2021
DOI: 10.1016/j.nucengdes.2021.111474
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Summary of comparative analysis and conclusions from OECD/NEA LWR-UAM benchmark Phase I

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Cited by 9 publications
(5 citation statements)
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“…For the k eff , we see that the 235 U νp at low energies is the most significant input. This is in line with results from the LWR-UAM Phase I benchmark for steady state [40], since the νp has a direct contribution to the produced neutrons and thus to the k eff . The positive correlation is reasonable, since an increase of the νp will lead to an increase of the neutron population and then a higher k eff .…”
Section: Resultssupporting
confidence: 90%
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“…For the k eff , we see that the 235 U νp at low energies is the most significant input. This is in line with results from the LWR-UAM Phase I benchmark for steady state [40], since the νp has a direct contribution to the produced neutrons and thus to the k eff . The positive correlation is reasonable, since an increase of the νp will lead to an increase of the neutron population and then a higher k eff .…”
Section: Resultssupporting
confidence: 90%
“…The results for the scalar outputs of interest are shown in Figure 14. The k eff shows an uncertainty of 0.44%, which is a result in the same range of that found in the literature for typical LWR uncertainty quantification studies (0.5%) such as in [40]. Small uncertainties of 0.81% and 0.37% are obtained for P max lin and D min cool , respectively.…”
Section: Resultssupporting
confidence: 84%
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“…When considering the presented results, it is useful to keep in mind results usually obtained for the same quantities in LWR analysis. A k eff uncertainty between 0.5% for fresh fuel and 0.8% for depleted fuel, and a fuel Doppler coefficient uncertainty between 1.2% and 1.8% is usually obtained (Aures et al, 2017;Delipei et al, 2021). Key contributors to these uncertainties are 238 U and 239 Pu radiative capture, as well as 235 U and 239 Pu neutron multiplicity.…”
Section: Nuclear Data Uncertainty Propagationmentioning
confidence: 99%