dc.creatorErices, Cristián
dc.creatorRiquelme, Miguel
dc.creatorRodríguez, Pablo
dc.date.accessioned2020-11-03T07:45:17Z
dc.date.accessioned2023-05-30T20:46:09Z
dc.date.available2020-11-03T07:45:17Z
dc.date.available2023-05-30T20:46:09Z
dc.date.created2020-11-03T07:45:17Z
dc.date.issued2019
dc.identifier2470-0010
dc.identifierhttp://repositorio.uss.cl/xmlui/handle/uss/243
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.100.126026
dc.identifier2470-0029
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/6446578
dc.description.abstractThe thermodynamic properties of the Bafiados-Teitelboim-Zanelli black hole endowed with Korteweg-de Vries (KdV)-type boundary conditions are reconsidered. This family of boundary conditions is labeled by a non-negative integer n, and gives rise to a dual theory which possesses anisotropic Lifshitz scaling invariance with dynamical exponent z = 2n + 1. We show that from the scale invariance of the action for stationary and circularly symmetric spacetimes, an anisotropic version of the Smarr relation arises. Finally, we analyze the global and local thermal stability of the system and we found that the specific heat of the black hole is positive for all possible values of z, and at the self-dual temperature T-s = 1/2 pi(1/z)(z/z+1), there is a Hawking-Page phase transition between the BTZ black hole and thermal AdS(3) spacetime.
dc.languageen
dc.publisherFacultad de Ingeniería y Tecnología
dc.relationvol. 100, no. 12
dc.relationIndexado en WOS
dc.rightshttps://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.sourcePhysical Review D
dc.subjectCRITICAL-BEHAVIOR
dc.subjectCLASSICAL BLACK HOLES
dc.subjectGRAVITY IN DIMENSIONS OTHER THAN FOUR
dc.subjectGRAVITATION, COSMOLOGY & ASTROPHYSICS
dc.titleBTZ black hole with Korteweg-de Vries-type boundary conditions: Thermodynamics revisited
dc.typeArticle


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