Abstract
We calculate the baryon asymmetry of the Universe which would arise during a first-order electroweak phase transition due to minimal-standard-model processes. It agrees in sign and magnitude with the observed baryonic excess, for reasonable Kobayashi-Maskawa parameters and mt in the expected range, and plausible values of bubble velocity and other high temperature effects.
Original language | English (US) |
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Pages (from-to) | 2833-2836 |
Number of pages | 4 |
Journal | Physical Review Letters |
Volume | 70 |
Issue number | 19 |
DOIs | |
State | Published - 1993 |
ASJC Scopus subject areas
- General Physics and Astronomy