Anisotropic Friedmann-Robertson-Walker universe from nonlinear massive
  gravity
  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.
