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Stability of Non-Abelian Black Holes

K. Maeda·T. Tachizawa·T. Torii·T. Maki
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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.

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K. Maeda, T. Tachizawa, T. Torii, T. Maki. 1993-10-08. Stability of Non-Abelian Black Holes. https://doi.org/10.1103/physrevlett.72.450

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