Abstract
We discuss the stability of static cosmological solutions in the framework of the dRGT theory of massive gravity (de Rham and Gabadadze, Phys. Rev. D82:044020, 2010). These solutions, only sourced by a perfect fluid, are either neutrally stable or unstable against spatially homogeneous and isotropic perturbations thus generalizing the Einstein static universe found in General Relativity. This paper summarises the results presented in (Phys Rev D 86:024035, 2012).
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