Quantum Gravity Evolution in the Hawking Radiation of a Rotating Regular Hayward Black Hole
arXiv:2201.02754 · doi:10.1016/j.dark.2022.100948
Abstract
In this paper, we study two different phenomena (the Newman-Janis algorithm and the semiclassical Hamilton-Jacobi method) to analyze the Hawking temperature () for massive -dimensional regular Hayward BH with spin parameter. First of all, we compute the rotating regular Hayward black hole solution by taking the Newman-Janis algorithmic rule. We derive the for rotating regular Hayward BH with the help of surface gravity. We have also analyzed the effects of spin parameter and free parameter on with the help of graphs. Moreover, we investigate the quantum corrected Hawking temperature () for rotating regular Hayward black hole. To do so, we utilize the Lagrangian filed equation in the background of GUP within the concept of WKB approximation and semiclassical Hamilton-Jacobi method. The of rotating regular Hayward BH depends upon correction parameter , BH mass , spin parameter , free parameter and BH radius . We also study the graphical behavior of versus event horizon for rotating regular Hayward BH and check the influences of quantum gravity parameter , spin parameter and free parameter on the stability of corresponding black hole. Moreover, we study the significance's of logarithmic entropy correction for regular rotating Hayward BH.
arXiv commentPhysics of the Dark Universe accepted version
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