Long-term evolutions and physical processes of massiv-star collapse

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Performing long-term simulations of post-bounce supernova evolutions in the context of neutrino-heating mechanism, we have revealed how the explosion energy depends on nuclear reactions. We have developed a new 3D Boltzmann solver. We have also computed neutrino and gravity wave emissions from black hole formations quantitatively. New insights into the jet formations have been obtained. Moreover, we have studied basic properties in the dynamics of quark star formations.