Five-Dimensional Charged Rotating Black Holes
General Relativity and Quantum Cosmology
2009-11-11 v1
Abstract
We consider charged rotating black holes in 5-dimensional Einstein-Maxwell theory. These black holes are asymptotically flat, they possess a regular horizon of spherical topology and two independent angular momenta associated with two distinct planes of rotation. We discuss their global and horizon properties, and derive a generalized Smarr formula. We construct these black holes numerically, focussing on black holes with a single angular momentum, and with two equal-magnitude angular momenta.
Cite
@article{arxiv.gr-qc/0503010,
title = {Five-Dimensional Charged Rotating Black Holes},
author = {Jutta Kunz and Francisco Navarro-Lerida and Anna Katinka Petersen},
journal= {arXiv preprint arXiv:gr-qc/0503010},
year = {2009}
}
Comments
13 pages, 8 figures