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Superstable regular pair interactions and configurational ensemble notation

Definition

Assume AC. Fix an integer dimension d≥1, use the Euclidean norm ∣⋅∣2 from The Euclidean inner product ⟨x,y⟩=∑k<nxkyk on Rn, define ∣x∣∞=max⁡j∣xj∣, and use the numerical coordinate conventions in Poisson Configuration Reference. A finite configuration is a finite subset ω⊂Rd with no repeated points; its number of points is N(ω). A pair potential is an even Borel function, measurable for the Borel sigma-algebra generated by open sets (The Borel sigma-algebra of a topological space), ϕ:Rd→R∪{+∞}, where even means ϕ(−x)=ϕ(x). Define Hϕ(ω)=∑{x,y}⊂ωϕ(x−y),Hϕ(∅)=0. The sum is over unordered two-point subsets, so every term is evaluated at a nonzero separation; if any term is +∞, the sum is +∞.

The potential is stable if some B≥0 satisfies Hϕ(ω)≥−BN(ω) for every finite configuration. It is superstable in the Georgii splitting convention if ϕ=ϕs+ϕr, where ϕs is stable and ϕr≥0 everywhere and, for some r0,δ>0, ϕr(x)≥δ whenever ∣x∣∞≤r0. It is lower regular if a nonnegative nonincreasing ψ:[0,∞)→[0,+∞] satisfies ϕ(x)≥−ψ(∣x∣∞),∫0∞ψ(r)rd−1 dr<∞. It is regular if it is lower regular and, for some R<∞, ϕ(x)≤ψ(∣x∣∞) whenever ∣x∣∞≥R. These are the conventions used for the interacting results on this page. A genuine divergent positive core is the separate additional condition that some nonincreasing χ:(0,r1]→(0,∞) satisfies ϕ(x)≥χ(∣x∣∞) for 0<∣x∣∞≤r1 and ∫0r1χ(r)rd−1dr=+∞; it is not implied by superstability.

For L>0 put ΛL=[0,L)d, VL=Ld, and let HL,free be Hϕ for configurations restricted to ΛL. For a regular potential and sufficiently large periodic cubes, periodize ω⊂ΛL by ωper={x+Lk:x∈ω, k∈Zd} and set HL,per(ω)=12∑x∈ω∑y∈ωper, y≠xϕ(y−x), interpreting the value as +∞ if a positive infinite term occurs. Under this regularity hypothesis, the far image sum is absolutely convergent for all sufficiently large L by Diagonal gap for a decreasing integrable interaction tail ↗; this is the image convention used below. With fixed numerical length and energy units, the canonical positional partition is Z(L,N;β)=1N!∫ΛLNe−βHϕ(q1,…,qN)dq1⋯dqN,Z(L,0;β)=1, where the tuple notation means Hϕ(q1,…,qN):=Hϕ({q1,…,qN}) when the coordinates are distinct, and Hϕ(q1,…,qN):=+∞ on collision diagonals. The integrand is therefore zero on collisions; these diagonals have product Lebesgue measure zero by the no-collision construction in Poisson Configuration Reference, so this convention leaves all partition integrals unchanged. For N=0 the empty tuple has energy zero. Here β>0, and the grand partition is Ξ(L;a,β)=∑N≥0aNZ(L,N;β) for numerical activity a>0. The normalized unit-intensity Poisson version is ZQ(L;z,β)=EQΛL[zNΛLe−βHL,free]; since the Poisson density contributes e−VL, Ξ(L;z,β)=eVLZQ(L;z,β). A physical pressure identification is not part of this mathematical definition.

For a probability law P on the configuration space of Poisson Configuration Reference, stationarity means P∘Tx−1=P for every x∈Rd. When P is stationary and EPN[0,1)d<∞ (finite intensity), write ρ(P)=EPN[0,1)d. Use the finite-region relative entropy D defined in Relative Entropy of Probability Measures. If ϕ is stable with constant B, then HL,free≥−BNΛL, so the negative part of HL,free is P-integrable for every such P. Whenever the limit exists, write E(P)=lim⁡L→∞VL−1EPHL,free,I(P)=lim⁡L→∞VL−1D(PΛL∥QΛL). In the variational results below, Φ(P) denotes this same positional energy density: Φ(P):=E(P). The cited results establish existence under their stated hypotheses; this definition does not assume either limit exists for every stationary finite-intensity law.

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