Slowly Rotating Dilaton Black hole In Anti-de Sitter Spacetime
Tanwi Ghosh, Soumitra SenGupta
TL;DR
This paper derives a rotating dilaton black hole solution in anti-de Sitter spacetime, analyzing its physical properties such as angular momentum, magnetic dipole moment, and gyromagnetic ratio for various coupling parameters.
Contribution
It presents a new solution for slowly rotating dilaton black holes in AdS spacetime with detailed physical property calculations for arbitrary coupling.
Findings
Derived the black hole solution in the small angular momentum limit.
Calculated angular momentum, magnetic dipole moment, and gyromagnetic ratio.
Analyzed effects of dilaton-electromagnetic coupling on black hole properties.
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.
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