Entropy Production in Collisionless Systems. II. Arbitrary Phase-Space Occupation Numbers
Eric I. Barnes (1), Liliya L.R. Williams (2) ((1) Univ. of Wisconsin -, La Crosse, (2) Univ. of Minnesota)

TL;DR
This paper compares two thermodynamic methods for determining equilibrium states of self-gravitating systems, extending previous analyses by avoiding Stirling approximation and applying to both collisionless and collisional models, finding that entropy production extremization yields maximum entropy configurations.
Contribution
It introduces a Stirling-approximation-free analysis of entropy maximization and production extremization for self-gravitating systems, unifying collisionless and collisional models under a common framework.
Findings
Entropy extremization leads to maximum entropy states.
Both Lynden-Bell and Maxwell-Boltzmann approaches produce the same equilibria.
The methods are valid for systems with finite mass and arbitrary phase-space occupation.
Abstract
We present an analysis of two thermodynamic techniques for determining equilibria of self-gravitating systems. One is the Lynden-Bell entropy maximization analysis that introduced violent relaxation. Since we do not use the Stirling approximation which is invalid at small occupation numbers, our systems have finite mass, unlike Lynden-Bell's isothermal spheres. (Instead of Stirling, we utilize a very accurate smooth approximation for .) The second analysis extends entropy production extremization to self-gravitating systems, also without the use of the Stirling approximation. In addition to the Lynden-Bell (LB) statistical family characterized by the exclusion principle in phase-space, and designed to treat collisionless systems, we also apply the two approaches to the Maxwell-Boltzmann (MB) families, which have no exclusion principle and hence represent collisional systems. We…
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