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A New Method to Study the Hawking Radiation from the Kerr-NUT Black Hole

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Abstract

Developing Hamilton-Jacobi method, we discuss the Hawking radiation of Kerr-NUT black hole by considering the self-gravitation interaction as well as the energy conservation and angular momentum conservation. The result shows that the factual spectrum deviates from the precisely thermal one and the tunneling rate is related to the change of Bekenstein-Hawking entropy, which is accordant with that obtained by Parikh and Wilczek’s method and gives an interesting correction to the Hawking radiation of the black hole.

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Authors and Affiliations

  1. Institute of Theoretical Physics, China West Normal University, Nanchong, 637002, China

    Hong-Lin Liu, Zi-Xiang Liu, Jian-Song Hou & Shu-Zheng Yang

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  1. Hong-Lin Liu
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  2. Zi-Xiang Liu
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  3. Jian-Song Hou
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  4. Shu-Zheng Yang
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Correspondence to Hong-Lin Liu.

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Liu, HL., Liu, ZX., Hou, JS. et al. A New Method to Study the Hawking Radiation from the Kerr-NUT Black Hole. Int J Theor Phys 47, 2960–2965 (2008). https://doi.org/10.1007/s10773-008-9730-1

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  • DOI: https://doi.org/10.1007/s10773-008-9730-1

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