Contribution of the M1 process to the astrophysical S-factor of the p2H radiative capture |
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Authors: | S. B. Dubovichenko |
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Affiliation: | 1.V. G. Fesenkov Astrophysical Institute of the National Center of Space Research and Technologies of the National Space Agency of Republic Kazakhstan,Almaty,Republic Kazakhstan;2.Nuclear Physics Institute of the National Nuclear Center of Republic Kazakhstan,Almaty,Republic Kazakhstan |
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Abstract: | 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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