Neutrino oscillations in oxygen-neon-magnesium supernovae Cecilia Lunardini Arizona State University And RIKEN-BNL Research Center C.L., B. Mueller and.
Computational grid size ~0.5 m Process ~5 mm REV Maco-Micro Modeling— Simple methods for incorporating small scale effects into large scale solidification.
Neutrino oscillations in oxygen-neon-magnesium supernovae
