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Continuous ideal-gas bulk limit and finite-block bridge

Statement

Assume the Axiom of Countable Choice (The Axiom of Countable Choice (ACω)). Fix dimension d≥1, particle mass m>0, action reference h>0, inverse energy β>0, and positive cube volumes VN with N/VN→ρ∈(0,∞). For N indistinguishable classical noninteracting particles in a cube of volume VN, use the phase-space reference dq dp/(N!hdN) and Hamiltonian HN(q,p)=∑i=1N∣pi∣2/(2m). Define λβ=hβ/(2πm). Then the dimensionless partition integral and free-energy limits are ZN=VNNN!λβdN,−β−1log⁡ZNN⟶β−1[log⁡(ρλβd)−1],−β−1log⁡ZNVN⟶β−1ρ[log⁡(ρλβd)−1]. There is also the following finite-momentum-block limit. Let M=dN, let G1,…,GM be independent standard normal variables, set AN=M−1∑a=1MGa2, and define canonical momenta Pacan=m/β Ga and shell-prepared momenta Pash=m/β Ga/AN. On the null event AN=0, set the shell-prepared vector to (mM/β,0,…,0). The shell-prepared vector has exactly energy dN/(2β), and for every fixed r and bounded continuous ψ:Rr→R, Eψ(P1sh,…,Prsh)⟶Eψ(P1can,…,Prcan). This is weak convergence for each fixed block in this free-particle model. The shell preparation is the stated normalized-Gaussian construction, and no finite-width shell or interacting-gas equivalence is asserted.

Facts & Assumptions

Given: The free-particle Hamiltonian, phase-space normalization, and normalized-Gaussian shell preparation.

[A1]

Assume the Axiom of Countable Choice (The Axiom of Countable Choice (ACω)), as required by the Lebesgue-measure construction and change-of-variables suppliers below. d,N≥1, m,h,β,VN>0, N/VN→ρ∈(0,∞), and the N-particle Hamiltonian is additive kinetic energy in a cubic position box.

[A2]

For the block limit, the Ga are independent with density (2π)−1/2e−x2/2 and r is fixed while N→∞.

[F2]

The product measure of two sigma-finite measure spaces and For sigma-finite factors, the product measure exists, has the rectangle formula, is sigma-finite, and is unique: finite products of the sigma-finite Lebesgue factors carry the rectangular product measure. The Euclidean Lebesgue measure is the completion of the product of the factor Lebesgue measures identifies its completion with Euclidean Lebesgue measure, so the displayed Borel densities have the same integrals in either convention.

[F3]

Tonelli's theorem for nonnegative measurable functions on a sigma-finite product and Fubini's theorem for L^1 functions on a sigma-finite product: nonnegative product integrals factor by Tonelli; integrable products may be evaluated iteratively.

[F4]

The Gaussian integral ∫−∞∞e−x2 dx=π: the improper Riemann Gaussian integral is ∫−∞∞e−x2 dx=π. A nonnegative improper Riemann integral on a half-line agrees with the Lebesgue integral identifies each convergent nonnegative improper integral on [0,∞) with its Lebesgue integral. Apply it to the continuous even Gaussian and its even polynomial moments; reflection gives the negative half-line. Thus the improper integral evaluations below also evaluate their Lebesgue integrals.

[F7]

If u,v are differentiable on [a,b] with u′,v′ integrable, then ∫abuv′=u(b)v(b)−u(a)v(a)−∫abu′v: on each finite interval, differentiable factors with integrable derivatives obey the ordinary integration-by-parts identity.

[F8]

The exponential dominates every fixed nonnegative integer power at +∞: Rke−R2/2→0 for each fixed nonnegative integer k, by setting x=R2/2 and bounding xk/2 by a larger integer power.

Proof

Given: [A1] and, for the second conclusion, [A2].

1.1A1F1F2F3F4F5

The integrand is nonnegative, so [F3] factors the position and momentum integrals: ZN=1N!hdN∫ΛNN∫RdNe−β∑i∣pi∣2/(2m) dp dq=VNNN!hdN(∫Re−βp2/(2m) dp)dN. By [F4]–[F5] the one-coordinate integral is 2πm/β, proving the stated exact formula with λβ=hβ/(2πm). The dimensions are consistent: λβ is a length, so VNN/λβdN and ZN are dimensionless.

1.2A2F1F2F3F4F5F7F8algebra

Let G have the density in [A2]. By [F4]–[F5], it is normalized. The polynomial and Gaussian factors have continuous derivatives on every finite interval, so apply [F7] on [−R,R] first with u(x)=x, v′(x)=xe−x2/2, and then with u(x)=x3, v′(x)=xe−x2/2. In each case v(x)=−e−x2/2. Letting R→∞, the endpoint terms vanish by [F8], giving EG2=1 and EG4=3. Thus E(G2−1)=0 and E(G2−1)2=2. The independence in [A2] and [F3] factor the cross integrals, so expanding the square gives E(AN−1)2=M−2∑a=1M2=2/M. For any η>0, η21{∣AN−1∣>η}≤(AN−1)2, so integration proves P(∣AN−1∣>η)≤2/(Mη2)→0. Hence AN→1 in probability.

2.1A1F6step 1.1algebra

Monotonicity of log⁡ from [F6] gives ∫1Nlog⁡x dx≤log⁡N!≤∫1N+1log⁡x dx, hence log⁡N!=Nlog⁡N−N+O(log⁡(N+1)). Again by [F6], 0≤log⁡x=∫1xdt/t≤2x for x≥1, so log⁡(N+1)/N≤2N+1/N→0. Substituting the exact ZN yields N−1log⁡ZN=log⁡(VN/N)+1−dlog⁡λβ+o(1)→−log⁡ρ+1−dlog⁡λβ. Multiplication by −β−1 proves the per-particle limit; multiplying by N/VN→ρ proves the per-volume limit.

2.2A2step 1.2

Since AN>0 almost surely, the shell-prepared formulas define random variables on a probability-one set. On the null event AN=0, assign the fixed shell vector (mM/β,0,…,0); this measurable extension leaves every expectation unchanged and has the same stated energy. On AN>0, algebra gives ∑a=1dN(Pash)22m=12βAN∑aGa2=M2β=dN2β. This exact energy constraint holds on every outcome where AN>0, an event of probability one since the joint Gaussian density assigns zero mass to the origin.

2.3A2F1F3F9step 1.2

For fixed r, the scalar multiplier AN−1/2 tends to 1 in probability by continuity at 1 and step 1.2. Therefore (P1sh,…,Prsh)−(P1can,…,Prcan) tends to zero in probability: restrict first to the event ∑a=1rGa2≤R2, where its norm is at most m/βR∣AN−1/2−1∣, and then bound the complement by P(∑a=1rGa2>R2)≤r/R2 using the second moment. For bounded continuous ψ, choose R so this tail is small and additionally restrict to ∣AN−1/2−1∣≤1, whose complement has probability tending to zero. On this event both blocks lie in the ball of radius 2m/βR. Use uniform continuity of ψ on the compact ball of radius 2m/βR, and then use convergence in probability of the difference. For any ϵ>0, choose δ>0 by that uniform continuity. The expectation difference is at most ϵ+2∥ψ∥∞[r/R2+P(∣AN−1/2−1∣>1)+P(∥P1:rsh−P1:rcan∥>δ)], with the multiplier assigned arbitrarily on its null exceptional event. Sending first N→∞ and then R→∞ proves the claimed expectation limit.

3.1A1A2F1step 2.3∎

If positions are included, choose them independently and uniformly in the same cube under both preparations. After coordinatewise rescaling by the side length, every fixed position block already has the same uniform law in both models and is independent of the momentum vector. The same bounded-continuous test argument as in 2.3, first on compact sets and then on their small tails, proves the joint fixed-block limit. This does not change the energy computation because the Hamiltonian has no position dependence.

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