This work is focused on a recent analysis of the 11B(p,α 0)8Be reaction by means of the Trojan Horse Method (THM) applied to the 2H(11B,α 08Be)n process. This approach allows one to extract the S(E) factor for the astrophysically relevant 11B(p,α 0)8Be reaction right in the region of the relevant Gamow peak (∼10 keV) where both electron screening and extrapolations could influence the available direct data. The experimental approach and the preliminary data of such investigation will be discussed.

Improved results on the extraction of 11B(p,α 0)8Be S(E)-factor via the Trojan Horse Method

Lamia L.;Romano S.;Cherubini S.;La Cognata M.;Pizzone R. G.;Puglia S. M. R.;Rapisarda G. G.;Sergi M. L.;
2009-01-01

Abstract

This work is focused on a recent analysis of the 11B(p,α 0)8Be reaction by means of the Trojan Horse Method (THM) applied to the 2H(11B,α 08Be)n process. This approach allows one to extract the S(E) factor for the astrophysically relevant 11B(p,α 0)8Be reaction right in the region of the relevant Gamow peak (∼10 keV) where both electron screening and extrapolations could influence the available direct data. The experimental approach and the preliminary data of such investigation will be discussed.
2009
Nuclear Physics: Cross section measurements
Nuclear Physics: Indirect methods
Stars: abundances
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11769/593881
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