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dc.contributor.authorDias, ÓJC
dc.contributor.authorHorowitz, GT
dc.contributor.authorSantos, JE
dc.date.accessioned2022-04-26T15:24:22Z
dc.date.available2022-04-26T15:24:22Z
dc.date.issued2022
dc.date.submitted2021-11-17
dc.identifier.issn1029-8479
dc.identifier.otherjhep01(2022)064
dc.identifier.other17556
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/336469
dc.description.abstractWe study a family of four-dimensional, asymptotically flat, charged black holes that develop (charged) scalar hair as one increases their charge at fixed mass. Surprisingly, the maximum charge for given mass is a nonsingular hairy black hole with nonzero Hawking temperature. The implications for Hawking evaporation are discussed.
dc.languageen
dc.publisherSpringer Science and Business Media LLC
dc.subjectRegular Article - Theoretical Physics
dc.subjectBlack Holes
dc.subjectClassical Theories of Gravity
dc.titleExtremal black holes that are not extremal: maximal warm holes
dc.typeArticle
dc.date.updated2022-04-26T15:24:22Z
prism.issueIdentifier1
prism.publicationNameJournal of High Energy Physics
prism.volume2022
dc.identifier.doi10.17863/CAM.83887
dcterms.dateAccepted2021-12-21
rioxxterms.versionofrecord10.1007/JHEP01(2022)064
rioxxterms.versionVoR
rioxxterms.licenseref.urihttp://creativecommons.org/licenses/by/4.0/
dc.identifier.eissn1029-8479
dc.publisher.urlhttp://dx.doi.org/10.1007/JHEP01(2022)064
pubs.funder-project-idScience and Technology Facilities Council (ST/P000673/1)
cam.issuedOnline2022-01-13
dc.identifier.arxiv2109.14633


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