On the astrophysical S-factor of 3He(αa, γ)7Be and 3H(αa, γ)7Li reactions at zero energy

Details On the astrophysical S-factor of 3He(αa, γ)7Be and 3H(αa, γ)7Li reactions at zero energy On the astrophysical S-factor of 3He(αa, γ)7Be and 3H(αa, γ)7Li reactions at zero energy

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phlb..229..316c&link_type=abstract

Physics Letters B, Volume 229, Issue 4, p. 316-320.

Physics

4

Scientific paper

The astrophysical S-factor of radiative capture reactions 3He(α, γ)7Be and H(α, γ)7Li has been calculated directly at zero energy. With this purpose in view, we make use of the zero energy continuum wave function of interacting clusters 3H (or 3He) and α, which takes into account both the Pauli principle correlations and the distortion effects due to the NN interaction in the internal region.

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