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Co-Precipitation Synthesis and Spectral Characteristics of Long Afterglow Phosphor Y_2O_2S:Sm^(3+), Mg^(2+), Ti^(4+) 被引量:3

Co-Precipitation Synthesis and Spectral Characteristics of Long Afterglow Phosphor Y_2O_2S:Sm^(3+), Mg^(2+), Ti^(4+)
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摘要 Y2O2S:Sm^3+, Mg^2+, Ti^4+ phosphor was synthesized by co-precipitation method. The crystalline structure of all synthesized phosphors was investigated by XRD. The result showed that all synthesized phosphors had a hexagonal crystal structure, which was the same as Y2O2S. The emission spectrum and excitation spectrum were measured, and the effect of Sm^3 + molar ratio on the spectra was discussed. The emission spectra of the phosphors showed three emission peaks due to typical transitions of Sm^3 + (4G5/2→6HJ ,J = 5/2, 7/2, 9/2), and the emission peaks at 606 nm was stronger than others. With the increase of Sm^3 + molar ratio, the emission intensity was strengthened. The excitation peaks were ascribed to the representative energy transition 4f→4f of Ti^4+ phosphor prepared by co-precipitation method was Sm^3+ ions. The results indicated that the Y2O2S : Sm^3+ , Mg^2+ , an efficient long afterglow phosphor. Y2O2S:Sm^3+, Mg^2+, Ti^4+ phosphor was synthesized by co-precipitation method. The crystalline structure of all synthesized phosphors was investigated by XRD. The result showed that all synthesized phosphors had a hexagonal crystal structure, which was the same as Y2O2S. The emission spectrum and excitation spectrum were measured, and the effect of Sm^3 + molar ratio on the spectra was discussed. The emission spectra of the phosphors showed three emission peaks due to typical transitions of Sm^3 + (4G5/2→6HJ ,J = 5/2, 7/2, 9/2), and the emission peaks at 606 nm was stronger than others. With the increase of Sm^3 + molar ratio, the emission intensity was strengthened. The excitation peaks were ascribed to the representative energy transition 4f→4f of Ti^4+ phosphor prepared by co-precipitation method was Sm^3+ ions. The results indicated that the Y2O2S : Sm^3+ , Mg^2+ , an efficient long afterglow phosphor.
出处 《Journal of Rare Earths》 SCIE EI CAS CSCD 2007年第1期23-26,共4页 稀土学报(英文版)
基金 Project supported by the Hebei Developing Foundation of Science&Technology (51215103b)
关键词 Y2O2S: Sm^3+ Mg^2+ Ti^4+ CO-PRECIPITATION emission spectra excitation spectra rare earths Y2O2S: Sm^3+ , Mg^2+ , Ti^4+ co-precipitation emission spectra excitation spectra rare earths
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