Neutrinos, Weak Interactions, and r-process Nucleosynthesis

Physics – Nuclear Physics – Nuclear Theory

Scientific paper

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To be published in the Proceedings of "International Symposium on Structure of Exotic Nuclei and Nuclear Forces (SENUF 06)", M

Scientific paper

Two of the key issues in understanding the neutron-to-proton ratio in a
core-collapse supernova are discussed. One of these is the behavior of the
neutrino-nucleon cross sections as supernova energies. The other issue is the
many-body properties of the neutrino gas near the core when both one- and
two-body interaction terms are included.

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