Long-time 3D supernova simulations of non-rotating progenitors with magnetic fields

Bailey Sykes, Bernhard Müller

We perform five 3D magnetohydrodynamic (MHD) core-collapse supernova simulations for non-rotating progenitors between 9.5 $M_{\odot }$ and 24 $M_{\odot }$. Four of the five models produc…