Phys. Rev. D 51, 4054–4066 (1995)Non-Abelian black holes and catastrophe theory. II. Charged typeReceived 12 October 1994; published in the issue dated 15 April 1995 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 nontrivial solutions exhibit fine and complicated structures, we find that stability is systematically understood via a swallow tail catastrophe. The Reissner-Nordström trivial solution becomes unstable from the point where the nontrivial 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. © 1995 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevD.51.4054
DOI:
10.1103/PhysRevD.51.4054
PACS:
04.70.Bw, 11.15.-q, 95.30.Tg, 14.80.Hv
|
|
About | Terms and Conditions | Subscriptions | Search | Help
Use of the American Physical Society websites and journals implies that the user has read and agrees to our Terms and Conditions and any applicable Subscription Agreement. Physical Review®, Physical Review Letters®, Reviews of Modern Physics®, and Physical Review Special Topics® are trademarks of the American Physical Society.