Speaker
Dr
Quynh Lan Nguyen
(University of Notre Dame)
Description
In this talk, we will present a mechanism that provides self-interacting dark matter that can explain the small-scale structure problems such as the core cusp and too big to fail issues. We summarize simulations of self-interacting dark matter in models for galaxy formation and evolution. Then, constraints on the self-interacting dark matter with the cosmic microwave background and gravitational wave are summarized.
| Please select a main topic related to your abstract | Big Bang Cosmology and Primordial Nucleosynthesis |
|---|
Primary author
Dr
Quynh Lan Nguyen
(University of Notre Dame)
