Slowly Rotating Dilaton Black hole In Anti-de Sitter Spacetime
arXiv:0709.2754 · doi:10.1103/PhysRevD.76.087504
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