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The {sup 92}Zr(n,gamma) reaction and its implications for stellar nucleosynthesis

Journal Article · · Physical Review. C, Nuclear Physics
 [1]; ; ; ; ;  [2]; ; ; ; ; ; ; ;  [3]; ; ;  [4]; ; ;  [5]
  1. Istituto Nazionale di Fisica Nucleare (INFN), Bari (Italy)
  2. Istituto Nazionale di Fisica Nucleare (INFN), Trieste (Italy)
  3. CEA/Saclay-IRFU, Gif-sur-Yvette (France)
  4. Universidade de Santiago de Compostela, Santiago de Compostela, Galicia (Spain)
  5. Centro de Investigaciones Energeticas Medioambientales y Technologicas, Madrid (Spain)
Because the relatively small neutron capture cross sections of the zirconium isotopes are difficult to measure, the results of previous measurements are often not adequate for a number of problems in astrophysics and nuclear technology. Therefore, the {sup 92}Zr(n,gamma) cross section has been remeasured at the CERN n{sub T}OF facility, providing a set of improved parameters for 44 resonances in the neutron energy range up to 40 keV. With this information the cross-section uncertainties in the keV region could be reduced to 5% as required for s-process nucleosynthesis studies and technological applications.
OSTI ID:
21389071
Journal Information:
Physical Review. C, Nuclear Physics, Journal Name: Physical Review. C, Nuclear Physics Journal Issue: 5 Vol. 81; ISSN 0556-2813; ISSN PRVCAN
Country of Publication:
United States
Language:
English