Standard Model Baryogenesis
| dc.creator | Gavela, M. B. | |
| dc.creator | Hernández, P. | |
| dc.creator | Orloff, J. | |
| dc.creator | Pène, O. | |
| dc.date | 1994-07-29 | |
| dc.date | 1994-07-31 | |
| dc.date.accessioned | 2026-07-07T09:00:01Z | |
| dc.date.available | 2026-07-07T09:00:01Z | |
| dc.description | Simply on CP arguments, we argue against a Standard Model explanation of baryogenesis via the charge transport mechanism. A CP-asymmetry is found in the reflection coefficients of quarks hitting the electroweak phase boundary created during a first order phase transition. The problem is analyzed both in an academic zero temperature case and in the realistic finite temperature one. At finite temperature, a crucial role is played by the damping rate of quasi-quarks in a hot plasma, which induces loss of spatial coherence and suppresses reflection on the boundary even at tree-level. The resulting baryon asymmetry is many orders of magnitude below what observation requires. We comment as well on related works. | |
| dc.description | 10 pages, CERN-TH. 7368/94, LPTHE Orsay-94/71, HD-THEP-94-24 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9407403 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9407403 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/147921 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.title | Standard Model Baryogenesis | |
| dc.type | text |