Physics
Scientific paper
Jan 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aipc..124..511m&link_type=abstract
AIP Conference Proceedings, Volume 124, pp. 511-514 (1985).
Physics
1
Elementary Particle Processes, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages
Scientific paper
We summarize the stellar parameters which characterize the s-process σN curve in the framework of models which produce an exponential distribution of exposures by periodic time-dependent neutron irradiations. The optimum parameter space, defined by the best fit to the solar-system σN curve, is distinctively different than the classical smooth monotonically decreasing curve. Constraints are placed on the s-process environment. The needs for better neutron-capture data in various mass regions are highlighted.
Howard Michael W.
Mathews Grant J.
Takahashi Keitaro
Ward Richard A.
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