Recent Status of Core-collapse supernova Simulations from viewpoint of the microphysics

Detail of core-collapse supernova mechanism is controlled by nuclear physics: nuclear equation of state(EoS), interaction between neutrinos and nuclei and nucleosyntesis. Recently significant updates are reported in this area, e.g. new EoS is provided by Togashi et al. (2017) and neutrino scattering rate on nucleons is modified by Horowitz (2017). Employment of these new models will substantially change the dynamics of shocked matter in the supernovae. In my talk, I will demonstrate the results of my simulations with updated microphysics.