dc.creatorMaeda, Hideki
dc.creatorGiribet, Gaston Enrique
dc.date.accessioned2018-08-23T14:33:45Z
dc.date.accessioned2018-11-06T15:03:27Z
dc.date.available2018-08-23T14:33:45Z
dc.date.available2018-11-06T15:03:27Z
dc.date.created2018-08-23T14:33:45Z
dc.date.issued2011-11
dc.identifierMaeda, Hideki; Giribet, Gaston Enrique; Lifshitz black holes in Brans-Dicke theory; Springer; Journal of High Energy Physics; 2011; 11; 11-2011; 15-36
dc.identifier1126-6708
dc.identifierhttp://hdl.handle.net/11336/56758
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1893309
dc.description.abstractWe present an exact asymptotically Lifshitz black hole solution in Brans-Dicke theory of gravity in arbitrary n(≥ 3) dimensions in presence of a power-law potential. In this solution, the dynamical exponent z is determined in terms of the Brans-Dicke parameter ! and n. Asymptotic Lifshitz condition at infinity requires z > 1, which corresponds to ?(n ? 1)/(n ? 2) ≥ w ?n/(n ? 1). On the other hand, the no-ghost condition for the scalar field in the Einstein frame requires 0 < z ≤ 2(n ? 2)/(n ? 3). We compute the Hawking temperature of the black hole solution and discuss the problems encountered and the proposals in defining its thermodynamic properties. A generalized solution charged under the Maxwell field is also presented. © 2011 SISSA.
dc.languageeng
dc.publisherSpringer
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007/JHEP11(2011)015
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1007/JHEP11(2011)015
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectADS-CFT CORRESPONDENCE
dc.subjectBLACK HOLES
dc.subjectCLASSICAL THEORIES OF GRAVITY
dc.titleLifshitz black holes in Brans-Dicke theory
dc.typeArtículos de revistas
dc.typeArtículos de revistas
dc.typeArtículos de revistas


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