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Abstract

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.

Additional information

Authors: CORVI F, JRC Geel (BE);FIONI G, JRC Geel (BE);BABELIOWSKY T, JRC Geel (BE);MAURI A, ENEA, Centro Ricerche Energia Frascati, Roma (IT)
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
Category: PUBLICATION
Original language: en
Available languages: en