Properties of black hole solutions in the SU(3) Einstein-Yang-Mills-dilaton system

Keiichi Maeda, Masakazu Inada

    Research output: Contribution to journalArticle

    Abstract

    We consider black hole solutions in the SU(3) Einstein-Yang-Mills-dilaton system under the static and spherically symmetric ansatz. We reveal some properties which were not investigated before. In particular, we find that there appears a shell-like structure in the energy density distribution outside the horizon which can be interpreted as a symptom of the instability of black holes.

    Original languageEnglish
    Number of pages1
    JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
    Volume63
    Issue number8
    DOIs
    Publication statusPublished - 2001 Jan 1

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    horizon
    density distribution
    flux density

    ASJC Scopus subject areas

    • Nuclear and High Energy Physics
    • Physics and Astronomy (miscellaneous)

    Cite this

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    abstract = "We consider black hole solutions in the SU(3) Einstein-Yang-Mills-dilaton system under the static and spherically symmetric ansatz. We reveal some properties which were not investigated before. In particular, we find that there appears a shell-like structure in the energy density distribution outside the horizon which can be interpreted as a symptom of the instability of black holes.",
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