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Core-collapse simulations of massive stars are performed using the equationof state (EOS) based on the microscopic variational calculation with realisticnuclear forces. The progenitor models with the initial masses of $15M_\odot$,$9.6M_\odot$, and $30M_\odot$ are adopted as examples of the ordinarycore-collapse supernova with a shock stall, the low-mass supernova with asuccessful explosion, and the black hole formation, respectively. Moreover, theneutrinos emitted from the stellar collapse are assessed. Then, the variationalEOS is confirmed to work well in all cases. The EOS dependences of thedynamics, thermal structure, and neutrino emission of the stellar collapse arealso investigated.

Numerical Study of Stellar Core Collapse and Neutrino Emission Using the Nuclear Equation of State Obtained by the Variational Method