The B10(p,α0)Be7 excitation function has been studied in a wide energy range, from 2.2 MeV down to astrophysical energies, reproducing the cross section above and below the Coulomb barrier in a single experiment. An optimized experimental setup ensured good energy resolution and for the first time a clear separation of α0 and α1 channels of the B10+H2 interaction has been achieved by applying the Trojan Horse method. An improved normalization of the Trojan Horse bare-nucleus astrophysical S(E)-factor to direct data was performed and a value of Ue=391±74eV was obtained for the electron screening potential.
Trojan horse measurement of the B-10(p,alpha(0))Be-7 cross section in the energy range from 3 keV to 2.2 MeV
Spitaleri, C.;Spartá, R.;Rapisarda, G. G.;Puglia, S. M. R.;La Cognata, M.;Cherubini, S.;Guardo, G. L.;Gulino, M.;Lamia, L.;Pizzone, R. G.;Romano, S.;Sergi, M. L.;Tumino, A.
2018-01-01
Abstract
The B10(p,α0)Be7 excitation function has been studied in a wide energy range, from 2.2 MeV down to astrophysical energies, reproducing the cross section above and below the Coulomb barrier in a single experiment. An optimized experimental setup ensured good energy resolution and for the first time a clear separation of α0 and α1 channels of the B10+H2 interaction has been achieved by applying the Trojan Horse method. An improved normalization of the Trojan Horse bare-nucleus astrophysical S(E)-factor to direct data was performed and a value of Ue=391±74eV was obtained for the electron screening potential.File in questo prodotto:
File | Dimensione | Formato | |
---|---|---|---|
c99-aleks-b10-prc2018.pdf
solo gestori archivio
Tipologia:
Versione Editoriale (PDF)
Dimensione
4.15 MB
Formato
Adobe PDF
|
4.15 MB | Adobe PDF | Visualizza/Apri |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.