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Nuclear Astrophysics and Neutron Induced Reactions: Quasi-Free Reactions and RIBs

Abstract : The use of quasi-free reactions in studying nuclear reactions between charged particles of astrophysical interest has received much attention over the last two decades. The Trojan Horse Method is based on this approach and it has been used to study a number of reactions relevant for Nuclear Astrophysics. Recently we applied this method to the study of nuclear reactions that involve radioactive species, namely to the study of the 18F+p-->15O+α process at temperatures corresponding to the energies available in the classical novae scenario. Quasi-free reactions can also be exploited to study processes induced by neutrons. This technique is particularly interesting when applied to reaction induced by neutrons on unstable short-lived nuclei. Such processes are very important in the nucleosynthesis of elements in the sand r-processes scenarios and this technique can give hints for solving key questions in nuclear astrophysics where direct measurements are practically impossible.
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Contributor : Christine Hadrossek <>
Submitted on : Friday, February 17, 2012 - 11:16:41 AM
Last modification on : Wednesday, September 16, 2020 - 4:17:40 PM

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S. Cherubini, A. Coc, S. Kubono, C. Spitaleri, D. N. Binh, et al.. Nuclear Astrophysics and Neutron Induced Reactions: Quasi-Free Reactions and RIBs. THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010, Mar 2010, pp.98-103, ⟨10.1063/1.3485215⟩. ⟨in2p3-00671329⟩

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