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.File in questo prodotto:
File | Dimensione | Formato | |
---|---|---|---|
epjconf_ena2018_02002-improved.pdf
accesso aperto
Tipologia:
Versione Editoriale (PDF)
Licenza:
Creative commons
Dimensione
258.59 kB
Formato
Adobe PDF
|
258.59 kB | Adobe PDF | Visualizza/Apri |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.