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

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

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..97...95b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 97, no. 1, Nov. 1983, p. 95-119.

Physics

20

Neutron Cross Sections, Nuclear Fusion, Solar Physics, Xenon Isotopes, Abundance, Carbonaceous Chondrites, Meteoritic Composition, Neutron Activation Analysis, Neutron Beams, Radioactive Decay

Scientific paper

The neutron capture cross-sections of 124,132,134Xe have been measured by the activation technique at 25 keV neutron energy. These data were supplemented by calculated capture cross-sections for 128,129,130,131Xe via the statistical model. The complete set of capture cross-sections obtained in this way served to determine the solar xenon abundance through s-process systematics and to study a variety of isotopic anomalies.

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