Determination of the 13N(p,γ)14O reaction cross section using a 13N radioactive ion beam

Details Determination of the 13N(p,γ)14O reaction cross section using a 13N radioactive ion beam Determination of the 13N(p,γ)14O reaction cross section using a 13N radioactive ion beam

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvl..67..808d&link_type=abstract

Physical Review Letters, Volume 67, Issue 7, August 12, 1991, pp.808-811

Astronomy and Astrophysics

Astrophysics

78

Radiative Capture, 6<=A<=19, Elementary Particle Processes

Scientific paper

The cross section for the astrophysically important 13N(p,γ)14O reaction has been measured directly with an intense (3×108 particles/s) and pure (>99%) 8.2-MeV 13N radioactive ion beam. The average value, for the 5.8-8.2-MeV 13N energy range, is 106(30) μb. The partial γ width of the resonance which occurs in this reaction at a center-of-mass energy of 0.545 MeV has been deduced to be 3.8(1.2) eV. It is compared with theoretical predictions and indirect determinations.

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