Non-gaussianity in curvaton models with nearly quadratic potentials

被引:121
作者
Enqvist, K
Nurmi, S
机构
[1] Univ Helsinki, Inst Phys, FIN-00014 Helsinki, Finland
[2] Univ Helsinki, Dept Phys Sci, FIN-00014 Helsinki, Finland
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2005年 / 10期
关键词
cosmological perturbation theory; inflation;
D O I
10.1088/1475-7516/2005/10/013
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider curvaton models with potentials that depart slightly from the quadratic form. We show that although such a small departure does not significantly modify 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, vertical bar fNL vertical bar << 1, is quite possible even with small curvaton energy density r << 1. Furthermore, non-Gaussianity does not imply any strict bounds on r, but the bounds depend on the assumptions about the higher order terms in the curvaton potential.
引用
收藏
页码:163 / 173
页数:11
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