Stability of Non-Abelian Black Holes
General Relativity and Quantum Cosmology
2009-10-22 v1 High Energy Physics - Theory
Abstract
Two types of self-gravitating particle solutions found in several theories with non-Abelian fields are smoothly connected by a family of non-trivial black holes. There exists a maximum point of the black hole entropy, where the stability of solutions changes. This criterion is universal, and the changes in stability follow from a catastrophe-theoretic analysis of the potential function defined by black hole entropy.
Keywords
Cite
@article{arxiv.gr-qc/9310015,
title = {Stability of Non-Abelian Black Holes},
author = {K. Maeda and T. Tachizawa and T. Torii and T. Maki},
journal= {arXiv preprint arXiv:gr-qc/9310015},
year = {2009}
}
Comments
4 Figures to be sent on request,8 pages, WU-AP/33/93