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Proceedings Paper

Shell and neutron-skin effects in r-process isotopes
Author(s): B. Pfeiffer; K. L. Kratz; P. Moeller; J. Dobaczewski; F. K. Theilemann
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Paper Abstract

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.

Paper Details

Date Published: 3 March 1995
PDF: 5 pages
Proc. SPIE 2339, International Conference on Neutrons and Their Applications, (3 March 1995); doi: 10.1117/12.204185
Show Author Affiliations
B. Pfeiffer, Univ. Mainz (Germany)
K. L. Kratz, Univ. Mainz (Germany)
P. Moeller, Los Alamos National Lab. (United States)
J. Dobaczewski, Warsaw Univ. (Poland)
F. K. Theilemann, Univ. Basel (Switzerland)


Published in SPIE Proceedings Vol. 2339:
International Conference on Neutrons and Their Applications
George Vourvopoulos; Themis Paradellis, Editor(s)

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