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Indirect study of the 16O+16O fusion reaction toward stellar energies by the Trojan Horse Method

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dc.contributor.author Hayakawa, S.
dc.contributor.author Spitaleri, C.
dc.contributor.author Burtebayev, N.
dc.contributor.author Aimaganbetov, A.
dc.contributor.author Figuera, P.
dc.contributor.author Fisichella, M.
dc.contributor.author Guardo, G.L.
dc.contributor.author Igamov, S.
dc.contributor.author Indelicato, I.
dc.contributor.author Kiss, G.
dc.contributor.author Kliczewski, S.
dc.contributor.author La Cognata, M.
dc.contributor.author Lamia, L.
dc.contributor.author Lattuada, M.
dc.contributor.author Piasecki, E.
dc.contributor.author Rapisarda, G.G.
dc.contributor.author Romano, S.
dc.contributor.author Sakuta, S.B.
dc.contributor.author Siudak, R.
dc.contributor.author Trzcinska, A.
dc.contributor.author Tumino, A.
dc.contributor.author Urkinbayev, A.
dc.date.accessioned 2024-04-02T07:03:32Z
dc.date.available 2024-04-02T07:03:32Z
dc.date.issued 2016
dc.identifier.issn 2100-014X
dc.identifier.other DOI: 10.1051/ conf/201611 09013
dc.identifier.uri http://rep.enu.kz/handle/enu/13245
dc.description.abstract The 16O+16O fusion reaction is important in terms of the explosive oxygen burning process during late evolution stage of massive stars as well as understanding of the mechanism of low-energy heavy-ion fusion reactions. We aim to determine the excitation function for the most major exit channels, α+28Si and p+31P, toward stellar energies indirectly by the Trojan Horse Method via the 16O(20Ne, α28Si)α and 16O(20Ne, p31P)α three-body reactions. We report preliminary results involving reaction identification, and determination of the momentum distribution of α16O intercluster motion in the projectile 20Ne nucleus. ru
dc.language.iso en ru
dc.publisher EPJ Web of Conferences ru
dc.relation.ispartofseries 117;09013
dc.title Indirect study of the 16O+16O fusion reaction toward stellar energies by the Trojan Horse Method ru
dc.type Article ru


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