρc(x)=−Sc(x)\eta(x)=\rho_{c}(x)^{-1}D\rho_{c}(x)=-S_{c}(x). Its squared norm ∥Sc∥2\lVert S_{c}\rVert^{2} has γc\gamma_{c}-integral at most cmin⁡−2M2(γc)<∞c_{\min}^{-2}M_{2}(\gamma_{c})<\infty, where cmin⁡c_{\min} is the least variance and M2(γc)M_{2}(\gamma_{c}) the second moment of γc\gamma_{c}, by the bound displayed in the preamble of Finite Fisher Information Relative to a Diagonal Gaussian Measure: the Ornstein-Uhlenbeck Functional, the Relative Score and the Relative Fisher Information, which holds for every member of P2(Rd)\mathcal{P}_{2}(\mathbb{R}^{d}). Moreover Sc∈TγcS_{c}\in T_{\gamma_{c}} by Relative Entropy and Relative Score with Respect to a Diagonal Gaussian Measure: Comparison with the Entropy, the Score and the Relative Free Energy of a Quadratic Potential §tangent, and TγcT_{\gamma_{c}} is a linear subspace of L2(γc;Rd)L^{2}(\gamma_{c};\mathbb{R}^{d}) by Basic Properties of the Tangent Space: Closed Subspace, the Identity Map Belongs to It, Second-Moment Limits, and Representation of Bounded Functionals on Gradients §closed, so η=−Sc∈Tγc\eta=-S_{c}\in T_{\gamma_{c}}. Hence γc\gamma_{c} has finite Fisher information by The Score of a Measure with a Positive Continuously Differentiable Density §projection, and its score is

ξγc=−Sc\xi_{\gamma_{c}}=-S_{c}

by The Score of a Measure with a Positive Continuously Differentiable Density §equality.

Step 4 (An optimal map). By Existence of an Optimal Coupling of Two Probability Measures with Finite Second Moment, read with m=dm=d, there is an optimal coupling π\pi of γc\gamma_{c} and μ\mu, both being in P2(Rd)\mathcal{P}_{2}(\mathbb{R}^{d}) by Step 2. Since γc\gamma_{c} is absolutely continuous (Step 2), Brenier's Theorem: Optimal Couplings out of an Absolutely Continuous Measure are Induced by a Unique Map §map, with γc\gamma_{c} in place of μ\mu and μ\mu in place of ν\nu, gives a Borel map T:Rd→RdT:\mathbb{R}^{d}\to\mathbb{R}^{d} with π=(id,T)#γc\pi=(\mathrm{id},T)_{\#}\gamma_{c} and T#γc=μT_{\#}\gamma_{c}=\mu. Thus TT is an optimal map from γc\gamma_{c} to μ\mu in the sense of Optimal Transport Maps and Uniquely Mapped Pairs of Probability Measures §map. Its coordinate functions are written TkT_{k}, as in the statement.

Step 5 (The tangent inequality). By Steps 2 and 3, γc,μ∈P2Ent(Rd)\gamma_{c},\mu\in\mathcal{P}_{2}^{\mathrm{Ent}}(\mathbb{R}^{d}) and γc\gamma_{c} has finite Fisher information, and by Step 4, TT is an optimal map from γc\gamma_{c} to μ\mu. So McCann's Tangent Inequality: the Entropy Lies Above its Tangent Along Optimal Maps §tangent, with γc\gamma_{c} in place of μ\mu and μ\mu in place of ν\nu, gives Ent(γc)+⟨ξγc,T−id⟩γc≤Ent(μ)\mathrm{Ent}(\gamma_{c})+\langle\xi_{\gamma_{c}},T-\mathrm{id}\rangle_{\gamma_{c}}\le\mathrm{Ent}(\mu). By the preamble of McCann's Tangent Inequality: the Entropy Lies Above its Tangent Along Optimal Maps, the Borel maps TT and id\mathrm{id} are square-integrable random vectors on the probability space (Rd,B(Rd),γc)(\mathbb{R}^{d},\mathcal{B}(\mathbb{R}^{d}),\gamma_{c}), so their pointwise difference T−idT-\mathrm{id} is one too, by The Space of Square-Integrable Random Vectors §space read on that probability space as in Wasserstein Spaces, Random Vectors, Vector Fields and Symmetric Matrices in Every Dimension: Standing Notation §fields; that is, x↦T(x)−xx\mapsto T(x)-x is Borel and ∫Rd∥T(x)−x∥2 γc(dx)<∞\int_{\mathbb{R}^{d}}\lVert T(x)-x\rVert^{2}\,\gamma_{c}(dx)<\infty. By Step 3, ScS_{c} is Borel (preamble of Finite Fisher Information Relative to a Diagonal Gaussian Measure: the Ornstein-Uhlenbeck Functional, the Relative Score and the Relative Fisher Information) and ∫Rd∥Sc∥2 dγc<∞\int_{\mathbb{R}^{d}}\lVert S_{c}\rVert^{2}\,d\gamma_{c}<\infty. Hence the function ff on Rd\mathbb{R}^{d} given by f(x)=Sc(x)⋅(T(x)−x)f(x)=S_{c}(x)\cdot(T(x)-x) is Borel, and ∣f(x)∣≤12(∥Sc(x)∥2+∥T(x)−x∥2)|f(x)|\le\tfrac12\bigl(\lVert S_{c}(x)\rVert^{2}+\lVert T(x)-x\rVert^{2}\bigr) for every x∈Rdx\in\mathbb{R}^{d}, both by Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets §functions. So, by monotonicity, additivity and positive homogeneity of the integral of nonnegative measurable functions (Linearity and Monotonicity of the Lebesgue Integral §nonnegative),

∫Rd∣f∣ dγc≤12∫Rd∥Sc∥2 dγc+12∫Rd∥T(x)−x∥2 γc(dx)<∞,\int_{\mathbb{R}^{d}}|f|\,d\gamma_{c}\le\tfrac12\int_{\mathbb{R}^{d}}\lVert S_{c}\rVert^{2}\,d\gamma_{c}+\tfrac12\int_{\mathbb{R}^{d}}\lVert T(x)-x\rVert^{2}\,\gamma_{c}(dx)<\infty,

and ff is integrable with respect to γc\gamma_{c} by Integrable Function and the Lebesgue Integral. By Step 3, ξγc\xi_{\gamma_{c}} is the class of −Sc-S_{c}, and (−Sc(x))⋅(T(x)−x)=−f(x)(-S_{c}(x))\cdot(T(x)-x)=-f(x) for every x∈Rdx\in\mathbb{R}^{d}; so the formula for the inner product of L2(γc;Rd)L^{2}(\gamma_{c};\mathbb{R}^{d}) in Wasserstein Spaces, Random Vectors, Vector Fields and Symmetric Matrices in Every Dimension: Standing Notation §fields, followed by Linearity and Monotonicity of the Lebesgue Integral §integrable (with ff in place of both ff and gg, a=−1a=-1 and b=0b=0), gives ⟨ξγc,T−id⟩γc=∫Rd(−f) dγc=−∫RdSc(x)⋅(T(x)−x) γc(dx)\langle\xi_{\gamma_{c}},T-\mathrm{id}\rangle_{\gamma_{c}}=\int_{\mathbb{R}^{d}}(-f)\,d\gamma_{c}=-\int_{\mathbb{R}^{d}}S_{c}(x)\cdot(T(x)-x)\,\gamma_{c}(dx). Therefore

Ent(γc)−∫RdSc(x)⋅(T(x)−x) γc(dx)≤Ent(μ).(2)\mathrm{Ent}(\gamma_{c})-\int_{\mathbb{R}^{d}}S_{c}(x)\cdot\bigl(T(x)-x\bigr)\,\gamma_{c}(dx)\le\mathrm{Ent}(\mu).\tag{2}

Step 6 (The weighted square of the map). The function y↦∣y∣c2y\mapsto|y|_{c}^{2} is Borel and integrable with respect to μ\mu (Step 2; μ=T#γc\mu=T_{\#}\gamma_{c} by Step 4). By the change-of-variables formula of Probability Measures on Euclidean Space and Random Vectors: Standing Notation §pushforward, the function x↦∣T(x)∣c2x\mapsto|T(x)|_{c}^{2} is integrable with respect to γc\gamma_{c} and

∫Rd∣T(x)∣c2 γc(dx)=∫Rd∣y∣c2 μ(dy).(3)\int_{\mathbb{R}^{d}}|T(x)|_{c}^{2}\,\gamma_{c}(dx)=\int_{\mathbb{R}^{d}}|y|_{c}^{2}\,\mu(dy).\tag{3}

Step 7 (Conclusion). For every x∈Rdx\in\mathbb{R}^{d} put v=T(x)−xv=T(x)-x. Expanding (xk+vk)2=xk2+2xkvk+vk2(x_{k}+v_{k})^{2}=x_{k}^{2}+2x_{k}v_{k}+v_{k}^{2}, dividing by ckc_{k} and summing over k∈{1,…,d}k\in\{1,\dots,d\} gives

∣T(x)∣c2=∣x∣c2+2 Sc(x)⋅(T(x)−x)+∑k=1d(Tk(x)−xk)2ck.|T(x)|_{c}^{2}=|x|_{c}^{2}+2\,S_{c}(x)\cdot\bigl(T(x)-x\bigr)+\sum_{k=1}^{d}\frac{\bigl(T_{k}(x)-x_{k}\bigr)^{2}}{c_{k}} .

Hence the nonnegative function x↦∑k=1dck−1(Tk(x)−xk)2x\mapsto\sum_{k=1}^{d}c_{k}^{-1}(T_{k}(x)-x_{k})^{2} equals ∣T(x)∣c2−∣x∣c2−2 Sc(x)⋅(T(x)−x)|T(x)|_{c}^{2}-|x|_{c}^{2}-2\,S_{c}(x)\cdot(T(x)-x), a linear combination of three functions that are integrable with respect to γc\gamma_{c} by Steps 6, 2 and 5; so it is Borel and integrable with respect to γc\gamma_{c}, and by Linearity and Monotonicity of the Lebesgue Integral §integrable

12∫Rd∑k=1d(Tk(x)−xk)2ck γc(dx)=12∫Rd∣T(x)∣c2 γc(dx)−12∫Rd∣x∣c2 γc(dx)−∫RdSc(x)⋅(T(x)−x) γc(dx).\tfrac12\int_{\mathbb{R}^{d}}\sum_{k=1}^{d}\frac{\bigl(T_{k}(x)-x_{k}\bigr)^{2}}{c_{k}}\,\gamma_{c}(dx) =\tfrac12\int_{\mathbb{R}^{d}}|T(x)|_{c}^{2}\,\gamma_{c}(dx)-\tfrac12\int_{\mathbb{R}^{d}}|x|_{c}^{2}\,\gamma_{c}(dx)-\int_{\mathbb{R}^{d}}S_{c}(x)\cdot\bigl(T(x)-x\bigr)\,\gamma_{c}(dx).

By (3), the first term on the right is 12∫Rd∣y∣c2 μ(dy)\tfrac12\int_{\mathbb{R}^{d}}|y|_{c}^{2}\,\mu(dy); by the second identity in (1), the second term is Ent(γc)+Zc\mathrm{Ent}(\gamma_{c})+Z_{c}. So the right-hand side equals

12∫Rd∣y∣c2 μ(dy)+Zc+(Ent(γc)−∫RdSc(x)⋅(T(x)−x) γc(dx))≤12∫Rd∣y∣c2 μ(dy)+Zc+Ent(μ)=H(μ ∣ γc),\tfrac12\int_{\mathbb{R}^{d}}|y|_{c}^{2}\,\mu(dy)+Z_{c}+\Bigl(\mathrm{Ent}(\gamma_{c})-\int_{\mathbb{R}^{d}}S_{c}(x)\cdot\bigl(T(x)-x\bigr)\,\gamma_{c}(dx)\Bigr) \le\tfrac12\int_{\mathbb{R}^{d}}|y|_{c}^{2}\,\mu(dy)+Z_{c}+\mathrm{Ent}(\mu)=H(\mu\,|\,\gamma_{c}),

by (2) and then the first identity in (1). Multiplying by 22 gives the inequality of the statement, for the Borel map TT of Step 4, which satisfies T#γc=μT_{\#}\gamma_{c}=\mu.

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