Throughout, each result cited is universally quantified over the data appearing in its own statement and is applied to the data named here. Let ι \iota ι be the canonical map from N \mathbb{N} N to R \mathbb{R} R , positive by claim 3 of Properties of the Canonical Map from the Natural Numbers to an Ordered Field . For a Borel map S : R d → R d S:\mathbb{R}^{d}\to\mathbb{R}^{d} S : R d → R d write
D S ( z ) = ∥ S ( p r 1 ( z ) ) − p r 2 ( z ) ∥ 2 ( z ∈ R d + d ) , D_{S}(z)=\bigl\lVert S(\mathrm{pr}_{1}(z))-\mathrm{pr}_{2}(z)\bigr\rVert^{2}\qquad(z\in\mathbb{R}^{d+d}), D S ( z ) = S ( pr 1 ( z )) − pr 2 ( z ) 2 ( z ∈ R d + d ) ,
Borel and nonnegative by Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets (iv) , in agreement with the notation D T D_{T} D T of the statement. For every π ′ ∈ Π ( μ , ν ) \pi'\in\Pi(\mu,\nu) π ′ ∈ Π ( μ , ν ) the change-of-variables formula , with ( p r 1 ) # π ′ = μ (\mathrm{pr}_{1})_{\#}\pi'=\mu ( pr 1 ) # π ′ = μ and ( p r 2 ) # π ′ = ν (\mathrm{pr}_{2})_{\#}\pi'=\nu ( pr 2 ) # π ′ = ν , gives
∫ R d + d ∥ S ( p r 1 ( z ) ) − T ( p r 1 ( z ) ) ∥ 2 π ′ ( d z ) = ∫ R d ∥ S − T ∥ 2 d μ , ∫ R d + d ∥ p r 2 ( z ) ∥ 2 π ′ ( d z ) = M 2 ( ν ) . ( ∗ ) \int_{\mathbb{R}^{d+d}}\lVert S(\mathrm{pr}_{1}(z))-T(\mathrm{pr}_{1}(z))\rVert^{2}\,\pi'(dz)=\int_{\mathbb{R}^{d}}\lVert S-T\rVert^{2}\,d\mu,\qquad \int_{\mathbb{R}^{d+d}}\lVert\mathrm{pr}_{2}(z)\rVert^{2}\,\pi'(dz)=M_{2}(\nu). \tag{$*$} ∫ R d + d ∥ S ( pr 1 ( z )) − T ( pr 1 ( z )) ∥ 2 π ′ ( d z ) = ∫ R d ∥ S − T ∥ 2 d μ , ∫ R d + d ∥ pr 2 ( z ) ∥ 2 π ′ ( d z ) = M 2 ( ν ) . ( ∗ )
Step 1 (Comparison of two maps). Let S : R d → R d S:\mathbb{R}^{d}\to\mathbb{R}^{d} S : R d → R d be Borel with ∫ ∥ S ∥ 2 d μ < ∞ \int\lVert S\rVert^{2}\,d\mu<\infty ∫ ∥ S ∥ 2 d μ < ∞ and let π ′ ∈ Π ( μ , ν ) \pi'\in\Pi(\mu,\nu) π ′ ∈ Π ( μ , ν ) . Writing a = T ( p r 1 ( z ) ) a=T(\mathrm{pr}_{1}(z)) a = T ( pr 1 ( z )) , b = S ( p r 1 ( z ) ) b=S(\mathrm{pr}_{1}(z)) b = S ( pr 1 ( z )) and c = p r 2 ( z ) c=\mathrm{pr}_{2}(z) c = pr 2 ( z ) , the inequality ∥ x − y ∥ 2 ≤ 2 ∥ x ∥ 2 + 2 ∥ y ∥ 2 \lVert x-y\rVert^{2}\le2\lVert x\rVert^{2}+2\lVert y\rVert^{2} ∥ x − y ∥ 2 ≤ 2 ∥ x ∥ 2 + 2 ∥ y ∥ 2 of Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets (iv) , applied to x = a − b x=a-b x = a − b and y = c − b y=c-b y = c − b , gives D T ( z ) ≤ 2 ∥ a − b ∥ 2 + 2 D S ( z ) D_{T}(z)\le2\lVert a-b\rVert^{2}+2D_{S}(z) D T ( z ) ≤ 2 ∥ a − b ∥ 2 + 2 D S ( z ) pointwise. Integrating against π ′ \pi' π ′ and using claim 1 of Linearity and Monotonicity of the Lebesgue Integral, and the Integrability Criterion and ( ∗ ) (*) ( ∗ ) ,
∫ R d + d D T d π ′ ≤ 2 ∫ R d ∥ T − S ∥ 2 d μ + 2 ∫ R d + d D S d π ′ . ( ∗ ∗ ) \int_{\mathbb{R}^{d+d}}D_{T}\,d\pi'\le2\int_{\mathbb{R}^{d}}\lVert T-S\rVert^{2}\,d\mu+2\int_{\mathbb{R}^{d+d}}D_{S}\,d\pi' . \tag{$**$} ∫ R d + d D T d π ′ ≤ 2 ∫ R d ∥ T − S ∥ 2 d μ + 2 ∫ R d + d D S d π ′ . ( ∗ ∗ )
Step 2 (A uniform tail bound). For j ∈ N j\in\mathbb{N} j ∈ N put R j = ι ( j ) R_{j}=\iota(j) R j = ι ( j ) and h j ( y ) = ∥ y ∥ 2 h_{j}(y)=\lVert y\rVert^{2} h j ( y ) = ∥ y ∥ 2 if R j < ∥ y ∥ 2 R_{j}<\lVert y\rVert^{2} R j < ∥ y ∥ 2 and h j ( y ) = 0 h_{j}(y)=0 h j ( y ) = 0 otherwise; each h j h_{j} h j is Borel by Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets (iv) , satisfies 0 ≤ h j ≤ ∥ ⋅ ∥ 2 0\le h_{j}\le\lVert\cdot\rVert^{2} 0 ≤ h j ≤ ∥ ⋅ ∥ 2 , and converges pointwise to 0 0 0 , since for fixed y y y claim 1 of The Archimedean Property of the Real Numbers gives j j j with ∥ y ∥ 2 < ι ( j ) \lVert y\rVert^{2}<\iota(j) ∥ y ∥ 2 < ι ( j ) and claim 6 of Properties of the Canonical Map from the Natural Numbers to an Ordered Field makes h j ′ ( y ) = 0 h_{j'}(y)=0 h j ′ ( y ) = 0 for every j ′ ≥ j j'\ge j j ′ ≥ j . As ∥ ⋅ ∥ 2 \lVert\cdot\rVert^{2} ∥ ⋅ ∥ 2 is integrable with respect to ν \nu ν , claim 7 of The Lebesgue Integral and Null Sets gives that ( ∫ R d h j d ν ) j ∈ N \bigl(\int_{\mathbb{R}^{d}}h_{j}\,d\nu\bigr)_{j\in\mathbb{N}} ( ∫ R d h j d ν ) j ∈ N converges to 0 0 0 .
Step 3 (The limit of a weakly convergent subsequence is the coupling induced by T T T ). Let ( σ k ) k ∈ N (\sigma_{k})_{k\in\mathbb{N}} ( σ k ) k ∈ N be a sequence in Π ( μ , ν ) \Pi(\mu,\nu) Π ( μ , ν ) with ( I ( σ k ) ) k (I(\sigma_{k}))_{k} ( I ( σ k ) ) k converging to W 2 ( μ , ν ) 2 W_{2}(\mu,\nu)^{2} W 2 ( μ , ν ) 2 . By Tightness from Bounded Second Moments, and Tightness of the Couplings of Two Measures with Finite Second Moment (ii) the set Π ( μ , ν ) \Pi(\mu,\nu) Π ( μ , ν ) is a tight family , so Prokhorov's Theorem on Euclidean Space: a Tight Sequence of Probability Measures Has a Weakly Convergent Subsequence provides a subsequence ( σ k j ) j (\sigma_{k_{j}})_{j} ( σ k j ) j converging weakly to some π ∈ P ( R d + d ) \pi\in\mathcal{P}(\mathbb{R}^{d+d}) π ∈ P ( R d + d ) , and π ∈ Π ( μ , ν ) \pi\in\Pi(\mu,\nu) π ∈ Π ( μ , ν ) by The Couplings of Two Probability Measures on Euclidean Space are Closed under Weak Convergence .
Since ( I ( σ k j ) ) j (I(\sigma_{k_{j}}))_{j} ( I ( σ k j ) ) j converges to W 2 ( μ , ν ) 2 W_{2}(\mu,\nu)^{2} W 2 ( μ , ν ) 2 by A Subsequence of a Convergent Sequence Has the Same Limit , for every positive real η \eta η there is j 0 j_{0} j 0 with I ( σ k j ) ≤ W 2 ( μ , ν ) 2 + η I(\sigma_{k_{j}})\le W_{2}(\mu,\nu)^{2}+\eta I ( σ k j ) ≤ W 2 ( μ , ν ) 2 + η for every j ≥ j 0 j\ge j_{0} j ≥ j 0 , so Continuity of the Coordinate Projections and of the Quadratic Cost Function, and Passage of a Cost Bound to a Weak Limit (iii) , applied with c = W 2 ( μ , ν ) 2 c=W_{2}(\mu,\nu)^{2} c = W 2 ( μ , ν ) 2 , gives I ( π ) ≤ W 2 ( μ , ν ) 2 I(\pi)\le W_{2}(\mu,\nu)^{2} I ( π ) ≤ W 2 ( μ , ν ) 2 ; the reverse inequality holds because W 2 ( μ , ν ) 2 W_{2}(\mu,\nu)^{2} W 2 ( μ , ν ) 2 is the greatest lower bound of the costs of couplings of μ \mu μ and ν \nu ν , by The Quadratic Wasserstein Distance on Euclidean Space (i) . Hence I ( π ) = W 2 ( μ , ν ) 2 I(\pi)=W_{2}(\mu,\nu)^{2} I ( π ) = W 2 ( μ , ν ) 2 and π \pi π is optimal . The coupling ( i d , T ) # μ (\mathrm{id},T)_{\#}\mu ( id , T ) # μ is optimal as well, T T T being an optimal map , so both equal the coupling ( i d , T 0 ) # μ (\mathrm{id},T_{0})_{\#}\mu ( id , T 0 ) # μ induced by the optimal map T 0 T_{0} T 0 witnessing unique mapping ; hence π = ( i d , T ) # μ \pi=(\mathrm{id},T)_{\#}\mu π = ( id , T ) # μ .
Step 4 (The subsequence has vanishing discrepancy). Keep the notation of Step 3 and let η \eta η be a positive real number. The map T T T is Borel with ∫ R d ∥ T ∥ 2 d μ = M 2 ( ν ) < ∞ \int_{\mathbb{R}^{d}}\lVert T\rVert^{2}\,d\mu=M_{2}(\nu)<\infty ∫ R d ∥ T ∥ 2 d μ = M 2 ( ν ) < ∞ by the change-of-variables formula , T # μ = ν T_{\#}\mu=\nu T # μ = ν and ν ∈ P 2 ( R d ) \nu\in\mathcal{P}_{2}(\mathbb{R}^{d}) ν ∈ P 2 ( R d ) , so its class lies in the space L 2 ( μ ; R d ) L^{2}(\mu;\mathbb{R}^{d}) L 2 ( μ ; R d ) of Square-Integrable Vector Fields Against a Probability Measure on Euclidean Space, and Test Functions: Standing Notation (ii) . Put η ′ = min ( η , 1 ) \eta'=\min(\eta,1) η ′ = min ( η , 1 ) , a positive real number. By The Bounded Lipschitz Vector Fields are Dense in the Square-Integrable Vector Fields Against a Probability Measure (i) , applied with slack η ′ \eta' η ′ , there is a bounded Lipschitz S : R d → R d S:\mathbb{R}^{d}\to\mathbb{R}^{d} S : R d → R d , say with ∥ S ∥ ≤ M S \lVert S\rVert\le M_{S} ∥ S ∥ ≤ M S , such that ∥ T − S ∥ μ ≤ η ′ \lVert T-S\rVert_{\mu}\le\eta' ∥ T − S ∥ μ ≤ η ′ ; by the formula for ∥ ⋅ ∥ μ \lVert\cdot\rVert_{\mu} ∥ ⋅ ∥ μ in Square-Integrable Vector Fields Against a Probability Measure on Euclidean Space, and Test Functions: Standing Notation (ii) , and as 0 < η ′ ≤ 1 0<\eta'\le1 0 < η ′ ≤ 1 ,
∫ R d ∥ T − S ∥ 2 d μ = ∥ T − S ∥ μ 2 ≤ η ′ 2 ≤ η ′ ≤ η . \int_{\mathbb{R}^{d}}\lVert T-S\rVert^{2}\,d\mu=\lVert T-S\rVert_{\mu}^{2}\le\eta'^{2}\le\eta'\le\eta . ∫ R d ∥ T − S ∥ 2 d μ = ∥ T − S ∥ μ 2 ≤ η ′ 2 ≤ η ′ ≤ η .
The function D S D_{S} D S is continuous : S S S is continuous by A Lipschitz Map is Uniformly Continuous and Continuous , the projections are continuous by claim 1 of Continuity of the Coordinate Projections and of the Quadratic Cost Function, and Passage of a Cost Bound to a Weak Limit , and D S D_{S} D S is obtained from them by composition and by the continuous map v ↦ ∥ v ∥ 2 v\mapsto\lVert v\rVert^{2} v ↦ ∥ v ∥ 2 , continuous by claim 3 of Euclidean Space Is Open in Itself ; claim 3 of Semicontinuity and Continuity Under Composition with a Continuous Map gives the composition. Moreover
D S ( z ) ≤ 2 M S 2 + 2 ∥ p r 2 ( z ) ∥ 2 D_{S}(z)\le2M_{S}^{2}+2\lVert\mathrm{pr}_{2}(z)\rVert^{2} D S ( z ) ≤ 2 M S 2 + 2 ∥ pr 2 ( z ) ∥ 2
pointwise, by Pairs of Euclidean Points: Coordinate Projections, Pairings, the Product Measure on a Euclidean Space, Borel Norm Functions and Finite Sets (iv) .
By Step 2 choose j 1 ∈ N j_{1}\in\mathbb{N} j 1 ∈ N with ∫ R d h j 1 d ν ≤ η \int_{\mathbb{R}^{d}}h_{j_{1}}\,d\nu\le\eta ∫ R d h j 1 d ν ≤ η and with 2 M S 2 ≤ R j 1 2M_{S}^{2}\le R_{j_{1}} 2 M S 2 ≤ R j 1 ; the order of choice is η \eta η , then S S S and M S M_{S} M S , then j 1 j_{1} j 1 . Put R = R j 1 R=R_{j_{1}} R = R j 1 and K = 4 R K=4R K = 4 R , and let g = min ( D S , K ) g=\min(D_{S},K) g = min ( D S , K ) , which is continuous by claim 4 of Continuity of the Absolute Value, Maximum and Minimum of Real-Valued Functions on a Metric Space and satisfies 0 ≤ g ≤ K 0\le g\le K 0 ≤ g ≤ K , hence is bounded .
Let π ′ ∈ Π ( μ , ν ) \pi'\in\Pi(\mu,\nu) π ′ ∈ Π ( μ , ν ) and let E = { z : K < D S ( z ) } E=\{z:K<D_{S}(z)\} E = { z : K < D S ( z )} , a Borel set. For z ∈ E z\in E z ∈ E one has 4 R < D S ( z ) ≤ 2 M S 2 + 2 ∥ p r 2 ( z ) ∥ 2 ≤ R + 2 ∥ p r 2 ( z ) ∥ 2 4R<D_{S}(z)\le2M_{S}^{2}+2\lVert\mathrm{pr}_{2}(z)\rVert^{2}\le R+2\lVert\mathrm{pr}_{2}(z)\rVert^{2} 4 R < D S ( z ) ≤ 2 M S 2 + 2 ∥ pr 2 ( z ) ∥ 2 ≤ R + 2 ∥ pr 2 ( z ) ∥ 2 , so R < ∥ p r 2 ( z ) ∥ 2 R<\lVert\mathrm{pr}_{2}(z)\rVert^{2} R < ∥ pr 2 ( z ) ∥ 2 and therefore 2 M S 2 ≤ R ≤ ∥ p r 2 ( z ) ∥ 2 2M_{S}^{2}\le R\le\lVert\mathrm{pr}_{2}(z)\rVert^{2} 2 M S 2 ≤ R ≤ ∥ pr 2 ( z ) ∥ 2 , whence D S ( z ) ≤ 3 ∥ p r 2 ( z ) ∥ 2 = 3 h j 1 ( p r 2 ( z ) ) D_{S}(z)\le3\lVert\mathrm{pr}_{2}(z)\rVert^{2}=3h_{j_{1}}(\mathrm{pr}_{2}(z)) D S ( z ) ≤ 3 ∥ pr 2 ( z ) ∥ 2 = 3 h j 1 ( pr 2 ( z )) . Since D S = g D_{S}=g D S = g off E E E and D S ≤ 3 h j 1 ∘ p r 2 D_{S}\le3\,h_{j_{1}}\circ\mathrm{pr}_{2} D S ≤ 3 h j 1 ∘ pr 2 on E E E , claim 1 of Linearity and Monotonicity of the Lebesgue Integral, and the Integrability Criterion , together with the change-of-variables formula and ( p r 2 ) # π ′ = ν (\mathrm{pr}_{2})_{\#}\pi'=\nu ( pr 2 ) # π ′ = ν , gives
∫ R d + d D S d π ′ ≤ ∫ R d + d g d π ′ + 3 ∫ R d h j 1 d ν ≤ ∫ R d + d g d π ′ + 3 η . ( † ) \int_{\mathbb{R}^{d+d}}D_{S}\,d\pi'\le\int_{\mathbb{R}^{d+d}}g\,d\pi'+3\int_{\mathbb{R}^{d}}h_{j_{1}}\,d\nu\le\int_{\mathbb{R}^{d+d}}g\,d\pi'+3\eta . \tag{$\dagger$} ∫ R d + d D S d π ′ ≤ ∫ R d + d g d π ′ + 3 ∫ R d h j 1 d ν ≤ ∫ R d + d g d π ′ + 3 η . ( † )
Using π = ( i d , T ) # μ \pi=(\mathrm{id},T)_{\#}\mu π = ( id , T ) # μ together with g ≤ D S g\le D_{S} g ≤ D S , claim 1 of Linearity and Monotonicity of the Lebesgue Integral, and the Integrability Criterion and the change-of-variables formula,
∫ R d + d g d π ≤ ∫ R d + d D S d π = ∫ R d ∥ S − T ∥ 2 d μ ≤ η . \int_{\mathbb{R}^{d+d}}g\,d\pi\le\int_{\mathbb{R}^{d+d}}D_{S}\,d\pi=\int_{\mathbb{R}^{d}}\lVert S-T\rVert^{2}\,d\mu\le\eta . ∫ R d + d g d π ≤ ∫ R d + d D S d π = ∫ R d ∥ S − T ∥ 2 d μ ≤ η .
Since g g g is bounded and continuous and ( σ k j ) j (\sigma_{k_{j}})_{j} ( σ k j ) j converges weakly to π \pi π , the sequence ( ∫ g d σ k j ) j \bigl(\int g\,d\sigma_{k_{j}}\bigr)_{j} ( ∫ g d σ k j ) j converges to ∫ g d π ≤ η \int g\,d\pi\le\eta ∫ g d π ≤ η , so there is j 2 j_{2} j 2 with ∫ g d σ k j ≤ 2 η \int g\,d\sigma_{k_{j}}\le2\eta ∫ g d σ k j ≤ 2 η for every j ≥ j 2 j\ge j_{2} j ≥ j 2 . Combining this with ( † ) (\dagger) ( † ) applied to σ k j \sigma_{k_{j}} σ k j and then with ( ∗ ∗ ) (**) ( ∗ ∗ ) ,
∫ R d + d D T d σ k j ≤ 2 η + 2 ( 2 η + 3 η ) = 12 η for every j ≥ j 2 . \int_{\mathbb{R}^{d+d}}D_{T}\,d\sigma_{k_{j}}\le2\eta+2\bigl(2\eta+3\eta\bigr)=12\eta\qquad\text{for every }j\ge j_{2}. ∫ R d + d D T d σ k j ≤ 2 η + 2 ( 2 η + 3 η ) = 12 η for every j ≥ j 2 .
Step 5 (Claim 1). Suppose the sequence ( ∫ D T d π n ) n ∈ N \bigl(\int D_{T}\,d\pi_{n}\bigr)_{n\in\mathbb{N}} ( ∫ D T d π n ) n ∈ N does not converge to 0 0 0 . Its terms are nonnegative, so there are a positive real ε \varepsilon ε and a subsequence ( π n k ) k ∈ N (\pi_{n_{k}})_{k\in\mathbb{N}} ( π n k ) k ∈ N with ε ≤ ∫ D T d π n k \varepsilon\le\int D_{T}\,d\pi_{n_{k}} ε ≤ ∫ D T d π n k for every k k k . By A Subsequence of a Convergent Sequence Has the Same Limit the costs I ( π n k ) I(\pi_{n_{k}}) I ( π n k ) converge to W 2 ( μ , ν ) 2 W_{2}(\mu,\nu)^{2} W 2 ( μ , ν ) 2 , so Steps 3 and 4 apply to σ k = π n k \sigma_{k}=\pi_{n_{k}} σ k = π n k and yield, for every positive real η \eta η , a further subsequence along which ∫ D T d σ k j ≤ 12 η \int D_{T}\,d\sigma_{k_{j}}\le12\eta ∫ D T d σ k j ≤ 12 η eventually. Taking η = ε 24 \eta=\tfrac{\varepsilon}{24} η = 24 ε produces an index j j j with ∫ D T d π n k j ≤ ε 2 < ε \int D_{T}\,d\pi_{n_{k_{j}}}\le\tfrac{\varepsilon}{2}<\varepsilon ∫ D T d π n k j ≤ 2 ε < ε , contradicting the choice of the subsequence. Hence ( ∫ D T d π n ) n \bigl(\int D_{T}\,d\pi_{n}\bigr)_{n} ( ∫ D T d π n ) n converges to 0 0 0 , which is claim 1.