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Stellar (n, gamma) cross sections of neutron-rich nuclei

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3362587· OSTI ID:21371071
 [1];  [2];  [1];  [3]
  1. GSI Helmholtzzentrum fuer Schwerionenforschung GmbH, Planckstr. 1, D-64291 Darmstadt (Germany)
  2. Physik-Department E12 and Excellence Cluster Universe, Technische Universitaet Muenchen, 85748 Garching (Germany)
  3. Forschungszentrum Karlsruhe, Institut fuer Kernphysik, 76344 Eggenstein-Leopoldshafen (Germany)
The present measurements were performed by means of the activation technique. Neutrons were produced at the Karlsruhe Van de Graaff accelerator via the {sup 7}Li(p,n){sup 7}Be reaction. For proton energies just above threshold, one obtains a neutron spectrum similar to a Maxwellian distribution for kT = 25 keV. This quasi-stellar neutron spectrum allowed us to measure the Maxwellian averaged cross sections directly. The experimental results of {sup 174,176}Yb, {sup 184,186}W, {sup 190,192}Os, {sup 196,198}Pt, and {sup 202}Hg were extrapolated from kT = 25 keV to lower and higher temperatures.
OSTI ID:
21371071
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1213; ISSN 0094-243X; ISSN APCPCS
Country of Publication:
United States
Language:
English

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