The10B(p,α0)7Be reaction has been studied by applying the Trojan Horse method to the 2H(10B,α07Be)n reaction. The bare-nucleus astrophysical S(E)-factor in absolute units was extracted in a wide energy range, from 2.2 MeV to 3 keV and normalized to the direct experimental data, thus allowing determination of the electron screening potential for which a value of Ue=391±74 eV was obtained.

Improved information on astrophysical S-factor for the10B(p, α0)7Be reaction using the Trojan Horse method

Spartá, R.;Rapisarda, G. G.;Puglia, S. M. R.;La Cognata, M.;Cherubini, S.;Guardo, G. L.;Lamia, L.;Pizzone, R. G.;Romano, S.;Sergi, M. L.;
2018-01-01

Abstract

The10B(p,α0)7Be reaction has been studied by applying the Trojan Horse method to the 2H(10B,α07Be)n reaction. The bare-nucleus astrophysical S(E)-factor in absolute units was extracted in a wide energy range, from 2.2 MeV to 3 keV and normalized to the direct experimental data, thus allowing determination of the electron screening potential for which a value of Ue=391±74 eV was obtained.
2018
Physics and Astronomy (all)
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11769/357944
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