Within the frame of the modified potential cluster model with classification of orbital states according to Young’s diagrams, the astrophysical S-factor of radiative p11C capture was calculated. The calculations considered all scattering resonances up to 3.5 MeV and were performed at energies up to 5 MeV. On the basis of the obtained total cross sections, the reaction rate was calculated at temperatures from 0.01 to 10.0 Т9, and its simple parameterization was proposed.
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 9, pp. 142–148, September, 2021.
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Dubovichenko, S.B., Burkova, N.A. & Shamitova, R.R. Radiative p11C Capture Reaction Rate. Russ Phys J 64, 1741–1748 (2022). https://doi.org/10.1007/s11182-022-02515-6
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DOI: https://doi.org/10.1007/s11182-022-02515-6