Horizon Properties of Einstein-Yang-Mills Black Hole
General Relativity and Quantum Cosmology
2009-11-07 v1
Abstract
We consider static axially symmetric Einstein-Yang-Mills black holes in the isolated horizon formalism. The mass of these hairy black holes is related to the mass of the corresponding particle-like solutions by the horizon mass. The hairy black holes violate the ``quasi-local uniqueness conjecture'', based on the horizon charges.
Keywords
Cite
@article{arxiv.gr-qc/0110084,
title = {Horizon Properties of Einstein-Yang-Mills Black Hole},
author = {B. Kleihaus and J. Kunz and A. Sood and M. Wirschins},
journal= {arXiv preprint arXiv:gr-qc/0110084},
year = {2009}
}
Comments
4 pages, 3 figues