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Hawking radiation as tunneling with back-reaction for the Kerr-anti-de Sitter black hole

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Abstract

Medved and Vagenas demonstrated how the Angheben-Nadalini-Vanzo-Zerbini analysis can be adapted in describing the effects of the gravitational back-reaction for the generic spherically symmetric black hole. We extend the Medved-Vagenas quantum tunneling method to the case of the stationary axisymmetric Kerr black hole in anti-de Sitter space-times. We find a correction to the Hawking radiation by considering the effects of the gravitational back-reaction and also energy conservation and angular momentum conservation.

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Authors and Affiliations

  1. College of Physics Science and Technology, Shenyang Normal University, Shenyang, China

    Hui-Ling Li, Rong Lin, Teng-Jiao Zhou & Tao Huang

Authors
  1. Hui-Ling Li
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  2. Rong Lin
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  3. Teng-Jiao Zhou
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  4. Tao Huang
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Corresponding author

Correspondence to Hui-Ling Li.

Additional information

Prepared from an English manuscript submitted by the authors; for the Russian version, see Teoreticheskaya i Matematicheskaya Fizika, Vol. 161, No. 1, pp. 136–144, October, 2009.

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Li, HL., Lin, R., Zhou, TJ. et al. Hawking radiation as tunneling with back-reaction for the Kerr-anti-de Sitter black hole. Theor Math Phys 161, 1438–1444 (2009). https://doi.org/10.1007/s11232-009-0130-3

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  • DOI: https://doi.org/10.1007/s11232-009-0130-3

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