Computational Challenges with Modeling Core Collapse Supernovae - IPAM at UCLA
Institute for Pure & Applied Mathematics (IPAM) via YouTube
Overview
Syllabus
Introduction
Its a good time to be a supernova modeler
Overview
Guardian Angel
Delayed Shock Mechanism
neutrino driven convection
turbulence
sloshing
magnetic fields
general relativistic
neutrino heating
neutrino distribution function
Eddington factor
Realizability
Where we are
Weak interaction physics
First 3D model
Explosion energy vs time
gravitational wave signatures
Taught by
Institute for Pure & Applied Mathematics (IPAM)