English

The self-interacting curvaton

Cosmology and Nongalactic Astrophysics 2015-05-20 v1

Abstract

The evolution of the curvature perturbation is highly non-trivial for curvaton models with self-interactions and is very sensitive to the parameter values. The final perturbation depends also on the curvaton decay rate Γ\Gamma. As a consequence, non-gaussianities can be greatly different from the purely quadratic case, even if the deviation is very small. Here we consider a class of polynomial curvaton potentials and discuss the dynamical behavior of the curvature perturbation. We point out that, for example, it is possible that the non-gaussianity parameter \fnl0\fnl\simeq 0 while \gnl\gnl is non-zero. In the case of a curvaton with mass mO(1)m\sim {\cal O}(1) TeV we show that one cannot ignore non-quadratic terms in the potential, and that only a self-interaction of the type Vint=σ8/M4V_{\rm int}=\sigma^8/M^4 is consistent with various theoretical and observational constraints. Moreover, the curvaton decay rate should then be in the range Γ=10151017\Gamma=10^{-15}- 10^{-17} GeV.

Keywords

Cite

@article{arxiv.1012.1711,
  title  = {The self-interacting curvaton},
  author = {Kari Enqvist},
  journal= {arXiv preprint arXiv:1012.1711},
  year   = {2015}
}

Comments

Invited talk given at the YKIS2010 symposium, Kyoto, Japan, July 2010, to appear in the Progress of Theoretical Physics Supplement

R2 v1 2026-06-21T16:55:18.055Z