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General Tortoise Coordinate Transformation in a Dynamical Kerr-Newman Black Hole

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Abstract

Under the extended dynamical tortoise coordinate transformation, Damour-Ruffini method has been applied to calculate the charged particles’ Hawking radiation from the apparent horizon of a dynamical Kerr-Newman black hole. It is shown that Hawking radiation is still purely thermal black body spectrum. Moreover, the temperature of Hawking radiation is corresponding to the apparent horizon surface gravity and the first law of thermodynamics can also be constructed successfully on the apparent horizon in the dynamical Kerr-Newman black hole.

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Authors and Affiliations

  1. Department of Physics, Hubei University for Nationalities, Enshi, Hubei, 445000, China

    Xian-Ming Liu

  2. Department of Physics, Institute of Theoretical Physics, Beijing Normal University, Beijing, 100875, China

    Xian-Ming Liu, Su-Jun Cheng & Wen-Biao Liu

  3. Department of Physics, Xinxiang University, Xinxiang, Henan, 453000, China

    Su-Jun Cheng

Authors
  1. Xian-Ming Liu
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  2. Su-Jun Cheng
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  3. Wen-Biao Liu
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Correspondence to Wen-Biao Liu.

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Liu, XM., Cheng, SJ. & Liu, WB. General Tortoise Coordinate Transformation in a Dynamical Kerr-Newman Black Hole. Int J Theor Phys 51, 518–525 (2012). https://doi.org/10.1007/s10773-011-0930-8

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  • DOI: https://doi.org/10.1007/s10773-011-0930-8

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