Color tunable emission from Eu3+ and Tm3+ co-doped CsPbBr3 quantum dot glass nanocomposites†
Received
3rd November 2021
, Accepted 6th December 2021
First published on 6th December 2021
Abstract
Cesium lead bromide (CsPbBr3) quantum dots (QDs) have shown great potential in the field of luminescent materials owing to their superior optical and electrical properties. However, instability and lack of multicolor emissions resulting from the intrinsic nature of CsPbBr3 QDs are still the major challenge for their commercialization. Herein, Eu3+ and Tm3+ co-doped CsPbBr3 QD glass nanocomposites (GNCs) are successfully synthesized via traditional melt-quenching followed by a heat-treatment route to obtain tunable emission in a durable host material. Tm3+ ions are doped to blue-shift the main emission peak of CsPbBr3 QDs, while Eu3+ ions are incorporated to compensate for the red deficiency. Accordingly, a tunable color emission spanning the entire visible spectrum is achieved from GNCs with a fixed composition. The incorporation of Eu3+ and Tm3+ ions promotes the crystallization of CsPbBr3 QDs in the glass host resulting in ∼100% photoluminescence quantum yield (PLQY) using a dilution method. The selected glass host has also been proven to effectively protect CsPbBr3 QDs against chemical, thermal and photo degradation. Interestingly, the selected Eu3+/Tm3+ co-doped CsPbBr3 QD GNC shows warm-white light with a low color temperature of 3692 K without utilizing any commercial phosphors. This indicates that the produced GNCs have the potential to be used as light convertor materials in multi-color LED or warm white LED applications due to their robust stability and extremely pure and tunable emission colors.
1. Introduction
All-inorganic CsPbX3 (X = Br−, Cl−, and I−) perovskite quantum dots (QDs) have significantly contributed to the development of cutting-edge products in many fields including optoelectronics,1,2 photovoltaics,3,4 sensing,5,6 and photocatalysis7,8 owing to their superior properties such as high photoluminescence quantum yield (PLQY), excellent color purity (narrow full-width at half maximum) and tunable emission color (with a tunable band gap).9–12 Among different perovskite QDs, brilliant green-emitting bromide-based perovskites (CsPbBr3 QDs) step forward especially for backlit displays13 and green-emitting LEDs14,15 because of the hypersensitivity of the human eye to green light.13 Despite the unique optical and electronic properties of solution-processable perovskite QDs, their notorious chemical, thermal and photo stability causing them to degrade when exposed to humidity, light or elevated temperatures near 150 °C pose a serious challenge to their commercialization.16–18 Despite the fact that many methods have been explored for improving the long-term stability of perovskite QDs, e.g., surface passivation,18 integration of various polymeric or inorganic host materials19,20 and ion co-doping,21 none of them have provided adequate protection. Furthermore, the synthesis of high-quality colloidal perovskite QDs necessitates a sophisticated reaction setup such as an inert environment as well as time-consuming preparation operations that ultimately results in high cost and difficulty of commercial application.22 In this regard, perovskite QD glass nanocomposites (GNCs) shine as the most effective approach to further improve long-term stability since the high rigidity and stability of the glass structure ensures that the QDs are effectively protected under environmental conditions.23–28
The lack of red and blue emitting components in CsPbBr3 QD GNCs, however, limits the color tunability of their emission and makes it difficult to incorporate them into novel applications. The doping of lanthanide ions (Ln3+) together with CsPbBr3 QDs allows further control of optical and electronic properties of QDs such as broadening their emission color into the desired spectral region and improving their PLQY values.29,30 Among different Ln3+ ions, Eu3+ ions – a well-known ideal red-emitting center with narrow linewidth ascribed to 5D0 → 7FJ (J = 0, 1, 2, 3, 4) transitions – have demonstrated promising improvements in performance and color tunability of CsPbBr3 QD GNCs.31 Until now, the strong red emission of Eu3+ coupled with green-emitting CsPbBr3 QD GNCs demonstrated promising potential in a variety of applications, including multicolor LEDs,32 white-LEDs,29,33 and X-ray imaging.34 However, in most of the existing studies emission color of Ln3+-doped QDs is controlled by adjusting the lanthanide concentration. For instance, Yuan et al. achieved multicolor LED fabrication by combining the Eu3+-doped CsPbBr3 QD GNCs with a UV chip. When the Eu3+ concentration is increased from 0 to 1.44, and 3.18 (mol%) multi-color emission from green to orange, and red is achieved under 365 nm illumination.32 Hence, a further study is urgently required to acquire a better understanding of how to improve the emission properties and produce multiple colors from Ln3+-doped CsPbBr3 QD GNCs at fixed lanthanide concentration.
In this work, highly stable and tunable Eu3+ and Tm3+ co-doped CsPbBr3 QD GNCs are successfully synthesized for the first time through a conventional melt-quenching method followed by controlled heat-treatment. Tm3+ ions are chosen to shift the main emission peak of CsPbBr3 QDs to shorter wavelengths as well as to be used as a blue light source.35 Eu3+ ions, on the other hand, are selected for compensating the red deficiency to obtain a broader emission spectrum. The incorporation of Eu3+ and Tm3+ ions to CsPbBr3 QD GNCs not only enriches the luminescence characteristics of QDs but also allows them to crystallize easily in the glass matrix. By rigorously controlling the heat-treatment temperature or time, tunable emission colors (from blue to cyan, violet, red, green, and eventually white) are achieved under UV excitation at a fixed lanthanide concentration. Ultimately, these findings suggest that Eu3+/Tm3+ co-doped CsPbBr3 QD GNCs – that show high thermal, chemical, and photo-stability features together with outstanding and widely tunable emission colors – are suitable candidates for new type warm light sources or multicolor LEDs.
2. Experimental studies
2.1. Sample preparation
Eu3+ and Tm3+ co-doped CsPbBr3 QD GNC samples with a nominal composition of 5CaO–12ZnO–2Al2O3–30B2O3–(35−x−y)SiO2–(6NaBr–7Cs2O–3PbBr2) + xEu2O3, yTm2O3 (x = 0–1.25; y = 0–0.75 in mol%) are synthesized via the conventional melt-quenching route and subsequent heat-treatment (for the crystallization of CsPbBr3 QDs). High-purity raw materials of SiO2, H3BO3, ZnO, CaCO3, Al2O3, NaBr, Cs2CO3, PbBr2, Eu2O3, and Tm2O3 purchased from Sigma-Aldrich and Alfa Aesar are mixed and ground to fine powder by using an agate mortar and pestle to form a homogeneous mixture. The well-mixed raw materials are put into corundum crucibles and melted in a furnace at 1100 °C for 30 min under an air atmosphere. Afterwards, the obtained melt is poured into a pre-heated stainless-steel mold and pressed by another steel plate to obtain as-cast samples. Subsequently, the as-cast samples are annealed at 400 °C (lower than the crystallization temperature of CsPbBr3 QDs and the glass matrix itself) for 5 h in a muffle furnace to eliminate internal stresses resulting from rapid cooling, and then naturally cooled down to room temperature. Finally, Eu3+ and Tm3+ co-doped CsPbBr3 GNC samples are obtained through controlled heat-treatment (crystallization). After controlled crystallization, the GNC samples are cut and well-polished into small specimens with a thickness of ∼2 mm to obtain a high quality surface for optical measurements.
Here we present a series of experiments describing how to determine ideal lanthanide doping concentrations for a tunable emission color from current GNC samples. Briefly, when the doping concentrations of Eu3+ and Tm3+ are selected to be 1 and 0.75 mol%, respectively, undesirable self-crystallization of QDs occurs before applying any heat-treatment (see Fig. S1, ESI†). Although the self-crystallization of CsPbBr3 offers some favorable properties in terms of energy efficiency,36 it is not convenient in this study as it does not allow size control of CsPbBr3 QDs. Furthermore, when Eu3+ and Tm3+ doping concentrations are selected as 0.5 and 0.5 mol%, respectively, a red emission deficit arises from Eu3+ ions, resulting in failure of wide color tuning and ultimately white light emission. Eventually, optimum doping concentrations of Eu3+ and Tm3+ are determined to be 0.75 and 0.5 mol%, respectively and used throughout this study. After finding the ideal doping concentrations for Eu3+ and Tm3+, a series of GNC samples is prepared by heat-treating the as-cast sample at a fixed temperature of 500 °C for different times (2, 3, 4, 5 and 15 h). Based on these results, the as-cast sample is further heat-treated at 510 °C for 3 h (to achieve white light emission). Consequently, synthesized samples (undoped and Eu3+/Tm3+ co-doped QD GNCs) are coded according to their heat-treatment temperatures (i.e., 500 °C and 510 °C) and times (i.e., 2, 3, 4, 5, and 15 h), e.g., 500 °C/3 h (see Table 1).
Table 1 Band gap, particle radii and absolute PLQY values for prepared as-cast and GNCs
Eu3+/Tm3+ co-doped QD GNCs |
E
g (eV) |
Radii of QDs (nm) |
Absolute PLQY (%) (lexc: 365 nm) |
PLQY value observed in the as-cast sample is due to emission of Eu3+ and Tm3+ ions.
|
As-cast sample |
3.34 |
— |
9.37a |
500 °C/2 h |
3.30 |
2.05 |
9.95 |
500 °C/3 h |
2.59 |
3.45 |
15.02 |
510 °C/3 h |
2.56 |
3.59 |
18.02 |
500 °C/4 h |
2.54 |
3.71 |
19.48 |
500 °C/5 h |
2.51 |
3.90 |
21.50 |
500 °C/15 h |
2.45 |
4.40 |
96.75 |
Undoped (500 °C/15 h) |
2.46 |
4.35 |
84.61 |
2.2. Characterization studies
The final chemical composition of the selected as-cast sample is investigated through the energy dispersive X-ray spectroscopy (EDS) technique. A Zeiss EVO LS 10 SEM linked with the EDAX Element SDD system is used for EDS analysis. The electron beam is accelerated to 15 kV for EDS measurements. The K lines are used for characterization of B, Na, Al, Si, Ca, and Zn, the L lines for analysis of Cs, Eu, and Tm, and M lines for detection of Pb. The final chemical composition of the selected as-cast sample is calculated by taking seven different EDS spectra from different spots on the sample and the average of these measurements are given in wt% (see Table S1, ESI†). Differential thermal analysis (DTA) measurements are carried out using a PerkinElmer™ Diamond TG/DTA (with an error estimate of ±1 °C) instrument to investigate the thermal behavior of the as-cast sample. Accordingly, 25 ± 1 mg of the powdered sample is heated in a platinum pan at a heating rate of 10 °C min−1 under a nitrogen atmosphere to determine the glass transition (Tg) temperature. The amorphous nature of the as-cast sample and phase characteristics of the CsPbBr3 embedded GNC samples are identified via XRD measurements using a Philips/PANalytical X'pert Pro diffractometer with an average wavelength of Cu Kα1 and Cu Kα2 radiation (λ = 0.15418 nm, voltage: 45 kV, current: 40 mA) in the 2θ range from 10 to 80° with a scanning step size of 0.02°. The XRD peak positions and intensities of crystallized phases are compared with the PDF card files. The optical absorption spectra of samples are measured using PG T80+ UV-Vis spectrophotometer operated at a resolution of 1 nm in the wavelength range from 300 to 900 nm.
Subsequently, the optical bandgap (Eg) values are calculated using the Tauc relationship37 by extrapolating the linear part of the plot of (αhν)2versus hν – considering a direct transition between the valence and conduction band – where α is the optical absorption coefficient, and hν is the energy of the incident photon. Using the determined band gap values, the effective mass approximation (EMA) method is then utilized to calculate the crystallite sizes of CsPbBr3 QDs. EMA proposed by L. E. Brus is a well-known approach to calculate radii of small nanoparticles with respect to their measured band gap values.24,25,38
Hence, crystallite sizes of CsPbBr3 QDs is calculated through the EMA method according to the following relation:24,39
|  | (1) |
where
Eg,bulk (CsPbBr
3: 2.3 eV) is the bulk band gap,
r is the nanoparticle radius,

(CsPbBr
3: 0.15
me) and

(CsPbBr
3: 0.14
me) are effective mass of electron and hole, respectively.
40ε0 is the vacuum permittivity,
ε (CsPbBr
3: 4.797) is the relative permittivity, ℏ is Planck's constant, and
e is the charge of the electron.
41
Photoluminescence measurements are recorded on an Edinburgh Instruments FS5 fluorescence spectrophotometer equipped with a 150W xenon lamp as the excitation source having a high spectral resolution (signal to noise ratio of water Raman signal >6000
:
1). PLQY measurements are conducted with a signal to noise ratio of the water Raman signal greater than 6000
:
1 and 0.5 nm spectral resolution using same PL setup in an integrated sphere (150 mm internal spherical cavity, polytetrafluoroethylene coated) under a 365 nm excitation wavelength and evaluated by the following equation with an estimated error rate of ±5%24
|  | (2) |
where
Ereference and
Esample are the scattering intensities of excitation light not absorbed by the reference and the sample, respectively.
Lsample is emission intensity determined by integrating the area under the calibrated emission spectra. The difference in scattering integrated areas between the reference and the sample determines the number of absorbed photons.
PL emission spectra of samples are used to determine the colorimetric properties, such as Commission Internationale d'Eclairage (CIE) 1931 color coordinates, color rendering index (CRI), and correlated color temperature (CCT) by using OSRAM ColorCalculator through the equations explained in our previous study.42–44
Thermal, chemical and photo stability tests are carried out on a selected GNC sample heat-treated at 500 °C for 15 h. Accordingly, temperature-dependent PL measurements (thermal stability tests) are recorded up to 8 heating–cooling cycles by placing a Pike Technologies heated solid transmission attachment in the fluorescence spectrophotometer and by increasing the temperature from 25 °C to 250 °C and then cooling down to room temperature. The photostability is assessed by stimulating the sample under a 442 nm laser with power density of 5 W cm−2 up to 10 h and recording the PL emission at various time intervals. PL emission spectra are measured with a ±3% error rate. Chemical stability is investigated by immersing the selected GNC sample in deionized water for up to 45 days at room temperature and recording the corresponding PLQY value with an ±5% error rate to interpret the chemical effect of moisture on emission intensities at different time intervals.
3. Results and discussion
3.1. Thermal and structural analysis
The DTA result of the as-cast sample is used to determine the appropriate heat-treatment temperatures to form CsPbBr3 QDs in the glass matrix. As can be clearly seen in Fig. 1aTg is noted to be ∼485 °C. Accordingly, CsPbBr3 QDs are grown by heat-treating the as-cast sample to slightly above Tg at 500 °C (for 2, 3, 4, 5, and 15 h) and 510 °C (for 3 h). Fig. 1b reveals five diffraction peaks at 2θ values of 15.21°, 21.55°, 30.47°, 37.54°, and 43.66° attributed to the (100), (110), (200), (211) and (220) crystalline planes of cubic CsPbBr3, respectively (superimposed on the broad halo peak) for the samples heat-treated at 500 °C for 15 h (for both Eu3+ and Tm3+ co-doped and undoped GNCs) – evidencing that the QDs are successfully prepared in the glass matrix via heat-treatment.26,27 Importantly, the XRD diffraction peaks of the CsPbBr3 QD GNC sample heat-treated at 500 °C for 15 h become slightly more intense and sharper upon the doping of Eu3+ and Tm3+ ions. This is probably because the incorporation of Eu3+ and Tm3+ acts as a nucleating agent and facilitates the crystallization and growth of CsPbBr3 QDs in the glass matrix.34 The XRD pattern of the as-cast sample, on the other hand, exhibits diffuse scattering halo without any diffraction peaks due to its amorphous character.24 Meanwhile, GNC samples heat-treated at 500 °C for 2, 3, 4, 5 h and at 510 °C for 3 h also display the same broad halo peaks indicating that heat-treatment time is insufficient to induce complete crystallization of CsPbBr3 QDs. Hence, it can be concluded that the size of CsPbBr3 QDs in glasses increases with the increasing heat-treatment time.
 |
| Fig. 1 (a) DTA curve of the as-cast sample, (b) XRD patterns of the as-cast sample, undoped and Eu3+/Tm3+ co-doped CsPbBr3 QD GNCs. The vertical bars depict the diffraction data of the cubic CsPbBr3 phase (PDF No. 54-0752). Inset shows the zoomed in region of 2θ = 10–20° for the 500 °C/15 h sample to provide a clearer display of the (100) peak. | |
3.2. Optical absorption properties
The digital images of the as-cast sample and Eu3+/Tm3+ co-doped GNCs under daylight and their corresponding optical absorption spectra are illustrated in Fig. 2. As displayed in Fig. 2a, the as-cast sample is colorless and transparent. On the other hand, colors of GNCs change from very pale (except for the 500 °C/2 h sample) to vivid yellow with increasing heat-treatment time demonstrating the successful growth of CsPbBr3 QDs in the glass network. However, the absence of color change in the 500 °C/2 h sample indicates that the applied heat-treatment temperature and time is not enough to form CsPbBr3 QDs. The very pale-yellow colors observed in the 500 °C/3 h and 510 °C/3 h samples are probably due to the partial crystallization (or relatively small average size) of the CsPbBr3 QDs. This is consistent with the XRD patterns of the related samples (see Fig. 1b) in which diffraction peaks are not observed unless the heat-treatment is increased to sufficient temperatures or times. As represented in Fig. 2b, the absorbance spectra of samples display five absorption bands located at 358 nm (3H6 → 1D2 transition of Tm3+), 393 nm (7F0 → 5L6 transition of Eu3+), 465 nm (7F0 → 2D2 transition of Eu3+), 686 nm (3H6 → 3F2,3 transition of Tm3+), and 792 nm (3H6 → 3H4 transition of Tm3+).35,45–47 With increasing heat-treatment time (from 2 h to 3 4, 5, and 15 h) or temperature (from 500 °C to 510 °C) intensities of the absorption bands at 686 and 792 nm remain unchanged, while intensities of the absorption bands at 358, 393 and 465 nm disappear gradually. This is attributed to the crystallization of QDs causing the samples to change their color towards the red end of the visible spectrum. In addition, the exciton absorption peak of the CsPbBr3 QDs becomes observable in the 500 °C/3 h sample (indicated as number 4 on the graph given in Fig. 2b) and shifts towards the long wavelength region with increasing heat-treatment time or temperature. The redshift in exciton absorption proves the growth and increment in the mean size of CsPbBr3 QDs in the glass network – ultimately revealing the size and band gap modulation of QDs that is attributed to the quantum confinement effect.24,26,48 Accordingly, the band gap values (in the range of 2.45–3.34 eV) and estimated crystallite sizes (in the range of 2.05–4.40 nm) of the as-cast sample and CsPbBr3 QD GNCs are detailed in Table 1 and Fig. S2 (ESI†).
 |
| Fig. 2 (a) Digital images of as-cast and Eu3+/Tm3+ co-doped GNC samples under daylight and (b) corresponding optical absorption spectra. Red and blue colored vertical bars show the absorption band positions of Eu3+ (illustrated as numbers 2 and 3) and Tm3+ ions (illustrated as numbers 1, 5, and 6), respectively. Green arrow represents the exciton absorption peak of CsPbBr3 QDs. | |
3.3. Photoluminescence, color tunability and colorimetric properties
3.3.1. PL excitation measurements.
PL excitation (PLE) spectra of the selected sample (heat-treated at 510 °C for 3 h) are recorded by monitoring the characteristic emission bands of Eu3+, Tm3+ and CsPbBr3 QDs at 613, 453 and 500 nm excitation wavelengths, respectively (see Fig. S3, ESI†). PLE measurements are conducted to find the most appropriate excitation wavelength where the material emits its intense characteristic light. The excitation spectra of Eu3+ ions consist of various bands between 350 and 420 nm that are assigned to the 4f–4f transitions of Eu3+ ions.49 The strongest among them is located at 393 nm owing to the 7F0 → 5L6 transition (see Fig. S3a, ESI†). For Tm3+ ions, the main excitation band peak at 357 nm is attributed to the 3H6 → 1D2 transition50 (see Fig. S3b, ESI†). The main excitation peak of CsPbBr3 is detected at 375 nm corresponding to the band-to-band transition (see Fig. S3c, ESI†). Considering PLE results, 355, 365, 375, 385 and 395 nm are chosen as different excitation wavelengths to record the PL emission spectra and to demonstrate the tunable emission of samples.
3.3.2. Emission color modulation at different excitation wavelengths.
The PL emission spectra of samples are monitored by changing the excitation wavelengths from 355 to 365, 375, 385, and 395 nm. Accordingly, the CIE color coordinates of all samples excited with changing excitation wavelengths are given in Table S2 (ESI†). As shown in Fig. 3, changes in the excitation wavelength enable the color emission tunability of samples. For instance, as-cast and 500 °C/2 h samples with similar luminescence behavior exhibit blue and red emissions when the samples are irradiated with 355 nm (the wavelength at which Tm3+ ions are the most sensitive) and 395 nm (the wavelength at which Eu3+ ions are the most sensitive), respectively (see Fig. 3a, b, h and i). On the other hand, red, blue, and violet emission colors are obtained for 500 °C/3 h sample by changing the stimulation wavelength from 355 to 395 nm owing to the partial crystallization of QDs (see Fig. 3c and j). It is unambiguous that 500 °C/3 h is close to the white light coordinates (under 375 nm excitation) but an increase in green light intensity is still required to achieve pure white light emission. Hence, when the heat-treatment temperature increases to 510 °C, eventually a white light emission (owing to 481 nm and 500 nm centered emissions of CsPbBr3 QDs and red emission of Eu3+) is obtained under 375 nm (see Fig. 3h and h). On the other hand, the degree of color shifts in the 500 °C/4 h (see Fig. 3e and l) and 500 °C/5 h (see Fig. 3f and m) samples depending on excitation wavelength are relatively low due to suppression of Ln3+ emissions by partially crystallized QDs and these samples are in the bluish and cyan regions, respectively. Finally, CsPbBr3 QDs emission dominates the PL spectrum of the 500 °C/15 h sample and thus the characteristic emission of Eu3+/Tm3+ is almost suppressed although they are still observable (see Fig. 3g and n). This is ascribable to the high emission intensity of fully crystalline CsPbBr3 QDs that obscures the Eu3+ and Tm3+ emissions. A similar observation revealing that the Eu3+ emission intensity is barely observable due to the strong band-to-band emission of CsPbBr3 QDs is also reported in the literature.34
 |
| Fig. 3 PL spectra for the (a) as-cast sample, and (b) 500 °C/2 h, (c) 500 °C/3 h, (d) 510 °C/3 h, (e) 500 °C/4 h, (f) 500 °C/5 h and (g) 500 °C/15 h samples. The corresponding CIE color chromaticity diagrams for the (h) as-cast sample, and (i) 500 °C/2 h, (j) 500 °C/3 h, (k) 510 °C/3 h, (l) 500 °C/4 h, (m) 500 °C/5 h and (n) 500 °C/15 h samples under varying excitation wavelengths ranging from 355 to 365, 375, 385, and 395 nm. Vertical arrows show the emission peak position of Eu3+ (depicted in red), Tm3+ ions (depicted in blue), and CsPbBr3 QDs (depicted in green). | |
As demonstrated in Fig. S4a (ESI†), extremely intense green emission of CsPbBr3 QDs (heat-treated at 500 °C for 15 h) can be clearly seen even under ambient light. The PLQY value of the 500 °C/15 h sample is found to be 50.42% from the bulk glass under 365 nm excitation. Multiple re-absorption and re-emission processes are assumed to be responsible for the lower-than-expected PLQY value.13 Therefore, according to a method reported by Lin et al., the Eu3+/Tm3+ co-doped 500 °C/15 h GNC sample is ground into powder and mixed with non-luminescent Al2O3 for dilution to uncover the real PLQY value of the sample.13 Indeed, near-unity PLQY (96.75%) is obtained by repeated PLQY measurements (see Fig. S5, ESI†). Furthermore, almost identical PL intensities and emission wavelengths obtained from measurements on different parts of the sample demonstrate a homogeneous distribution of QDs in the glass (see Fig. S6, ESI†). Besides, the PLQY value of un-doped CsPbBr3 QD GNCs (84.61%) is lower than that of its doped counterparts confirming that Eu3+ and Tm3+ promote the nucleation of CsPbBr3 QDs in glass. Digital images and PL spectra of undoped CsPbBr3 QD GNC are also provided in ESI† (see Fig. S7). On the other hand, PLQY values for other samples including as-cast, 500 °C/2 h, 500 °C/3 h, 500 °C/4 h, 510 °C/3 h and 500 °C/5 h are obtained as 9.37, 9.95, 15.02, 18.02, 19.48, 21.50%, under 365 nm excitation, respectively (see Table 1). As a result, PL performance of GNCs is either higher or competitive/superior to the findings of previously reported CsPbBr3 QD GNCs,13,48 colloidal CsPbBr3 QDs9,51–53 or different nanocrystal embedded samples.54–56
3.3.3. Emission color modulation at a fixed excitation wavelength.
In a further experiment, all samples are excited at 375 nm to gain more insights into tunable color emission depending on a fixed excitation wavelength. Fig. 4a, b and c represent the PL spectra, digital images, and the corresponding CIE color chromaticity diagram of samples, respectively. Since the emission colors of lanthanides are independent of the applied heat-treatment, tunable color emission under the fixed excitation wavelength of 375 nm is obtained by adjusting the size and luminescence intensities of the CsPbBr3 QDs through heat-treatment. As can be clearly seen in Fig. 4a, emission peaks of CsPbBr3 QDs shift from 478 to 484, 495, and 512 nm as the heat-treatment time is increased from 3 to 4, 5, and 15 h, respectively. On the other hand, when the heat-treatment temperature is increased to 510 °C for 3 h, the PL spectrum of the related sample exhibits two emission peaks at 481 and 500 nm (see Fig. 4a). In addition, PL spectra reveal five apparent peaks of Eu3+ ions located at 577 nm, 590 nm, 613 nm, 653 nm, and 700 nm originating from the 5D0 → 7FJ (J = 0, 1, 2, 3, 4) transitions, respectively.46 Among these five transitions, the 5D0 → 7F2 transition (613 nm, red) rules over the emission spectra. However, emission peak at 454 nm ascribed to the 1D2 → 3F4 transition of Tm3+ exhibits very weak emission signal under 375 nm excitation.57,58 As seen in digital images and in the CIE color chromaticity diagram, heat-treatment time, and temperature both contribute to the emission color tuning (see Fig. 4b and c). In particular, the as-cast sample and 500 °C/2 h samples emit red light and when the heat-treatment time is increased to 3, 4, 5, and 15 h the samples emit violet, blue, cyan, and green light, respectively. Increasing the heat-treatment temperature to 510 °C for 3 h results in the sample emitting white light under 375 nm excitation with color coordinates (x = 0.3840, y = 0.3543) close to that of pure white light, a CRI of 30.7, and a CCT of 3692 K located in a warm white area. The reason behind this low CRI value is due to the insufficient blue emission that is naturally emitted by the sample compared to the commercial WLEDs based on blue LED-chips (450–460 nm) excited yellow-emitting phosphors. However, numerous recent studies have reported that narrowband LEDs with low CRI values resulted from the very sharp emission bands of RGB colors are desirable compared to broadband LEDs with high CRI values.59 In this regard, 510 °C/3 h GNC sample synthesized in the current study is comparable to its counterparts prepared by the same procedure. The CCT, CRI and CIE color coordinate values of recent studies on Eu3+-doped CsPbBr3 QD GNCs for solid-state-lighting are summarized in Table S3 (ESI†) for comparison purposes. In summary, contrary to previous studies suggesting that color emission is dependent on lanthanide concentration, this study shows that multicolor emissions from blue to cyan, violet, red, green, and white can be easily tuned in CsPbBr3 QD GNCs with constant Eu3+ and Tm3+ doping concentrations by meticulously tuning the heat-treatment parameters.
 |
| Fig. 4 (a) PL spectra, (b) digital images and (c) the corresponding CIE color chromaticity diagram for the as-cast sample and Eu3+/Tm3+ co-doped CsPbBr3 QD GNCs under 375 nm excitation. Vertical arrows in the PL spectra show the emission peak positions of Eu3+ (shown in red), and Tm3+ ions (shown in blue). The horizontal arrow represents the shift in the emission band of CsPbBr3 QDs. The digital images of the samples are taken under a 375 nm LED chip, whereas those given as the inset in the CIE color chromaticity diagram are taken by fixing the wavelength of a xenon lamp on the PL spectrophotometer at 375 nm. | |
3.4. Chemical, photo, and thermal stability investigations
Chemical, photo and thermal stability features are critically important in the practical applications of QDs for solid state lighting. To demonstrate the benefits of incorporating CsPbBr3 QDs into a glass matrix chemical and photo stability tests and temperature-dependent PL measurements including heating–cooling cycles are performed with the selected 500 °C/15 h sample. Chemical stability of the selected GNC sample is assessed by storing it in water and monitoring its PLQY value at different intervals up to 45 days (see Fig. 5a). No noticeable decrease in PLQY of the selected GNC sample is observed even after 45 days of storage in water revealing that the rigid nature of glasses inhibits possible chemical reactions between the QDs and the external environment.
 |
| Fig. 5 Stability tests of selected Eu3+/Tm3+ co-doped CsPbBr3 QD GNCs heat-treated at 500 °C for 15 h. (a) Chemical stability test by immersion in water up to 45 days, (b) photo stability test by excitation at 442 nm laser with 5 W cm−2, (c) temperature-dependent PL intensity, and (d) heating–cooling cycle from 25 °C to 225 °C. | |
Photostability test of the selected GNC is determined by recording the PL emission intensity at various time intervals upon stimulating the sample under a powerful laser excitation (see Fig. 5b). As depicted in Fig. 5b, no substantial change in PL intensity values can be noticed due to the robust protection provided by the rigid glass structure.
Thermal stability analysis of CsPbBr3 QDs in glass is carried out by recording temperature-dependent PL spectra of the selected sample up to 225 °C (see Fig. 5c and d). The thermal quenching mechanism causes the PL emission intensity to decrease as the temperature increases from 25 to 225 °C. However, after cooling the sample back to 25 °C, it recovers its original intensity value (see Fig. 5c). Additionally, thermal cycling experiments further demonstrate that the emission properties of QDs are highly reversible as evidenced by the absence of a significant reduction in PL intensity of the selected sample after 8 heating–cooling cycles (see Fig. 5d). The above results show that the Eu3+ and Tm3+ co-doped CsPbBr3 QD GNCs have excellent chemical, photo and thermal stability, making them a suitable choice for solid-state lighting applications.
4. Conclusions
In conclusion, Eu3+ and Tm3+ co-doped CsPbBr3 QD GNCs are successfully synthesized in a glass host via the melt-quenching method followed by a controlled heat-treatment process. The incorporation of Eu3+ and Tm3+ into CsPbBr3 QD GNCs not only improves the PLQY but also provides unique features such as efficient tuning of emission colors from blue to cyan, violet, red, green, and white by simply controlling the heat-treatment conditions – that could be a promising way to obtain multi-color LEDs or other optoelectronic devices. The produced GNC samples demonstrate superior thermal, chemical and photo stability features by preserving their original PL intensities even after being subjected to temperatures as high as 225 °C, immersion in water for 45 days, and laser irradiation at 5 W cm−2 for 10 h, respectively. The encouraging results of this research might provide further insight into new approaches for developing innovative and high-performance solid-state lighting devices for use in a variety of applications.
Conflicts of interest
The authors declare no competing financial interest.
Acknowledgements
This work was supported by Yildiz Technical University Scientific Research Projects Coordination Unit under project number FBA-2021-4543. The authors of this study express their gratitude to Naji Vahedigharehchopogh for his help in digital imaging, and to Ulaş Korkmaz, Beyza Özlem, Utku Ekim and Boğaçhan Ertekin for their help in sample preparation studies. The authors would like to acknowledge that this paper is submitted in partial fulfilment of the requirements for a PhD degree at Yildiz Technical University.
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Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/d1cp05016h |
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