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Phase transition and entropy force between two horizons in (n+2)-dimensional de Sitter space

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arxiv 2004.06796 v1 pith:35MYJ5VU submitted 2020-03-31 hep-th gr-qc

Yang Zhang , Wen-qi Wang , Yu-bo Ma , Jun Wang This is my paper · ORCID
classification hep-thgr-qc
keywords acceleratingcosmicdimensionaleffectiveentropyexpansionforcehorizons
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In this paper, the effect of the space-time dimension on effective thermodynamic quantities in (n+2)-dimensional Reissoner-Nordstrom-de Sitter space has been stud ied. Based on derived effective thermodynamic quantities, conditions for the phase transition are obtained. The result shows that the accelerating cosmic expansion can be attained by the entropy force arisen from the interaction between horizons of black holes and our universe, which provides a possible way to explain the physical mechanism for the accelerating cosmic expansion.

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Cited by 1 Pith paper

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  1. Phase Transition and Critical Phenomena of Charged Einstein-Maxwell-Scalar Black Holes

    gr-qc 2025-05 conditional novelty 5.0 of 10

    Charged EMs black holes show van der Waals-type phase transitions with mean-field critical exponents, and the phase transition disappears above a threshold scalar charge.

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