Title of article :
Bare astrophysical S(E)-factor for the 6Li(d, α)4He and 7Li(p, α)4He reactions at astrophysical energies
Original Research Article
Author/Authors :
Bare astrophysical S(E)-factor for the 6Li(d، نويسنده , , ?)4He and 7Li(p، نويسنده , , ?)4He reactions at astrophysical energies
Original Research Article
Pages 496-498
R.G. Pizzone، نويسنده , , C. Spitaleri، نويسنده , , M. Lattuada، نويسنده , , A. Musumarra، نويسنده , , M.G. Pellegriti، نويسنده , , S. Romano، نويسنده , , A. Tumino، نويسنده , , S. Cherubini، نويسنده , , P. Figuera، نويسنده , , D. Miljani?، نويسنده , , C. Rolfs، نويسنده , , S. Typel، نويسنده , , H.H. Wolter، نويسنده , , V. Castellani، نويسنده , , S. DeglʹInnocenti، نويسنده , , A. Imperio
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Abstract :
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.
