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Bismuth germanate coupled to near ultraviolet silicon photomultipliers for time-of-flight PET

机译:锗酸铋与近紫外硅光电倍增管耦合用于飞行时间PET

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摘要

Bismuth germanate (BGO) was a very attractive scintillator in early-generation positron emission tomography (PET) scanners. However, the major disadvantages of BGO are lower light yield and longer rise and decay time compared to currently popular scintillators such as LSO and LYSO. This results in poorer coincidence timing resolution and it has generally been assumed that BGO is not a suitable scintillator for time-of-flight (TOF) PET applications. However, when a 511-keV photon interacts in a scintillator, a number of Cerenkov photons are produced promptly by energetic electrons released by photoelectric or Compton interactions. If these prompt photons can be captured, they could provide a better timing trigger for PET. Since BGO has a high refractive index (increasing the Cerenkov light yield) and excellent optical transparency down to 320 nm (Cerenkov light yield is higher at shorter wavelengths), we hypothesized that the coincidence timing resolution of BGO can be significantly improved by efficient detection of the Cerenkov photons. However, since the number of Cerenkov photons is far less than the number of scintillation photons, and they are more abundant in the UV and blue part of the spectrum, photosensors need to have high UV/blue sensitivity, fast temporal response, and very low noise in order to trigger on the faint Cerenkov signal. In this respect, NUV-HD silicon photomultipliers (SiPMs) (FBK, Trento, Italy) are an excellent fit for our approach. In this study, coincidence events were measured using BGO crystals coupled with NUV-HD SiPMs. The existence and influence of Cerenkov photons on the timing measurements were studied using different configurations to exploit the directionality of the Cerenkov emissions. Coincidence resolving time values (FWHM) of ~270 ps from 2 × 3 × 2 mm3 BGO crystals and ~560 ps from 3 × 3 × 20 mm3 BGO crystals were obtained. To our knowledge, these are the best coincidence resolving time values reported for BGO to date. With these values, BGO can be considered as a relevant scintillator for TOF PET scanners, especially if photodetectors with even better near UV/blue response can be developed to further improve the efficiency of Cerenkov light detection.
机译:在早期的正电子发射断层扫描(PET)扫描仪中,锗酸铋(BGO)是非常吸引人的闪烁体。但是,与LSO和LYSO等目前流行的闪烁体相比,BGO的主要缺点是发光量低,上升和衰减时间长。这导致较差的重合定时分辨率,并且通常认为BGO不是适用于飞行时间(TOF)PET应用的闪烁体。但是,当511-keV光子在闪烁体中相互作用时,光电或康普顿相互作用释放的高能电子会迅速产生大量切伦科夫光子。如果可以捕获这些即时的光子,则它们可以为PET提供更好的时序触发。由于BGO的折射率高(增加了Cerenkov的光通量),并且在低至320 nm的情况下具有出色的光学透明度(在较短的波长下Cerenkov的光通量更高),因此我们假设通过有效地检测BGO可以显着提高BGO的同时定时分辨率。切伦科夫光子。但是,由于切伦科夫光子的数量远远少于闪烁光子的数量,并且它们在光谱的紫外线和蓝色部分更为丰富,因此光电传感器需要具有较高的紫外线/蓝色灵敏度,快速的时间响应和非常低的灵敏度噪声以触发微弱的切伦科夫信号。在这方面,NUV-HD硅光电倍增管(SiPM)(FBK,意大利特伦托)非常适合我们的方法。在这项研究中,巧合事件是使用BGO晶体和NUV-HD SiPM进行测量的。使用不同的配置来研究切伦科夫光子的存在和影响,以利用切伦科夫发射的方向性。 2×3×2 mm 3 BGO晶体的重合分辨时间值(FWHM)约为〜270 ps,而3×3×20 mm 3 BGO晶体的重合分辨时间值为〜560 ps获得。据我们所知,这是迄今为止BGO报告的最佳重合时间值。有了这些值,BGO可以被认为是TOF PET扫描仪的相关闪烁体,特别是如果可以开发出具有更好的近紫外/蓝光响应的光电探测器以进一步提高切伦科夫光探测效率的话。

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