Rotating Black Holes in Einstein-Maxwell-Dilaton Gravity

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dc.creatorSheykhi, Ahmad
dc.date2007-11-28
dc.date2008-05-10
dc.date.accessioned2026-07-07T11:38:57Z
dc.date.available2026-07-07T11:38:57Z
dc.descriptionWe present a new class of slowly rotating black hole solutions in $(n+1)$-dimensional $(n\geq3)$ Einstein-Maxwell-dilaton gravity in the presence of Liouville-type potential for the dilaton field and an arbitrary value of the dilaton coupling constant. Because of the presence of the dilaton field, the asymptotic behaviour of these solutions are neither flat nor (A)dS. In the absence of a dilaton field, our solution reduces to the $(n+1)$-dimensional Kerr-Newman modification thereof for small rotation parameter \cite{Aliev2}. We also compute the angular momentum and the gyromagnetic ratio of these rotating dilaton black holes.
dc.description9 pages, 7 figures, references added, to appear in Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/0711.4422
dc.identifierhttp://arxiv.org/abs/0711.4422
dc.identifierPhys.Rev.D77:104022,2008
dc.identifierdoi:10.1103/PhysRevD.77.104022
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/199754
dc.subjectHigh Energy Physics - Theory
dc.titleRotating Black Holes in Einstein-Maxwell-Dilaton Gravity
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