r-process isotopes in the 132Sn region

Details r-process isotopes in the 132Sn region r-process isotopes in the 132Sn region

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005epjas..25..633k&link_type=abstract

The European Physical Journal A, Volume 25, Supplement, Issue 1, pp.633-638

Astronomy and Astrophysics

Astrophysics

5

Scientific paper

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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