The 30keV Averaged Neutron Capture Cross Sections of 56Fe and 60Ni

Details The 30keV Averaged Neutron Capture Cross Sections of 56Fe and 60Ni The 30keV Averaged Neutron Capture Cross Sections of 56Fe and 60Ni

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..238..906c&link_type=abstract

Capture gamma-ray spectroscopy. AIP Conference Proceedings, Volume 238, pp. 906-908 (1991).

Physics

Radiative Capture, 39<=A<=58, 59<=A<=89, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

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 nucleosynthesis.

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