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Modeling beta-gamma coincidence spectra of Xe-131m, Xe-133, Xe-133m, and Xe-135

机译:对Xe-131m,Xe-133,Xe-133m和Xe-135的β-伽马重合谱建模

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摘要

In support of the Comprehensive Nuclear-Test-Ban Treaty (CTBT), improvements have been made to the model of the Automated Radioxenon Sampler/Analyzer (ARSA) beta-gamma coincidence detector for radioxenon monitoring. MCNPX is used to simulate the detector response for all the electrons and photons emitted from Xe-131m, Xe-133, Xe-133m, Xe-135, and Cs-137 signals. A MatLab code was written to incorporate the MCNPX results in the calculation of beta-gamma coincidence spectra. These will aid in the development of the Spectral Deconvolution Analysis Tool (SDAT)(1) and to calibrate beta-gamma coincidence systems. The models developed for this work include improvements over previous models in their ability to address Compton scattering in the beta-cell, and the beta-distribution offset in the 31 keV gamma-ray region for (133)xe.
机译:为了支持《全面禁止核试验条约》(CTBT),对用于放射性氙监测的自动放射性氙取样器/分析仪(ARSA)β-γ巧合探测器的模型进行了改进。 MCNPX用于模拟从Xe-131m,Xe-133,Xe-133m,Xe-135和Cs-137信号发射的所有电子和光子的探测器响应。编写了MatLab代码,将MCNPX结果合并到β-γ重合谱的计算中。这些将有助于频谱反卷积分析工具(SDAT)(1)的开发并校准β-γ符合系统。为这项工作开发的模型包括对先前模型的改进,使其能够解决β细胞中的康普顿散射,以及(133)xe在31 keV伽马射线区域中的β分布偏移。

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