以反滴定共沉淀方法制备了Sc2O3:Nd、Sc2O3 :Yb纳米粉体,用热重、差热分析、X射线衍射对前驱体相变及粉体结构进行了研究,并研究了其光致发光.Sc2O3:Nd、 Sc2O3:Yb前躯体的热重和差热曲线分别在73 ℃、77 ℃与434 ℃、436 ℃出现了明显的热失重和吸热峰,结合XRD表明约在450 ℃,前驱体粉体经γ-ScOOH相转变为立方Sc2O3相.Reitveld方法精修给出Sc、O的原子坐标.结果表明,掺杂离子导致了晶格畸变.在825 nm光激发下,粉体Sc2O3 :Nd的1084 nm主荧光峰为Nd3+的4F3/2→4I11/2跃迁;在937 nm光激发下,粉体Sc2O3:Yb的1044 nm主荧光峰为Yb3+的2F5/2→2F7/2跃迁.Sc2O3:Nd、Sc2O3:Yb的发光光谱表明激活离子处于较强晶场中,Stark能级分裂大,有利于降低Yb3+的激光阈值、提高激光热稳定性.
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