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.
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Beer, H., Käppeler, F., Reffo, G. et al. Neutron capture cross-sections of stable xenon isotopes and their application in stellar nucleosynthesis. Astrophys Space Sci 97, 95–119 (1983). https://doi.org/10.1007/BF00684613
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DOI: https://doi.org/10.1007/BF00684613