14N(3He,d)15O as a probe of direct capture in the 14N(p,γ)15O reaction

Details 14N(3He,d)15O as a probe of direct capture in the 14N(p,γ)15O reaction 14N(3He,d)15O as a probe of direct capture in the 14N(p,γ)15O reaction

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002phrvc..66e5804b&link_type=abstract

Physical Review C, vol. 66, Issue 5, id. 055804

Astronomy and Astrophysics

Astrophysics

20

Radiative Capture, Transfer Reactions, Hydrostatic Stellar Nucleosynthesis, Origin, Formation, And Abundances Of The Elements

Scientific paper

Spectroscopic factors and asymptotic normalization coefficients (ANCs) have been determined for bound states in 15O using the 14N(3He,d)15O reaction. These results are used to calculate the astrophysical S factor for direct capture in the 14N(p,γ)15O reaction. We also discuss how uncertainties in optical-model parameters influence both the spectroscopic factors and the ANCs, and the effect that this has on the predicted direct-capture reaction rate.

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