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
C. Lederer, G. Giubrone, C. Massimi, P. Zugec, M. Barbagallo, N. Colonna, et al. (2014). Neutron Capture Reactions on Fe and Ni Isotopes for the Astrophysical s-process. NUCLEAR DATA SHEETS, 120, 201-204 [10.1016/j.nds.2014.07.046].
Neutron Capture Reactions on Fe and Ni Isotopes for the Astrophysical s-process
MASSIMI, CRISTIAN;MINGRONE, FEDERICA;VANNINI, GIANNI;
2014
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 discussedI documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
