An approach toward the successful supernova explosion by physics of   unstable nuclei
  We study the explosion mechanism of collapse-driven supernovae by numerical simulations with a new nuclear EOS based on unstable nuclei. We report new results of simulations of general relativistic hydrodynamics together with the Boltzmann neutrino-transport in spherical symmetry. We adopt the new data set of relativistic EOS and the conventional set of EOS (Lattimer-Swesty EOS) to examine the influence on dynamics of core-collapse, bounce and shock propagation. We follow the behavior of stalled shock more than 500 ms after the bounce and compare the evolutions of supernova core. 
K. Sumiyoshi (Numazu College of Technology), S. Yamada (Waseda Univ.),   H. Suzuki (Tokyo Univ. of Sci.), H. Shen (Nankai Un...