Slowly Rotating Dilaton Black hole In Anti-de Sitter Spacetime

Abstract

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

References in corpus (2)

• Dark energy cosmology from higher-order, string-inspired gravity and its reconstruction
• Electromagnetic Properties of Kerr-Anti-de Sitter Black Holes

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