Non-Gaussianity in Curvaton Models with Nearly Quadratic Potential
Astrophysics
2008-11-26 v2
Abstract
We consider curvaton models with potentials that depart slightly from the quadratic form. We show that although such a small departure does not modify significantly the Gaussian part of the curvature perturbation, it can have a pronounced effect on the level of non-Gaussianity. We find that unlike in the quadratic case, the limit of small non-Gaussianity, , is quite possible even with small curvaton energy density . Furthermore, non-Gaussianity does not imply any strict bounds on but the bounds depend on the assumptions about the higher order terms in the curvaton potential.
Cite
@article{arxiv.astro-ph/0508573,
title = {Non-Gaussianity in Curvaton Models with Nearly Quadratic Potential},
author = {Kari Enqvist and Sami Nurmi},
journal= {arXiv preprint arXiv:astro-ph/0508573},
year = {2008}
}
Comments
11 pages, 3 figures. Minor changes. Typos corrected and a reference added