Gravitational partition function modified by super-light brane world perturbative modes

TL;DR

This paper investigates how super-light brane world modes modify gravitational interactions and galaxy clustering, using statistical methods to derive a finite partition function and analyze thermodynamic stability.

Contribution

It introduces a regularized partition function for galaxy systems in brane world models, accounting for large-distance gravity modifications and analyzing thermodynamic stability.

Findings

Large galaxy numbers may cause thermodynamic instability.

Modified potential affects galaxy clustering behavior.

Finite partition function is derived for the brane world model.

Abstract

In this paper, we will analyze the effects of super-light brane world perturbative modes on clustering of galaxies. In present manuscript, we use the Boltzmann and Tsallis statistical approaches to study the large distance modification of gravity in the brane world. The impact of modified potential on clustering of galaxies is analyzed in both the approaches. The infinities associated with Newtonian point mass approximation of gravity models is removed using the analytical extensions. The regularized and finite partition function is obtained for the system of galaxies in the brane world model and is used to evaluate the regularized thermodynamic properties of the system in the form of equations of state. Hence, we study thermodynamic quantities and discuss about the thermodynamic stability of the model. We find that large number of galaxies may lead to the thermodynamic instability.