General Non-Extremal Rotating Black Holes in Minimal Five-Dimensional Gauged Supergravity

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dc.creatorChong, Z. -W.
dc.creatorCvetic, M.
dc.creatorLu, H.
dc.creatorPope, C. N.
dc.date2005-06-02
dc.date.accessioned2026-07-07T11:27:15Z
dc.date.available2026-07-07T11:27:15Z
dc.descriptionWe construct the general solution for non-extremal charged rotating black holes in five-dimensional minimal gauged supergravity. They are characterised by four non-trivial parameters, namely the mass, the charge, and the two independent rotation parameters. The metrics in general describe regular rotating black holes, providing the parameters lie in appropriate ranges so that naked singularities and closed timelike curves (CTC's) are avoided. We calculate the conserved energy, angular momenta and charge for the solutions, and show how supersymmetric solutions arise in a BPS limit. These have naked CTC's in general, but for special choices of the parameters we obtain new regular supersymmetric black holes or smooth topological solitons.
dc.descriptionrevtex, 4 pages
dc.identifierhttps://arxiv.org/abs/hep-th/0506029
dc.identifierhttp://arxiv.org/abs/hep-th/0506029
dc.identifierPhys.Rev.Lett.95:161301,2005
dc.identifierdoi:10.1103/PhysRevLett.95.161301
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196093
dc.subjectHigh Energy Physics - Theory
dc.titleGeneral Non-Extremal Rotating Black Holes in Minimal Five-Dimensional Gauged Supergravity
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