Constant curvature black holes in Einstein AdS gravity

Euclidean action and thermodynamics

Pablo Guilleminot, Rodrigo Olea, Alexander N. Petrov

Resultado de la investigación: Article

Resumen

We compute the Euclidean action for constant curvature black holes (CCBHs), as an attempt to associate thermodynamic quantities to these solutions of Einstein anti-de Sitter (AdS) gravity. CCBHs are gravitational configurations obtained by identifications along isometries of a D-dimensional globally AdS space, such that the Riemann tensor remains constant. Here, these solutions are interpreted as extended objects, which contain a (D-2)-dimensional de-Sitter brane as a subspace. Nevertheless, the computation of the free energy for these solutions shows that they do not obey standard thermodynamic relations.

Idioma originalEnglish
Número de artículo064046
PublicaciónPhysical Review D
Volumen97
N.º6
DOI
EstadoPublished - 15 mar 2018

Huella dactilar

curvature
gravitation
thermodynamics
free energy
tensors
configurations

ASJC Scopus subject areas

  • Physics and Astronomy (miscellaneous)

Citar esto

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Constant curvature black holes in Einstein AdS gravity : Euclidean action and thermodynamics. / Guilleminot, Pablo; Olea, Rodrigo; Petrov, Alexander N.

En: Physical Review D, Vol. 97, N.º 6, 064046, 15.03.2018.

Resultado de la investigación: Article

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AB - We compute the Euclidean action for constant curvature black holes (CCBHs), as an attempt to associate thermodynamic quantities to these solutions of Einstein anti-de Sitter (AdS) gravity. CCBHs are gravitational configurations obtained by identifications along isometries of a D-dimensional globally AdS space, such that the Riemann tensor remains constant. Here, these solutions are interpreted as extended objects, which contain a (D-2)-dimensional de-Sitter brane as a subspace. Nevertheless, the computation of the free energy for these solutions shows that they do not obey standard thermodynamic relations.

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