Late-time Affleck-Dine baryogenesis after thermal inflation
| dc.creator | Kawasaki, Masahiro | |
| dc.creator | Nakayama, Kazunori | |
| dc.date | 2006-08-31 | |
| dc.date | 2006-12-13 | |
| dc.date.accessioned | 2026-07-07T10:25:21Z | |
| dc.date.available | 2026-07-07T10:25:21Z | |
| dc.description | Thermal inflation can solve serious cosmological problems such as overproduction of gravitinos and moduli. However, it also dilutes the preexisting baryon asymmetry. We investigate a possibility that Affleck-Dine mechanism works after thermal inflation and generate the baryon number at an acceptable level using lattice calculation. We find that a proper amount of baryon number can be generated for appropriate model parameters. | |
| dc.description | 6 pages, 5 figures, reference added | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0608335 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0608335 | |
| dc.identifier | Phys.Rev.D74:123508,2006 | |
| dc.identifier | doi:10.1103/PhysRevD.74.123508 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/176514 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Late-time Affleck-Dine baryogenesis after thermal inflation | |
| dc.type | text |