Tunneling analysis of Kerr–Newman black hole-like solution in Rastall theory
Riasat AliKazuharu BambaFaculty of Symbiotic Systems Science, Fukushima University, Fukushima 960-1296, JapanSyed Adnan Alı ShahDepartment of Mathematics and Statistics, The University of Lahore, 1-Km Raiwind Road, Sultan Town, Lahore 54000, PakistanMuhammad Junaid SaleemNCBA and E Multan Campus, Multan 66000, Pakistan
2022en
ABI
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 paper, the corrected Hawking temperature is computed by considering the effects of quantum gravity. In our analysis, the Rastall gravity BH solution surrounded 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.
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