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

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Scientific paper

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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