The experimental study of the 17O(n,α)14C reaction has been performed in the energy range 0-350 keV. This reaction could play an important role in explaining heavy elements (s-process) nucleosynthesis in various astrophysical scenario. To overcome the practical problems arising from the neutrons production, a new application of the Trojan Horse Method has been recently suggested. In more details, the 17O(n,α) 14C reaction has been studied using the quasi-free 2H( 17O,α14C)1H reaction, induced at an energy of 43.5 MeV. The measurement allows one to investigate the ℓ=3, 75 keV resonance (E*=8.125 MeV, Jπ=5-), absent in the available direct measurements because of centrifugal suppression effects. © 2014 AIP Publishing LLC.
CITATION STYLE
Guardo, G. L., Lamia, L., Spitaleri, C., Gulino, M., Tang, X. D., Bucher, B., … Wiescher, M. (2014). Study of the 17O (n,α) 14C reaction: Extension of the Trojan Horse Method to neutron induced reactions. In AIP Conference Proceedings (Vol. 1594, pp. 215–219). American Institute of Physics Inc. https://doi.org/10.1063/1.4874071
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