Influence of defects on luminescence properties of Gd3(Al,Ga)5O12:Ce scintillation crystals

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

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