Baryogenesis in the wake of inflation
High Energy Physics - Phenomenology
2007-05-23 v1 Astrophysics
General Relativity and Quantum Cosmology
Abstract
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.
Cite
@article{arxiv.hep-ph/0112009,
title = {Baryogenesis in the wake of inflation},
author = {Alexander Kusenko},
journal= {arXiv preprint arXiv:hep-ph/0112009},
year = {2007}
}
Comments
7 pages, 3 figures, invited plenary talk at COSMO-01, Rovaniemi, Finland (August 29 - September 4, 2001)