The influence of a curved spacetime M on the physical behavior of an ideal gas of N
particles is analyzed by considering the phase space of the system as a region of the …

We attempt to construct a (two-dimensional) statistical mechanics description of the scenario
in which the experiment in [T. Westphal et al., Nature 591, 225 (2021)] was made. It includes …

We discuss the clustering of core halo-galaxies of radius predicted by gravitational lensing.
We appeal to a blend of recent (1) mathematical results and (2) statistical mechanics …

Using the potential associated with NFW mass profile (Navarro et al. in Mon. Not. R. Astron.
Soc. 402: 21, 2010) enclosed at scale radius rs r_s, we calculate the partition function of the …

We studied galaxy clustering in the light of a modified theory of gravity motivated by a
logarithmic correction term. We solved the problem of divergence of the configurational …

The purpose of this paper is to study the main thermodynamic functions for two-dimensional
gravity and three-dimensional one. The cases treated here refer to extended mass located at …

We develop a statistical physics' picture of classical Newtonian gravitation and uncover
rather notable entropic features. In particular, applying the classical canonical ensemble …

We consider a model for galaxies with halo advanced by Tohline. With it we discuss galaxy
clusters withinthe strictures of Gibbs' ensembles in statistical mechanics. We consider (1) the …

We present a novel perspective on the Schwarzschild black hole solution, a cornerstone of
general relativity, by employing a distributional approach. The conventional solution is …

We consider a model for galaxies with halo advanced by Tohline. With it we discuss galaxy
clusters within the strictures of Gibbs' ensembles in statistical mechanics. We consider (1) …