English

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 U(1)U(1). 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 U(1)U(1) 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.

Keywords

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

R2 v1 2026-07-22T14:25:42.065Z