A boundary value problem for the five-dimensional stationary rotating black holes
General Relativity and Quantum Cosmology
2010-11-19 v1
Abstract
We study the boundary value problem for the stationary rotating black hole solutions to the five-dimensional vacuum Einstein equation. Assuming the two commuting rotational symmetry and the sphericity of the horizon topology, we show that the black hole is uniquely characterized by the mass, and a pair of the angular momenta.
Cite
@article{arxiv.gr-qc/0401100,
title = {A boundary value problem for the five-dimensional stationary rotating black holes},
author = {Yoshiyuki Morisawa and Daisuke Ida},
journal= {arXiv preprint arXiv:gr-qc/0401100},
year = {2010}
}
Comments
16 pages, no figures