Structure formation with warm clumpy dark matter

by Mehrdad Mirbabayi

Wednesday 16 Apr 2025, 14:30 → 15:30 Europe/Rome

aula 281 (Sesto Fiorentino)

Models of ultralight dark matter can lead to significant iso-curvature fluctuations, in the form of a white-noise at the time of formation, and a non-negligible velocity dispersion. These modify the gravitational growth of structures and can introduce distinct features in the observed matter distribution.