On the gravitational stability of D1-D5-P black holes

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dc.creatorCardoso, Vitor
dc.creatorDias, Oscar J. C.
dc.creatorMyers, Robert C.
dc.date2007-07-23
dc.date2007-10-08
dc.date.accessioned2026-07-07T10:56:53Z
dc.date.available2026-07-07T10:56:53Z
dc.descriptionWe examine the stability of the nonextremal D1-D5-P black hole solutions. In particular, we look for the appearance of a superradiant instability for the spinning black holes but we find no evidence of such an instability. We compare this situation with that for the smooth soliton geometries, which were recently observed to suffer from an ergoregion instability, and consider the implications for the fuzzball proposal.
dc.description18 pages, 3 figures. Minor comments added to match published version
dc.identifierhttps://arxiv.org/abs/0707.3406
dc.identifierhttp://arxiv.org/abs/0707.3406
dc.identifierPhys.Rev.D76:105015,2007
dc.identifierdoi:10.1103/PhysRevD.76.105015
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186567
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn the gravitational stability of D1-D5-P black holes
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