Journal
PHYSICAL REVIEW C
Volume 68, Issue 6, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.68.065804
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The N-14((p) over right arrow,gamma)O-15 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 gamma 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 N-14((p) over right arrow,gamma)O-15 reaction is discussed.
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