Asymptotically non-flat rotating dilaton black holes
General Relativity and Quantum Cosmology
2017-08-23 v2 High Energy Physics - Theory
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.
Keywords
Cite
@article{arxiv.gr-qc/0212057,
title = {Asymptotically non-flat rotating dilaton black holes},
author = {Tanwi Ghosh and P. Mitra},
journal= {arXiv preprint arXiv:gr-qc/0212057},
year = {2017}
}
Comments
LaTeX, 8 pages, slightly modified version to appear in Classical and Quantum Gravity (http://www.iop.org)