PHYSICS LETTERS B

dc.creatorAstorino, Marco
dc.creatorCanfora, Fabrizio
dc.creatorGiacomini-Baumhogger, Alex
dc.creatorOrtaggio, Marcello
dc.date2021-08-23T22:58:57Z
dc.date2022-07-07T14:55:48Z
dc.date2021-08-23T22:58:57Z
dc.date2022-07-07T14:55:48Z
dc.date2018
dc.date.accessioned2023-08-21T20:56:38Z
dc.date.available2023-08-21T20:56:38Z
dc.identifier1150246
dc.identifier1150246
dc.identifierhttps://hdl.handle.net/10533/252459
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8281306
dc.descriptionAn exact hairy asymptotically locally AdS black hole solution with a flat horizon in the Einstein-nonlinear sigma model system in (3+1) dimensions is constructed. The ansatz for the nonlinear SU(2) field is regular everywhere and depends explicitly on Killing coordinates, but in such a way that its energymomentum tensor is compatible with a metric with Killing fields. The solution is characterized by a discrete parameter which has neither topological nor Noether charge associated with it and therefore represents a hair. A U(1) gauge field interacting with Einstein gravity can also be included. The thermodynamics is analyzed. Interestingly, the hairy black hole is always thermodynamically favouredwith respect to the corresponding black hole with vanishing Pionic field. (C) 2017 The Authors. Published by Elsevier B.V.
dc.descriptionRegular 2015
dc.descriptionFONDECYT
dc.descriptionFONDECYT
dc.languageeng
dc.relationhandle/10533/111557
dc.relationhandle/10533/111541
dc.relationhandle/10533/108045
dc.relationhttps://doi.org/10.1016/j.physletb.2017.11.051
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsinfo:eu-repo/semantics/article
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleHairy AdS black holes with a toroidal horizon in 4D Einstein-nonlinear sigma-model system
dc.titlePHYSICS LETTERS B
dc.typeArticulo
dc.typeinfo:eu-repo/semantics/publishedVersion


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