Th/Nd cosmochronology and a constant r/s ratio

Details Th/Nd cosmochronology and a constant r/s ratio Th/Nd cosmochronology and a constant r/s ratio

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.237...67m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 237, March 1, 1989, p. 67-79.

Statistics

Computation

13

Cosmology, Metallic Stars, Neodymium, Nuclear Fusion, Thorium, Chemical Evolution, Computational Astrophysics, Dwarf Stars

Scientific paper

The possibility of simulating a primary s-process which observations of stellar abundances would appear to imply is studied. It is found that a mechanism based only on the metallicity dependence of the neutron exposure does not produce the required s-process production. If the effect of N-14 production in stars with different initial metallicity is included, then it becomes possible to reproduce the observed primary nature of the s-process abundances.

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