Yang Sheng, Li Mohan, Reed Michael, Hugg James, Chen Henry, Abbaszadeh Shiva
Department of Nuclear, Plasma, and Radiological Engineering, University of Illinois at Urbana-Champaign, Urbana, IL, 61801 USA.
Kromek USA/eV Products, Saxonburg, PA, 16056, USA.
IEEE Trans Radiat Plasma Med Sci. 2020 Jan;4(1):91-97. doi: 10.1109/TRPMS.2019.2915054. Epub 2019 May 6.
Improving 511 keV photon detection sensitivity is a common goal for positron emission tomography system designers. One attractive approach to increase sensitivity is recovering events that are normally rejected. The kinematics of Compton scattering can be used to recover the line of response through direction difference angle (DDA). The uncertainty of DDA is determined by the energy and spatial resolution of a system. In this work, we evaluated the performance of small animal CZT-based positron emission tomography systems with energy resolution of 1%, 4%, and 6% and different spatial resolution based on prior work for guiding new design efforts. Designs with energy resolution limited by counting statistics and by electronic noise were considered. The influence of modifying the conventional energy window and uncertainty of DDA was investigated. For a system with 4% energy resolution and limited by electronic noise, the figure of merit of noise equivalent count increases by 65% as the lower energy bound increases from 471 keV to 493 keV. If the system-wide energy resolution becomes worse than 4% of the full width half maximum at 511 keV, going to a pixel size finer than 1 mm has very limited effect in reducing total angular uncertainty. For a system with 1% energy resolution, as the spatial resolution improves from 1 mm to 0.5 mm, the contrast-to-noise ratio increases by 9%.
提高511 keV光子探测灵敏度是正电子发射断层扫描系统设计者的一个共同目标。一种提高灵敏度的有吸引力的方法是恢复通常被拒收的事件。康普顿散射的运动学可用于通过方向差角(DDA)恢复响应线。DDA的不确定性由系统的能量和空间分辨率决定。在这项工作中,我们基于先前的工作评估了能量分辨率分别为1%、4%和6%且具有不同空间分辨率的基于CZT的小动物正电子发射断层扫描系统的性能,以指导新的设计工作。考虑了能量分辨率受计数统计和电子噪声限制的设计。研究了修改传统能量窗的影响以及DDA的不确定性。对于一个能量分辨率为4%且受电子噪声限制的系统,当较低能量界限从471 keV增加到493 keV时,噪声等效计数的品质因数增加65%。如果全系统的能量分辨率变得比511 keV处半高宽的4%更差,采用小于1 mm的像素尺寸在降低总角不确定性方面的效果非常有限。对于一个能量分辨率为1%的系统,当空间分辨率从1 mm提高到0.5 mm时,对比度噪声比增加9%。