Non-thermal Hawking radiation from the Kerr black hole

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HAN Yi-Wen and HAO Jia-Bo. Non-thermal Hawking radiation from the Kerr black hole[J]. Chinese Physics C, 2009, 33(2): 94-97. doi: 10.1088/1674-1137/33/2/003
HAN Yi-Wen and HAO Jia-Bo. Non-thermal Hawking radiation from the Kerr black hole[J]. Chinese Physics C, 2009, 33(2): 94-97.  doi: 10.1088/1674-1137/33/2/003 shu
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Received: 2008-05-09
Revised: 2008-08-03
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Non-thermal Hawking radiation from the Kerr black hole

    Corresponding author: HAN Yi-Wen,

Abstract: 

We present a short and direct derivation of Hawking radiation by using the Damour-Ruffini method, as taking into account the self-gravitational interaction from the Kerr black hole. It is found that the radiation is not exactly thermal, and because the derivation obeys conservation laws, the non-thermal Hawking radiation can carry information from the black hole. So it can be used to explain the black hole information paradox, and the process satisfies unitary.

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