1971
DOI: 10.1016/0375-9474(71)90936-5
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Spectra of high-energy photons following the capture of 14 MeV neutrons by 133Cs, 139La, Ce and 159Tb

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Cited by 25 publications
(4 citation statements)
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“…Capture Cross Section Figure 5 illustrates capture cross sections for 133{137 Cs in JENDL-4.0, which are compared with those of the measurements 7,28,32,33,41,[44][45][46][47][48][49][50][51] and of JENDL-3.3, ENDF/B-VII.0 and JEFF-3.1.1. Figure 6 focuses on the present result for 133 Cs in the keV region, whose evaluation was based on the average cross sections derived by Macklin. 44) The JENDL-4.0 data have slightly large cross sections relative to those of Yamamuro et al 46) and Bokhovko et al 47) in the incident energies below 80 keV, above which the influence of inelastic scattering becomes important.…”
Section: Evaluated Results and Discussionmentioning
confidence: 99%
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“…Capture Cross Section Figure 5 illustrates capture cross sections for 133{137 Cs in JENDL-4.0, which are compared with those of the measurements 7,28,32,33,41,[44][45][46][47][48][49][50][51] and of JENDL-3.3, ENDF/B-VII.0 and JEFF-3.1.1. Figure 6 focuses on the present result for 133 Cs in the keV region, whose evaluation was based on the average cross sections derived by Macklin. 44) The JENDL-4.0 data have slightly large cross sections relative to those of Yamamuro et al 46) and Bokhovko et al 47) in the incident energies below 80 keV, above which the influence of inelastic scattering becomes important.…”
Section: Evaluated Results and Discussionmentioning
confidence: 99%
“…Figure 6 focuses on the present result for 133 Cs in the keV region, whose evaluation was based on the average cross sections derived by Macklin. 44) The JENDL-4.0 data have slightly large cross sections relative to those of Yamamuro et al 46) and Bokhovko et al 47) in the incident energies below 80 keV, above which the influence of inelastic scattering becomes important. In the 14-15 MeV region, several measurements were carried out, and cross sections of about 1.5 mb were obtained by Rigaud et al 32) and Wagner and Warhanek.…”
Section: Evaluated Results and Discussionmentioning
confidence: 99%
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“…As described above, the contribution of such neutrons was calculated with the MCNP code, based on the neutron generator model. The validation of this model has been performed by the reaction 159 Tb(n,γ ) 160 Tb, because there is only one experimental value for the mentioned reaction [σ = (1.75 ± 0.45) mb] at a neutron energy around 14 MeV [37]. After correction of our measured cross section by a factor (1-FC), the value (1.8 ± 2.0) mb was obtained.…”
Section: Estimation Of the Error Sourcesmentioning
confidence: 99%