Anisotropic Friedmann-Robertson-Walker universe from nonlinear massive gravity
arXiv:1206.2723 · doi:10.1016/j.physletb.2012.09.049
Abstract
In the scope of the nonlinear massive gravity, we study fixed points of evolution equations for a Bianchi type--I universe. We find a new attractor solution with non-vanishing anisotropy, on which the physical metric is isotropic but the Stuckelberg configuration is anisotropic. As a result, at the background level, the solution describes a homogeneous and isotropic universe, while a statistical anisotropy is expected from perturbations, suppressed by smallness of the graviton mass.
4 pages, 1 figure, REVTeX4; V2 with minor revison, and to appear on PLB
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