Dan Qin and
Wanjun Tang*
Hubei Key Laboratory for Catalysis and Material Science, College of Chemistry and Material Science, South-Central University for Nationalities, Wuhan 430074, P.R. China. E-mail: tangmailbox@126.com; Fax: +86-27-67842752; Tel: +86-27-67842752
First published on 4th May 2016
A series of Tb3+ and/or Eu3+-doped Na5Ln(WO4)4−z(MoO4)z (0 ≤ z ≤ 4, Ln = La, Y, Gd) phosphors have been prepared via a simple Pechini method. X-ray diffraction (XRD) profile analyses have verified the formation of a single phase with scheelite-like structure. The scheelite-like tetragonal structure provides the Na5Ln(WO4)4 hosts the possibility of doping with Tb3+/Eu3+ ions without substantial luminescence quenching. Under near UV light excitation, Tb3+ and Eu3+-doped Na5Ln(WO4)4 phosphors exhibit characteristic emissions of Tb3+ (5D3,4 → 7FJ) and Eu3+ (5D0 → 7FJ), respectively. By codoping the Tb3+ and Eu3+ ions into the Na5Ln(WO4)4 host and tuning their relative concentration ratio, multicolor tunable emissions are obtained by varying the ratio of Tb3+/Eu3+. The energy transfer from Tb3+ to Eu3+ in Na5Ln(WO4)4 has been investigated by photoluminescence and decay measurements. The influence of W substitution by Mo on the luminescence properties of Na5Ln(WO4)4−z(MoO4)z:Tb3+/Eu3+ has also been investigated. Both the emission intensities of Tb3+ and Eu3+ ions were found to reach a maximum when the molar ratio of W/Mo was 2:
2. The results suggest that Na5Ln(WO4)4−z(MoO4)z:Tb3+/Eu3+ phosphors might find potential applications in the field of solid state lighting and field emission displays.
Alkali metal rare-earth molybdate and tungstate compounds of the general formula, A5Ln(MO4)4 (A = alkali metals; Ln = trivalent rare earth ion; M = Mo, W), have been reported to crystallize in the tetragonal crystal system with a scheelite-like structure.6 A5Ln(MO4)4 has been regarded as one class of hosts with high quenching concentration for high luminescence output, low sintering temperature, high efficiency matrix.7–9 These compounds containing tetrahedral anions such as MoO42− and WO42− were reported to be excellent phosphor hosts due to their high thermal and chemical stability, structural diversity, and capacity of hosting rare earth. The doping content of rare earth can be up to nearly 100%, in other words, the sites of Ln (Ln = La, Y, Gd) can be completely replaced, which means that this kind of matrix is unquenched. The reason is that the bond angles of O–M–O and Eu–O–M in the A5Ln(MO4)4 structure are 105 and 100°, respectively, resulting in the long distance between the sensitizer ions, which hinders the energy transfer occur between rare earth ions. Recently, Eu3+ activated A5Ln(WO4)4 phosphors with scheelite structure have gained much attention due to their good optical properties, high chemical stability, and a relatively simple preparation.7–10 However, the luminescence properties of Tb3+ doped A5Ln(WO4)4 have received less attention, especial for Tb3+/Eu3+ codoped A5Ln(WO4)4. To the best of our knowledge, the tunable luminescence properties of Na5Ln(WO4)4:Tb3+,Eu3+ phosphors have not yet been reported in the literature. Here, we synthesized Tb3+/Eu3+ singly doped or codoped Na5Ln(WO4)4 phosphors, and investigated their luminescence and energy transfer properties in detail. We found that their emission color can be tuned from green to yellow and red by increasing the ratio of Eu3+/Tb3+. Energy transfer mechanism between Tb3+ and Eu3+ ions in Na5Ln(WO4)4 hosts was discussed. What is more, the similar ionic radii of tetrahedral Mo6+ (0.41 Å) and W6+ (0.42 Å)11 may make it possible to prepare solid solutions of the scheelite-type Na5Ln(WO4)4−z(MoO4)z (0 ≤ z ≤ 4). Hence, we can expect that the progressive substitution of W in Na5Ln(WO4)4 hosts by Mo leads to change in the luminescence property. With this in view, a series of Na5La(WO4)4−z(MoO4)z:Tb3+/Eu3+ phosphors were synthesized and the influence of the W/Mo ratio on the structure and luminescent properties have also been studied.
Powder X-ray diffraction (XRD) measurement was performed on a Bruker D8 X-ray diffractometer (Bruker Co. Ltd., Karlsruhe, Germany) to check the phase purity of the as-prepared samples. The photoluminescence emission (PL) and excitation (PLE) spectra were recorded using a fluorescence spectrophotometer (F-7000, Hitachi, Japan) equipped with a 150 W xenon light source. The decay curves were collected on an Edinburgh FLS920 combined fluorescence lifetime and steady state spectrometer (Edinburgh Instruments Ltd, Edinburgh, England) with a 450 W xenon lamp and 60 μF flash lamp, respectively. The quantum yield (QY) was measured using the integrating sphere on the FLS920 fluorescence spectrophotometer. For comparison, all measurements were carried out at room temperature with the identical instrumental parameters.
Fig. 1b presents the XRD patterns of Na5Eu(WO4)4, Na5Tb(WO4)4, Na5Tb0.5Eu0.5(WO4)4, Na5La0.4Tb0.5Eu0.1(WO4)2(MoO4)2 and Na5Ln0.7Tb0.2Eu0.1(WO4)4 (Ln = La, Y, Gd) samples obtained after sintering at 700 °C. These samples show the very similar XRD patterns. Obviously, all the diffraction peaks can be well assigned to the corresponding standard data for the tetragonal phase of Na5La(WO4)4, indicating no phase transformation or structural variation occurs in the host upon Eu/Tb doping or W substitution by Mo. The strong and sharp diffraction peaks of the samples indicate that the as-obtained samples are well crystallized. The results show that different rare earth concentrations do not result in any other phase except for the main phase. The panel on the right in Fig. 1b shows the reflection peak near 29° (2θ). We find that the characteristic diffraction peak (132) of Na5Gd0.7Tb0.2Eu0.1(WO4)4 and Na5Y0.7Tb0.2Eu0.1(WO4)4 shifts obviously to higher angles with that of Na5La0.7Tb0.2Eu0.1(WO4)4. The effective ionic radii for eight-coordinated La3+, Y3+, Gd3+, Eu3+, and Tb3+ are 1.16, 1.019, 1.053, 1.066, and 1.04 Å,11 respectively. According to Bragg's law, 2dsin
θ = nλ, where n is an integer, λ is the wavelength of X-ray, d is the spacing between the planes in the atomic lattice, and θ is the angle between the incident ray and the scattering planes. Shrinkage of the lattice volume (d) will lead to the increase of the 2θ value. As shown in Fig. 1b, the 2θ value of the (132) peak is 28.78° for the Na5La0.7Tb0.2Eu0.1(WO4)4 sample. When La3+ is replaced by the smaller Gd3+ and Y3+ ions, the volume shrinks and the 2θ value increases to 29.11° and 29.25°, respectively. In addition, the 2θ value of the (132) increases from 29.06° (x = 0) to 29.07° (x = 0.5) and further to 29.12° (x = 1) for Na5Eu1−xTbx(WO4)4 samples. This variation could also be due to the different ionic radii for Eu3+ and Tb3+. The Na5La0.4Tb0.5Eu0.1(WO4)2(MoO4)2 sample is still single phase with good crystalline nature, suggesting that Na5Ln(WO4)4−z(MoO4)z samples with different W/Mo ratios can form a single phase due to the almost identical ionic radius of Mo6+ (0.41 Å) and W6+ (0.42 Å). Therefore, the as-prepared Na5Ln(WO4)4−z(MoO4)z (Ln = La, Y, Gd, Tb, Eu; 0 ≤ z ≤ 4) phosphors share the same scheelite structure with the space group I41/a.
Fig. 2 depicts the crystal structure of tetragonal Na5Ln(WO4)4 (along the c axis), as well as the coordination condition of metal cations. There are two nonequivalent Na+ lattice sites. One Na+ lattice sites (Na1) is coordinated by four O2− ions. The other one (Na2) is six-fold coordinated by six O2− ions. The W6+ ions are surrounded by four oxygen ions and form WO4 tetrahedron. The Ln3+ lattice sites, isolated from each other, are eight-coordinated to O2− ions to form LnO8 dodecahedron. In view of the similar ion radius and identical valence, the Eu3+/Tb3+ and Mo6+ ions are expected to occupy the crystallographic sites of Ln3+ and W6+ ions, respectively, in the Na5Ln(WO4)4 crystal host.
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Fig. 2 The crystal structure of Na5Ln(WO4)4 (Ln = La, Y, Gd) (along the c axis), as well as the coordination condition of metal cations. |
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Fig. 3 The PL excitation and emission spectra of the as prepared Na5Tb(WO4)4 (a) and Na5Eu(WO4)4 (b). |
Monitored at 616 nm, the PLE spectrum of (Fig. 3b, left) of Na5Eu(WO4)4 comprises of a broad band at 220–300 nm and some sharp lines between 360 nm and 480 nm. The weak broad excitation band exhibits two absorption peaks centred at 228 and 260 nm, respectively. The excitation band peaked at about 228 nm is ascribed to a charge-transfer band (CTB) of O2− → W6+ transition within the WO42− group. The excitation band peaked at longer wavelength (260 nm) correspond to the CTB of O2− → Eu3+ transition. This phenomenon is similar to CTBs of O2− → W6+ and O2− → Eu3+ transitions in Eu2(WO4)3 (ref. 15) and (Ca,Eu)WO4.16 In the spectral region from 360 to 480 nm, the PLE spectrum shows characteristic intra-configurational 4f → 4f transition of Eu3+: 364 nm (5F0 → 5D4), 384 nm (5F0 → 5L7), 394 nm (5F0 → 5L6), 418 nm (5F0 → 5D3), and 465 nm (5F0 → 5D2). The emission spectrum (Fig. 3b, right) consists of typical 4f levels specific transitions of Eu3+, that is, 5D0 → 5FJ (J = 0, 1, 2, 3, 4), which is ascribed to the emission peaks at 537, 592, 616, 655, and 704 nm, respectively. As well known, the emission at 593 nm is due to the 5D0 → 7F1 magnetic dipole transition of the Eu3+ ions, which is insensitive to the site symmetry. By contrast, the intensity of the 5D0 → 7F2 transition (616 nm) is strongly dependent on the surroundings of the Eu3+ ion because of its magnetic dipole character. Thus, the R/O ratio (emission intensity ratio of 5D0 → 7F2 to 5D0 → 7F1) strongly depends on the local symmetry of the Eu3+ ions in host lattice. The R/O ratio was calculated to be about 8.5, indicating that Eu3+ occupied the lattice site of noncentrosymmetric environment in the scheelite phases. Although no emission corresponding to tungstates is observed, the presence of CTB resulting from oxygen to tungstates in Fig. 3b has indicated that the energy absorbed by the WO42− group is transferred to Eu3+ levels nonradiatively, which is also known as “host-sensitized”.14
Since the properties are similar for La, Y, Gd, only the optical properties of Na5La1−xTbx(WO4)4 (0 ≤ x ≤ 1) and Na5La1−yEuy(WO4)4 (0 ≤ y ≤ 1) will be discussed in detail as a representative when Tb3+ or Eu3+ is doped in Na5Ln(WO4)4 host. Fig. 4a presents the PL spectra of Na5La1−xTbx(WO4)4 with different Tb3+ doping concentrations (x). Under 378 nm UV excitation, the PL spectra of the as-prepared Na5La1−xTbx(WO4)4 phosphors consist of the 5D3,4 → 7FJ transitions of Tb3+ ions. The emission peaks at 414 and 438 nm are attributed to the 5D3 → 7F5,4 transitions, while the emission peaks between 490 and 630 nm are ascribed to the 5D4 → 7F6,5,4,3 transitions. The PL spectra exhibit various ratios between the 5D3 and 5D4 emissions with changing Tb3+ concentrations (x). The emission intensity of 5D3 is continuously reduced, and the emission from the 5D4 level becomes dominant with increasing the Tb3+ concentration. The quenching of the emission from the 5D3 level is due to the cross-relaxation via the resonant energy transfer process: Tb3+ (5D3) + Tb3+ (7F6) → Tb3+ (5D4) + Tb3+ (7F0). The cross-relaxation effect becomes stronger with higher doping concentration (x), and the emission of 5D3 → 7FJ transitions quenches, resulting in the enhancement of the emission from the 5D4 to the 7FJ levels.17 Fig. 4b exhibits the PL spectra of Na5La1−yEuy(WO4)4 obtained by exciting with 394 nm light. The increasing concentrations of the Eu3+ ion bring no alteration in the shape of the PL spectra of the samples. No additional peaks or shifts in peak positions are observed, only the relative intensity changes.
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Fig. 4 The PL emission spectra of Na5La1−xTbx(WO4)4 (a) and Na5La1−yEuy(WO4)4 (b) samples under UV excitation of 378 and 394 nm, respectively. |
The dependences of the normalized PL intensities (5D4 → 7F5 transition of Tb3+, λex = 378 nm; 5D0 → 7F2 transition of Eu3+, λex = 394 nm) on the Tb3+ and Eu3+ concentrations are shown in Fig. 5a and b, respectively. The emission intensities of Na5Ln0.8Eu0.2(WO4)4 samples increase in the order of ILa < IGd < IY under the excitation of 394 nm. Considering the ionic radii of Y3+, Gd3+, La3+, and Eu3+,10 the ionic radii of Gd3+ and Eu3+ are closer than those of Y3+/La3+ and Eu3+, which induces a weaker local distortion in the lattice. The larger degree of disorder and the lower local symmetry of Eu3+ ions lead to an enhancement of the 5D0 → 7F2 transitions.18 This is the reason that the Eu3+ luminescence in Na5Gd0.8Eu0.2(WO4)4 is weaker than that in Na5Y0.8Eu0.2(WO4)4. The ionic radii increase in the order of Y3+ < Eu3+ < La3+, thus the Eu3+ ions have a stiff lattice environment in Na5Y0.8Eu0.2(WO4)4, but a loose one in Na5La0.8Eu0.2(WO4)4. The Eu3+ ion is strongly restricted by the surrounding in Na5Y(WO4)4 in comparison with that of Eu3+ in Na5La(WO4)4. More nonradiative relaxation occurs in Na5La(WO4)4 than that in Na5Y(WO4)4, thus the intensity of Na5Y(WO4)4 is higher than that of Na5La(WO4)4.19 In the samples with high Eu3+ ion doping concentration, the effect of ionic radii difference on the Eu3+ luminescence becomes unobvious.
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Fig. 5 The concentration dependence of the peak intensity 5D4 → 7F5 of Tb3+ (a) and 5D0 → 7F2 of Eu3+ (b) in Na5Ln(WO4)4 (Ln = La, Y, Gd). |
With increasing the doping content, the variation trend of emission intensity for Tb3+ or Eu3+ is similar. The emission intensity of Tb3+ or Eu3+ increases gradually with its concentration, and reaches a maximum at which the Ln3+ sites are replaced by Tb3+ or Eu3+ completely. This observation confirms that the concentration quenching of Tb3+ or Eu3+ never occurs in Na5Ln(WO4)4 host, so highly doping concentration samples are performed here. Usually, concentration quenching occurs because of pairing or aggregation of the identical luminescent centers at high concentrations, which lead to a small average distance and efficient resonant energy transfer between Eu3+–Eu3+ or Tb3+–Tb3+ ion pairs. In the compounds Na5Tb(WO4)4 and Na5Eu(WO4)4, the bond angles of O–W–O and Eu/Tb–O–W are 105° and 100°,20 respectively, resulting in the long distance between Eu3+–Eu3+ or Tb3+–Tb3+ ion pairs, which blocks energy transfer between ion pairs. Thus, the special scheelite-like tetragonal structure provides these Na5Ln(WO4)4 hosts for the possibility of doping with a high concentration of Tb3+/Eu3+ ions without concentration quenching.
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Fig. 6 The PL spectra of the phosphors Na5La0.5−yTb0.5Euy(WO4)4 (y = 0–0.5) (a) and Na5La0.9−xTbxEu0.1(WO4)4 (x = 0–0.9) (b) under 378 nm excitation. |
Fig. 6b shows the PL spectra of Na5La0.9−xTbxEu0.1(WO4)4 with different Tb3+-doping concentrations. Excited at 378 nm, the intense characteristic emission peaks of Tb3+ and Eu3+ can both be observed in the emission spectra of all samples. The PL intensity of Eu3+ dramatically increases with increasing Tb3+ concentration (x). And both emission intensities of Tb3+ and Eu3+ are increased with increasing the Tb3+ content when x = 0.9. All these results can validate the efficient energy transfer from Tb3+ to Eu3+.
The Na5Ln(WO4)4 samples in which all of the Ln sites are substituted by La3+, Y3+ and Gd3+ cations are investigated. The PL spectra of the Na5La0.5−yTb0.5Euy(WO4)4 and Na5La0.9−xTbxEu0.1(WO4)4 (Ln = La, Y, Gd) phosphors are illustrated in Fig. S1–S6 (in the ESI†), respectively. The variation of the normalized peak intensity 5D0 → 7F2 of Eu3+ at 616 nm and 5D4 → 7F5 of Tb3+ at 547 nm in Na5Ln0.5−yTb0.5Euy(WO4)4 system with various Eu3+ doping concentrations (y) are shown in Fig. 7a. Here the Tb3+ concentration is fixed at 0.5 as the Eu3+ concentration (y) increases; the emission intensity of Eu3+ is enhanced clearly whereas the section of Tb3+ is decreased. As shown in Fig. 7b, the variation trends of normalized intensity for Tb3+ and Eu3+ in the Na5Ln0.9−xEu0.1Tbx(WO4)4 system are similar. Both the Tb3+ and Eu3+ emissions are increased progressively with increasing the Tb3+ concentration (x). The concentration quenching effect is unobvious, which could be attributed to the weak interaction among the activators.
I(t) = I0![]() | (1) |
ηET = 1 − τ/τ0 | (2) |
It is well known that the energy transfer takes place via exchange interaction and/or multipolar interaction. The exchange interaction needs a large overlap between sensitizer and activator orbitals and the distances Rc between the sensitizer and activator is less than 5 Å. Otherwise, the electric multipolar interaction may dominate.23 As suggested by Blasse,24 the distance Rc between Tb3+ and Eu3+ ions in Na5Ln(WO4)4 hosts can be estimated by the following formula:
![]() | (3) |
According to Dexter's energy transfer formula and Reisfeld's approximation,25 the following relation can be obtained:
ln(τ0/τ) ∝ c and τ0/τ ∝ cα/3 | (4) |
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Fig. 9 Dependence of ln(τ0/τ) on cTb+Eu (a) and the dependence of τ0/τ on (b) cTb+Eu6/3, (c) cTb+Eu8/3 and (d) cTb+Eu10/3. |
Composition | CIE coordinates (x,y) | ||
---|---|---|---|
Ln = La | Ln = Y | Ln = Gd | |
Na5La0.5Tb0.5(WO4)4 | (0.2935,0.5994) | (0.2914,0.5953) | (0.3064,0.5892) |
Na5La0.45Tb0.5Eu0.05(WO4)4 | (0.3637,0.5395) | (0.3712,0.5277) | (0.3842,0.5192) |
Na5La0.4Tb0.5Eu0.1(WO4)4 | (0.4365,0.4769) | (0.4294,0.4768) | (0.4192,0.4859) |
Na5La0.3Tb0.5Eu0.2(WO4)4 | (0.5113,0.4258) | (0.5087,0.4280) | (0.5091,0.4271) |
Na5La0.1Tb0.5Eu0.4(WO4)4 | (0.5841,0.3746) | (0.5889,0.3703) | (0.5809,0.3715) |
Na5Tb0.5Eu0.5(WO4)4 | (0.6038,0.3566) | (0.6054,0.3566) | (0.6015,0.3562) |
Na5La0.9Eu0.1(WO4)4 | (0.4539,0.2765) | (0.5174,0.2888) | (0.5056,0.2888) |
Na5La0.8Tb0.1Eu0.1(WO4)4 | (0.3989,0.3300) | (0.3966,0.3381) | (0.3907,0.3363) |
Na5La0.7Tb0.2Eu0.1(WO4)4 | (0.3968,0.4166) | (0.3957,0.4171) | (0.3931,0.4220) |
Na5La0.1Tb0.8Eu0.1(WO4)4 | (0.4284,0.4988) | (0.4328,0.4964) | (0.4316,0.4865) |
Na5Tb0.9Eu0.1(WO4)4 | (0.4297,0.5011) | (0.4324,0.5009) | (0.4283,0.4877) |
Na5La0.4Tb0.5Eu0.1(WO4)3(MoO4) | (0.4467,0.4754) | — | — |
Na5La0.4Tb0.5Eu0.1(WO4)2(MoO4)2 | (0.4533,0.4706) | — | — |
Na5La0.4Tb0.5Eu0.1(WO4)(MoO4)3 | (0.4761,0.4453) | — | — |
Na5La0.4Tb0.5Eu0.1(MoO4)4 | (0.5469,0.3427) | — | — |
For Na5La0.4Tb0.5Eu0.1(WO4)4−z(MoO4)z samples, the values for R/O ratio vary from 5.84 for z = 0 to 8.61 for z = 4, which is in line with that reported for other scheelite related phosphors.28 Based on these values, we can expect that the degree of the local symmetry around Eu3+ ions decreases with increasing Mo proportion. Similar observation to change W/Mo relative ratio has also been witnessed in some systems such as M5Eu(WO4)4−x(MoO4)x, (M = Li, Na, K) (x = 0−4),9 CaGd2(1−x)Eu2x(MoO4)4(1−y)(WO4)4y (0 ≤ x ≤ 1, 0 ≤ y ≤ 1),29 and AgLa0.95Eu0.05(WO4)2−x(MoO4)x (x = 0–2).30
Footnote |
† Electronic supplementary information (ESI) available: Fig. S1 PL spectra of Na5La0.5−yTb0.5Euy(WO4)4; Fig. S2 PL spectra of Na5Y0.5−yTb0.5Euy(WO4)4; Fig. S3 PL spectra of Na5Gd0.5−yTb0.5Euy(WO4)4; Fig. S4 PL spectra of Na5La0.9−xTbxEu0.1(WO4)4; Fig. S5 PL spectra of Na5Y0.9−xTbxEu0.1(WO4)4; Fig. S6 PL spectra of Na5Gd0.9−xTbxEu0.1(WO4)4. See DOI: 10.1039/c6ra10763j |
This journal is © The Royal Society of Chemistry 2016 |