The Accuracy of Cerenkov Photons Simulation in Geant4/Gate Depends on the Parameterization of Primary Electron Propagation.

IF 1.9 3区 物理与天体物理 Q2 PHYSICS, MULTIDISCIPLINARY Frontiers in Physics Pub Date : 2022-01-01 Epub Date: 2022-04-28 DOI:10.3389/fphy.2022.891602
Carlotta Trigila, Gerard Ariño-Estrada, Sun Il Kwon, Emilie Roncali
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Abstract

Energetic electrons traveling in a dispersive medium can produce Cerenkov radiation. Cerenkov photons' prompt emission, combined with their predominantly forward emission direction with respect to the parent electron, makes them extremely promising to improve radiation detector timing resolution. Triggering gamma detections based on Cerenkov photons to achieve superior timing resolution is challenging due to the low number of photons produced per interaction. Monte Carlo simulations are fundamental to understanding their behavior and optimizing their pathway to detection. Therefore, accurately modeling the electron propagation and Cerenkov photons emission is crucial for reliable simulation results. In this work, we investigated the physics characteristics of the primary electrons (velocity, energy) and those of all emitted Cerenkov photons (spatial and timing distributions) generated by 511 keV photoelectric interactions in a bismuth germanate crystal using simulations with Geant4/GATE. Geant4 uses a stepwise particle tracking approach, and users can limit the electron velocity change per step. Without limiting it (default Geant4 settings), an electron mean step length of ~250 μm was obtained, providing only macroscopic modeling of electron transport, with all Cerenkov photons emitted in the forward direction with respect to the incident gamma direction. Limiting the electron velocity change per step reduced the electron mean step length (~0.200 μm), leading to a microscopic approach to its transport which more accurately modeled the electron physical properties in BGO at 511 keV. The electron and Cerenkov photons rapidly lost directionality, affecting Cerenkov photons' transport and, ultimately, their detection. Results suggested that a deep understanding of low energy physics is crucial to perform accurate optical Monte Carlo simulations and ultimately use them in TOF PET detectors.

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Geant4/Gate 中的塞伦科夫光子模拟精度取决于初级电子传播的参数化。
在色散介质中运动的高能电子可以产生塞伦科夫辐射。切伦科夫光子发射迅速,而且相对于母体电子而言主要是向前发射,因此极有希望提高辐射探测器的定时分辨率。由于每次相互作用产生的光子数量较少,因此基于塞伦科夫光子触发伽马射线探测以实现更高的定时分辨率具有挑战性。蒙特卡洛模拟是了解其行为和优化其探测路径的基础。因此,准确模拟电子传播和塞伦科夫光子发射对于获得可靠的模拟结果至关重要。在这项工作中,我们利用 Geant4/GATE 模拟研究了锗酸铋晶体中 511 千伏光电相互作用产生的初级电子(速度、能量)和所有发射的切伦科夫光子(空间和时间分布)的物理特性。Geant4 采用逐步跟踪粒子的方法,用户可以限制每一步的电子速度变化。在没有限制的情况下(Geant4 的默认设置),得到的电子平均步长约为 250 μm,只提供了电子传输的宏观模型,所有的塞伦科夫光子都是在相对于入射伽马方向的前进方向发射的。限制每一步的电子速度变化可以减小电子平均步长(~0.200 μm),从而采用微观方法进行电子传输,更准确地模拟了511 keV波长下BGO中的电子物理性质。电子和塞伦科夫光子迅速失去了方向性,影响了塞伦科夫光子的传输,并最终影响了它们的探测。研究结果表明,深入理解低能物理对于进行精确的光学蒙特卡洛模拟并最终将其用于TOF PET探测器至关重要。
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来源期刊
Frontiers in Physics
Frontiers in Physics Mathematics-Mathematical Physics
CiteScore
4.50
自引率
6.50%
发文量
1215
审稿时长
12 weeks
期刊介绍: Frontiers in Physics publishes rigorously peer-reviewed research across the entire field, from experimental, to computational and theoretical physics. This multidisciplinary open-access journal is at the forefront of disseminating and communicating scientific knowledge and impactful discoveries to researchers, academics, engineers and the public worldwide.
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