Speaker
Dr
Giorgio Arcadi
(University of Rome 3)
Description
We ilustrate an accurate numerical Analysis of the scenario of real scalar dark matter with negligible coupling with the SM states. Assuming that the DM is produced during inflation and can reach at least kinetic Equilibrium due to its self-coupling, we illustrate a fully relativistic analysis of dark matter evolution, thermalization conditions and different freeze– out regimes, including the chemical potential effects.
Primary author
Dr
Giorgio Arcadi
(University of Rome 3)
Co-authors
Prof.
Oleg Lebedev
(University of Helsinki)
Prof.
Stefan Pokorski
(University of Warsow)
Dr
Toma Takashi
(McGill University)