Analyzing power measurement for the 14 N ( p→ ,γ) 15 O reaction at astrophysically relevant energies

Details Analyzing power measurement for the 14 N ( p→ ,γ) 15 O reaction at astrophysically relevant energies Analyzing power measurement for the 14 N ( p→ ,γ) 15 O reaction at astrophysically relevant energies

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003phrvc..68f5804n&link_type=abstract

Physical Review C, vol. 68, Issue 6, id. 065804

Astronomy and Astrophysics

Astrophysics

14

Hydrostatic Stellar Nucleosynthesis

Scientific paper

The 14 N ( p→ ,γ ) 15 O reaction has been investigated by measuring the angular distributions of its cross section and analyzing power using a 270-keV polarized proton beam. Calculations using a direct-capture-plus-resonance model were compared with the data. The results indicate the presence of γ transition amplitudes which were not considered in previous extrapolations of the astrophysical S factor to low energies. The impact on the zero-energy S factor of the 14 N ( p→ ,γ ) 15 O reaction is discussed.

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