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Astrophysical S-factor for the radiative-capture reaction p 13C → 14Nγ

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Abstract

The possibility of describing experimental data on the astrophysical S factor for radiative proton capture on a 13C nucleus at energies in the range 0.03–0.8 MeV is considered within the potential cluster model involving forbidden states. It is shown that the energy dependence of this astrophysical S factor can be reasonably explained on the basis of the E1 transition to the 3 P 1-wave bound state of the 14N nucleus in the p 13C channel from the 3 S 1 wave of p 13C scattering in the resonance energy region around 0.55 MeV in the laboratory frame.

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Authors and Affiliations

  1. V.G. Fessenkov Astrophysical Institute, Almaty, 050022, Republic of Kazakhstan

    S. B. Dubovichenko

  2. Institute of Nuclear Physics, National Nuclear Center of Republic of Kazakhstan, ul. Ibragimova 1, Almaty, 050032, Republic of Kazakhstan

    S. B. Dubovichenko

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  1. S. B. Dubovichenko
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Correspondence to S. B. Dubovichenko.

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Original Russian Text © S.B. Dubovichenko, 2012, published in Yadernaya Fizika, 2012, Vol. 75, No. 2, pp. 196–203.

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Dubovichenko, S.B. Astrophysical S-factor for the radiative-capture reaction p 13C → 14Nγ . Phys. Atom. Nuclei 75, 173–181 (2012). https://doi.org/10.1134/S1063778812020044

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