Non-thermal Hawking radiation from the Kerr black hole

HAN Yi-Wen; HAO Jia-Bo

doi:10.1088/1674-1137/33/2/003

Chinese Physics C> 2009, Vol. 33> Issue(2) : 94-97 DOI: 10.1088/1674-1137/33/2/003

Non-thermal Hawking radiation from the Kerr black hole

HAN Yi-Wen ^, ,
HAO Jia-Bo

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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.

References

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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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