余辉
发光
共沉淀
热液循环
矿物学
材料科学
亮度
分析化学(期刊)
化学
物理
光学
天体物理学
地质学
无机化学
光电子学
色谱法
地震学
伽马射线暴
作者
Ou Hai,Bin Qin,Xin Xiao,Qiang Ren,Xiu Lan Wu,Meng Pei,Jian Li
摘要
Abstract The afterglow properties of long afterglow luminescent materials are greatly affected by their defects, which are distributed on the grain surface. Increasing the exposed surface area is an important method to improve the afterglow performance. In this research, long rod‐shaped long afterglow materials Sr 2 MgSi 2 O 7 :Eu 2+ ,Dy 3+ were prepared using the hydrothermal‐coprecipitation method. When the reaction time reached 96 h, the length of the afterglow materials could grow to 2 mm, and the sintering temperature was just 1150°C. The emission spectra of all obtained samples upon excitation at 397 nm had a maximum of 465 nm, which belonged to the representative transition of Eu 2+ . The initial brightness was 1.35 cd/m 2 . The afterglow time could reach 19 h, giving a good afterglow performance. The research on this kind of material has essential significance in the exploration of luminescence mechanisms and their applications.
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