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Self-acceleration with quasidilaton

Gregory GabadadzeCenter for Cosmology and Particle Physics, Department of Physics, New York University, New York, New York 10003, USARampei KimuraResearch Center for the Early Universe, The University of Tokyo, Tokyo 113-0033, JapanDavid PirtskhalavaScuola Normale Superiore, Piazza dei Cavalieri 7, 56126 Pisa, Italy
2014en
ABI

Аннотация

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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