Non-thermal Hawking radiation from the Kerr black hole

HAN Yi-Wen; HAO Jia-Bo

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

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2024年10月30日

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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. Hawking S W. Nature, 1974, 248: 302. Hawking S W. Commun. Math. Phys., 1975, 43: 1993. Damuor T, Ruffini R. Phys. Rev. D, 1976, 14: 3324. Kraus P, Wilczek F. Nucl. Phys. B, 1995, 433: 4035. Parikh M K, Wiclzek F. Phys. Rev. Lett., 2000, 85: 50426. Vagenas E C. Phys. Lett. B, 2001, 503 : 3997. Medved A J M. Phys. Rev. D, 2002, 66: 1240098. Vagenas E C. Phys. Lett. B, 2003, 559: 659. Parikh M K. Int. J. Mod. Phys. D, 2004, 13: 235510. ZHANG J Y, ZHAO Z. Mod. Phys. Lett. A, 2005, 20: 167311. Setare M R, Vagenas E C. Int. J. Mod. Phys. A, 2005, 20:721912. LIU W B. Phys. Lett. B, 2006, 634: 54113. ZHANG J Y, FAN J H. Phys. Lett. B, 2007, 648: 13314. LIU W B. Acta Phys. Sin., 2007, 56: 616415. Kerr R P. Pyhs. Rev. Lett., 1963, 11: 237

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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

HAN Yi-Wen ^,
HAO Jia-Bo

Corresponding author: HAN Yi-Wen,

Received Date: 2008-05-09
Accepted Date: 2008-08-03
Available Online: 2009-02-05

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.