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Stable cosmology in ghost-free quasidilaton theory

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arxiv 1707.02004 v1 pith:NEIUZOW3 submitted 2017-07-07 hep-th astro-ph.COgr-qc

classification hep-thastro-ph.COgr-qc
keywords quasidilatonsolutiontheorycosmologicalfutureghost-freeacquireasymptotic
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We present a novel cosmological solution in the framework of extended quasidilaton theory which underwent scrutiny recently. We only consider terms that do not generate the Boulware-Deser degree of freedom, hence the "ghost-free" quasidilaton theory, and show three new branches of cosmological evolution therein. One of the solutions passes the perturbative stability tests. This new solution exhibits a late time self-acceleration and all graviton polarizations acquire masses that converge to a constant in the asymptotic future. Moreover, all modes propagate at the speed of light. We propose that this solution can be used as a benchmark model for future phenomenological studies.

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Cited by 1 Pith paper

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  1. Vector Perturbations in Ghost-Free Quasidilaton Massive Gravity

    gr-qc 2026-08 conditional novelty 6.0 of 10

    Minimal scalar, Maxwell, or Proca matter does not restore the vanishing vector kinetic coefficient K_V on Branch II of ghost-free quasidilaton massive gravity.

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