Abstract
An IAEA project to update the Neutron Standards is near completion. Traditionally, the Thermal Neutron Constants (TNC) evaluated data by Axton for thermal-neutron scattering, capture and fission on four fissile nuclei and the total nu-bar of 252 Cf(sf) are used as input in the combined least-square fit with neutron cross section standards. The evaluation by Axton (1986) was based on a least-square fit of both thermal-spectrum averaged cross sections (Maxwellian data) and microscopic cross sections at 2200 m/s. There is a second Axton evaluation based exclusively on measured microscopic cross sections at 2200 m/s (excluding Maxwellian data). Both evaluations disagree within quoted uncertainties for fission and capture cross sections and total multiplicities of uranium isotopes. There are two factors, which may lead to such difference: Westcott g-factors with estimated 0.2% uncertainties used in the Axton's fit, and deviation of the thermal spectra from Maxwellian shape. To exclude or mitigate the impact of these factors, a new combined GMA fit of standards was undertaken with Axton's TNC evaluation based on 2200 m/s data used as a prior. New microscopic data at the thermal point, available since 1986, were added to the combined fit. Additionally, an independent evaluation of TNC was undertaken using CONRAD code. Both GMA and CONRAD results are consistent within quoted uncertainties. New evaluation shows a small increase of fission and capture thermal cross sections, and a corresponding decrease in evaluated thermal nubar for uranium isotopes and 239 Pu.
Highlights
New evaluation shows a small increase of fission and capture thermal cross sections, and a corresponding decrease in evaluated thermal nubar for uranium isotopes and 239Pu
An IAEA project [1] to update the 2006 Neutron Standards [2] is close to conclusion
The marginalization was implemented in the CONRAD code to avoid problems when highly correlated data are introduced in the fitting procedure
Summary
An IAEA project [1] to update the 2006 Neutron Standards [2] is close to conclusion. This project constitutes an important contribution to the CIELO collaboration [3]. In a comprehensive paper published in 1984 Divadeenam and Stehn used both Maxwellian and 2200 m/s data to derive a new set of TNC constants [8] They assumed Maxwellian prompt fission neutron spectra (PFNS) in their analysis of reactor spectra This discrepancy was observed and discussed by Lemmel [5]
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