Higher dimensional slowly rotating dilaton black holes in AdS spacetime
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In 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.
11 pages, 1 figure, the version to appear in Phys. Rev. D
11 pages, 1 figure, the version to appear in Phys. Rev. D