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dc.contributor.authorDias, Óscar J. C.
dc.contributor.authorHorowitz, Gary T.
dc.contributor.authorSantos, Jorge E.
dc.date.accessioned2022-03-31T16:30:02Z
dc.date.available2022-03-31T16:30:02Z
dc.date.issued2021-12-23
dc.date.submitted2021-11-17
dc.identifier.otherjhep12(2021)179
dc.identifier.other17451
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/335582
dc.description.abstractAbstract: We study the interior of a recently constructed family of asymptotically flat, charged black holes that develop (charged) scalar hair as one increases their charge at fixed mass. Inside the horizon, these black holes resemble the interior of a holographic superconductor. There are analogs of the Josephson oscillations of the scalar field, and the final Kasner singularity depends very sensitively on the black hole parameters near the onset of the instability. In an appendix, we give a general argument that Cauchy horizons cannot exist in a large class of stationary black holes with scalar hair.
dc.languageen
dc.publisherSpringer Berlin Heidelberg
dc.subjectRegular Article - Theoretical Physics
dc.subjectBlack Holes
dc.subjectClassical Theories of Gravity
dc.titleInside an asymptotically flat hairy black hole
dc.typeArticle
dc.date.updated2022-03-31T16:30:02Z
prism.issueIdentifier12
prism.publicationNameJournal of High Energy Physics
prism.volume2021
dc.identifier.doi10.17863/CAM.83013
dcterms.dateAccepted2021-12-07
rioxxterms.versionofrecord10.1007/jhep12(2021)179
rioxxterms.versionVoR
rioxxterms.licenseref.urihttp://creativecommons.org/licenses/by/4.0/
dc.identifier.eissn1029-8479
dc.identifier.arxiv2110.06225


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