Synthesis and photoluminescent behavior of Eu3+-doped alkaline-earth tungstates
Eu3+-doped alkaline-earth tungstates MWO4 (M=Ca2+, Sr2+, Ba2+) were prepared by a polymeric precursor method based on the Pechini process. The polymeric precursors were calcined at 700°C for 2h in order to obtain well-crystallized powders and then characterized by X-ray diffraction (XRD), thermograv...
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Published in: | The Journal of physics and chemistry of solids Vol. 73; no. 5; pp. 635 - 640 |
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Main Authors: | , , , , |
Format: | Journal Article |
Language: | English |
Published: |
Elsevier Ltd
01-05-2012
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Subjects: | |
Online Access: | Get full text |
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Summary: | Eu3+-doped alkaline-earth tungstates MWO4 (M=Ca2+, Sr2+, Ba2+) were prepared by a polymeric precursor method based on the Pechini process. The polymeric precursors were calcined at 700°C for 2h in order to obtain well-crystallized powders and then characterized by X-ray diffraction (XRD), thermogravimetric analysis (TG), scanning electron microscopy (SEM), Fourier-transform infrared (FTIR) spectroscopy and photoluminescence spectroscopy (PL). All prepared samples showed a pure crystalline phase with scheelite-type structure confirmed by XRD. It was noted that the charge-transfer band shifted from 260 to 283nm when calcium is replaced by strontium. However, this band was not observed for Eu3+-doped barium tungstate. Upon excitation at 260nm, the emission spectra are dominated by the red 5D0→7F2 transition at 618nm. By analyzing of the emission lines, it was inferred that Eu3+ ions occupy low symmetry sites in the host lattice. It was also found that Eu3+-doped SrWO4 displays better chromaticity coordinates and greater luminescence intensity than the other samples.
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► A series of Eu3+-doped alkaline-earth tungstates were prepared by a polymeric precursor method. ► Eu3+ ions occupy low symmetry sites in the host lattice. ► The effect of the alkaline-earth ionic radius on the energy transfer from WO4 groups to Eu3+ ions was studied. ► The SrWO4:Eu3+ phosphor showed strongest luminescence intensity and better chromatic coordinates. |
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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 0022-3697 1879-2553 |
DOI: | 10.1016/j.jpcs.2011.12.026 |