pith. sign in

arxiv: 1210.3421 · v2 · pith:2MDVGHZ5new · submitted 2012-10-12 · 🌌 astro-ph.CO · hep-ph· hep-th

Passive Curvaton

classification 🌌 astro-ph.CO hep-phhep-th
keywords curvatonpassivefieldmodelsnon-gaussianitycouplesgaugemodel
0
0 comments X
read the original abstract

We propose a class of curvaton models which we call passive curvaton. In this paper, two kinds of passive curvaton is considered. The first one is a pseudoscalar curvaton couples to a gauge field. Different from the inflaton case, the constraint from formation of primordial black holes (PBHs) is much weaker and large non-gaussianity (of the equiliteral type) can be produced. The second model is a dilaton-like scalar curvaton couples to a gauge field. We investigate the scale dependence of non-gaussianity in this model. In both models, the spectrum and non-Gaussianity are enhanced by the slow-roll parameter of the curvaton field. Other possible passive curvaton models are also mentioned.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.