Cherenkov Radiation Based Coincidence Time Resolution Measurements in BGO Scintillators

Handle

https://riunet.upv.es/handle/10251/232761

Cita bibliográfica

Gonzalez-Montoro, A.; Pourashraf, S.; Cates, JW.; Levin, CS. (2022). Cherenkov Radiation Based Coincidence Time Resolution Measurements in BGO Scintillators. Frontiers in Physics. 10. https://doi.org/10.3389/fphy.2022.816384

Titulación

Resumen

[EN] Bismuth germanate oxide (BGO) scintillators can be re-introduced in time-of-flight positron emission tomography (TOF-PET) by exploiting the Cherenkov luminescence emitted as a result from 511 keV interactions. Accessing the timing information from the relatively few emitted Cherenkov photons is now possible due to the recent improvements in enhanced near-ultraviolet high-density (NUV-HD) silicon photomultiplier (SiPM) technology, fast and low noise readout electronics, and the development of efficient data post-processing methods. In this work, we aim to develop a scalable detector element able to achieve excellent coincidence time resolution (CTR) required for TOF-PET using BGO scintillator elements of various lengths. The proposed detector element is optically coupled to 3.14 x 3.14 mm(2) NUV-sensitive SiPMs mounted on a custom design circuit board. In particular, we have evaluated the CTR performance of BGO crystal elements of dimensions 3 x 3 x 3 mm(3), 3 x 3 x 5 mm(3), 3 x 3 x 10 mm(3), and 3 x 3 x 15 mm(3), with chemically etched surfaces and wrapped in Teflon tape. To achieve excellent CTR performance, we apply state-of-the-art post-processing methods during data analysis. Best values of 156 & PLUSMN; 6 ps, 188 & PLUSMN; 5 ps, 228 & PLUSMN; 8 ps, and 297 & PLUSMN; 8 ps CTR FWHM have been achieved for the 3, 5, 10, and 15 mm length BGO crystals, respectively. These values improve to 105 & PLUSMN; 6 ps, 127 & PLUSMN; 8 ps, 133 & PLUSMN; 4 ps, and 189 & PLUSMN; 8 ps CTR FWHM, when only considering the Cherenkov component of the timing signal, which is extracted by considering the events with the fastest rise time (20% of the total data). The accurate classification of the events based on their rise time is possible; thanks to the implementation of a dual threshold approach that sets the lower threshold below one light photon equivalent level and the upper one above the signal amplitude of a single photon avalanche diode (SPAD).

Fuente

Frontiers in Physics

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