The astrophysically relevant He-3(d,p)He-4 reaction was indirectly studied by means of the Trojan Horse Method applied to the Li-6(He-3, p alpha)He-4 three body process performed at 5 and 6 MeV. The bare astrophysical S(E)-factor extracted in Modified Plane Wave Born Approximation was compared with the free behaviour and an independent estimate of the screening potential was obtained, confirming the discrepancy with the adiabatic limit.
The astrophysically relevant He-3(d,p)He-4 reaction was indirectly studied by means of the Trojan Horse Method applied to the Li-6(He-3, p alpha)He-4 three body process performed at 5 and 6 MeV. The bare astrophysical S(E)-factor extracted in Modified Plane Wave Born Approximation was compared with the free behaviour and an independent estimate of the screening potential was obtained, confirming the discrepancy with the adiabatic limit.
Study of the He-3(d, p)He-4 reaction through the Trojan Horse Method
MUSUMARRA, Agatino;CHERUBINI, SILVIO;LAMIA, LIVIO;Pizzone RG;ROMANO, Stefano;TUDISCO, SALVATORE;
2005-01-01
Abstract
The astrophysically relevant He-3(d,p)He-4 reaction was indirectly studied by means of the Trojan Horse Method applied to the Li-6(He-3, p alpha)He-4 three body process performed at 5 and 6 MeV. The bare astrophysical S(E)-factor extracted in Modified Plane Wave Born Approximation was compared with the free behaviour and an independent estimate of the screening potential was obtained, confirming the discrepancy with the adiabatic limit.| File | Dimensione | Formato | |
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