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Palmerini, S.; La Cognata, M.; Hammache, F.; Acosta, L.; Alba, R.; Burjan, V.; Chávez, E.; Cherubini, S.; Cvetinović, A.; D’Agata, G.; de Séréville, N.; Di Pietro, A.; Figuera, P.; Fülöp, Z.; Gaitán De Los Rios, K.; Guardo, G. L.; Gulino, M.; Hayakawa, S.; Kiss, G. G.; La Commara, M.; Lamia, L.; Maiolino, C.; Manicó, G.; Matei, C.; Mazzocco, M.; Mrazek, J.; Parascandolo, T.; Petruse, T.; Pierroutsakou, D.; Pizzone, R. G.; Rapisarda, G. G.; Romano, S.; Santonocito, D.; Sergi, M. L.; Spartà, R.; Tumino, A.; Yamaguchi, H.
European physical journal plus, 1/9, Letnik: 136, Številka: 9Journal Article
The 27 Al ( p , α ) 24 Mg reaction, which drives the destruction of 27 Al and the production of 24 Mg in stellar hydrogen burning, has been investigated via the Trojan Horse Method (THM), by measuring the 2 H ( 27 Al , α 24 Mg ) n three-body reaction. The experiment covered a broad energy range ( E c . m . ≤ 1.5 MeV ), aiming to investigate those of interest for astrophysics. The results confirm the THM as a valuable technique for the experimental study of fusion reactions at very low energies and suggest the presence of a rich pattern of resonances in the energy region close to the Gamow window of stellar hydrogen burning (70–120 keV), with potential impact on astrophysics. To estimate such an impact a second run of the experiment is needed, since the background due the three-body reaction hampered to collect enough data to resolve the resonant structures and extract the reaction rate.
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Leto | Faktor vpliva | Izdaja | Kategorija | Razvrstitev | ||||
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JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
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Vir: Osebne bibliografije
in: SICRIS
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