无机材料学报 ›› 2021, Vol. 36 ›› Issue (2): 188-196.DOI: 10.15541/jim20200268

所属专题: 【虚拟专辑】透明陶瓷与光学晶体 【信息功能】透明陶瓷与光学晶体

• 研究论文 • 上一篇    下一篇

Gd3(Al,Ga)5O12:Ce闪烁晶体扭曲生长、组分偏析与性能研究

孟猛1,2,3(), 祁强1,4, 丁栋舟1,5(), 赫崇君2,3(), 赵书文1, 万博1, 陈露1, 施俊杰1,5, 任国浩1,5   

  1. 1.中国科学院 上海硅酸盐研究所, 上海 201899
    2.南京航空航天大学 工业和信息化部重点实验室, 空间光电探测与感知实验室, 南京 210016
    3.南京航空航天大学 航天学院, 南京 210016
    4.上海理工大学 材料科学与工程学院, 上海 200093
    5.中国科学院 海西创新研究院, 福建 350002
  • 收稿日期:2020-05-15 修回日期:2020-08-03 出版日期:2021-02-20 网络出版日期:2020-09-09
  • 通讯作者: 赫崇君, 副教授. E-mail: hechongjun@nuaa.edu.cn;
  • 作者简介:孟 猛(1994-), 男, 硕士研究生. E-mail: 865770183@qq.com
  • 基金资助:
    国家自然科学基金(61675095);“中国科学院关键技术人才”项目(Y74YQ3130G);中科院上海硅酸盐研究所科技创新重点项目(Y74ZC5152G);海西研究院自主部署项目(FJCXY18040202)

Twisted Growth, Component Segregation and Characteristics of Gd3(Al,Ga)5O12:Ce Scintillation Crystal

MENG Meng1,2,3(), QI Qiang1,4, DING Dongzhou1,5(), HE Chongjun2,3(), ZHAO Shuwen1, WAN Bo1, CHEN Lu1, SHI Junjie1,5, REN Guohao1,5   

  1. 1. Shanghai Institute of Ceramics, Chinese Academy of Sciences, Shanghai 201899, China
    2. Key Laboratory of Space Photoelectric Detection and Perception, Ministry of Industry and Information Technology, Nanjing University of Aeronautics and Astronautics, Nanjing 210016, China
    3. College of Astronautics, Nanjing University of Aeronautics and Astronautics, Nanjing 210016, China
    4. School of Materials Science and Engineering, University of Shanghai for Science and Technology, Shanghai 200093, China
    5. Fujian Institute of Innovation, Chinese Academy of Sciences, Fujian 350002, China
  • Received:2020-05-15 Revised:2020-08-03 Published:2021-02-20 Online:2020-09-09
  • About author:MENG Meng(1994-), male, Master candidate. E-mail: 865770183@qq.com
  • Supported by:
    National Natural Science Foundation of China(61675095);Project of “Key Technical Talents of the Chinese Academy of Sciences”(Y74YQ3130G);Key Project of Science and Technology Innovation of Shanghai Institute of Ceramics of Chinese Academy of Sciences(Y74ZC5152G);Independent Deployment Project of Hercynian Research Institute(FJCXY18040202)

摘要:

新型闪烁晶体Gd3(Al,Ga)5O12:Ce(简写为GAGG:Ce)在制备过程中易出现多晶扭曲生长、组分偏析等问题, 严重影响晶体的性能。为了得到大尺寸高质量的GAGG:Ce晶体, 采用X射线衍射(XRD)、电感耦合等离子体发射光谱(ICP-OES)和X射线激发发射谱(XEL)等手段, 结合熔体特性分析了GAGG:Ce晶体多晶扭曲生长、组分偏析的形成机制。通过调整温场、抑制组分挥发等方法生长出φ50 mm×120 mm的GAGG:Ce晶体, 并重点研究了GAGG:Ce晶体的光谱特性与闪烁性能。结果表明: GAGG:Ce晶体的光输出达58000 ph./MeV, 能量分辨率为6.4%@662 keV, 在550~800 nm波长区间的透过率约为82%。晶体闪烁衰减快分量为126 ns (83%), 慢分量为469 ns (17%)。晶体的发射峰中心波长在550 nm左右, 与硅光电倍增管的接收波长匹配, 且发光峰值处的透过率EWLT(Emission Weighted Longitudinal Transmittance)值高达79.8%。GAGG:Ce晶体兼具高光输出与高能量分辨率, 在中子和伽马射线探测领域具有广阔的应用前景。

关键词: 多晶扭曲生长, 温度梯度, 组分偏析, 衰减时间

Abstract:

There are many problems such as polycrystal twisted growth and component segregation during the preparation of the new scintillation crystal Gd3(Al,Ga)5O12:Ce (abbreviated as GAGG:Ce) by the Czochralski method. In order to solve these problems to obtain large-size and high-quality GAGG:Ce crystals, with a combination of melt characteristics, formation mechanism of twisted growth, component segregation, spectral characteristics and scintillation performance of GAGG:Ce crystals were studied. A complete GAGG:Ce crystal with size of ?50 mm× 120 mm was successfully grown by adjusting the temperature field and inhibiting the volatilization of the components. The results show that light output of the GAGG:Ce crystal sample (10 mm×10 mm×2 mm) is 58000 ph./MeV, while energy resolution is 6.4%@662 keV with transmittance at 550 nm of 82%, decay time of 126 ns (83%), and the slow component is 469 ns (17%). The peak position of emission wavelength of the crystal is about 550 nm, which matches well with the silicon photomultiplier. Meanwhile, the emission weighted longitudinal transmittance is as high as 79.8%. GAGG:Ce crystal has an excellent combination of high light output and energy resolution, and all of these properties show that GAGG:Ce crystal is a promising scintillator for neutron and gamma detection applications.

Key words: polycrystal twisted growth, temperature gradient, component segregation, decay time

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