Supernova Simulations with Updated Microphysics

Abstract

Core-collapse supernovae is an important touchstone of nuclear physics. The detail of the explosion is affected by nuclear equation of state, interaction between neutrios and nuclei and nucleosyntesis. Recently modern models of core-collapse supernovae have been presented under different setups of input physics thanks to the the help of development of numerical techniques on radiation hydrodynamics and increased CPU resoureces. Careful comparison between these models and future observations would make our insight of nuclear physics deepen. In this paper, we demonstarete the results of my updated simulastions which employ all standard neutrino reactions and beyond.