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Hard-core exclusion does not guarantee a finite unscaled-gravity limit

Statement refuted

Fix β>0 and consider the fixed-density sequence indexed by N=n3. Let VN be the box volume, ZN(β) the canonical partition function, and FN(β)=−β−1log⁡ZN(β). The per-particle free-energy density is fN=FN/N (in joules), and the per-volume free-energy density is gN=FN/VN (in joules per cubic metre). Here a “finite extensive free-energy density” means that the chosen normalized sequence has a finite real thermodynamic-limit value as n→∞. The claim refuted is that a fixed hard-core exclusion distance and fixed particle density guarantee this for the unscaled Newtonian long-range attraction.

Facts & Assumptions

Given: The unscaled point attraction −Gm2/r, a positive hard-core separation, and boxes with side proportional to N1/3.

[F1]

For N=n3, a cubic packing with fixed minimum separation still has interaction energy at most −c0N5/3 on positive-volume position sets, and its canonical free energy per particle tends to −∞. (Point collapse and unscaled gravity nonextensivity)

Counterexample

1.1givenF1construct

Fix a grid spacing larger than the hard-core radius and take N=n3 particles, one in each small cube around the cubic grid sites. The enclosing box has side proportional to n=N1/3 and the product of the small cubes is an admissible positive-volume position set, matching [F1].

2.1F1step 1.1algebra∎

By [F1], fN=FN/N=−β−1log⁡ZN/N→−∞. Here VN=∣Bn∣=d3N, so gN=FN/VN=d−3fN→−∞. Neither normalization has a finite real thermodynamic-limit value, contradicting the claimed guarantee.

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