Non-Gaussianity from Broken Symmetries
Astrophysics
2008-11-26 v1 High Energy Physics - Phenomenology
High Energy Physics - Theory
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.
Cite
@article{arxiv.astro-ph/0511198,
title = {Non-Gaussianity from Broken Symmetries},
author = {Edward W. Kolb and Antonio Riotto and Alberto Vallinotto},
journal= {arXiv preprint arXiv:astro-ph/0511198},
year = {2008}
}
Comments
7 pages, 1 figure