Towards the robustness of Affleck-Dine mechanism
| dc.creator | Kasuya, Shinta | |
| dc.date | 2006-10-31 | |
| dc.date.accessioned | 2026-07-07T11:02:03Z | |
| dc.date.available | 2026-07-07T11:02:03Z | |
| dc.description | 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. | |
| dc.description | 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 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0610428 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0610428 | |
| dc.identifier | J.Phys.A40:6999-7004,2007 | |
| dc.identifier | doi:10.1088/1751-8113/40/25/S52 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/188132 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Towards the robustness of Affleck-Dine mechanism | |
| dc.type | text |