Ponente
Laura Lopez-Honorez
(ULB)
Descripción
In my talk I will briefly introduce dark matter scenarios beyond the vanilla WIMP (and cold) dark matter models. I will then move to feebly interacting to non-interacting dark matter scenarios which can be challenging to probe. Yet they may leave specific imprint in cosmology observables. I will in particular focus on Non-Cold dark matter signatures that can be expected when the dark matter production mechanism give rise to non-negligible velocity dispersion at the time of structure formation.
Autor primario
Laura Lopez-Honorez
(ULB)
