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RESEARCH PRODUCT

Inverted-conical light guide for crosstalk reduction in tightly-packed scintillator matrix and MAPMT assembly

Yu Kai ChangM. A. HuangM. A. HuangJ. J. HuangM. Z. WangJiwoo NamJ. LeeH. S. ChoiS. JeongA. J. Castro-tiradoC. R. ChenJakub ŘíPaCarl Budtz-jørgensenC. J. EylesI. V. YashinS. W. KimIl Han ParkM. B. KimSøren BrandtVasily PetrovK. W. MinP. H. ConnellV. V. BogomolovVictor RegleroPisin ChenTsung-che LiuS. I. SvertilovH. LimJ. M. RodrigoJ. KimM. I. Panasyuk

subject

PhysicsNuclear and High Energy PhysicsScintillationTotal internal reflectionOptical fiberPhysics::Instrumentation and Detectorsbusiness.industryDetectorScintillatorPhotocathodeParticle detectorlaw.inventionOpticslawScintillation counterOptoelectronicsbusinessInstrumentation

description

Abstract In this paper we present the Inverted-Conical light guide designed for optical crosstalk reduction in the scintillator-MAPMT assemblies. The research was motivated by the 30% crosstalk observed in UFFO X-ray telescope , UBAT, during the preliminary calibration with MAPMTs of 64 2.88 × 2.88 mm2 pixels and identically gridded YSO crystal matrices. We began the study with the energy and crosstalk calibrations of the detector, then we constructed a GEANT4 simulation with the customized metallic film model as the MAPMT photocathode . The simulation reproduced more than 70% of the crosstalk and explained it as a consequence of the total reflection produced by the photocathode. The result indicated that the crosstalk mechanism could be a common case in most of the contact-assembled scintillation detectors. The concept of the Inverted-Conical light guide was to suppress the total reflection by contracting the incident angle of the scintillation. We optimized the design in the simulation and fabricated a test sample. The test sample reduced 52% crosstalk with a loss of 6% signal yield. The idea of the Inverted-Conical light guide can be adapted by scintillation detectors multi-pixel, imaging-purpose scintillation detectors such as the ultra-fast GRB observatory UFFO-UBAT, whose performances are sensitive to responding time, image resolution, and geometrical modifications.

https://doi.org/10.1016/j.nima.2014.10.037