Vainshtein solutions without superluminal modes

Gregory Gabadadze, Rampei Kimura, David Pirtskhalava

    Research output: Contribution to journalArticle

    Abstract

    The Vainshtein mechanism suppresses the fifth force at astrophysical distances, while enabling it to compete with gravity at cosmological scales. Typically, Vainshtein solutions exhibit superluminal perturbations. However, a restricted class of solutions with special boundary conditions was shown to be devoid of the faster-than-light modes. Here we extend this class by finding solutions in a theory of quasidilaton, amended by derivative terms consistent with its symmetries. Solutions with Minkowski asymptotics are not stable, while the ones that exhibit the Vainshtein mechanism by transitioning to cosmological backgrounds are free of ghosts, tachyons, gradient instability, and superluminality, for all propagating modes present in the theory. These solutions require a special choice of the strength and signs of nonlinear terms, as well as a choice of asymptotic cosmological boundary conditions.

    Original languageEnglish (US)
    Article number124024
    JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
    Volume91
    Issue number12
    DOIs
    StatePublished - Jun 8 2015

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    boundary conditions
    tachyons
    ghosts
    astrophysics
    gravitation
    perturbation
    gradients
    symmetry

    ASJC Scopus subject areas

    • Nuclear and High Energy Physics

    Cite this

    Vainshtein solutions without superluminal modes. / Gabadadze, Gregory; Kimura, Rampei; Pirtskhalava, David.

    In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 91, No. 12, 124024, 08.06.2015.

    Research output: Contribution to journalArticle

    Gabadadze, Gregory ; Kimura, Rampei ; Pirtskhalava, David. / Vainshtein solutions without superluminal modes. In: Physical Review D - Particles, Fields, Gravitation and Cosmology. 2015 ; Vol. 91, No. 12.
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