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Neutron capture reactions on Fe and Ni isotopes for the astrophysical s-process

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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.
2014-12-15
ACADEMIC PRESS INC ELSEVIER SCIENCE
JRC85822
0090-3752,   
http://www.sciencedirect.com/science/article/pii/S0090375214004980,    http://dx.doi.org/10.1016/j.nds.2014.07.046,    https://publications.jrc.ec.europa.eu/repository/handle/JRC85822,   
10.1016/j.nds.2014.07.046,   
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