The Relation between the Quasi-Localized Energy-Momentum Complexes and the Thermodynamic Potential for the Schwarzschild-de Sitter Black Hole

The Schwarzschild-de Sitter black hole solution, which has two event horizons, is considered to examine the relation between the energy component of quasi-localized energy-momentum complexes on M and the heat flows passing through its boundary ∂M. Here M is the patch between cosmological event horiz...

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Main Author: I-Ching Yang
Format: Article
Language:English
Published: Wiley 2017-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2017/2482940
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author I-Ching Yang
author_facet I-Ching Yang
author_sort I-Ching Yang
collection DOAJ
description The Schwarzschild-de Sitter black hole solution, which has two event horizons, is considered to examine the relation between the energy component of quasi-localized energy-momentum complexes on M and the heat flows passing through its boundary ∂M. Here M is the patch between cosmological event horizon and black hole event horizon of the SdS black hole solution. Conclusively, the relation, like the Legendre transformation, between the energy component of quasi-localized Einstein and Møller energy-momentum complex and the heat flows passing through the boundary is obeyed, and these two energy components of quasi-localized energy-momentum complexes could be corresponding to thermodynamic potentials.
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spelling doaj-art-d6ab58b0f6d5443a812b0c5022ed04e42025-02-03T01:07:26ZengWileyAdvances in High Energy Physics1687-73571687-73652017-01-01201710.1155/2017/24829402482940The Relation between the Quasi-Localized Energy-Momentum Complexes and the Thermodynamic Potential for the Schwarzschild-de Sitter Black HoleI-Ching Yang0Department of Applied Science, National Taitung University, Taitung 95002, TaiwanThe Schwarzschild-de Sitter black hole solution, which has two event horizons, is considered to examine the relation between the energy component of quasi-localized energy-momentum complexes on M and the heat flows passing through its boundary ∂M. Here M is the patch between cosmological event horizon and black hole event horizon of the SdS black hole solution. Conclusively, the relation, like the Legendre transformation, between the energy component of quasi-localized Einstein and Møller energy-momentum complex and the heat flows passing through the boundary is obeyed, and these two energy components of quasi-localized energy-momentum complexes could be corresponding to thermodynamic potentials.http://dx.doi.org/10.1155/2017/2482940
spellingShingle I-Ching Yang
The Relation between the Quasi-Localized Energy-Momentum Complexes and the Thermodynamic Potential for the Schwarzschild-de Sitter Black Hole
Advances in High Energy Physics
title The Relation between the Quasi-Localized Energy-Momentum Complexes and the Thermodynamic Potential for the Schwarzschild-de Sitter Black Hole
title_full The Relation between the Quasi-Localized Energy-Momentum Complexes and the Thermodynamic Potential for the Schwarzschild-de Sitter Black Hole
title_fullStr The Relation between the Quasi-Localized Energy-Momentum Complexes and the Thermodynamic Potential for the Schwarzschild-de Sitter Black Hole
title_full_unstemmed The Relation between the Quasi-Localized Energy-Momentum Complexes and the Thermodynamic Potential for the Schwarzschild-de Sitter Black Hole
title_short The Relation between the Quasi-Localized Energy-Momentum Complexes and the Thermodynamic Potential for the Schwarzschild-de Sitter Black Hole
title_sort relation between the quasi localized energy momentum complexes and the thermodynamic potential for the schwarzschild de sitter black hole
url http://dx.doi.org/10.1155/2017/2482940
work_keys_str_mv AT ichingyang therelationbetweenthequasilocalizedenergymomentumcomplexesandthethermodynamicpotentialfortheschwarzschilddesitterblackhole
AT ichingyang relationbetweenthequasilocalizedenergymomentumcomplexesandthethermodynamicpotentialfortheschwarzschilddesitterblackhole