Hawking Radiation of Schwarzschild-de Sitter Black Hole by Hamilton-Jacobi method
arXiv:1205.1216 · doi:10.1016/j.physletb.2012.04.049
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 Wilczek\rq s opinion and gives a correction to the Hawking radiation of SdS black hole.
arXiv comment9 page. arXiv admin note: text overlap with arXiv:1205.1390
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