Asymptotically non-flat rotating dilaton black holes
arXiv:gr-qc/0212057 · doi:10.1088/0264-9381/20/7/311
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.
LaTeX, 8 pages, slightly modified version to appear in Classical and Quantum Gravity (http://www.iop.org)
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