Abstract
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 in this contribution to the links between nuclear and astrophysics for the synthesis of the stable neutron-rich Ca-Ti-Cr-Fe-Ni isotopes.
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Sorlin, O. (2002). 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. In: Manuel, O. (eds) Origin of Elements in the Solar System. Springer, Boston, MA. https://doi.org/10.1007/0-306-46927-8_7
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DOI: https://doi.org/10.1007/0-306-46927-8_7
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