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arXiv 2510.03488physics.ins-dethep-exphysics.med-ph
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用于 keV–GeV 能量范围超快计时的闪烁体集成微通道板光电倍增管

Scintillator-integrated microchannel plate photomultiplier tubes for ultrafast timing over keV-GeV energy scales

Ryosuke Ota, Yuya Onishi, Daehee Lee, Yuki Ichikawa, Koji Kuramoto, Kenshi Shimano, Yutaka Hasegawa, Eric Berg, Takahiro Moriya, Simon R. Cherry, Sun Il Kwon

AI总结:

本文提出集成氟化钡或锗酸铋的 SCI-IMP 探测器,利用 511 keV 伽马射线和 GeV 级宇宙射线 μ 子验证其兼具能量测量与数十皮秒乃至 16.8 ps 超快计时能力。

摘要:

长期以来,辐射的精确测量在从超越标准模型的基础物理到飞行时间正电子发射断层扫描等医学成像的广泛研究和工业领域中发挥着至关重要的作用。开发能够实现数十皮秒量级高计时精度并具备能量测量能力的辐射探测器仍然不可或缺且颇具挑战。在本研究中,我们开发了两种闪烁体集成微通道板光电倍增管(SCI-IMPs),一种集成氟化钡,另一种集成锗酸铋,以实现同时的高精度计时和能量测量。为评估其在 keV 到 GeV 量级宽能量范围内的性能,研究使用了电子-正电子湮灭伽马射线和宇宙射线 μ 子。在能量测量方面,两种探测器在 511 keV 下均实现了约 35% 的能量分辨率。在使用 511 keV 进行计时测量时,两种探测器均获得了约 50 ps 半高全宽(FWHM)的符合时间分辨率(CTR)。相比之下,在宇宙射线 μ 子能量通常为 GeV 量级的宇宙射线 μ 子实验中,基于氟化钡和锗酸铋的探测器测得的 CTR 分别为 25.1 和 16.8 ps FWHM。本研究建立的通用闪烁体集成技术可拓宽新开发的 SCI-IMPs 的适用性。特别是,这些结果表明,所开发的探测器在保留能量测量能力的同时突破了计时性能边界,并有望在未来的基础物理实验和医学成像中获得应用。

英文摘要:

Precise measurement of radiation has long played a vital role in a wide range of research and industrial fields, from fundamental physics beyond the Standard Model to medical imaging such as time-of-flight positron emission tomography. Developing radiation detectors that achieve high timing precision-on the order of a few tens of picoseconds-and energy measurement capabilities remains indispensable yet challenging. In this study, we developed two types of scintillator-integrated microchannel plate photomultiplier tubes (SCI-IMPs), one incorporating barium fluoride, and the other bismuth germanate, to enable simultaneous high-precision timing and energy measurements. To evaluate their performance over a wide energy range from keV- to GeV-scale, electron-positron annihilation gamma rays and cosmic ray muons were used. For energy measurements, both detectors achieved an energy resolution of approximately 35% at 511 keV. For timing measurements using 511 keV, coincidence time resolutions (CTRs) of approximately 50 ps full width at half maximum (FWHM) were obtained for both detectors. In contrast, for cosmic ray muon experiments where cosmic ray muon energy is typically on the order of GeV, CTRs were measured to be 25.1 and 16.8 ps FWHM for barium fluoride- and bismuth germanate-based detectors, respectively. The versatile scintillator-integration technique established in this study can broaden the applicability of the newly developed SCI-IMPs. In particular, these results demonstrate that the developed detectors push the boundaries of timing performance while retaining energy measurement and hold promise for future applications in fundamental physics experiments and medical imaging.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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