Asymptotically non-flat rotating dilaton black holes

Details Asymptotically non-flat rotating dilaton black holes Asymptotically non-flat rotating dilaton black holes

2002-12-12

arxiv.org/abs/gr-qc/0212057v2

Class.Quant.Grav. 20 (2003) 1403-1410

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

LaTeX, 8 pages, slightly modified version to appear in Classical and Quantum Gravity (http://www.iop.org)

Scientific paper

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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