Freeman, S.; Oliva, A. A.; Tumino, A.; Soić, Neven; Prajapati, P. M.; Acosta, L.; Alba, R.; Barba, F.; Cherubini, S.; D’Agata, G.; Dell’Aquila, D.; Di Pietro, A.; Fernandez, J.P.; Figuera, P.; Galaviz Redondo, D.; Guardo, L.; Gulino, M.; Hammache, F.; Jelavic Malenica, D.; Kiliç, A.I.; La Cognata, M.; La Commara, M.; Lamia, L.; Lattuada, D.; Maiolino, C.; Manicò, G.; Mazzocco, M.; Milin, M.; Nanru, Ma (2023) Study of the 12C +16 O fusion reaction in carbon burning via the Trojan Horse Method. In: Nuclear Physics in Astrophysics – X (NPA-X 2022). Pariz, EDP Sciences, .
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Abstract
C-12 +C-12 is the main reaction during core and shell carbon burning in massive stars, however, at temperatures higher than K-109 when most of the carbon is depleted and its abundance is lower than O-16, the C-12 +O-16 fusion can also become relevant. Moreover, C-12 +O-16 reaction can ignite also in the scenario of explosive carbon burning. The astrophysical energy region of interest thus ranges from 3 to 7.2 MeV in the center-of-mass frame. There are various measurements of the cross-section available in the literature, however, they all stop around 4 MeV, making extrapolation necessary at lower energies. To try to solve this uncertainty and corroborate direct measurement the Trojan Horse Method was applied to three-body processes O-16(N-14, alpha Mg-24)H-2 and O-16(N-14, p(27)Al)H-2 to study the O-16(C-12, alpha)Mg-24 and O-16(C-12, p)Al-27 reactions.
| Item Type: | Conference or workshop item published in conference proceedings (UNSPECIFIED) |
|---|---|
| Uncontrolled Keywords: | nucleosynthesis |
| Subjects: | NATURAL SCIENCES > Physics NATURAL SCIENCES > Physics > Physics of Elementary Particles and Fields NATURAL SCIENCES > Physics > Nuclear Physics NATURAL SCIENCES > Physics > Astronomy and Astrophysics |
| Divisions: | Division of Experimental Physics |
| Depositing User: | Kristina Ciglar |
| Date Deposited: | 15 Jul 2026 13:16 |
| URI: | https://fulir.irb.hr:/id/eprint/12085 |
| DOI: | 10.1051/epjconf/202327911015 |
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