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Thermodynamics of the Reissner-Nordström-de Sitter black hole

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Abstract

Considering the relationship between the black hole horizon and the cosmological horizon, the thermodynamic property of the charged de Sitter spacetime is discussed. The effective temperature and energy are obtained. The result shows that the upper limit of the energy in the charged de Sitter spacetime is just the energy in the pure de Sitter spacetime. The thermal capacity of the charged de Sitter spacetime is positive, thus satisfying the thermal stability condition.

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Authors and Affiliations

  1. Institute of Theoretical Physics, Department of Physics, Shanxi Datong University, Datong, 037009, China

    LiChun Zhang, HuaiFan Li & Ren Zhao

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  1. LiChun Zhang
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  2. HuaiFan Li
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  3. Ren Zhao
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Correspondence to Ren Zhao.

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Zhang, L., Li, H. & Zhao, R. Thermodynamics of the Reissner-Nordström-de Sitter black hole. Sci. China Phys. Mech. Astron. 54, 1384–1387 (2011). https://doi.org/10.1007/s11433-011-4381-2

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  • DOI: https://doi.org/10.1007/s11433-011-4381-2

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