Astrophysical S factors of radiative 3He4He, 3H4He, and 2H4He capture
S. B. DubovichenkoFesenkov Astrophysical Institute, National Academy of Sciences of the Republic of Kazakstan, Almaty, 480068, Republic of Kazakhstan
2010en
ABI
Abstract
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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