TY - JOUR
T1 - Development of 2 cm-square Hamamatsu avalanche photodiodes for high-resolution X-rays and γ-rays detection
AU - Sato, R.
AU - Kataoka, J.
AU - Kanai, Y.
AU - Ishikawa, Y.
AU - Kawabata, N.
AU - Ikagawa, T.
AU - Saito, T.
AU - Kuramoto, Y.
AU - Kawai, N.
N1 - Copyright:
Copyright 2008 Elsevier B.V., All rights reserved.
PY - 2006/1/15
Y1 - 2006/1/15
N2 - The avalanche photodiodes (APDs) have attracted considerable attention in various field of experimental physics, but their uses are still limited in only a few experiments, possibly due to their small surface areas. Here, we report the development of the large-area (∼20mm square) APDs, for future applications to high-resolution X-rays and γ-rays detection. We have made two prototypes of reverse-type APDs based on different concepts, one consists of a 2×2 array of 10×10mm2 pixels (APD1) and the other is a monolithic pixel of 19×19mm2 size (APD2) to achieve a large effective area. By comparing the dark current and gain characteristics at room temperature (+20°C) and lightly cooled environment (-20°C), we quantitatively discussed the origin of predominant noise source at different temperatures. As a performance demonstration of newly developed APDs, we made a scintillation γ-ray detector consisting of a 20×20×5mm3 CsI(Tl) crystal and a 2 cm-square APD. The best FWHM energy resolution of 5.5±0.2% were obtained for 662keVγ-rays at room temperature. Similarly, the best FWHM energy resolution of 8.5±0.2% were obtained for 122 keV γ-rays at lightly cooled environment. We showed that the minimum detectable energy for scintillation light was 15 keV at 20°C and less than 5 keV at -20°C.
AB - The avalanche photodiodes (APDs) have attracted considerable attention in various field of experimental physics, but their uses are still limited in only a few experiments, possibly due to their small surface areas. Here, we report the development of the large-area (∼20mm square) APDs, for future applications to high-resolution X-rays and γ-rays detection. We have made two prototypes of reverse-type APDs based on different concepts, one consists of a 2×2 array of 10×10mm2 pixels (APD1) and the other is a monolithic pixel of 19×19mm2 size (APD2) to achieve a large effective area. By comparing the dark current and gain characteristics at room temperature (+20°C) and lightly cooled environment (-20°C), we quantitatively discussed the origin of predominant noise source at different temperatures. As a performance demonstration of newly developed APDs, we made a scintillation γ-ray detector consisting of a 20×20×5mm3 CsI(Tl) crystal and a 2 cm-square APD. The best FWHM energy resolution of 5.5±0.2% were obtained for 662keVγ-rays at room temperature. Similarly, the best FWHM energy resolution of 8.5±0.2% were obtained for 122 keV γ-rays at lightly cooled environment. We showed that the minimum detectable energy for scintillation light was 15 keV at 20°C and less than 5 keV at -20°C.
KW - Avalanche photodiode
KW - Scintillation detection
KW - γ-rays
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U2 - 10.1016/j.nima.2005.11.050
DO - 10.1016/j.nima.2005.11.050
M3 - Article
AN - SCOPUS:29444448415
SN - 0168-9002
VL - 556
SP - 535
EP - 542
JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
IS - 2
ER -