Luminescence properties of Eu3+, Bi3+ coactivated CaLaNbWO8 red phosphors under near UV and blue excitations

Scheelite type red phosphors CaLa1–xNbWO8: xEu3+ (x = 0.01, 0.03, 0.05, 0.1, 0.15, 0.2, and 0.25) and CaLa0.8–yNbWO8: 0.2Eu3+, yBi3+(y = 0.1, 0.15, and 0.2) were prepared by conventional solid state reaction route. The crystalline structure, morphology and absorbance of these phosphors were characte...

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Published inPhysica status solidi. A, Applications and materials science Vol. 208; no. 9; pp. 2170 - 2175
Main Authors Thomas, Mariyam, Rao, Padala Prabhakar, Mahesh, Sundaresan Pillai Kamalam, Kumari, Leela Sandhya, Koshy, Peter
Format Journal Article
LanguageEnglish
Published Berlin WILEY-VCH Verlag 01.09.2011
WILEY‐VCH Verlag
Wiley-VCH
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Summary:Scheelite type red phosphors CaLa1–xNbWO8: xEu3+ (x = 0.01, 0.03, 0.05, 0.1, 0.15, 0.2, and 0.25) and CaLa0.8–yNbWO8: 0.2Eu3+, yBi3+(y = 0.1, 0.15, and 0.2) were prepared by conventional solid state reaction route. The crystalline structure, morphology and absorbance of these phosphors were characterized by powder X‐ray diffraction (XRD), scanning electron microscope (SEM), Fourier transform infrared (FT‐IR), and UV–Visible absorption spectroscopy. Investigations on their photoluminescent properties indicated that both Eu3+ doped and Eu3+, Bi3+ coactivated samples emit strong red light at 615 nm under both near UV (394 nm) and blue (465 nm) excitations. Bi3+ codoped system showed broadened charge transfer band (CTB) and stronger excitation peaks at 394 and 465 nm. The red emission intensity of CaLa0.8NbWO8: 0.2Eu3+ phosphor is improved by a factor of 2 as 20 mol% Bi3+ is introduced into the system, and is four times stronger than that of the commercial Y2O3:Eu3+ red phosphor. These phosphors are characterized by sharp red emission with color coordinates closer to the standard red phosphors. Thus, the above phosphors could be a promising red candidate for the phosphor converted white light emitting diodes (pc‐WLEDs).
Bibliography:ark:/67375/WNG-5BS791QK-D
Kerala State Council for Science
istex:EF7C9C82C4B6B840B858E98657A76E67E57A99FF
Technology and Environment (KSCSTE)
ArticleID:PSSA201026702
ISSN:1862-6300
1862-6319
DOI:10.1002/pssa.201026702