Spectroscopic study of low-lying N16 levels

Details Spectroscopic study of low-lying N16 levels Spectroscopic study of low-lying N16 levels

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008phrvc..78e2801b&link_type=abstract

Physical Review C, vol. 78, Issue 5, id. 052801

Physics

Spectroscopic Factors And Asymptotic Normalization Coefficients, Transfer Reactions, Nucleosynthesis In Late Stellar Evolution, 6<=A<=19

Scientific paper

The magnitude of the 15N(n,γ)16N reaction rate in asymptotic giant branch stars depends directly on the neutron spectroscopic factors of low-lying N16 levels. A new study of the 15N(d,p)16N reaction is reported populating the ground and first three excited states in N16. The measured spectroscopic factors are near unity as expected from shell model calculations, resolving a long-standing discrepancy with earlier measurements that had never been confirmed or understood. Updated 15N(n,γ)16N reaction rates are presented.

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