Cosmology in massive gravity

Abstract

We argue that more cosmological solutions in massive gravity can be obtained if the metric tensor and the tensor ${\Sigma }_{\mu \nu }$ defined by Stückelberg fields take the homogeneous and isotropic form. The standard cosmology with matter and radiation dominations in the past can be recovered and $\Lambda$CDM model is easily obtained. The dynamical evolution of the universe is modified at very early times.

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• Oscillating universe in massive gravity
• Perturbations for massive gravity theories
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• Hamiltonian Formalism of Bimetric Gravity In Vierbein Formulation
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• Perturbations of Cosmological and Black Hole Solutions in Massive gravity and Bi-gravity
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• Milgrom's Law and Lambda's Shadow: How Massive Gravity Connects Galactic and Cosmic Dynamics