Bare astrophysical S(E)-factor for the 6Li(d, α)4He and 7Li(p, α)4He reactions at astrophysical energies

Details Bare astrophysical S(E)-factor for the 6Li(d, α)4He and 7Li(p, α)4He reactions at astrophysical energies Bare astrophysical S(E)-factor for the 6Li(d, α)4He and 7Li(p, α)4He reactions at astrophysical energies

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003nupha.718..496p&link_type=abstract

Nuclear Physics A, Volume 718, p. 496-498.

Physics

Nuclear Physics

4

Scientific paper

The Trojan Horse Method has been applied to study the 7Li(p, α)4He and 6(Li(d, α)4He reactions through the 7Li(d, αα)n and 6Li(6Li, αα)4He three body processes, respectively. The electron screening potential deduced from these experiments is much larger than the adiabatic approximation prediction for both cases; the systematic discrepancy between data and theoretical predictions is thus confirmed. Astrophysical implications of these measurements are also discussed.

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