https://doi.org/10.1051/epjconf/201611709013
Indirect Study of the 16O+16O Fusion Reaction Toward Stellar Energies by the Trojan Horse Method
1 Center for Nuclear Study, University of Tokyo, Wako, Japan
2 INFN - Laboratori Nazionali del Sud, Catania, Italy
3 Department of Physics and Astronomy, University of Catania, Catania, Italy
4 Institute of Nuclear Physics of National Nuclear Center, Almaty Kazakhstan
5 Gumilyov Eurasian National University, Astana, Kazakhstan
6 Uzbek. Acad. Sci., Inst. Nucl. Phys., Tashkent, Uzbekistan
7 MTA-Atomiki, Debrecen, Hungary
8 The H. Niewodniczański Institute of Nuclear Physics PAN, Kraków, Poland
9 Heavy Ion Laboratory, University of Warsaw, Warsaw, Poland
10 National Research Center “Kurchatov Institute”, Moscow, Russia
11 Kore University of Enna, Enna, Italy
Published online: 11 May 2016
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 α-16O intercluster motion in the projectile 20Ne nucleus.
© Owned by the authors, published by EDP Sciences - SIF, 2016
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.