Tao Jiang,
Mingming Xing,
Ying Tian,
Yao Fu,
Xiumei Yin,
Hong Wang,
Xin Feng and
Xixian Luo*
Physics Department, Dalian Maritime University, Dalian, Liaoning 116026, PR China. E-mail: 13904119628@139.com
First published on 31st October 2016
Y2−xErxMo4O15 (x = 0.04, 0.08, 0.16, 0.32, 0.64, 2.0) phosphors were synthesised at 700 °C through a solid-state reaction method. The samples were characterised by XRD and emission spectra analysis. Y2−xErxMo4O15 samples showed a strong green emission (2H11/2, 4S3/2 → 4I15/2) and a weak red emission (4F9/2 → 4I15/2) under 1550 and 980 nm excitation. The green emission intensity was enhanced increasing the Er3+ ion doping content, whereas the red emission was basically unchanged. Thus, Er2Mo4O15 exhibited an abnormal green up-conversion luminescence without concentration quenching under 1550 and 980 nm excitation. The dominating green up-conversion luminescence was due to the larger adjacent Er3+⋯Er3+ distance caused by the special structure of Er2Mo4O15, which limited the energy-transfer process and cross-relaxation responsible for the red up-conversion emission. Therefore, the up-conversion luminescence mechanism was excited-state absorption under 1550 nm excitation.
Among them, Ln2Mo4O15 is a newly discovered rare-earth molybdate, so related research is scarce. Ln2Mo4O15 is characterised by drastic changes in the structure and performance with different rare-earth ion substitutions. The structure of Ln2Mo4O15 can be divided into three types: type I: Ln = La, monoclinic, space group P21/n;21,22 type II: Ln = Ce–Tb, triclinic, space group, P23,24 and type III: Ln = Dy–Lu and Y, monoclinic, space group P21/c.25,26 The structure of Er2Mo4O15 is shown in Fig. 1, which is similar to that of Y2Mo4O15, and the two compounds can form a continuous solid solution (Y2−xErxMo4O15, x = 0–2).1,27 Ln2Mo4O15 can be applied to optical electronics devices28–30 owing to its unique negative thermal expansion properties.31–35 Several studies can been found about the down-shift in luminescence, such as the Eu3+-doped R2Mo4O15 (R = Y, Gd, La)36–39 and Y2Mo4O15:xSm3+ (0.01 ≤ x ≤ 0.20),1 which can be applied to white LED. However, the UCL of Ln2Mo4O15 has not been reported yet.
In this paper, Er2Mo4O15 phosphors were synthesised using the conventional solid-state reaction method, and their UCL properties were characterised for the first time under 1550 and 980 nm excitation. The UCL mechanism was also analysed.
X-ray powder diffraction (XRD) was performed at 40 kV and 40 mA, with a D/MAX-Ultima X-ray generator employing Cu Kα radiation (λ = 0.15406 nm) over the 2θ range of 10° to 70°. The morphology of samples was examined by using a JEOL JSM-7001F thermal field emission scanning electric microscope (SEM). The particle size was analysed using a Coulter LS100Q laser diffraction particle size analyser. Diffuse reflectance spectra were measured using a Shimadzu UV-3600 UV/VIS/NIR spectrophotometer. The Fourier transform infrared (FTIR) spectra were recorded in KBr pellets using a Nicolet 550 Magna-IR spectrophotometer. A micro-Raman spectroscope (Jobin Yvon HR800, excited by 633 nm He–Ne laser with a laser spot size of 1 μm2, in line mapping mode) was adopted to measure the maximum phonon energy of the Er2Mo4O15 host lattice. Photoluminescence (PL) spectra and UCL spectra (200–900 nm) were recorded using a Hitachi F-4500 fluorescence spectrophotometer (slit width: 1 nm) equipped with a 1550 (0–700 mW, 0–3.2 A, CNI Laser, MDL-III-1550 nm) and 980 nm (0–800 mW, 0–1.2 A, CNI Laser, MDL-III-980 nm) fibre laser diode (LD). The scanning speed was 1200 nm min−1 and the power of the LD was measured with a laser power meter (LPE-type). The UCL brightness of the phosphors was recorded using a CS-100A luminance meter, and the LD was focused with a light beam area of about 1 mm2 before UCL brightness measurement.
Fig. 4 shows the FTIR and Raman spectra of the Er2Mo4O15 sample. The absorption bands at 750–960 cm−1 are attributed to the stretching vibration of tetrahedral [MoO4]. The absorption peaks at 1630 and 3500 cm−1 arise from the absorption of the O–H vibration (Fig. 4a). The Raman spectrum of rare-earth molybdates between 450–700 cm−1 is a blank area, and the stretching vibration tetrahedral [MoO4] is located between 700–950 cm−1.40 However, there are several peaks between 450–700 cm−1 in the Raman spectrum of the Er2Mo4O15 sample, which can be assigned to the characteristic peaks of the Er3+ ion (Fig. 4b).41 Therefore, the maximum phonon energy of the Er2Mo4O15 host lattice is ħω = 955 cm−1 (Fig. 4b).
Fig. 5 shows the diffuse reflectance spectrum and the PL spectrum of Er2Mo4O15 phosphor samples excited at 380 nm. The absorption peaks at 380, 407, 452, 490, 523, 546, 654, 799, 978 and 1505 nm are assigned to the transitions of 4I15/2 to 4G11/2, 2H9/2, 4F5/2, 4F7/2, 2H11/2, 4S3/2, 4F9/2, 4I9/2, 4I11/2 and 4I13/2 levels of Er3+ ions,42 respectively. Er2Mo4O15 shows broad and intense absorption peaks at 1500–1540 nm in the NIR region. The emission peaks were observed at 409, 467, 532 and 555 nm under 380 nm excitation, which can be attributed to the transition of Er3+ ions 2H9/2, 4F5/2, 2H11/2 and 4S3/2 level to 4I15/2 ground state, respectively. It means that Er3+ ions are excited to the 4G11/2 level by absorption of 380 nm photons, and they decay to the 2H9/2, 4F5/2, and 2H11/2/4S3/2 levels rapidly by non-radiative relaxation processes (e.g. 4G11/2 → 2H9/2, 2H9/2 → 4F3/2 → 4F5/2, 4F5/2 → 4F7/2 → 2H11/2 in the energy level diagram of Fig. 5b) and then return to the 4I15/2 ground state by producing 409, 467, 532, and 555 nm emissions, respectively. However, no red emission of Er3+ ions (4F9/2 → 4I15/2) between 640 and 680 nm was observed. It suggests that the non-radiative relaxation process 4S3/2 → 4F9/2 can hardly occur, and it is helpful for us to understand the UCL mechanism (Fig. 5b).
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Fig. 5 (a) Diffuse reflectance spectrum and (b) PL spectrum of Er2Mo4O15 (inset: energy level diagram of Er3+). |
Through pumping with a 1550 nm laser, Y2−xErxMo4O15 samples exhibited a bright green emission luminescence during day time as observed with the naked eye. Fig. 6a presents the UCL spectra of Y2−xErxMo4O15 (x = 0.08, 0.16, 0.32, 0.64, 2.0) samples with 1550 nm pumping. The spectrum is mainly composed of three emission bands: (1) the NIR emission band between 780–830 nm (NIR) belongs to the 4I9/2 → 4I15/2 transition of Er3+ ions. (2) The red emission band between 640–700 nm (R) belongs to the 4F9/2 → 4I15/2 transition of Er3+ ions. (3) The green emission band between 545–580 nm (G2) belongs to the 4S3/2 → 4I15/2 transition of Er3+ ions, and the green emission band located between 520–540 nm (G1) belongs to the 2H11/2 → 4I15/2 transition of Er3+ ions. The peak of the blue emission (2H9/2 → 4I15/2) located at 409 nm is very weak. The red emission band appeared in the UCL spectra compared with the PL spectra in Fig. 5b. The green up-conversion emission (2H11/2, 4S3/2 → 4I15/2) intensity was enhanced with the increase in Er3+ ion concentration under equivalent excitation conditions. Concentration quenching was not observed, even when the Y3+ ions were completely replaced by Er3+ ions (Fig. 6a). The relationship between the green up-conversion emission (4S3/2 → 4I15/2) intensity and the Er3+ doping concentration was linear (inset in Fig. 6a), indicating that the UCL mechanism of Y2−xErxMo4O15 was mainly ESA under 1550 nm excitation, which was different from the results of Meijerink et al.,43 who demonstrated that energy transfer (ETU) between Er3+ ions was responsible for the UCL in Gd2O2S:Er3+ under 1510 nm excitation even if the Er3+ ion concentration is only 0.1 mol%.
Fig. 7 shows the UCL spectra of the Er2Mo4O15 sample under 1550 and 980 nm excitation. Compared with the UCL spectrum excited at 1550 nm, Er2Mo4O15 phosphors showed similar emission peak positions and profiles under 980 nm excitation, whereas the components of red emission were enhanced significantly. Er2Mo4O15 phosphors demonstrated almost the same UCL brightness under a relatively low powered 1550 and 980 nm excitation (inset in Fig. 7). The brightness of Er2Mo4O15 under 1550 nm excitation was much greater than that under 980 nm excitation with increasing excitation power, suggesting that Er2Mo4O15 phosphors present higher UCL efficiency under the 1550 nm excitation. However, the UCL brightness of Er2Mo4O15 experienced a saturation effect under the higher excitation power of 1550 nm (>200 mW) (inset in Fig. 7).
As we can see from Fig. 8, the green emission intensity of Er2Mo4O15 rose rapidly with the increment in the excitation current of 1550 nm LD (and 980 nm LD), whereas the red emission almost remained unchanged. The increasing rate of green emission intensity was much faster than that of red emission with the same increment in excitation current. The ratio of green and red emission intensities (IG/IR) (inset in Fig. 8) also confirmed this observation. The IG/IR increased with the increment in excitation current of 1550 and 980 nm LD. The samples presented green emission when IG:
IR = 7.07
:
1 and 12.99
:
1, whereas at 0.5 and 1.1 A under 1550 nm excitation, the IG
:
IR were 3.12
:
1 and 7.87
:
1 under 980 nm excitation, respectively. The emission colour always focused on the green area with the increment in current, and the green emission was adjusted by changing the current. Such emission behaviour indicates that Er2Mo4O15 phosphors have quite good colour stability (Fig. 6b).
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Fig. 8 Green (IG) and red (IR) UCL intensity of Er2Mo4O15 phosphors versus excitation current of 1550 and 980 nm LD (inset: relationship between IG/IR and 1550 and 980 nm LD excitation current). |
The red emission component in the UCL spectra can be enhanced by increasing the doping concentration of Er3+ ions in conventional UCL materials under 980 nm excitation. For example, TiO2:Er3+, BaTiO3:Er3+ or Y2O3:Er3+ presented significant red emission, whereas dominating red emission was obtained by further increasing the concentration of Er3+ ions above 1 mol% due to the cross relaxation processes between Er3+ ions.44 Because of the small energy gap between the 4I9/2 and 4I11/2 levels, the 4F7/2 levels can be populated via a non-radioactive transition of 4I9/2 → 4I11/2 and a subsequent 4I11/2 + hν1550 nm → 4F7/2 transition. Moreover, in the condition 4I9/2 + hν1550 nm → 2H11/2, the 4S3/2 transition can hardly occur due to the short lifetime of the 4I9/2 level. Therefore, Er3+-doped UCL materials usually present high red emission under 1550 nm excitation. For example, M2O2S:Er (M = Y, Gd, La),45 Yb3+ and Er3+ co-doped Y2O2S,46 Y2O3,47 LaOCl48 and YOCl49 presented high colour purity red emission. The as-prepared Y2−xErxMo4O15 phosphor, even when Er2Mo4O15 was present, showed a dominating green emission under 1550 or 980 nm excitation that was independent of the amount of doping Er3+ ions. This abnormal result is obviously different from the above conclusion. A similar phenomenon can also be found in our previous study for NaY(WO4)2. Er3+ and Yb3+/Er3+ co-doped samples presented high purity green-coloured emissions whether under 1550 or 980 nm excitation when the optimum doping concentration of Er3+ of 24 mol% was used.50 Thus, this UCL mechanism is worthy of further research.
The UCL population mechanism can be further studied by determining the relationship between the up-conversion emission intensity and pump power, i.e.:
Iup ∝ Ipn | (1) |
Fig. 9 shows the double-logarithmic fitting of red and green UCL intensities (Iup) to excitation power (Ip) of the Er2Mo4O15 sample under 980 and 1550 nm excitation. The red (n = 1.36) and green (n = 1.80) emissions under the 980 nm excitation are the two-photon process. However, under 1550 nm excitation, the n value of the red and green emission changed with the increment in excitation power: the n value of green emission decreased from 2.07 to 1.72 with the increment in excitation power and the red emission also showed a similar trend due to the saturation effects. Similar results can also be observed in Y2O2S:Yb3+,Er3+.46
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Fig. 9 Dependence of UCL intensities of Er2Mo4O15 phosphor on pump power under 980 and 1550 nm excitation. |
The UCL mechanisms consist of ground state absorption (GSA), ESA, ETU and so on. For the green UCL mechanism of Er3+ ions doped systems under 980 nm excitation: GSA process 1, 4I15/2 + hν980 nm → 4I11/2, ESA or ETU process 2, 4I11/2 + hν980 nm → 4F7/2, non-radiation relaxation process 3, 4F7/2 → 2H11/2 → 4S3/2 and radiation process 4, 2H11/2, 4S3/2 → 4I15/2 + green emission. However, the red UCL mechanism of the Er3+ ions-doped systems was much more complex under the 980 nm excitation, and three possible mechanisms are responsible for red UCL: (1) non-radiation relaxation: 4S3/2 → 4F9/2, (2) non-radiation relaxation: 4I11/2 → 4I13/2 and subsequent 4I11/2 + hν980 nm → 4F7/2 transition and (3) cross relaxation process between Er3+ ions. Few UCL mechanisms have been reported under the 1550 nm excitation.
According to the Miyakawa–Dexter theory, the rate of multiphonon relaxation is dependent upon the energy gap separating the upper and lower states. The rate of the multiphonon relaxation (ωP) can be expressed as:51
![]() | (2) |
The 4f shell of rare-earth ions is shielded by the outermost layer 5s and 5p, and the matrix material possesses a relatively small impact on 4f electron transitions. The difference between the energy level data of Er3+ ions in different matrix material was small. On the other hand, the shape and peaks of Er2Mo4O15 UCL spectra were similar to those of Y2O2S:Yb3+,Er3+ (Fig. 8).52 Therefore, we inferred the energy level data of Er3+ ions in Er2Mo4O15 from that in Y2O2S:Er3+.53 The energy gap ΔE of Er3+ ions 4S3/2–4F9/2 and 4I11/2–4I13/2 was 2980 and 3400 cm−1, respectively, and the ΔE/ħω was 3.1 and 3.6, respectively. Red emission (4F9/2 → 4I15/2) of Er3+ ions was not observed in the PL spectrum when the 4G11/2 level was pumped directly (Fig. 5b), indicating that the probability of non-radiation relaxation of 4S3/2 → 4F9/2 was quite low. Therefore, the probability of non-radiation relaxation of 4I11/2 → 4I13/2 was smaller than that of 4S3/2 → 4F9/2, according to the above energy gap law data; and the 4I13/2 + hν980 nm → 4F7/2 process was also not the major cause of red emission. Thus, cross relaxation between Er3+ ions was responsible for red UCL (4F9/2 → 4I15/2), which depended on the distance between Er3+ ions.
As can be observed from Fig. 1, the minimum distance between Er3+ ions in Er2Mo4O15 was 5.2680 Å, which can also be confirmed from the data for Y2Mo4O15.37 This minimum distance was much larger than the other matrix, for example, the shortest distances between the rare earth ions in β-NaYF4, Y2O2S, Y2O3 were 3.2344, 3.5751 and 3.5130 Å, respectively. Therefore, the luminescence energy transfer or diffusions were limited by the long distances between Er3+ ions that are based on a special structure, and which suppressed the cross relaxation between Er3+ ions and caused a weak red emission in Er2Mo4O15. The study by Fischer et al.54 shows that the average distance between Er3+ ions is 6.63 Å for β-NaYF4:0.25 mol Er3+ and 7.53 Å for Gd2O2S:0.1 mol Er3+. These data further support our results. In addition, Er2Mo4O15 is a compound oxide, and the Er3+ ions account for only 9.5% of the total number of atoms, which is another possible reason for the absence of UCL quenching.
In this system, Er2Mo4O15 showed a strong green emission under 1550 nm excitation, and its UCL mechanism can be speculated from the above analysis (Fig. 10). For the green emission process:
GSA: 4I15/2 + hν1550 nm → 4I13/2 process (1) in Fig. 10 |
ESA: 4I13/2 + hν1550 nm → 4I9/2 process (2) in Fig. 10 |
ESA: 4I9/2 + hν1550 nm → 2H11/2, 4S3/2 process (3) in Fig. 10 |
For the red emission process:
GSA: 4I15/2 + hν1550 nm → 4I13/2 process (1) in Fig. 10 |
ESA: 4I13/2 + hν1550 nm → 4I9/2 process (2) in Fig. 10 |
Non-radiation relaxation: 4I9/2 → 4I11/2 |
ESA: 4I11/2 + hν1550 nm → 4F9/2 process (4) in Fig. 10 |
The NIR emission intensity of Er2Mo4O15 was much stronger than that of Y2O2S:Yb3+,Er3+, as shown in Fig. 7, which was the probable reason for the weak red UCL in Er2Mo4O15 under the 1550 nm excitation.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c6ra21580g |
This journal is © The Royal Society of Chemistry 2016 |