Classical non-Gaussianity from non-linear evolution of curvature
  perturbations
  We study the non-linear evolution of the curvature perturbations during
matter dominated era. We show that regardless of the origin of the primordial
perturbation, the Bardeen potential and curvature receive sizable contributions
from the classical non-linear evolution effects, and quantify them exactly. On
the super-horizon scales we have squeezed peak of the bispectrum with
magnitude, in terms of the local non-linear parameters of Bardeen curvature,
1/6 < f_{NL} 19/15, and of Bardeen potential, -1/4 < f_{NL} < 7/5, depending on
the configuration of momenta. On the sub-horizon scales the bispectrum show
equilateral shape, and can serve as a potential probe of general relativity.
