光谱学与光谱分析 |
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Effect of Eu3+ Molar Ratio on the Spectra of Y2O2S:Eu3+, Mg2+ and Ti4+ Red Phosphor |
YANG Zhi-ping, GUO Zhi, ZHU Sheng-chao, WANG Wen-jie |
Physics Science and Technology College, Hebei University, Baoding 071002, China |
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Abstract Synthesis of Y2O2S:Eu3+, Mg2+ and Ti4+red phosphor by flux fusion method was presented. The decay curve of Y2O2S:Eu3+, Mg2+ and Ti4+ red phosphor was measured and the afterglow time was over one hour. The emission spectra and excitation spectra were measured, and the effect of Eu3+ molar ratio on the emission spectra and excitation spectra were also discussed. The emission spectra showed that Y2O2S:Eu3+, Mg2+ and Ti4+ had narrow emission peaks. The emission peaks ascribed to Eu3+ ions transition from 5DJ (J=0, 1, 2, 3,) to 7FJ (J=0,1,2,3,4,5) were found. With the increase of Eu3+ molar ratio, the emission peaks 513.6, 540.1,556.4,587.3 and 589.3 nm ascribed to the energy transition 5D2,5D1 to 7FJ(J=0, 1, 2, 3, 4) deteriorated gradually relative to the main emission peak at 627.0 nm. The emission peaks ascribed to energy transition 5D0 to 7FJ(J=0, 1, 2, 3, 4) didn’t weaken relative to the main emission peak. It was probably due to the so-called true activator saturation effect. This function on the higher activated states 5D2 and 5D1 was more distinct. The excitation spectra of Y2O2S:Eu3+, Mg2+ and Ti4+ showed that it had excitation peaks at 350 nm nearby, which was ascribed to the absorption of charge transfer (Eu3+-O2-, Eu3+-S2-). The excitation peaks at 468, 520 and 540 nm were ascribed to the representative energy transition 4f-4f of Eu3+ ions. With the increase of Eu3+ molar ratio, the excitation peaks 468, 520 and 540 nm strengthened relative to the main absorption peak at 350 nm nearby.
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Received: 2003-08-18
Accepted: 2003-12-29
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Corresponding Authors:
YANG Zhi-ping
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Cite this article: |
YANG Zhi-ping,GUO Zhi,ZHU Sheng-chao, et al. Effect of Eu3+ Molar Ratio on the Spectra of Y2O2S:Eu3+, Mg2+ and Ti4+ Red Phosphor [J]. SPECTROSCOPY AND SPECTRAL ANALYSIS, 2004, 24(12): 1506-1510.
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URL: |
https://www.gpxygpfx.com/EN/Y2004/V24/I12/1506 |
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