Shell and neutron-skin effects in r-process isotopes

Details Shell and neutron-skin effects in r-process isotopes Shell and neutron-skin effects in r-process isotopes

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995spie.2339...72p&link_type=abstract

Proc. SPIE Vol. 2339, p. 72-76, International Conference on Neutrons and Their Applications, George Vourvopoulos; Themis Paradel

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From calculations of the r-process abundance pattern, constraints on stellar as well as nuclear parameters are deduced. Deviations between calculated and observed abundances are interpreted as hints to deficiencies in existing nuclear models. New structure effects related to the extreme neutron-excesses of the nuclei in the r-process path are discussed.

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