Neutron Capture Reactions on Fe and Ni Isotopes for the Astrophysical s-process

Abstract : Neutron capture cross sections in the keV neutron energy region are the key nuclear physics input to study the astrophysical slow neutron capture process. In the past years, a series of neutron capture cross section measurements has been performed at the neutron time-of-flight facility n_TOF at CERN focussing on the Fe/Ni mass region. Recent results and future developments in the neutron time-of-flight technique are discussed.
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Nuclear Data Sheets, Elsevier, 2014, 120, pp.201-204. 〈10.1016/j.nds.2014.07.046〉
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Contributeur : Sophie Heurteau <>
Soumis le : lundi 13 octobre 2014 - 10:58:24
Dernière modification le : mercredi 31 janvier 2018 - 12:16:00

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C. Lederer, L. Audouin, L.S. Leong, L. Tassan-Got, F. Gunsing, et al.. Neutron Capture Reactions on Fe and Ni Isotopes for the Astrophysical s-process. Nuclear Data Sheets, Elsevier, 2014, 120, pp.201-204. 〈10.1016/j.nds.2014.07.046〉. 〈in2p3-01074163〉

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