A study of the astrophysical S factor of the reactions 3H(α,γ)7Li and 3He(α,γ)7Be at zero energy.

Details A study of the astrophysical S factor of the reactions 3H(α,γ)7Li and 3He(α,γ)7Be at zero energy. A study of the astrophysical S factor of the reactions 3H(α,γ)7Li and 3He(α,γ)7Be at zero energy.

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989svjnp..50..827c&link_type=abstract

Sov. J. Nucl. Phys., Vol. 50, No. 5, p. 827 - 829

Astronomy and Astrophysics

Astrophysics

Nuclear Reactions

Scientific paper

An example is presented showing that the transition to astrophysical energies in the S factor for radiative-capture reactions can be performed conveniently when one separates beforehand the Coulomb cutoff component in the cross section. If one makes use of the continuous-spectrum wave function of two interacting clusters with zero energy of their relative motion, then the corresponding S factor can be calculated at E = 0. The S factor for the reactions 3H(α,γ)7Li and 3He(α,γ)7Be at E = 0 is calculated.

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