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Two of the key issues in understanding the neutron-to-proton ratio in acore-collapse supernova are discussed. One of these is the behavior of theneutrino-nucleon cross sections as supernova energies. The other issue is themany-body properties of the neutrino gas near the core when both one- andtwo-body interaction terms are included.Comment: To be published in the Proceedings of "International Symposium on  Structure of Exotic Nuclei and Nuclear Forces (SENUF 06)", March 2006, Tokyo,  Japa

Neutrinos, Weak Interactions, and r-process Nucleosynthesis