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CHARACTERIZATION OF SPENT PWR FUEL FOR DECAY HEAT, NEUTRON AND GAMMA-RAY EMISSION: CODE COMPARISON

机译:用于衰减热,中子和伽马射线排放的废水PWR燃料的特征:代码比较

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Coupled neutron transport and fuel depletion codes were compared on a simplified ref-erence case of a PWR fuel assembly with initial 235U enrichment of 4% and burnup of51 GWd/tHM. Two Monte Carlo (MC) codes, Serpent and ALEPH2, and two determin-istic codes, SCALE and DRAGON, were considered. A part of the nuclide vector wascompared for a cooling period of 5 years. Additionally, observables, measurable by non-destructive analysis methods, i.e. decay heat, neutron and -ray emission rates, werecompared as a function of cooling time. The differences between the two MC codes aresmall, mostly within 1%. The differences in results obtained by deterministic codes arelarger, and for production of actinides heavier than plutonium they may reach 7%. Thedecay heat predictions with Serpent, ALEPH2 and DRAGON agree within 1% for cool-ing time period 1-1000 years, while the prediction with SCALE module Polaris deviatesby around 2% within that cooling time period.
机译:在简化的ref-比较耦合中子传输和燃料耗尽码PWR燃料组件的含义件初始235U富集4%和燃烧51 gwd / thm。两个蒙特卡罗(MC)代码,蛇和亚麻肤2,以及两个决定 - ISTIC代码,规模和龙,被考虑。核素载体的一部分是与5年的冷却期相比。另外,可观察到,可通过非 - 破坏性分析方法,即衰变热,中子和 - 射线排放率是与冷却时间的函数相比。两个MC代码之间的差异是小,主要在1%之内。通过确定性代码获得的结果的差异是较大,而且对于钚的曲线通常比钚的生产重达7%。这用蛇的衰变热预测,Aleph2和Dragon在1%内达到凉爽 - 时间期间1-1000岁,而尺度模块Polaris的预测偏离在该冷却时间段内约2%。

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