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We study the few body reactions in explosive nucleosynthesis oflight-to-heavy mass elements in various astrophysical conditions. Inneutrino-driven winds of gravitational core collapse of SNeII, several lightnuclei as well as heavy unstable nuclei paly significant roles in producingr-process elements. We discuss how the three-body reaction $^4$He$(\alpha n,\gamma)^9$Be, whose cross section is poorly known, plays very critical role. Wemake note that several other reactions in the r-process are relevant to aBig-Bang nucleosynthesis. We discuss briefly a Galactic chemical evolution.

Impact of Few-Body Reactions on Explosive Nucleosynthesis: The Big-Bang and Supernovae