Microscopic 130Ba(n, γ) Cross Section and the Origin of 131Xe on the Moon

Details Microscopic 130Ba(n, γ) Cross Section and the Origin of 131Xe on the Moon Microscopic 130Ba(n, γ) Cross Section and the Origin of 131Xe on the Moon

Jun 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973phrvc...7.2522b&link_type=abstract

Physical Review C, vol. 7, Issue 6, pp. 2522-2531

Physics

6

Scientific paper

The 130Ba(n, γ) cross section has been measured from 0.5 to 5000 eV with an energy resolution of 0.4%. The large epithermal resonances found in this experiment explain the anomalously high concentrations of 131Xe found in lunar rocks, and the measured resonance parameters provide one with a quantitative tool for correlating burial depth with exposure age for lunar samples.

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