Phase Transition and Entropy Force between Two Horizons in (n+2)-Dimensional de Sitter Space

In this paper, the effect of the space-time dimension on effective thermodynamic quantities in (n+2)-dimensional Reissner-Nordstrom-de Sitter space has been studied. Based on derived effective thermodynamic quantities, conditions for the phase transition are obtained. The result shows that the accel...

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Main Authors: Yang Zhang, Wen-qi Wang, Yu-bo Ma, Jun Wang
Format: Article
Language:English
Published: Wiley 2020-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2020/7263059
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author Yang Zhang
Wen-qi Wang
Yu-bo Ma
Jun Wang
author_facet Yang Zhang
Wen-qi Wang
Yu-bo Ma
Jun Wang
author_sort Yang Zhang
collection DOAJ
description In this paper, the effect of the space-time dimension on effective thermodynamic quantities in (n+2)-dimensional Reissner-Nordstrom-de Sitter space has been studied. 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.
format Article
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institution Kabale University
issn 1687-7357
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language English
publishDate 2020-01-01
publisher Wiley
record_format Article
series Advances in High Energy Physics
spelling doaj-art-51eddbe43ecc48d09a45d00dd8b041b72025-02-03T06:45:47ZengWileyAdvances in High Energy Physics1687-73571687-73652020-01-01202010.1155/2020/72630597263059Phase Transition and Entropy Force between Two Horizons in (n+2)-Dimensional de Sitter SpaceYang Zhang0Wen-qi Wang1Yu-bo Ma2Jun Wang3Department of Physics, Shanxi Datong University, Datong 037009, ChinaDepartment of Physics, Shanxi Datong University, Datong 037009, ChinaDepartment of Physics, Shanxi Datong University, Datong 037009, ChinaSchool of Physics and Astronomy, Yunnan University, Kunming 650091, ChinaIn this paper, the effect of the space-time dimension on effective thermodynamic quantities in (n+2)-dimensional Reissner-Nordstrom-de Sitter space has been studied. 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.http://dx.doi.org/10.1155/2020/7263059
spellingShingle Yang Zhang
Wen-qi Wang
Yu-bo Ma
Jun Wang
Phase Transition and Entropy Force between Two Horizons in (n+2)-Dimensional de Sitter Space
Advances in High Energy Physics
title Phase Transition and Entropy Force between Two Horizons in (n+2)-Dimensional de Sitter Space
title_full Phase Transition and Entropy Force between Two Horizons in (n+2)-Dimensional de Sitter Space
title_fullStr Phase Transition and Entropy Force between Two Horizons in (n+2)-Dimensional de Sitter Space
title_full_unstemmed Phase Transition and Entropy Force between Two Horizons in (n+2)-Dimensional de Sitter Space
title_short Phase Transition and Entropy Force between Two Horizons in (n+2)-Dimensional de Sitter Space
title_sort phase transition and entropy force between two horizons in n 2 dimensional de sitter space
url http://dx.doi.org/10.1155/2020/7263059
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AT wenqiwang phasetransitionandentropyforcebetweentwohorizonsinn2dimensionaldesitterspace
AT yuboma phasetransitionandentropyforcebetweentwohorizonsinn2dimensionaldesitterspace
AT junwang phasetransitionandentropyforcebetweentwohorizonsinn2dimensionaldesitterspace