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2013

Stability of the Self-accelerating Universe in Massive Gravity

Khosravi, Nima, Niz, Gustavo, Koyama, Kazuya et al.

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We study linear perturbations around time dependent spherically symmetric solutions in the Lambda_3 massive gravity theory, which self-accelerate in the vacuum.

We find that the dynamics of the scalar perturbations depend on the coordinate choice for the background solutions.
For particular choices of coordinates there is a symmetry enhancement, leaving no propagating scalar degrees of freedom at linear order in perturbations.
In contrast, any other coordinate choice propagates a single scalar mode.

Stability of the Self-accelerating Universe in Massive Gravity · Around

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