Stability of Non-Abelian Black Holes
arXiv:gr-qc/9310015 · doi:10.1103/PhysRevLett.72.450
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.
4 Figures to be sent on request,8 pages, WU-AP/33/93
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