FIMPs and their signatures

by Geneviève Bélanger (LAPTh, Annecy)

Friday, 23 November 2018 from to (Europe/Amsterdam)
at Nikhef ( H331 )
Dark matter that is extremely weakly coupled to the standard model can 
be directly produced in the early universe  via the freeze-in mechanism.
After describing this  mechanism, I will present some specific models 
where freeze-in can be realised and discuss the implications for dark 
matter searches in astrophysics and at the LHC.