Baryogenesis in the wake of inflation
| dc.creator | Kusenko, Alexander | |
| dc.date | 2001-12-02 | |
| dc.date.accessioned | 2026-07-07T03:46:01Z | |
| dc.date.available | 2026-07-07T03:46:01Z | |
| dc.description | Electroweak baryogenesis could be very efficient at the end of an electroweak-scale inflation. Reheating that followed inflation could create a highly non-equilibrium plasma, in which the baryon number violating transitions were rapid. In addition, the time-dependent motions of the scalar degrees of freedom could provide the requisite CP violation. If the final reheat temperature was below 100 GeV, there was no wash-out of the baryon asymmetry after thermalization. The observed value of the baryon asymmetry can be attained in a number of models, some of which do not require a significant departure from the Standard Model. | |
| dc.description | 7 pages, 3 figures, invited plenary talk at COSMO-01, Rovaniemi, Finland (August 29 - September 4, 2001) | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0112009 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0112009 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/41136 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Baryogenesis in the wake of inflation | |
| dc.type | text |