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Preparation and Properties of Ti, Eu Co-doped Y_2O_2S:0.06Ti,0.08Eu Phosphor with Red Long Afterglow

机译:Ti,欧盟共掺杂Y_2O_2S的制备及性能:0.06Ti,0.08eu磷,红色余辉

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Ti,Eu co-doped Y_2O_2S:0.06Ti,0.08Eu phosphor with red long afterglow emission from Eu ions was synthesized via traditional sintering method. Results showed that sintering temperature has great influence on the crystal structure, luminescence and afterglow property of the phosphors. The best luminescence and afterglow properties were obtained for the phosphors sintered at 1200°C for 2.5h. Furthermore, only emissions originated from charge transition of Eu~(3+) was found in the luminescence spectra whereas the afterglow spectra were composed of two sets of emissions: a broad yellow emission band around 565nm and a group of narrow peaks in the wavelength range above 530 nm. The origin of afterglow spectra was discussed: the former is likely related to emission from Ti related traps and the latter is supposed to come from the Eu~(3+) through an energy transfer process from Ti emission to Eu~(3+).
机译:TI,欧盟共掺杂Y_2O_2S:0.06TI,通过传统烧结法合成了欧盟离子的红色长期含量的0.08EU磷光体。结果表明,烧结温度对磷光体的晶体结构,发光和余辉特性产生了很大影响。获得了在1200℃下烧结的磷光体的最佳发光和余辉性能2.5h。此外,在发光光谱中发现源自Eu〜(3+)的电荷转变的排放,而余辉光谱由两组排放组成:宽的黄色发射带宽约为565nm,并且在波长范围内的一组窄峰组成超过530纳米。讨论了余辉光谱的起源:前者可能与TI相关陷阱的发射有关,后者应该通过从TI发射到EU〜(3+)的能量转移过程中来自EU〜(3+)。

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