Slowly Rotating Dilaton Black hole In Anti-de Sitter Spacetime

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Rotating 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.
5 pages, Revtex, To appear in Phys.Rev.D

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High Energy Physics - Theory, General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/199146

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0709.2754
 http://arxiv.org/abs/0709.2754
 Phys.Rev.D76:087504,2007
 doi:10.1103/PhysRevD.76.087504

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arXiv