Hawking radiation of Schwarzschild–de Sitter black hole by Hamilton–Jacobi method

Abstract

We investigate the Hawking radiation of Schwarzschild–de Sitter (SdS) black hole by massive particles tunneling method. We consider the spacetime background to be dynamical, incorporate the self-gravitation effect of the emitted particles and show that the tunneling rate is related to the change of Bekenstein–Hawking entropy and the derived emission spectrum deviates from the pure thermal spectrum when energy and angular momentum are conserved. Our result is also in accordance with Parikh and Wilczekʼs opinion and gives a correction to the Hawking radiation of SdS black hole.