1301.6552 (N. A. Koshelev)
N. A. Koshelev
The general expression for the second order large scale curvature perturbation in the form of a functional over a background solution is derived. The explicit expressions was obtained for two special forms of the inflationary potential. In the considered cases, it is shown that a significant level of non-Gaussianity can be generated during the super-Hubble evolution only if nonadiabatic perturbations dominate at the end of inflation.
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http://arxiv.org/abs/1301.6552
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