Study of 3 He(n,p) 3 H reaction at cosmological energies with trojan horse method
In the network of reactions present in the Big Bang nucleosynthesis, the 3 He(n, p) 3 H has an important role which impacts the final 7 Li abundance. The Trojan Horse Method (THM) has been applied to the 3 He(d, pt)H reaction in order to extract the astrophysical S(E)-factor of the 3 He(n, p ) 3 H i...
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| creator | Spampinato, C. Pizzone, R.G. Spartà, R. Couder, M. Tan, W. Burian, V. Chae, K.Y. D’Agata, G. Guardo, G.L. Indelicato, I. Cognata, M. La Lamia, L. Lattuada, D. Mrazek, J. Oliva, A. Palmerini, S. Prajapati, P.M. Rapisarda, G.G. Romano, S. Sergi, M.L. Spitaleri, C. Tumino, A. Wiescher, M. Anguilar, S. Bardyan, D. Blankstein, D. Boccioli, L. Callahan, L. Clark, A. Frentz, B. Hall, M. Gula, A. Henderson, S. Kelmar, R. Liu, Q. Long, J. Majumdar, A. McGuinness, S. Nelson, A. O’Malley, P. Seyymour, C. Skulski, M. Wilkinson, J. |
| description | In the network of reactions present in the Big Bang nucleosynthesis, the
3
He(n, p)
3
H
has an important role which impacts the final
7
Li
abundance. The Trojan Horse Method (THM) has been applied to the
3
He(d, pt)H
reaction in order to extract the astrophysical S(E)-factor of the
3
He(n,
p
)
3
H
in the Gamow energy range. The experiment will be described in the present work together with the first preliminary results. |
| doi_str_mv | 10.1051/epjconf/202022702013 |
| format | Article |
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3
He(n, p)
3
H
has an important role which impacts the final
7
Li
abundance. The Trojan Horse Method (THM) has been applied to the
3
He(d, pt)H
reaction in order to extract the astrophysical S(E)-factor of the
3
He(n,
p
)
3
H
in the Gamow energy range. The experiment will be described in the present work together with the first preliminary results.</description><identifier>ISSN: 2100-014X</identifier><identifier>EISSN: 2100-014X</identifier><identifier>DOI: 10.1051/epjconf/202022702013</identifier><language>eng</language><ispartof>EPJ Web of conferences, 2020, Vol.227, p.2013</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c963-f828b09b22509020c0ab2022254d9ca2197721bb3ad1519174cea6d794bb39023</citedby><cites>FETCH-LOGICAL-c963-f828b09b22509020c0ab2022254d9ca2197721bb3ad1519174cea6d794bb39023</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,864,4022,27921,27922,27923</link.rule.ids></links><search><contributor>Lamia, L.</contributor><contributor>Pizzone, R.G.</contributor><contributor>Romano, S.</contributor><contributor>La Cognata, M.</contributor><contributor>Spitaleri, C.</contributor><creatorcontrib>Spampinato, C.</creatorcontrib><creatorcontrib>Pizzone, R.G.</creatorcontrib><creatorcontrib>Spartà, R.</creatorcontrib><creatorcontrib>Couder, M.</creatorcontrib><creatorcontrib>Tan, W.</creatorcontrib><creatorcontrib>Burian, V.</creatorcontrib><creatorcontrib>Chae, K.Y.</creatorcontrib><creatorcontrib>D’Agata, G.</creatorcontrib><creatorcontrib>Guardo, G.L.</creatorcontrib><creatorcontrib>Indelicato, I.</creatorcontrib><creatorcontrib>Cognata, M. La</creatorcontrib><creatorcontrib>Lamia, L.</creatorcontrib><creatorcontrib>Lattuada, D.</creatorcontrib><creatorcontrib>Mrazek, J.</creatorcontrib><creatorcontrib>Oliva, A.</creatorcontrib><creatorcontrib>Palmerini, S.</creatorcontrib><creatorcontrib>Prajapati, P.M.</creatorcontrib><creatorcontrib>Rapisarda, G.G.</creatorcontrib><creatorcontrib>Romano, S.</creatorcontrib><creatorcontrib>Sergi, M.L.</creatorcontrib><creatorcontrib>Spitaleri, C.</creatorcontrib><creatorcontrib>Tumino, A.</creatorcontrib><creatorcontrib>Wiescher, M.</creatorcontrib><creatorcontrib>Anguilar, S.</creatorcontrib><creatorcontrib>Bardyan, D.</creatorcontrib><creatorcontrib>Blankstein, D.</creatorcontrib><creatorcontrib>Boccioli, L.</creatorcontrib><creatorcontrib>Callahan, L.</creatorcontrib><creatorcontrib>Clark, A.</creatorcontrib><creatorcontrib>Frentz, B.</creatorcontrib><creatorcontrib>Hall, M.</creatorcontrib><creatorcontrib>Gula, A.</creatorcontrib><creatorcontrib>Henderson, S.</creatorcontrib><creatorcontrib>Kelmar, R.</creatorcontrib><creatorcontrib>Liu, Q.</creatorcontrib><creatorcontrib>Long, J.</creatorcontrib><creatorcontrib>Majumdar, A.</creatorcontrib><creatorcontrib>McGuinness, S.</creatorcontrib><creatorcontrib>Nelson, A.</creatorcontrib><creatorcontrib>O’Malley, P.</creatorcontrib><creatorcontrib>Seyymour, C.</creatorcontrib><creatorcontrib>Skulski, M.</creatorcontrib><creatorcontrib>Wilkinson, J.</creatorcontrib><title>Study of 3 He(n,p) 3 H reaction at cosmological energies with trojan horse method</title><title>EPJ Web of conferences</title><description>In the network of reactions present in the Big Bang nucleosynthesis, the
3
He(n, p)
3
H
has an important role which impacts the final
7
Li
abundance. The Trojan Horse Method (THM) has been applied to the
3
He(d, pt)H
reaction in order to extract the astrophysical S(E)-factor of the
3
He(n,
p
)
3
H
in the Gamow energy range. 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3
He(n, p)
3
H
has an important role which impacts the final
7
Li
abundance. The Trojan Horse Method (THM) has been applied to the
3
He(d, pt)H
reaction in order to extract the astrophysical S(E)-factor of the
3
He(n,
p
)
3
H
in the Gamow energy range. The experiment will be described in the present work together with the first preliminary results.</abstract><doi>10.1051/epjconf/202022702013</doi></addata></record> |
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| title | Study of 3 He(n,p) 3 H reaction at cosmological energies with trojan horse method |
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