Curvaton Scenario with Affleck-Dine Baryogenesis
High Energy Physics - Phenomenology
2009-11-10 v1
Abstract
We discuss the curvaton scenario with the Affleck-Dine baryogenesis. In this scenario, non-vanishing baryonic entropy fluctuation may be generated even without primordial fluctuation of the Affleck-Dine field. Too large entropy fluctuation is inconsistent with the observations and hence constraints on the curvaton scenario with the Affleck-Dine baryogenesis are obtained. We calculate the baryonic entropy fluctuation (as well as other cosmological density fluctuations) in this case and derive constraints. Implications to some of the models of the curvaton are also discussed.
Cite
@article{arxiv.hep-ph/0404253,
title = {Curvaton Scenario with Affleck-Dine Baryogenesis},
author = {Maki Ikegami and Takeo Moroi},
journal= {arXiv preprint arXiv:hep-ph/0404253},
year = {2009}
}
Comments
16 pages,2 figures