Single and multi-event canonical r-process: astrophysics and nuclear physics considerations.

Details Single and multi-event canonical r-process: astrophysics and nuclear physics considerations. Single and multi-event canonical r-process: astrophysics and nuclear physics considerations.

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...305.1005b&link_type=abstract

Astronomy and Astrophysics, v.305, p.1005

Astronomy and Astrophysics

Astrophysics

22

Nucleosynthesis, Stars: Supernovae

Scientific paper

We study the influence of nuclear mass formulae as well as β-decay models on the r-abundance distribution resulting from canonical calculations of the nucleosynthesis r-process. This analysis is performed considering a single astrophysical event, or a more realistic superposition of events. We discuss conditions of validity of the waiting point approximation, propose an explanation of the smoothness of the r-elements abundance curve, and show that no unique fit to the observed r-abundance profile can be extracted.

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