Non-Abelian black holes and catastrophe theory. II. Charged type

T. Tachizawa, Keiichi Maeda, T. Torii

    Research output: Contribution to journalArticle

    61 Citations (Scopus)

    Abstract

    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.

    Original languageEnglish
    Pages (from-to)4054-4066
    Number of pages13
    JournalPhysical Review D
    Volume51
    Issue number8
    DOIs
    Publication statusPublished - 1995

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    catastrophe theory
    monopoles
    fine structure
    specific heat

    ASJC Scopus subject areas

    • Physics and Astronomy (miscellaneous)

    Cite this

    Non-Abelian black holes and catastrophe theory. II. Charged type. / Tachizawa, T.; Maeda, Keiichi; Torii, T.

    In: Physical Review D, Vol. 51, No. 8, 1995, p. 4054-4066.

    Research output: Contribution to journalArticle

    Tachizawa, T. ; Maeda, Keiichi ; Torii, T. / Non-Abelian black holes and catastrophe theory. II. Charged type. In: Physical Review D. 1995 ; Vol. 51, No. 8. pp. 4054-4066.
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