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Proof of Gibbs Maximisers for the Regularised N-Particle Dyson Solutions Tested at a Local Extremum: Energy Bound, Concentration and the Score Identity

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· 22,719 chars · 19 deps · depth 48 Reason: Proof of energy bound, Fisher bound and concentration of the localised Gibbs maximisers.

The Gibbs measure of the tilted regularised solution is compared with the uniform law on a small cube around a separated recovery configuration, which gives a lower bound on its value; a compactness argument gives a uniform quadratic upper bound on the integrand, and together with the Gaussian lower bound for the entropy these yield the energy and Fisher bounds and the concentration.

Proof

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 N1≥N0≥2N_{1}\ge N_{0}\ge2, so Nk→∞N_{k}\to\infty. For a fixed kk we write N=NkN=N_{k}, w=w‾N,τw=\overline{w}_{N,\tau}, χ=χN+\chi=\chi^{+}_{N}, p0=p0,Np_{0}=p_{0,N}, W(x)=W2(μxN,μ^)W(x)=W_{2}(\mu^{N}_{x},\hat{\mu}), ∥⋅∥\lVert\cdot\rVert for the Euclidean norm of RN\mathbb{R}^{N} and ∥⋅∥μ^\lVert\cdot\rVert_{\hat{\mu}}, ⟨⋅,⋅⟩μ^\langle\cdot,\cdot\rangle_{\hat{\mu}} for those of L2(μ^;R)L^{2}(\hat{\mu};\mathbb{R}); BiB_{i}, TxT_{x}, qˉi\bar{q}_{i}, mim_{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^=uˉτ(μ^)−δE(μ^),Gk(x)=w(x)N−χ(x)−δPN(x)N(x∈WN),\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}),

and, for P∈DNP\in\mathcal{D}_{N} such that w−Nχw-N\chi is PP-integrable (integrals of functions on WNW_{N} are over WNW_{N}, which has full PP-measure), Φk(P)=∫(w−Nχ) dP−δ EN(P)=δ(∫fˉk dP−EN(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), with fˉk\bar{f}_{k} equal to fkf_{k} on WNW_{N} and to 00 off it. Since EN(P)=aNEnt(P)+∫PN dP\mathcal{E}_{N}(P)=a_{N}\mathrm{Ent}(P)+\int P_{N}\,dP by The Relative Free Energy and the Relative Score of a Probability Measure for a Potential on an Open Set §energy,

Φk(P)N=∫Gk dP−δ aNN Ent(P).(0)\frac{\Phi_{k}(P)}{N}=\int G_{k}\,dP-\delta\,\frac{a_{N}}{N}\,\mathrm{Ent}(P).\qquad(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<10<\delta<1, ∣m^∣≤λ−1bg+∣E(μ^)∣|\hat{m}|\le\lambda^{-1}b_{g}+|\mathcal{E}(\hat{\mu})|. Let e∗,A0e_{*},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≤PNe_{*}N\le P_{N} on WNW_{N}, hence e∗N≤p0e_{*}N\le 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^(Bi)=1N\hat{\mu}(B_{i})=\frac1N (Quantile Blocks of an Atomless Measure on the Line: Block Maps, Distances to Ordered Empirical Measures, and the Block Test Function §blocks) gives Nχ(x)=K∥x∥2+∑i(qˉi−2Kmi)xi+cχN\chi(x)=K\lVert x\rVert^{2}+\sum_{i}(\bar{q}_{i}-2Km_{i})x_{i}+c_{\chi} for a real cχc_{\chi}. (F2) By Cauchy-Schwarz on each block, qˉi2≤N∫Biq2 dμ^\bar{q}_{i}^{2}\le N\int_{B_{i}}q^{2}\,d\hat{\mu} and (xi−mi)2=(N∫Bi(xi−s) μ^(ds))2≤N∫Bi(xi−s)2 μ^(ds)(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); 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 xx, ∑iqˉi2≤N∥q∥μ^2\sum_{i}\bar{q}_{i}^{2}\le N\lVert q\rVert_{\hat{\mu}}^{2} and ∑i(xi−mi)2≤NW(x)2\sum_{i}(x_{i}-m_{i})^{2}\le NW(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 xx

∥N∇χ(x)∥2=∑i(qˉi+2K(xi−mi))2≤2N∥q∥μ^2+8K2N W(x)2.(F3)\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)

(F4) For ordered xx (in particular x∈WNx\in 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} and T=idT=\mathrm{id} gives W(x)=∥Tx−id∥μ^W(x)=\lVert T_{x}-\mathrm{id}\rVert_{\hat{\mu}}, and W(x)2=∑i∫Bi(xi−s)2 μ^(ds)W(x)^{2}=\sum_{i}\int_{B_{i}}(x_{i}-s)^{2}\,\hat{\mu}(ds) is a polynomial in xx; 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,Tx−id⟩μ^+KW(x)2\chi(x)=\langle q,T_{x}-\mathrm{id}\rangle_{\hat{\mu}}+KW(x)^{2}, so −∥q∥μ^W(x)+KW(x)2≤χ(x)≤∥q∥μ^W(x)+KW(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} and χ(x)≥−∥q∥μ^2/(4K)≥−∥q∥μ^2\chi(x)\ge-\lVert q\rVert_{\hat{\mu}}^{2}/(4K)\ge-\lVert q\rVert_{\hat{\mu}}^{2} (as K≥1K\ge1). Also NW(x)2≤2∥x∥2+2NM2(μ^)NW(x)^{2}\le2\lVert x\rVert^{2}+2NM_{2}(\hat{\mu}).

Step 1 (hypotheses; optimal maps; clause (a)). WNW_{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). PNP_{N} is a penalty on WNW_{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=PNU=P_{N}, a=aNa=a_{N} is the function gNg_{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 Rn\mathbb{R}^n, w+12τ∥x∥2w+\frac{1}{2\tau}\lVert x\rVert^{2} is convex on WNW_{N}; by (F1), −Nχ+K∥x∥2-N\chi+K\lVert x\rVert^{2} is affine; so fk+12δ−1(τ−1+2K)∥x∥2=δ−1[(w+12τ∥x∥2)+(−Nχ+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] is convex, and fkf_{k} is semiconvex on WNW_{N} with constant δ−1(τ−1+2K)\delta^{-1}(\tau^{-1}+2K). 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), fk≤δ−1(λ−1Nbg+∣e∗∣+N∥q∥μ^2)f_{k}\le\delta^{-1}(\lambda^{-1}Nb_{g}+|e_{*}|+N\lVert q\rVert_{\hat{\mu}}^{2}) on WNW_{N}. Since χ\chi is C2C^{2}, fkf_{k} is differentiable at x∈WNx\in W_{N} exactly when ww is, and then Dfk(x)=δ−1(Dw(x)−N∇χ(x))Df_{k}(x)=\delta^{-1}(Dw(x)-N\nabla\chi(x)). At such xx, 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 ∥Dw(x)∥2≤τ−2rN(x)2=2τ(2λ−1Nbg+PN(x)−p0N)\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), 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≤2N∥q∥μ^2+8K2(2A0(N+p0−e∗N)+2A0(PN(x)−p0)+2NM2(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). Hence ∥Dfk(x)∥2≤2δ−2(∥Dw(x)∥2+∥N∇χ(x)∥2)≤A+B(PN(x)−p0)\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}) for nonnegative A,BA,B depending on kk. All hypotheses of Gibbs Maximisers of the Relative Free Energy: the Variational Principle and the Relative Score hold, so πk\pi_{k} is defined, πk∈DN\pi_{k}\in\mathcal{D}_{N}, πk(WN)=1\pi_{k}(W_{N})=1 and Φk(πk)=δaNlog⁡Z\Phi_{k}(\pi_{k})=\delta a_{N}\log Z (Gibbs Maximisers of the Relative Free Energy: the Variational Principle and the Relative Score §gibbs), and Φk(P)≤δaNlog⁡Z=Φk(πk)\Phi_{k}(P)\le\delta a_{N}\log Z=\Phi_{k}(\pi_{k}) for every admissible PP (Gibbs Maximisers of the Relative Free Energy: the Variational Principle and the Relative Score §variational, multiplied by δ\delta). Moreover GkG_{k} is πk\pi_{k}-integrable: ww 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 is a polynomial of degree at most 22 and πk∈P2(RN)\pi_{k}\in\mathcal{P}_{2}(\mathbb{R}^{N}), and PNP_{N} is πk\pi_{k}-integrable as πk∈DN\pi_{k}\in\mathcal{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∈P2(R)\nu\in\mathcal{P}_{2}(\mathbb{R}) and let TT be an optimal map from μ^\hat{\mu} to ν\nu. By the change-of-variables formula of Probability Measures on Euclidean Space and Random Vectors: Standing Notation §pushforward, ∫T2 dμ^=∫t2 ν(dt)<∞\int T^{2}\,d\hat{\mu}=\int t^{2}\,\nu(dt)<\infty, so the class of TT lies in L2(μ^;R)L^{2}(\hat{\mu};\mathbb{R}), and the quadratic cost of (id,T)#μ^(\mathrm{id},T)_{\#}\hat{\mu} is ∫∣s−T(s)∣2 μ^(ds)=∥T−id∥μ^2\int|s-T(s)|^{2}\,\hat{\mu}(ds)=\lVert T-\mathrm{id}\rVert_{\hat{\mu}}^{2}; this coupling being optimal, ∥T−id∥μ^=W2(μ^,ν)=W2(ν,μ^)\lVert T-\mathrm{id}\rVert_{\hat{\mu}}=W_{2}(\hat{\mu},\nu)=W_{2}(\nu,\hat{\mu}).

Clause (a). By Gibbs Maximisers of the Relative Free Energy: the Variational Principle and the Relative Score §score, πk∈DNΣ\pi_{k}\in\mathcal{D}^{\Sigma}_{N} and ΣN(πk)=∇fk\Sigma_{N}(\pi_{k})=\nabla f_{k} in L2(πk;RN)L^{2}(\pi_{k};\mathbb{R}^{N}) for every gradient map ∇fk\nabla f_{k} of fkf_{k}. Let ∇w\nabla w be a gradient map of ww (Gradient Maps of a Function on an Open Subset of Euclidean Space §gradient-map), with null set N′N'. The map δ−1(∇w−N∇χ)\delta^{-1}(\nabla w-N\nabla\chi) is Borel (∇χ\nabla\chi being continuous), and at every x∈WN∖N′x\in W_{N}\setminus N' the function ww, hence fkf_{k}, is differentiable with Dfk(x)=δ−1(∇w(x)−N∇χ(x))Df_{k}(x)=\delta^{-1}(\nabla w(x)-N\nabla\chi(x)); so it is a gradient map of fkf_{k}, and δ−1(∇w−N∇χ)=ΣN(πk)\delta^{-1}(\nabla w-N\nabla\chi)=\Sigma_{N}(\pi_{k}) in L2(πk;RN)L^{2}(\pi_{k};\mathbb{R}^{N}). As N∇χN\nabla\chi is affine and πk∈P2(RN)\pi_{k}\in\mathcal{P}_{2}(\mathbb{R}^{N}), its class lies in L2(πk;RN)L^{2}(\pi_{k};\mathbb{R}^{N}), hence so does that of ∇w=N∇χ+δ∇fk\nabla w=N\nabla\chi+\delta\nabla f_{k}, and ∇w=N∇χ+δΣN(πk)\nabla w=N\nabla\chi+\delta\Sigma_{N}(\pi_{k}) there.

Step 2 (value lower bound). Claim: for every positive ε\varepsilon there is k0k_{0} with Φk(πk)/N≥m^−ε\Phi_{k}(\pi_{k})/N\ge\hat{m}-\varepsilon for every k≥k0k\ge k_{0}.

Diagonal choice. For each natural j≥1j\ge1, The Discrete Dyson Energy per Particle: Bounds, Compactness with a Lower Limit, and Recovery Configurations with Separated Particles §recovery applied to μ^\hat{\mu} and 1/j1/j gives positive cj,Rjc_{j},R_{j} and N1(j)≥2N_{1}(j)\ge2; replacing cjc_{j} by min⁡(cj,1)\min(c_{j},1) keeps its gap condition, so we assume cj≤1c_{j}\le1. Let LjL_{j} be the maximum of ∣V′∣|V'| on [−Rj−1,Rj+1][-R_{j}-1,R_{j}+1] (V′V' is continuous, VV being C2C^{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 Λj=log⁡(1/cj)+Lj≥0\Lambda_{j}=\log(1/c_{j})+L_{j}\ge0. For each kk let SkS_{k} be the set of j∈[k]j\in[k] with Nk≥N1(i)N_{k}\ge N_{1}(i) and Nk≥i(1+Λi)N_{k}\ge i(1+\Lambda_{i}) for every i∈[j]i\in[j]. Since Nk→∞N_{k}\to\infty, each jj lies in SkS_{k} for all large kk; let k1k_{1} be such that 1∈Sk1\in S_{k} for k≥k1k\ge k_{1}, and put j(k)=max⁡Skj(k)=\max S_{k} for k≥k1k\ge k_{1}. Then j(k)→∞j(k)\to\infty, Nk≥N1(j(k))N_{k}\ge N_{1}(j(k)) and Λj(k)≤Nk/j(k)\Lambda_{j(k)}\le N_{k}/j(k). For k≥k1k\ge k_{1} let yk∈WNky^{k}\in 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) and N=NkN=N_{k}, and for k<k1k<k_{1} any point of WNkW_{N_{k}}. Then W(yk)<1/j(k)→0W(y^{k})<1/j(k)\to0 and PNk(yk)≤c′NkP_{N_{k}}(y^{k})\le c'N_{k} for all kk, with c′c' the largest of E(μ^)+1\mathcal{E}(\hat{\mu})+1 and the finitely many PNk(yk)/NkP_{N_{k}}(y^{k})/N_{k}, k<k1k<k_{1}; so w(yk)/Nk→uˉτ(μ^)w(y^{k})/N_{k}\to\bar{u}_{\tau}(\hat{\mu}) 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≥k1k\ge k_{1} and write j=j(k)j=j(k), c=cjc=c_{j}, L=LjL=L_{j}, Λ=Λj\Lambda=\Lambda_{j}, y=yky=y^{k}, h=c/(4N)≤1/(4N)h=c/(4N)\le1/(4N) and Q={z∈RN:∣zi−yi∣≤h for every i}Q=\{z\in\mathbb{R}^{N}:|z_{i}-y_{i}|\le h\text{ for every }i\}. For i<li<l, summing gaps, yi−yl≥(l−i)c/N≥4hy_{i}-y_{l}\ge(l-i)c/N\ge4h, so for z∈Qz\in Q, zi−zl≥yi−yl−2h≥12(yi−yl)>0z_{i}-z_{l}\ge y_{i}-y_{l}-2h\ge\frac12(y_{i}-y_{l})>0; thus Q⊆WNQ\subseteq W_{N}. Also ∥z−y∥≤hN\lVert z-y\rVert\le h\sqrt{N} for z∈Qz\in Q.

(2a) Energy on QQ. Let z∈Qz\in Q and i<li<l; with t=(zi−zl)/(yi−yl)t=(z_{i}-z_{l})/(y_{i}-y_{l}) and u=2h/(yi−yl)≤12u=2h/(y_{i}-y_{l})\le\frac12 we have t≥1−ut\ge1-u, and 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, −log⁡t≤t−1−1≤u/(1−u)≤2u=4h/(yi−yl)≤1/(l−i)-\log t\le t^{-1}-1\le u/(1-u)\le2u=4h/(y_{i}-y_{l})\le1/(l-i). By The Logarithmic Energy of N Ordered Particles on the Weyl Chamber §energy with strength bN=β/(2(N−1))b_{N}=\beta/(2(N-1)),

HbN(z)−HbN(y)=−bN∑i<llog⁡t≤bN∑m=1N−1N−mm≤bNN(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),

using 1m≤log⁡mm−1\frac1m\le\log\frac{m}{m-1} for m≥2m\ge2 (The Function slog⁡ss\log s: Continuity, Young's Inequality and Lower Bounds, with the Elementary Bounds for the Exponential and the Logarithm §log). As ∣zi∣,∣yi∣≤Rj+1|z_{i}|,|y_{i}|\le R_{j}+1, the mean value theorem gives ∣V(zi)−V(yi)∣≤Lh≤L/(4N)≤Λ/N≤1/j|V(z_{i})-V(y_{i})|\le Lh\le L/(4N)\le\Lambda/N\le1/j. Hence, with the bound on PN(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≤PN(z)≤Nek,ek=E(μ^)+2j+β(1+log⁡N)2(N−1)≤eˉ=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,

using 1+log⁡N≤N≤2(N−1)1+\log N\le N\le2(N-1) (The Function slog⁡ss\log s: Continuity, Young's Inequality and Lower Bounds, with the Elementary Bounds for the Exponential and the Logarithm §log).

(2b) ww on QQ. 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) in place of (x,y)(x,y), w(y)≤w(z)+12τ∥y−z∥(3∥y−z∥+2rN(z))w(y)\le w(z)+\frac{1}{2\tau}\lVert y-z\rVert(3\lVert y-z\rVert+2r_{N}(z)), so w(z)/N≥w(y)/N−12τ(3h2+2hrN(z)/N)w(z)/N\ge w(y)/N-\frac{1}{2\tau}(3h^{2}+2hr_{N}(z)/\sqrt{N}). By (2a) and p0≥e∗Np_{0}\ge e_{*}N, rN(z)2/N=2τ(2λ−1bg+(PN(z)−p0)/N2)≤2τ(2λ−1bg+eˉ−e∗)=:ρ2r_{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}, so with h≤1h\le1, w(z)/N≥w(y)/N−(3+2ρ)h/(2τ)w(z)/N\ge w(y)/N-(3+2\rho)h/(2\tau).

(2c) χ\chi on QQ. By Quantile Blocks of an Atomless Measure on the Line: Block Maps, Distances to Ordered Empirical Measures, and the Block Test Function §block-maps, ∥Tz−Ty∥μ^=∥z−y∥/N≤h\lVert T_{z}-T_{y}\rVert_{\hat{\mu}}=\lVert z-y\rVert/\sqrt{N}\le h; with (F4), χ(z)≤χ(y)+∥q∥μ^h+Kh(2W(y)+h)\chi(z)\le\chi(y)+\lVert q\rVert_{\hat{\mu}}h+Kh(2W(y)+h) and χ(y)≤∥q∥μ^W(y)+KW(y)2\chi(y)\le\lVert q\rVert_{\hat{\mu}}W(y)+KW(y)^{2}.

(2d) The competitor. Let PP be the measure with density (2h)−N1Q(2h)^{-N}\mathbf{1}_{Q} with respect to Lebesgue measure (QQ has Lebesgue measure (2h)N(2h)^{N}). It is a probability measure with bounded support, so P∈P2(RN)P\in\mathcal{P}_{2}(\mathbb{R}^{N}), with P(WN)=1P(W_{N})=1; by The Entropy of a Probability Measure on Euclidean Space §entropy (with ϕ(0)=0\phi(0)=0) it has finite entropy Ent(P)=−Nlog⁡(2h)=Nlog⁡(2N/c)\mathrm{Ent}(P)=-N\log(2h)=N\log(2N/c); PNP_{N} is bounded on QQ by (2a), so P∈DNP\in\mathcal{D}_{N}; and w−Nχw-N\chi is bounded on QQ 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),

Φk(πk)N≥Φk(P)N≥w(y)N−(3+2ρ)h2τ−∥q∥μ^(W(y)+h)−K(W(y)2+2hW(y)+h2)−δek−aN(log⁡(2N)+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).

As k→∞k\to\infty: w(yk)/Nk→uˉτ(μ^)w(y^{k})/N_{k}\to\bar{u}_{\tau}(\hat{\mu}), W(yk)→0W(y^{k})\to0, h≤1/(4Nk)→0h\le1/(4N_{k})\to0, ek→E(μ^)e_{k}\to\mathcal{E}(\hat{\mu}), aNlog⁡(2N)→0a_{N}\log(2N)\to0, and aNΛ≤σ2Λ/N≤σ2/j(k)→0a_{N}\Lambda\le\sigma^{2}\Lambda/N\le\sigma^{2}/j(k)\to0. The right side tends to m^\hat{m}, which proves the claim.

Step 3 (entropy bound; clause (b)). Let c1c_{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 NN. By The Gaussian Kernels on Euclidean Space: Scaling, Derivatives up to Order Three, the Convolution Identity, Moments and Tails §moments with q=Nq=N, s=1s=1 and R=2NR=\sqrt{2N}, the Gaussian weight g1≤c1g_{1}\le c_{1} has mass at most 12\frac12 outside the ball of radius RR, which lies in the cube [−R,R]N[-R,R]^{N} of Lebesgue measure (2R)N(2R)^{N}; so 12≤c1(2R)N\frac12\le c_{1}(2R)^{N} and log⁡c1≥−log⁡2−N2log⁡(8N)\log c_{1}\ge-\log2-\frac N2\log(8N). For P∈DNP\in\mathcal{D}_{N} put X(P)=1N∫PN dPX(P)=\frac1N\int P_{N}\,dP; by The Discrete Dyson Energy per Particle: Bounds, Compactness with a Lower Limit, and Recovery Configurations with Separated Particles §bounds, M2(P)≤A0N(1+X(P)−e∗)M_{2}(P)\le 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

δaNNEnt(P)≥−δεN−δθNX(P),εN=aN(log⁡2+12log⁡(8N)+A02(1+∣e∗∣)),θN=aNA02,(3a)\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})

where εN,θN→0\varepsilon_{N},\theta_{N}\to0 as k→∞k\to\infty. Write Xk=X(πk)X_{k}=X(\pi_{k}). By (0), (3a) and Step 2, for every positive ε\varepsilon and k≥k0(ε)k\ge k_{0}(\varepsilon),

∫Gk dπk≥m^−ε−δεN−δθNXk.(3b)\int G_{k}\,d\pi_{k}\ge\hat{m}-\varepsilon-\delta\varepsilon_{N}-\delta\theta_{N}X_{k}.\qquad(3\mathrm{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), Gk≤λ−1bg+∣e∗∣+∥q∥μ^2−δPN/NG_{k}\le\lambda^{-1}b_{g}+|e_{*}|+\lVert q\rVert_{\hat{\mu}}^{2}-\delta P_{N}/N on WNW_{N}, so

∫Gk dπk≤λ−1bg+∣e∗∣+∥q∥μ^2−δXk.(3c)\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})

Energy bound. Let C1=2λ−1bg+∣e∗∣+∣E(μ^)∣+∥q∥μ^2C_{1}=2\lambda^{-1}b_{g}+|e_{*}|+|\mathcal{E}(\hat{\mu})|+\lVert q\rVert_{\hat{\mu}}^{2}, so E1=δ−1(C1+2)E_{1}=\delta^{-1}(C_{1}+2). Take ε=12\varepsilon=\frac12 in (3b) and k0≥k0(12)k_{0}\ge k_{0}(\frac12) with εN≤12\varepsilon_{N}\le\frac12 and θN(C1+2)≤1\theta_{N}(C_{1}+2)\le1 for k≥k0k\ge k_{0}. For such kk, (3b), (3c), −m^≤λ−1bg+∣E(μ^)∣-\hat{m}\le\lambda^{-1}b_{g}+|\mathcal{E}(\hat{\mu})| and δ<1\delta<1 give δXk≤C1+1+δθNXk\delta X_{k}\le C_{1}+1+\delta\theta_{N}X_{k}. If Xk≤0X_{k}\le0 then Xk≤E1X_{k}\le E_{1}; otherwise δXk≤(C1+1)/(1−θN)≤C1+2\delta X_{k}\le(C_{1}+1)/(1-\theta_{N})\le C_{1}+2, as θN(C1+2)≤1\theta_{N}(C_{1}+2)\le1. So Xk≤E1X_{k}\le E_{1}.

Fisher bound. Let ∇fk\nabla f_{k} be a gradient map of fkf_{k} (Gibbs Maximisers of the Relative Free Energy: the Variational Principle and the Relative Score §score) with null set N′N'. Since πk\pi_{k} has a density with respect to Lebesgue measure, πk(N′)=0\pi_{k}(N')=0; and πk(WN)=1\pi_{k}(W_{N})=1. For x∈WN∖N′x\in W_{N}\setminus 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),

1N∥∇fk(x)∥2≤2δ2(2∥q∥μ^2+8K2W(x)2+2τ(2λ−1bg+PN(x)−p0N2)).\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).

Integrating against πk\pi_{k}, with ∥ΣN(πk)∥πk2=∫∥∇fk∥2 dπk\lVert\Sigma_{N}(\pi_{k})\rVert_{\pi_{k}}^{2}=\int\lVert\nabla f_{k}\rVert^{2}\,d\pi_{k} and 0≤1N2∫(PN−p0) dπk≤Xk−p0/N≤E1+∣e∗∣0\le\frac1{N^{2}}\int(P_{N}-p_{0})\,d\pi_{k}\le X_{k}-p_{0}/N\le E_{1}+|e_{*}| (as N≥1N\ge1, p0≥e∗Np_{0}\ge e_{*}N), gives the Fisher bound, since 2τ(2λ−1bg+E1+∣e∗∣)≤4τ(λ−1bg+E1+∣e∗∣)\frac2\tau(2\lambda^{-1}b_{g}+E_{1}+|e_{*}|)\le\frac4\tau(\lambda^{-1}b_{g}+E_{1}+|e_{*}|).

Step 4 (uniform upper estimate). Claim: for every positive ε\varepsilon there is k0k_{0} such that for every k≥k0k\ge k_{0} and every x∈WNx\in W_{N}

Gk(x)≤m^+η′22K+ε−K4W(x)2.G_{k}(x)\le\hat{m}+\frac{\eta'^{2}}{2K}+\varepsilon-\frac K4W(x)^{2}.

Suppose not. Then there are a positive ε\varepsilon, a strictly increasing sequence (kl)l(k_{l})_{l} and xl∈WNklx^{l}\in W_{N_{k_{l}}} violating the inequality at k=klk=k_{l}; write N=NklN=N_{k_{l}} and Wl=W(xl)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), Gk(x)≤λ−1bg+∣e∗∣+∥q∥μ^W(x)−KW(x)2−δPN(x)/NG_{k}(x)\le\lambda^{-1}b_{g}+|e_{*}|+\lVert q\rVert_{\hat{\mu}}W(x)-KW(x)^{2}-\delta P_{N}(x)/N, so the violation gives

δPN(xl)N<λ−1bg+∣e∗∣+∣m^∣+∥q∥μ^Wl−3K4Wl2≤λ−1bg+∣e∗∣+∣m^∣+∥q∥μ^23K.\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}.

So PNkl(xl)≤c′′NklP_{N_{k_{l}}}(x^{l})\le c''N_{k_{l}} for a constant 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 ll, and ν∈D\nu\in\mathcal{D} with W2(μxlN,ν)→0W_{2}(\mu^{N}_{x^{l}},\nu)\to0 and, for every positive ε′′\varepsilon'', E(ν)≤PN(xl)/N+ε′′\mathcal{E}(\nu)\le P_{N}(x^{l})/N+\varepsilon'' for large ll. 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 NklN_{k_{l}} being strictly increasing and at least N0N_{0}), w(xl)/N≤uˉτ(ν)+ε′′w(x^{l})/N\le\bar{u}_{\tau}(\nu)+\varepsilon'' for large ll. By On the Real Line an Atomless Source is Uniquely Mapped, by a Nondecreasing Optimal Map §monotone (μ^\hat{\mu} atomless) there is an optimal map TT from μ^\hat{\mu} to ν\nu, Borel and nondecreasing on a Borel set of full μ^\hat{\mu}-measure; Quantile Blocks of an Atomless Measure on the Line: Block Maps, Distances to Ordered Empirical Measures, and the Block Test Function §optimal gives ∥Txl−T∥μ^=W2(μxlN,ν)→0\lVert T_{x^{l}}-T\rVert_{\hat{\mu}}=W_{2}(\mu^{N}_{x^{l}},\nu)\to0. With (F4) and Step 1, Wl=∥Txl−id∥μ^→∥T−id∥μ^=Wν:=W2(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}) and χ(xl)→⟨q,T−id⟩μ^+KWν2\chi(x^{l})\to\langle q,T-\mathrm{id}\rangle_{\hat{\mu}}+KW_{\nu}^{2}. Letting l→∞l\to\infty in the violated inequality and then ε′′→0\varepsilon''\to0,

uˉτ(ν)−δE(ν)−⟨q,T−id⟩μ^−KWν2≥m^+η′22K+ε−K4Wν2.(4a)\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})

If Wν<r0W_{\nu}<r_{0}, the hypothesis of clause 1 and η′Wν≤η′22K+K2Wν2\eta'W_{\nu}\le\frac{\eta'^{2}}{2K}+\frac K2W_{\nu}^{2} bound the left side of (4a) by m^+η′22K−K2Wν2\hat{m}+\frac{\eta'^{2}}{2K}-\frac K2W_{\nu}^{2}, whence ε≤−K4Wν2≤0\varepsilon\le-\frac K4W_{\nu}^{2}\le0, a contradiction. If Wν≥r0W_{\nu}\ge r_{0}, then uˉτ(ν)≤λ−1bg\bar{u}_{\tau}(\nu)\le\lambda^{-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), −δE(ν)≤∣e0∣-\delta\mathcal{E}(\nu)\le|e_{0}|, and −⟨q,T−id⟩μ^≤∥q∥μ^Wν≤K4Wν2+∥q∥μ^2K-\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}; with −m^≤λ−1bg+∣E(μ^)∣-\hat{m}\le\lambda^{-1}b_{g}+|\mathcal{E}(\hat{\mu})| and K≥1K\ge1, (4a) gives ε≤S−K2Wν2≤S−K2r02≤0\varepsilon\le S-\frac K2W_{\nu}^{2}\le S-\frac K2r_{0}^{2}\le0, where S=2λ−1bg+∣e0∣+∣E(μ^)∣+∥q∥μ^2S=2\lambda^{-1}b_{g}+|e_{0}|+|\mathcal{E}(\hat{\mu})|+\lVert q\rVert_{\hat{\mu}}^{2} and Kr02≥2SKr_{0}^{2}\ge2S by hypothesis; a contradiction.

Step 5 (clause (c)). Let ε>0\varepsilon>0 and ε′=ε/12\varepsilon'=\varepsilon/12. Choose, in this order, k0k_{0} from Step 4 for ε′\varepsilon', then k0′≥k0k_{0}'\ge k_{0} at least k0(ε′)k_{0}(\varepsilon') of (3b) and the k0k_{0} of the energy bound, and such that εN+θNE1≤ε′\varepsilon_{N}+\theta_{N}E_{1}\le\varepsilon' for k≥k0′k\ge k_{0}'. For k≥k0′k\ge k_{0}', (3b) with Xk≤E1X_{k}\le E_{1} gives ∫Gk dπk≥m^−2ε′\int G_{k}\,d\pi_{k}\ge\hat{m}-2\varepsilon', while integrating Step 4 against πk\pi_{k} (all terms are integrable, W2W^{2} being a polynomial on WNW_{N} by (F4)) gives ∫Gk dπk≤m^+η′22K+ε′−K4∫W2 dπk\int G_{k}\,d\pi_{k}\le\hat{m}+\frac{\eta'^{2}}{2K}+\varepsilon'-\frac K4\int W^{2}\,d\pi_{k}. Hence K∫W2 dπk≤2η′2K+12ε′=2η′2K+εK\int W^{2}\,d\pi_{k}\le\frac{2\eta'^{2}}{K}+12\varepsilon'=\frac{2\eta'^{2}}{K}+\varepsilon.

Clause 2 (supersolution side). The proof is the same with the following changes. w=w‾N,τw=\underline{w}_{N,\tau}, χ=χN−\chi=\chi^{-}_{N} (data (q,−K)(q,-K)), fk=δ−1(Nχ−w)f_{k}=\delta^{-1}(N\chi-w), m^=−(u‾τ(μ^)+δE(μ^))\hat{m}=-(\underline{u}_{\tau}(\hat{\mu})+\delta\mathcal{E}(\hat{\mu})), Gk=−w/N+χ−δPN/NG_{k}=-w/N+\chi-\delta P_{N}/N and Φk(P)=∫(Nχ−w) dP−δEN(P)\Phi_{k}(P)=\int(N\chi-w)\,dP-\delta\mathcal{E}_{N}(P), so that (0) holds and maximising Φk\Phi_{k} is minimising ∫(w−Nχ) dP+δEN(P)\int(w-N\chi)\,dP+\delta\mathcal{E}_{N}(P); ∣m^∣≤λ−1bg+∣E(μ^)∣|\hat{m}|\le\lambda^{-1}b_{g}+|\mathcal{E}(\hat{\mu})| 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), Nχ(x)=−K∥x∥2+∑i(qˉi+2Kmi)xi+cχN\chi(x)=-K\lVert x\rVert^{2}+\sum_{i}(\bar{q}_{i}+2Km_{i})x_{i}+c_{\chi}; in (F3), qˉi−2K(xi−mi)\bar{q}_{i}-2K(x_{i}-m_{i}) replaces qˉi+2K(xi−mi)\bar{q}_{i}+2K(x_{i}-m_{i}), with the same bound; in (F4), χ(x)=⟨q,Tx−id⟩μ^−KW(x)2\chi(x)=\langle q,T_{x}-\mathrm{id}\rangle_{\hat{\mu}}-KW(x)^{2}, so −∥q∥μ^W−KW2≤χ≤∥q∥μ^W−KW2≤∥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}. Step 1: −w-w is semiconvex with constant τ−1\tau^{-1} and −w≤λ−1Nbg+∣e∗∣-w\le\lambda^{-1}Nb_{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)), Nχ+K∥x∥2N\chi+K\lVert x\rVert^{2} is affine, Nχ≤N∥q∥μ^2N\chi\le N\lVert q\rVert_{\hat{\mu}}^{2} on WNW_{N}, and (iii) applies to w‾N,τ\underline{w}_{N,\tau}; clause (a) becomes δ−1(N∇χ−∇w)=ΣN(πk)\delta^{-1}(N\nabla\chi-\nabla w)=\Sigma_{N}(\pi_{k}), that is, ∇w=N∇χ−δΣN(πk)\nabla w=N\nabla\chi-\delta\Sigma_{N}(\pi_{k}). Step 2: the levels are realising for u‾τ\underline{u}_{\tau}, so w(yk)/Nk→u‾τ(μ^)w(y^{k})/N_{k}\to\underline{u}_{\tau}(\hat{\mu}) 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)−12τ∥y−z∥(3∥y−z∥+2rN(z))w(y)\ge w(z)-\frac{1}{2\tau}\lVert y-z\rVert(3\lVert y-z\rVert+2r_{N}(z)), giving −w(z)/N≥−w(y)/N−(3+2ρ)h/(2τ)-w(z)/N\ge-w(y)/N-(3+2\rho)h/(2\tau); (2c) becomes χ(z)≥χ(y)−∥q∥μ^h−Kh(2W(y)+h)\chi(z)\ge\chi(y)-\lVert q\rVert_{\hat{\mu}}h-Kh(2W(y)+h) and χ(y)≥−∥q∥μ^W(y)−KW(y)2\chi(y)\ge-\lVert q\rVert_{\hat{\mu}}W(y)-KW(y)^{2}; the lower bound for Φk(πk)/N\Phi_{k}(\pi_{k})/N tends to −u‾τ(μ^)−δE(μ^)=m^-\underline{u}_{\tau}(\hat{\mu})-\delta\mathcal{E}(\hat{\mu})=\hat{m}. Step 3 is unchanged, (3c) following from −w/N≤λ−1bg+∣e∗∣-w/N\le\lambda^{-1}b_{g}+|e_{*}| and χ≤∥q∥μ^2\chi\le\lVert q\rVert_{\hat{\mu}}^{2}. Step 4: Gk(x)≤λ−1bg+∣e∗∣+∥q∥μ^W(x)−KW(x)2−δPN(x)/NG_{k}(x)\le\lambda^{-1}b_{g}+|e_{*}|+\lVert q\rVert_{\hat{\mu}}W(x)-KW(x)^{2}-\delta 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(xl)/N≤−u‾τ(ν)+ε′′-w(x^{l})/N\le-\underline{u}_{\tau}(\nu)+\varepsilon'' for large ll; χ(xl)→⟨q,T−id⟩μ^−KWν2\chi(x^{l})\to\langle q,T-\mathrm{id}\rangle_{\hat{\mu}}-KW_{\nu}^{2}; and (4a) reads −u‾τ(ν)−δE(ν)+⟨q,T−id⟩μ^−KWν2≥m^+η′22K+ε−K4Wν2-\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}. If Wν<r0W_{\nu}<r_{0}, the hypothesis of clause 2 gives −u‾τ(ν)−δE(ν)+⟨q,T−id⟩μ^≤m^+η′Wν-\underline{u}_{\tau}(\nu)-\delta\mathcal{E}(\nu)+\langle q,T-\mathrm{id}\rangle_{\hat{\mu}}\le\hat{m}+\eta'W_{\nu}, and if Wν≥r0W_{\nu}\ge r_{0} one uses −u‾τ(ν)≤λ−1bg-\underline{u}_{\tau}(\nu)\le\lambda^{-1}b_{g}, −δE(ν)≤∣e0∣-\delta\mathcal{E}(\nu)\le|e_{0}| and ⟨q,T−id⟩μ^≤∥q∥μ^Wν\langle q,T-\mathrm{id}\rangle_{\hat{\mu}}\le\lVert q\rVert_{\hat{\mu}}W_{\nu}; the contradictions follow verbatim. Step 5 is unchanged.

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