Astrophysics and Space Science

, Volume 97, Issue 1, pp 95–119

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

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

DOI: 10.1007/BF00684613

Cite this article as:
Beer, H., Käppeler, F., Reffo, G. et al. Astrophys Space Sci (1983) 97: 95. doi:10.1007/BF00684613

Abstract

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.

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