NEUTRINO-DRIVEN CONVECTION in CORE-COLLAPSE SUPERNOVAE: HIGH-RESOLUTION SIMULATIONS

Keyphrases

• Convection 100%
• High-resolution Simulation 100%
• Neutrinos 100%
• Core-collapse Supernovae 100%
• Accretion Flow 66%
• Shock 33%
• High-resolution 33%
• Dissociation 33%
• Non-radial 33%
• Shock Front 33%
• Turbulence 33%
• Grid Resolution 33%
• Energy Transport 33%
• Energy Accumulation 33%
• Internal Dynamics 33%
• Shock Evolution 33%
• Approximation Formula 33%
• Energy Flux 33%
• Net Positive Energy 33%
• Turbulent Convection 33%
• Kolmogorov Length Scale 33%
• Accretion Shock 33%
• Pressure Support 33%
• Energy-momentum 33%
• Effective Pressure 33%
• Numerical Artifacts 33%
• Heating-cooling 33%
• Downward Transport 33%
• Transfer Heat 33%
• Shallow Slope 33%
• Buoyant Plume 33%
• Turbulent Kinetic Energy Spectra 33%

Earth and Planetary Sciences

• Supernovae 100%
• Kinetic Energy 50%
• Energy Spectra 50%
• Energy Flux 50%
• Shock Front 50%

Physics

• High Resolution 100%
• Core-Collapse Supernovae 100%
• Kinetic Energy 33%
• Shock Front 33%
• Energy Spectra 33%