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 discussed
2014
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].
C. Lederer;G. Giubrone;C. Massimi;P. Zugec;M. Barbagallo;N. Colonna;C. Domingo-Pardo;C. Guerrero;F. Gunsing;F. Kaeppeler;J. L. Tain;S. Altstadt;J. And...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/412777
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