Monopole inflation in Brans-Dicke theory

Nobuyuki Sakai, Jun'ichi Yokoyama, Keiichi Maeda

    Research output: Contribution to journalArticle

    4 Citations (Scopus)

    Abstract

    According to previous work, topological defects expand exponentially without end if the vacuum expectation value of the Higgs field is of the order of the Planck mass. We extend the study of inflating topological defects to Brans-Dicke gravity. With the help of numerical simulations we investigate the dynamics and spacetime structure of a global monopole. Contrary to the case of Einstein gravity, any inflating monopole eventually shrinks and takes a stable configuration. We also discuss cosmological constraints on the model parameters.

    Original languageEnglish
    Pages (from-to)1-8
    Number of pages8
    JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
    Volume59
    Issue number10
    Publication statusPublished - 1999 May 15

    Fingerprint

    inflating
    Topological Defects
    Monopole
    monopoles
    Inflation
    Gravity
    gravitation
    defects
    Higgs
    Expand
    Albert Einstein
    Vacuum
    Space-time
    Numerical Simulation
    vacuum
    Configuration
    configurations
    simulation
    Model

    ASJC Scopus subject areas

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

    Cite this

    Monopole inflation in Brans-Dicke theory. / Sakai, Nobuyuki; Yokoyama, Jun'ichi; Maeda, Keiichi.

    In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 59, No. 10, 15.05.1999, p. 1-8.

    Research output: Contribution to journalArticle

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