Speaker:
Tanja Rindler-Daller
Institution:
Vienna University Observatory, U. Vienna
Date:
Thursday, March 27, 2025
Time:
11:00 am
Location:
ISEB 1310
Special Cosmology Center Seminar
Abstract: Galaxy and halo formation in the overall context of cosmological structure formation is a computationally challenging topic. However, the calculations of the "simpler" single-halo infall problem reveal already a lot of the inherent physics at play, when considering various dark matter candidates. In this talk, I will focus on a comparison between CDM and SFDM/FDM models, in terms of fundamental dynamical differences and similarities, and add a few comments on how to distinguish these observationally.
Host:
Kevork Abazajian