Gravitational analysis of Einstein-non-linear-Maxwell-Yukawa black hole under the effect of Newman-Janis algorithm

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.

Study of tunneling radiation and thermal fluctuations of a gauge super gravity like black hole

“…Zhang and Pradhan [43] investigated that how corrected entropy affected the Kerr-Newman-AdS and RN-AdS BHs, they found that there was a quadratic phase transition occurring because of the thermal fluctuations. Moreover, the thermodynamics of various types of BHs under the influence of correction parameter is analyzed, they checked the relation of other thermodynamics quantities with the corrected entropy and for stability reasons [44][45][46][47][48][49][50][51][52][53].…”