Author:
Zarei Hajar,Nagao Yuto,Yamamoto Kohei,Itoh Masatoshi,Yamaguchi Mitsutaka,Kawachi Naoki,Watabe Hiroshi
Abstract
Abstract
In our previous work, a cost-effective Compton camera (CC)
using Ce doped Gd3(Al,Ga)5O12(Ce:GAGG) scintillator
consisting of two detectors, scatterer
(20.8 × 20.8 × 5 mm3) and absorber
(41.7 × 41.7 × 10 mm3), was developed to image
gamma rays having energy more than 511 keV. This study fabricated
a newly developed CC with a larger scatterer and thinner
absorber. The system consists of two detectors: a scatterer and an
absorber of Ce:GAGG scintillator. The size of the scatterer and
absorber is the same; a
40-mm × 40-mm × 5-mm array block consists
of 40 × 40 pixels. The size of each scintillator pixel is
0.85 mm × 0.85 mm for both systems. Imaging
experiments of Na-22 and Cs-137 point sources were performed to
investigate the imaging capability of the new camera, and then the
obtained data were compared to the previous CC. The current CC's
absolute detection efficiency (DE
a
) and photopeak detection
efficiency (DE
p
) are improved by 1.6 and 2 times greater than
the previous one. At the same time, both systems' spatial and
angular resolutions are almost the same value at 511 keV. The
Compton camera module (CCMod) in GATE v9.0 was employed for Monte
Carlo simulations to reproduce the experimental data showing a good agreement.
Subject
Mathematical Physics,Instrumentation
Cited by
2 articles.
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