Open Access Article
Ahmed G.
Attallah†
*ab,
Arzu
Cosgun Ergene†
c,
Eric
Hirschmann
a,
Maik
Butterling‡
a,
Dmitry
Busko
c,
Aditya
Chauhan
c,
Bryce S.
Richards
cd and
Andrey
Turshatov
*c
aHelmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, 01328 Dresden, Germany. E-mail: a.elsherif@hzdr.de
bPhysics Department, Faculty of Science, Minia University, 61519 Minia, Egypt
cKarlsruhe Institute of Technology (KIT), Institute of Microstructure Technology (IMT), 76344 Eggenstein-Leopoldshafen, Germany. E-mail: andrey.turshatov@kit.edu
dKarlsruhe Institute of Technology (KIT), Light Technology Institute (LTI), 76131 Karlsruhe, Germany
First published on 5th November 2025
Upconversion (UC) luminescence enhancement in trivalent lanthanide-doped materials – particularly the ytterbium (Yb3+)/erbium (Yb3+) ion pair – remains challenging due to complex, interdependent mechanisms involving structural modifications and defect formation. Here, we present a systematic investigation of UC enhancement in relation to defect formation in GdVO4:Yb3+/Er3+ microcrystals through strategic co-doping with optically inactive ions (Sc3+, Cd2+, Zn2+). We employ a novel multi-technique approach combining positron annihilation lifetime spectroscopy (PALS) – to quantify vacancy-type defects in UC materials – with X-ray diffraction and photoluminescence quantum yield (PLQY) measurements to establish direct structure–defect–property relationships. Our results reveal that dopant valence and ionic radius dictate distinct defect formation patterns: isovalent Sc3+ substitution primarily induces lattice contraction with minimal point defect generation, while aliovalent Cd2+ and Zn2+ doping creates extensive Gd vacancy networks through charge compensation mechanisms. Critically, we demonstrate that defect cluster size and spatial distribution, rather than total defect concentration, govern UC efficiency. Zn3+ co-doping achieves a remarkable PLQY enhancement through progressive suppression of large vacancy clusters at grain boundaries, coupled with favorable redistribution of oxygen vacancies within crystallite interiors. In contrast, Cd2+ doping, despite similar charge compensation requirements, produces extended defect clusters that act as efficient non-radiative quenching centers, limiting PLQY improvement. These findings establish defect engineering as a powerful strategy for UC optimization and provide a quantitative framework for rational design of high-efficiency lanthanide-based photonic materials.
UC processes are commonly categorized into lanthanide (Ln3+)-based UC, where emissive Ln3+ ions play the central role.20 Transition metal21 and actinide ions22 also exhibit UC capabilities together with a distinct category termed triplet–triplet annihilation UC.23 However, this work focuses on the former. Ln3+-based UC materials primarily rely on a robust solid inorganic matrix, such as glass, or a crystalline host exemplified by metal fluorides, oxides, phosphates, or vanadates. These matrices are doped with either a single Ln3+ ion – for example, Er3+, which is then used for near-infrared (NIR, 1500 nm to NIR, 980 nm) UC24 – or a combination of Ln3+ ions, such as Yb3+ as a sensitizer ion (980 nm excitation, which is then paired with an activator ions such as Er3+ (green/red emission) Tm3+ (blue/800 nm emission) or Ho3+ (green emission).25
Among the host matrices, gadolinium vanadate (GdVO4) stands out as a good host candidate for UC applications, valued for its high chemical stability, low phonon energy, and strong crystal field splitting.19 GdVO4 readily accommodates diverse lanthanide ion doping26 and exhibits tunable UC emission colors under NIR excitation.27,28 However, the efficiency of UC emission in the GdVO4 host is hindered by constraints arising from concentration quenching and cross-relaxation processes intrinsic to activator ions. In addition, surface and defect induced quenching plays a dominant role when GdVO4 nanocrystals are synthesized by co-precipitation or sol–gel methods.29
To overcome these limitations, metal-ion co-doping has been widely adopted as a strategy to enhance UC efficiency by tailoring the local structure, improving energy transfer efficiency, and reducing non-radiative losses. However, as previously noted, the enhancement mechanisms are often multifactorial and interdependent, making it difficult to isolate the contribution of individual structural changes.30 Factors such as lattice strain, particle size, surface-to-volume ratio, phonon energy, local symmetry, and particularly crystal defects can each influence UC intensity, often in overlapping and nontrivial ways.19
Our previous work19 on co-doping GdVO4:Yb3+/Er3+ with Zn2+ and Sc3+ demonstrated significant UC enhancement via distinct mechanisms: Zn2+ co-doping induced both lattice shrinkage and grain growth, leading to up to a 60-fold increase in UC intensity, whereas Sc3+ introduced isovalent lattice contraction with relatively modest enhancement (∼20× UC). These enhancements were attributed to a combination of structural stabilization and more efficient energy migration. However, in both cases, the explicit role of crystal defects – and their potential as non-radiative centers or sensitization sites – was not fully delineated due to simultaneous morphological changes.
Given the anticipated relationship between atomic-scale defect formation – induced by co-doping – and the evolution of UC luminescence in lanthanide-doped GdVO4 crystals, this study aims to elucidate the respective roles of crystal defects and structural modifications. In this context, we propose a more comprehensive co-doping strategy that expands beyond Zn2+ and Sc3+ to include a set of optically inactive co-dopants with distinct physical and chemical characteristics. Specifically, we selected Cd2+, Bi3+, and In3+, in addition to Zn2+ and Sc3+, to explore the influence of ionic radius, valence state, and intermediate compound behavior. This selection allows for systematic modulation of charge compensation, lattice volume, defect density, and particle size – while controlling for synthesis conditions by using the same co-precipitation route followed by high-temperature calcination (700–850 °C) to ensure uniform grain growth. A summary of these co-dopants, their corresponding intermediate phases, ionic radii, melting points, and dominant structural effects is provided in Table 1. Results for Zn2+ and Sc3+ are drawn from our previous study,19 while new data for Cd2+, Bi3+, and In3+ are presented herein. This table outlines the expected structural modifications induced by the ion co-doping and provides a foundation for our correlative analysis using a multi-technique approach combining positron annihilation lifetime spectroscopy (PALS) (to probe vacancy-type defects), X-ray diffraction (XRD) (to assess lattice distortion), and photoluminescence quantum yield (PLQY) (to quantify emission efficiency of luminescence).
| Ion | Intermediate | Ion radius (pm) | Melting point (°C) | Main effect | Source |
|---|---|---|---|---|---|
| Zn2+ | Zn2V2O7 | 90 | 88019 | Lattice shrinkage + structural defects + particle growth (∼60× UC) | Previous work19 |
| Sc3+ | ScVO4 | 83 | 166319 | Lattice shrinkage only (∼20× UC) | Previous work19 |
| Bi3+ | BiVO4 | 117 | 94333 | Lattice expansion + moderate flux effect | Current work |
| Cd2+ | Cd4Na(VO4)3 | 110 | 89234 | Particle growth + defect formation | Current work |
| In3+ | InVO4 | 92 | 113435 | Lattice shrinkage + charge compensation + mild flux effect | Current work |
PALS is a powerful, non-destructive technique for probing atomic-scale defects in solids.31 Unlike surface-sensitive methods such as X-ray photoelectron spectroscopy (XPS), which typically investigate a few nanometers beneath the surface, source-based conventional PALS techniques can probe deeper sites. In these techniques, positrons, the antimatter counterparts of electrons, are emitted by a 22Na radioisotope, featuring a continuous energy spectrum with an end point energy Emax of 0.545 MeV, and can penetrate metals to mean implantation depths ranging from approximately 10 to 160 µm.32
Such a mean implantation depth, z, depends on material's density ρ as
,36 therefore z in GdVO4 of ρ ≈ 5.3 g cm−3 is ca. 50 µm. PALS probes defects in solids by exploiting the sensitivity of positron–electron annihilation to the local electronic environment. Upon implantation into the material, positrons rapidly thermalize within a few picoseconds and diffuse through the lattice.37 In their thermalized state, positrons (as positively charged anti particles) are preferentially attracted to neutral and negatively charged open-volume defects – such as vacancies, dislocations, or voids – where the Coulomb repulsion from atomic nuclei is minimized and electron density is locally reduced. Once trapped in such sites, positrons ultimately annihilate with electrons, emitting typically two 511 keV gamma photons. Importantly, the positron lifetime prior to annihilation is governed by the local electron density: lower densities (e.g., in larger open defects) yield longer lifetimes, while denser regions (such as the defect-free bulk) lead to rapid annihilation.32,37,38 Moreover, the relative intensity of different lifetime components – obtained through spectral decomposition – offers insight into the abundance of each defect type.38,39 While this section introduces the foundational physics behind PALS, the detailed interpretation of lifetime components and their correlation to defect size, type, and concentration – along with the theoretical models used for analysis – is provided in the Results section. This structure ensures a smoother narrative flow and avoids redundancy, allowing for deeper engagement. The PALS technique can serve as a valuable complement to other bulk-sensitive characterization methods, such as electron spin resonance (ESR) spectroscopy. However, to the best of our knowledge, ESR characterization of even pure GdVO4 has not been reported, likely due to the extremely broad and low-information signals originating from its magnetically dense Gd3+ lattice. In ESR studies, isolated paramagnetic centers are typically preferred,40,41 which makes it challenging to detect defect-related states—such as oxygen vacancies—against the strong Gd3+ background.
Previous investigations have highlighted the utility of positron annihilation in probing defect structures relevant to luminescence. For example, in γ-Al2O3:Mn4+,Mg2+ nanowires, PALS, alongside XRD and photoluminescence (PL), was used to identify oxygen vacancy-rich clusters and voids that enhanced PL intensities at optimal dopant concentrations.42 In another study on Nd3+-doped Y2Si2O7 phosphors, PALS was applied to analyze multiple lifetime components, which were related to structural defects within grains and at grain boundaries, affecting phase stability and emission characteristics.43 Furthermore, in Er3+-doped PbO–B2O3–SeO2 glass ceramics, a correlation was drawn between increased free-volume defect concentrations – quantified via PALS – and the improvement in PL efficiency.44 While these works underscore the relevance of PALS in luminescent materials, they typically focus on qualitative or partial defect–property relationships, often lacking a comprehensive, quantitative framework that integrates defect structure with phase analysis (XRD) and absolute luminescence efficiency (PLQY).
In this context, our study presents an integrated investigation aimed at quantitatively deconvoluting the structural and optical effects of co-doping in lanthanide-doped GdVO4 UC phosphors. While dopant valence and ionic radius are known to influence defect formation, our work focuses on how defect spatial arrangement, clustering, and size influence upconversion efficiency. By combining PALS, XRD, and PLQY measurements, we aim to establish quantitative structure–defect–property relationships, providing a framework for rational defect engineering in co-doped GdVO4. Our current investigation proceeds in two stages:
• First, we analyze the individual structural effects induced by dopants. Zn2+ and Cd2+, which introduce a charge imbalance, are expected to create a number of vacancy-type defects. These are directly characterized by PALS to quantify defect types. In contrast, Sc3+ – with a smaller ionic radius and isovalent substitution – is used as a control to assess lattice contraction in the absence of charge-induced defect formation. This dopant is also examined by PALS. Additionally, XRD is also used to assess the structural impact upon co-doping.
• Second, to probe dopants that do not significantly introduce structural defects, we employ Bi3+ and In3+. These ions influence the lattice primarily through expansion (Bi3+) or mild contraction (In3+) and may act as fluxing agents during synthesis. Structural signatures are explored via XRD.
In each case, the corresponding optical performance is evaluated by PLQY measurements to isolate the influence of crystallographic distortion on UC efficiency. Additionally, scanning electron microscopic (SEM) images have been recorded to examine the particle size and morphology after co-doping. Together, this approach enables a systematic deconvolution of the overlapping effects of lattice modification, defect formation, and particle growth, thus offering a comprehensive understanding of the mechanisms governing UC enhancement in lanthanide-doped GdVO4.
000) were obtained from Sigma-Aldrich and used without further purification. The vanadium precursors, Na3VO4 and NH4VO3 (each ≥99% purity), were purchased from Acros Organics and used without modification.
A schematic representation of the synthesis steps is shown in Fig. 1. The standard co-precipitation procedure involved dissolving sodium vanadate (4 mM) in water to form solution A. Separately, the remaining metal salts and PVP were dissolved in an equivalent volume of water, creating solution B. Once both solutions were fully dissolved, solution A was gradually introduced into solution B under continuous stirring. Initially, the mixture remained clear but soon became turbid, eventually leading to the formation of a white precipitate within a few minutes. The amount of each component in the reaction mixture was calculated to provide nominal doping composition of Yb3+-10%,Er3+-2% (in all samples) and variable concentrations (5 and 15%) of co-dopants: Sc3+, Bi3+, In3+, Zn2+, and Cd2+. GdVO4:Yb/Er/xMe, where x = 5 or 15 and Me = Sc, Bi, In, Zn, or Cd, will be further used through the paper as a name of samples. The choice of 5% and 15% co-doping concentrations is based on our previous work investigating co-doping with Sc3+ and Zn2+. It was demonstrated that selected 5% and 15% are representative concentrations—corresponding to the rising and near-maximum regions of PLQY – allowing direct comparison and focused analysis of co-dopant-induced defect interactions.19 Hence, the selected concentrations ensure continuity with our previous dataset and effectively capture the most relevant regimes for understanding the influence of co-doping on luminescence and defect behavior.
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| Fig. 1 Flowchart illustrating the synthesis process of doped GdVO4-based compounds via the co-precipitation method, followed by drying and calcination. | ||
The reaction mixture was stirred for an additional 30 min to ensure completion. Subsequently, stirring was halted, allowing the precipitate to settle naturally. The solid was then separated by centrifugation (6000 rpm for 5 minutes) and thoroughly washed multiple times with deionized water to eliminate any residual reagents. A final wash with isopropanol was performed to aid in moisture removal. The collected precipitate was dried overnight at 80 °C in a vacuum oven at 10 mbar. After drying, the material was finely ground using a mortar and pestle, then subjected to calcination at different temperatures in a muffle furnace (Thermoconcept, KLS-05/13) at 850 °C, with a ramp rate of 5 °C per minute. To mitigate the pronounced particle growth induced by Zn2+ and Cd2+ at 850 °C, GdVO4:Yb/Er/Zn and GdVO4:Yb/Er/Cd were instead calcined at 700 °C and 750 °C, respectively. The resulting calcined powder was ground once more and stored in polystyrene cuvettes for further characterization presents a flowchart summarizing the synthesis process.
The microstructure of the calcined powders was imaged using a scanning electron microscope (SEM; Zeiss Supra 60VP) equipped with an SE-II detector. The samples were sputter coated with a thin layer of silver (∼10 nm) to aid the SEM imaging.
, with τi and Ii
are the positron lifetime and intensity of the ith component, respectively.38,47 Hence, PALS analysis comprised fitting exponential decay curves to histograms of recorded time differences. Al and Sn reference samples with known lifetimes were used to estimate the resolution functions and source contribution. About 10.60% of all positrons annihilate within the used source itself, and therefore this value is referred as source contribution (shared between Kapton foil (0.382 ns/10.40%) and glue (2.60 ns/0.20%)) and an average time resolution of 0.28 ns (at full width at half maximum) have been defined during the fitting process.
| Sample | a = b (pm) | c (pm) | V (pm3) × 106 | Goodness of FIT |
|---|---|---|---|---|
| GdVO4 | 721.18 | 635.16 | 330.35 | 1.32 |
| GdVO4:Yb/Er | 719.97 | 634.41 | 328.85 | 1.41 |
| GdVO4:Yb/Er/5Sc | 718.86 | 633.95 | 327.60 | 1.50 |
| GdVO4:Yb/Er/15Sc | 715.61 | 632.39 | 323.84 | 1.57 |
| GdVO4:Yb/Er/5Bi | 719.37 | 634.75 | 328.48 | 1.59 |
| GdVO4:Yb/Er/15Bi | 720.02 | 635.84 | 329.65 | 1.46 |
| GdVO4:Yb/Er/5In | 718.86 | 633.94 | 327.59 | 2.02 |
| GdVO4:Yb/Er/15In | 717.64 | 633.77 | 326.40 | 1.96 |
| GdVO4:Yb/Er/5Cd | 719.22 | 633.64 | 327.77 | 1.10 |
| GdVO4:Yb/Er/15Cd | 719.58 | 633.96 | 328.26 | 1.11 |
| GdVO4:Yb/Er/5Zn | 719.08 | 633.52 | 327.58 | 1.12 |
| GdVO4:Yb/Er/15Zn | 718.97 | 633.51 | 327.47 | 1.20 |
The calculations of crystallite size and strain were performed using Williamson–Hall–Langford (WHL) method (Fig. S1–S12, SI). It is known from the literature that using different equations, such as Williamson–Hall, Halder–Wagner, or size-strain plot48 results in slightly different values of crystallite size and microstrain. Taking this potential source of error into account, we use these values primarily as an indicator for trends in the in the variation of crystallite size and micro-strain with co-doping.
The addition of Sc3+ with an ionic radius of 87 pm leads to a decrease in the cell volume and crystallographic parameters (compared to GdVO4:Yb/Er) (Table 2). This observation is valid for both nominal Sc3+ concentrations (5 and 15 mol%) and the reduction in cell volume is greater at the higher concentration of Sc3+. To confirm the presence of Sc3+ in the co-precipitated sample, the elemental composition was analyzed using XRF – a non-destructive method that detects characteristic X-rays emitted by elements upon excitation with high-energy X-rays. This technique allowed quantification of the relative amounts of Gd3+, Yb3+, Er3+, and Sc3+. Under the assumption that Yb3+, Er3+ and Sc3+ substitute Gd3+, the compositions of (Gd0.79Yb0.13Er0.02Sc0.06)VO4 and (Gd0.72Yb0.12Er0.03Sc0.13)VO4 were found with nominal Sc3+ concentration of 5 and 15%, respectively. The only small deviations between nominal and experimental concentrations indicate successful co-doping with Sc3+ ions via co-precipitation method. Microstructural analysis of XRD data using the WHL method results in crystallite size of 30 ± 1 nm (for 5% Sc3+) and 51 ± 4 nm (for 15% Sc3+) and micro-strain of (7.5 ± 0.9) × 10−3 and (7.0 ± 0.8) × 10−3, respectively (Fig. 3 and Fig. S13).
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| Fig. 3 Summary of crystallite size and microstrain calculated using WHL equation for samples with 15% of Sc3+, Bi3+, In3+, Zn2+, Cd2+ and the reference GVO4:Yb/Er sample. | ||
Co-doping with nominal 5 mol% Bi3+ (ionic radius – 117 pm) results in pure GdVO4 phase. In contrast, 15% Bi3+ provides an additional phase – 5.3 wt% identified as Bi23(VO4)4O28.5 based on the powder diffraction file PDF 04-020-1954 (Fig. 2f). The substantial increase in cell volume was only observed at 15% nominal Bi3+ doping (Table 2). In order to understand exactly how much Bi3+ is present in the samples, an XRF analysis was carried out, similar to the Sc3+ doped samples. The compositions (Gd0.79Yb0.12Er0.02Bi0.06)VO4 and (Gd0.68Yb0.12Er0.02Bi0.18)VO4 were found for the samples with nominal Bi3+ concentrations of 5 and 15% respectively. The amount of Bi3+ found is slightly larger than expected from the nominal composition with 15% co-doping, which can be explained by the existence of a secondary Bi-based phase Bi23(VO4)4O28.5. Microstructural analysis of XRD data using the WHL method shows an increase in crystallite size, 80 ± 10 nm (for 5% Bi3+) and 46 ± 9 nm (for 15% Bi3+) compared to the GdVO4:Yb/Er sample. Similarly, compared to the GdVO4:Yb/Er sample, the microstrain decreases in the sample with 5% Bi3+ – (1.9 ± 1.7) × 10−3 (Fig. S13). In contrast, the reduction is less pronounced in the sample with 15% Bi3+, where the microstrain reaches – (4.0 ± 2.4) × 10−3 (Fig. 3).
As the ionic radius of In3+ (92 pm) is smaller than the lanthanide ions (Gd3+, Yb3+, Er3+), the co-doping with In3+ leads to a decrease of the crystallographic parameters (Table 2). This effect can be observed for both nominal doping concentrations. Furthermore, the use of nominal concentration of 15% leads to appearance of a secondary phase – In2O3 (8.6 wt%) (Fig. 2h). The compositions of (Gd0.80Yb0.12Er0.02In0.06)VO4 and (Gd0.67Yb0.11Er0.02In0.20)VO4 were found for the samples with nominal Bi3+ concentration 5 and 15%, respectively. The apparent increase in In3+ content beyond the nominal 15% is likely attributable to the formation of the secondary In2O3 phase. Co-doping with 5% mol% In3+ still provides pure GdVO4 phase, and the experimental composition is close to the nominal one. Microstructural analysis of XRD data using the WHL method results in increased crystallite size of 111 ± 14 nm, (for 5% In3+) and 79 ± 15 nm (for 15% In3+). Simultaneously, the microstrain was calculated as (2.0 ± 1.2) × 10−3 and (1.1 ± 1.0) × 10−3, respectively (Fig. 3 and Fig. S13).
As the next ion to be compared, Cd2+ co-doping was investigated. Ionic radius of Cd2+ (110 pm) is significantly larger than radius of lanthanides. Table 2 indicates that co-doping with Cd2+ (the sample was calcined at lower temperature of 750 °C to maintain the particle size compared to co-doping with other ions) leads to a pronounce increase of cell volume. However, the analysis of chemical composition shows some deficiency of Cd2+ in comparison to the nominal composition – (Gd0.84Yb0.13Er0.02Cd0.01)VO4 (for 5% Cd2+) and (Gd0.80Yb0.14Er0.02Cd0.04)VO4 (for Cd2+). The crystallite size increases up to 80 ± 5 nm and 79 ± 6 nm for co-doping with 5 and 15% Cd2+, respectively. The microstrain decreases with amount of Cd2+ – (1.7 ± 0.8) × 10−3 and (1.0 ± 1.9) × 10−3 for 5% and 15% Cd2+, respectively (Fig. 3 and Fig. S13).
Co-doping with Zn2+ leads to a reduction in the lattice parameters and overall unit cell volume (Table 2) of GdVO4:Yb/Er, consistent with the substitution of smaller Zn2+ ions (ionic radius 90 pm) for the larger Gd3+ ions (105 pm). The composition of the synthesized materials, (Gd0.78Yb0.12Er0.02Zn0.08)VO4 and (Gd0.62Yb0.11Er0.02Zn0.25)VO4, confirms successful incorporation of Zn2+ into the lattice. Interestingly, while the unit cell contracts due to the smaller ionic radius of Zn2+, the crystallite size increases, reaching 76 ± 8 nm and 88 ± 4 nm for 5% and 15% Zn2+ co-doping, respectively. This size growth is accompanied by a reduction in microstrain, from the baseline value to (3.2 ± 1.0) × 10−3 (for 5% Zn2+) and (1.2 ± 0.7) × 10−3 (for 15% Zn2+). These trends suggest improved crystalline order and fewer structural imperfections upon Zn2+ incorporation (Fig. 3 and Fig. S13). It should be noted that an increase in crystallite size and a decrease in macrostrain were observed despite the lower calcination temperature of 700 °C in contrast to 850 °C (for Sc3+, Bi3+ and In3+) to maintain the particle size.
The microstructural information obtained from XRD analysis is further corroborated by SEM observations. It is important to note that different calcination temperatures were applied for the Zn2+ and Cd2+ co-doped samples in order to achieve comparable particle size, ensuring a meaningful comparison between their morphological and structural characteristics. Previous findings demonstrated that calcination of Zn2+ co-doped samples at 850 °C results in the formation of large particles, typically on the order of ∼1000 nm.19
SEM images reveal that the samples GdVO4, GdVO4:Yb/Er, GdVO4:Yb/Er/5Sc, GdVO4:Yb/Er/15Sc, and GdVO4:Yb/Er/5Cd (Fig. 4a–d and i, respectively) exhibit similar particle size. The powder consists of partially sintered small nanoparticles (∼70 nm scale) that cluster together to form loosely packed agglomerates on the micron size scale. It appears that even small amount (5%) of Bi3+ facilitated crystallization of GdVO4 (Fig. 4e) resulting in formation of particles exhibiting a mix of rod-like structures (100–300 nm range in length) and aggregated clusters with relatively rough surface. Increase concentration of Bi3+ doesn’t change particles view (Fig. 4f). Doping with In3+ (Fig. 4g and k) results in particles (with size 400–600 nm) exhibiting a smooth, faceted, and polyhedral morphology. Some small nanoscale deposits or secondary formations can be observed on the surface, which might be the secondary phase of In2O3. When GdVO4 is doped with of Cd2+ and Zn2+ (GdVO4:Yb/Er/15Cd and GdVO4:Yb/Er/5Zn samples, Fig. 4j and k, respectively), the micrographs reveal a densely packed morphology composed of aggregated, rounded nanoparticles that have grown in size to reach a scale of up to ∼300 nm. The particles formed in the presence of 15% Zn2+ (Fig. 4l) resemble those observed in case of In3+ co-doping (Fig. 4h), despite the lower calcination temperature of 700 °C vs. 850 °C, respectively.
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| Fig. 5 (a) UC luminescence of GdVO4:Yb/Er/15Bi sample excited with 980 nm laser with intensity of 15 W cm−2; (b) PLQY of GdVO4:Yb/Er samples co-doped with 5 and 15% Sc3+, Bi3+, In3+, Zn2+ and Cd2+. | ||
Steady-state luminescence spectra were excluded from comparative analysis because of the unpredictable and sample-dependent influence of light scattering, which may distort intensity readings. Instead, we measured the absolute UC PLQY using an integrating sphere. PLQY, defined as the ratio of emitted to absorbed photons, serves as a key figure-of-merit for luminescence, enabling a quantitative comparison of different materials. Fig. 5b summarizes the UC PLQY values of GdVO4:Yb/Er UC materials synthesized in the presence of a series of additional ions (Sc3+, Bi3+, In3+, Cd2+ and Zn2+). All measurements of UC PLQY were performed at excitation intensity of 15 W cm−2. It is important to note that the goal is not to obtain the most efficient UC material, but rather to elucidate the role of co-dopants using PLQY as a figure-of-merit parameter. The reference material, with a UC PLQY of 0.003%, is a GdVO4:Yb/Er sample synthesized via co-precipitation followed by calcination at 850 °C. While the UC PLQY value is low, it can still be measured with high precision. The uncertainty in UC PLQY measurements depends mainly on the percentage of absorbed light and the uncertainty in our experiments is relatively low (<10%) as all samples absorb 30–40% of the incident radiation.49Fig. 5b shows that co-doping with Sc3+ enhances UC PLQY, reaching 0.02% and 0.07% for 5% and 15% Sc3+, respectively. These results are consistent with previously reported values,19 highlighting the reproducibility of both the synthesis approach and the optical characterization methodology. Co-doping with Bi3+ and In3+ also improves PLQY at lower doping concentrations (5%) – achieving 0.06 and 0.05%, respectively; however, at 15% doping, the PLQY remains comparable to that of Sc3+ co-doping – achieving 0.08 and 0.07%, respectively. Co-doping with Cd2+ gives a slightly lower PLQY of 0.02 and 0.04% for 5 and 15% Cd2+ respectively. Notably, the most significant increase in PLQY was observed with Zn2+ co-doping, achieving PLQY of 0.06 and 0.11% for 5 and 15% Zn2+, respectively. This represents a 37-fold increase over the reference sample and a 1.4-fold increase over the second-best co-dopant – Bi3+, despite the much lower calcination temperature of 700 °C used for Zn2+-containing samples.
![]() | (1) |
Discrepancies from this expression indicate the presence of complex trapping scenarios involving multiple defect types or shallow traps, which cannot be fully resolved in the two-component lifetime analysis. The average positron lifetime, calculated as τavg = τ1I1 + τ2I2, serves as a cumulative indicator of the material's defect content. An average positron lifetime exceeding that of defect-free bulk material signifies the presence of open-volume defects,52 and correlates with defect type and density.53
To further investigate this hypothesis, we performed temperature-dependent PALS measurements (Fig. S19, SI). The results show a reduction in the average lifetime upon cooling – a behavior consistent with the observation of shallow traps.38 However, the temperature-dependent changes also suggest the presence of neutral defects in addition to the shallow traps.38 Most likely, these neutral defects are oxygen vacancies (V_O), which according to DFT calculations exhibit a lifetime of 187 ps (Table S1). The observed τ1 = 170 ps thus reflects the weighted average of reduced bulk annihilation, shallow trap contributions (dislocations), and neutral oxygen vacancy trapping. Although the presence of such defects would typically lead to a τ1 value exceeding the bulk lifetime, the reduced bulk contribution – with its intrinsically shorter lifetime and higher annihilation probability – appears to dominate. This indicates that the influence of defect-related trapping is relatively minor, and the reduced bulk state largely determines the observed τ1. Worth noting, because τ1 contains unresolved contributions from multiple defect types, absolute defect densities cannot be reliably calculated (see the PALS section in SI). This limitation applies equally to doped samples, where unresolved contributions from shallow traps and/or oxygen vacancies would similarly obscure individual defect signatures. Meanwhile, τ2 is more reliably assigned to annihilation at deeper defects. Based on DFT simulations (Table S2), τ2 corresponds to positrons trapped at big neutral clusters involving Gd atoms (ca. V10_Gd), as shown in Fig. 6b. Likely, these defect clusters are located at grain boundaries.
XRD analysis (Table 1 and Fig. 3) confirms lattice contraction and increased microstrain in the Yb3+/Er3-doped samples, consistent with dopant-induced structural distortion. While dislocations may be still present, their limited trapping efficiency at room temperature renders their contribution to τ1 relatively minor. More importantly, the observed τ1 = 186 ps matches well with DFT predictions for neutral V_O (Table S1), indicating their enhanced formation. Despite the isovalent nature of Yb3+/Er3+, their size mismatch perturbs the bonding network, facilitating V_O generation. Temperature-dependent PALS (Fig. S19) further supports this interpretation: the change is less pronounced than in the undoped reference. In the doped state, this weaker temperature dependence of τavg (constant values until 100 K) implies a shift in the dominant trapping mechanism. Specifically, it suggests that positron annihilation predominantly occurs in neutral defects, V_O, which remain effective across the temperature range. The increasing abundance of V_O in the Yb3+/Er3+ doped material thus tends to stabilize τavg closer to its room temperature value, effectively masking the temperature sensitivity typically associated with shallower traps.
Simultaneously, the longer lifetime component τ2 increases from 348 ps in the undoped sample to 384 ps in the doped case (Fig. 6b). Based on DFT modeling, this value corresponds to annihilation at quite larger open-volume defects such as twenty-atom gadolinium vacancy clusters (V20_Gd), which likely form at grain boundaries under the influence of accumulated strain.
Interestingly, the intensities I1 and I2 remain nearly unchanged compared to the undoped GdVO4 (Fig. 6d and e), indicating that the overall positron trapping probability has not substantially increased, despite the introduction of additional defect types such as neutral V_O and large gadolinium vacancy clusters (V20_Gd). Similarly, the average positron lifetime τavg (Fig. 6c) exhibits only minor variation upon doping. This outcome may seem unexpected, given the considerable reduction in crystallite size from 44 ± 2 nm in the undoped sample to 29 ± 1 nm in the Yb3+/Er3+-doped material – an effect typically associated with enhanced positron trapping at grain boundaries, which would be reflected by an increase in I2. The stable value of I2, however, suggests that positron trapping at bulk-related defects, effectively competes with trapping at grain boundaries. This indicates a reduced positron diffusion length, limiting the probability of positrons reaching grain boundaries before annihilation. Consequently, the effective defect density probed by τavg remains nearly constant, highlighting the dominant role of bulk trapping centers in the doped material.
Notably, the vacancy cluster-related positron lifetime component, τ2, remains essentially unchanged upon Sc3+ co-doping (Fig. 6b), indicating that the nature and size of these open-volume defects are not significantly altered. In contrast, the intensities I1 and I2 exhibit notable variation as a function of Sc3+ concentration (Fig. 6d and e). This behavior can be interpreted in the context of crystallite size evolution. At 5% Sc3+, the average crystallite size (∼30 nm) permits a larger fraction of positrons to diffuse toward and annihilate at vacancy clusters located at grain boundaries, contributing to the elevated I2. However, when the Sc3+ concentration increases to 15%, the crystallite size expands to ∼51 nm, thereby increasing the likelihood that positrons annihilate within the bulk-like regions before reaching the grain boundaries. This shift results in an increase in I1 and a corresponding decrease in I2.
Although the average positron lifetime, τavg, changes with increasing Sc3+ content (Fig. 6c), this should not be taken as a direct indication of altered defect concentration. The individual lifetime components, τ1 and τ2, remain nearly constant, indicating that the nature and size of annihilation sites do not significantly change. Instead, variations in τavg mainly result from changes in the relative intensities I1 and I2, which represent the fraction of positrons annihilating in the crystal bulk versus vacancy clusters near grain boundaries. Due to the change in crystallite size with Sc3+ doping, it is difficult to separate positron trapping at specific defects from general annihilation influenced by crystallite size. Therefore, the decrease in τavg with increasing Sc3+ content is mainly driven by microstructural effects – specifically the spatial distribution of annihilation sites – rather than a reduction in defect concentration.
The second positron lifetime component, τ2, associated with larger vacancy clusters or extended open-volume defects, increases to 406 ps at 5% Cd, which is characteristic of large Gd vacancy clusters such as >V20_Gd, Table S1, but this size is considered a rough estimate since the exact cluster geometry has an influence on the open volume and therefore calculated lifetime. At 15% Cd, τ2 decreases to a value indicative of smaller clusters close to the reference sample (390 ps for ∼V20_Gd), suggesting a possible recombination or fragmentation of vacancy clusters as the Cd content increases. The intensity parameters I1 and I2 also evolve with Cd doping: I1 increases at 5% Cd, reflecting a greater proportion of positrons annihilating in monovacancies, while I2 decreases, indicating a reduced fraction of positron annihilation in larger vacancy clusters. This behavior persists at 15% Cd doping; however, the increase in I1 does not scale proportionally with Cd content, indicating that the formation of Gd monovacancies occurs in a nonlinear manner with respect to Cd2+ concentration.
The average positron lifetime, τavg, decreases with Cd doping almost linearly (Fig. 6c). Crucially, XRD analysis shows that the crystallite size remains nearly constant at approximately 80 nm for both 5% and 15% Cd-doped samples. This constancy confirms that the variations observed in positron annihilation parameters – particularly in τavg – are indicative of intrinsic modifications in the defect structure. It further suggests that the overall defect density decreases with increasing Cd content, primarily due to a reduction in the density of defect clusters located at grain boundaries.
A key difference in Zn2+ co-doping emerges in the defect cluster behavior. The τ2 component exhibits a marked decrease with increasing Zn2+ concentration, reflecting a progressive reduction in the size of vacancy clusters at grain boundaries. This decline results in τ2 values that are even shorter than those measured in undoped GdVO4, indicating a significant suppression of defect clustering.
Regarding intensities, both I1 and I2 change with Zn content, but these variations can be largely attributed to the increase in crystallite size, which grows from approximately 30 nm in the undoped sample to 78 nm at 5% Zn and 88 nm at 15% Zn. Larger crystallites enhance the probability that positrons annihilate within the bulk, thereby increasing I1 and reducing I2, which corresponds to positron annihilation at vacancy clusters near grain boundaries. This microstructural effect must be considered alongside defect evolution when interpreting intensity changes.
The decreasing τavg must be treated with caution. While the reduction in τavg may suggest a decrease in overall defect density, it also reflects a shift in the nature and size of the trapping sites. Given the strong influence of crystallite size on intensity components, it is not possible to unambiguously attribute this trend to a lower total defect density, like in the Sc3+ case. However, the consistent decline in τ2 suggests that large defect clusters become smaller with Zn co-doping.
By combining PALS results with structural characterization by XRD, the following table can be provided. The data in Table 3 indicate that dopant valence strongly influences defect types: isovalent ions (Yb3+, Er3+, Sc3+) mainly cause lattice strain, while aliovalent dopants (Cd2+, Zn2+) induce additional charge compensation defects. Ionic size mismatch drives defect formation, especially oxygen vacancies (V_O), with larger mismatches increasing defect prevalence. Crystallite size affects positron annihilation sensitivity – small crystallites (∼29 nm) enhance defect detection at boundaries, whereas larger ones (∼88 nm) favor bulk annihilation signals.
| Doping system | Primary defects | Key evolution pattern | Cluster behavior | Crystallite size | PLQY trend |
|---|---|---|---|---|---|
| GdVO4:Yb/Er | V_O dominant | Size mismatch → V_O formation | V20_Gd clusters | 29 nm | Baseline |
| GdVO4:Yb/Er/Sc | V_O suppressed | Lattice contraction → V_O elimination | Clusters unchanged | 30 → 51 nm | ↑ |
| GdVO4:Yb/Er/Cd | V_Gd dominant | Charge compensation → strong V_Gd | > V_20 → V20_Gd fragmentation | ∼80 nm | ↓ |
| GdVO4:Yb/Er/Zn | V_Gd + V_O mixed | Partial charge compensation | Progressive cluster suppression | 78 → 88 nm | ↑↑ |
For a comparative analysis over the samples and to link the structural defects to the PQLY, one observes the PLQY trend: Cd2+ < Sc3+ < Zn2+ (lowest → highest), as summarized in Table 3. This observed trend is directly correlated with the distinct defect microstructures and their impact on radiative and non-radiative recombination pathways, as elaborated below:
(i) Charge compensation and vacancy type: aliovalent doping with Cd2+ and Zn2+ leads to the formation of Gd vacancies (V_Gd), while Sc3+, being isovalent, does not induce such defects. However, PLQY trends do not correlate directly with vacancy presence. Although Zn2+ introduces V_Gd, it exhibits the highest PLQY – highlighting that the type and arrangement of defects, rather than their presence alone, is crucial.
(ii) Defect cluster size and distribution: a major distinguishing factor is the extent of defect clustering. Cd2+-doped samples show the formation of large, spatially extended V_Gd clusters, which act as efficient non-radiative quenching centers, thereby suppressing PLQY. In contrast, Zn2+ shows a marked suppression in defect cluster growth, leading to smaller defect sites that reduce quenching. This cluster suppression appears to be the key factor governing the improved PLQY in Zn.
(iii) Grain boundary vs. crystallite contributions: PALS data suggest that Zn2+ may additionally favor the localization of beneficial oxygen vacancies (V_O) within crystallite interiors rather than at boundaries, while simultaneously minimizing extended defect structures at grain interfaces. This spatial redistribution of defects supports radiative recombination pathways and further boosts luminescence efficiency.
(iv) Scandium case – minimal point defects but clustered vacancies: although Sc3+-doped samples show defect clusters of comparable size to Cd2+ at high co-doping levels, their PLQY is significantly better. This improvement can be attributed to the lack of point defects like V_Gd and V_O and a more compact, structurally ordered lattice, which compensates for the quenching effect of vacancy clusters and supports moderately efficient light emission.
To this end, the superior PLQY observed in Zn-doped GdVO4 can be primarily attributed to the suppression of defect cluster formation, which drastically reduces non-radiative recombination. Additionally, a favorable distribution of oxygen vacancies inside the crystallites, rather than at grain boundaries, may contribute synergistically. These effects outweigh the influence of microstrain or simple vacancy presence.
PALS, alongside X-ray diffraction and optical measurements, reveals that aliovalent dopants such as Cd2+ and Zn2+ introduce charge imbalance that is compensated by the formation of Gd vacancies. However, the structural response to this compensation varies significantly between the two systems. In the case of Cd2+ co-doping, charge compensation leads to the formation of large and spatially extended vacancy clusters, potentially concentrated at grain boundaries. These clusters act as effective non-radiative recombination centers, significantly quenching the UC emission and resulting in low PLQY. Despite exhibiting relatively low microstrain, the defect morphology in the Cd2+ system remains detrimental due to the high degree of defect clustering.
By contrast, Zn2+ co-doping results in a markedly different defect structure. Although similar charge compensation mechanisms are at play, the Zn2+-doped system suppresses the expansion of vacancy clusters, leading to more confined and less interconnected defect configurations. This refined cluster morphology reduces the density of non-radiative quenching sites, particularly at grain interfaces, while potentially preserving optically active oxygen vacancies within the crystallites. The resulting defect topology enables a more favorable radiative-to-nonradiative recombination balance and corresponds to the highest observed PLQY among the systems investigated.
The case of Sc3+ co-doping offers a contrasting scenario where no charge compensation is required. The absence of aliovalent substitution leads to a more compact lattice with negligible formation of point defects. While defect clusters persist – likely remnants from synthesis or structural relaxation – they are not accompanied by high internal strain or deep trapping states. Consequently, the PLQY in the Sc3+ system is superior to that of Cd2+-doped samples but remains lower than in Zn2+ due to the lack of beneficial oxygen vacancies and the persistence of moderate-sized clusters.
Isovalent co-doping with Bi3+ and In3+ – both of which possess larger ionic radii compared to Sc3+ – leads to the formation of larger microcrystals with reduced lattice strain. This structural modification contributes to an increase in PLQY at lower doping concentrations (5%). However, at higher doping levels (15%), the PLQY values remain comparable across all three dopants: Sc3+, Bi3+, and In3+.
Overall, the findings demonstrate that optimizing UC performance is not simply a matter of reducing total defect density, but rather of engineering the size, location, and distribution of defect clusters within the microstructure. Zn2+ co-doping achieves the most advantageous configuration by combining efficient charge compensation with spatial control over defect clustering and potential redistribution of optically beneficial defects. These mechanistic insights underscore the importance of targeted defect engineering in the design of efficient UC materials and establish PALS as a critical technique for decoding the structure–luminescence relationships at the nanoscale.
The data that support the findings of this study are available from the corresponding author upon reasonable request.
Footnotes |
| † Equal contribution. |
| ‡ Present address: Reactor Institute Delft, Department of Radiation Science and Technology, Faculty of Applied Sciences, Delft University of Technology, Mekelweg 15, NL-2629 JB Delft, The Netherlands. |
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