The experimental data on the astrophysical S-factor of the p 2H radiative capture are well described for energies from 1 keV to 10 MeV using the potential cluster model and the Young schemes of orbital cluster state classification with allowance for the E1 and M1 transitions.
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 2, pp. 28–34, February, 2011.
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Dubovichenko, S.B. Contribution of the M1 process to the astrophysical S-factor of the p 2H radiative capture. Russ Phys J 54, 157–164 (2011). https://doi.org/10.1007/s11182-011-9593-4
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DOI: https://doi.org/10.1007/s11182-011-9593-4