Non-Equilibrium Thermal Dark Matter

23 May 2013, 18:00
25m
Small Lecture Hall Mathematics (Bonn)

Small Lecture Hall Mathematics

Bonn

Speaker

Bryan Zaldivar

Description

Dark Matter (DM) may have been produced out of thermal equilibrium in the early universe. This possibility has been investigated before through the so-called "Freeze-in" scenario of Feebly-Interacting-Massive-Particles. In this talk I show that this is just a particular case of a general out-of-equilibrium-generated DM, by describing new alternatives which are totally different at a fundamental level. As an example, Grand Unification Theories can naturally lead to such mechanisms, where a DM with unsuppressed couplings can populate the universe to the relic density values we observe today, while never reaching equilibrium with the thermal bath.

Presentation materials