Note the time!
Theory seminar: Very Early Universe and Non-Thermal Dark Matters
Bryan Zaldivar, Université Libre de Bruxelles
This talk is about mechanisms to generate the observed Dark Matter abundance, which has not been in thermal equilibrium with the radiation plasma in the early universe. They are complementary to the standard "WIMP" paradigm. Special focus on the inflationary reheating period is given. Finally, some thoughts about possible implications of primordial gravitational waves's measurements on Dark Matter are presented.
Published Mar. 28, 2014 10:25 AM
- Last modified Mar. 28, 2014 10:25 AM