TY - JOUR
T1 - An active gain-control system for Avalanche photo-diodes under moderate temperature variations
AU - Kataoka, J.
AU - Sato, R.
AU - Ikagawa, T.
AU - Kotoku, J.
AU - Kuramoto, Y.
AU - Tsubuku, Y.
AU - Saito, T.
AU - Yatsu, Y.
AU - Kawai, N.
AU - Ishikawa, Y.
AU - Kawabata, N.
N1 - Funding Information:
We greatly appreciate an anonymous referee for his/her comments to improve this manuscript. We also thank Dr. Phil Edwards for his constructive suggestions and careful comments to complete this work. J.Kataoka acknowledges a support by JSPS.KAKENHI (16206080).
PY - 2006/8/1
Y1 - 2006/8/1
N2 - Avalanche photodiodes (APDs) are a promising light sensor for various fields of experimental physics. It has been argued, however, that variation of APD gain with temperature could be a serious problem preventing APDs from replacing traditional photomultiplier tubes (PMTs) in some applications. Here we develop an active gain-control system to keep the APD gain stable under moderate temperature variations. As a performance demonstration of the proposed system, we have tested the response of a scintillation photon detector consisting of a 5 × 5 mm2 reverse-type APD optically coupled with a CsI(Tl) crystal. We show that the APD gain was successfully controlled under a temperature variation of Δ T = 20 {ring operator} C, within a time-cycle of 6000 s. The best FWHM energy resolution of 6.1 ± 0.2 % was obtained for 662 keV γ-rays, and the energy threshold was as low as 6.5 keV, by integrating data from + 20 {ring operator} C-0 {ring operator} C cycles. The corresponding values for - 20 {ring operator} C-0 {ring operator} C cycles were 6.9 ± 0.2 % and 5.2 keV, respectively. These results are comparable, or only slightly worse than that obtained at a fixed temperature. Our results suggest new potential uses for APDs in various space researches and nuclear physics. As examples, we briefly introduce the NeXT and Cute-1.7 satellite missions that will carry the APDs as scientific instruments for the first time.
AB - Avalanche photodiodes (APDs) are a promising light sensor for various fields of experimental physics. It has been argued, however, that variation of APD gain with temperature could be a serious problem preventing APDs from replacing traditional photomultiplier tubes (PMTs) in some applications. Here we develop an active gain-control system to keep the APD gain stable under moderate temperature variations. As a performance demonstration of the proposed system, we have tested the response of a scintillation photon detector consisting of a 5 × 5 mm2 reverse-type APD optically coupled with a CsI(Tl) crystal. We show that the APD gain was successfully controlled under a temperature variation of Δ T = 20 {ring operator} C, within a time-cycle of 6000 s. The best FWHM energy resolution of 6.1 ± 0.2 % was obtained for 662 keV γ-rays, and the energy threshold was as low as 6.5 keV, by integrating data from + 20 {ring operator} C-0 {ring operator} C cycles. The corresponding values for - 20 {ring operator} C-0 {ring operator} C cycles were 6.9 ± 0.2 % and 5.2 keV, respectively. These results are comparable, or only slightly worse than that obtained at a fixed temperature. Our results suggest new potential uses for APDs in various space researches and nuclear physics. As examples, we briefly introduce the NeXT and Cute-1.7 satellite missions that will carry the APDs as scientific instruments for the first time.
KW - Avalanche photodiode
KW - Gain-control
KW - Scintillation detection
KW - γ-rays
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U2 - 10.1016/j.nima.2006.03.033
DO - 10.1016/j.nima.2006.03.033
M3 - Article
AN - SCOPUS:33745916749
SN - 0168-9002
VL - 564
SP - 300
EP - 307
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 - 1
ER -