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Thermodynamic Phase Transition and Critical Behavior of a Spherical Symmetric Black Hole

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Abstract

In this paper, we builded the thermodynamics model of black hole based on the method of York. We obtained the reduced temperature reciprocal function using the action of the system. We studied the phase structure of black holes and Hawking-Page phase transition. We obtained the first order phase transition and critical values of black hole in Rerssner-NordstrÖm space time. The results showed that only when two-phase coexistence appeared only when |q| < |q c |.

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Authors and Affiliations

  1. Department of Physics and Electronic Engineering, Heze University, Heze, Shandong, 274015, China

    Ji-Jian Jiang & Chuan-An Li

  2. School of Electronic Science and Engineering, Nanjing University of Posts and Telecommunications, Nanjing, Jiangsu, 210000, China

    Xie-Feng Cheng

Authors
  1. Ji-Jian Jiang
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  2. Chuan-An Li
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  3. Xie-Feng Cheng
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Corresponding author

Correspondence to Chuan-An Li.

Additional information

Project supported by the National Natural Science Foundation of China (Grant No. 61271334) and the Shandong Provincial Natural Science Foundation (Grant No. ZR2011AM020)

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Jiang, JJ., Li, CA. & Cheng, XF. Thermodynamic Phase Transition and Critical Behavior of a Spherical Symmetric Black Hole. Int J Theor Phys 55, 2053–2060 (2016). https://doi.org/10.1007/s10773-015-2845-2

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  • DOI: https://doi.org/10.1007/s10773-015-2845-2

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