Entropy of Higher-Dimensional Charged de Sitter Black Holes and Phase Transition

Ren Zhao, Li-Chun Zhang

doi:10.1088/0253-6102/70/5/578

Communications in Theoretical Physics >

2018 , Vol. 70 >Issue 05: 578 - 584

DOI: https://doi.org/10.1088/0253-6102/70/5/578

Gravitation Theory, Astrophysics and Cosmology

Entropy of Higher-Dimensional Charged de Sitter Black Holes and Phase Transition

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

Received date: 2018-04-12

Revised date: 2018-04-26

Online published: 2018-11-01

Supported by

Supported in part by the National Natural Science Foundation of China under Grant No. 11475108

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Abstract

From a new perspective, we discuss the thermodynamic entropy of (n+2)-dimensional Reissner-Nordströmde Sitter (RNdS) black hole and analyze the phase transition of the effective thermodynamic system. Considering the correlations between the black hole event horizon and the cosmological horizon, we conjecture that the total entropy of the RNdS black hole should contain an extra term besides the sum of the entropies of the two horizons. In the lukewarm case, the effective temperature of the RNdS black hole is the same as that of the black hole horizon and the cosmological horizon. Under this condition, we obtain the extra contribution to the total entropy. With the corrected entropy, we derive other effective thermodynamic quantities and analyze the phase transition of the RNdS black hole in analogy to the usual thermodynamic system.

Key words： de Sitter space; black hole entropy; phase transition

Cite this article

Ren Zhao, Li-Chun Zhang . Entropy of Higher-Dimensional Charged de Sitter Black Holes and Phase Transition[J]. Communications in Theoretical Physics, 2018 , 70(05) : 578 -584 . DOI: 10.1088/0253-6102/70/5/578

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