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arXiv · 1908.08247

Constraints on Quasi-dilaton Massive Gravity

Katarina Martinovic·Mairi Sakellariadou
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Abstract

The last decade has seen great advancements in the field of modified gravity, motivated by the dark energy problem, or by the search for a fundamental quantum gravity theory. With a phenomenologically-driven approach, we consider dRGT theory and its extension, quasi-dilaton massive gravity (QDMG). When looking for ways to constrain the theory, a promising direction appeared to be astrophysical tests. The scalar gravitational degree of freedom and quasi-dilaton degree of freedom alter the evolution of Bardeen potentials, which in turn affects the galaxy rotation curves. We find an upper bound on graviton mass in QDMG to be $m \leq 10^{-31} {\rm eV}$. This result agrees with bounds from LIGO and numerous Solar System tests. However, the extremely small mass of the graviton remains a detection out of reach, with LISA's sensitivity exploring the parameter space up to $m \leq 10^{-25} {\rm eV}$.

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BibTeXRIS

Katarina Martinovic, Mairi Sakellariadou. 2019-08-22. Constraints on Quasi-dilaton Massive Gravity. https://doi.org/10.1103/physrevd.100.124016

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