The S-factor of the p 9Be → 10Bγ radiative capture is considered at astrophysical energies in the potential cluster model where orbital states are classified by the Young schemes.
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 7, pp. 80–86, July, 2011.
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Dubovichenko, S.B. Astrophysical S-factor of the p 9Be → 10Bγ radiative capture. Russ Phys J 54, 814–821 (2011). https://doi.org/10.1007/s11182-011-9688-y
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DOI: https://doi.org/10.1007/s11182-011-9688-y