硅光电倍增管
光电倍增管
物理
雪崩光电二极管
飞行时间
光学
光子计数
光电子学
击穿电压
紫外线
光子
电压
能量(信号处理)
探测器
闪烁体
量子力学
作者
Florin-Adrian Popescu,G. Chiritoi,E.M. Popescu
标识
DOI:10.1109/cas52836.2021.9604171
摘要
The silicon photomultiplier (SiPM) is increasingly used in single-photon or few-photon based applications such as spectroscopy, quantum experiments and distance measurements (LIDAR). Also, it founds its niche in fast timing applications such as time of flight positron emission tomography (TOF-PET) and in high energy physics (HEP). In astrophysics, SiPM arrays find their use in the development of near-UV telescopes for the observation from space of the ultraviolet tracks (290-430 nm) associated with giant extensive air showers produced by ultra-high energy primaries propagating in the earth's atmosphere with highest time precision. Accurate measurements of detected optical energy rely on the gain and breakdown setup of the SiPMs arrays, as individual cells in the array may require bespoken setting. The present paper presents methods for accurate determination of the breakdown voltage and gain for SiPM arrays.
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