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- W2012294818 abstract "Abstract We discuss various neutrino-nucleus interactions in connection with the supernova r-process nucleosynthesis, which possibly occurs in the neutrino-driven wind of a young neutron star. These interactions include νe and ν e absorptions on free nucleons, νe captures on neutron-rich nuclei, and neutral-current νμ(τ) and ν μ(τ) interactions with α-particles and neutron-rich nuclei. We describe how these interactions can affect the r-process nucleosynthesis and discuss the implications of their effects for the physical conditions leading to a successful supernova r-process. We conclude that a low electron fraction and/or a short dynamic time scale may be required to give the sufficient neutron-to-seed ratio for an r-process in the neutrino-driven wind. In the case of a short dynamic time scale, the wind has to be contained during the r-process. Possible mechanisms which can give a low electron fraction or contain the wind are discussed." @default.
- W2012294818 created "2016-06-24" @default.
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- W2012294818 date "1997-08-01" @default.
- W2012294818 modified "2023-10-01" @default.
- W2012294818 title "Neutrino-nucleus interaction and supernova r-process nucleosynthesis" @default.
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- W2012294818 doi "https://doi.org/10.1016/s0375-9474(97)00272-8" @default.
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