Study of the 13N(d,n)14O reaction cross section and its astrophysical implications for the 13N proton capture reaction

Details Study of the 13N(d,n)14O reaction cross section and its astrophysical implications for the 13N proton capture reaction Study of the 13N(d,n)14O reaction cross section and its astrophysical implications for the 13N proton capture reaction

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phrvc..48.2057d&link_type=abstract

Physical Review C (Nuclear Physics), Volume 48, Issue 4, October 1993, pp.2057-2067

Physics

Nuclear Physics

17

Transfer Reactions, Radiative Capture, Elementary Particle Processes

Scientific paper

The total cross section for the 13N(d,n)14Og.s. reaction has been measured with 13N radioactive beams at laboratory energies of 8.2, 12.0, 16.2, and 28.5 MeV. A spectroscopic factor of 0.9 is obtained from a distorted-wave Born approximation analysis of this transfer reaction. The astrophysical S factor for the 13N(p,γ)14O reaction is calculated using the experimentally known resonance parameters for the resonant contribution and the direct-capture model with the experimental spectroscopic factor for the nonresonant contribution.

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