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 Elsevier Inc.
|Titolo:||Neutron Capture Reactions on Fe and Ni Isotopes for the Astrophysical s-process|
|Data di pubblicazione:||2014|
|Appare nelle tipologie:||1.1 Articolo in rivista|