The 30 keV averaged neutron capture cross sections of 56Fe and 60Ni
High resolution neutron capture measurements of 56Fe and 60Ni were performed, with total energy detectors in the energy range 1-200 keV. The data have been used to derive the Maxwellian-averaged cross sections for thermal energies around kT=30 keV, corresponding to the mean temperature of the s-process of stellar nucleo-synthesis.
Bibliographic Reference: Paper presented: 7th International Symposium on Capture Gamma-Ray Spectroscopy and Related Topics, Asilomar, Pacific Grove (US), Oct. 14-19, 1990
Availability: Available from (1) as Paper EN 35788 ORA
Record Number: 199011623 / Last updated on: 1994-12-02
Original language: en
Available languages: en