Energy-Dependent Topological Black Holes in Massive Gravity Coupled to Double-Logarithmic Electrodynamics

TL;DR

This paper explores the properties of nonlinear magnetized black holes in massive gravity's rainbow with double-logarithmic electrodynamics, analyzing their horizons, thermodynamics, and stability.

Contribution

It introduces new anti-de Sitter black hole solutions in massive gravity coupled with nonlinear electrodynamics, considering rainbow functions and graviton effects.

Findings

Massive gravity and nonlinearity affect black hole horizons.

Thermodynamic quantities are derived and analyzed.

Stability conditions depend on rainbow functions and nonlinearity.

Abstract

In this paper, I investigate the nonlinear magnetized black holes of massive gravity's rainbow. In order to achieve this, I use the double-logarithmic electromagnetic field as a matter source and derive the new anti-de Sitter black hole solution. The effects of the massive graviton, rainbow functions, and nonlinearity of the electromagnetic field on the black hole's inner and outer horizons are also studied. The black hole's thermodynamic properties are studied, and the mathematical expressions for temperature, heat capacity, and Gibbs free energy are found. The extended first law and Smarr's formula are derived as well. Using the behaviour of thermodynamic quantities as a starting point, I also study the local and global thermodynamic stabilities.