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• W2056558731 abstract "Recent work, which treats the Hawking radiation as a semiclassical tunneling process at the horizon of the Schwarzschild and Reissner-Nordstrom spacetimes, indicates that the exact radiant spectrum is no longer pure thermal after considering the black hole background as dynamical and the conservation of energy. In this paper, we extend the method to investigate Hawking radiation as massless particles tunneling across the event horizon of the Kerr black hole and that of charged particles from the Kerr-Newman black hole by taking into account the energy conservation, the angular momentum conservation, and the electric charge conservation. Our results show that when self-gravitation is considered, the tunneling rate is related to the change of Bekenstein-Hawking entropy and the derived emission spectrum deviates from the pure thermal spectrum, but is consistent with an underlying unitary theory." @default.
• W2056558731 created "2016-06-24" @default.
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• W2056558731 date "2006-03-03" @default.
• W2056558731 modified "2023-10-07" @default.
• W2056558731 title "Hawking radiation as tunneling from the Kerr and Kerr-Newman black holes" @default.
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• W2056558731 doi "https://doi.org/10.1103/physrevd.73.064003" @default.
• W2056558731 hasPublicationYear "2006" @default.
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