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dc.contributor.authorAyón-Beato, Eloy
dc.contributor.authorBravo-Gaete, Moises
dc.contributor.authorCorrea, Francisco
dc.contributor.authorMokhtar, Hassaine
dc.contributor.authorJuárez-Aubry, María Montserrat
dc.date.accessioned2019-12-12T15:50:35Z
dc.date.available2019-12-12T15:50:35Z
dc.date.issued2019
dc.identifier.urihttp://repositorio.ucm.cl/handle/ucm/2535
dc.description.abstractIn arbitrary dimension, we consider a theory described by the most general quadratic curvature corrections of Einstein gravity together with a self-interacting nonminimally coupled scalar field. This theory is shown to admit five different families of Lifshitz black holes dressed with a nontrivial scalar field. The entropy of these configurations is microscopically computed by means of a higher-dimensional anisotropic Cardy-like formula where the role of the ground state is played by the soliton obtained through a double analytic continuation. This involves calculating the correct expressions for the masses of the higher-dimensional Lifshitz black hole as well as their corresponding soliton. The robustness of this Cardy-like formula is checked by showing that the microscopic entropy is in perfect agreement with the gravitational Wald entropy. Consequently, the calculated global charges are compatible with the first law of thermodynamics as well as an anisotropic higher-dimensional version of the Smarr formula. Some of these configurations exist on Lifshitz critical points of the theory where all their extensive thermodynamic quantities vanis.es_CL
dc.language.isoenes_CL
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
dc.sourcePhysical Review D, 100(4), 044024es_CL
dc.titleMicroscopic entropy of higher-dimensional nonminimally dressed Lifshitz black holeses_CL
dc.typeArticlees_CL
dc.ucm.facultadFacultad de Ciencias Básicases_CL
dc.ucm.indexacionScopuses_CL
dc.ucm.indexacionIsies_CL
dc.ucm.urijournals.aps.org/prd/abstract/10.1103/PhysRevD.100.044024es_CL
dc.ucm.doidoi.org/10.1103/PhysRevD.100.044024es_CL


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