Chaotic Inflation based on an Abelian D-flat Direction
High Energy Physics - Phenomenology
2009-10-28 v1 Astrophysics
Abstract
We study the inflation due to the D-flat direction of an extra . This scenario is a hybrid of a right-handed sneutrino inflaton scenario and a gauge non-singlet inflaton scenario. The inflaton is a gauge non-singlet field which induces a right-handed neutrino mass spontaneously through an extra D-flat direction. This right-handed neutrino mass can explain the solar neutrino problem. The reheating temperature resulting from the decay of the coherent oscillation of the right-handed sneutrino is sufficiently high so that the baryogenesis based on the lepton number asymmetry can be applicable. We also discuss the realistic model building.
Cite
@article{arxiv.hep-ph/9504395,
title = {Chaotic Inflation based on an Abelian D-flat Direction},
author = {Daijiro Suematsu and Yoshio Yamagishi},
journal= {arXiv preprint arXiv:hep-ph/9504395},
year = {2009}
}
Comments
10 pages, LaTeX