Towards the robustness of Affleck-Dine mechanism
Abstract
In this talk we considered the Affleck-Dine mechanism with various types of the Kahler potential, and investigate whether or not the Affleck-Dine field could acquire a large VEV as an initial condition for successful baryogenesis. In addition to a negative Hubble-induced mass term, we found examples that large enough Hubble-induced A-terms could also develop the minima at large amplitude of the field. It is concluded, therefore, that the Affleck-Dine mechanism works for broader classes of the theories. This talk is based on Ref.[1]. Here I extend the discussion from more generic standpoint, and find that essentially there are three cases that large enough A terms develop minima at large field values.
Keywords
Cite
@article{arxiv.hep-ph/0610428,
title = {Towards the robustness of Affleck-Dine mechanism},
author = {Shinta Kasuya},
journal= {arXiv preprint arXiv:hep-ph/0610428},
year = {2008}
}
Comments
6 pages, to appear in the proceedings of IRGAC 2006, 2nd International Conference on Quantum Theories and Renormalization Group in Gravity and Cosmology, Barcelona, July 11-15 2006