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Selfacceleration with Quasidilaton

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arxiv 1401.5403 v1 pith:J3BPLZZP submitted 2014-01-21 hep-th astro-ph.CO

Selfacceleration with Quasidilaton

classification hep-th astro-ph.CO
keywords solutiontheorymassiveperturbationsquasidilatonself-acceleratedspaceadditional
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Quasidilaton massive gravity is an extension of massive General Relativity to a theory with additional scale invariance and approximate internal Galilean symmetry. The theory has a novel self-accelerated solution with the metric indistinguishable (in the decoupling limit) from the de Sitter space, its curvature set by the graviton mass. The spectra of tensor, vector, and scalar perturbations on this solution contain neither ghosts, nor gradient instabilities or superluminal modes, for a range of the parameter space. This represents an example of a self-accelerated solution with viable perturbations, attainable within a low energy effective field theory.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Cosmological horizon thermodynamics in Gauss-Bonnet quasi-dilaton Massive Gravity

    gr-qc 2026-07 reject novelty 5.0

    Gauss-Bonnet quasi-dilaton massive gravity is claimed to obey horizon thermodynamics and the holographic entropy bound, provided the Gauss-Bonnet coupling is non-negative.