28 May 2022 to 1 June 2022
La Biodola, Isola d'Elba
Europe/Rome timezone

Sub-100 ps Coincidente Time Resolution for ToF-PET detectors using FastIC

30 May 2022, 18:20
20m
Maria Luisa

Maria Luisa

Oral New technologies for PET/MR and TB-PET New technologies for PET/MR and TB-PET

Speaker

Antonio Mariscal-Castilla (Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos, University of Barcelona, Barcelona, Spain)

Description

Recent developments in Silicon Photomultiplier (SiPM) sensors and fast readout electronics are enabling new achievements in Coincidence-Time Resolution (CTR) for Positron-Emission Tomography (PET) detectors. The new 8-channel FastIC ASIC developed in CMOS 65~nm technology provides an accurate time-stamping of the detected particles and a linear energy measurement while having a power consumption of 12~mW/Ch. The ASIC have the capability of summing different readout channels in clusters of 4 channels before measuring time and energy. Evaluation of the ASIC showed CTR values of 94 ± 2 and 76 ± 2 ps FWHM for HPK SiPM S13360-3050PE and new technology FBK HD-NUV Low Field (3.2 x 3.12 mm² pixel, 40 μm cell) coupled to a pair of LSO:Ce:Ca 0.2% measuring 2 x 2 x 3 mm³. Furthermore, new FBK HD-NUV Low Field SiPM coupled to LYSO:Ce:Ca 0.2% measuring 3.13 x 3.13 x 20 mm³ yielded a CTR value of 126 ± 2 ps FWHM. Additionally, first measurements of the chip confirmed its ability to detect prompt light emitters e.g., using Cherenkov radiators like TlCl and PbF₂.

Primary authors

Antonio Mariscal-Castilla (Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos, University of Barcelona, Barcelona, Spain) Dr Sergio Gomez (Institut d’Estudis Espacials de Catalunya, University of Barcelona, 08028 Barcelona, Spain) Jose M. Fernández-Tenllado (Dept. F ́ısica Qua`ntica i Astrof ́ısica, Institut de Cie`ncies Del Cosmos (ICCUB), University of Barcelona (IEEC-UB), Barcelona, Spain) Joan Mauricio (Dept. F ́ısica Qua`ntica i Astrof ́ısica, Institut de Cie`ncies Del Cosmos (ICCUB), University of Barcelona (IEEC-UB), Barcelona, Spain) Nicolaus Kratochwil (CERN, Esplanade des Particules 1, 1211 Meyrin, Switzerland) Jerome Alozy (CERN, Esplanade des Particules 1, 1211 Meyrin, Switzerland) Gerard Arino-Estrada (University of California Davis, Davis, CA 95616, United States of America) Giancomo Borghi (Fondazione Bruno Kessler, 38123 Povo TN, Italy) Alberto Gola (Fondazione Bruno Kessler, 38123 Povo TN, Italy) Stanislaw Majewski (University of California Davis, Davis, CA 95616, United States of America) Rafel Manera (Dept. F ́ısica Qua`ntica i Astrof ́ısica, Institut de Cie`ncies Del Cosmos (ICCUB), University of Barcelona (IEEC-UB), Barcelona, Spain.) Rok Pestotnik (Jozˇef Stefan Institute, 1000 Ljubljana, Slovenia) Markus Piller (CERN, Esplanade des Particules 1, 1211 Meyrin, Switzerland) Anand Sanmukh (Dept. F ́ısica Qua`ntica i Astrof ́ısica, Institut de Cie`ncies Del Cosmos (ICCUB), University of Barcelona (IEEC-UB), Barcelona, Spain.) Andreu Sanuy (Dept. F ́ısica Qua`ntica i Astrof ́ısica, Institut de Cie`ncies Del Cosmos (ICCUB), University of Barcelona (IEEC-UB), Barcelona, Spain.) Etienne Auffray (CERN, Esplanade des Particules 1, 1211 Meyrin, Switzerland) Rafael Ballabriga (CERN, Esplanade des Particules 1, 1211 Meyrin, Switzerland) Michael Campbell (CERN, Esplanade des Particules 1, 1211 Meyrin, Switzerland) Georges El Fakhri (Gordon Center for Medical Imaging and Harvard Medical School, Boston, MA 02114, United States) David Gascón (Dept. F ́ısica Qua`ntica i Astrof ́ısica, Institut de Cie`ncies Del Cosmos (ICCUB), University of Barcelona (IEEC-UB), Barcelona, Spain.)

Presentation materials