TheoremBase

Lattice Fourier identities turn the potential's Hessian, slope and curvature into site sums, which gives admissibility and the gradient formula. A finite-dimensional density computation shows that the Ising Gaussian reference has a Gaussian density relative to the split Gaussian, so the field law is the Gibbs measure; the relative score integrand does not depend on the split, which gives split-independence of the entropy pair, and a dressed-Gaussian lemma gives equality of the noise-connected sets.

Proof

Each result cited is universally quantified over the data in its own statement. Real order and arithmetic are those of The Real Numbers: Standing Notation and Background; finite sums over finite index sets are manipulated (agreement with indexed sums, reindexing along a bijection, additivity, homogeneity, dropping vanishing terms, interchange) by claims 1 to 4 of Properties of a Sum over a Finite Index Set and claims 1, 4 and 5 of Peeling, Splitting, and Interchange for Sums over a Finite Index Set, and this is not repeated below.

Step 0 (Conventions). Write d=dMd=d_{M}, χ=χM\chi=\chi_{M}, Γ=ΓM\Gamma=\Gamma_{M} and L=LM\mathbb{L}=\mathbb{L}_{M}. For j∈Nj\in\mathbb{N}, aj>0a_{j}>0, since aa is a weight sequence by White Noise in the Square-Integrable Space and the Free Field on the Torus as Noise Weights and a Variance Sequence on a Negative Sobolev Space §weights, whose terms are positive by Weight Sequences and the Weighted Fisher Information Relative to a Diagonal Gaussian Measure on a Hilbert Space §weights, and cj>0c_{j}>0 by White Noise in the Square-Integrable Space and the Free Field on the Torus as Noise Weights and a Variance Sequence on a Negative Sobolev Space §variances and Variance Sequences and Their Truncations §variances; aj1/2a_{j}^{1/2} is the positive square root of aja_{j} and aj−1/2a_{j}^{-1/2} its inverse, so aj(aj−1/2)2=1a_{j}(a_{j}^{-1/2})^{2}=1 and ajaj−1/2=aj1/2a_{j}a_{j}^{-1/2}=a_{j}^{1/2}. Likewise L−n/2L^{-n/2} is the inverse of the positive square root Ln/2L^{n/2} of LnL^{n}, so (L−n/2)2=L−n(L^{-n/2})^{2}=L^{-n} and L−n/2Ln=Ln/2L^{-n/2}L^{n}=L^{n/2}. By The Galerkin Wick-Ordered Phi^4 Potential and Its Wick Constant on the Torus §head-dimension, κ(j)∉Γ\kappa(j)\notin\Gamma for j>dj>d, and for j∈[d]j\in[d], χ(j)∈{0,1}\chi(j)\in\{0,1\} with χ(j)=1\chi(j)=1 exactly when κ(j)∈Γ\kappa(j)\in\Gamma; hence, for j∈Nj\in\mathbb{N}, κ(j)∈Γ\kappa(j)\in\Gamma if and only if j≤dj\le d and χ(j)=1\chi(j)=1, and χ(j)2=χ(j)\chi(j)^{2}=\chi(j). Let JMJ_{M} be the set of j∈[d]j\in[d] with χ(j)=1\chi(j)=1, that is, with κ(j)∈Γ\kappa(j)\in\Gamma: the set of active indices of The Galerkin Wick-Ordered Phi^4 Potential and Its Wick Constant on the Torus §head-dimension at cutoff MM.

For j∈[d]j\in[d] and z∈Lz\in\mathbb{L} put ωj(z)=L−n/2χ(j) aj−1/2ψκ(j)(z)\omega_{j}(z)=L^{-n/2}\chi(j)\,a_{j}^{-1/2}\psi_{\kappa(j)}(z), and for u∈Rdu\in\mathbb{R}^{d} let ℓu\ell_{u} be the lattice field ℓu(z)=∑j=1dωj(z) uj\ell_{u}(z)=\sum_{j=1}^{d}\omega_{j}(z)\,u_{j}. Then vς(u)=∑z∈Lfς(ℓu(z))v_{\varsigma}(u)=\sum_{z\in\mathbb{L}}f_{\varsigma}(\ell_{u}(z)) by the definition of vςv_{\varsigma}, and for x∈Xx\in X, φx=ℓpd(x)\varphi_{x}=\ell_{p_{d}(x)} by The White-Noise Embedding of Lattice Fields: Linearity, Inversion by the Site Field, the Site Sum as the White-Noise Norm, and Coordinates §coordinates, since pd(x)=(x1,…,xd)p_{d}(x)=(x_{1},\dots,x_{d}) by Borel Probability Measures on a Real Hilbert Space with an Orthonormal Basis: Standing Notation §coordinates. For a lattice field FF and k∈Γk\in\Gamma, The Lattice Torus of Odd Side, Lattice Fields, and the Discrete Fourier Coefficients of a Lattice Field §coefficients gives

L−n/2∑z∈LF(z) ψk(z)=L−n/2LnF^(k)=Ln/2F^(k).(F)L^{-n/2}\sum_{z\in\mathbb{L}}F(z)\,\psi_{k}(z)=L^{-n/2}L^{n}\hat{F}(k)=L^{n/2}\hat{F}(k).\tag{F}

Step 1 (Lattice identities). (R) For every map g:Γ→Rg:\Gamma\to\mathbb{R}, ∑j=1dχ(j) g(κ(j))=∑k∈Γg(k)\sum_{j=1}^{d}\chi(j)\,g(\kappa(j))=\sum_{k\in\Gamma}g(k). Indeed, κ\kappa is a bijection N→Zn\mathbb{N}\to\mathbb{Z}^{n}; for k∈Γk\in\Gamma the index j=κ−1(k)j=\kappa^{-1}(k) has κ(j)∈Γ\kappa(j)\in\Gamma, so j∈JMj\in J_{M} by Step 0. Hence the restriction of κ\kappa to JMJ_{M} is a bijection JM→ΓJ_{M}\to\Gamma, and JMJ_{M} is nonempty as Γ\Gamma is nonempty (The Cubes of the Integer Lattice are Finite, Nested, Exhaust the Lattice and Have (2N+1)^n Points §finite). The summand χ(j)g(κ(j))\chi(j)g(\kappa(j)) vanishes for j∈[d]∖JMj\in[d]\setminus J_{M} and equals g(κ(j))g(\kappa(j)) for j∈JMj\in J_{M}, so the sum is ∑j∈JMg(κ(j))=∑k∈Γg(k)\sum_{j\in J_{M}}g(\kappa(j))=\sum_{k\in\Gamma}g(k).

(G) For j,k∈[d]j,k\in[d], ∑z∈Lωj(z)ωk(z)=χ(j) δjk/aj\sum_{z\in\mathbb{L}}\omega_{j}(z)\omega_{k}(z)=\chi(j)\,\delta_{jk}/a_{j}, with δjk=1\delta_{jk}=1 if j=kj=k and 00 otherwise. Indeed, the left side is χ(j)χ(k)aj−1/2ak−1/2 L−n∑zψκ(j)(z)ψκ(k)(z)\chi(j)\chi(k)a_{j}^{-1/2}a_{k}^{-1/2}\,L^{-n}\sum_{z}\psi_{\kappa(j)}(z)\psi_{\kappa(k)}(z). If χ(j)χ(k)=0\chi(j)\chi(k)=0 both sides vanish (if j=kj=k then χ(j)=0\chi(j)=0). Otherwise κ(j),κ(k)∈Γ\kappa(j),\kappa(k)\in\Gamma, and by Discrete Fourier Analysis on the Lattice Torus: Counting, Orthogonality, Inversion, Parseval, and the Spin Sum §orthogonality the last factor is 11 if κ(j)=κ(k)\kappa(j)=\kappa(k), that is j=kj=k (κ\kappa being injective), and 00 otherwise; and aj−1/2aj−1/2=1/aja_{j}^{-1/2}a_{j}^{-1/2}=1/a_{j}.

(Q) For u,w∈Rdu,w\in\mathbb{R}^{d}, expanding both factors and using (G),

∑z∈Lℓu(z)ℓw(z)=∑j=1d∑k=1dujwk∑z∈Lωj(z)ωk(z)=∑j=1dχ(j)ujwjaj.\sum_{z\in\mathbb{L}}\ell_{u}(z)\ell_{w}(z)=\sum_{j=1}^{d}\sum_{k=1}^{d}u_{j}w_{k}\sum_{z\in\mathbb{L}}\omega_{j}(z)\omega_{k}(z)=\sum_{j=1}^{d}\chi(j)\frac{u_{j}w_{j}}{a_{j}} .

In particular ∑zℓu(z)2=∑j=1dχ(j)uj2/aj\sum_{z}\ell_{u}(z)^{2}=\sum_{j=1}^{d}\chi(j)u_{j}^{2}/a_{j}, and, taking for ww the kk-th unit vector (for which ℓw=ωk\ell_{w}=\omega_{k}), ∑zℓu(z)ωk(z)=χ(k)uk/ak\sum_{z}\ell_{u}(z)\omega_{k}(z)=\chi(k)u_{k}/a_{k} for k∈[d]k\in[d]. With u=pd(x)u=p_{d}(x), x∈Xx\in X, Step 0 gives ∑zφx(z)2=∑j=1dχ(j)xj2/aj\sum_{z}\varphi_{x}(z)^{2}=\sum_{j=1}^{d}\chi(j)x_{j}^{2}/a_{j}.

(D) For every y∈Ly\in\mathbb{L}, ∑k∈Γψk(y)2=Ln\sum_{k\in\Gamma}\psi_{k}(y)^{2}=L^{n}. Let ιy\iota_{y} be the lattice field equal to 11 at yy and 00 elsewhere. By The Lattice Torus of Odd Side, Lattice Fields, and the Discrete Fourier Coefficients of a Lattice Field §coefficients, ι^y(k)=L−nψk(y)\hat{\iota}_{y}(k)=L^{-n}\psi_{k}(y) (only the summand at z=yz=y survives), and Discrete Fourier Analysis on the Lattice Torus: Counting, Orthogonality, Inversion, Parseval, and the Spin Sum §inversion-formula at yy gives 1=ιy(y)=∑k∈ΓL−nψk(y)21=\iota_{y}(y)=\sum_{k\in\Gamma}L^{-n}\psi_{k}(y)^{2}.

(P) For every lattice field FF, ∑k=1dak(∑z∈LF(z)ωk(z))2=∑z∈LF(z)2\sum_{k=1}^{d}a_{k}\bigl(\sum_{z\in\mathbb{L}}F(z)\omega_{k}(z)\bigr)^{2}=\sum_{z\in\mathbb{L}}F(z)^{2}. Indeed, by (F), ∑zF(z)ωk(z)=χ(k)ak−1/2Ln/2F^(κ(k))\sum_{z}F(z)\omega_{k}(z)=\chi(k)a_{k}^{-1/2}L^{n/2}\hat{F}(\kappa(k)), the right side read as 00 when χ(k)=0\chi(k)=0; so ak(∑zF(z)ωk(z))2=χ(k)LnF^(κ(k))2a_{k}(\sum_{z}F(z)\omega_{k}(z))^{2}=\chi(k)L^{n}\hat{F}(\kappa(k))^{2}, and by (R) and Discrete Fourier Analysis on the Lattice Torus: Counting, Orthogonality, Inversion, Parseval, and the Spin Sum §parseval (with f=g=Ff=g=F) the sum over kk is Ln∑l∈ΓF^(l)2=LnL−n∑zF(z)2L^{n}\sum_{l\in\Gamma}\hat{F}(l)^{2}=L^{n}L^{-n}\sum_{z}F(z)^{2}.

Step 2 (Claim 1). Let ς\varsigma be an admissible split and k∈Γk\in\Gamma; write rk=rk(ς)r_{k}=r^{(\varsigma)}_{k}. As 0<qk<ς0<\mathfrak{q}_{k}<\varsigma, the numbers qkς\mathfrak{q}_{k}\varsigma and ς−qk\varsigma-\mathfrak{q}_{k} are positive, so rk>0r_{k}>0 and 1/rk=(ς−qk)/(qkς)=1/qk−1/ς1/r_{k}=(\varsigma-\mathfrak{q}_{k})/(\mathfrak{q}_{k}\varsigma)=1/\mathfrak{q}_{k}-1/\varsigma. Hence every cj(ς)c^{(\varsigma)}_{j} is positive (Step 0). For j∈Nj\in\mathbb{N}, aj=μκ(j)cja_{j}=\mu_{\kappa(j)}c_{j} by White Noise in the Square-Integrable Space and the Free Field on the Torus as Noise Weights and a Variance Sequence on a Negative Sobolev Space §ratio, so μκ(j)=aj/cj>0\mu_{\kappa(j)}=a_{j}/c_{j}>0 and cj(ς)=cjwjc^{(\varsigma)}_{j}=c_{j}w_{j} with wj=μκ(j)rκ(j)w_{j}=\mu_{\kappa(j)}r_{\kappa(j)} if κ(j)∈Γ\kappa(j)\in\Gamma and wj=1w_{j}=1 otherwise. Let DD be the greatest entry of the tuple consisting of 11 followed by the numbers μkrk\mu_{k}r_{k} along an enumeration of Γ\Gamma (Greatest Element of a Finite Family in a Totally Ordered Set); then 0≤wj≤D0\le w_{j}\le D, and ∑j=1∞cj(ς)\sum_{j=1}^{\infty}c^{(\varsigma)}_{j} converges by Series of Nonnegative Real Numbers, Comparison, and the Geometric Series §tail-bound, applied to the nonnegative terms cjc_{j}, whose series converges by White Noise in the Square-Integrable Space and the Free Field on the Torus as Noise Weights and a Variance Sequence on a Negative Sobolev Space §variances, and to the factors wjw_{j} with the bound DD. So c(ς)c^{(\varsigma)} is a variance sequence (Variance Sequences and Their Truncations §variances). Finally 1≤rˉς1\le\bar{r}_{\varsigma} and rk≤rˉςr_{k}\le\bar{r}_{\varsigma} for k∈Γk\in\Gamma; if κ(j)∈Γ\kappa(j)\in\Gamma then cj(ς)=ajrκ(j)≤rˉςajc^{(\varsigma)}_{j}=a_{j}r_{\kappa(j)}\le\bar{r}_{\varsigma}a_{j}, and otherwise cj(ς)=cj≤aj≤rˉςajc^{(\varsigma)}_{j}=c_{j}\le a_{j}\le\bar{r}_{\varsigma}a_{j} by White Noise in the Square-Integrable Space and the Free Field on the Torus as Noise Weights and a Variance Sequence on a Negative Sobolev Space §ratio. This proves claim 1. We record that, for j∈Nj\in\mathbb{N}, κ(j)∈Γ\kappa(j)\in\Gamma gives

1cj(ς)=1ajrκ(j)=1ajqκ(j)−1ajς=1cjJ,η−1ajς,(S)\frac{1}{c^{(\varsigma)}_{j}}=\frac{1}{a_{j}r_{\kappa(j)}}=\frac{1}{a_{j}\mathfrak{q}_{\kappa(j)}}-\frac{1}{a_{j}\varsigma}=\frac{1}{c^{J,\eta}_{j}}-\frac{1}{a_{j}\varsigma},\tag{S}

by The Hubbard-Stratonovich Transform of the Ising Measure on the Lattice Torus §variances, while cj(ς)=cj=cjJ,ηc^{(\varsigma)}_{j}=c_{j}=c^{J,\eta}_{j} if κ(j)∉Γ\kappa(j)\notin\Gamma.

Step 3 (One-variable calculus). Fix an admissible split ς\varsigma and write f=fςf=f_{\varsigma}. Every point of R\mathbb{R} is an interior point of the interval R\mathbb{R} by Basic Facts about Intervals of the Real Line and Their Interior Points §whole-line; derivatives are those of Derivative at an Interior Point. For t∈Rt\in\mathbb{R} put E(t)=exp⁡(t)E(t)=\exp(t), Eˉ(t)=exp⁡(−t)\bar{E}(t)=\exp(-t), h=E+Eˉh=E+\bar{E}, g=E−Eˉg=E-\bar{E} and τ=g/h\tau=g/h; EE and Eˉ\bar{E} are positive by claim 2 of Basic Properties of the Exponential Function, so h>0h>0, lch⁡=log⁡∘h\operatorname{lch}=\log\circ h, and −h<g<h-h<g<h, whence ∣τ(t)∣<1|\tau(t)|<1 and 0≤τ(t)2<10\le\tau(t)^{2}<1.

(i) E′=EE'=E by claim 3 of Basic Properties of the Exponential Function; t↦−t=(−1)t1t\mapsto-t=(-1)t^{1} has derivative −1-1 by claim 1 of Derivative of a Polynomial Function on the Real Line and claim 2 of Sum, Constant Multiple, and Product Rules for One-Dimensional Derivatives, so Eˉ′=−Eˉ\bar{E}'=-\bar{E} by Chain Rule for One-Dimensional Derivatives. By claim 2 of Sum, Constant Multiple, and Product Rules for One-Dimensional Derivatives, h′=gh'=g.

(ii) By (i) and claim 2 of Sum, Constant Multiple, and Product Rules for One-Dimensional Derivatives, hh and gg are differentiable at every point with h′=gh'=g and g′=E+Eˉ=hg'=E+\bar{E}=h; so hh is smooth on R1\mathbb{R}^{1} by claim 3 of One-Dimensional Derivatives, Partial Derivatives, and Smoothness on the Real Line (with {h,g}\{h,g\} as the set of functions there), and ∂1h=h′=g\partial_{1}h=h'=g by claim 2 there. By The Natural Logarithm, log⁡\log is smooth on (0,∞)(0,\infty), an open subset of R1\mathbb{R}^{1} (for s>0s>0, ∣r−s∣<s/2|r-s|<s/2 forces r>0r>0), and its derivative log⁡′(s)=1/s\log'(s)=1/s is the one of the smooth inverse function theorem with n=1n=1, that is, ∂1log⁡(s)=1/s\partial_{1}\log(s)=1/s for s>0s>0; and hh takes values in (0,∞)(0,\infty). Smooth maps being of class C1C^{1} (Smooth Map on a Euclidean Open Set), claim 1 of A Composition of CkC^k Maps Between Euclidean Open Sets is of Class CkC^k (with n=m=p=1n=m=p=1, U=RU=\mathbb{R}, open in R1\mathbb{R}^{1} by claim 1 of Euclidean Space is Open in Itself, and CkC^k Maps are Continuous, V=(0,∞)V=(0,\infty), F=hF=h and G=log⁡G=\log) gives ∂1lch⁡(t)=∂1log⁡(h(t)) ∂1h(t)=g(t)/h(t)=τ(t)\partial_{1}\operatorname{lch}(t)=\partial_{1}\log(h(t))\,\partial_{1}h(t)=g(t)/h(t)=\tau(t). So, by claim 2 of One-Dimensional Derivatives, Partial Derivatives, and Smoothness on the Real Line applied to lch⁡:R→R\operatorname{lch}:\mathbb{R}\to\mathbb{R}, lch⁡\operatorname{lch} is differentiable at every t∈Rt\in\mathbb{R} with lch⁡′(t)=τ(t)\operatorname{lch}'(t)=\tau(t).

(iii) Since exp⁡(log⁡s)=s\exp(\log s)=s (The Natural Logarithm) and by claim 2 of Basic Properties of the Exponential Function, exp⁡(−lch⁡(t))=1/h(t)\exp(-\operatorname{lch}(t))=1/h(t), so τ=g⋅(exp⁡∘(−lch⁡))\tau=g\cdot(\exp\circ(-\operatorname{lch})). By (ii), claim 2 of Sum, Constant Multiple, and Product Rules for One-Dimensional Derivatives and Chain Rule for One-Dimensional Derivatives, exp⁡∘(−lch⁡)\exp\circ(-\operatorname{lch}) has derivative −τ(t)/h(t)-\tau(t)/h(t) at tt; g′=hg'=h by (ii); so by claim 3 of Sum, Constant Multiple, and Product Rules for One-Dimensional Derivatives, τ′(t)=h(t)/h(t)−g(t)τ(t)/h(t)=1−τ(t)2\tau'(t)=h(t)/h(t)-g(t)\tau(t)/h(t)=1-\tau(t)^{2}.

(iv) By claim 1 of Derivative of a Polynomial Function on the Real Line (t↦t2t\mapsto t^{2} has derivative 2t2t), claims 1 to 3 of Sum, Constant Multiple, and Product Rules for One-Dimensional Derivatives, (ii) and (iii): ff is differentiable at every tt with derivative f′(t)=t/ς−τ(t)f'(t)=t/\varsigma-\tau(t), which is the map fς′f'_{\varsigma} of claim 3; f′f' is differentiable with derivative f′′(t)=1/ς−1+τ(t)2f''(t)=1/\varsigma-1+\tau(t)^{2}; and f′′f'' is differentiable (product rule for τ2\tau^{2}).

(v) ff is of class C2C^{2} on R=R1\mathbb{R}=\mathbb{R}^{1}, open by claim 1 of Euclidean Space is Open in Itself, and CkC^k Maps are Continuous, with ∂1f=f′\partial_{1}f=f' and ∂1f′=f′′\partial_{1}f'=f''. Indeed, for a map P:R→RP:\mathbb{R}\to\mathbb{R} differentiable at every point with derivative P′P', claim 2 of One-Dimensional Derivatives, Partial Derivatives, and Smoothness on the Real Line, with R\mathbb{R} regarded as R1\mathbb{R}^{1}, shows that for every t∈Rt\in\mathbb{R} the partial derivative ∂1P(t)\partial_{1}P(t) of Partial Derivative on a Euclidean Open Set exists and equals P′(t)P'(t); and PP is continuous at every point in the sense of Continuity at a Point for Maps Between Euclidean Spaces, because by Differentiability at an Interior Point Implies Continuity There it is continuous for the metric ∣s−t∣|s-t|, and for n=m=1n=m=1 and positive δ,ε\delta,\varepsilon the conditions (s−t)2<δ2(s-t)^{2}<\delta^{2} and (P(s)−P(t))2<ε2(P(s)-P(t))^{2}<\varepsilon^{2} are equivalent to ∣s−t∣<δ|s-t|<\delta and ∣P(s)−P(t)∣<ε|P(s)-P(t)|<\varepsilon. Applying this to P=f,f′,f′′P=f,f',f'' (by (iv)) and using clauses 1 to 3 of C^k Maps on a Euclidean Open Set: f′f' is of class C1C^{1}, and ff is of class C1C^{1} with ∂1f=f′\partial_{1}f=f' of class C1C^{1}, that is, of class C2C^{2}.

(vi) Bounds. Let KςK_{\varsigma} be the greater of 00 and 1−ς−11-\varsigma^{-1}; then 0≤Kς0\le K_{\varsigma} and, by (iv) and 0≤τ2<10\le\tau^{2}<1,

−Kς≤1ς−1≤f′′(t)<1ς,f′(t)2≤2t2ς2+2τ(t)2≤2t2ς2+2,-K_{\varsigma}\le\frac{1}{\varsigma}-1\le f''(t)<\frac{1}{\varsigma},\qquad f'(t)^{2}\le\frac{2t^{2}}{\varsigma^{2}}+2\tau(t)^{2}\le\frac{2t^{2}}{\varsigma^{2}}+2,

the second from (p+q)2≤2p2+2q2(p+q)^{2}\le2p^{2}+2q^{2}. The map log⁡\log is increasing on (0,∞)(0,\infty): if 0<s≤s′0<s\le s' and log⁡s′<log⁡s\log s'<\log s, then s′=exp⁡(log⁡s′)<exp⁡(log⁡s)=ss'=\exp(\log s')<\exp(\log s)=s by claim 4 of Basic Properties of the Exponential Function, a contradiction. As t≤∣t∣t\le|t| and −t≤∣t∣-t\le|t|, claim 4 of Basic Properties of the Exponential Function gives h(t)≤2exp⁡(∣t∣)h(t)\le2\exp(|t|), so, by The Natural Logarithm (log⁡(st)=log⁡s+log⁡t\log(st)=\log s+\log t and log⁡exp⁡(∣t∣)=∣t∣\log\exp(|t|)=|t|), lch⁡(t)≤∣t∣+log⁡2\operatorname{lch}(t)\le|t|+\log2; and log⁡2≥log⁡1=0\log2\ge\log1=0, since exp⁡(0)=1\exp(0)=1 by claim 1 of Basic Properties of the Exponential Function. From (∣t∣−ς)2≥0(|t|-\varsigma)^{2}\ge0 and (∣t∣−2ς)2≥0(|t|-2\varsigma)^{2}\ge0, ∣t∣≤t2/(2ς)+ς/2|t|\le t^{2}/(2\varsigma)+\varsigma/2 and ∣t∣≤t2/(4ς)+ς|t|\le t^{2}/(4\varsigma)+\varsigma; hence

f(t)≥t22ς−∣t∣−log⁡2≥−(ς2+log⁡2),f(t)≥t24ς−ς−log⁡2.f(t)\ge\frac{t^{2}}{2\varsigma}-|t|-\log2\ge-\Bigl(\frac{\varsigma}{2}+\log2\Bigr),\qquad f(t)\ge\frac{t^{2}}{4\varsigma}-\varsigma-\log2 .

Step 4 (Claim 2). Keep ς\varsigma, ff and KςK_{\varsigma} of Step 3, and write v=vςv=v_{\varsigma}, V=VςV=V_{\varsigma}. By Step 0, V(x)=∑zf(ℓpd(x)(z))=v(pd(x))V(x)=\sum_{z}f(\ell_{p_{d}(x)}(z))=v(p_{d}(x)), so V=v∘pdV=v\circ p_{d}.

Regularity and derivatives. Rd\mathbb{R}^{d} is open by claim 1 of Euclidean Space is Open in Itself, and CkC^k Maps are Continuous. For z∈Lz\in\mathbb{L} let Lz:Rd→RL_{z}:\mathbb{R}^{d}\to\mathbb{R}, Lz(u)=ℓu(z)=∑j=1dωj(z)ujL_{z}(u)=\ell_{u}(z)=\sum_{j=1}^{d}\omega_{j}(z)u_{j}. For m∈[d]m\in[d] let Lz[m]:Rd→RL^{[m]}_{z}:\mathbb{R}^{d}\to\mathbb{R}, Lz[m](u)=∑j=1mωj(z)ujL^{[m]}_{z}(u)=\sum_{j=1}^{m}\omega_{j}(z)u_{j}, and let πl\pi_{l} be the ll-th coordinate function on Rd\mathbb{R}^{d}. Let IzI_{z} be the set of m∈Nm\in\mathbb{N} such that, if m≤dm\le d, then Lz[m]L^{[m]}_{z} is smooth on Rd\mathbb{R}^{d}. Then 1∈Iz1\in I_{z}: if 1≤d1\le d, claim 1 of Properties of Finite Sums gives Lz[1]=ω1(z)π1L^{[1]}_{z}=\omega_{1}(z)\pi_{1}, which is smooth by claims 2 and 3 of Constants, Coordinate Functions, Sums and Products of CkC^k Functions on a Euclidean Open Set. And S(m)∈IzS(m)\in I_{z} for m∈Izm\in I_{z}: if S(m)≤dS(m)\le d, then m<S(m)m<S(m) by Properties of the Order on the Natural Numbers §successor, so m≤dm\le d by Properties of the Order on the Natural Numbers §basic and Lz[m]L^{[m]}_{z} is smooth; as S(m)∈[d]S(m)\in[d], claim 1 of Properties of Finite Sums gives Lz[S(m)]=Lz[m]+ωS(m)(z)πS(m)L^{[S(m)]}_{z}=L^{[m]}_{z}+\omega_{S(m)}(z)\pi_{S(m)}, which is smooth by claims 2 and 3 of Constants, Coordinate Functions, Sums and Products of CkC^k Functions on a Euclidean Open Set. By Principle of Induction for the Natural Numbers, Iz=NI_{z}=\mathbb{N}; since d≤dd\le d (Properties of the Order on the Natural Numbers §basic), Lz=Lz[d]L_{z}=L^{[d]}_{z} is smooth, hence of class C2C^{2} by Smooth Map on a Euclidean Open Set; and ∂iLz(u)=ωi(z)\partial_{i}L_{z}(u)=\omega_{i}(z) by claim 1 of Constants, Coordinate Functions, Sums and Products of CkC^k Functions on a Euclidean Open Set, because the difference quotient of Partial Derivative on a Euclidean Open Set for the ll-th coordinate function in the ii-th variable is constantly 11 if l=il=i and 00 otherwise. By claim 2 of A Composition of CkC^k Maps Between Euclidean Open Sets is of Class CkC^k (with k=2k=2, F=LzF=L_{z} and G=fG=f, of class C2C^{2} on R\mathbb{R} by Step 3(v)), f∘Lzf\circ L_{z} is of class C2C^{2} on Rd\mathbb{R}^{d}; by claim 1 there, applied with G=fG=f and with G=f′G=f' (of class C1C^{1} by Step 3(v)), ∂i(f∘Lz)(u)=f′(ℓu(z))ωi(z)\partial_{i}(f\circ L_{z})(u)=f'(\ell_{u}(z))\omega_{i}(z) and ∂k(f′∘Lz)(u)=f′′(ℓu(z))ωk(z)\partial_{k}(f'\circ L_{z})(u)=f''(\ell_{u}(z))\omega_{k}(z). As ∂i(f∘Lz)\partial_{i}(f\circ L_{z}) is the scalar multiple ωi(z) (f′∘Lz)\omega_{i}(z)\,(f'\circ L_{z}), claim 1 of Constants, Coordinate Functions, Sums and Products of CkC^k Functions on a Euclidean Open Set gives ∂k∂i(f∘Lz)(u)=f′′(ℓu(z)) ωk(z) ωi(z)\partial_{k}\partial_{i}(f\circ L_{z})(u)=f''(\ell_{u}(z))\,\omega_{k}(z)\,\omega_{i}(z). Now sum over the finite set L\mathbb{L} along an enumeration z1,…,zm0z_{1},\dots,z_{m_{0}} of L\mathbb{L}, and for m∈[m0]m\in[m_{0}] let v[m]=∑q=1mf∘Lzqv^{[m]}=\sum_{q=1}^{m}f\circ L_{z_{q}}. Say that m∈[m0]m\in[m_{0}] has property (Cm_{m}) if v[m]v^{[m]} is of class C2C^{2} on Rd\mathbb{R}^{d} with ∂iv[m](u)=∑q=1mf′(ℓu(zq)) ωi(zq)\partial_{i}v^{[m]}(u)=\sum_{q=1}^{m}f'(\ell_{u}(z_{q}))\,\omega_{i}(z_{q}) and ∂k∂iv[m](u)=∑q=1mf′′(ℓu(zq)) ωk(zq) ωi(zq)\partial_{k}\partial_{i}v^{[m]}(u)=\sum_{q=1}^{m}f''(\ell_{u}(z_{q}))\,\omega_{k}(z_{q})\,\omega_{i}(z_{q}) for all u∈Rdu\in\mathbb{R}^{d} and i,k∈[d]i,k\in[d]. Let II be the set of m∈Nm\in\mathbb{N} such that, if m≤m0m\le m_{0}, then (Cm_{m}) holds. Then 1∈I1\in I: if 1≤m01\le m_{0}, claim 1 of Properties of Finite Sums gives v[1]=f∘Lz1v^{[1]}=f\circ L_{z_{1}} and reduces the two sums to their single terms, so (C1_{1}) is what was just shown for z=z1z=z_{1}. And S(m)∈IS(m)\in I for m∈Im\in I: if S(m)≤m0S(m)\le m_{0}, then m<S(m)m<S(m) by Properties of the Order on the Natural Numbers §successor, so m≤m0m\le m_{0} by Properties of the Order on the Natural Numbers §basic and (Cm_{m}) holds; as S(m)∈[m0]S(m)\in[m_{0}], claim 1 of Properties of Finite Sums gives v[S(m)]=v[m]+f∘LzS(m)v^{[S(m)]}=v^{[m]}+f\circ L_{z_{S(m)}}, and likewise splits off the last term of the two derivative sums; so v[S(m)]v^{[S(m)]} is of class C2C^{2} by claim 3 of Constants, Coordinate Functions, Sums and Products of CkC^k Functions on a Euclidean Open Set, and claim 1 of Constants, Coordinate Functions, Sums and Products of CkC^k Functions on a Euclidean Open Set, applied to the sum and then to the sum of the first partial derivatives, gives the two formulas, that is, (CS(m)_{S(m)}). By Principle of Induction for the Natural Numbers, I=NI=\mathbb{N}; since m0≤m0m_{0}\le m_{0} (Properties of the Order on the Natural Numbers §basic), (Cm0_{m_{0}}) holds, and v=v[m0]v=v^{[m_{0}]}. Hence vv is of class C2C^{2} on Rd\mathbb{R}^{d}, and for u∈Rdu\in\mathbb{R}^{d} and i,k∈[d]i,k\in[d]

∂iv(u)=∑z∈Lf′(ℓu(z)) ωi(z),∂k∂iv(u)=∑z∈Lf′′(ℓu(z)) ωk(z) ωi(z).(V)\partial_{i}v(u)=\sum_{z\in\mathbb{L}}f'(\ell_{u}(z))\,\omega_{i}(z),\qquad\partial_{k}\partial_{i}v(u)=\sum_{z\in\mathbb{L}}f''(\ell_{u}(z))\,\omega_{k}(z)\,\omega_{i}(z).\tag{V}

In particular ∂iv=0\partial_{i}v=0 when χ(i)=0\chi(i)=0, since then ωi=0\omega_{i}=0.

We verify the four conditions of Admissible Cylindrical Potentials on a Hilbert Space in the Noise Geometry §admissible with head dimension dd, profile vv and the nonnegative constant KςK_{\varsigma}. Let u∈Rdu\in\mathbb{R}^{d}; by Discrete Fourier Analysis on the Lattice Torus: Counting, Orthogonality, Inversion, Parseval, and the Spin Sum §count-sites, a sum over z∈Lz\in\mathbb{L} of a constant ss equals LnsL^{n}s.

(a) By Step 3(vi), v(u)=∑zf(ℓu(z))≥−Ln(ς/2+log⁡2)=−bv(u)=\sum_{z}f(\ell_{u}(z))\ge-L^{n}(\varsigma/2+\log2)=-b; this is Admissible Cylindrical Potentials on a Hilbert Space in the Noise Geometry §below.

(b) Let ξ∈Rd\xi\in\mathbb{R}^{d}. By (V), expanding as in (Q),

∑j=1d∑k=1d∂j∂kv(u) ξjξk=∑z∈Lf′′(ℓu(z)) ℓξ(z)2≥−Kς∑z∈Lℓξ(z)2=−Kς∑j=1dχ(j)ξj2aj≥−Kς∑j=1dξj2aj,\sum_{j=1}^{d}\sum_{k=1}^{d}\partial_{j}\partial_{k}v(u)\,\xi_{j}\xi_{k}=\sum_{z\in\mathbb{L}}f''(\ell_{u}(z))\,\ell_{\xi}(z)^{2}\ge-K_{\varsigma}\sum_{z\in\mathbb{L}}\ell_{\xi}(z)^{2}=-K_{\varsigma}\sum_{j=1}^{d}\chi(j)\frac{\xi_{j}^{2}}{a_{j}}\ge-K_{\varsigma}\sum_{j=1}^{d}\frac{\xi_{j}^{2}}{a_{j}},

by Step 3(vi) with ℓξ(z)2≥0\ell_{\xi}(z)^{2}\ge0, by (Q), and since 0≤χ(j)≤10\le\chi(j)\le1, ξj2/aj≥0\xi_{j}^{2}/a_{j}\ge0 and Kς≥0K_{\varsigma}\ge0. This is Admissible Cylindrical Potentials on a Hilbert Space in the Noise Geometry §semiconvex.

(c) By (V) and (P) with F=f′∘ℓuF=f'\circ\ell_{u}, then Step 3(vi),

∑k=1dak(∂kv(u))2=∑z∈Lf′(ℓu(z))2≤2ς2∑z∈Lℓu(z)2+2Ln.\sum_{k=1}^{d}a_{k}\bigl(\partial_{k}v(u)\bigr)^{2}=\sum_{z\in\mathbb{L}}f'(\ell_{u}(z))^{2}\le\frac{2}{\varsigma^{2}}\sum_{z\in\mathbb{L}}\ell_{u}(z)^{2}+2L^{n}.

The second bound on ff in Step 3(vi) gives t2≤4ς(f(t)+ς+log⁡2)t^{2}\le4\varsigma(f(t)+\varsigma+\log2), so ∑zℓu(z)2≤4ς(v(u)+Ln(ς+log⁡2))\sum_{z}\ell_{u}(z)^{2}\le4\varsigma\bigl(v(u)+L^{n}(\varsigma+\log2)\bigr). Hence, with A=8Ln(ς+log⁡2)/ς+2Ln>0A=8L^{n}(\varsigma+\log2)/\varsigma+2L^{n}>0 and C=8/ς+AC=8/\varsigma+A,

∑k=1dak(∂kv(u))2≤8ςv(u)+A≤8ς∣v(u)∣+A≤C(1+∣v(u)∣)≤C(1+∣v(u)∣)2,\sum_{k=1}^{d}a_{k}\bigl(\partial_{k}v(u)\bigr)^{2}\le\frac{8}{\varsigma}v(u)+A\le\frac{8}{\varsigma}|v(u)|+A\le C\bigl(1+|v(u)|\bigr)\le C\bigl(1+|v(u)|\bigr)^{2},

the last since 1≤1+∣v(u)∣1\le1+|v(u)|. This is Admissible Cylindrical Potentials on a Hilbert Space in the Noise Geometry §slope.

(d) For k∈[d]k\in[d] and z∈Lz\in\mathbb{L}, akωk(z)2=L−nχ(k)ψκ(k)(z)2a_{k}\omega_{k}(z)^{2}=L^{-n}\chi(k)\psi_{\kappa(k)}(z)^{2} (Step 0), so by (R) and (D), ∑k=1dakωk(z)2=L−n∑l∈Γψl(z)2=1\sum_{k=1}^{d}a_{k}\omega_{k}(z)^{2}=L^{-n}\sum_{l\in\Gamma}\psi_{l}(z)^{2}=1. Hence by (V) and Step 3(vi),

∑k=1dak ∂k∂kv(u)=∑z∈Lf′′(ℓu(z))∑k=1dakωk(z)2=∑z∈Lf′′(ℓu(z))≤Lnς.\sum_{k=1}^{d}a_{k}\,\partial_{k}\partial_{k}v(u)=\sum_{z\in\mathbb{L}}f''(\ell_{u}(z))\sum_{k=1}^{d}a_{k}\omega_{k}(z)^{2}=\sum_{z\in\mathbb{L}}f''(\ell_{u}(z))\le\frac{L^{n}}{\varsigma}.

For positive ε\varepsilon put Cε=Ln/ς>0C_{\varepsilon}=L^{n}/\varsigma>0; since ε∑kak(∂kv(u))2≥0\varepsilon\sum_{k}a_{k}(\partial_{k}v(u))^{2}\ge0 and 1+∑kuk2≥11+\sum_{k}u_{k}^{2}\ge1, the right side of Admissible Cylindrical Potentials on a Hilbert Space in the Noise Geometry §curvature is at least CεC_{\varepsilon}, which proves (d).

So VV is an admissible cylindrical potential with head dimension dd, profile vv and semiconvexity constant KςK_{\varsigma}, and bb serves in (a). This proves claim 2.

Step 5 (Claim 3). Let x∈Xx\in X, u=pd(x)u=p_{d}(x) and F=f′∘φx=f′∘ℓuF=f'\circ\varphi_{x}=f'\circ\ell_{u} (Step 0), and let w=∇aV(x)=∑k=1dak∂kv(u) ekw=\nabla_{a}V(x)=\sum_{k=1}^{d}a_{k}\partial_{k}v(u)\,e_{k} (Admissible Cylindrical Potentials on a Hilbert Space in the Noise Geometry §gradient) and y=EMF∈Xy=\mathcal{E}_{M}F\in X (The White-Noise Embedding of Lattice Fields into the Negative Sobolev Space of the Torus, and the Site Field of a Distribution §embedding). For i∈Ni\in\mathbb{N}, the orthonormality of (ej)(e_{j}) (White Noise in the Square-Integrable Space and the Free Field on the Torus as Noise Weights and a Variance Sequence on a Negative Sobolev Space §basis) gives wi=⟨w,ei⟩H−m=ai∂iv(u)w_{i}=\langle w,e_{i}\rangle_{H^{-m}}=a_{i}\partial_{i}v(u) if i≤di\le d and wi=0w_{i}=0 if i>di>d. By (V), (F) and Step 0, for i≤di\le d with χ(i)=1\chi(i)=1,

ai∂iv(u)=aiai−1/2L−n/2∑z∈LF(z)ψκ(i)(z)=ai1/2Ln/2F^(κ(i))=ai1/2 y(κ(i)),a_{i}\partial_{i}v(u)=a_{i}a_{i}^{-1/2}L^{-n/2}\sum_{z\in\mathbb{L}}F(z)\psi_{\kappa(i)}(z)=a_{i}^{1/2}L^{n/2}\hat{F}(\kappa(i))=a_{i}^{1/2}\,y(\kappa(i)),

while ai∂iv(u)=0a_{i}\partial_{i}v(u)=0 if χ(i)=0\chi(i)=0. On the other hand yi=ai1/2y(κ(i))y_{i}=a_{i}^{1/2}y(\kappa(i)) by The White-Noise Embedding of Lattice Fields: Linearity, Inversion by the Site Field, the Site Sum as the White-Noise Norm, and Coordinates §coordinates, and y(κ(i))=0y(\kappa(i))=0 whenever κ(i)∉Γ\kappa(i)\notin\Gamma. By Step 0, therefore, wi=yiw_{i}=y_{i} for every i∈Ni\in\mathbb{N}. Applying The White-Noise Embedding of Lattice Fields: Linearity, Inversion by the Site Field, the Site Sum as the White-Noise Norm, and Coordinates §coordinates to ww and yy, w(κ(i))=ai−1/2wi=ai−1/2yi=y(κ(i))w(\kappa(i))=a_{i}^{-1/2}w_{i}=a_{i}^{-1/2}y_{i}=y(\kappa(i)) for every ii; as κ\kappa is onto Zn\mathbb{Z}^{n}, the coefficient families ww and yy agree at every k∈Znk\in\mathbb{Z}^{n} (The Free Field on the Torus as the Gaussian Reference Measure, with Square-Integrable White Noise: Standing Notation §data), so ∇aV(x)=EM(f′∘φx)\nabla_{a}V(x)=\mathcal{E}_{M}(f'\circ\varphi_{x}). With Step 3(iv) this proves claim 3.

Step 6 (Claim 4). Write c′=cJ,ηc'=c^{J,\eta}; c(ς)c^{(\varsigma)} and c′c' are variance sequences (Step 2 and The Hubbard-Stratonovich Transform of the Ising Measure on the Lattice Torus §variances), with truncations (c(ς))(N)(c^{(\varsigma)})^{(N)} and c′(N)c'^{(N)} (Variance Sequences and Their Truncations §truncations); push-forwards, image measures and measures with densities are those of Borel Probability Measures on a Real Hilbert Space with an Orthonormal Basis: Standing Notation §pushforward and Image Measures, Measures with Densities, and Change of Variables. A map between Euclidean spaces or XX that is continuous is Borel by claim 3 of Borel Measurability and Bounded Integration on a Metric Space; exp⁡\exp is continuous by claim 3 of Basic Properties of the Exponential Function and Differentiability at an Interior Point Implies Continuity There, and the coordinate maps pNp_{N} are Borel by Borel Sets of a Hilbert Space with an Orthonormal Basis: Coordinates, Determination by Finite-Dimensional Projections, and Pairs §continuity.

(i) The density. Let G:X→RG:X\to\mathbb{R}, G(x)=exp⁡(−12ς∑z∈Lφx(z)2)G(x)=\exp\bigl(-\frac{1}{2\varsigma}\sum_{z\in\mathbb{L}}\varphi_{x}(z)^{2}\bigr). It is positive (claim 2 of Basic Properties of the Exponential Function), at most 11 (claim 4 there), and continuous, hence Borel: each x↦φx(z)x\mapsto\varphi_{x}(z) is continuous by The White-Noise Embedding of Lattice Fields: Linearity, Inversion by the Site Field, the Site Sum as the White-Noise Norm, and Coordinates §site-continuous, so is its square by Continuity of Sums and Products of Real-Valued Functions on a Metric Space §on-set, the finite sum x↦∑z∈Lφx(z)2x\mapsto\sum_{z\in\mathbb{L}}\varphi_{x}(z)^{2} over the nonempty finite set L\mathbb{L} is continuous by Finite Linear Combinations of Continuous Real-Valued Maps on a Metric Space are Continuous §continuous (all coefficients 11), its multiple by −1/(2ς)-1/(2\varsigma) by Continuity of Sums and Products of Real-Valued Functions on a Metric Space §on-set, and its composite with exp⁡\exp by claim 3 of Semicontinuity and Continuity Under Composition with a Continuous Map. For N∈NN\in\mathbb{N} with d≤Nd\le N, (Q) gives G=GN∘pNG=G_{N}\circ p_{N} with GN:RN→RG_{N}:\mathbb{R}^{N}\to\mathbb{R}, GN(u)=exp⁡(−∑i=1Nϵiui2/(2ςai))G_{N}(u)=\exp\bigl(-\sum_{i=1}^{N}\epsilon_{i}u_{i}^{2}/(2\varsigma a_{i})\bigr), where ϵi=1\epsilon_{i}=1 if κ(i)∈Γ\kappa(i)\in\Gamma and ϵi=0\epsilon_{i}=0 otherwise (so ϵi=χ(i)\epsilon_{i}=\chi(i) for i≤di\le d and ϵi=0\epsilon_{i}=0 for i>di>d, Step 0); GNG_{N} is continuous for the Euclidean distance, hence Borel: each coordinate function u↦uiu\mapsto u_{i} is 11-Lipschitz (∣ui−ui′∣≤∥u−u′∥|u_{i}-u'_{i}|\le\lVert u-u'\rVert), hence continuous, so u↦ui2u\mapsto u_{i}^{2} is continuous by Continuity of Sums and Products of Real-Valued Functions on a Metric Space §on-set, the map u↦∑i=1N(−ϵi/(2ςai))ui2u\mapsto\sum_{i=1}^{N}\bigl(-\epsilon_{i}/(2\varsigma a_{i})\bigr)u_{i}^{2}, a finite sum over the nonempty finite set [N][N], is continuous by Finite Linear Combinations of Continuous Real-Valued Maps on a Metric Space are Continuous §continuous (with coefficients bi=−ϵi/(2ςai)b_{i}=-\epsilon_{i}/(2\varsigma a_{i})), and its composite with exp⁡\exp by claim 3 of Semicontinuity and Continuity Under Composition with a Continuous Map; so 1BGN\mathbf{1}_{B}G_{N} is Borel for B∈B(RN)B\in\mathcal{B}(\mathbb{R}^{N}). By (S) and Step 2, 1/ci′=1/ci(ς)+ϵi/(ςai)1/c'_{i}=1/c^{(\varsigma)}_{i}+\epsilon_{i}/(\varsigma a_{i}) for every i∈Ni\in\mathbb{N}. Hence, with the diagonal Gaussian densities ρ(c(ς))(N)\rho_{(c^{(\varsigma)})^{(N)}} and the numbers Z(c(ς))(N)Z_{(c^{(\varsigma)})^{(N)}} of The Diagonal Gaussian Density on Euclidean Space and Its Notation §density and claim 1 of Basic Properties of the Exponential Function,

GN(u) ρ(c(ς))(N)(u)=exp⁡(−12∑i=1Nui2ci′−Z(c(ς))(N))=θN ρc′(N)(u),θN=exp⁡(Zc′(N)−Z(c(ς))(N))>0.G_{N}(u)\,\rho_{(c^{(\varsigma)})^{(N)}}(u)=\exp\Bigl(-\frac{1}{2}\sum_{i=1}^{N}\frac{u_{i}^{2}}{c'_{i}}-Z_{(c^{(\varsigma)})^{(N)}}\Bigr)=\theta_{N}\,\rho_{c'^{(N)}}(u),\qquad\theta_{N}=\exp\bigl(Z_{c'^{(N)}}-Z_{(c^{(\varsigma)})^{(N)}}\bigr)>0 .

Let B∈B(RN)B\in\mathcal{B}(\mathbb{R}^{N}). By claim 2 of Image Measures, Measures with Densities, and Change of Variables, (pN)#γc(ς)=γ(c(ς))(N)(p_{N})_{\#}\gamma_{c^{(\varsigma)}}=\gamma_{(c^{(\varsigma)})^{(N)}} (Diagonal Gaussian Measures on a Hilbert Space §measure), claim 3 of Image Measures, Measures with Densities, and Change of Variables for γ(c(ς))(N)\gamma_{(c^{(\varsigma)})^{(N)}}, the measure with density ρ(c(ς))(N)\rho_{(c^{(\varsigma)})^{(N)}} with respect to Lebesgue measure λN\lambda_{N} (Diagonal Gaussian Measures on Euclidean Space §measure), and Linearity and Monotonicity of the Lebesgue Integral §nonnegative,

∫X1pN−1(B)G dγc(ς)=∫X(1BGN)∘pN dγc(ς)=∫RN1BGN ρ(c(ς))(N) dλN=θN γc′(N)(B).(H)\int_{X}\mathbf{1}_{p_{N}^{-1}(B)}G\,d\gamma_{c^{(\varsigma)}}=\int_{X}(\mathbf{1}_{B}G_{N})\circ p_{N}\,d\gamma_{c^{(\varsigma)}}=\int_{\mathbb{R}^{N}}\mathbf{1}_{B}G_{N}\,\rho_{(c^{(\varsigma)})^{(N)}}\,d\lambda_{N}=\theta_{N}\,\gamma_{c'^{(N)}}(B).\tag{H}

With B=RNB=\mathbb{R}^{N}, ZG=∫XG dγc(ς)=θNZ_{G}=\int_{X}G\,d\gamma_{c^{(\varsigma)}}=\theta_{N}, a positive real number, γc′(N)\gamma_{c'^{(N)}} being a probability measure.

(ii) Identification of γc′\gamma_{c'}. Let ν\nu be the measure with density G/ZGG/Z_{G} with respect to γc(ς)\gamma_{c^{(\varsigma)}} (claim 3 of Image Measures, Measures with Densities, and Change of Variables); by Linearity and Monotonicity of the Lebesgue Integral §nonnegative, ν(A)=ZG−1∫X1AG dγc(ς)\nu(A)=Z_{G}^{-1}\int_{X}\mathbf{1}_{A}G\,d\gamma_{c^{(\varsigma)}}, so ν(X)=1\nu(X)=1 and ν∈P(X)\nu\in\mathcal{P}(X). For N≥dN\ge d, (H) and ZG=θNZ_{G}=\theta_{N} give (pN)#ν=γc′(N)(p_{N})_{\#}\nu=\gamma_{c'^{(N)}}. For N<dN<d, let π:Rd→RN\pi:\mathbb{R}^{d}\to\mathbb{R}^{N} keep the first NN coordinates; it is 11-Lipschitz for the Euclidean distances, hence Borel, and pN=π∘pdp_{N}=\pi\circ p_{d}; so, push-forwards composing since preimages do, (pN)#ν=π#(pd)#ν=π#γc′(d)=π#(pd)#γc′=(pN)#γc′=γc′(N)(p_{N})_{\#}\nu=\pi_{\#}(p_{d})_{\#}\nu=\pi_{\#}\gamma_{c'^{(d)}}=\pi_{\#}(p_{d})_{\#}\gamma_{c'}=(p_{N})_{\#}\gamma_{c'}=\gamma_{c'^{(N)}}, by Diagonal Gaussian Measures on a Hilbert Space §measure twice. By the uniqueness in Diagonal Gaussian Measures on a Hilbert Space §measure, ν=γc′\nu=\gamma_{c'}. Consequently, by claim 3 of Image Measures, Measures with Densities, and Change of Variables and Linearity and Monotonicity of the Lebesgue Integral §nonnegative, ∫XΦ dγc′=ZG−1∫XΦ G dγc(ς)\int_{X}\Phi\,d\gamma_{c'}=Z_{G}^{-1}\int_{X}\Phi\,G\,d\gamma_{c^{(\varsigma)}} for every Borel Φ:X→[0,∞)\Phi:X\to[0,\infty).

(iii) The Gibbs measure. Let ϱ=ϱJ,ηHS\varrho=\varrho^{\mathrm{HS}}_{J,\eta} be the density of The Hubbard-Stratonovich Transform Couples the Ising Measure and the Field Law: the Density of the Field Law, the Disintegration of the Joint Law, and Entropy Contraction under Both Kernels §density; it is positive and continuous, hence Borel. By that clause and claim 1 of Basic Properties of the Exponential Function, ϱ(x)=ϑexp⁡(∑zlch⁡(φx(z)))\varrho(x)=\vartheta\exp\bigl(\sum_{z}\operatorname{lch}(\varphi_{x}(z))\bigr) with ϑ=ZJ−1exp⁡(−ηLn/2)\vartheta=Z_{J}^{-1}\exp(-\eta L^{n}/2), which is positive because ϱ\varrho and exp⁡\exp are; so, by claim 1 of Basic Properties of the Exponential Function and the definition of ff,

ϱ(x) G(x)=ϑexp⁡(∑z∈L(lch⁡(φx(z))−φx(z)22ς))=ϑexp⁡(−V(x))=ϑ wV,1(x),\varrho(x)\,G(x)=\vartheta\exp\Bigl(\sum_{z\in\mathbb{L}}\Bigl(\operatorname{lch}(\varphi_{x}(z))-\frac{\varphi_{x}(z)^{2}}{2\varsigma}\Bigr)\Bigr)=\vartheta\exp\bigl(-V(x)\bigr)=\vartheta\,w_{V,1}(x),

with the weight wV,1w_{V,1} of The Gibbs Measure of an Admissible Cylindrical Potential Relative to a Diagonal Gaussian Measure §weight. For B∈B(X)B\in\mathcal{B}(X), by The Hubbard-Stratonovich Transform Couples the Ising Measure and the Field Law: the Density of the Field Law, the Disintegration of the Joint Law, and Entropy Contraction under Both Kernels §density, (ii) with Φ=1Bϱ\Phi=\mathbf{1}_{B}\varrho, and Linearity and Monotonicity of the Lebesgue Integral §nonnegative,

γJ,ηHS(B)=∫X1Bϱ dγc′=ϑZG∫X1B wV,1 dγc(ς).\gamma^{\mathrm{HS}}_{J,\eta}(B)=\int_{X}\mathbf{1}_{B}\varrho\,d\gamma_{c'}=\frac{\vartheta}{Z_{G}}\int_{X}\mathbf{1}_{B}\,w_{V,1}\,d\gamma_{c^{(\varsigma)}}.

For B=XB=X this reads 1=ϑZG−1ZV,11=\vartheta Z_{G}^{-1}Z_{V,1}, with the normaliser ZV,1Z_{V,1} of The Gibbs Measure of an Admissible Cylindrical Potential Relative to a Diagonal Gaussian Measure §normaliser; so ϑ/ZG=1/ZV,1\vartheta/Z_{G}=1/Z_{V,1} and γJ,ηHS(B)=γ1V(B)\gamma^{\mathrm{HS}}_{J,\eta}(B)=\gamma^{V}_{1}(B) by The Gibbs Measure of an Admissible Cylindrical Potential Relative to a Diagonal Gaussian Measure §gibbs, VV being admissible by claim 2 with bb as there. This proves claim 4.

Step 7 (Claim 5). Let ς,ς′\varsigma,\varsigma' be admissible splits; for s∈{ς,ς′}s\in\{\varsigma,\varsigma'\} write rk(s)r^{(s)}_{k}, c(s)c^{(s)}, Vs=vs∘pdV_{s}=v_{s}\circ p_{d} (Step 4) and ρs=γc(s)\rho_{s}=\gamma_{c^{(s)}}, and use the reading of the statement with ss. By claim 1, ck(s)≤rˉsakc^{(s)}_{k}\le\bar{r}_{s}a_{k} for every kk, with rˉs≥1>0\bar{r}_{s}\ge1>0; so the hypotheses of The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §hypothesis and The Gaussian Entropy Pair on the Noise Wasserstein Space: Relative Entropy and the Noise Score Field §hypothesis hold with the constant rˉs\bar{r}_{s}, and the Gibbs entropy pair (Ds,DΣs,Es,Σs)(\mathcal{D}^{s},\mathcal{D}^{s}_{\Sigma},\mathcal{E}^{s},\Sigma^{s}) with potential VsV_{s} (admissible by claim 2) and temperature 11 is defined (The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §pair).

(i) The noise-connected measures. Apply Changing the Variances of a Diagonal Gaussian Reference by a Diagonal Quadratic: the Same Measures and Domains, with Penalty and Score Shifted by a Diagonal Quadratic Profile in the reading with ς\varsigma, with β=1\beta=1, its constant rˉς\bar{r}_{\varsigma}, and the sequence written dd there taken to be δ=(δk)k∈N\delta=(\delta_{k})_{k\in\mathbb{N}}, δk=ϵk(1/ς−1/ς′)/ak\delta_{k}=\epsilon_{k}(1/\varsigma-1/\varsigma')/a_{k}, with ϵk\epsilon_{k} as in Step 6(i). It is admissible in the sense of Diagonal Quadratic Profiles on the Noise Wasserstein Space: Moment Bounds, a Lipschitz Estimate, the Gradient Field, and Noise Intrinsic Test Functions §admissible: the terms ∣δk∣ck(ς)|\delta_{k}|c^{(\varsigma)}_{k} vanish for k>dk>d (Step 0), so the partial sums of ∑k∣δk∣ck(ς)\sum_{k}|\delta_{k}|c^{(\varsigma)}_{k} are constant from dd on and the series converges (Series of Real Numbers §convergent); and ∣δk∣ak≤Δ|\delta_{k}|a_{k}\le\Delta with Δ=∣1/ς−1/ς′∣≥0\Delta=|1/\varsigma-1/\varsigma'|\ge0. By (S), if κ(k)∈Γ\kappa(k)\in\Gamma then 1/ck(ς)+δk=(1/qκ(k)−1/ς+1/ς−1/ς′)/ak=1/ck(ς′)1/c^{(\varsigma)}_{k}+\delta_{k}=\bigl(1/\mathfrak{q}_{\kappa(k)}-1/\varsigma+1/\varsigma-1/\varsigma'\bigr)/a_{k}=1/c^{(\varsigma')}_{k}, and otherwise δk=0\delta_{k}=0 and ck(ς)=ck=ck(ς′)c^{(\varsigma)}_{k}=c_{k}=c^{(\varsigma')}_{k}. So 1/ck(ς)+δk=1/ck(ς′)>01/c^{(\varsigma)}_{k}+\delta_{k}=1/c^{(\varsigma')}_{k}>0, the sequence written c′c' there is c(ς′)c^{(\varsigma')}, and Changing the Variances of a Diagonal Gaussian Reference by a Diagonal Quadratic: the Same Measures and Domains, with Penalty and Score Shifted by a Diagonal Quadratic Profile §space gives Pρς′a=Pρςa\mathcal{P}^{a}_{\rho_{\varsigma'}}=\mathcal{P}^{a}_{\rho_{\varsigma}}.

(ii) Penalty domain and penalty. By The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §penalty-domain and The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §pair, Ds\mathcal{D}^{s} is the set of μ∈P(X)\mu\in\mathcal{P}(X) of finite relative entropy with respect to γ1Vs\gamma^{V_{s}}_{1} and Es(μ)=H(μ ∣ γ1Vs)\mathcal{E}^{s}(\mu)=H(\mu\,|\,\gamma^{V_{s}}_{1}); since γ1Vs=γJ,ηHS\gamma^{V_{s}}_{1}=\gamma^{\mathrm{HS}}_{J,\eta} by claim 4, Dς=Dς′\mathcal{D}^{\varsigma}=\mathcal{D}^{\varsigma'} is the set described in claim 5, and Eς=Eς′=H(⋅ ∣ γJ,ηHS)\mathcal{E}^{\varsigma}=\mathcal{E}^{\varsigma'}=H(\cdot\,|\,\gamma^{\mathrm{HS}}_{J,\eta}). Write D\mathcal{D} for this set.

(iii) A split-free identity. For k∈Nk\in\mathbb{N} and x∈Xx\in X, with ∂kVs\partial_{k}V_{s} as in Admissible Cylindrical Potentials on a Hilbert Space in the Noise Geometry §gradient,

xkck(ς)+∂kVς(x)=xkck(ς′)+∂kVς′(x).(I)\frac{x_{k}}{c^{(\varsigma)}_{k}}+\partial_{k}V_{\varsigma}(x)=\frac{x_{k}}{c^{(\varsigma')}_{k}}+\partial_{k}V_{\varsigma'}(x).\tag{I}

Let u=pd(x)u=p_{d}(x) and, for k∈[d]k\in[d], Tk(u)=∑zτ(ℓu(z))ωk(z)T_{k}(u)=\sum_{z}\tau(\ell_{u}(z))\omega_{k}(z), which does not involve the split. If κ(k)∈Γ\kappa(k)\in\Gamma, then k≤dk\le d, χ(k)=1\chi(k)=1 and uk=xku_{k}=x_{k}, and by (V), Step 3(iv) and (Q), ∂kvs(u)=1s∑zℓu(z)ωk(z)−Tk(u)=xks ak−Tk(u)\partial_{k}v_{s}(u)=\frac{1}{s}\sum_{z}\ell_{u}(z)\omega_{k}(z)-T_{k}(u)=\frac{x_{k}}{s\,a_{k}}-T_{k}(u); so by (S) both sides of (I) equal xk/ckJ,η−Tk(u)x_{k}/c^{J,\eta}_{k}-T_{k}(u). If k≤dk\le d and χ(k)=0\chi(k)=0, then ∂kVs(x)=∂kvs(u)=0\partial_{k}V_{s}(x)=\partial_{k}v_{s}(u)=0 (Step 4), and if k>dk>d, ∂kVs(x)=0\partial_{k}V_{s}(x)=0 by definition; in both cases κ(k)∉Γ\kappa(k)\notin\Gamma and ck(s)=ckc^{(s)}_{k}=c_{k}, so both sides equal xk/ckx_{k}/c_{k}.

(iv) Score domain. Let μ∈D\mu\in\mathcal{D}. By Entropy and Score Relative to the Gibbs Measure Split into Their Gaussian Parts and the Potential, with a Fisher Information Bound §domain, in each reading, μ∈P2(X)\mu\in\mathcal{P}_{2}(X) and each ∂kVs\partial_{k}V_{s} is integrable with respect to μ\mu, so The Relative Score with Respect to the Gibbs Measure of an Admissible Cylindrical Potential applies to μ\mu for s=ςs=\varsigma and s=ς′s=\varsigma'. The class FCb1(X)\mathcal{F}C^{1}_{b}(X), the derivatives ∂kφ\partial_{k}\varphi and L2(μ)L^{2}(\mu) do not involve the variance sequence, and by (I) the integrands in The Relative Score with Respect to the Gibbs Measure of an Admissible Cylindrical Potential §score (with β=1\beta=1) coincide for the two splits. Hence μ\mu has a relative score with respect to γ1Vς\gamma^{V_{\varsigma}}_{1} if and only if it has one with respect to γ1Vς′\gamma^{V_{\varsigma'}}_{1}, and then, by the uniqueness in that clause, the components ζkV\zeta^{V}_{k} are the same. The series of The Weighted Fisher Information Relative to the Gibbs Measure of an Admissible Cylindrical Potential §information involves only these components and aa, so finite Fisher information relative to γ1Vς\gamma^{V_{\varsigma}}_{1} and relative to γ1Vς′\gamma^{V_{\varsigma'}}_{1} with weights aa are the same condition. By The Gibbs Entropy Pair on the Noise Wasserstein Space: Relative Entropy to the Gibbs Measure and the Gibbs Score Field §score-domain, DΣς=DΣς′\mathcal{D}^{\varsigma}_{\Sigma}=\mathcal{D}^{\varsigma'}_{\Sigma}.

(v) Score. Let μ∈DΣς\mu\in\mathcal{D}^{\varsigma}_{\Sigma} and s∈{ς,ς′}s\in\{\varsigma,\varsigma'\}. In the reading with ss, VsV_{s} is integrable with respect to μ\mu by Entropy and Score Relative to the Gibbs Measure Split into Their Gaussian Parts and the Potential, with a Fisher Information Bound §entropy, μ∈P2(X)\mu\in\mathcal{P}_{2}(X) by Entropy and Score Relative to the Gibbs Measure Split into Their Gaussian Parts and the Potential, with a Fisher Information Bound §domain, and by Entropy and Score Relative to the Gibbs Measure Split into Their Gaussian Parts and the Potential, with a Fisher Information Bound §splitting μ\mu has a relative score with respect to ρs\rho_{s}, finite Fisher information relative to ρs\rho_{s} with weights aa, and ∫X∣∇aVs∣a2 dμ<∞\int_{X}|\nabla_{a}V_{s}|_{a}^{2}\,d\mu<\infty. So Entropy and Score Relative to the Gibbs Measure Split into Their Gaussian Parts and the Potential, with a Fisher Information Bound §field (with β=1\beta=1) shows that Σs(μ)=Zμa+∇aVs\Sigma^{s}(\mu)=Z^{a}_{\mu}+\nabla_{a}V_{s}, an element of L2(μ;Xa)L^{2}(\mu;X^{a}), which does not involve the variance sequence, has coordinate ak1/2ζkVa_{k}^{1/2}\zeta^{V}_{k} along fkf_{k} for every kk, with the split-independent ζkV\zeta^{V}_{k} of (iv). By The Space of Square-Integrable Hilbert-Valued Maps is a Real Hilbert Space: Coordinates and Synthesis §coordinates the series ∑k∥ak1/2ζkV∥L2(μ)2\sum_{k}\lVert a_{k}^{1/2}\zeta^{V}_{k}\rVert_{L^{2}(\mu)}^{2} converges, so by the uniqueness in The Space of Square-Integrable Hilbert-Valued Maps is a Real Hilbert Space: Coordinates and Synthesis §synthesis, Σς(μ)=Σς′(μ)\Sigma^{\varsigma}(\mu)=\Sigma^{\varsigma'}(\mu).

By (i) to (v), Pρςa=Pρς′a\mathcal{P}^{a}_{\rho_{\varsigma}}=\mathcal{P}^{a}_{\rho_{\varsigma'}} and the two Gibbs entropy pairs are the same quadruple, with D\mathcal{D} and E\mathcal{E} as stated. This proves claim 5.

Citations

Loading…

Dependencies

Uses0

Loading…

Comments

Log in to comment.

Loading…