19–23 Jun 2023
Laboratori Nazionali di Frascati INFN
Europe/Rome timezone

Improving the time resolution of large area LaBr3:Ce detectors with SiPM array readout

22 Jun 2023, 12:30
20m
Aula Salvini (Laboratori Nazionali di Frascati INFN)

Aula Salvini

Laboratori Nazionali di Frascati INFN

Via E. Fermi 54 00044 Frascati (RM)

Speaker

Maurizio Giorgio Bonesini (Istituto Nazionale di Fisica Nucleare & Universita' di Milano Bicocca)

Description

LaBr3:Ce crystals have been introduced for radiation imaging in medical physics, with photomultiplier or single SiPM readout. An R&D was pursued with 1" LaBr3:Ce to realize compact large area detectors with SiPM array readout, aiming at high light yields, good energy resolution, good detector linearity and fast time response for low-energy X-rays.
A natural application was found inside the FAMU project at RIKEN-RAL muon facility, that aims at a precise measure of the proton Zemach radius to solve the so-called "proton radius puzzle", triggered by the recent measure of the proton charge radius at PSI. The goal is the detection of characteristic X-rays around 130 KeV. Other applications may be foreseen in medical physics, such as PET, and gamma-ray astronomy. A limiting factor, as compared to a photomultiplier (PMT) readout, is the poor timing characteristics of the detectors (especially falltime) due to the large capacity of the used SiPM arrays. With a standard parallel ganging typical risetime (falltime) of the order of 50 (300-400) ns are obtained. Long falltime are a problem in experiments as FAMU, where a "prompt" component must be separated from a "delayed" one in the signal X-rays to be detected. A dedicated R&D was pursued to settle this problem starting from hybrid ganging of SiPM cells, to development of a suitable zero pole circuit with increased overvoltage and to development of an ad-hoc electronics to split the 1" SiPM array in 4 quadrants, thus reducing the detectors' capacitance. The aim was to improve the timing characteristics, while keeping a good FWHM energy resolution. Reductions in falltime (risetime) up to a factor 3X were obtained with no deterioration of the energy resolution. A FWHM energy resolution better than 3% (8%) at the Cs137 (Co57) peak was obtained. These results compare well with the best results obtained with a PMT readout.

Primary authors

Maurizio Giorgio Bonesini (Istituto Nazionale di Fisica Nucleare & Universita' di Milano Bicocca) Mr Roberto Bertoni (Istituto Nazionale di Fisica Nucleare) Andrea Abba (Nuclear Instruments srl) Francesco Caponio (Nuclear Instruments srl) Marco Prata (PV) Massimo Rossella (Istituto Nazionale di Fisica Nucleare)

Presentation materials