Explore a cutting-edge kinetic-hydrodynamic coupling method for Self-Interacting Dark Matter (SIDM) in this 26-minute conference talk by Sarah Schon from The Pennsylvania State University. Delve into the latest advancements in dark matter research and gain insights into innovative computational techniques used to model SIDM behavior. Learn how this coupling method enhances our understanding of dark matter dynamics and its implications for cosmological simulations. Discover the potential impact of this research on our comprehension of galaxy formation and evolution in the context of SIDM models.
A Kinetic-Hydrodynamic Coupling Method for Self-Interacting Dark Matter (SIDM)
Overview
Syllabus
A kinetic-hydrodynamic coupling method for SIDM
Taught by
Fields Institute
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