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Propagation of Nuclear Data Uncertainties for ELECTRA Burn-up Calculations

机译:用于ELECTRA燃耗计算的核数据不确定性的传播

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The European Lead-Cooled Training Reactor (ELECTRA) has been proposed as a training reactor for fast systems within the Swedish nuclear program. It is a low-power fast reactor cooled by pure liquid lead. In this work, we propagate the uncertainties in ~(239)Pu transport data to uncertainties in the fuel inventory of ELECTRA during the reactor lifetime using the Total Monte Carlo approach (TMC). Within the TENDL project, nuclear models input parameters were randomized within their uncertainties and 740 ~(239)Pu nuclear data libraries were generated. These libraries are used as inputs to reactor codes, in our case SERPENT, to perform uncertainty analysis of nuclear reactor inventory during burn-up. The uncertainty in the inventory determines uncertainties in: the long-term radio-toxicity, the decay heat, the evolution of reactivity parameters, gas pressure and volatile fission product content. In this work, a methodology called fast TMC is utilized, which reduces the overall calculation time. The uncertainty of some minor actinides were observed to be rather large and therefore their impact on multiple recycling should be investigated further. It was also found that, criticality benchmarks can be used to reduce inventory uncertainties due to nuclear data. Further studies are needed to include fission yield uncertainties, more isotopes, and a larger set of benchmarks.
机译:欧洲铅冷训练堆(ELECTRA)已被提议作为瑞典核计划中快速系统的训练堆。这是一种由纯液体铅冷却的低功率快堆。在这项工作中,我们使用总蒙特卡洛方法(TMC)将〜(239)Pu输运数据中的不确定性传播到反应堆寿命期间ELECTRA的燃料库存中的不确定性。在TENDL项目中,核模型输入参数在其不确定性内随机化,并生成740〜(239)Pu核数据库。这些库用作反应堆代码(在我们的情况下为SERPENT)的输入,以在燃尽期间执行核反应堆库存的不确定性分析。库存中的不确定性决定了以下方面的不确定性:长期放射性毒性,衰变热,反应性参数的演变,气压和挥发性裂变产物含量。在这项工作中,使用了一种称为快速TMC的方法,该方法减少了总体计算时间。观察到一些次act系元素的不确定性相当大,因此应进一步研究它们对多次循环的影响。还发现,关键性基准可用于减少由于核数据引起的库存不确定性。需要进一步研究,以包括裂变产率的不确定性,更多的同位素和更大的基准集。

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  • 来源
    《Nuclear Data Sheets》 |2014年第4期|527-530|共4页
  • 作者单位

    Division of Applied Nuclear Physics, Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden;

    Division of Applied Nuclear Physics, Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden;

    Division of Applied Nuclear Physics, Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden;

    Division of Applied Nuclear Physics, Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden;

    Division of Applied Nuclear Physics, Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden,Nuclear Research and Consultancy Group (NRG), Petten, The Netherlands;

    Division of Applied Nuclear Physics, Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden;

    Nuclear Research and Consultancy Group (NRG), Petten, The Netherlands;

    Division of Applied Nuclear Physics, Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden;

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