Abstract.
A correct understanding of r-process nucleosynthesis requires the knowledge of nuclear-structure properties far from β-stability and a detailed description of the possible astrophysical environments. With respect to nuclear data, in recent years the main focus at CERN/ISOLDE has been put on the 132Sn region to explore the role of the N = 82 shell closure and its consequences on the r-process matter flow through the A ≃ 130 Solar-System r-abundance peak.
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Kratz, K.L., Pfeiffer, B., Arndt, O. et al. r-process isotopes in the 132Sn region. Eur. Phys. J. A 25 (Suppl 1), 633–638 (2005). https://doi.org/10.1140/epjad/i2005-06-157-2
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DOI: https://doi.org/10.1140/epjad/i2005-06-157-2