Cosmology of the Galileon from Massive Gravity
Claudia de Rham, Lavinia Heisenberg (DPT, CAP Geneve)

TL;DR
This paper studies a covariantized version of massive gravity's decoupling limit, revealing a self-accelerating cosmological solution, stability conditions, and effects on structure formation, highlighting the importance of frame choice in proxy theories.
Contribution
It introduces a covariant proxy for massive gravity's decoupling limit and analyzes its cosmological solutions, stability, and implications for structure formation.
Findings
Existence of a self-accelerating solution with Hubble parameter equal to graviton mass
Stable fluctuations around the self-accelerating background for certain parameters
Helicity-0 mode enhances structure formation relative to LCDM
Abstract
We covariantize the decoupling limit of massive gravity proposed in arXiv:1011.1232 and study the cosmology of this theory as a proxy, which embodies key features of the fully non-linear covariant theory. We first confirm that it exhibits a self-accelerating solution, similar to what has been found in arXiv:1010.1780, where the Hubble parameter corresponds to the graviton mass. For a certain range of parameters fluctuations relative to the self-accelerating background are stable and form an attractor solution. We also show that a degravitating solution can not be constructed in this covariantized proxy theory in a meaningful way. As for cosmic structure formation, we find that the helicity-0 mode of the graviton causes an enhancement relative to LCDM. For consistency we also compare proxy theories obtained starting from different frames in the decoupling limit and discuss the…
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