Non-Abelian Black Holes and Catastrophe Theory II: Charged Type

Details Non-Abelian Black Holes and Catastrophe Theory II: Charged Type Non-Abelian Black Holes and Catastrophe Theory II: Charged Type

1994-10-13

arxiv.org/abs/gr-qc/9410016v2

Phys.Rev. D51 (1995) 4054-4066

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

23 pages, LaTeX (Figures are available on request as hard copies.) WU-AP/40/93

Scientific paper

10.1103/PhysRevD.51.4054

We reanalyze the gravitating monopole and its black hole solutions in the Einstein-Yang-Mills-Higgs system and we discuss their stabilities from the point of view of catastrophe theory. Although these non-trivial solutions exhibit fine and complicated structures, we find that stability is systematically understood via a swallow tail catastrophe. The Reissner-Nordstr\"{o}m trivial solution becomes unstable from the point where the non-trivial monopole black hole appears. We also find that, within a very small parameter range, the specific heat of a monopole black hole changes its sign .

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