Starts 5 Feb 2019 14:30
Ends 5 Feb 2019 16:00
Central European Time
ICTP
Leonardo Building - Luigi Stasi Seminar Room
Abstract. Models with strong dynamics at the TeV scale feature a confinement phase transition which is first order and generically slow, and a late inflationary period is a natural expectation. We study the modeling relevant for this problem, as long as the cosmological implications of this epoch.