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.
CitationLederer, C. [et al.]. Neutron capture reactions on Fe and Ni isotopes for the astrophysical s-process. "Nuclear data sheets", 01 Juny 2014, vol. 120, p. 201-202.