Tunneling Analysis of Kerr-Newman Black Hole-Like Solution in Rastall Theory
arXiv:2206.01546 · doi:10.1142/S0218271822500699
Abstract
Hamilton-Jacobi ansatz is used to analyze boson charged particles tunneling in Rastall gravity Kerr- Newman black hole (BH) surrounded by perfect fluid matter through the horizon. The geometrical BH parameters are observed, how these are affecting the radiation utilizing the Lagrangian gravity equation. In this article, the corrected Hawking temperature is computed by considering the effects of quantum gravity. In our analysis, the Rastall gravity BH solution surround by perfect fluid matter effects on Hawking radiation is analyzed graphically. Moreover, the stability and instability of Rastall gravity BH are investigated. The influence of quantum gravity and rotation parameters on BH radiation are also observed by graphical representation.
8 pages, 2 figures, version accepted for publication in International Journal of Modern Physics D
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- Shadow of Kerr black hole surrounded by a cloud of strings in Rastall gravity and constraints from M87*