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A telescope detection system for direct and high resolution spectrometry of intense neutron fields

机译:用于中子场直接和高分辨率光谱测定的望远镜检测系统

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摘要

A high energy- and spatial-resolution telescope detector was designed and constructed for neutronudspectrometry of intense neutron fields. The detector is constituted by a plastic scintillator coupled to audmonolithic silicon telescope (MST), in turn consisting of a DE and an E stage. The scintillator behaves asudan “active” recoil-proton converter, since it measures the deposited energy of the recoil-protonsudgenerated across. The MST measures the residual energy of recoil-protons downstream of the converterudand also discriminates recoil-protons from photons associated to the neutron field. The lay-out ofudthe scintillator/MST system was optimized through an analytical model for selecting the angular range ofudthe scattered protons. The use of unfolding techniques for reconstructing the neutron energy distributionudwas thus avoided with reasonable uncertainty (about 1.6% in neutron energy) and efficiency (of the orderudof 106 counts per unit neutron fluence). A semi-empirical procedure was also developed for correctingudthe non-linearity in light emission from the organic scintillator. The spectrometer was characterized withudquasi-monoenergetic and continuous fields of neutrons generated at the CN Van De Graaff accelerator ofudthe INFN-Legnaro National Laboratory, Italy, showing satisfactory agreement with literature data.
机译:设计并制造了一种高能量和空间分辨率的望远镜探测器,用于强中子场的中子/超谱测量。该检测器由一个塑料闪烁体构成,该闪烁体耦合到一个单片硅望远镜(MST),又由DE和E级组成。闪烁体的作用就像是“主动”后座质子转换器,因为它可以测量产生的后座质子的沉积能量。 MST测量转换器下游的反冲质子的剩余能量,并从与中子场关联的光子中区分出反冲质子。通过选择散射质子角范围的分析模型优化了闪烁体/ MST系统的布局。因此避免了使用展开技术来重建中子能量分布 ud,并且具有合理的不确定性(中子能量约1.6%)和效率(每单位中子注量106 udud数量级)。还开发了一种半经验程序来校正/消除有机闪烁体发出的光的非线性。该光谱仪的特征是在意大利INFN-Legnaro国家实验室的CN Van De Graaff加速器上产生的中子具有准单能和连续场,与文献数据显示出令人满意的一致性。

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