Seminars IFIC

Baryogenesis with a low reheating temperature

por Dr. Sacha Davidson (Univ. of Oxford)

→ Europe/Madrid
Sala Seminarios IFIC (Edf. Institutos de Investigación)

Sala Seminarios IFIC

Edf. Institutos de Investigación

Descripción
The maximum temperature of the early Universe after inflation ends can be higher than the ``reheat temperature'' when the Universe becomes radiation dominated. If the reheat temperature is below the electroweak phase transition temperature, but T_{max} > T_{EPT}, electroweak B+L violation may be used to generate the observed baryon asymmetry.