arXiv · 1005.4800
Astrophysical S-factor of 4He12C radiative capture at low energies
Abstract
The possibility to describe the astrophysical S-factor of the 4He12C radiative capture is considered in the potential cluster model at the energy range 0.1-4.0 MeV. It is shown that the approach used, which takes into account E2 transitions only, gives a good description of the new experimental data for adjusted parameters of potentials and leads to the value S(300) = 16.0$\cdotp$keV b.
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S. B. Dubovichenko, A. V. Dzhazairov-Kakhramanov. 2010-05-26. Astrophysical S-factor of 4He12C radiative capture at low energies. https://doi.org/10.1007/s11182-011-9557-8
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