YoVDO

A Kinetic-Hydrodynamic Coupling Method for Self-Interacting Dark Matter (SIDM)

Offered By: Fields Institute via YouTube

Tags

Computational Astrophysics Courses Cosmology Courses Fluid Dynamics Courses Numerical Methods Courses Particle Physics Courses Hydrodynamics Courses Boltzmann Equation Courses Kinetic Theory Courses

Course Description

Overview

Save Big on Coursera Plus. 7,000+ courses at $160 off. Limited Time Only!
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.

Syllabus

A kinetic-hydrodynamic coupling method for SIDM


Taught by

Fields Institute

Related Courses

Multi-Dimensional Modeling of Core-Collapse Supernovae - IPAM at UCLA
Institute for Pure & Applied Mathematics (IPAM) via YouTube Introduction to Numerical Relativistic Hydrodynamics - Lecture 2
International Centre for Theoretical Sciences via YouTube Introduction to Numerical Relativistic Hydrodynamics - Lecture 5
International Centre for Theoretical Sciences via YouTube Open Source Software as Activism
Linux Foundation via YouTube Emulating InterStellar Medium Chemistry with Physics Informed Neural Networks
Alan Turing Institute via YouTube