Fluid-like entropy and equilibrium statistical mechanics of self-gravitating systems
Dong-Biao Kang, Ping He

TL;DR
This paper advances the understanding of self-gravitating systems by using a fluid-like entropy approach with improved extremizing methods, resulting in realistic density profiles consistent with observations and proposing a hybrid entropy model.
Contribution
It introduces an improved extremizing process for fluid-like entropy in self-gravitating systems, producing finite mass and energy density profiles aligned with observational data.
Findings
Derived density profiles with finite mass and energy
Profiles consistent with elliptical galaxy NGC 3379 observations
Proposed hybrid entropy model combining Boltzmann-Gibbs and Tsallis entropy
Abstract
The statistical mechanics of self-gravitating systems has not been well understood, and still remains an open question so far. In a previous study by Kang & He, we showed that the fluid approximation may give a clue to further investigate this problem. In fact, there are indeed many dynamical similarities between self-gravitating and fluid systems. Based on a fluid-like entropy, that work explained successfully the outer density profiles of dark matter halos, but there left some drawbacks with the calculation concerning extremizing process of the entropy. In the current paper, with the improved extremizing calculation -- including an additional differential constraint of dynamical equilibrium and without any other assumptions, we confirm that statistical-mechanical methods can give a density profile with finite mass and finite energy. Moreover, this density profile is also consistent…
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