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Instability and new phases of higher-dimensional rotating black holes

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dc.contributor.authorDias, Óscar J. C.
dc.contributor.authorFigueras, Pau
dc.contributor.authorMonteiro, Ricardo
dc.contributor.authorSantos, Jorge E.
dc.contributor.authorEmparan García de Salazar, Roberto A.
dc.date.accessioned2019-04-05T09:47:22Z
dc.date.available2019-04-05T09:47:22Z
dc.date.issued2009-12-29
dc.date.updated2019-04-05T09:47:23Z
dc.description.abstractIt has been conjectured that higher-dimensional rotating black holes become unstable at a sufficiently large value of the rotation, and that new black holes with pinched horizons appear at the threshold of the instability. We search numerically and find the stationary axisymmetric perturbations of Myers-Perry black holes with a single spin that mark the onset of the instability and the appearance of the new black hole phases. We also find new ultraspinning Gregory-Laflamme instabilities of rotating black strings and branes.
dc.format.extent5 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec576581
dc.identifier.issn1550-7998
dc.identifier.urihttps://hdl.handle.net/2445/131508
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.isformatofReproducció del document publicat a: https://doi.org/10.1103/PhysRevD.80.111701
dc.relation.ispartofPhysical Review D, 2009, vol. 80, num. 11, p. 111701(R)
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/FP7/220197/EU//GRAVEFTMICS
dc.relation.urihttps://doi.org/10.1103/PhysRevD.80.111701
dc.rights(c) American Physical Society, 2009
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationForats negres (Astronomia)
dc.subject.otherBlack holes (Astronomy)
dc.titleInstability and new phases of higher-dimensional rotating black holes
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion

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