Journal of Inorganic Materials

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Influence of Gamma-ray Irradiation on the Luminescence of LaBr3:Ce and CeBr3 Crystals

PENG Chen1, HE Weimin1, JIA Yuzhen1, SONG Baijun1, CHENG Yao1, FAN Xiaoyu1, BAI Qingrui1, CHANG Jun1, LIU Bo2, WANG Zhongzhi2, YANG Fan1   

  1. 1. School of Physics, Nankai University, Tianjin 300071, China;
    2. Baotou Research Institute of Rare Earths, Baotou, 014030, China
  • Received:2026-07-14 Revised:2026-07-28
  • Contact: YANG Fan, professor. E-mail: fan@nankai.edu.cn; WANG Zhongzhi, Senior Engineer. E-mail: 198322wzz@163.com
  • About author:PENG Chen (1997-), female, PhD candidate. E-mail: 1120220080@mail.nankai.edu.cn
  • Supported by:
    Development of Key Preparation Technologies for Rare-Earth Luminescent Materials for Next-Generation Solid-State Lighting and Displays (2025Z2633); National Natural Science Foundation of China (12575193); Funding of State Key Laboratory of Functional Crystals and Devices (SKLFCD202502SIC)

Abstract: LaBr3:Ce and CeBr3 crystals exhibit high light yield, fast decay, and good energy resolution. They are widely applied in γ-ray spectroscopy and space exploration. Therefore, it is essential to investigate their radiation damage effects. At present, changes in the luminescence behavior of these crystals after ionizing irradiation are not sufficiently studied. In this work, LaBr3:Ce and CeBr3 crystals were irradiated step by step with γ-rays. Radiation induced absorption coefficient (RIAC) spectra, photoluminescence (PL) spectra and PL decay curves were used to investigate the luminescence characteristic and decay kinetics of the crystals before and after irradiation. The results show that both crystals exhibit Ce3+ 5d→4f transition emission and self-trapped exciton (STE) broadband emission before irradiation. The overlap between the Ce3+ emission spectra and the excitation spectra of STE emission indicates that there may be the energy transfer process from Ce3+ emission to STE emission. The PL decay results show that the decay time of STE emission under 300 nm excitation is significantly longer than the intrinsic decay time measured under 450 nm excitation. It suggests that the STE emission under 300 nm excitation may involve two contributions: a fast process from direct STE excitation and a slow process associated with STE re-excitation by Ce3+ emission. After γ-ray irradiation, the RIAC values of both crystals gradually approach saturation with increasing cumulative irradiation dose. The relative STE emission intensity of LaBr3:Ce crystal increases significantly compared with that before irradiation, and the decay time of STE emission under 300 nm excitation is prolonged. In contrast, no obvious changes are observed in the PL spectral shape or decay time of CeBr3 crystal after irradiation. Combined with RIAC analysis, the enhanced STE emission in LaBr3:Ce after saturation of radiation-induced absorption may be related to changes in the local distribution of radiation-induced defects, which enhances the energy transfer process from Ce3+ emission to STE emission. The prolonged STE decay time under 300 nm excitation may be associated with the increased relative contribution of the slow emission process. This investigation provides experimental evidence for understanding the irradiation induced luminescence behavior and radiation damage effects of LaBr3:Ce and CeBr3 crystals.

Key words: LaBr3:Ce crystal, CeBr3 crystal, radiation damage, photoluminescence, decay time

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