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The neutron capture cross sections and the capture γ-ray spectra of 138Ba were measured in the astrophysically important energy region. Measurements were made at neutron energies from 15 to 80 keV. The neutron energy was determined by the time-of-flight method. The γ-ray spectra showed that the primary transition pattern strongly depended on the incident neutron energy. The neutron capture cross sections were derived by the pulse height weighting technique. The present cross section values were compared with evaluated cross section data and previous measurements

Neutron capture cross section and capture gamma-ray spectra of138Ba in the keV-neutron energy region

Neutron capture cross section and capture gamma-ray spectra of¹³⁸Ba in the keV-neutron energy region