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A new Recoil Proton Telescope for energy and fluence measurement of fast neutron fields

机译:新型Recoil质子望远镜,用于快速中子场的能量和注量测量

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The spectrometer ATHENA (Accurate Telescope for High Energy Neutron metrology Applications), is being developed at the IRSN / LMDN (Institut de Radioprotection et de S??ret?? nucleaire / Laboratoire de Metrologie et de dosimetrie des neutrons) and aims at characterizing energy and fluence of fast neutron fields. The detector is a Recoil Proton Telescope and measures neutron fields in the range of 5 to 20MeV. Since the institute is designated by the LNE (Laboratoire National de metrologie et d'Essais) under the label LNE-IRSN as a reference for the neutron fluence, dose equivalents and kerma quantities in neutron metrology, his telescope is intended to become a primary standard for both energy and fluence measurements. The neutron detection is achieved by a polyethylene radiator for n-p conversion, three 50??m thick silicon sensors that use CMOS technology for the proton tracking and a 3 mm thick silicon diode to measure the residual proton energy. This first prototype used CMOS sensors called MIMOSTAR, initially developed for heavy ion physics. The use of CMOS sensors and silicon diode increases the intrinsic efficiency of the detector by a factor of ten compared with conventional designs. The first prototype has already been done and was a successful study giving the results it offered in terms of energy and fluence measurements. For mono energetic beams going from 5 to 19MeV, the telescope's energy resolution was between 5 and 11% and fluence determination was in agreement with other measurement standards. A second and final prototype of the detector is being designed. It will hold upgraded CMOS sensors called FastPixN. These CMOS sensors are supposed to run 400 times faster than the older version and therefore give the telescope the ability to support neutron flux in the range of 107 to 108cm???2.s???1. The first prototype's results showed that a 50??m pixel size is enough for a precise scattering angle reconstruction. Simulations using MCNPX and GEANT4 are a- ready in place for further improvements. A DeltaE diode will replace the third CMOS sensor and will be installed right before the silicon diode for a better recoil proton selection. The final prototype with its new geometry will increase the telescope's efficiency by a factor of 1.5. It will also cover some of the most important points in metrology; repeatability, reproducibility and sustainability.
机译:光谱仪ATHENA(用于高能中子计量学的精确望远镜)是在IRSN / LMDN(核辐射研究所/核子实验室/中子计量实验室和中子实验室)开发的,旨在表征能量和快速中子场的影响。该探测器是反冲质子望远镜,可测量5至20MeV范围内的中子场。由于该研究所是由LNE(Laboratoire National de Metrologie et d'Essais)指定为LNE-IRSN作为中子计量学中子注量,当量当量和比释动能数量的参考,因此他的望远镜旨在成为主要标准用于能量和注量测量。中子检测是通过一个用于n-p转换的聚乙烯辐射体,三个使用CMOS技术进行质子跟踪的50?m厚的硅传感器以及一个3mm的硅二极管来测量剩余质子能量来实现的。第一个原型使用称为MIMOSTAR的CMOS传感器,最初是为重离子物理学而开发的。与传统设计相比,CMOS传感器和硅二极管的使用将检测器的固有效率提高了十倍。第一个原型已经完成,并且是一项成功的研究,给出了它在能量和注量测量方面所提供的结果。对于从5MeV到19MeV的单能光束,望远镜的能量分辨率在5%到11%之间,并且注量确定与其他测量标准一致。正在设计探测器的第二个也是最后一个原型。它将容纳升级后的称为FastPixN的CMOS传感器。这些CMOS传感器的运行速度应比旧版本快400倍,因此使望远镜能够支持107至108cm?2.s?1范围内的中子通量。第一个原型的结果表明,50微米的像素大小足以实现精确的散射角重建。已经准备好使用MCNPX和GEANT4进行仿真,以进行进一步的改进。 DeltaE二极管将取代第三个CMOS传感器,并将安装在硅二极管之前,以便更好地选择反冲质子。具有新几何形状的最终原型将使望远镜的效率提高1.5倍。它还将涵盖计量学中的一些最重要的要点;可重复性,可重复性和可持续性。

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