Neutron Capture Reactions on Fe and Ni Isotopes for the Astrophysical s-process

作者:Lederer C*; Giubrone G; Massimi C; Zugec P; Barbagallo M; Colonna N; Domingo Pardo C; Guerrero C; Gunsing F; Kaeppeler F; Tain J L; Altstadt S; Andrzejewski J; Audouin L; Becares V; Becvar F; Belloni F; Berthoumieux E; Billowes J; Boccone V; Bosnar D; Brugger M; Calviani M; Calvino F; Cano Ott D; Carrapico C; Cerutti F; Chiaveri E; Chin M; Cortes G; Cortes Giraldo M A; Diakaki M; Duran I; Dressler R; Dzysiuk N
来源:Nuclear Data Sheets, 2014, 120: 201-204.
DOI:10.1016/j.nds.2014.07.046

摘要

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.

  • 出版日期2014-6
  • 单位中国地震局