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Monte Carlo simulation study for gamma energy deposition in scintillator coupled silicon photomultiplier detector

机译:闪烁器耦合硅光电倍增器中伽马能量沉积的蒙特卡罗仿真研究

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摘要

Silicon photomultipliers (SiPMs) are gaining popularity over conventional photomultiplier tubes (PMTs) in various radiation detection applications. For this application, it is necessary to optimize the scintillator material and its geometry. In order to develop a compact, low power gamma spectrometry system based on a scintillator coupled SiPM detector, energy deposition in Gd_3Ga_3Al_2O_(12)(Ce) (abbreviated as GGAG(Ce)), NaI(Tl) and CsI(Tl) scintillators of different dimensionswas calculated using Monte Carlo simulation code FLUKA for different gamma energies from 60 keV to 2614 keV. It is observed that energy deposition is highest in GGAG(Ce) followed byCsI(Tl) and NaI(Tl) respectively. By increasing thepath length of the scintillator, energy deposition is seen to increase for energies 662 keV, 1250 keV and 2614 keV. However, for 60 keV, the increase in longitudinal dimension above 3 mm does not affect the energy deposition. Based on the simulation data, GGAG(Ce) scintillator with 3×3×24 mm~3 geometry was chosen for making a scintillator coupledSiPM detector.
机译:在各种辐射检测应用中,硅光电倍增器(SIPMS)在传统的光电倍增管(PMTS)上越来越受欢迎。对于此应用,有必要优化闪烁体材料及其几何形状。为了开发基于闪烁体耦合SIPM检测器的紧凑型低功率伽马光谱系统,GD_3GA_3AL_2O_(12)(CE)中的能量沉积(缩写为GGAG(CE)),NAI(TL)和CSI(TL)闪烁器使用Monte Carlo仿真代码Fluka计算不同的伽马能量,从60 kev到2614 kev计算不同的维度。观察到,GGAG(CE)中的能量沉积分别在GGAG(CE)中是最高的,然后分别是CATCSI(TL)和NAI(TL)。通过增加闪烁体的路径长度,可以看到能量沉积以增加能量662keV,1250keV和2614kev。然而,对于60keV,纵向尺寸的增加在3mm以上不会影响能量沉积。基于模拟数据,选择GGAG(CE)闪烁器,选择具有3×3×24mm〜3几何形状的,用于制作闪烁体耦合的探测器。

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