Artículo
Asymptotically AdS3 solutions to topologically massive gravity at special values of the coupling constants
Fecha de publicación:
12/2009
Editorial:
American Physical Society
Revista:
Physical Review D: Particles, Fields, Gravitation and Cosmology
ISSN:
1550-7998
Idioma:
Inglés
Tipo de recurso:
Artículo publicado
Clasificación temática:
Resumen
We study exact solutions to cosmological topologically massive gravity coupled to topologically massive electrodynamics at special values of the coupling constants. For the particular case of the so-called chiral point lμG=1, vacuum solutions (with vanishing gauge field) are exhibited. These correspond to a one-parameter deformation of general relativity solutions, and are continuously connected to the extremal Bañados- Teitelboim-Zanelli black hole with bare constants J=-lM. At the chiral point this extremal Bañados-Teitelboim-Zanelli black hole turns out to be massless, and thus it can be regarded as a kind of ground state. Although the solution is not asymptotically AdS3 in the sense of Brown-Henneaux boundary conditions, it does obey the weakened asymptotic recently proposed by Grumiller and Johansson. Consequently, we discuss the holographic computation of the conserved charges in terms of the stress tensor in the boundary. For the case where the coupling constants satisfy the relation lμG=1+ 2lμE, electrically charged analogues to these solutions exist. These solutions are asymptotically AdS3 in the strongest sense, and correspond to a logarithmic branch of self-dual solutions previously discussed in the literature. © 2009 The American Physical Society.
Palabras clave:
Topological
,
Black Holes
,
Anti-De Sitter
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Identificadores
Colecciones
Articulos(IFIBA)
Articulos de INST.DE FISICA DE BUENOS AIRES
Articulos de INST.DE FISICA DE BUENOS AIRES
Citación
Garbarz, Alan Nicolás; Giribet, Gaston Enrique; Vásquez, Yerko; Asymptotically AdS3 solutions to topologically massive gravity at special values of the coupling constants; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 79; 4; 12-2009; 1-9
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