High Energy Theory Group Seminars
Primordial black holes as dark matter
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Europe/Rome
P4C Edificio Paolotti (Dipartimento di Fisica e Astronomia - Edificio Paolotti)
P4C Edificio Paolotti
Dipartimento di Fisica e Astronomia - Edificio Paolotti
Description
Asteroid-mass primordial black holes are a candidate for explaining the dark matter in our Universe. After introducing the basics of this scenario, I will present the conditions under which such black holes may have originated from a single-field model of inflation. I will then discuss the impact of non-gaussianities on their abundance and phenomenology.
Organised by
INFN & DFA Dr. Francesco D'Eramo
Contact