3 March 1995 Shell and neutron-skin effects in r-process isotopes
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Proceedings Volume 2339, International Conference on Neutrons and Their Applications; (1995) https://doi.org/10.1117/12.204185
Event: 4th International Conference on Applications of Nuclear Techniques: Neutrons and their Applications, 1994, Crete, Greece
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.
© (1995) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
B. Pfeiffer, B. Pfeiffer, K. L. Kratz, K. L. Kratz, P. Moeller, P. Moeller, J. Dobaczewski, J. Dobaczewski, F. K. Theilemann, F. K. Theilemann, } "Shell and neutron-skin effects in r-process isotopes", Proc. SPIE 2339, International Conference on Neutrons and Their Applications, (3 March 1995); doi: 10.1117/12.204185; https://doi.org/10.1117/12.204185
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