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• W2093614352 abstract "A large fraction of the rare-earth elements observed in the solar system is produced in the astrophysical rapid neutron capture process (r-process). However, current stellar models cannot completely explain the relative abundance of these elements partially because of nuclear physics uncertainties. To address this problem, a β-decay spectroscopy experiment was performed at RI Beam Factory (RIBF) at RIKEN, aimed at studying a wide range of very neutron-rich nuclei with Z∼60 that are progenitors of the rare-earth elements with mass number A∼460. The experiment provides a test of nuclear models as well as experimental inputs for r-process calculations. This contribution presents the experimental setup and some preliminary results of the experiment." @default.
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• W2093614352 date "2014-01-01" @default.
• W2093614352 modified "2023-10-16" @default.
• W2093614352 title "β-decay of neutron-rich Z∼60 nuclei and the origin of rare earth elements" @default.
• W2093614352 doi "https://doi.org/10.1063/1.4874099" @default.
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