Thermodynamics of rotating black branes in gravity with first order string corrections

In this paper, the rotating black brane solutions with zero curvature horizon of classical gravity with first order string corrections are introduced. Although these solutions are not asymptotically anti de Sitter, one can use the counterterm method in order to compute the conserved quantities of th...

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Main Author: M. H. Dehghani
Format: Article
Language:English
Published: Isfahan University of Technology 2005-09-01
Series:Iranian Journal of Physics Research
Subjects:
Online Access:http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-230&slc_lang=en&sid=1
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author M. H. Dehghani
author_facet M. H. Dehghani
author_sort M. H. Dehghani
collection DOAJ
description In this paper, the rotating black brane solutions with zero curvature horizon of classical gravity with first order string corrections are introduced. Although these solutions are not asymptotically anti de Sitter, one can use the counterterm method in order to compute the conserved quantities of these solutions. Here, by reviewing the counterterm method for asymptotically anti de Sitter spacetimes, the conserved quantities of these rotating solutions are computed. Also a Smarr-type formula for the mass as a function of the entropy and the angular momenta is obtained, and it is shown that the conserved and thermodynamic quantities satisfy the first law of thermodynamics. Finally, a stability analysis in the canonical ensemble is performed, and it is shown that the system is thermally stable. This is in commensurable with the fact that there is no Hawking-Page phase transition for black object with zero curvature horizon.
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spelling doaj.art-9a60c0bb38634efea5e33a29795f71c02022-12-22T03:28:02ZengIsfahan University of TechnologyIranian Journal of Physics Research1682-69572005-09-0153160160Thermodynamics of rotating black branes in gravity with first order string correctionsM. H. DehghaniIn this paper, the rotating black brane solutions with zero curvature horizon of classical gravity with first order string corrections are introduced. Although these solutions are not asymptotically anti de Sitter, one can use the counterterm method in order to compute the conserved quantities of these solutions. Here, by reviewing the counterterm method for asymptotically anti de Sitter spacetimes, the conserved quantities of these rotating solutions are computed. Also a Smarr-type formula for the mass as a function of the entropy and the angular momenta is obtained, and it is shown that the conserved and thermodynamic quantities satisfy the first law of thermodynamics. Finally, a stability analysis in the canonical ensemble is performed, and it is shown that the system is thermally stable. This is in commensurable with the fact that there is no Hawking-Page phase transition for black object with zero curvature horizon.http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-230&slc_lang=en&sid=1black holesdilaton gravitycounterterm method
spellingShingle M. H. Dehghani
Thermodynamics of rotating black branes in gravity with first order string corrections
Iranian Journal of Physics Research
black holes
dilaton gravity
counterterm method
title Thermodynamics of rotating black branes in gravity with first order string corrections
title_full Thermodynamics of rotating black branes in gravity with first order string corrections
title_fullStr Thermodynamics of rotating black branes in gravity with first order string corrections
title_full_unstemmed Thermodynamics of rotating black branes in gravity with first order string corrections
title_short Thermodynamics of rotating black branes in gravity with first order string corrections
title_sort thermodynamics of rotating black branes in gravity with first order string corrections
topic black holes
dilaton gravity
counterterm method
url http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-230&slc_lang=en&sid=1
work_keys_str_mv AT mhdehghani thermodynamicsofrotatingblackbranesingravitywithfirstorderstringcorrections