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Determining the 9Be (n, γ) 10Be integral cross section at fission neutron energies

机译:确定裂变中子能量处的 9Be (n, γ) 10Be 积分截面

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Background: The 9Be neutron capture cross section has significant implications for Be materials in the nuclear industry as well as the alpha process in stellar nucleosynthesis. While the cross section is well constrained at thermal neutron energies, there is a lack of experimental data at higher neutron energies, and the evaluated nuclear data libraries can differ by up to two orders of magnitude. Purpose: We calculate the 9Be (n, gamma )10Be integral cross section at fission neutron energies in an effort to resolve disagreements amongst the nuclear data libraries. Methods: Foil irradiation experiments were performed using the Flattop critical assembly at the National Criticality Experiments Research Center with either the highly enriched U or Pu cores, with target foil stacks placed at multiple locations to exploit different neutron energy profiles. Accelerator mass spectrometry was used to measure the 10Be / 9Be ratio in irradiated Be foils, while all other activation products were quantified through gamma spectrometry. The experiments were simulated using the Monte Carlo N -Particle radiation transport code and combined with experimental results to determine the total neutron fluence, while the STAYSL-PNNL suite and FISPACT-II code were used to validate the model and assess the systematic uncertainty. Results: The new 9Be (n, gamma )10Be integral cross sections calculated in this work are 26.5 +/- 2.2 mu b at 0.59 +/- 0.07 MeV, 24 +/- 3 mu b at 0.98 +/- 0.14 MeV, 21.7 +/- 1.3 mu b at 1.26 +/- 0.11 MeV, 21.8 +/- 1.4 mu b at 1.32 +/- 0.11 MeV, and 18.6 +/- 1.1 mu b at 1.46 +/- 0.13 MeV. These results do not agree with integral cross sections from any of the nuclear data library evaluations. Conclusions: Discrepancies between the new integral cross sections reported here and the nuclear data libraries suggest a more complex cross-section structure in the MeV range which allows for more resonance contributions, and more work is needed to further constrain the evaluated cross sections.
机译:背景:9Be 中子俘获截面对核工业中的 Be 材料以及恒星核合成中的 α 过程具有重要意义。虽然横截面在热中子能量下受到很好的限制,但在较高的中子能量下缺乏实验数据,并且评估的核数据库可能相差多达两个数量级。目的:我们计算裂变中子能量处的 9Be (n, gamma )10Be 积分截面,以解决核数据库之间的分歧。方法:使用国家临界实验研究中心的 Flattop 临界组件进行箔辐照实验,使用高度浓缩的 U 或 Pu 芯,将目标箔堆栈放置在多个位置以利用不同的中子能量分布。加速器质谱法用于测量辐照 Be 箔中的 10Be / 9Be 比率,而所有其他活化产物则通过伽马能谱法进行定量。使用蒙特卡洛 N 粒子辐射输运代码对实验进行模拟,并结合实验结果确定总中子通量,同时使用 STAYSL-PNNL 套件和 FISPACT-II 代码验证模型并评估系统不确定性。结果:本研究中计算的新 9Be (n, gamma )10Be 积分截面为 26.5 +/- 2.2 mu b(0.59 +/- 0.07 MeV),24 +/- 3 mu b(0.98 +/- 0.14 MeV,21)。7 +/- 1.3 μ b 在 1.26 +/- 0.11 MeV,21.8 +/- 1.4 μ b 在 1.32 +/- 0.11 MeV 和 18.6 +/- 1.1 μ b 在 1.46 +/- 0.13 MeV。这些结果与任何核数据库评估的积分横截面不一致。结论:这里报告的新积分截面与核数据库之间的差异表明,MeV 范围内的截面结构更复杂,这允许更多的共振贡献,并且需要更多的工作来进一步约束评估的截面。

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