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Slowly rotating dilaton black hole in anti–de Sitter spacetime

Tanwi Ghosh* and Soumitra SenGupta

  • Department of Theoretical Physics, Indian Association for the Cultivation of Science, Jadavpur, Calcutta–700 032, India

  • *tanwi.ghosh@yahoo.co.in
  • tpssg@iacs.res.in

Phys. Rev. D 76, 087504 – Published 24 October, 2007

DOI: https://doi.org/10.1103/PhysRevD.76.087504

Abstract

A rotating dilaton black hole solution for asymptotically anti-de Sitter spacetime is 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.

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