AdS graviton stars and differential configurational entropy

TL;DR

This paper investigates the stability and properties of AdS graviton stars using differential configurational entropy, revealing stable configurations near neutron star densities through entropy analysis.

Contribution

It introduces a novel application of differential configurational entropy to analyze AdS graviton stars and identifies stability domains based on entropy minima.

Findings

Global minima of differential configurational entropy indicate stability regions.

AdS graviton stars exhibit stability near astrophysical neutron star densities.

The study provides insights into the stability and characteristics of graviton star solutions.

Abstract

AdS graviton stars are studied in the differential configurational entropy setup, as solutions of the effective Einstein field equations that backreact to compactification. With the critical central density of AdS graviton stars, the differential configurational entropy is derived and computed, presenting global minima for a wide range of stellar mass magnitude orders. It indicates insular domains of configurational stability for AdS graviton stars near astrophysical neutron star densities. Other relevant features are also reported.