BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Non-equilibrium in the early Universe via the Wilson Renormalizati
 on Group
DTSTART;VALUE=DATE-TIME:19980520T100000Z
DTEND;VALUE=DATE-TIME:19980520T110000Z
DTSTAMP;VALUE=DATE-TIME:20260618T034227Z
UID:indico-event-1075@indico.ific.uv.es
DESCRIPTION:Many interesting aspects of the Early Universe involve physics
  out of thermal equilibrium\, which cannot be studied reliably in the fram
 ework of thermal perturbation theory. After reviewing the shortcomings of 
 the perturbative approach\, we describe the use of the Wilson Renormalizat
 ion Group at finite temperature and its application in the cosmological co
 ntext. In particular we will discuss thermal masses\, damping rates\, phas
 e transitions\, and the anomalous baryon number violation above the electr
 oweak phase transition.\n\nhttps://indico.ific.uv.es/event/1075/
LOCATION:Dpto. de Fisica Teorica (UVEG) Sala Seminarios
URL:https://indico.ific.uv.es/event/1075/
END:VEVENT
END:VCALENDAR