Reaction rates of 21Ne(α, n)24Mg, 17O(α, n)20Ne and 18O(α, n)21Ne.

Details Reaction rates of 21Ne(α, n)24Mg, 17O(α, n)20Ne and 18O(α, n)21Ne. Reaction rates of 21Ne(α, n)24Mg, 17O(α, n)20Ne and 18O(α, n)21Ne.

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993nuas.symp..123d&link_type=abstract

"Nuclear Astrophysics, Proceedings of the 7th Workshop held 22-27 March 1993 at Ringberg Castle, Tegernsee,

Astronomy and Astrophysics

Astrophysics

Nuclear Reactions, Nucleosynthesis: Heavy Elements

Scientific paper

The nucleosynthesis of elements heavier than iron occurs mainly by neutron capture in the s- and r-process. In the course of an investigation program on all relevant (α, n)-reactions, the three possible neutron sources 21Ne(α, n)24Mg, 17O(α, n)20 Ne and 18O(α, n)21Ne have been investigated experimentally within the present limits of sensitivity (10-10barn). Cross sections, resonance parameters, S-factors and reaction rates have been deduced from these measurements.

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