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2013

Cosmology in General Massive Gravity Theories

Comelli, Denis, Nesti, Fabrizio, Pilo, Luigi

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We study the cosmology of general massive gravity theories with five propagating degrees of freedom.

This large class of theories includes both the case with a residual Lorentz invariance as the cases with simpler rotational invariance.
We find that the existence of a nontrivial homogeneous FRW background, in addition to selecting the lorentz-breaking case, implies in general that perturbations around strict Minkowski or dS space are strongly coupled.
The result is that dark energy can be naturally accounted for in massive gravity but its equation of state w_eff has to deviate from -1.

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