Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.creator | Giribet, Gaston Enrique | - |
| dc.creator | Oliva, Julio | - |
| dc.creator | Tempo, David | - |
| dc.creator | Troncoso, Ricardo | - |
| dc.date | 2018-09-26T16:44:02Z | - |
| dc.date | 2018-09-26T16:44:02Z | - |
| dc.date | 2009-12 | - |
| dc.date | 2018-09-24T14:33:16Z | - |
| dc.date.accessioned | 2019-04-29T15:43:22Z | - |
| dc.date.available | 2019-04-29T15:43:22Z | - |
| dc.date.issued | 2009-12 | - |
| dc.identifier | Giribet, Gaston Enrique; Oliva, Julio; Tempo, David; Troncoso, Ricardo; Microscopic entropy of the three-dimensional rotating black hole of Bergshoeff-Hohm-Townsend massive gravity; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 80; 12; 12-2009; 124046-124046 | - |
| dc.identifier | 1550-7998 | - |
| dc.identifier | http://hdl.handle.net/11336/60896 | - |
| dc.identifier | CONICET Digital | - |
| dc.identifier | CONICET | - |
| dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/300327 | - |
| dc.description | Asymptotically anti-de Sitter rotating black holes for the Bergshoeff-Hohm-Townsend massive gravity theory in three dimensions are considered. In the special case when the theory admits a unique maximally symmetric solution, apart from the mass and the angular momentum, the black hole is described by an independent "gravitational hair" parameter, which provides a negative lower bound for the mass. This bound is saturated at the extremal case, and since the temperature and the semiclassical entropy vanish, it is naturally regarded as the ground state. The absence of a global charge associated with the gravitational hair parameter reflects itself through the first law of thermodynamics in the fact that the variation of this parameter can be consistently reabsorbed by a shift of the global charges, giving further support to consider the extremal case as the ground state. The rotating black hole fits within relaxed asymptotic conditions as compared with the ones of Brown and Henneaux, such that they are invariant under the standard asymptotic symmetries spanned by two copies of the Virasoro generators, and the algebra of the conserved charges acquires a central extension. Then it is shown that Strominger's holographic computation for general relativity can also be extended to the Bergshoeff-Hohm-Townsend theory; i.e., assuming that the quantum theory could be consistently described by a dual conformal field theory at the boundary, the black hole entropy can be microscopically computed from the asymptotic growth of the number of states according to Cardy's formula, in exact agreement with the semiclassical result. © 2009 The American Physical Society. | - |
| dc.description | Fil: Giribet, Gaston Enrique. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina | - |
| dc.description | Fil: Oliva, Julio. Centro de Estudios Cientificos; Chile. Universidad Austral de Chile; Chile | - |
| dc.description | Fil: Tempo, David. Centro de Estudios Cientificos; Chile. Université Libre de Bruxelles; Bélgica. Universidad de Concepción; Chile | - |
| dc.description | Fil: Troncoso, Ricardo. Centro de Estudios Cientificos; Chile | - |
| dc.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.publisher | American Physical Society | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1103/PhysRevD.80.124046 | - |
| dc.rights | info:eu-repo/semantics/restrictedAccess | - |
| dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | - |
| dc.source | reponame:CONICET Digital (CONICET) | - |
| dc.source | instname:Consejo Nacional de Investigaciones Científicas y Técnicas | - |
| dc.source | instacron:CONICET | - |
| dc.subject | CFT | - |
| dc.subject | 3D Gravity | - |
| dc.subject | AdS/CFT | - |
| dc.subject | Black Holes | - |
| dc.subject | Astronomía | - |
| dc.subject | Ciencias Físicas | - |
| dc.subject | CIENCIAS NATURALES Y EXACTAS | - |
| dc.title | Microscopic entropy of the three-dimensional rotating black hole of Bergshoeff-Hohm-Townsend massive gravity | - |
| dc.type | info:eu-repo/semantics/article | - |
| dc.type | info:eu-repo/semantics/publishedVersion | - |
| dc.type | info:ar-repo/semantics/articulo | - |
| Aparece en las colecciones: | CONICET | |
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