不同传感器参数对单晶PET探测器空间分辨率性能的影响。

Xiaoli Li, Cate Lockhart, Tom K Lewellen, Robert S Miyaoka
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引用次数: 1

摘要

报道了采用新型入口表面传感器设计的单片晶体PET探测器的性能特点。为了方便这种设计,我们建议使用二维硅光电倍增管(SiPM)阵列器件。sipm是盖革-穆勒模式雪崩光电二极管(GMAPD)的一种形式,可以提供类似于光电倍增管(PMT)的信号增益。由于这些设备仍在积极开发中,其性能参数也在不断变化。采用多步仿真方法,研究了不同SiPM参数对单片晶体PET探测器性能的影响。这些参数包括不同信道间的增益可变性;获得不稳定;和黑暗计数噪音。模拟的探测器是一个49.6 mm × 49.6 mm × 15 mm的LYSO晶体探测器,由一个由2.8 mm × 2.8 mm SiPM元件组成的16 × 16阵列读出。为了减少需要采集的信号通道的数量,检测器采用行-列求和。采用基于统计的定位方法进行事件定位和交互深度(DOI)解码。在研究的变量中,暗计数噪声对固有空间分辨率的影响最大。探测器校准和探测器测试之间5-10%的增益差异对固有空间分辨率性能影响不大,导致定位偏差轻微。在单个SiPM通道之间,增益可变性高达25%,没有可测量的差异。基于这些结果,我们计划将探测器冷却到室温以下,以减少暗计数噪声,并主动控制sipm的温度,以减少增益随时间的漂移。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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Impact on the Spatial Resolution Performance of a Monolithic Crystal PET Detector Due to Different Sensor Parameters.

The performance characteristics of a monolithic crystal PET detector utilizing a novel sensor on the entrance surface (SES) design is reported. To facilitate this design, we propose to utilize a 2D silicon photomultiplier (SiPM) array device. SiPMs are a form of Geiger-Muller mode avalanche photodiodes (GMAPD) that can provide signal gain similar to a photomultiplier tube (PMT). Since these devices are still under active development, their performance parameters are changing. Using a multi-step simulation process, we investigated how different SiPM parameters affect the performance of a monolithic crystal PET detector. These parameters include gain variability between different channels; gain instability; and dark count noise. The detector simulated was a 49.6 mm by 49.6 mm by 15 mm LYSO crystal detector readout by a 16 by 16 array of 2.8 mm by 2.8 mm SiPM elements. To reduce the number of signal channels that need to be collected, the detector utilizes row-column summing. A statistics based positioning method is used for event positioning and depth of interaction (DOI) decoding. Of the variables investigated, the dark count noise had the largest impact on the intrinsic spatial resolution. Gain differences of 5-10% between detector calibration and detector testing had a modest impact on the intrinsic spatial resolution performance and led to a slight bias in positioning. There was no measurable difference with a gain variability of up to 25% between the individual SiPM channels. Based upon these results we are planning to cool our detectors below room temperature to reduce dark count noise and to actively control the temperature of the SiPMs to reduce drifts in gain over time.

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