余辉
掺杂剂
热释光
发光
荧光粉
兴奋剂
持续发光
激发态
光致发光
材料科学
化学
分析化学(期刊)
天体物理学
光电子学
原子物理学
物理
伽马射线暴
色谱法
作者
Wang Luo,Xintong Zhang,Kaofeng Huang,Bohan Wang,Yu Wang,Zhilie Tang,Kezhi Zheng
标识
DOI:10.1016/j.jlumin.2022.119512
摘要
Long afterglow materials feature long-lasting luminescence after the cessation of the excitation source. The rising demand for afterglow materials in many applications such as deep tissue imaging, ultrasensitive sensing, and radiation detection has led to extensive research on X-ray-activated afterglow systems. However, the progress in this field is constrained by the limitation and shortage of radiation-induced afterglow materials. Herein, a newly X-ray-excited long afterglow phosphor CaZnOS:Tb 3+ has been developed by using lithium-assisted synthetic protocol. Afterglow properties of Tb 3+ -doped CaZnOS microcrystals are systematically investigated by considering the dopant concentration, reaction temperature, reaction time, reaction atmosphere, and gas flow. As the gas flow of argon atmosphere increases from 0.05 to 0.5 L/min, the CaZnOS:Tb 3+ microcrystals exhibit a distinct change in trap depth from 0.59 to 0.75 eV, corresponding to a gradual increase in afterglow time. Together with thermoluminescence analysis, the long afterglow mechanism is also discussed in this work. These results highlight the importance of reaction gas flow for the efficient regulation of traps and defects in afterglow materials. Furthermore, they provide a fundamental design principle and new route for the creation of lanthanide-doped CaZnOS afterglow phosphors. • X-ray-excited long afterglow phosphor CaZnOS:Tb 3+ has been developed by using lithium-assisted synthetic protocol. • Afterglow luminescence of lanthanide (terbium) ions in CaZnOS hosts with high brightness and long duration time has been achieved for the first time. • The defects and traps in the long afterglow luminescent materials can be regulated by changing the gas flow of argon atmosphere.
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