Rotating Einstein-Maxwell-Dilaton Black Holes in D Dimensions

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dc.creatorKunz, Jutta
dc.creatorMaison, Dieter
dc.creatorNavarro-Lerida, Francisco
dc.creatorViebahn, Jan
dc.date2006-06-01
dc.date.accessioned2026-07-07T11:06:35Z
dc.date.available2026-07-07T11:06:35Z
dc.descriptionWe construct exact charged rotating black holes in Einstein-Maxwell-dilaton theory in $D$ spacetime dimensions, $D \ge 5$, by embedding the $D$ dimensional Myers-Perry solutions in $D+1$ dimensions, and performing a boost with a subsequent Kaluza-Klein reduction. Like the Myers-Perry solutions, these black holes generically possess $N=[(D-1)/2]$ independent angular momenta. We present the global and horizon properties of these black holes, and discuss their domains of existence.
dc.description12 pages, 6 figues
dc.identifierhttps://arxiv.org/abs/hep-th/0606005
dc.identifierhttp://arxiv.org/abs/hep-th/0606005
dc.identifierPhys.Lett.B639:95-100,2006
dc.identifierdoi:10.1016/j.physletb.2006.06.024
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/189570
dc.subjectHigh Energy Physics - Theory
dc.titleRotating Einstein-Maxwell-Dilaton Black Holes in D Dimensions
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