Gravitational Analysis of Einstein-Non-Linear-Maxwell-Yukawa Black Hole under the Effect of Newman-Janis Algorithm

TL;DR

This paper explores the properties of a rotating Einstein-non-linear-Maxwell-Yukawa black hole using the Newman-Janis algorithm, analyzing Hawking radiation, temperature corrections, and entropy to understand its physical and stable characteristics.

Contribution

It introduces a novel analysis of the rotating Einstein-non-linear-Maxwell-Yukawa black hole using the Newman-Janis algorithm and Hamilton-Jacobi method for temperature correction.

Findings

Hawking temperature varies with spin parameter.

Corrected temperature and entropy depend on charge, rotation, and gravity.

Graphical analysis shows stability conditions of the black hole.

Abstract

In this paper, we analyze the rotating Einstein-non-linear-Maxwell-Yukawa black hole solution by Janis-Newman algorithmic rule and complex calculations. We investigate the basic properties (i.e., Hawking radiation) for the corresponding black hole solution. From the horizon structure of the black hole, we discuss the graphical behavior of Hawking temperature $T_H$ and analyze the effects of spin parameter (appears due to Newman-Janis approach) on the $T_H$ of black hole. Furthermore, we investigate the corrected temperature for rotating Einstein-non-linear-Maxwell-Yukawa black hole by using the vector particles tunneling strategy which is based on Hamilton-Jacobi method. We additionally study the graphical explanation of corrected $T_H$ through outer horizon to investigate the physical and stable conditions of black hole. Finally, we compute the corrected entropy and check that the effect of charged, rotation and gravity on entropy.