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Co-precipitation Synthesis And Study Of Long Afterglow Phosphors

Posted on:2007-07-26Degree:MasterType:Thesis
Country:ChinaCandidate:X M LiFull Text:PDF
GTID:2121360182485646Subject:Optics
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Long afterglow luminescence materials, which have excellent luminescent properties have been widely investigated and application. It appears some new synthesized methods to effectively improve the luminescent property with the new luminescent materials of the rare earth come forth.hi this paper, the Y2O2S:R3+,Mg2+,Ti4+(R3+=Eu3+,Sm3+,Tb3+) phosphors were synthesized first by co-precipitation method. Its x-ray diffraction patterns, the structure of crystal lattice and the luminescent properties were studied. Compared with the Y2O2S:Eu3+,Mg2+,Ti4+ phosphorescence prepared by high temperature solid state method, we can see that the phosphors prepared by co-precipitation method not only have small granularity and loosen structure but also can made the Eu3+ enter into crystal lattice and form luminescent centre easily. So the luminescent properties of Y2O2S:Eu3+,Mg2+,Ti4+can improve effectively.The change of emission spectra in Y2O2S:Sm3+,Mg2+,Ti4+and Y2O2S:Tb3+,Mg2+,Ti4+ were studied though altering the concentration of activator. The emission spectra of Y2O2S:Sm3+,Mg2+,Ti4+ increased with the increasing of Sm3+. In the emission spectra of Y2O2S:Tb3+,Mg2+,Ti4+ phosphors, the spectra rooted in the 5D4→7Fs increased straight and the spectra come from 5D3→7F5 increased firstly and decreased afterwards with the increased of Tb3+. The intensity was the strongest when the concentration of Tb3+ is 2.0%.The long afterglow phosphor (Ca1-xSrx)S:Eu2+ was fabricated by co-precipitation. The effect of the ratio of Ca2+ and Sr2+ on the crystal lattice and the effect of the concentration of Eu2+ on the luminescent properties through the analysis of XRD, excitation and emission. The blue shifts were observed when Sr2+ increased. The luminescent properties reach the best when the concentration of Eu2+ is 0.6% and the sintering temperature is 1100℃.Through these investigations in this paper, it made us have more realize and understand for the long afterglow materials by co-precipitation method and offer important experiment foundation for more study the formation method of this material.
Keywords/Search Tags:Co-precipitation method, Long afterglow, Y2O2S:R3+, Mg2+, Ti4+, Ca1-xSrxS:Eu2+, Emission spectra
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