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Thermodynamics of regular black hole

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Abstract

We investigate thermodynamics for a magnetically charged regular black hole (MCRBH), which comes from the action of general relativity and nonlinear electromagnetics, comparing with the Reissner–Norström (RN) black hole in both four and two dimensions after dimensional reduction. We find that there is no thermodynamic difference between the regular and RN black holes for a fixed charge Q in both dimensions. This means that the condition for either singularity or regularity at the origin of coordinate does not affect the thermodynamics of black hole. Furthermore, we describe the near-horizon AdS2 thermodynamics of the MCRBH with the connection of the Jackiw–Teitelboim theory. We also identify the near-horizon entropy as the statistical entropy by using the AdS2/CFT1 correspondence.

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Authors and Affiliations

  1. Institute of Basic Science and School of Computer Aided Science, Inje University, Gimhae, 621-749, South Korea

    Yun Soo Myung & Yong-Wan Kim

  2. Department of Physics and Center for Quantum Spacetime, Sogang University, Seoul, 121-742, South Korea

    Young-Jai Park

Authors
  1. Yun Soo Myung
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  2. Yong-Wan Kim
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  3. Young-Jai Park
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Correspondence to Yong-Wan Kim.

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Myung, Y.S., Kim, YW. & Park, YJ. Thermodynamics of regular black hole. Gen Relativ Gravit 41, 1051–1067 (2009). https://doi.org/10.1007/s10714-008-0690-9

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