dc.creatorAceña, Andrés Esteban
dc.creatorLópez, Ericson
dc.creatorAldás, Franklin
dc.date.accessioned2021-09-07T15:38:18Z
dc.date.accessioned2022-10-15T04:31:07Z
dc.date.available2021-09-07T15:38:18Z
dc.date.available2022-10-15T04:31:07Z
dc.date.created2021-09-07T15:38:18Z
dc.date.issued2020-02
dc.identifierAceña, Andrés Esteban; López, Ericson; Aldás, Franklin; Circular geodesics stability in a static black hole in new massive gravity; Molecular Diversity Preservation International; Galaxies; 8; 1; 2-2020; 1-8
dc.identifier2075-4434
dc.identifierhttp://hdl.handle.net/11336/139815
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4345397
dc.description.abstractWe study the existence and stability of circular geodesics in a family of asymptotically AdS static black holes in New Massive Gravity theory. We show that the mathematical sign of the hair parameter determines the existence of such geodesics. For a positive hair parameter, the stability regions follow the usual pattern, with the innermost geodesic being null, unstable, and separated from the horizon, followed by a region of unstable timelike geodesics and then a region of stable timelike geodesics, which extends in the asymptotic region.
dc.languageeng
dc.publisherMolecular Diversity Preservation International
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://www.mdpi.com/2075-4434/8/1/14
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.3390/galaxies8010014
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectBLACK HOLES
dc.subjectCIRCULAR GEODESICS
dc.subjectNEW MASSIVE GRAVITY
dc.titleCircular geodesics stability in a static black hole in new massive gravity
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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