Abstract
Hydrodynamic calculations of stellar collapse in Type II Supernova are described using a variable nuclear adiabatic index and compressibility for the nuclear equation of state at high density. Initial models employing a relatively small mass core with low central entropy are necessary to achieve viable shocks; near success the models are sensitive to both neutrino emission and the high density equation of state. The treatment of neutrino production and transport is sketched and recent results reported.
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