首页> 外文期刊>Nuclear Instruments & Methods in Physics Research >Measurements and Monte Carlo calculations of forward-angle secondary-neutron-production cross-sections for 137 and 200 MeV proton-induced reactions in carbon
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Measurements and Monte Carlo calculations of forward-angle secondary-neutron-production cross-sections for 137 and 200 MeV proton-induced reactions in carbon

机译:碳中137和200 MeV质子诱发反应的前角次级中子产生截面的测量和蒙特卡洛计算

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摘要

Secondary neutron-production double-differential cross-sections (DDXs) have been measured from interactions of 137 MeV and 200 MeV protons in a natural carbon target. The data were measured between 0° and 25° in the laboratory. DDXs were obtained with high energy resolution in the energy region from 3 MeV up to the maximum energy. The experimental data of 137 MeV protons at 10° and 25° were in good agreement with that of 113 MeV protons at 7.5° and 30° at LANSCE/WNR in the energy region below 80 MeV. Benchmark calculations were carried out with the PHITS code using the evaluated nuclear data files of JENDL/HE-2007 and ENDF/B-Ⅶ, and the theoretical models of Bertini-GEM and ISOBAR-GEM. For the 137 MeV proton incidence, calculations using JENDL/HE-2007 generally reproduced the shape and the intensity of experimental spectra well including the ground state of the ~(12)N state produced by the ~(12)C(p,n)~(12)N reaction. For the 200 MeV proton incidence, all calculated results underestimated the experimental data by the factor of two except for the calculated result using ISOBAR model. ISOBAR predicts the nucleon emission to the forward angles qualitatively better than the Bertini model. These experimental data will be useful to evaluate the carbon data and as benchmark data for investigating the validity of the Monte Carlo simulation for the shielding design of accelerator facilities.
机译:从天然碳靶中137 MeV和200 MeV质子的相互作用测量了次级中子产生双微分截面(DDX)。数据是在实验室的0°和25°之间测得的。在3 MeV到最大能量的能量范围内以高能量分辨率获得了DDX。在低于80 MeV的能量区域内,在LANSCE / WNR处,在10°和25°时137 MeV质子的实验数据与在7.5°和30°时113 MeV质子的实验数据非常吻合。使用已评估的JENDL / HE-2007和ENDF /B-Ⅶ核数据文件以及Bertini-GEM和ISOBAR-GEM的理论模型,通过PHITS代码进行基准计算。对于137 MeV质子入射,使用JENDL / HE-2007进行的计算通常重现了实验光谱的形状和强度,包括〜(12)C(p,n)产生的〜(12)N态的基态。 〜(12)N反应。对于200 MeV质子入射,除使用ISOBAR模型的计算结果外,所有计算结果都低估了两倍的实验数据。 ISOBAR比Bertini模型定性地更好地预测了朝前角的核子发射。这些实验数据将有助于评估碳数据,并作为基准数据来研究蒙特卡洛模拟对加速器设施的屏蔽设计的有效性。

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