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Intrinsic spatial resolution of semiconductor X-ray detectors: a simulation study

机译:半导体X射线探测器的固有空间分辨率:模拟研究

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We have investigated the intrinsic limitation of the spatial resolution of a directly absorbing semiconductor detector. The primary interaction of an incident X-ray quantum is followed by a series of processes that generate Compton or fluorescence photons and subsequent electrons. Their ranges determine the spatial resolution of the detector, expressed in terms of the modulation transfer function. The effects of carrier transport have been neglected in this work. Monte Carlo simulations have been carried out in the 10-100 keV energy range with the program, ROSI (Roentgen Simulation), which is based on the well-established EGS4 algorithm. On a fine grid, the lateral distribution of deposited energy has been calculated in typical materials such as Se, CdTe, HgI_2 and PbI_2. The results can be used to either determine the point spread function of an energy-integrating detector, or to study multiple registration in adjacent pixels of photon-counting detectors. The results show that the complex absorption process determines the spatial resolution of the detector considerably. If a very high spatial resolution is required, a well-adapted semiconductor should be applied. Dependent on the energy range used, lists of favorable materials are given. At energies above 50keV, Compton scattering reduces spatial resolution in the high frequency range.
机译:我们研究了直接吸收半导体探测器的空间分辨率的内在限制。入射X射线量子的主要相互作用是一系列产生康普顿或荧光光子及后续电子的过程。它们的范围决定了检测器的空间分辨率,以调制传递函数表示。这项工作中忽略了承运人运输的影响。蒙特卡罗模拟已经在10-100 keV的能量范围内使用ROSI(伦琴模拟)程序进行了,该程序基于完善的EGS4算法。在精细的网格上,已在典型材料(例如Se,CdTe,HgI_2和PbI_2)中计算了沉积能量的横向分布。结果可用于确定能量积分探测器的点扩散函数,或用于研究光子计数探测器的相邻像素中的多重配准。结果表明,复杂的吸收过程在很大程度上决定了探测器的空间分辨率。如果需要很高的空间分辨率,则应使用适应性强的半导体。根据所使用的能量范围,列出了有利的材料。在能量超过50keV时,康普顿散射会降低高频范围内的空间分辨率。

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