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Viable cosmology in bimetric theory

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arxiv 1404.0008 v2 pith:MMQDSMK6 submitted 2014-03-31 hep-th astro-ph.COgr-qc

classification hep-thastro-ph.COgr-qc
keywords perturbationsabsencebimetricbranchconditioncosmologicalgradienthealthy
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We study cosmological perturbations in bimetric theory with two fluids each of which is coupled to one of the two metrics. Focusing on a healthy branch of background solutions, we clarify the stability of the cosmological perturbations. For this purpose, we extend the condition for the absence of the so-called Higuchi ghost, and show that the condition is guaranteed to be satisfied on the healthy branch. We also calculate the squared propagation speeds of perturbations and derive the conditions for the absence of the gradient instability. To avoid the gradient instability, we find that the model parameters are weakly constrained.

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  1. Dynamical Dark Energy Emerges from Massive Gravity

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    Bigravity with a graviton mass near 4e-33 eV reproduces the DESI-hinted evolving dark energy and is claimed to fit combined cosmological data better than LambdaCDM.

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