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2014

Stable and unstable cosmological models in bimetric massive gravity

Könnig, Frank, Akrami, Yashar, Amendola, Luca et al.

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Nonlinear, ghost-free massive gravity has two tensor fields; when both are dynamical, the mass of the graviton can lead to cosmic acceleration that agrees with background data, even in the absence of a cosmological constant.

Here the question of the stability of linear perturbations in this bimetric theory is examined.
Instabilities are presented for several classes of models, and simple criteria for the cosmological stability of massive bigravity are derived.
In this way, we identify a particular self-accelerating bigravity model, infinite-branch bigravity (IBB), which exhibits both viable background evolution and stable linear perturbations.

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