  We propose a curvaton model in which the initial condition of the curvaton
oscillation is determined by its attractor behavior during inflation. Assuming
a chaotic inflation model, we find that the initial condition determined by the
attractor behavior is appropriate to generate a sizable non-Gaussianity
contribution to the curvature perturbation, which will be tested in the
foreseeable future. Implications on the thermal history of the universe and on
particle physics models are also discussed.

High Energy Physics - Phenomenology;Cosmology and Nongalactic Astrophysics