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

The possibility of describing the astrophysical S factors for radiative 3 He 4 He capture at energies of up to 15 keV and radiative 3 H 4 He and 2 H 4 He capture at energies of up 5 keV is considered on the basis of the potential cluster model involving forbidden states.

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