Energy transfer and multicolor emission in single-phase Na5Ln(WO4)4−z(MoO4)z:Tb3+,Eu3+ (Ln = La, Y, Gd) phosphors

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

Received 26th April 2016 , Accepted 2nd May 2016

First published on 4th May 2016


Abstract

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+ (5D3,47FJ) and Eu3+ (5D07FJ), 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[thin space (1/6-em)]:[thin space (1/6-em)]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.


Introduction

Recently, the demand for novel red-emitting phosphors, especially that absorb in the near UV (350–400 nm), is gaining ever increasing importance.1 As one of the most frequently used red emitters in rare earth ion-doped materials, Eu3+ mainly presents high efficiency characteristic emissions related to the large energy gap between the emitting state 5D0,1,2 and the excited states 7FJ (J = 1, 2, 3, 4, 5) and offers an intense red composition. However, Eu3+-activated phosphors have narrow-line-shaped excitation peaks in the near UV region, which are not desirable for near UV LED application. In order to broaden the Eu3+ excitation band and improve the absorption efficiency, codoping Tb3+ with Eu3+ has been successfully employed in various hosts.2–5 Also, the Tb3+ ion-doped materials are often used as green phosphors due to the 5D47FJ (J = 6, 5, 4, and 3) transitions of Tb3+ ions. Therefore, it is hoped that dual emission might be realized in Eu3+/Tb3+ co-doped phosphors and the emission color is tuneable by adjusting the ratio of Tb3+ and Eu3+ ions.

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.

Experimental

Samples with the composition of Na5Ln1−xyTbxEuy(WO4)4−z(MoO4)z (0 ≤ x ≤ 1; 0 ≤ y ≤ 1; 0 ≤ z ≤ 4; Ln = La, Y, Gd) were synthesized via a simple Pechini method as follows. NaNO3 (Analytical Reagent, AR), H40N10O41W12·xH2O (AR), (NH4)6Mo7O24·4H2O (AR), La2O3 (99.99%), Y2O3 (99.99%), Gd2O3 (99.99%), Tb4O7 (99.99%), and Eu2O3 (99.99%) were used as the starting materials and were weighed in a proper stoichiometric ratio with an excess of 10% mole of W or Mo compensating for the evaporation loss. Rare earth oxides were dissolved in HNO3. These reagents were dissolved in deionized water, and an appropriate amount of CO(NH2)2 (AR) was added as fuel. The solutions were introduced into a muffle furnace maintained at 500 °C for 10 min. The as obtained mixed solid powders were ground thoroughly and reheated at various temperatures for 4 h in air. After firing, the samples were cooled to room temperature and reground for further measurements.

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.

Results and discussion

Crystal structure

The most suitable sintering temperature for the synthesis of single phase crystalline powders was investigated. Fig. 1a presents the XRD patterns of the sample Na5Tb0.5Eu0.5(WO4)4 sintered at different temperatures. The increase in the sintering temperature from 550 to 800 °C resulted in some differences of XRD intensity, which indicated that the sintering temperature can bring about significant influence on the crystallization of the samples. As shown in Fig. 1a, the samples obtained at 550, 600, 650, and 700 °C show the very similar XRD patterns. All the diffractions can be well indexed to pure tetragonal phase Na5La(WO4)4 (JCPDS no. 72-2157). With the increase in the sintering temperature, the intensity of the diffraction peaks increases. The intensity of peak at 29.13° of 700 °C is about 1.5 times that of 550 °C. The stronger diffraction peaks exist by virtue of the higher crystallinity. However, extra diffraction peaks centered at around 16.78°, 27.59°, and 32.50° form the impurity phases, which can be identified as Na2WO4, appear after annealing at 750 and 800 °C. Moreover, the XRD peak intensity of the tetragonal phase decreases as the sintering temperature was increased from 700 to 800 °C, while the intensities of the peaks for the Na2WO4 phase increase. This implies that the Na2WO4 crystalline phase formation may result from the dissolution of the Na5Tb0.5Eu0.5(WO4)4 crystalline phase, which is similar to that reported in the hosts such as Na5Ln(MoO4)4 (Ln = La, Y, Gd).7,10 We can conclude that the 700 °C is enough for the crystallization of as-prepared samples.
image file: c6ra10763j-f1.tif
Fig. 1 (a) XRD patterns of Na5Tb0.5Eu0.5(WO4)4 sintered at different temperature; (b) comparison of XRD profiles of typical Na5Ln1−xyTbxEuy(WO4)4−z(MoO4)z (Ln = La, Y, Gd) samples and the evolution on reflections near 2θ = 29°.

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, 2d[thin space (1/6-em)]sin[thin space (1/6-em)]θ = , 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.


image file: c6ra10763j-f2.tif
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.

Luminescence properties of Na5Ln(WO4)4:Eu3+ and Na5Ln(WO4)4:Tb3+ (Ln = La, Y, Gd)

The photoluminescence excitation (PLE) and emission (PL) spectra of Na5Tb(WO4)4 and Na5Eu(WO4)4 phosphors are shown in Fig. 3. The PLE spectrum (Fig. 3a, left) of Na5Tb(WO4)4 was recorded by monitored the green emission of Tb3+ 5D47F5 transition at 547 nm. The PLE spectrum consists of a strong and broad excitation band centred at 250 nm in the range of 200–300 nm, which corresponds to the charge transfer bands (CTB) of O2− → W6+ transitions,12 and spin-allowed 4f8 → 4f75d1 transitions of Tb3+ ions. In the range from 300 to 380 nm, Na5Tb(WO4)4 sample shows the characteristic f → f transitions of Tb3+: 7F65D2 transition for 353 nm, 7F65L10 transition for 360 nm, 7F65G5 transition for 371 nm, and 7F65G6 transition for 378 nm.13 Excited at 378 nm, the emission spectrum (Fig. 3a, right) shows typical emission lines of Tb3+ ion in the range of 480–700 nm. The emission lines are located at 491, 547, 585, and 624 nm, which are ascribed to the 5D47FJ (J = 6, 5, 4, and 3) transitions of Tb3+ ions, respectively. The green emission of 5D47F5 transition was found to be much stronger than that of 5D47F6,4,3. The energy absorbed by the WO42− group is transferred to Tb3+ levels nonradiatively, which is known as “host-sensitized”.14 Although the intensity of the CTBs is much stronger than that of Tb3+ 7F65G6 transition, the characteristic emission of WO42− is quenched completely and only the green-light emission of Tb3+ ions appears, revealing that the energy transfer from the WO42− group to Tb3+ is quite efficient in Na5Tb(WO4)4.
image file: c6ra10763j-f3.tif
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 (5F05D4), 384 nm (5F05L7), 394 nm (5F05L6), 418 nm (5F05D3), and 465 nm (5F05D2). The emission spectrum (Fig. 3b, right) consists of typical 4f levels specific transitions of Eu3+, that is, 5D05FJ (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 5D07F1 magnetic dipole transition of the Eu3+ ions, which is insensitive to the site symmetry. By contrast, the intensity of the 5D07F2 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 5D07F2 to 5D07F1) 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 5D3,47FJ transitions of Tb3+ ions. The emission peaks at 414 and 438 nm are attributed to the 5D37F5,4 transitions, while the emission peaks between 490 and 630 nm are ascribed to the 5D47F6,5,4,3 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 5D37FJ 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.


image file: c6ra10763j-f4.tif
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 (5D47F5 transition of Tb3+, λex = 378 nm; 5D07F2 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 5D07F2 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.


image file: c6ra10763j-f5.tif
Fig. 5 The concentration dependence of the peak intensity 5D47F5 of Tb3+ (a) and 5D07F2 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.

Multicolor tunable luminescence of Na5Ln(WO4)4:Eu3+/Tb3+ (Ln = La, Y, Gd)

Tb3+ ion can be used as green-emitting activator in commercial phosphors due to its predominant 5D47F5 transition, while the Eu3+ ion can be used as an activator of red emitting luminescent materials because the emission of the Eu3+ ion usually consists of lines in the red spectral area due to the 5D0 → 7FJ (J = 0, 1, 2, 3, and 4) transitions. In order to realize the multicolor tunable luminescence, Tb3+ and Eu3+ ions co-doped Na5Ln(WO4)4 (Ln = La, Y, Gd) phosphors were also prepared. Fig. 6 illustrates the PL spectra of Tb3+–Eu3+ doubly doped Na5La(WO4)4. Excited at 378 nm (7F65G6 of Tb3+), the characteristic sharp line emissions of Tb3+ and Eu3+ are both observed. Fig. 6a displays the variation of the PL spectra of Tb3+ and Eu3+ in the Na5La0.5−yTb0.5Euy(WO4)4 system with changing Eu3+ doping content (y). Here the Tb3+ content is fixed at 0.5. As the Eu3+ content increases, the PL intensity of Eu3+ increases at the expense of that of the Tb3+ ions. Therefore, we can speculate that the energy transfer from Tb3+ to Eu3+ occurs in the Na5La(WO4)4 host.
image file: c6ra10763j-f6.tif
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 5D07F2 of Eu3+ at 616 nm and 5D47F5 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.


image file: c6ra10763j-f7.tif
Fig. 7 The emission intensity of Tb3+ (5D47F5) and of Eu3+ (5D07F2) in phosphors Na5Ln0.5−yTb0.5Euy(WO4)4 (a) and Na5Ln0.9−xTbxEu0.1(WO4)4 (b) as a function of Eu3+ or Tb3+ concentration (λex = 378 nm).

Energy transfer mechanism in Na5Ln(WO4)4:Tb3+,Eu3+

An efficient energy transfer from Tb3+ to Eu3+ has been witnessed in various Na5Ln(WO4)4 hosts. In order to further demonstrate the ETTb→Eu process, the PL decay curves of Tb3+ emission of Na5La0.5−yTb0.5(WO4)4:yEu (y = 0–0.5) excited at 378 nm and monitored at 547 nm are shown in Fig. 8a. All decay curves can be well fitted by the first order exponential decay method using the formula:21,22
 
I(t) = I0[thin space (1/6-em)]exp(−t/τ) (1)
where I(t) and I0 are the luminescence intensities at time t and 0, and τ is the luminescence lifetime. The effective lifetime values were determined to be 0.740, 0.683, 0.436, 0.230, and 0.142 ms for Na5La(WO4)4:0.5Tb3+,yEu3+ with y = 0, 0.01, 0.1, 0.3, and 0.5, respectively. The lifetime of the Tb3+ ions decreases monotonically with an increase in the Eu3+ concentration, which can further confirm the existence of energy transfer from Tb3+ to Eu3+ ions. Therefore, the energy transfer efficiency ηET from Tb3+ to Eu3+ in Na5Ln(WO4)4 host can be calculated using the following expression:
 
ηET = 1 − τ/τ0 (2)
here τ0 and τ are the corresponding lifetimes of donor Tb3+ in the absence and presence of the acceptor Eu3+, and ηET is the calculation of energy transfer efficiency. As shown in Fig. 8b, the ηET value increases with increasing Eu3+ concentration, while the effective lifetime of Tb3+ decreases. The maximum energy transfer efficiency is about 91.7%, indicating that the ETTb→Eu process is quite efficient in the Na5La(WO4)4 host.

image file: c6ra10763j-f8.tif
Fig. 8 Decay time curves of Tb3+ in Na5La0.5−yEuyTb0.5(WO4)4 excited at 378 nm and monitored at 547 nm (a), and energy transfer efficiency from Tb3+ to Eu3+ and the lifetime of Tb3+ in Na5La0.5−yEuyTb0.5(WO4)4 (b).

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:

 
image file: c6ra10763j-t1.tif(3)
where V is the volume of the unit cell, χc is the total concentration of Eu3+ and Tb3+, and N is the number of host cations in the Na5Ln(WO4)4 unit cell. In this case, V = 1156.6 Å3 and N = 4. Since no concentration quenching exists in the compound Na5Ln(WO4)4 (Ln = La, Gd and Y), χc = 1. The distance RTb–Eu is determined to be about 8.2 Å, which is much larger than 5 Å, the critical distance of the exchange interaction.

According to Dexter's energy transfer formula and Reisfeld's approximation,25 the following relation can be obtained:

 
ln(τ0/τ) ∝ c and τ0/τcα/3 (4)
where ln(τ0/τ) ∝ c is corresponding to the exchange interaction; whereas α = 6, 8, 10, are dipole–dipole, dipole–quadrupole, and quadrupole–quadrupole interactions, respectively. The relationships are illustrated in Fig. 9a–d, respectively. The optimal linear relationship was obtained when α = 6, indicating that the energy transfer from Tb3+ to Eu3+ in Na5La0.5−yEuyTb0.5(WO4)4 occurs following a dipole–dipole interaction. This result agrees well with that reported on Tb3+ to Eu3+ energy transfer.26,27


image file: c6ra10763j-f9.tif
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.

Tunable luminescence properties of Na5Ln(WO4)4:Tb3+,Eu3+

Fig. 10a shows the luminescence photographs of Na5Ln0.5−yTb0.5Euy(WO4)4 (Ln = La, Y, Gd) powders with increasing the Eu3+ content (y) upon excitation with 365 nm from a UV lamp. When the Eu3+ content (y) is 0, the emission color of the phosphors is green. With increasing the Eu3+ content (y), the emission color can be tuned from green, green-yellow, and yellow, to red. This fact indicates that the tuning of the emission color from green to red can be realized in the Na5Ln(WO4)4:Tb3+,Eu3+ phosphors based on energy transfer. The CIE chromaticity diagram of the Na5La0.5−yTb0.5Euy(WO4)4 samples presented in Fig. 10b also support this result. The calculated CIE chromaticity coordinates (x,y) for Na5Ln0.5−yTb0.5Euy(WO4)4 samples are also listed in Table 1. The CIE coordinates vary systematically from green (x = 0.2935, y = 0.5994) to red (x = 0.6038, y = 0.3566) for Na5La0.5−yTb0.5Euy(WO4)4 samples with increase in the Eu3+ content (y). Table 1 also presents the CIE color coordinates (x,y) on its doping Eu3+ concentration in the Na5Ln0.5−yTb0.5Euy(WO4)4 (Ln = Y, Gd) samples under 378 nm excitation. Thus, for the series of Na5Ln0.5−yTb0.5Euy(WO4)4 (Ln = La, Y, Gd) phosphors, the emission color can be tuned from green to red by adjusting the ratio of Tb3+ and Eu3+. As given in Table 1, the CIE chromaticity coordinates (x,y) for Na5Ln0.9−xTbxEu0.1(WO4)4 samples with the changes of the Tb3+ concentration (y) are too close to be distinguished from each other in a chromaticity diagram. We measured the absolute quantum yields (QYs) of Na5La0.5Tb0.5(WO4)4 and Na5Tb0.5Eu0.5(WO4)4 samples. Under the excitation of 378 nm UV, the obtained values of absolute QYs are determined to be 76% and 91%, respectively. The luminescence properties of Na5Ln(WO4)4:Tb3+,Eu3+ (Ln = La, Y, Gd) phosphors indicate that the prepared samples may serve as single-component color-tunable phosphor in the fields of lighting and display devices.
image file: c6ra10763j-f10.tif
Fig. 10 Luminescence photographs of Na5Ln0.5−yTb0.5Euy(WO4)4 (Ln = La, Y, Gd; y = 0, 0.05, 0.1, 0.2, 0.4, 0.5) phosphors under 365 nm UV lamp (a); and CIE chromaticity diagram of the selected Na5La0.5−yTb0.5Euy(WO4)4 phosphors under 378 nm excitation (b).
Table 1 The CIE chromaticity coordinates (x,y) for Na5Ln(WO4)4:0.5Tb,yEu (0 ≤ y ≤ 0.5), Na5Ln(WO4)4:0.1Eu,xTb (0 ≤ x ≤ 0.9) and Na5La0.4Tb0.5Eu0.1(WO4)4−z(MoO4)z (0 ≤ z ≤ 4) samples excited at 378 nm
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)


The influence of W/Mo on the luminescence properties

Mo6+ and W6+ have similar ionic radius and can be substituted for each other. The sub-lattice structures around activators such as Tb3+ and Eu3+ will be somewhat changed. Therefore, the ratio of W to Mo is expected to have an impact on the luminescence properties. The emission spectra of as-prepared molybdotungstate samples with selected compositions of Na5La0.4Tb0.5Eu0.1(WO4)4−z(MoO4)z (z = 0, 1, 2, 3, 4) are recorded after excitation at 378 nm and are shown in Fig. 11a. Moreover, the variation trend of emission intensities of Tb3+ ions at 547 nm and Eu3+ ions at 593 and 616 nm are displayed in Fig. 11b. When W is gradually replaced by Mo, the emission intensities of Tb3+ and Eu3+ are both found to increase, reaching a peak at z = 2. The reason for the luminescence enhancement may be due to the advent of ion pair interaction between Tb3+ and Eu3+ ions, which is expected to be much stronger when Mo/W occupied bisection of the lattice sites separately. When the content of MoO42− is greater than that of WO42−, the emission intensities of Eu3+ and Tb3+ decrease simultaneously with increasing in the Mo/W ratio. The Mo6+ substitution of W6+ results in changing the sub-lattice structures around Tb3+ or Eu3+ ions, therefore, the luminescent properties are expected to be tunable. For the series of Na5La0.4Tb0.5Eu0.1(WO4)4−z(MoO4)z samples with different Mo/W ratios, the CIE (x,y) coordinates listed in Table 1 indicate that as the concentration of Mo increases, the value of x coordinate increases while y-value decreases and the chromaticity is shift slightly from red toward deep-red.
image file: c6ra10763j-f11.tif
Fig. 11 PL spectra of Na5La0.4Tb0.5Eu0.1(WO4)4−z(MoO4)z (z = 0, 1, 2, 3, 4) under 378 nm excitation (a), and the normalized intensities at 547, 593, and 616 nm as a function of the Mo content (z), respectively (b).

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

Conclusions

In summary, Na5Ln(MO4)4:Tb3+,Eu3+ (Ln = La, Y, Gd; M = W, Mo) solid solutions with scheelite-type structure were prepared using a simple Pechini method. The introduction of different rare-earth ions or replacement of W6+ by Mo6+ has no effect on the crystal structure. The concentration quenching of Tb3+ or Eu3+ ions does not occur, which is ascribed to the special structure of Na5Ln(MO4)4 hosts. The photoluminescence spectra, the decay curves, and the effect of the Eu3+/Tb3+ ratio have been used to investigated the energy transfer from Tb3+ → Eu3+. It is demonstrated that the luminescence of Eu3+ can efficiently sensitized by Tb3+ ions under NUV. Under 378 nm excitation, the emission color of Na5Ln0.5−yTb0.5Euy(WO4)4 (y = 0–0.5) phosphors can be tunable from green through yellow and eventually to red region by adjusting the ratio of Eu3+ and Tb3+. Moreover, the W/Mo ratio-dependence of luminescence shows that the emission intensities of both Tb3+ and Eu3+ were found to reach a maximum when the molar ratio of Mo/W was 2[thin space (1/6-em)]:[thin space (1/6-em)]2. These results indicate that Tb3+ and Eu3+-codoped Na5Ln(WO4)2(MoO4)2 phosphor can find application in the field of NUV-based WLEDs.

Acknowledgements

This research was financially supported by “the Fundamental Research Funds for the Central Universities”, South-Central University for Nationalities (CZY15002).

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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

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