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Astrophysical S factors of radiative 3He4He, 3H4He, and 2H4He capture

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Abstract

The possibility of describing the astrophysical S factors for radiative 3He4He capture at energies of up to 15 keV and radiative 3H4He and 2H4He capture at energies of up 5 keV is considered on the basis of the potential cluster model involving forbidden states.

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Authors and Affiliations

  1. Fesenkov Astrophysical Institute, National Academy of Sciences of the Republic of Kazakstan, Almaty, 480068, 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, 2010, published in Yadernaya Fizika, 2010, Vol. 73, No. 9, pp. 1573–1584.

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Dubovichenko, S.B. Astrophysical S factors of radiative 3He4He, 3H4He, and 2H4He capture. Phys. Atom. Nuclei 73, 1526–1538 (2010). https://doi.org/10.1134/S1063778810090073

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