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In order to explore various aspects of stellar evolution, supernovae, gammaray bursts and nucleosynthesis, we have developed a new efficient stellarevolution code. In this paper we describe this new code and compare the resultswith the ones calculated by the previous code. Specifically we focus on theprogenitor evolution of lower end of the Fe-core collapse supernovae, and massdistribution of remnant neutron stars. We describe how different assumptionswill lead different neutron star mass distribution. We also review recent worksof our research group.

Massive Star Evolution and Nucleosynthesis -Lower End of Fe-Core Collapse Supernova Progenitors and Remnant Neutron Star Mass Distribution-