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First Law of Black Hole Thermodynamics for the Kerr–Newman Spacetime Using Foliation

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Abstract

This article follows a simpler approach (Siddiqui et al. 2011) using the foliation concept with virtual displacement of hypersurfaces near the event horizon to derive the first law of black hole thermodynamics for the Kerr–Newman black hole spacetime.

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Authors and Affiliations

  1. Department of Mathematics, COMSATʼS University Islamabad, Wah Campus, G.T. Road, Wah Cantt, 47040, Pakistan

    Syed Muhammad Jawwad Riaz

  2. School of Natural Sciences, National University of Sciences and Technology, H-12, Islamabad, 46000, Pakistan

    Azad A. Siddiqui

Authors
  1. Syed Muhammad Jawwad Riaz
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  2. Azad A. Siddiqui
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Correspondence to Syed Muhammad Jawwad Riaz or Azad A. Siddiqui.

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Jawwad Riaz, S.M., Siddiqui, A.A. First Law of Black Hole Thermodynamics for the Kerr–Newman Spacetime Using Foliation. Gravit. Cosmol. 26, 82–85 (2020). https://doi.org/10.1134/S0202289320010119

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  • DOI: https://doi.org/10.1134/S0202289320010119

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