Each result cited is universally quantified over the data in its own statement, and is applied to the data named here. We prove clause 1 in full and then list the changes for clause 2.
Notation. The realising levels of Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §realising are strictly increasing with N 1 ≥ N 0 ≥ 2 N_{1}\ge N_{0}\ge2 N 1 ≥ N 0 ≥ 2 , so N k → ∞ N_{k}\to\infty N k → ∞ . For a fixed k k k we write N = N k N=N_{k} N = N k , w = w ‾ N , τ w=\overline{w}_{N,\tau} w = w N , τ , χ = χ N + \chi=\chi^{+}_{N} χ = χ N + , p 0 = p 0 , N p_{0}=p_{0,N} p 0 = p 0 , N , W ( x ) = W 2 ( μ x N , μ ^ ) W(x)=W_{2}(\mu^{N}_{x},\hat{\mu}) W ( x ) = W 2 ( μ x N , μ ^ ) , ∥ ⋅ ∥ \lVert\cdot\rVert ∥ ⋅ ∥ for the Euclidean norm of R N \mathbb{R}^{N} R N and ∥ ⋅ ∥ μ ^ \lVert\cdot\rVert_{\hat{\mu}} ∥ ⋅ ∥ μ ^ , ⟨ ⋅ , ⋅ ⟩ μ ^ \langle\cdot,\cdot\rangle_{\hat{\mu}} ⟨ ⋅ , ⋅ ⟩ μ ^ for those of L 2 ( μ ^ ; R ) L^{2}(\hat{\mu};\mathbb{R}) L 2 ( μ ^ ; R ) ; B i B_{i} B i , T x T_{x} T x , q ˉ i \bar{q}_{i} q ˉ i , m i m_{i} m i are as in Quantile Blocks of an Atomless Measure on the Line: Block Maps, Distances to Ordered Empirical Measures, and the Block Test Function . Put
m ^ = u ˉ τ ( μ ^ ) − δ E ( μ ^ ) , G k ( x ) = w ( x ) N − χ ( x ) − δ P N ( x ) N ( x ∈ W N ) , \hat{m}=\bar{u}_{\tau}(\hat{\mu})-\delta\mathcal{E}(\hat{\mu}),\qquad G_{k}(x)=\frac{w(x)}{N}-\chi(x)-\delta\frac{P_{N}(x)}{N}\quad(x\in W_{N}), m ^ = u ˉ τ ( μ ^ ) − δ E ( μ ^ ) , G k ( x ) = N w ( x ) − χ ( x ) − δ N P N ( x ) ( x ∈ W N ) ,
and, for P ∈ D N P\in\mathcal{D}_{N} P ∈ D N such that w − N χ w-N\chi w − N χ is P P P -integrable (integrals of functions on W N W_{N} W N are over W N W_{N} W N , which has full P P P -measure), Φ k ( P ) = ∫ ( w − N χ ) d P − δ E N ( P ) = δ ( ∫ f ˉ k d P − E N ( P ) ) \Phi_{k}(P)=\int(w-N\chi)\,dP-\delta\,\mathcal{E}_{N}(P)=\delta\bigl(\int\bar{f}_{k}\,dP-\mathcal{E}_{N}(P)\bigr) Φ k ( P ) = ∫ ( w − N χ ) d P − δ E N ( P ) = δ ( ∫ f ˉ k d P − E N ( P ) ) , with f ˉ k \bar{f}_{k} f ˉ k equal to f k f_{k} f k on W N W_{N} W N and to 0 0 0 off it. Since E N ( P ) = a N E n t ( P ) + ∫ P N d P \mathcal{E}_{N}(P)=a_{N}\mathrm{Ent}(P)+\int P_{N}\,dP E N ( P ) = a N Ent ( P ) + ∫ P N d P by The Relative Free Energy and the Relative Score of a Probability Measure for a Potential on an Open Set §energy ,
Φ k ( P ) N = ∫ G k d P − δ a N N E n t ( P ) . ( 0 ) \frac{\Phi_{k}(P)}{N}=\int G_{k}\,dP-\delta\,\frac{a_{N}}{N}\,\mathrm{Ent}(P).\qquad(0) N Φ k ( P ) = ∫ G k d P − δ N a N Ent ( P ) . ( 0 )
By Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §bounds and 0 < δ < 1 0<\delta<1 0 < δ < 1 , ∣ m ^ ∣ ≤ λ − 1 b g + ∣ E ( μ ^ ) ∣ |\hat{m}|\le\lambda^{-1}b_{g}+|\mathcal{E}(\hat{\mu})| ∣ m ^ ∣ ≤ λ − 1 b g + ∣ E ( μ ^ ) ∣ . Let e ∗ , A 0 e_{*},A_{0} e ∗ , A 0 be as in The Discrete Dyson Energy per Particle: Bounds, Compactness with a Lower Limit, and Recovery Configurations with Separated Particles §bounds ; then e ∗ N ≤ P N e_{*}N\le P_{N} e ∗ N ≤ P N on W N W_{N} W N , hence e ∗ N ≤ p 0 e_{*}N\le p_{0} e ∗ N ≤ p 0 .
Facts on the block test function. (F1) Expanding the formula of Quantile Blocks of an Atomless Measure on the Line: Block Maps, Distances to Ordered Empirical Measures, and the Block Test Function §test-function with μ ^ ( B i ) = 1 N \hat{\mu}(B_{i})=\frac1N μ ^ ( B i ) = N 1 (Quantile Blocks of an Atomless Measure on the Line: Block Maps, Distances to Ordered Empirical Measures, and the Block Test Function §blocks ) gives N χ ( x ) = K ∥ x ∥ 2 + ∑ i ( q ˉ i − 2 K m i ) x i + c χ N\chi(x)=K\lVert x\rVert^{2}+\sum_{i}(\bar{q}_{i}-2Km_{i})x_{i}+c_{\chi} N χ ( x ) = K ∥ x ∥ 2 + ∑ i ( q ˉ i − 2 K m i ) x i + c χ for a real c χ c_{\chi} c χ . (F2) By Cauchy-Schwarz on each block, q ˉ i 2 ≤ N ∫ B i q 2 d μ ^ \bar{q}_{i}^{2}\le N\int_{B_{i}}q^{2}\,d\hat{\mu} q ˉ i 2 ≤ N ∫ B i q 2 d μ ^ and ( x i − m i ) 2 = ( N ∫ B i ( x i − s ) μ ^ ( d s ) ) 2 ≤ N ∫ B i ( x i − s ) 2 μ ^ ( d s ) (x_{i}-m_{i})^{2}=\bigl(N\int_{B_{i}}(x_{i}-s)\,\hat{\mu}(ds)\bigr)^{2}\le N\int_{B_{i}}(x_{i}-s)^{2}\,\hat{\mu}(ds) ( x i − m i ) 2 = ( N ∫ B i ( x i − s ) μ ^ ( d s ) ) 2 ≤ N ∫ B i ( x i − s ) 2 μ ^ ( d s ) ; summing, and using Quantile Blocks of an Atomless Measure on the Line: Block Maps, Distances to Ordered Empirical Measures, and the Block Test Function §optimal for ordered x x x , ∑ i q ˉ i 2 ≤ N ∥ q ∥ μ ^ 2 \sum_{i}\bar{q}_{i}^{2}\le N\lVert q\rVert_{\hat{\mu}}^{2} ∑ i q ˉ i 2 ≤ N ∥ q ∥ μ ^ 2 and ∑ i ( x i − m i ) 2 ≤ N W ( x ) 2 \sum_{i}(x_{i}-m_{i})^{2}\le NW(x)^{2} ∑ i ( x i − m i ) 2 ≤ N W ( x ) 2 . With the gradient formula of Quantile Blocks of an Atomless Measure on the Line: Block Maps, Distances to Ordered Empirical Measures, and the Block Test Function §test-function , for ordered x x x
∥ N ∇ χ ( x ) ∥ 2 = ∑ i ( q ˉ i + 2 K ( x i − m i ) ) 2 ≤ 2 N ∥ q ∥ μ ^ 2 + 8 K 2 N W ( x ) 2 . ( F 3 ) \lVert N\nabla\chi(x)\rVert^{2}=\sum_{i}\bigl(\bar{q}_{i}+2K(x_{i}-m_{i})\bigr)^{2}\le2N\lVert q\rVert_{\hat{\mu}}^{2}+8K^{2}N\,W(x)^{2}.\qquad(\mathrm{F}3) ∥ N ∇ χ ( x ) ∥ 2 = i ∑ ( q ˉ i + 2 K ( x i − m i ) ) 2 ≤ 2 N ∥ q ∥ μ ^ 2 + 8 K 2 N W ( x ) 2 . ( F 3 )
(F4) For ordered x x x (in particular x ∈ W N x\in W_{N} x ∈ W N ), Quantile Blocks of an Atomless Measure on the Line: Block Maps, Distances to Ordered Empirical Measures, and the Block Test Function §optimal with ν = μ ^ \nu=\hat{\mu} ν = μ ^ and T = i d T=\mathrm{id} T = id gives W ( x ) = ∥ T x − i d ∥ μ ^ W(x)=\lVert T_{x}-\mathrm{id}\rVert_{\hat{\mu}} W ( x ) = ∥ T x − id ∥ μ ^ , and W ( x ) 2 = ∑ i ∫ B i ( x i − s ) 2 μ ^ ( d s ) W(x)^{2}=\sum_{i}\int_{B_{i}}(x_{i}-s)^{2}\,\hat{\mu}(ds) W ( x ) 2 = ∑ i ∫ B i ( x i − s ) 2 μ ^ ( d s ) is a polynomial in x x x ; by Quantile Blocks of an Atomless Measure on the Line: Block Maps, Distances to Ordered Empirical Measures, and the Block Test Function §test-function , χ ( x ) = ⟨ q , T x − i d ⟩ μ ^ + K W ( x ) 2 \chi(x)=\langle q,T_{x}-\mathrm{id}\rangle_{\hat{\mu}}+KW(x)^{2} χ ( x ) = ⟨ q , T x − id ⟩ μ ^ + K W ( x ) 2 , so − ∥ q ∥ μ ^ W ( x ) + K W ( x ) 2 ≤ χ ( x ) ≤ ∥ q ∥ μ ^ W ( x ) + K W ( x ) 2 -\lVert q\rVert_{\hat{\mu}}W(x)+KW(x)^{2}\le\chi(x)\le\lVert q\rVert_{\hat{\mu}}W(x)+KW(x)^{2} − ∥ q ∥ μ ^ W ( x ) + K W ( x ) 2 ≤ χ ( x ) ≤ ∥ q ∥ μ ^ W ( x ) + K W ( x ) 2 and χ ( x ) ≥ − ∥ q ∥ μ ^ 2 / ( 4 K ) ≥ − ∥ q ∥ μ ^ 2 \chi(x)\ge-\lVert q\rVert_{\hat{\mu}}^{2}/(4K)\ge-\lVert q\rVert_{\hat{\mu}}^{2} χ ( x ) ≥ − ∥ q ∥ μ ^ 2 / ( 4 K ) ≥ − ∥ q ∥ μ ^ 2 (as K ≥ 1 K\ge1 K ≥ 1 ). Also N W ( x ) 2 ≤ 2 ∥ x ∥ 2 + 2 N M 2 ( μ ^ ) NW(x)^{2}\le2\lVert x\rVert^{2}+2NM_{2}(\hat{\mu}) N W ( x ) 2 ≤ 2 ∥ x ∥ 2 + 2 N M 2 ( μ ^ ) .
Step 1 (hypotheses; optimal maps; clause (a)). W N W_{N} W N (The Weyl Chamber of Ordered Points in Euclidean Space ) is open and convex, being a finite intersection of open half-spaces, and nonempty, containing ( N , N − 1 , … , 1 ) (N,N-1,\dots,1) ( N , N − 1 , … , 1 ) . P N P_{N} P N is a penalty on W N W_{N} W N with monotone gradient (The N-Particle Dyson Potential on the Weyl Chamber: Penalty, Monotone Gradient, Dissipation with Constants Uniform in N, and Gibbs Integrability §penalty ), and the Gibbs integrability function of Gibbs Maximisers of the Relative Free Energy: the Variational Principle and the Relative Score for U = P N U=P_{N} U = P N , a = a N a=a_{N} a = a N is the function g N g_{N} g N of The N-Particle Dyson Potential on the Weyl Chamber: Penalty, Monotone Gradient, Dissipation with Constants Uniform in N, and Gibbs Integrability §gibbs , which is integrable. By Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §regularised (ii) and Semiconvex Function on a Convex Subset of R n \mathbb{R}^n R n , w + 1 2 τ ∥ x ∥ 2 w+\frac{1}{2\tau}\lVert x\rVert^{2} w + 2 τ 1 ∥ x ∥ 2 is convex on W N W_{N} W N ; by (F1), − N χ + K ∥ x ∥ 2 -N\chi+K\lVert x\rVert^{2} − N χ + K ∥ x ∥ 2 is affine; so f k + 1 2 δ − 1 ( τ − 1 + 2 K ) ∥ x ∥ 2 = δ − 1 [ ( w + 1 2 τ ∥ x ∥ 2 ) + ( − N χ + K ∥ x ∥ 2 ) ] f_{k}+\frac{1}{2}\delta^{-1}(\tau^{-1}+2K)\lVert x\rVert^{2}=\delta^{-1}\bigl[(w+\frac{1}{2\tau}\lVert x\rVert^{2})+(-N\chi+K\lVert x\rVert^{2})\bigr] f k + 2 1 δ − 1 ( τ − 1 + 2 K ) ∥ x ∥ 2 = δ − 1 [ ( w + 2 τ 1 ∥ x ∥ 2 ) + ( − N χ + K ∥ x ∥ 2 ) ] is convex, and f k f_{k} f k is semiconvex on W N W_{N} W N with constant δ − 1 ( τ − 1 + 2 K ) \delta^{-1}(\tau^{-1}+2K) δ − 1 ( τ − 1 + 2 K ) . By Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §regularised (i) and (F4), f k ≤ δ − 1 ( λ − 1 N b g + ∣ e ∗ ∣ + N ∥ q ∥ μ ^ 2 ) f_{k}\le\delta^{-1}(\lambda^{-1}Nb_{g}+|e_{*}|+N\lVert q\rVert_{\hat{\mu}}^{2}) f k ≤ δ − 1 ( λ − 1 N b g + ∣ e ∗ ∣ + N ∥ q ∥ μ ^ 2 ) on W N W_{N} W N . Since χ \chi χ is C 2 C^{2} C 2 , f k f_{k} f k is differentiable at x ∈ W N x\in W_{N} x ∈ W N exactly when w w w is, and then D f k ( x ) = δ − 1 ( D w ( x ) − N ∇ χ ( x ) ) Df_{k}(x)=\delta^{-1}(Dw(x)-N\nabla\chi(x)) D f k ( x ) = δ − 1 ( D w ( x ) − N ∇ χ ( x )) . At such x x x , Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §regularised (iii) gives ∥ D w ( x ) ∥ 2 ≤ τ − 2 r N ( x ) 2 = 2 τ ( 2 λ − 1 N b g + P N ( x ) − p 0 N ) \lVert Dw(x)\rVert^{2}\le\tau^{-2}r_{N}(x)^{2}=\frac{2}{\tau}\bigl(2\lambda^{-1}Nb_{g}+\frac{P_{N}(x)-p_{0}}{N}\bigr) ∥ D w ( x ) ∥ 2 ≤ τ − 2 r N ( x ) 2 = τ 2 ( 2 λ − 1 N b g + N P N ( x ) − p 0 ) , and (F3), (F4) and The Discrete Dyson Energy per Particle: Bounds, Compactness with a Lower Limit, and Recovery Configurations with Separated Particles §bounds give ∥ N ∇ χ ( x ) ∥ 2 ≤ 2 N ∥ q ∥ μ ^ 2 + 8 K 2 ( 2 A 0 ( N + p 0 − e ∗ N ) + 2 A 0 ( P N ( x ) − p 0 ) + 2 N M 2 ( μ ^ ) ) \lVert N\nabla\chi(x)\rVert^{2}\le2N\lVert q\rVert_{\hat{\mu}}^{2}+8K^{2}\bigl(2A_{0}(N+p_{0}-e_{*}N)+2A_{0}(P_{N}(x)-p_{0})+2NM_{2}(\hat{\mu})\bigr) ∥ N ∇ χ ( x ) ∥ 2 ≤ 2 N ∥ q ∥ μ ^ 2 + 8 K 2 ( 2 A 0 ( N + p 0 − e ∗ N ) + 2 A 0 ( P N ( x ) − p 0 ) + 2 N M 2 ( μ ^ ) ) . Hence ∥ D f k ( x ) ∥ 2 ≤ 2 δ − 2 ( ∥ D w ( x ) ∥ 2 + ∥ N ∇ χ ( x ) ∥ 2 ) ≤ A + B ( P N ( x ) − p 0 ) \lVert Df_{k}(x)\rVert^{2}\le2\delta^{-2}(\lVert Dw(x)\rVert^{2}+\lVert N\nabla\chi(x)\rVert^{2})\le A+B(P_{N}(x)-p_{0}) ∥ D f k ( x ) ∥ 2 ≤ 2 δ − 2 (∥ D w ( x ) ∥ 2 + ∥ N ∇ χ ( x ) ∥ 2 ) ≤ A + B ( P N ( x ) − p 0 ) for nonnegative A , B A,B A , B depending on k k k . All hypotheses of Gibbs Maximisers of the Relative Free Energy: the Variational Principle and the Relative Score hold, so π k \pi_{k} π k is defined, π k ∈ D N \pi_{k}\in\mathcal{D}_{N} π k ∈ D N , π k ( W N ) = 1 \pi_{k}(W_{N})=1 π k ( W N ) = 1 and Φ k ( π k ) = δ a N log Z \Phi_{k}(\pi_{k})=\delta a_{N}\log Z Φ k ( π k ) = δ a N log Z (Gibbs Maximisers of the Relative Free Energy: the Variational Principle and the Relative Score §gibbs ), and Φ k ( P ) ≤ δ a N log Z = Φ k ( π k ) \Phi_{k}(P)\le\delta a_{N}\log Z=\Phi_{k}(\pi_{k}) Φ k ( P ) ≤ δ a N log Z = Φ k ( π k ) for every admissible P P P (Gibbs Maximisers of the Relative Free Energy: the Variational Principle and the Relative Score §variational , multiplied by δ \delta δ ). Moreover G k G_{k} G k is π k \pi_{k} π k -integrable: w w w is bounded (Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §regularised (i)), χ \chi χ is a polynomial of degree at most 2 2 2 and π k ∈ P 2 ( R N ) \pi_{k}\in\mathcal{P}_{2}(\mathbb{R}^{N}) π k ∈ P 2 ( R N ) , and P N P_{N} P N is π k \pi_{k} π k -integrable as π k ∈ D N \pi_{k}\in\mathcal{D}_{N} π k ∈ D N (The Relative Free Energy and the Relative Score of a Probability Measure for a Potential on an Open Set §energy ).
Optimal maps. Let ν ∈ P 2 ( R ) \nu\in\mathcal{P}_{2}(\mathbb{R}) ν ∈ P 2 ( R ) and let T T T be an optimal map from μ ^ \hat{\mu} μ ^ to ν \nu ν . By the change-of-variables formula of Probability Measures on Euclidean Space and Random Vectors: Standing Notation §pushforward , ∫ T 2 d μ ^ = ∫ t 2 ν ( d t ) < ∞ \int T^{2}\,d\hat{\mu}=\int t^{2}\,\nu(dt)<\infty ∫ T 2 d μ ^ = ∫ t 2 ν ( d t ) < ∞ , so the class of T T T lies in L 2 ( μ ^ ; R ) L^{2}(\hat{\mu};\mathbb{R}) L 2 ( μ ^ ; R ) , and the quadratic cost of ( i d , T ) # μ ^ (\mathrm{id},T)_{\#}\hat{\mu} ( id , T ) # μ ^ is ∫ ∣ s − T ( s ) ∣ 2 μ ^ ( d s ) = ∥ T − i d ∥ μ ^ 2 \int|s-T(s)|^{2}\,\hat{\mu}(ds)=\lVert T-\mathrm{id}\rVert_{\hat{\mu}}^{2} ∫ ∣ s − T ( s ) ∣ 2 μ ^ ( d s ) = ∥ T − id ∥ μ ^ 2 ; this coupling being optimal , ∥ T − i d ∥ μ ^ = W 2 ( μ ^ , ν ) = W 2 ( ν , μ ^ ) \lVert T-\mathrm{id}\rVert_{\hat{\mu}}=W_{2}(\hat{\mu},\nu)=W_{2}(\nu,\hat{\mu}) ∥ T − id ∥ μ ^ = W 2 ( μ ^ , ν ) = W 2 ( ν , μ ^ ) .
Clause (a). By Gibbs Maximisers of the Relative Free Energy: the Variational Principle and the Relative Score §score , π k ∈ D N Σ \pi_{k}\in\mathcal{D}^{\Sigma}_{N} π k ∈ D N Σ and Σ N ( π k ) = ∇ f k \Sigma_{N}(\pi_{k})=\nabla f_{k} Σ N ( π k ) = ∇ f k in L 2 ( π k ; R N ) L^{2}(\pi_{k};\mathbb{R}^{N}) L 2 ( π k ; R N ) for every gradient map ∇ f k \nabla f_{k} ∇ f k of f k f_{k} f k . Let ∇ w \nabla w ∇ w be a gradient map of w w w (Gradient Maps of a Function on an Open Subset of Euclidean Space §gradient-map ), with null set N ′ N' N ′ . The map δ − 1 ( ∇ w − N ∇ χ ) \delta^{-1}(\nabla w-N\nabla\chi) δ − 1 ( ∇ w − N ∇ χ ) is Borel (∇ χ \nabla\chi ∇ χ being continuous), and at every x ∈ W N ∖ N ′ x\in W_{N}\setminus N' x ∈ W N ∖ N ′ the function w w w , hence f k f_{k} f k , is differentiable with D f k ( x ) = δ − 1 ( ∇ w ( x ) − N ∇ χ ( x ) ) Df_{k}(x)=\delta^{-1}(\nabla w(x)-N\nabla\chi(x)) D f k ( x ) = δ − 1 ( ∇ w ( x ) − N ∇ χ ( x )) ; so it is a gradient map of f k f_{k} f k , and δ − 1 ( ∇ w − N ∇ χ ) = Σ N ( π k ) \delta^{-1}(\nabla w-N\nabla\chi)=\Sigma_{N}(\pi_{k}) δ − 1 ( ∇ w − N ∇ χ ) = Σ N ( π k ) in L 2 ( π k ; R N ) L^{2}(\pi_{k};\mathbb{R}^{N}) L 2 ( π k ; R N ) . As N ∇ χ N\nabla\chi N ∇ χ is affine and π k ∈ P 2 ( R N ) \pi_{k}\in\mathcal{P}_{2}(\mathbb{R}^{N}) π k ∈ P 2 ( R N ) , its class lies in L 2 ( π k ; R N ) L^{2}(\pi_{k};\mathbb{R}^{N}) L 2 ( π k ; R N ) , hence so does that of ∇ w = N ∇ χ + δ ∇ f k \nabla w=N\nabla\chi+\delta\nabla f_{k} ∇ w = N ∇ χ + δ ∇ f k , and ∇ w = N ∇ χ + δ Σ N ( π k ) \nabla w=N\nabla\chi+\delta\Sigma_{N}(\pi_{k}) ∇ w = N ∇ χ + δ Σ N ( π k ) there.
Step 2 (value lower bound). Claim: for every positive ε \varepsilon ε there is k 0 k_{0} k 0 with Φ k ( π k ) / N ≥ m ^ − ε \Phi_{k}(\pi_{k})/N\ge\hat{m}-\varepsilon Φ k ( π k ) / N ≥ m ^ − ε for every k ≥ k 0 k\ge k_{0} k ≥ k 0 .
Diagonal choice. For each natural j ≥ 1 j\ge1 j ≥ 1 , The Discrete Dyson Energy per Particle: Bounds, Compactness with a Lower Limit, and Recovery Configurations with Separated Particles §recovery applied to μ ^ \hat{\mu} μ ^ and 1 / j 1/j 1/ j gives positive c j , R j c_{j},R_{j} c j , R j and N 1 ( j ) ≥ 2 N_{1}(j)\ge2 N 1 ( j ) ≥ 2 ; replacing c j c_{j} c j by min ( c j , 1 ) \min(c_{j},1) min ( c j , 1 ) keeps its gap condition, so we assume c j ≤ 1 c_{j}\le1 c j ≤ 1 . Let L j L_{j} L j be the maximum of ∣ V ′ ∣ |V'| ∣ V ′ ∣ on [ − R j − 1 , R j + 1 ] [-R_{j}-1,R_{j}+1] [ − R j − 1 , R j + 1 ] (V ′ V' V ′ is continuous, V V V being C 2 C^{2} C 2 by The N-Particle Dyson Potential on the Weyl Chamber: Penalty, Monotone Gradient, Dissipation with Constants Uniform in N, and Gibbs Integrability §hypotheses ) and Λ j = log ( 1 / c j ) + L j ≥ 0 \Lambda_{j}=\log(1/c_{j})+L_{j}\ge0 Λ j = log ( 1/ c j ) + L j ≥ 0 . For each k k k let S k S_{k} S k be the set of j ∈ [ k ] j\in[k] j ∈ [ k ] with N k ≥ N 1 ( i ) N_{k}\ge N_{1}(i) N k ≥ N 1 ( i ) and N k ≥ i ( 1 + Λ i ) N_{k}\ge i(1+\Lambda_{i}) N k ≥ i ( 1 + Λ i ) for every i ∈ [ j ] i\in[j] i ∈ [ j ] . Since N k → ∞ N_{k}\to\infty N k → ∞ , each j j j lies in S k S_{k} S k for all large k k k ; let k 1 k_{1} k 1 be such that 1 ∈ S k 1\in S_{k} 1 ∈ S k for k ≥ k 1 k\ge k_{1} k ≥ k 1 , and put j ( k ) = max S k j(k)=\max S_{k} j ( k ) = max S k for k ≥ k 1 k\ge k_{1} k ≥ k 1 . Then j ( k ) → ∞ j(k)\to\infty j ( k ) → ∞ , N k ≥ N 1 ( j ( k ) ) N_{k}\ge N_{1}(j(k)) N k ≥ N 1 ( j ( k )) and Λ j ( k ) ≤ N k / j ( k ) \Lambda_{j(k)}\le N_{k}/j(k) Λ j ( k ) ≤ N k / j ( k ) . For k ≥ k 1 k\ge k_{1} k ≥ k 1 let y k ∈ W N k y^{k}\in W_{N_{k}} y k ∈ W N k be the point of The Discrete Dyson Energy per Particle: Bounds, Compactness with a Lower Limit, and Recovery Configurations with Separated Particles §recovery for j = j ( k ) j=j(k) j = j ( k ) and N = N k N=N_{k} N = N k , and for k < k 1 k<k_{1} k < k 1 any point of W N k W_{N_{k}} W N k . Then W ( y k ) < 1 / j ( k ) → 0 W(y^{k})<1/j(k)\to0 W ( y k ) < 1/ j ( k ) → 0 and P N k ( y k ) ≤ c ′ N k P_{N_{k}}(y^{k})\le c'N_{k} P N k ( y k ) ≤ c ′ N k for all k k k , with c ′ c' c ′ the largest of E ( μ ^ ) + 1 \mathcal{E}(\hat{\mu})+1 E ( μ ^ ) + 1 and the finitely many P N k ( y k ) / N k P_{N_{k}}(y^{k})/N_{k} P N k ( y k ) / N k , k < k 1 k<k_{1} k < k 1 ; so w ( y k ) / N k → u ˉ τ ( μ ^ ) w(y^{k})/N_{k}\to\bar{u}_{\tau}(\hat{\mu}) w ( y k ) / N k → u ˉ τ ( μ ^ ) by Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §realising .
Fix k ≥ k 1 k\ge k_{1} k ≥ k 1 and write j = j ( k ) j=j(k) j = j ( k ) , c = c j c=c_{j} c = c j , L = L j L=L_{j} L = L j , Λ = Λ j \Lambda=\Lambda_{j} Λ = Λ j , y = y k y=y^{k} y = y k , h = c / ( 4 N ) ≤ 1 / ( 4 N ) h=c/(4N)\le1/(4N) h = c / ( 4 N ) ≤ 1/ ( 4 N ) and Q = { z ∈ R N : ∣ z i − y i ∣ ≤ h for every i } Q=\{z\in\mathbb{R}^{N}:|z_{i}-y_{i}|\le h\text{ for every }i\} Q = { z ∈ R N : ∣ z i − y i ∣ ≤ h for every i } . For i < l i<l i < l , summing gaps, y i − y l ≥ ( l − i ) c / N ≥ 4 h y_{i}-y_{l}\ge(l-i)c/N\ge4h y i − y l ≥ ( l − i ) c / N ≥ 4 h , so for z ∈ Q z\in Q z ∈ Q , z i − z l ≥ y i − y l − 2 h ≥ 1 2 ( y i − y l ) > 0 z_{i}-z_{l}\ge y_{i}-y_{l}-2h\ge\frac12(y_{i}-y_{l})>0 z i − z l ≥ y i − y l − 2 h ≥ 2 1 ( y i − y l ) > 0 ; thus Q ⊆ W N Q\subseteq W_{N} Q ⊆ W N . Also ∥ z − y ∥ ≤ h N \lVert z-y\rVert\le h\sqrt{N} ∥ z − y ∥ ≤ h N for z ∈ Q z\in Q z ∈ Q .
(2a) Energy on Q Q Q . Let z ∈ Q z\in Q z ∈ Q and i < l i<l i < l ; with t = ( z i − z l ) / ( y i − y l ) t=(z_{i}-z_{l})/(y_{i}-y_{l}) t = ( z i − z l ) / ( y i − y l ) and u = 2 h / ( y i − y l ) ≤ 1 2 u=2h/(y_{i}-y_{l})\le\frac12 u = 2 h / ( y i − y l ) ≤ 2 1 we have t ≥ 1 − u t\ge1-u t ≥ 1 − u , and by The Function s log s s\log s s log s : Continuity, Young's Inequality and Lower Bounds, with the Elementary Bounds for the Exponential and the Logarithm §log , − log t ≤ t − 1 − 1 ≤ u / ( 1 − u ) ≤ 2 u = 4 h / ( y i − y l ) ≤ 1 / ( l − i ) -\log t\le t^{-1}-1\le u/(1-u)\le2u=4h/(y_{i}-y_{l})\le1/(l-i) − log t ≤ t − 1 − 1 ≤ u / ( 1 − u ) ≤ 2 u = 4 h / ( y i − y l ) ≤ 1/ ( l − i ) . By The Logarithmic Energy of N Ordered Particles on the Weyl Chamber §energy with strength b N = β / ( 2 ( N − 1 ) ) b_{N}=\beta/(2(N-1)) b N = β / ( 2 ( N − 1 )) ,
H b N ( z ) − H b N ( y ) = − b N ∑ i < l log t ≤ b N ∑ m = 1 N − 1 N − m m ≤ b N N ( 1 + log N ) , H_{b_{N}}(z)-H_{b_{N}}(y)=-b_{N}\sum_{i<l}\log t\le b_{N}\sum_{m=1}^{N-1}\frac{N-m}{m}\le b_{N}N(1+\log N), H b N ( z ) − H b N ( y ) = − b N i < l ∑ log t ≤ b N m = 1 ∑ N − 1 m N − m ≤ b N N ( 1 + log N ) ,
using 1 m ≤ log m m − 1 \frac1m\le\log\frac{m}{m-1} m 1 ≤ log m − 1 m for m ≥ 2 m\ge2 m ≥ 2 (The Function s log s s\log s s log s : Continuity, Young's Inequality and Lower Bounds, with the Elementary Bounds for the Exponential and the Logarithm §log ). As ∣ z i ∣ , ∣ y i ∣ ≤ R j + 1 |z_{i}|,|y_{i}|\le R_{j}+1 ∣ z i ∣ , ∣ y i ∣ ≤ R j + 1 , the mean value theorem gives ∣ V ( z i ) − V ( y i ) ∣ ≤ L h ≤ L / ( 4 N ) ≤ Λ / N ≤ 1 / j |V(z_{i})-V(y_{i})|\le Lh\le L/(4N)\le\Lambda/N\le1/j ∣ V ( z i ) − V ( y i ) ∣ ≤ L h ≤ L / ( 4 N ) ≤ Λ/ N ≤ 1/ j . Hence, with the bound on P N ( y ) P_{N}(y) P N ( y ) from The Discrete Dyson Energy per Particle: Bounds, Compactness with a Lower Limit, and Recovery Configurations with Separated Particles §recovery ,
e ∗ N ≤ P N ( z ) ≤ N e k , e k = E ( μ ^ ) + 2 j + β ( 1 + log N ) 2 ( N − 1 ) ≤ e ˉ = E ( μ ^ ) + 2 + β , e_{*}N\le P_{N}(z)\le Ne_{k},\qquad e_{k}=\mathcal{E}(\hat{\mu})+\frac{2}{j}+\frac{\beta(1+\log N)}{2(N-1)}\le\bar{e}=\mathcal{E}(\hat{\mu})+2+\beta, e ∗ N ≤ P N ( z ) ≤ N e k , e k = E ( μ ^ ) + j 2 + 2 ( N − 1 ) β ( 1 + log N ) ≤ e ˉ = E ( μ ^ ) + 2 + β ,
using 1 + log N ≤ N ≤ 2 ( N − 1 ) 1+\log N\le N\le2(N-1) 1 + log N ≤ N ≤ 2 ( N − 1 ) (The Function s log s s\log s s log s : Continuity, Young's Inequality and Lower Bounds, with the Elementary Bounds for the Exponential and the Logarithm §log ).
(2b) w w w on Q Q Q . By Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §regularised (iv) with the pair ( y , z ) (y,z) ( y , z ) in place of ( x , y ) (x,y) ( x , y ) , w ( y ) ≤ w ( z ) + 1 2 τ ∥ y − z ∥ ( 3 ∥ y − z ∥ + 2 r N ( z ) ) w(y)\le w(z)+\frac{1}{2\tau}\lVert y-z\rVert(3\lVert y-z\rVert+2r_{N}(z)) w ( y ) ≤ w ( z ) + 2 τ 1 ∥ y − z ∥ ( 3 ∥ y − z ∥ + 2 r N ( z )) , so w ( z ) / N ≥ w ( y ) / N − 1 2 τ ( 3 h 2 + 2 h r N ( z ) / N ) w(z)/N\ge w(y)/N-\frac{1}{2\tau}(3h^{2}+2hr_{N}(z)/\sqrt{N}) w ( z ) / N ≥ w ( y ) / N − 2 τ 1 ( 3 h 2 + 2 h r N ( z ) / N ) . By (2a) and p 0 ≥ e ∗ N p_{0}\ge e_{*}N p 0 ≥ e ∗ N , r N ( z ) 2 / N = 2 τ ( 2 λ − 1 b g + ( P N ( z ) − p 0 ) / N 2 ) ≤ 2 τ ( 2 λ − 1 b g + e ˉ − e ∗ ) = : ρ 2 r_{N}(z)^{2}/N=2\tau\bigl(2\lambda^{-1}b_{g}+(P_{N}(z)-p_{0})/N^{2}\bigr)\le2\tau(2\lambda^{-1}b_{g}+\bar{e}-e_{*})=:\rho^{2} r N ( z ) 2 / N = 2 τ ( 2 λ − 1 b g + ( P N ( z ) − p 0 ) / N 2 ) ≤ 2 τ ( 2 λ − 1 b g + e ˉ − e ∗ ) =: ρ 2 , so with h ≤ 1 h\le1 h ≤ 1 , w ( z ) / N ≥ w ( y ) / N − ( 3 + 2 ρ ) h / ( 2 τ ) w(z)/N\ge w(y)/N-(3+2\rho)h/(2\tau) w ( z ) / N ≥ w ( y ) / N − ( 3 + 2 ρ ) h / ( 2 τ ) .
(2c) χ \chi χ on Q Q Q . By Quantile Blocks of an Atomless Measure on the Line: Block Maps, Distances to Ordered Empirical Measures, and the Block Test Function §block-maps , ∥ T z − T y ∥ μ ^ = ∥ z − y ∥ / N ≤ h \lVert T_{z}-T_{y}\rVert_{\hat{\mu}}=\lVert z-y\rVert/\sqrt{N}\le h ∥ T z − T y ∥ μ ^ = ∥ z − y ∥ / N ≤ h ; with (F4), χ ( z ) ≤ χ ( y ) + ∥ q ∥ μ ^ h + K h ( 2 W ( y ) + h ) \chi(z)\le\chi(y)+\lVert q\rVert_{\hat{\mu}}h+Kh(2W(y)+h) χ ( z ) ≤ χ ( y ) + ∥ q ∥ μ ^ h + K h ( 2 W ( y ) + h ) and χ ( y ) ≤ ∥ q ∥ μ ^ W ( y ) + K W ( y ) 2 \chi(y)\le\lVert q\rVert_{\hat{\mu}}W(y)+KW(y)^{2} χ ( y ) ≤ ∥ q ∥ μ ^ W ( y ) + K W ( y ) 2 .
(2d) The competitor. Let P P P be the measure with density ( 2 h ) − N 1 Q (2h)^{-N}\mathbf{1}_{Q} ( 2 h ) − N 1 Q with respect to Lebesgue measure (Q Q Q has Lebesgue measure ( 2 h ) N (2h)^{N} ( 2 h ) N ). It is a probability measure with bounded support, so P ∈ P 2 ( R N ) P\in\mathcal{P}_{2}(\mathbb{R}^{N}) P ∈ P 2 ( R N ) , with P ( W N ) = 1 P(W_{N})=1 P ( W N ) = 1 ; by The Entropy of a Probability Measure on Euclidean Space §entropy (with ϕ ( 0 ) = 0 \phi(0)=0 ϕ ( 0 ) = 0 ) it has finite entropy E n t ( P ) = − N log ( 2 h ) = N log ( 2 N / c ) \mathrm{Ent}(P)=-N\log(2h)=N\log(2N/c) Ent ( P ) = − N log ( 2 h ) = N log ( 2 N / c ) ; P N P_{N} P N is bounded on Q Q Q by (2a), so P ∈ D N P\in\mathcal{D}_{N} P ∈ D N ; and w − N χ w-N\chi w − N χ is bounded on Q Q Q by Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §regularised (i) and (2c). By Step 1, (0) and (2a)--(2c),
Φ k ( π k ) N ≥ Φ k ( P ) N ≥ w ( y ) N − ( 3 + 2 ρ ) h 2 τ − ∥ q ∥ μ ^ ( W ( y ) + h ) − K ( W ( y ) 2 + 2 h W ( y ) + h 2 ) − δ e k − a N ( log ( 2 N ) + Λ ) . \frac{\Phi_{k}(\pi_{k})}{N}\ge\frac{\Phi_{k}(P)}{N}\ge\frac{w(y)}{N}-\frac{(3+2\rho)h}{2\tau}-\lVert q\rVert_{\hat{\mu}}(W(y)+h)-K\bigl(W(y)^{2}+2hW(y)+h^{2}\bigr)-\delta e_{k}-a_{N}\bigl(\log(2N)+\Lambda\bigr). N Φ k ( π k ) ≥ N Φ k ( P ) ≥ N w ( y ) − 2 τ ( 3 + 2 ρ ) h − ∥ q ∥ μ ^ ( W ( y ) + h ) − K ( W ( y ) 2 + 2 hW ( y ) + h 2 ) − δ e k − a N ( log ( 2 N ) + Λ ) .
As k → ∞ k\to\infty k → ∞ : w ( y k ) / N k → u ˉ τ ( μ ^ ) w(y^{k})/N_{k}\to\bar{u}_{\tau}(\hat{\mu}) w ( y k ) / N k → u ˉ τ ( μ ^ ) , W ( y k ) → 0 W(y^{k})\to0 W ( y k ) → 0 , h ≤ 1 / ( 4 N k ) → 0 h\le1/(4N_{k})\to0 h ≤ 1/ ( 4 N k ) → 0 , e k → E ( μ ^ ) e_{k}\to\mathcal{E}(\hat{\mu}) e k → E ( μ ^ ) , a N log ( 2 N ) → 0 a_{N}\log(2N)\to0 a N log ( 2 N ) → 0 , and a N Λ ≤ σ 2 Λ / N ≤ σ 2 / j ( k ) → 0 a_{N}\Lambda\le\sigma^{2}\Lambda/N\le\sigma^{2}/j(k)\to0 a N Λ ≤ σ 2 Λ/ N ≤ σ 2 / j ( k ) → 0 . The right side tends to m ^ \hat{m} m ^ , which proves the claim.
Step 3 (entropy bound; clause (b)). Let c 1 c_{1} c 1 be the Gaussian constant of 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 in dimension N N N . By The Gaussian Kernels on Euclidean Space: Scaling, Derivatives up to Order Three, the Convolution Identity, Moments and Tails §moments with q = N q=N q = N , s = 1 s=1 s = 1 and R = 2 N R=\sqrt{2N} R = 2 N , the Gaussian weight g 1 ≤ c 1 g_{1}\le c_{1} g 1 ≤ c 1 has mass at most 1 2 \frac12 2 1 outside the ball of radius R R R , which lies in the cube [ − R , R ] N [-R,R]^{N} [ − R , R ] N of Lebesgue measure ( 2 R ) N (2R)^{N} ( 2 R ) N ; so 1 2 ≤ c 1 ( 2 R ) N \frac12\le c_{1}(2R)^{N} 2 1 ≤ c 1 ( 2 R ) N and log c 1 ≥ − log 2 − N 2 log ( 8 N ) \log c_{1}\ge-\log2-\frac N2\log(8N) log c 1 ≥ − log 2 − 2 N log ( 8 N ) . For P ∈ D N P\in\mathcal{D}_{N} P ∈ D N put X ( P ) = 1 N ∫ P N d P X(P)=\frac1N\int P_{N}\,dP X ( P ) = N 1 ∫ P N d P ; by The Discrete Dyson Energy per Particle: Bounds, Compactness with a Lower Limit, and Recovery Configurations with Separated Particles §bounds , M 2 ( P ) ≤ A 0 N ( 1 + X ( P ) − e ∗ ) M_{2}(P)\le A_{0}N(1+X(P)-e_{*}) M 2 ( P ) ≤ A 0 N ( 1 + X ( P ) − e ∗ ) , and 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 §lower gives
δ a N N E n t ( P ) ≥ − δ ε N − δ θ N X ( P ) , ε N = a N ( log 2 + 1 2 log ( 8 N ) + A 0 2 ( 1 + ∣ e ∗ ∣ ) ) , θ N = a N A 0 2 , ( 3 a ) \delta\frac{a_{N}}{N}\mathrm{Ent}(P)\ge-\delta\varepsilon_{N}-\delta\theta_{N}X(P),\qquad\varepsilon_{N}=a_{N}\Bigl(\log2+\tfrac12\log(8N)+\tfrac{A_{0}}{2}(1+|e_{*}|)\Bigr),\quad\theta_{N}=\frac{a_{N}A_{0}}{2},\qquad(3\mathrm{a}) δ N a N Ent ( P ) ≥ − δ ε N − δ θ N X ( P ) , ε N = a N ( log 2 + 2 1 log ( 8 N ) + 2 A 0 ( 1 + ∣ e ∗ ∣ ) ) , θ N = 2 a N A 0 , ( 3 a )
where ε N , θ N → 0 \varepsilon_{N},\theta_{N}\to0 ε N , θ N → 0 as k → ∞ k\to\infty k → ∞ . Write X k = X ( π k ) X_{k}=X(\pi_{k}) X k = X ( π k ) . By (0), (3a) and Step 2, for every positive ε \varepsilon ε and k ≥ k 0 ( ε ) k\ge k_{0}(\varepsilon) k ≥ k 0 ( ε ) ,
∫ G k d π k ≥ m ^ − ε − δ ε N − δ θ N X k . ( 3 b ) \int G_{k}\,d\pi_{k}\ge\hat{m}-\varepsilon-\delta\varepsilon_{N}-\delta\theta_{N}X_{k}.\qquad(3\mathrm{b}) ∫ G k d π k ≥ m ^ − ε − δ ε N − δ θ N X k . ( 3 b )
By Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §regularised (i) and (F4), G k ≤ λ − 1 b g + ∣ e ∗ ∣ + ∥ q ∥ μ ^ 2 − δ P N / N G_{k}\le\lambda^{-1}b_{g}+|e_{*}|+\lVert q\rVert_{\hat{\mu}}^{2}-\delta P_{N}/N G k ≤ λ − 1 b g + ∣ e ∗ ∣ + ∥ q ∥ μ ^ 2 − δ P N / N on W N W_{N} W N , so
∫ G k d π k ≤ λ − 1 b g + ∣ e ∗ ∣ + ∥ q ∥ μ ^ 2 − δ X k . ( 3 c ) \int G_{k}\,d\pi_{k}\le\lambda^{-1}b_{g}+|e_{*}|+\lVert q\rVert_{\hat{\mu}}^{2}-\delta X_{k}.\qquad(3\mathrm{c}) ∫ G k d π k ≤ λ − 1 b g + ∣ e ∗ ∣ + ∥ q ∥ μ ^ 2 − δ X k . ( 3 c )
Energy bound. Let C 1 = 2 λ − 1 b g + ∣ e ∗ ∣ + ∣ E ( μ ^ ) ∣ + ∥ q ∥ μ ^ 2 C_{1}=2\lambda^{-1}b_{g}+|e_{*}|+|\mathcal{E}(\hat{\mu})|+\lVert q\rVert_{\hat{\mu}}^{2} C 1 = 2 λ − 1 b g + ∣ e ∗ ∣ + ∣ E ( μ ^ ) ∣ + ∥ q ∥ μ ^ 2 , so E 1 = δ − 1 ( C 1 + 2 ) E_{1}=\delta^{-1}(C_{1}+2) E 1 = δ − 1 ( C 1 + 2 ) . Take ε = 1 2 \varepsilon=\frac12 ε = 2 1 in (3b) and k 0 ≥ k 0 ( 1 2 ) k_{0}\ge k_{0}(\frac12) k 0 ≥ k 0 ( 2 1 ) with ε N ≤ 1 2 \varepsilon_{N}\le\frac12 ε N ≤ 2 1 and θ N ( C 1 + 2 ) ≤ 1 \theta_{N}(C_{1}+2)\le1 θ N ( C 1 + 2 ) ≤ 1 for k ≥ k 0 k\ge k_{0} k ≥ k 0 . For such k k k , (3b), (3c), − m ^ ≤ λ − 1 b g + ∣ E ( μ ^ ) ∣ -\hat{m}\le\lambda^{-1}b_{g}+|\mathcal{E}(\hat{\mu})| − m ^ ≤ λ − 1 b g + ∣ E ( μ ^ ) ∣ and δ < 1 \delta<1 δ < 1 give δ X k ≤ C 1 + 1 + δ θ N X k \delta X_{k}\le C_{1}+1+\delta\theta_{N}X_{k} δ X k ≤ C 1 + 1 + δ θ N X k . If X k ≤ 0 X_{k}\le0 X k ≤ 0 then X k ≤ E 1 X_{k}\le E_{1} X k ≤ E 1 ; otherwise δ X k ≤ ( C 1 + 1 ) / ( 1 − θ N ) ≤ C 1 + 2 \delta X_{k}\le(C_{1}+1)/(1-\theta_{N})\le C_{1}+2 δ X k ≤ ( C 1 + 1 ) / ( 1 − θ N ) ≤ C 1 + 2 , as θ N ( C 1 + 2 ) ≤ 1 \theta_{N}(C_{1}+2)\le1 θ N ( C 1 + 2 ) ≤ 1 . So X k ≤ E 1 X_{k}\le E_{1} X k ≤ E 1 .
Fisher bound. Let ∇ f k \nabla f_{k} ∇ f k be a gradient map of f k f_{k} f k (Gibbs Maximisers of the Relative Free Energy: the Variational Principle and the Relative Score §score ) with null set N ′ N' N ′ . Since π k \pi_{k} π k has a density with respect to Lebesgue measure, π k ( N ′ ) = 0 \pi_{k}(N')=0 π k ( N ′ ) = 0 ; and π k ( W N ) = 1 \pi_{k}(W_{N})=1 π k ( W N ) = 1 . For x ∈ W N ∖ N ′ x\in W_{N}\setminus N' x ∈ W N ∖ N ′ , by Step 1, (iii) of Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §regularised and (F3),
1 N ∥ ∇ f k ( x ) ∥ 2 ≤ 2 δ 2 ( 2 ∥ q ∥ μ ^ 2 + 8 K 2 W ( x ) 2 + 2 τ ( 2 λ − 1 b g + P N ( x ) − p 0 N 2 ) ) . \frac1N\lVert\nabla f_{k}(x)\rVert^{2}\le\frac{2}{\delta^{2}}\Bigl(2\lVert q\rVert_{\hat{\mu}}^{2}+8K^{2}W(x)^{2}+\frac{2}{\tau}\Bigl(2\lambda^{-1}b_{g}+\frac{P_{N}(x)-p_{0}}{N^{2}}\Bigr)\Bigr). N 1 ∥ ∇ f k ( x ) ∥ 2 ≤ δ 2 2 ( 2 ∥ q ∥ μ ^ 2 + 8 K 2 W ( x ) 2 + τ 2 ( 2 λ − 1 b g + N 2 P N ( x ) − p 0 ) ) .
Integrating against π k \pi_{k} π k , with ∥ Σ N ( π k ) ∥ π k 2 = ∫ ∥ ∇ f k ∥ 2 d π k \lVert\Sigma_{N}(\pi_{k})\rVert_{\pi_{k}}^{2}=\int\lVert\nabla f_{k}\rVert^{2}\,d\pi_{k} ∥ Σ N ( π k ) ∥ π k 2 = ∫ ∥ ∇ f k ∥ 2 d π k and 0 ≤ 1 N 2 ∫ ( P N − p 0 ) d π k ≤ X k − p 0 / N ≤ E 1 + ∣ e ∗ ∣ 0\le\frac1{N^{2}}\int(P_{N}-p_{0})\,d\pi_{k}\le X_{k}-p_{0}/N\le E_{1}+|e_{*}| 0 ≤ N 2 1 ∫ ( P N − p 0 ) d π k ≤ X k − p 0 / N ≤ E 1 + ∣ e ∗ ∣ (as N ≥ 1 N\ge1 N ≥ 1 , p 0 ≥ e ∗ N p_{0}\ge e_{*}N p 0 ≥ e ∗ N ), gives the Fisher bound, since 2 τ ( 2 λ − 1 b g + E 1 + ∣ e ∗ ∣ ) ≤ 4 τ ( λ − 1 b g + E 1 + ∣ e ∗ ∣ ) \frac2\tau(2\lambda^{-1}b_{g}+E_{1}+|e_{*}|)\le\frac4\tau(\lambda^{-1}b_{g}+E_{1}+|e_{*}|) τ 2 ( 2 λ − 1 b g + E 1 + ∣ e ∗ ∣ ) ≤ τ 4 ( λ − 1 b g + E 1 + ∣ e ∗ ∣ ) .
Step 4 (uniform upper estimate). Claim: for every positive ε \varepsilon ε there is k 0 k_{0} k 0 such that for every k ≥ k 0 k\ge k_{0} k ≥ k 0 and every x ∈ W N x\in W_{N} x ∈ W N
G k ( x ) ≤ m ^ + η ′ 2 2 K + ε − K 4 W ( x ) 2 . G_{k}(x)\le\hat{m}+\frac{\eta'^{2}}{2K}+\varepsilon-\frac K4W(x)^{2}. G k ( x ) ≤ m ^ + 2 K η ′ 2 + ε − 4 K W ( x ) 2 .
Suppose not. Then there are a positive ε \varepsilon ε , a strictly increasing sequence ( k l ) l (k_{l})_{l} ( k l ) l and x l ∈ W N k l x^{l}\in W_{N_{k_{l}}} x l ∈ W N k l violating the inequality at k = k l k=k_{l} k = k l ; write N = N k l N=N_{k_{l}} N = N k l and W l = W ( x l ) W_{l}=W(x^{l}) W l = W ( x l ) . By Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §regularised (i) and (F4), G k ( x ) ≤ λ − 1 b g + ∣ e ∗ ∣ + ∥ q ∥ μ ^ W ( x ) − K W ( x ) 2 − δ P N ( x ) / N G_{k}(x)\le\lambda^{-1}b_{g}+|e_{*}|+\lVert q\rVert_{\hat{\mu}}W(x)-KW(x)^{2}-\delta P_{N}(x)/N G k ( x ) ≤ λ − 1 b g + ∣ e ∗ ∣ + ∥ q ∥ μ ^ W ( x ) − K W ( x ) 2 − δ P N ( x ) / N , so the violation gives
δ P N ( x l ) N < λ − 1 b g + ∣ e ∗ ∣ + ∣ m ^ ∣ + ∥ q ∥ μ ^ W l − 3 K 4 W l 2 ≤ λ − 1 b g + ∣ e ∗ ∣ + ∣ m ^ ∣ + ∥ q ∥ μ ^ 2 3 K . \delta\frac{P_{N}(x^{l})}{N}<\lambda^{-1}b_{g}+|e_{*}|+|\hat{m}|+\lVert q\rVert_{\hat{\mu}}W_{l}-\frac{3K}{4}W_{l}^{2}\le\lambda^{-1}b_{g}+|e_{*}|+|\hat{m}|+\frac{\lVert q\rVert_{\hat{\mu}}^{2}}{3K}. δ N P N ( x l ) < λ − 1 b g + ∣ e ∗ ∣ + ∣ m ^ ∣ + ∥ q ∥ μ ^ W l − 4 3 K W l 2 ≤ λ − 1 b g + ∣ e ∗ ∣ + ∣ m ^ ∣ + 3 K ∥ q ∥ μ ^ 2 .
So P N k l ( x l ) ≤ c ′ ′ N k l P_{N_{k_{l}}}(x^{l})\le c''N_{k_{l}} P N k l ( x l ) ≤ c ′′ N k l for a constant c ′ ′ c'' c ′′ , and The Discrete Dyson Energy per Particle: Bounds, Compactness with a Lower Limit, and Recovery Configurations with Separated Particles §liminf gives a further strictly increasing subsequence, along which we continue to index by l l l , and ν ∈ D \nu\in\mathcal{D} ν ∈ D with W 2 ( μ x l N , ν ) → 0 W_{2}(\mu^{N}_{x^{l}},\nu)\to0 W 2 ( μ x l N , ν ) → 0 and, for every positive ε ′ ′ \varepsilon'' ε ′′ , E ( ν ) ≤ P N ( x l ) / N + ε ′ ′ \mathcal{E}(\nu)\le P_{N}(x^{l})/N+\varepsilon'' E ( ν ) ≤ P N ( x l ) / N + ε ′′ for large l l l . By Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §sequences (the levels N k l N_{k_{l}} N k l being strictly increasing and at least N 0 N_{0} N 0 ), w ( x l ) / N ≤ u ˉ τ ( ν ) + ε ′ ′ w(x^{l})/N\le\bar{u}_{\tau}(\nu)+\varepsilon'' w ( x l ) / N ≤ u ˉ τ ( ν ) + ε ′′ for large l l l . By On the Real Line an Atomless Source is Uniquely Mapped, by a Nondecreasing Optimal Map §monotone (μ ^ \hat{\mu} μ ^ atomless) there is an optimal map T T T from μ ^ \hat{\mu} μ ^ to ν \nu ν , Borel and nondecreasing on a Borel set of full μ ^ \hat{\mu} μ ^ -measure; Quantile Blocks of an Atomless Measure on the Line: Block Maps, Distances to Ordered Empirical Measures, and the Block Test Function §optimal gives ∥ T x l − T ∥ μ ^ = W 2 ( μ x l N , ν ) → 0 \lVert T_{x^{l}}-T\rVert_{\hat{\mu}}=W_{2}(\mu^{N}_{x^{l}},\nu)\to0 ∥ T x l − T ∥ μ ^ = W 2 ( μ x l N , ν ) → 0 . With (F4) and Step 1, W l = ∥ T x l − i d ∥ μ ^ → ∥ T − i d ∥ μ ^ = W ν : = W 2 ( ν , μ ^ ) W_{l}=\lVert T_{x^{l}}-\mathrm{id}\rVert_{\hat{\mu}}\to\lVert T-\mathrm{id}\rVert_{\hat{\mu}}=W_{\nu}:=W_{2}(\nu,\hat{\mu}) W l = ∥ T x l − id ∥ μ ^ → ∥ T − id ∥ μ ^ = W ν := W 2 ( ν , μ ^ ) and χ ( x l ) → ⟨ q , T − i d ⟩ μ ^ + K W ν 2 \chi(x^{l})\to\langle q,T-\mathrm{id}\rangle_{\hat{\mu}}+KW_{\nu}^{2} χ ( x l ) → ⟨ q , T − id ⟩ μ ^ + K W ν 2 . Letting l → ∞ l\to\infty l → ∞ in the violated inequality and then ε ′ ′ → 0 \varepsilon''\to0 ε ′′ → 0 ,
u ˉ τ ( ν ) − δ E ( ν ) − ⟨ q , T − i d ⟩ μ ^ − K W ν 2 ≥ m ^ + η ′ 2 2 K + ε − K 4 W ν 2 . ( 4 a ) \bar{u}_{\tau}(\nu)-\delta\mathcal{E}(\nu)-\langle q,T-\mathrm{id}\rangle_{\hat{\mu}}-KW_{\nu}^{2}\ge\hat{m}+\frac{\eta'^{2}}{2K}+\varepsilon-\frac K4W_{\nu}^{2}.\qquad(4\mathrm{a}) u ˉ τ ( ν ) − δ E ( ν ) − ⟨ q , T − id ⟩ μ ^ − K W ν 2 ≥ m ^ + 2 K η ′ 2 + ε − 4 K W ν 2 . ( 4 a )
If W ν < r 0 W_{\nu}<r_{0} W ν < r 0 , the hypothesis of clause 1 and η ′ W ν ≤ η ′ 2 2 K + K 2 W ν 2 \eta'W_{\nu}\le\frac{\eta'^{2}}{2K}+\frac K2W_{\nu}^{2} η ′ W ν ≤ 2 K η ′ 2 + 2 K W ν 2 bound the left side of (4a) by m ^ + η ′ 2 2 K − K 2 W ν 2 \hat{m}+\frac{\eta'^{2}}{2K}-\frac K2W_{\nu}^{2} m ^ + 2 K η ′ 2 − 2 K W ν 2 , whence ε ≤ − K 4 W ν 2 ≤ 0 \varepsilon\le-\frac K4W_{\nu}^{2}\le0 ε ≤ − 4 K W ν 2 ≤ 0 , a contradiction. If W ν ≥ r 0 W_{\nu}\ge r_{0} W ν ≥ r 0 , then u ˉ τ ( ν ) ≤ λ − 1 b g \bar{u}_{\tau}(\nu)\le\lambda^{-1}b_{g} u ˉ τ ( ν ) ≤ λ − 1 b g (Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §bounds ), − δ E ( ν ) ≤ ∣ e 0 ∣ -\delta\mathcal{E}(\nu)\le|e_{0}| − δ E ( ν ) ≤ ∣ e 0 ∣ , and − ⟨ q , T − i d ⟩ μ ^ ≤ ∥ q ∥ μ ^ W ν ≤ K 4 W ν 2 + ∥ q ∥ μ ^ 2 K -\langle q,T-\mathrm{id}\rangle_{\hat{\mu}}\le\lVert q\rVert_{\hat{\mu}}W_{\nu}\le\frac K4W_{\nu}^{2}+\frac{\lVert q\rVert_{\hat{\mu}}^{2}}{K} − ⟨ q , T − id ⟩ μ ^ ≤ ∥ q ∥ μ ^ W ν ≤ 4 K W ν 2 + K ∥ q ∥ μ ^ 2 ; with − m ^ ≤ λ − 1 b g + ∣ E ( μ ^ ) ∣ -\hat{m}\le\lambda^{-1}b_{g}+|\mathcal{E}(\hat{\mu})| − m ^ ≤ λ − 1 b g + ∣ E ( μ ^ ) ∣ and K ≥ 1 K\ge1 K ≥ 1 , (4a) gives ε ≤ S − K 2 W ν 2 ≤ S − K 2 r 0 2 ≤ 0 \varepsilon\le S-\frac K2W_{\nu}^{2}\le S-\frac K2r_{0}^{2}\le0 ε ≤ S − 2 K W ν 2 ≤ S − 2 K r 0 2 ≤ 0 , where S = 2 λ − 1 b g + ∣ e 0 ∣ + ∣ E ( μ ^ ) ∣ + ∥ q ∥ μ ^ 2 S=2\lambda^{-1}b_{g}+|e_{0}|+|\mathcal{E}(\hat{\mu})|+\lVert q\rVert_{\hat{\mu}}^{2} S = 2 λ − 1 b g + ∣ e 0 ∣ + ∣ E ( μ ^ ) ∣ + ∥ q ∥ μ ^ 2 and K r 0 2 ≥ 2 S Kr_{0}^{2}\ge2S K r 0 2 ≥ 2 S by hypothesis; a contradiction.
Step 5 (clause (c)). Let ε > 0 \varepsilon>0 ε > 0 and ε ′ = ε / 12 \varepsilon'=\varepsilon/12 ε ′ = ε /12 . Choose, in this order, k 0 k_{0} k 0 from Step 4 for ε ′ \varepsilon' ε ′ , then k 0 ′ ≥ k 0 k_{0}'\ge k_{0} k 0 ′ ≥ k 0 at least k 0 ( ε ′ ) k_{0}(\varepsilon') k 0 ( ε ′ ) of (3b) and the k 0 k_{0} k 0 of the energy bound, and such that ε N + θ N E 1 ≤ ε ′ \varepsilon_{N}+\theta_{N}E_{1}\le\varepsilon' ε N + θ N E 1 ≤ ε ′ for k ≥ k 0 ′ k\ge k_{0}' k ≥ k 0 ′ . For k ≥ k 0 ′ k\ge k_{0}' k ≥ k 0 ′ , (3b) with X k ≤ E 1 X_{k}\le E_{1} X k ≤ E 1 gives ∫ G k d π k ≥ m ^ − 2 ε ′ \int G_{k}\,d\pi_{k}\ge\hat{m}-2\varepsilon' ∫ G k d π k ≥ m ^ − 2 ε ′ , while integrating Step 4 against π k \pi_{k} π k (all terms are integrable, W 2 W^{2} W 2 being a polynomial on W N W_{N} W N by (F4)) gives ∫ G k d π k ≤ m ^ + η ′ 2 2 K + ε ′ − K 4 ∫ W 2 d π k \int G_{k}\,d\pi_{k}\le\hat{m}+\frac{\eta'^{2}}{2K}+\varepsilon'-\frac K4\int W^{2}\,d\pi_{k} ∫ G k d π k ≤ m ^ + 2 K η ′ 2 + ε ′ − 4 K ∫ W 2 d π k . Hence K ∫ W 2 d π k ≤ 2 η ′ 2 K + 12 ε ′ = 2 η ′ 2 K + ε K\int W^{2}\,d\pi_{k}\le\frac{2\eta'^{2}}{K}+12\varepsilon'=\frac{2\eta'^{2}}{K}+\varepsilon K ∫ W 2 d π k ≤ K 2 η ′ 2 + 12 ε ′ = K 2 η ′ 2 + ε .
Clause 2 (supersolution side). The proof is the same with the following changes. w = w ‾ N , τ w=\underline{w}_{N,\tau} w = w N , τ , χ = χ N − \chi=\chi^{-}_{N} χ = χ N − (data ( q , − K ) (q,-K) ( q , − K ) ), f k = δ − 1 ( N χ − w ) f_{k}=\delta^{-1}(N\chi-w) f k = δ − 1 ( N χ − w ) , m ^ = − ( u ‾ τ ( μ ^ ) + δ E ( μ ^ ) ) \hat{m}=-(\underline{u}_{\tau}(\hat{\mu})+\delta\mathcal{E}(\hat{\mu})) m ^ = − ( u τ ( μ ^ ) + δ E ( μ ^ )) , G k = − w / N + χ − δ P N / N G_{k}=-w/N+\chi-\delta P_{N}/N G k = − w / N + χ − δ P N / N and Φ k ( P ) = ∫ ( N χ − w ) d P − δ E N ( P ) \Phi_{k}(P)=\int(N\chi-w)\,dP-\delta\mathcal{E}_{N}(P) Φ k ( P ) = ∫ ( N χ − w ) d P − δ E N ( P ) , so that (0) holds and maximising Φ k \Phi_{k} Φ k is minimising ∫ ( w − N χ ) d P + δ E N ( P ) \int(w-N\chi)\,dP+\delta\mathcal{E}_{N}(P) ∫ ( w − N χ ) d P + δ E N ( P ) ; ∣ m ^ ∣ ≤ λ − 1 b g + ∣ E ( μ ^ ) ∣ |\hat{m}|\le\lambda^{-1}b_{g}+|\mathcal{E}(\hat{\mu})| ∣ m ^ ∣ ≤ λ − 1 b g + ∣ E ( μ ^ ) ∣ by Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §bounds . In (F1), N χ ( x ) = − K ∥ x ∥ 2 + ∑ i ( q ˉ i + 2 K m i ) x i + c χ N\chi(x)=-K\lVert x\rVert^{2}+\sum_{i}(\bar{q}_{i}+2Km_{i})x_{i}+c_{\chi} N χ ( x ) = − K ∥ x ∥ 2 + ∑ i ( q ˉ i + 2 K m i ) x i + c χ ; in (F3), q ˉ i − 2 K ( x i − m i ) \bar{q}_{i}-2K(x_{i}-m_{i}) q ˉ i − 2 K ( x i − m i ) replaces q ˉ i + 2 K ( x i − m i ) \bar{q}_{i}+2K(x_{i}-m_{i}) q ˉ i + 2 K ( x i − m i ) , with the same bound; in (F4), χ ( x ) = ⟨ q , T x − i d ⟩ μ ^ − K W ( x ) 2 \chi(x)=\langle q,T_{x}-\mathrm{id}\rangle_{\hat{\mu}}-KW(x)^{2} χ ( x ) = ⟨ q , T x − id ⟩ μ ^ − K W ( x ) 2 , so − ∥ q ∥ μ ^ W − K W 2 ≤ χ ≤ ∥ q ∥ μ ^ W − K W 2 ≤ ∥ q ∥ μ ^ 2 -\lVert q\rVert_{\hat{\mu}}W-KW^{2}\le\chi\le\lVert q\rVert_{\hat{\mu}}W-KW^{2}\le\lVert q\rVert_{\hat{\mu}}^{2} − ∥ q ∥ μ ^ W − K W 2 ≤ χ ≤ ∥ q ∥ μ ^ W − K W 2 ≤ ∥ q ∥ μ ^ 2 . Step 1: − w -w − w is semiconvex with constant τ − 1 \tau^{-1} τ − 1 and − w ≤ λ − 1 N b g + ∣ e ∗ ∣ -w\le\lambda^{-1}Nb_{g}+|e_{*}| − w ≤ λ − 1 N b g + ∣ e ∗ ∣ (Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §regularised (ii), (i)), N χ + K ∥ x ∥ 2 N\chi+K\lVert x\rVert^{2} N χ + K ∥ x ∥ 2 is affine, N χ ≤ N ∥ q ∥ μ ^ 2 N\chi\le N\lVert q\rVert_{\hat{\mu}}^{2} N χ ≤ N ∥ q ∥ μ ^ 2 on W N W_{N} W N , and (iii) applies to w ‾ N , τ \underline{w}_{N,\tau} w N , τ ; clause (a) becomes δ − 1 ( N ∇ χ − ∇ w ) = Σ N ( π k ) \delta^{-1}(N\nabla\chi-\nabla w)=\Sigma_{N}(\pi_{k}) δ − 1 ( N ∇ χ − ∇ w ) = Σ N ( π k ) , that is, ∇ w = N ∇ χ − δ Σ N ( π k ) \nabla w=N\nabla\chi-\delta\Sigma_{N}(\pi_{k}) ∇ w = N ∇ χ − δ Σ N ( π k ) . Step 2: the levels are realising for u ‾ τ \underline{u}_{\tau} u τ , so w ( y k ) / N k → u ‾ τ ( μ ^ ) w(y^{k})/N_{k}\to\underline{u}_{\tau}(\hat{\mu}) w ( y k ) / N k → u τ ( μ ^ ) by the second part of Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §realising ; (2b) uses the second inequality of (iv), w ( y ) ≥ w ( z ) − 1 2 τ ∥ y − z ∥ ( 3 ∥ y − z ∥ + 2 r N ( z ) ) w(y)\ge w(z)-\frac{1}{2\tau}\lVert y-z\rVert(3\lVert y-z\rVert+2r_{N}(z)) w ( y ) ≥ w ( z ) − 2 τ 1 ∥ y − z ∥ ( 3 ∥ y − z ∥ + 2 r N ( z )) , giving − w ( z ) / N ≥ − w ( y ) / N − ( 3 + 2 ρ ) h / ( 2 τ ) -w(z)/N\ge-w(y)/N-(3+2\rho)h/(2\tau) − w ( z ) / N ≥ − w ( y ) / N − ( 3 + 2 ρ ) h / ( 2 τ ) ; (2c) becomes χ ( z ) ≥ χ ( y ) − ∥ q ∥ μ ^ h − K h ( 2 W ( y ) + h ) \chi(z)\ge\chi(y)-\lVert q\rVert_{\hat{\mu}}h-Kh(2W(y)+h) χ ( z ) ≥ χ ( y ) − ∥ q ∥ μ ^ h − K h ( 2 W ( y ) + h ) and χ ( y ) ≥ − ∥ q ∥ μ ^ W ( y ) − K W ( y ) 2 \chi(y)\ge-\lVert q\rVert_{\hat{\mu}}W(y)-KW(y)^{2} χ ( y ) ≥ − ∥ q ∥ μ ^ W ( y ) − K W ( y ) 2 ; the lower bound for Φ k ( π k ) / N \Phi_{k}(\pi_{k})/N Φ k ( π k ) / N tends to − u ‾ τ ( μ ^ ) − δ E ( μ ^ ) = m ^ -\underline{u}_{\tau}(\hat{\mu})-\delta\mathcal{E}(\hat{\mu})=\hat{m} − u τ ( μ ^ ) − δ E ( μ ^ ) = m ^ . Step 3 is unchanged, (3c) following from − w / N ≤ λ − 1 b g + ∣ e ∗ ∣ -w/N\le\lambda^{-1}b_{g}+|e_{*}| − w / N ≤ λ − 1 b g + ∣ e ∗ ∣ and χ ≤ ∥ q ∥ μ ^ 2 \chi\le\lVert q\rVert_{\hat{\mu}}^{2} χ ≤ ∥ q ∥ μ ^ 2 . Step 4: G k ( x ) ≤ λ − 1 b g + ∣ e ∗ ∣ + ∥ q ∥ μ ^ W ( x ) − K W ( x ) 2 − δ P N ( x ) / N G_{k}(x)\le\lambda^{-1}b_{g}+|e_{*}|+\lVert q\rVert_{\hat{\mu}}W(x)-KW(x)^{2}-\delta P_{N}(x)/N G k ( x ) ≤ λ − 1 b g + ∣ e ∗ ∣ + ∥ q ∥ μ ^ W ( x ) − K W ( x ) 2 − δ P N ( x ) / N as before; the first inequality of Half-Relaxed Limits of the Sup- and Inf-Convolved N-Particle Dyson Solutions: Bounds, Continuity and Limits along Configurations of Bounded Energy §sequences gives − w ( x l ) / N ≤ − u ‾ τ ( ν ) + ε ′ ′ -w(x^{l})/N\le-\underline{u}_{\tau}(\nu)+\varepsilon'' − w ( x l ) / N ≤ − u τ ( ν ) + ε ′′ for large l l l ; χ ( x l ) → ⟨ q , T − i d ⟩ μ ^ − K W ν 2 \chi(x^{l})\to\langle q,T-\mathrm{id}\rangle_{\hat{\mu}}-KW_{\nu}^{2} χ ( x l ) → ⟨ q , T − id ⟩ μ ^ − K W ν 2 ; and (4a) reads − u ‾ τ ( ν ) − δ E ( ν ) + ⟨ q , T − i d ⟩ μ ^ − K W ν 2 ≥ m ^ + η ′ 2 2 K + ε − K 4 W ν 2 -\underline{u}_{\tau}(\nu)-\delta\mathcal{E}(\nu)+\langle q,T-\mathrm{id}\rangle_{\hat{\mu}}-KW_{\nu}^{2}\ge\hat{m}+\frac{\eta'^{2}}{2K}+\varepsilon-\frac K4W_{\nu}^{2} − u τ ( ν ) − δ E ( ν ) + ⟨ q , T − id ⟩ μ ^ − K W ν 2 ≥ m ^ + 2 K η ′ 2 + ε − 4 K W ν 2 . If W ν < r 0 W_{\nu}<r_{0} W ν < r 0 , the hypothesis of clause 2 gives − u ‾ τ ( ν ) − δ E ( ν ) + ⟨ q , T − i d ⟩ μ ^ ≤ m ^ + η ′ W ν -\underline{u}_{\tau}(\nu)-\delta\mathcal{E}(\nu)+\langle q,T-\mathrm{id}\rangle_{\hat{\mu}}\le\hat{m}+\eta'W_{\nu} − u τ ( ν ) − δ E ( ν ) + ⟨ q , T − id ⟩ μ ^ ≤ m ^ + η ′ W ν , and if W ν ≥ r 0 W_{\nu}\ge r_{0} W ν ≥ r 0 one uses − u ‾ τ ( ν ) ≤ λ − 1 b g -\underline{u}_{\tau}(\nu)\le\lambda^{-1}b_{g} − u τ ( ν ) ≤ λ − 1 b g , − δ E ( ν ) ≤ ∣ e 0 ∣ -\delta\mathcal{E}(\nu)\le|e_{0}| − δ E ( ν ) ≤ ∣ e 0 ∣ and ⟨ q , T − i d ⟩ μ ^ ≤ ∥ q ∥ μ ^ W ν \langle q,T-\mathrm{id}\rangle_{\hat{\mu}}\le\lVert q\rVert_{\hat{\mu}}W_{\nu} ⟨ q , T − id ⟩ μ ^ ≤ ∥ q ∥ μ ^ W ν ; the contradictions follow verbatim. Step 5 is unchanged.