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Computational Challenges with Modeling Core Collapse Supernovae - IPAM at UCLA
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- 1 Introduction
- 2 Its a good time to be a supernova modeler
- 3 Overview
- 4 Guardian Angel
- 5 Delayed Shock Mechanism
- 6 neutrino driven convection
- 7 turbulence
- 8 sloshing
- 9 magnetic fields
- 10 general relativistic
- 11 neutrino heating
- 12 neutrino distribution function
- 13 Eddington factor
- 14 Realizability
- 15 Where we are
- 16 Weak interaction physics
- 17 First 3D model
- 18 Explosion energy vs time
- 19 gravitational wave signatures
