Influence of defects on luminescence properties of Gd3(Al,Ga)5O12:Ce scintillation crystals
-
Published:2021
Issue:6
Volume:70
Page:066101
-
ISSN:1000-3290
-
Container-title:Acta Physica Sinica
-
language:
-
Short-container-title:Acta Phys. Sin.
Author:
Meng Meng,Qi Qiang,He Chong-Jun,Ding Dong-Zhou,Zhao Shu-Wen,Shi Jun-Jie,Ren Guo-Hao, , , , ,
Abstract
There are many problems during the preparation of the scintillation crystal Gd<sub>3</sub>(Al,Ga)<sub>5</sub>O<sub>12</sub>:Ce (abbreviated as GAGG:Ce), such as inclusions and antisite-defect. In order to inhibit these defects and obtain large-size and high-quality GAGG:Ce crystal, this study uses Gd<sub>3</sub>(Al,Ga)<sub>5</sub>O<sub>12</sub> as the matrix and Ce<sup>3+</sup> as the doping ions to grow the GAGG:Ce crystal by the Czochralski method. The phase structure, micro-region composition, optical and scintillation properties of GAGG:Ce are tested and compared. It is found that tipical Ce<sup>3+</sup> absorption bands are at 340 nm and 440 nm, and the linear transmittance at 550 nm is 82%. The transmittance of the crystal tail drops to about 70% due to the macroscopic defects such as inclusions. The micro-region composition analysis shows that the three types of inclusions in GAGG:Ce crystal are Gd-rich phase, Ce-rich phase, and (Al,Ga)<sub>2</sub>O<sub>3</sub> phase. The Ce<sup>3+</sup> ion emission wavelength of GAGG:Ce crystal is about 550 nm excited by the X-ray, and there is also an emission wavelength caused by the Gd<sub>Al/Ga</sub> antisite-defect at 380 nm. The emission intensity of Gd<sub>Al/Ga</sub> antisite-defect in the lack of (Al,Ga) component is higher than that in the excess (Al,Ga) component. The inclusions and Gd<sub>Al/Ga</sub> antisite-defect make the luminous efficiency of GAGG:Ce crystal decrease by 12.5% and the corresponding light yield decreases from 58500 to 52000 photon/MeV. The tunneling effect between Gd<sub>Al/Ga</sub> antisite-defect ions and neighboring Ce<sup>3+</sup> ions makes the decay time of the GAGG:Ce crystal extend from 117.7 to 121.9 ns, and the ratio of slow component increases from 16% to 17.2%. The migration of energy along the Gd<sup>3+</sup> sublattice makes the rise time of the GAGG:Ce crystal extend from 8.6 to 10.7 ns. The above conclusions further deepen the understanding of the source of inclusions and the relationship between the Gd<sub>Al/Ga</sub> antisite-defect and crystal composition, and provide a theoretical basis for restraining the defects and improving the crystal properties.
Publisher
Acta Physica Sinica, Chinese Physical Society and Institute of Physics, Chinese Academy of Sciences
Subject
General Physics and Astronomy
Reference22 articles.
1. He W, Zhang Y P, Wang J H, Wang S X, Xia H P 2011 Acta Phys. Sin. 60 042901 何伟, 张约品, 王金浩, 王实现, 夏海平 2011 物理学报 60 042901 2. Meng M, Qi Q, Ding D Z, He C J, Shi J J, Ren G H 2019 J. Synth. Cryst. 48 8 孟猛, 祁强, 丁栋舟, 赫崇君, 施俊杰, 任国浩 2019 人工晶体学报 48 8 3. Sakthong O, Chewpraditkul W, Wanarak C, Kamada K, Yoshikawa A, Prusa P, Nikl M 2014 Nucl. Instrum. Methosds Phys. Res. A 751 1 4. Tamagawa Y, Inukai Y, Ogawa I, Kobayashi M 2015 Nucl. Instrum. Methods Phys. Res. A 795 192 5. Kochurikhin V, Kamada K, Kim J, Ivanov M, Yoshikawa A 2020 J. Cryst. Growth 531 1
Cited by
2 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
|
|