The Role of the N = 28 and N = 40 Closed Shells in the Production of the Neutron-Rich Ca-Ti-Cr-Fe-Ni Elements in the Universe
作者： O. Sorlin
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摘要: The nuclear structure of neutron-rich elements, as for instance their beta-decay times, may considerably influence the neutron-capture paths in explosive stellar events. Special care is given this contribution to links between and astrophysics synthesis stable Ca-Ti-Cr-Fe-Ni isotopes.
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