Astrophysics and Space Science

, Volume 97, Issue 1, pp 95–119 | Cite as

Neutron capture cross-sections of stable xenon isotopes and their application in stellar nucleosynthesis

  • H. Beer
  • F. Käppeler
  • G. Reffo
  • G. Venturini


The neutron capture cross-sections of124, 132, 134Xe have been measured by the activation technique at 25 keV neutron energy. These data were supplemented by calculated capture cross-sections for128, 129, 130, 131Xe via the statistical model. The complete set of capture cross-sections obtained in this way served to determine the solar xenon abundance throughs-process systematics and to study a variety of isotopic anomalies.


Statistical Model Xenon Neutron Energy Neutron Capture Activation Technique 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© D. Reidel Publishing Company 1983

Authors and Affiliations

  • H. Beer
    • 1
  • F. Käppeler
    • 1
  • G. Reffo
    • 2
  • G. Venturini
    • 2
  1. 1.Institut für kernphysikKernforschungszentrum Karlsruhe GmbHKarlsruheDeutschland
  2. 2.Laboratorio Dati NucleariEnte Nazionale per l'Energie AlternativeBolognaItalia

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