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兆伏能量下闪烁晶体光输出的蒙特卡罗和朗伯光导模型。

Monte Carlo and Lambertian light guide models of the light output from scintillation crystals at megavoltage energies.

作者信息

Evans Philip M, Mosleh-Shirazi M Amin, Harris Emma J, Seco Joao

机构信息

Joint Physics Department, Institute of Cancer Research and Royal Marsden NHS Foundation Trust, Downs Road, Sutton, Surrey, SM2 5PT United Kingdom.

出版信息

Med Phys. 2006 Jun;33(6):1797-809. doi: 10.1118/1.2199597.

Abstract

A new model of the light output from single-crystal scintillators in megavoltage energy x-ray beams has been developed, based on the concept of a Lambertian light guide model (LLG). This was evaluated in comparison with a Monte Carlo (MC) model of optical photon transport, previously developed and reported in the literature, which was used as a gold standard. The LLG model was developed to enable optimization of scintillator detector design. In both models the dose deposition and light propagation were decoupled, the scintillators were cuboids, split into a series of cells as a function of depth, with Lambertian side and entrance faces, and a specular exit face. The signal in a sensor placed 1 and 1000 mm beyond the exit face was calculated. Cesium iodide (CSI) crystals of 1.5 and 3 mm square cross section and 1, 5, and 10 mm depth were modeled. Both models were also used to determine detector signal and optical gain factor as a function of CsI scintillator thickness, from 2 to 10 mm. Results showed a variation in light output with position of dose deposition of a factor of up to approximately 5, for long, thin scintillators (such as 10 X 1.5 x 1.5 mm3). For short, fat scintillators (such as 1 X 3 X 3 mm3) the light output was more uniform with depth. MC and LLG generally agreed to within 5%. Results for a sensor distance of 1 mm showed an increase in light output the closer the light originates to the exit face, while a distance of 1000 mm showed a decrease in light output the closer the light originates to the exit face. For a sensor distance of 1 mm, the ratio of signal for a 10 mm scintillator to that for a 2 mm scintillator was 1.98, whereas for the 1000 mm distance the ratio was 3.00. The ratio of quantum efficiency (QE) between 10 and 2 mm thicknesses was 4.62. We conclude that these models may be used for detector optimization, with the light guide model suitable for parametric study.

摘要

基于朗伯光导模型(LLG)的概念,开发了一种用于兆伏能量X射线束中单晶闪烁体光输出的新模型。将其与文献中先前开发并报道的光学光子传输蒙特卡罗(MC)模型进行比较评估,该MC模型用作金标准。开发LLG模型是为了实现闪烁体探测器设计的优化。在这两种模型中,剂量沉积和光传播是解耦的,闪烁体为长方体,根据深度分成一系列单元,侧面和入射面为朗伯面,出射面为镜面。计算了放置在出射面1毫米和1000毫米处的传感器中的信号。对横截面为1.5毫米×1.5毫米和3毫米×3毫米、深度为1毫米、5毫米和10毫米的碘化铯(CSI)晶体进行了建模。这两种模型还用于确定探测器信号和光学增益因子随CsI闪烁体厚度(从2毫米到10毫米)的变化。结果表明,对于长而薄的闪烁体(如10×1.5×1.5立方毫米),光输出随剂量沉积位置的变化高达约5倍。对于短而厚的闪烁体(如1×3×3立方毫米),光输出随深度更均匀。MC和LLG的结果一般在5%以内相符。传感器距离为1毫米时的结果表明,光越靠近出射面产生,光输出增加,而距离为1000毫米时,光越靠近出射面产生,光输出减少。对于传感器距离为1毫米,10毫米闪烁体与2毫米闪烁体的信号比为1.98,而对于距离为1000毫米时,该比值为3.00。10毫米和2毫米厚度之间的量子效率(QE)比为4.62。我们得出结论,这些模型可用于探测器优化,光导模型适用于参数研究。

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