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

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dc.creatorChong, Z. W.
dc.creatorCvetic, M.
dc.creatorLu, H.
dc.creatorPope, C. N.
dc.date2006-06-21
dc.date2006-10-30
dc.date.accessioned2026-07-07T11:06:43Z
dc.date.available2026-07-07T11:06:43Z
dc.descriptionSupersymmetric black holes in five-dimensional gauged supergravity must necessarily be rotating, and so in order to study the passage to black holes away from supersymmetry, it is of great interest to obtain non-extremal black holes that again have non-zero rotation. In this paper we find a simple framework for describing non-extremal rotating black holes in five-dimensional gauged supergravities. Using this framework, we are able to construct a new solution, describing the general single-charge solution of N=2 gauged supergravity, with arbitrary values for the two rotation parameters. Previously-obtained solutions with two or three equal charges also assume a much simpler form in the new framework, as also does the general solution with three unequal charges in ungauged N=2 supergravity. We discuss the thermodynamics and BPS limit of the new single-charge solutions, and we discuss the separability of the Hamilton-Jacobi and Klein-Gordan equations in these backgrounds.
dc.descriptionLatex, 12 pages. Mis-statement about separability of Hamilton-Jacobi and Klein-Gordon equations corrected
dc.identifierhttps://arxiv.org/abs/hep-th/0606213
dc.identifierhttp://arxiv.org/abs/hep-th/0606213
dc.identifierPhys.Lett.B644:192-197,2007
dc.identifierdoi:10.1016/j.physletb.2006.11.012
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/189613
dc.subjectHigh Energy Physics - Theory
dc.titleNon-Extremal Rotating Black Holes in Five-Dimensional Gauged Supergravity
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