Quantum gravity evolution in the Hawking radiation of a rotating regular Hayward black hole

In this paper, we study two different phenomena (the Newman–Janis algorithm and the semiclassical Hamilton–Jacobi method) to analyze Hawking temperature (TH) for massive 4-dimensional regular Hayward BH with spin parameter. First of all, compute rotating black hole solution by taking algorithmic rule. We derive TH help surface gravity. have also analyzed effects parameter a free l on graphs. Moreover, investigate quantum corrected (TH?) hole. To do so, utilize Lagrangian filed equation in background GUP within concept WKB approximation method. The TH? depends upon correction ?, mass m, a, radius r+. graphical behavior versus event horizon r+ check influences gravity stability corresponding significance’s logarithmic entropy BH.