Asymptotically non-flat rotating dilaton black holes
classification
🌀 gr-qc
hep-th
keywords
solutionsasymptoticallyblackdilatonflatholerotatingadded
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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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