The 10B(p,α)7Be reaction is the main responsible for the 10B destruction in stellar interior [1]. In such environments this p-capture process occurs at a Gamow energy of 10 keV and takes places mainly through a resonant state (Ex = 8.701 MeV) of the compound 11C nucleus. Thus a resonance right in the region of the Gamow peak is expected to significantly influence the behavior of the astrophysical S(E)-factor. The 10B(p,α)7Be reaction was studied via the Trojan Horse Method (THM) applied to the 2H(10B,α7Be)n in order to extract the astrophysical S(E)-factor in a wide energy range from 5 keV to 1.5 MeV.
Titolo: | The 10B(p, α)7Be S(E)-factor from 5 keV to 1.5 MeV using the Trojan Horse Method |
Autori interni: | |
Data di pubblicazione: | 2017 |
Rivista: | |
Handle: | http://hdl.handle.net/20.500.11769/357925 |
ISBN: | 9782759890309 |
Appare nelle tipologie: | 4.1 Contributo in Atti di convegno |
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epjconf_npa82017_01042.pdf | Versione Editoriale (PDF) | Open Access Visualizza/Apri |
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