Slowly Rotating Dilaton Black hole In Anti-de Sitter Spacetime

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dc.creatorGhosh, Tanwi
dc.creatorSenGupta, Soumitra
dc.date2007-09-18
dc.date.accessioned2026-07-07T11:37:15Z
dc.date.available2026-07-07T11:37:15Z
dc.descriptionRotating dilaton black hole solution for asymptotically anti-de Sitter spacetime are obtained in the small angular momentum limit with an appropriate combination of three Liouville-type dilaton potentials. The angular momentum, magnetic dipole moment and the gyromagnetic ratio of such a black hole are determined for arbitrary values of the dilaton-electromagnetic coupling parameter.
dc.description5 pages, Revtex, To appear in Phys.Rev.D
dc.identifierhttps://arxiv.org/abs/0709.2754
dc.identifierhttp://arxiv.org/abs/0709.2754
dc.identifierPhys.Rev.D76:087504,2007
dc.identifierdoi:10.1103/PhysRevD.76.087504
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/199146
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSlowly Rotating Dilaton Black hole In Anti-de Sitter Spacetime
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