Higher dimensional slowly rotating dilaton black holes in AdS spacetime

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dc.creatorSheykhi, A.
dc.creatorAllahverdizadeh, M.
dc.date2008-09-06
dc.date2008-09-21
dc.date.accessioned2026-07-07T11:45:45Z
dc.date.available2026-07-07T11:45:45Z
dc.descriptionIn this paper, with an appropriate combination of three Liouville-type dilaton potentials, we obtain the higher dimensional charged slowly rotating dilaton black hole solution for asymptotically anti-de Sitter spacetime. The angular momentum and the gyromagnetic ratio of such a black hole are determined for the arbitrary values of the dilaton coupling constant. It is shown that the dilaton field modifies the gyromagnetic ratio of the rotating dilaton black holes.
dc.description11 pages, 1 figure, the version to appear in Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/0809.1131
dc.identifierhttp://arxiv.org/abs/0809.1131
dc.identifierPhys.Rev.D78:064073,2008
dc.identifierdoi:10.1103/PhysRevD.78.064073
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201988
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHigher dimensional slowly rotating dilaton black holes in AdS spacetime
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