The Progenitor Dependence of Core-collapse Supernovae from Three-dimensional Simulations with Progenitor Models of 12-40 M_o

Keyphrases

• Neutrinos 100%
• Core-collapse Supernovae 100%
• Three Dimensional Simulation 100%
• Shock 83%
• Runaway 50%
• Three-dimensional (3D) 33%
• Density Profile 33%
• Accretion Rate 33%
• Accretion Shock 33%
• Shock Instability 33%
• Explosion Dynamics 33%
• Turbulence 16%
• Convection 16%
• Density Structure 16%
• Full Three-dimensional 16%
• Small Core 16%
• Main Sequence 16%
• Multigroup 16%
• Three-dimensional Flow 16%
• Black Hole Formation 16%
• Turbulent Convection 16%
• Small Densities 16%
• Non-monotonic Relationship 16%
• Density Discontinuity 16%
• Radiation Hydrodynamics 16%
• Remnant Mass 16%
• Intermediate Progenitors 16%
• Strong Discontinuities 16%
• Post-core 16%
• Neutrino Radiation 16%
• Massive Core 16%
• Explosion Time 16%

Physics

• Core-Collapse Supernovae 100%
• Three Dimensional Flow 50%
• Black Holes 50%
• Zero-Age Main Sequence Stars 50%