dc.creatorCañate P.
dc.creatorBreton N.
dc.date.accessioned2020-03-26T16:32:36Z
dc.date.accessioned2022-09-28T20:20:16Z
dc.date.available2020-03-26T16:32:36Z
dc.date.available2022-09-28T20:20:16Z
dc.date.created2020-03-26T16:32:36Z
dc.date.issued2018
dc.identifierPhysical Review D; Vol. 98, Núm. 10
dc.identifier24700010
dc.identifierhttps://hdl.handle.net/20.500.12585/8920
dc.identifier10.1103/PhysRevD.98.104012
dc.identifierUniversidad Tecnológica de Bolívar
dc.identifierRepositorio UTB
dc.identifier55744418600
dc.identifier6701747290
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3725887
dc.description.abstractIn this paper we present two results in (2+1) gravity coupled to nonlinear electrodynamics. First we determine the general form of the electromagnetic field tensor in (2+1) gravity coupled to nonlinear electrodynamics in stationary cyclic spacetimes. Secondly, we determine a family of exact solutions in (2+1) gravity sourced by a nonlinear electromagnetic field. The solutions are characterized by five parameters: mass M, angular momentum J, cosmological constant Λ, and two electromagnetic charges qα and qβ. Remarkably, the solution can be interpreted as a traversable wormhole, provided the fulfillment of certain inequalities by the characteristic parameters; fine-tuning of the cosmological constant leads to an extreme black hole, whereas by switching off one of the electromagnetic charges, we obtain the Bañados-Teitelboim-Zanelli (BTZ) black hole. © 2018 American Physical Society.
dc.languageeng
dc.publisherAmerican Physical Society
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.rightsAtribución-NoComercial 4.0 Internacional
dc.sourcehttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85057772233&doi=10.1103%2fPhysRevD.98.104012&partnerID=40&md5=0a6573cbebc63c34ae6fdd9e2e8fab3a
dc.titleBlack hole-wormhole transition in (2+1)-dimensional Einstein-anti-de Sitter gravity coupled to nonlinear electrodynamics BLACK HOLE-WORMHOLE TRANSITION in (2+1)- ⋯ PEDRO CAÑATE and NORA BRETON


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