G. Seeta
Rama Raju
,
E.
Pavitra
,
Goli
Nagaraju
,
Xiang-Yu
Guan
and
Jae Su
Yu
*
Department of Electronics and Radio Engineering, Institute for Laser Engineering, Kyung Hee University, 1 Seocheon-dong, Giheung-gu, Yongin-si, Gyeonggi-do 446-701, Republic of Korea. E-mail: jsyu@khu.ac.kr; Fax: +82-31-206-2820; Tel: +82-31-201-3820
First published on 19th February 2015
Green color-emitting novel CaGd2ZnO5:Tb3+ (CGZO:Tb3+) nanophosphors were synthesized by a citrate sol–gel method. The structural and morphological properties were elucidated by X-ray diffraction and transmission electron microscope measurements. The photoluminescence properties of orthorhombic-phased CGZO:Tb3+ nanophosphors were studied as a function of Tb3+ ion concentration. The CGZO:Tb3+ nanophosphors revealed the enhanced broadband excitation between ultraviolet (UV)-B and UV-A regions. Under 317 nm excitation, even at dilute Tb3+ ion concentrations, only the emission transitions from 5D4 energy level were exhibited. This unusual behavior is due to the occurrence of nonradiative energy transfer via f–d transition rather than cross-relaxation process. The cathodoluminescence also showed similar behavior at low accelerating voltages. These luminescent powders are expected to find potential applications such as white light-emitting diodes and optical display systems.
To the best of our knowledge, no reports have been found so far on the luminescent properties of Tb3+ ions activated CGZO host lattice. In this work, we reported the structural and detailed luminescent properties of CGZO:Tb3+ nanophosphors by a facile sol–gel synthesis. This phosphor showed the broadened excitation region and provided green emissions almost similar to the commercial green phosphor. In order to explore its suitability for field-emission displays (FEDs), cathodoluminescence (CL) properties have also been studied.
Fig. 1 (a) XRD patterns of the CGZO nanophosphors doped with different concentrations of Tb3+ ions, (b) TEM image, and (c) SAED pattern of the CGZO:4Tb3+ nanophosphor. (In (a), the (h k l) planes are presented based on the ref. 16 and the inset shows the photographs of Tb3+ ions activated CGZO host lattices before and after annealing in reduced atmosphere). |
The XRD patterns of the CGZO:Tb3+ nanophosphors were recorded on Mac Science (M18XHF-SRA) X-ray powder diffractometer with CuKα = 1.5406 Å, and their morphological feature was observed by the field-emission transmission electron microscope (FE-TEM: JEOL JEM-2100F) images. Fourier transform infrared (FTIR) spectrum of the CGZO:Tb3+ nanophosphors was recorded on a thermo Nicolet-5700 spectrophotometer. The room-temperature photoluminescence (PL) spectra were measured by using a Photon Technology International (PTI, USA) fluorimeter with a Xe-arc lamp of 60 W power and the lifetime was measured with a phosphorimeter attachment to the main system with a Xe-flash lamp (25 watt power). For lifetime measurement, the start delay (0 μs) and end delay (4000 μs) with a count of 400 channels and 5 shots for each channel (average 3 times), an integration time of 50 μs, and a frequency of 10 Hz were used as parameters in the ph decay mode of PTI fluorimeter. The CL properties were measured by a Gatan (UK) MonoCL3 system attached with the scanning electron microscope (SEM: Hitachi S-4300 SE).
The presence of metal ions in the CGZO:4Tb3+ nanophosphor was also been confirmed by the FTIR spectroscopy. Fig. 2 shows the FTIR spectrum of the CGZO:4Tb3+ nanophosphor, which consists of the vibrational bands at 3641, 1415, 873, 712, 545, and 433 cm−1. The sharp band at 3641 cm−1 corresponds to the O–H stretching vibrational mode of the non-hydrogen bonded hydroxyl groups in the Ca(OH)2 and the moderate broadband at 1415 cm−1 is related to the asymmetric stretching vibration of O–C–O.18 The absorption peaks at 875 and 712 cm−1 belong to the symmetric and asymmetric bending vibrations of CO32− groups and the characteristic stretching vibration of Gd–O appeared at 545 cm−1.19,20 The band centered at 433 cm−1 is related to the Zn–O stretching vibration.21–23 The absorption spectrum of the CGZO:4Tb3+ nanophosphor is also shown in Fig. 2(b). The spectrum revealed absorption bands in the visible to UV-A, UV-B, and UV-C regions due to the absorption of CGZO host lattice also called the host absorption band (HAB) and the 4f7–5d1 transition of Tb3+ ions. These broad absorption bands offer a vast selection of possible excitation wavelengths between the UV and visible regions.24–26 The absorption behaviors between 200–250 and 360–550 nm are due to the host absorption and the broad band between 250 and 360 nm is due to the 4f7–5d1 transition of Tb3+ ions. The observed absorption bands are well in agreement with the PL excitation (PLE) spectra of CGZO host lattice (Fig. S1†) and CGZO:Tb3+ nanophosphors (Fig. 3(a)).
Fig. 2 (a) FTIR and (b) absorption spectra of the CGZO:4Tb3+ nanophosphor after annealing at 1000 °C in reduced atmosphere. |
Fig. 3(a) shows the PLE spectra of the CGZO:Tb3+ nanophosphors as a function of Tb3+ ion concentration by monitoring the emission wavelength at 541 nm. The PLE spectra are made of two groups of excitation bands with inter-configurational 4fn → 4fn−15d1 (f–d transition) and 4f intra-configurational transitions of Tb3+ ions along with the weak HAB. The HAB appeared between 200 and 250 nm. At dilute concentration, the sharp edge of the f–d transition at 314 nm is related to the (8S7/2 → 6P7/2) Gd3+ transition. However, at 5 mol% Tb3+ ion concentration, the HAB disappeared totally and the f–d transition exhibited the smoother peak with a band maximum at 317 nm, indicating that the possibility of efficient energy transfer from Gd3+ to Tb3+ ions. Besides, the second group consists of 4f intra-configurational transitions of Tb3+ ions located in the higher wavelength region, which appeared more pronouncedly with increasing the Tb3+ ion concentration. It is noted that the f–d transition of Tb3+ ions seems unlikely as it is broadened upto 30 and 40 nm from the previously reported Gd2O3:3Tb3+ (inset of Fig. 3(a)) and Y2O3:Tb3+ phosphors, respectively.20,27 The reason is that the f–d transition is related to the Tb3+ local environment and the 5d orbital is strongly influenced by the strength and symmetry of crystal field experienced by the active ions.28,29 The enhanced broadness hints that the CGZO:Tb3+ nanophosphors are a promising material for UV and NUV based lighting or optical display applications. For better understanding, the f–d transition of the CGZO:4Tb3+ nanophosphor was deconvolved by the Gaussian fitting, as shown in Fig. 3(b). There are four bands between the UV and NUV regions. The bands centered at 287 and 317 nm are related to the spin allowed (low spin) and spin forbidden (high spin) f–d transitions of Tb3+ ions, respectively. The bands located at 356 nm (7F6 → 5G5) and 376 nm (7F6 → 5D3) are ascribed to the intra-configurational 4f transitions. The band centered at 483 nm is related to the (7F6 → 5D4) transition (Fig. 3(a) and (b)). It is known that the low spin transition is more intense than that of high spin transition, but the contrary result was observed in this work. The reason behind this change is that the f–f transitions of Gd3+ and Tb3+ ions at 309 and 314 nm due to the (8S7/2 → 6PJ=7/2,5/2) and (7F6 → 5HJ=6,7) transitions, respectively, overlaid with each other and the high spin f–d transition covered all these transitions including the (7F6 → 5D0) transition of Tb3+ ions. The f–f transitions in the higher energy side of the excitation spectrum is unusual, and the detailed explanation about this unusual appearance was done in the earlier report.30 Briefly, the intra 4f transitions of Tb3+ ions in the shorter wavelength region obtain intensity when uneven components are mixed with the opposite parity wave functions (such as 5d) into the 4f wave functions. Therefore, the intensity of Gd3+ ion transitions increased due to the increased intensity of these Tb3+ ion transitions. As a result, the high spin f–d transition gained higher intensity than that of the low spin f–d transition of Tb3+ ions. This kind of result based on the f–d transition of Tb3+ ions was not reported so far. In view of the above result, we selected the 317 nm as the excitation wavelength for the emission measurements.
The PL spectra of the CGZO:Tb3+ nanophosphors as a function of Tb3+ ion concentration under 317 nm excitation are shown in Fig. 4(a). In the case of Tb3+ ions, usually, two groups of emission transitions appeared from the 5D3 and 5D4 energy levels, and the position of terbium ions is barely influenced due to the screen effect of 4f electrons, which are protected by its outer electron layer. However, in the present work, the PL spectra of the CGZO:Tb3+ nanophosphors exhibited the emission transitions at 482, 541, 580 and 620 nm corresponding to the 5D4→7FJ (J=6,5,4 and 3) transitions.31 No 5D3 emissions were observed even at dilute concentrations. This sort of result was also observed by Blasse et al.32 in the case of monoclinic Gd2O3:Tb3+ phosphors, indicating that the nonradiative transition occurs from 5D3 to 5D4 level via f–d transition instead of cross-relaxation process. This is possible only if the f–d transition appears in the low energy region (longer wavelength side). Due to this kind of nonradiative transition, the PL spectra exhibited mainly 5D4 emission bands even at dilute Tb3+ ion concentrations. Therefore, the CGZO:Tb3+ nanophosphors show the predominant green color from the magnetic dipole transition (5D4 → 7F5) at 541 nm, which can be explained by the large values of the reduced matrix element at J = 5 and the Judd–Ofelt theory.33,34 The Stark splitting in the emission peaks of Tb3+ ions is attributed to the effect of ligand field on terbium ions. It can also be found that the (5D4 → 7Fj) emission intensities of Tb3+ ions increased upto 4 mol% of Tb3+ ion concentration in CGZO host lattice due to the reduced loss of excitation energy. While the Tb3+ ion concentration increased over 4 mol%, the emission intensities decreases due to the concentration quenching, as shown in the inset of Fig. 4(a). The concentration quenching might be due to the excitation energy migration to the quenching centers. Furthermore, the decay profile for the 5D4 → 7F5 emission level of the CGZO:4Tb3+ nanophosphor under 317 nm excitation wavelength is shown in the Fig. 4(b). The results revealed that the decay curve was well fitted to a single exponential function of I = I0exp(−t/τ), where τ is the decay time. From the fitted curve, the calculated decay time of the CGZO:4Tb3+ was 1.37 ms.
Fig. 4 (a) PL spectra of the CGZO:Tb3+ nanophosphors as a function of Tb3+ ion concentration (inset shows the concentration quenching effect), and (b) decay curve of the CGZO:4Tb3+ nanophsophor. |
Fig. 5 shows the CL spectra of the CGZO:4Tb3+ nanophosphor as a function of (a) accelerating voltage and (b) filament current. The CL spectra revealed almost similar behavior except intensity. However, the CGZO:4Tb3+ nanophosphor showed weak emission bands in the blue wavelength region at the accelerating voltage of 5 kV (inset (i) of Fig. 5(a)). These bands were not observed in the PL spectra. This can be explained in view of the different mechanisms between CL and PL processes. In the PL process, UV or visible light based photons with the energy of only 4–6 eV are used. However, in the CL process, the fast energetic electrons are used from the anode voltage, which can be tuned from few electron volts to thousands of electron volts. So, the excitation energy on the dopant ion is much larger in CL than that in PL. However, the fast electrons as a high-energy particle always excite the host lattice. After being penetrated into the host lattice of a luminescent material, the fast primary electron will cause ionization and create many secondary electrons. The secondary electrons can also give rise to ionization and create more secondary electrons. These secondary electrons excite the host lattice and create many electron–hole pairs. Therefore, the high energy electron beam easily excite the HAB or charge transfer bands (CTB) of Tb3+ ions (O2− → Tb3+ (≈152 nm)) and (O2− → Gd3+ (≈155 nm)), which may be overlapped with each other. Due to the strong interaction with the crystal lattice, the excited electrons tend to relax from CT states via a multiple-phonon emission process to the lowest levels of 4f–5d states. Hence, at higher accelerating voltage, the transition probability from 4f–5d configuration to 5D3, and 5D4 metastable states is expected to be large as compared to the PL process. Furthermore, the intensity was increased with increasing the accelerating voltage (Fig. 5(a)) or filament current (Fig. 5(b)) due to the improved penetration depth by the recombination of increased excitons.35 Because of the deeper penetration depth, more activator ions were excited at almost all parts of the particles including boundaries, surfaces and inside of particles. The electron penetration depth for the CGZO:Tb3+ nanophosphors was calculated by the following formula:20,36
The Commission International De l'Eclairage (CIE) chromaticity coordinates of the CGZO:Tb3+ nanophosphor at the optimized concentration at 4 mol% from PL the spectrum and from the CL spectra as a function of accelerating voltage and filament current were calculated (the calculations were presented in the ESI†) and the selected chromaticity coordinates were represented in Fig. 6. The PL spectrum exhibited the CIE chromaticity coordinate of (0.305, 0.556). From the CL spectra, the CIE chromaticity coordinates were (0.319, 0.469), (0.305, 0.567), and (0.309, 0.568) at 1, 3, and 5 kV of accelerating voltage, respectively, under a fixed filament current of 55 μA. Slight variations in the coordinates were observed as a function of filament current, indicating (0.308, 0.570), (0.306, 0.569), and (0.309, 0.568) for 33, 45, and 55 μA, respectively. The calculated CIE chromaticity coordinates of the CGZO:4Tb3+ nanophosphor indicate better green color purity than those of available green phosphors such as Y2O3:Tb3+ (0.319, 0.597)37 and SrGa2S:Eu2+ (0.32, 0.63)38 and are also in close proximity to the European broadcasting union (EBU) used green (0.29, 0.60) coordinate.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c4ra15376f |
This journal is © The Royal Society of Chemistry 2015 |