arXiv:astro-ph/0511198·v1·Astrophysics
Non-Gaussianity from Broken Symmetries
Edward W. Kolb🇺🇸 · Antonio Riotto🇨🇭 · Alberto Vallinotto🇺🇸
Abstract
Recently we studied inflation models in which the inflaton potential is characterized by an underlying approximate global symmetry. In the first work we pointed out that in such a model curvature perturbations are generated after the end of the slow-roll phase of inflation. In this work we develop further the observational implications of the model and compute the degree of non-Gaussianity predicted in the scenario. We find that the corresponding nonlinearity parameter, , can be as large as 10^2.
Comments: 7 pages, 1 figure