Open Access Article
Shangkun
Li
a,
Yingchao
Meng
a,
Yujia
Guo
a,
Tian
Liu
b,
Stavros
Stavrakis
a,
Philip D.
Howes
*a and
Andrew J.
deMello
*a
aInstitute for Chemical and Bioengineering, Department of Chemistry and Applied Biosciences, ETH Zürich, Vladimir Prelog Weg 1, 8093 Zürich, Switzerland. E-mail: andrew.demello@chem.ethz.ch; philip.howes@chem.ethz.ch
bLaboratory for Multifunctional Materials, Department of Materials, ETH Zürich, Vladimir Prelog Weg 1, 8093 Zürich, Switzerland
First published on 19th November 2020
Rare-earth-doped upconversion nanoparticles (UCNPs) show great promise in a range of applications, including biological imaging and sensing, solar cells and security inks. Although their emission color can be tuned widely as a function of host matrix and dopant composition, the high dimensionality of the associated parameter space and the sensitivity of emission to these parameters make optimization and precision tuning difficult. Herein, we present a new time-efficient synthetic route to NaYF4:Yb,Er,Tm UCNPs and a high-throughput microfluidic reactor to synthesize and precisely tune the emission characteristics of the particles in situ and in real time. We synthesize a range of particles with optimized emission intensity and wide color distribution by changing the doping degree of sensitizer Yb to provide for green-orange tunability, and the ratio of Tm–Er to give green–blue tunability. With the two tunable dimensions, we realize true white light emitting UCNPs based on optimized red, green and blue (RGB) emission ratios from a single composition NaYF4:Yb,Er,Tm nanocrystal—a demanding task for such materials—with CIE 1931 coordinates of (0.29, 0.34) and doping degrees of 60% Yb, 0.45% Er, and 1.05% Tm. Finally, we demonstrate the efficacy of these materials in a thin film format through the fabrication of an anti-counterfeit device.
Rare-earth (RE) UCNPs, typically co-doped with sensitizer ions of ytterbium (Yb3+) and activator ions of X3+ (X = Er, Tm, and/or Ho) in the same nanocrystal host, can yield non-linear anti-Stokes luminescence via sequential absorption of two or more low energy near-infrared (NIR) photons.11,12 UCNPs are free of reabsorption, emit with narrow peaks and are photostable, with tunable lifetimes and low toxicity.13,14 Long-wavelength NIR excitation leads to less scatter, minimizes photodamage and autofluorescence of biological samples and allows deep tissue penetration.15 Standout applications of UCNPs include biological imaging and therapy,16 photonic devices,17 luminescence thermometry,18 biosensing,19 and anti-counterfeiting.20–22 Regarding white light emission, it is possible to tune rare-earth UCNPs to act as single entity white light emitters, overcoming the previously noted problems encountered in heterogeneous populations. For example, Sivakumar et al. demonstrated a white light thin film made from RE3+-doped LaF3 nanoparticles, which could be excited using a single NIR source.4 Subsequently, Wang et al. reported white upconversion rare-earth oxide materials Tm2O3 and Yb2O3, which achieved pure white light emission using single source excitation.23 More recently, Zhang et al. designed a core–shell–shell nanostructure incorporating several RE3+ within a single nanocrystal, and whose emission colors could be tuned by changing the excitation power density for white light.9 Additionally, Wang and co-workers have reported a Yb3+/Er3+/Tm3+ tridoped hexagonal β-NaYF4 microrod for white-light lasing at room temperature.24 Despite these successes, the precision tuning of emission characteristics across a wide range and using a single nanocrystal composition is still a challenge, and there is much potential still to be unlocked.
During the last decade, several UCNP synthesis methods have been proposed,25 including hydrothermal, thermal decomposition, and thermal co-precipitation reactions.26–28 However, these typically require harsh reaction conditions (i.e. high temperatures and/or high pressures), and extended reaction times. Moreover, bulk reaction approaches to nanocrystal synthesis typically necessitate large investments of time and materials to effectively map an inherently complex reaction parameter space. This is especially problematic for UCNPs, as their properties are extremely sensitive to the exact preparation conditions, in particular the doping degree of the sensitizers and activators, and thus they would benefit hugely from a more comprehensive characterization and optimization process. Further, we propose that the development of UCNPs will drastically benefit from a more efficient, economic and greener strategy for fast parameter screening, with a view to optimizing properties for advanced applications.
Since the pioneering works of nearly two decades ago,29–31 great strides have been made in establishing the field of microfluidic-based nanoparticle synthesis. In the field of rare-earth UCNPs, previous reports have demonstrated the utility of continuous flow microfluidic approaches.32–34 However, such methods are not suitable for high-throughput screening because of difficulties in controlling cross-contamination between solutions run with different reaction parameter sets. In contrast, droplet-based microfluidic reactors have engendered a time-efficient high-throughput screening approach for some years now,35 due to efficient heat and mass transfer within droplets, and the ability to analyze products and tune reactions in real-time.36 However, rare-earth UCNPs have not benefitted from this approach due to their restrictively long reaction times and the difficulty in preparing single compositional element sources (i.e. precursors that deliver only one of the elements that form the final NC). Unlike in common bulk reactions where the RE3+, Na+ and F− are premixed in one solution, in the proposed high-throughput screening method it is imperative that each of the compositional elements can be delivered by a separate syringe to allow fine control of reaction stoichiometry. However, this isolation of precursors causes solubility issues, which necessitates redesigning the reaction in terms of solvent, reagents and ligands.
In this paper, we detail a new synthetic approach for rare-earth UCNPs that allows for facile parametric space mapping and fine tuning of RGB emission under NIR excitation. Focussing on Yb–Er–Tm tri-doped NaYF4 UCNPs, we first develop a novel reaction formulation that enables time-efficient screening, where each compositional element can be delivered in a separate precursor for precise tuning of elemental ratios (in terms of F− and Na+ for the host matrix, Yb3+ as a sensitizer, and Er3+ and Tm3+ as the activators). Second, and to achieve rapid and efficient parameter mapping and product optimization, we show for the first time the use of a high-throughput droplet-based microfluidic reactor with inline emission analysis for rapid lanthanide-doped UCNP synthesis and compositional tuning. This approach was used to scan and tune the RGB emission attainable from a single NaYF4:Yb,Er,Tm nanocrystal composition (as opposed to a mixed population) by optimizing elemental ratios, engendering tunable true white light emission based on optimized RGB intensity ratios under single excitation. These developments encompass a new strategy for rapid UCNP synthesis, characterization and optimization. Expansion of this approach will pave the way for advanced applications of these promising materials.
The ability to rapidly scan precursor ratios allows for fast, accurate, reproducible and efficient parameter screening.37 In this regard, it should be noted that droplet-based microfluidic systems benefit from rapid heat and mass transfer, which ensures prompt mixing and temperature equilibration on ultra-short timescales.38 To assess the temperature equilibration time in our reactor, we conducted computational fluid dynamic (CFD) simulations of the heat transfer from the heating rod (Fig. 1b) into the reaction solution (Fig. 1c and Fig. S1, ESI†). At a total flow rate 80 μL min−1, the reaction solution reaches the target temperature (i.e. room temperature to 220 °C) after 3 mm of travel, and within 500 ms (Fig. 1d). This significantly improves upon the heat transfer efficiency obtained in flask-based systems, and reduces reaction times for UCNPs synthesis. Further details on the simulations are provided in the ESI.†
To tune or optimize the properties of NaYF4:Yb,Er,Tm UCNPs by reaction parameter screening, the precursor ratios between each constituent element must be controllable, meaning that each element must to be delivered in a separate precursor. This is not typically the case in bulk reactions, where Na+, RE3+, and F− are combined within a single precursor.26–28 In our new strategy, we are able to deliver each element in a separate precursor. Furthermore, instead of using 1-octadecene, we employed TEGDME as the solvent for all precursors due to its high boiling point (275 °C) and excellent solubility for F−, Na+, and RE3+. Finally, it should be noted that modulation of droplet residence times in the heated zone allows for control over the total reaction time.
To better compare the green and red emission from NaYF4:Yb,Er, the PL peaks at 652 nm (4F9/2 → 4I15/2) and 543 nm (4S3/2 → 4I15/2) were chosen as indices (see Fig. 5c). The optimized PL intensity occurs when R1 lies between 1.5 and 2.5 (peak at 1.8), where both the green and red light obtain their maximum intensity, with the intensity at 652 nm always being higher than at 543 nm. However, when R1 is larger than 2.5, the PL intensity at 543 nm exceeds the PL intensity at 652 nm. This switching of dominance between the two peaks allows facile tuning of the green to red emission ratio via modulation of the Na/RE molar ratio (R1).
The PL intensity of UCNPs was then optimized using an R2 (F/RE) scan, from 2.4 to 6.0, uncovering an optimal range of 3.2–3.6 (Fig. 2c and d). Interestingly this ratio is less than the 4
:
1 stoichiometry of NaYF4. Indeed, the most popular methods for NaYF4:Yb,Er synthesis (Table 1) all use a stoichiometry of 4 or higher.
| Precursors | Solvent | R 1 Na/RE | R 2 F/RE | R 3 Yb/RE (%) | R 4 Er/RE (%) | T (°C) | Time (min) | Phase | Ref. |
|---|---|---|---|---|---|---|---|---|---|
| a Time used for high-throughput screening of emission characteristics. | |||||||||
| Na(CF3COO) | ODE/OA/OM | 1 | 4 | 20 | 2 | 250 | 45 | Cubic | 28 |
| RE(CF3COO)3 | ODE/OA/OM | 1.8 | 4.8 | 20 | 2 | 330 | 30 | Hexagonal | |
| OM | 2 | 5 | 20 | 2 | 330 | 60 | Hexagonal | 42 | |
| NaF, RE-oleate | ODE | 4.8 | 4.8 | 17 | 3 | 260 | 360 | Hexagonal | 43 |
| 4.8 | 4.8 | 17 | 3 | 210 | 360 | Cubic | |||
| RE-oleate | ODE/OA | 9.5 | 4 | 18 | 2 | 300 | 30 | Hexagonal | 39 |
| NaOH | ODE/OA | 2.5 | 4 | 18 | 2 | 280 | 30 | Cubic | |
| NH4F | ODE/OA | 2.5 | 4 | 18 | 2 | 115–155 | 8–9 | Cubic | 33 |
| 300 | 30 | Hexagonal | |||||||
| RE(CO3)3 | OM | 17.6 | 4.4 | 11.5 | 2.2 | 280 | 120 | Cubic/hexagonal/NaF | 44 |
| Na2CO3 | |||||||||
| NH4F | |||||||||
| RE(III)-2-Ethylhexanoate | TEGDME | 1.5–2.1 | 3.2–3.6 | 15 | 1.5 | 200–240 | 0.1–4a | Cubic/hexagonal | This work |
| Na-2-Ethylhexanoate | |||||||||
| CsF | |||||||||
Ratios R3 (Yb/RE) and R4 (Er/RE) control the rare-earth element doping (i.e. percentage versus total RE content) for NaYF4:Yb,Er. From the R3 scan we observed divergent behaviour for the red and green PL peaks (Fig. 2e and f). The PL from both red and green increases up to 15% doping, where they both form a local maximum. However, above 15%, green emission decreases steadily whereas the red emission increases again. This phenomenon means that the red to green intensity ratio may be adjusted via control of Yb content, R3. After normalizing the PL at 543 nm (Fig. 3a), it is evident that the red emission increases with Yb3+ doping concentration (from 5% to 90%) due to the influence of the cross-relaxation process.24,40 To achieve higher intensity emission from UCNPs, the activator doping ratio of Er3+ was optimized in Fig. 2g and h, where the optimum value of R4 was found to be 1.5%.
Fig. 3c presents a CIE chromaticity diagram, where the CIE chromaticity coordinates vary from x = 0.3332, y = 0.6503 (green) to x = 0.5020, y = 0.4710 (orange) by increasing the doping ratio of Yb3+ from 5 to 90%. To obtain a better understanding of color evolution, spectra were converted into RGB tristimulus values (Fig. 3b) based on the CIE colour matching functions.41 The RGB percentages are shown in Fig. 3d. With increasing Yb3+ content, the percentage of red emission smoothly increases from 21 to 65%. In contrast, the percentage of green emission decreases from 79 to 34%. The blue emission is near zero across the whole range. Overall, we see that the emission color from NaYF4:Yb,Er UCNPs can be tuned from green to orange by changing the doping ratio of Yb3+ in RE.
After scanning precursor ratios for emission color tuning, we conducted a study of the impact of reaction temperature and residence time, with a view to further optimizing reaction parameters and understanding the influence of these factors on UCNP properties (Fig. 4). For temperature optimization, we used the optimal ratios established previously, i.e. R1 = 1.8, R2 = 3.2, R3 = 15%, and R4 = 1.5%, respectively, with a total reaction time of 48 seconds. In the range of 160 to 240 °C, there was a continual increase in PL from effectively zero at 160 °C (Fig. 4b). It is evident that the PL has not reached a global maximum by 240 °C, however this was the highest accessible temperature using the current reactor set-up, since temperatures higher than this led to gas evolution from the reaction solution (the b.p. of TEGDME is 275 °C). For the reaction time study, the temperature was set at 230 °C (to ensure sufficient PL intensity, whilst prohibiting gas evolution).
In this work we sought to minimize the required reaction time in order to increase the experimental throughput and the rapidity of optimization. As shown in Fig. 4c and d, the PL of the formed UCNPs increases with the residence time, approaching a plateau by ca. 4 minutes. Further, it was imperative to prove that the PL spectral shape (i.e. color) did not change substantially at longer reaction times versus the short reaction time to be used in our reactor. To confirm this, we ran a further bulk experiment to demonstrate that the PL (judged by the RGB%) was consistent between a 4 minute reaction at 230 °C (as used in the microfluidic reactor) and a longer ‘standard’ reaction (we chose 60 minutes and 270 °C as representative) in the flask, which would justify our premise of using the microfluidic reactor to tune emission color. Although the size and phase of the nanocrystals did not remain constant (Fig. S3a–e, ESI†), the RGB% values were consistent (Fig. S3f and g, ESI†). Therefore, we determined that a reaction of 4 minutes and temperature of 230 °C was sufficient for rapid color tuning of the UCNP emission in our microfluidic reactor.
In Table 1 we provide a direct comparison between the synthesis method developed herein and other approaches from the literature. Overall, we find a Na-rich and F-deficient reaction formulation (versus the stoichiometry of NaYF4:Yb,Er) benefits the PL intensity, while color can be adjusted by tuning the doping degree of Yb3+. This is an important observation, and worthy of further study in future work. Moreover, results highlight the powerful capabilities of high-throughput microfluidic screening platforms in understanding complex synthetic systems. Indeed, in an experiment with N synthetic variables (multiple precursors ratios, residence time, temperature, etc.), each having M levels (defining the selected range of each factor), the overall number of required experimental iterations scales as MN. The time needed for these iterations is then given by MN × t, where t is the time for one iteration. In the case of NaYF4:Yb,Er UCNPs, a reaction time of at least 60 minutes is typical for one bulk synthesis. Thus, conducting comprehensive parameter space mapping using standard flask-based approaches would rapidly become unmanageable due to the excessive time required, whereas it remains easily accessible using our modified synthesis route and screening approach.
:
Er ratio. Specifically, we used the previously optimized parameters for NaYF4:Yb,Er, except that R1 was varied to control the red-green balance. Fig. 5a shows spectra originating from NaYF4:Yb,Er,Tm (20% Yb) with different degrees of Tm doping (R5). The blue region (with peaks at 478 nm and 453 nm) arises from Tm3+, while green (543 and 524 nm) and red (652 nm) emissions arise from the Er3+ doping (Fig. 5d). To better understand the color evolution, spectra were converted into RGB tristimulus values based on the CIE colour matching functions.41 As R5 increases, the blue value exhibits a continuous increase (Fig. 5b), and the red value a continuous decrease, across the entire range. The value of green emission was not significantly affected before an R5 of ca. 80%, but experienced a sharp decrease with any further increase in Tm3+ ratio. The percentage of the red and green emission (Fig. 5c) decreased with increasing R5 (decreasing Er3+). The percentage of blue color increased from 0 to 95%, as R5 increased from 0 to 100%. As a result of the low percentage of red color across the whole range of R5, UCNP emission gradually changed from green to cold white and to blue with the different degrees of doping, as shown in Fig. 5e. The cold white light emitting NaYF4:Yb,Er,Tm nanocrystals were obtained for R5 values between 70 and 80%. Fig. 5d shows the energy level diagram of Yb3+–Er3+–Tm3+ tri-doped NaYF4 nanocrystals. The Yb3+ is initially excited at 980 nm from its ground state 2F7/2 level to the 2F5/2 level, followed by energy transfer to Er3+ and Tm3+. The Er3+ then undergoes 4S3/2 → 4I15/2 (543 nm, green), 2H11/2 → 4I15/2 (524 nm, green), and 4F9/2 → 4I15/2 (652 nm, red) transitions. The Tm3+ undergoes 1G4 → 3H6 (478 nm, blue) and 1D2 → 3F4 (453 nm, blue) transitions. In order to obtain white-light emission at a high excitation power, a high ratio of R5 is required to ensure sufficient blue emission intensity. Fig. S4 (ESI†) shows the CIE chromaticity diagram for NaYF4:Yb,Er,Tm UCNPs (20% Yb) with varying values of R5. The CIE chromaticity coordinates change from x = 0.3776, y = 0.6091 (green) to x = 0.2292, y = 0.3585 (cold white), ending at x = 0.1475, y = 0.1121 (blue), when increasing the doping ratio of Tm3+ from 0 to 100%. With 20% Yb3+, we achieve ‘cold’ white light rather than ‘true’ white due to a lack of red. However, by increasing the doping degree of Yb3+ to 60%, we can increase the red light content (Fig. S5, ESI†), thereby achieving true white light emission. The emission spectra of NaYF4:Yb,Er,Tm nanocrystals with 60% Yb and variable Tm doping (R5) are shown in Fig. S5a (ESI†). The red and green emission were similar across the entire range of R5 (Fig. S5c and d, ESI†), which benefits targeting of true white light emission. The corresponding CIE chromaticity diagram (Fig. S5b, ESI†) shows an R5 of 60–70%, yielding white light under 980 nm excitation (Movie S1, ESI†). Overall, the emission colors of the products display a wide variation from orange to blue, and pass through the white emission zone.
The above results powerfully demonstrate the merits of rapid reaction tuning for NaYF4:Yb,Er,Tm UCNPs in obtaining precise multicolor emission in the visible region when exited by a single wavelength light source. Fig. 6a reports that the emission color of NaYF4:Yb,Er,Tm can be adjusted in two dimensions, by varying the Yb percentage to tune the green–red ratio, and varying the Tm percentage to tune the green–blue ratio. Fig. 6b shows the XRD pattern of three samples, with R5 equal to 0, 70 and 100%, yielding NaYF4:Yb,Tm, NaYF4:Yb,Er,Tm, and NaYF4:Yb,Er, respectively. All three samples exhibit peaks from both the cubic (α-) and hexagonal (β-) phases. The diffraction peaks from the β-phase of the 0% sample (NaYF4:Yb,Er) were weaker than those for the 70% (NaYF4:Yb,Er,Tm) or 100% (NaYF4:Yb,Tm) samples. This implies that the β-phase ratio in the absence of Tm is less than in the Tm-doped UCNPs. TEM images (Fig. S6, ESI†) show that ‘popcorn-like’ NaYF4:Yb,Er nanocrystals were obtained. The sizes of the nanocrystals (Fig. 6c–e) did not significantly vary as a function of Tm doping. The R5 at 0, 70 and 100% samples exhibited average diameters of 53.4 ± 8.5, 49.5 ± 7.7, and 50.2 ± 8 nm, respectively. Therefore, the size of the NaYF4:Yb,Er,Tm UCNPs seems to primarily depend on the NaYF4:Yb matrix rather than the doping degree of the activators.
Footnote |
| † Electronic supplementary information (ESI) available. See DOI: 10.1039/d0tc04309e |
| This journal is © The Royal Society of Chemistry 2021 |