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Asymptotically non-flat rotating dilaton black holes

Tanwi Ghosh·P. Mitra
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Abstract

Dilaton black hole solutions which are neither asymptotically flat nor (anti)-de Sitter but reduce to asymptotically flat solutions in some special limits have been known for a Liouville type dilatonic potential. It is shown how, by solving a pair of coupled differential equations, infinitesimally small angular momentum can be added to these static solutions to produce rotating black hole solutions.

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Tanwi Ghosh, P. Mitra. 2003-03-13. Asymptotically non-flat rotating dilaton black holes. https://doi.org/10.1088/0264-9381%2F20%2F7%2F311

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