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Enhanced Luminescence and Thermal Stability in High Gd3+/Eu3+ Co-Doped Ba3Y4O9 Phosphors via Co-Precipitation Method

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31 January 2025

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03 February 2025

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Abstract

The co-precipitation method was successfully used to synthesize BYGO: Eu3+ phosphors with high Gd3+ doping, resulting in significantly enhanced thermal stability and luminescence performance. Structural analyses confirm that Gd3+ and Eu3+ ions substitute Y3+ in the lattice, causing lattice expansion and improving crystal asymmetry, which enhances Eu3+ emission. The incorporation of Gd3+ creates efficient energy transfer pathways to Eu3+ while suppressing non-radiative relaxation, leading to stable fluorescence lifetimes even at elevated temperatures. With a thermal activation energy of ~0.3051 eV, the BYGO: Eu3+ system exhibits superior resistance to thermal quenching compared to BYO: Eu3+ and many conventional red phosphors. Furthermore, the reduced color temperature and stable emission spectra across a wide temperature range highlight its potential for advanced lighting and display technologies in high-temperature environments.

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1. Introduction

Inorganic phosphors play a crucial role in white light-emitting diodes (W-LEDs) due to their high luminous efficiency, strong brightness, and long operational lifespan, making them indispensable in the lighting industry. The most advanced commercial W-LEDs typically combine gallium nitride (GaN) blue LED chips with Y3Al5O12: Ce3+ yellow phosphors [1,2,3]. However, these systems face limitations, including a low color rendering index and high correlated color temperature (CCT), primarily due to insufficient red emission from the phosphor and the dominance of blue light emitted by the LED chip [4,5]. Moreover, the performance of red phosphors often deteriorates under high-temperature conditions, as their emission intensity is affected by radiation transitions and the thermal effects of the chip, further limiting their practical applications in scenarios requiring vivid color rendering. To overcome these challenges, recent research has focused on UV-excited phosphors, utilizing red, green, and blue tricolor emissions to generate white light [6,7,8]. By optimizing doping levels and selecting appropriate tricolor phosphor combinations, W-LEDs with low CCT, high brightness, and superior color quality can be achieved [9,10,11,12]. Enhancing the red emission intensity and thermal stability of phosphors remains a critical objective for advancing next-generation W-LED technologies suitable for high-performance lighting applications.
Phosphor materials for W-LEDs generally feature an inert host lattice that provides a stable luminescent environment, with optically active ions serving as activators. Ba3Y4O9 (BYO) has emerged as a promising host material for red phosphors due to its unique physicochemical properties [13,14,15,16]. Compared to conventional hosts like Y2O3 and Gd2O3, BYO offers superior structural stability, an optimal bandgap (~3.436 eV), lower phonon energy, and a higher proportion of asymmetric lattice sites, making it highly compatible with Eu3+ doping [17,18]. The 4f energy levels of Eu3+ lie outside BYO's band structure and align well with its electronic configuration, facilitating the formation of discrete luminescent centers [19]. However, the luminescence efficiency of BYO: Eu3+ decreases significantly at elevated temperatures, limiting its practical application in high-temperature environments [20]. Enhancing the thermal stability and high-temperature performance of BYO: Eu3+ is therefore essential for advancing its utility in lighting technologies.
The absorption spectrum of Eu³⁺ primarily involves 4f-4f transitions. These transitions are parity-forbidden for electric dipole transitions and only allow weak magnetic dipole transitions, resulting in narrow bands and low absorption efficiency [21,22,23]. When the electrons in the 2p orbitals of ligand oxygen (O2-) are transferred to the partially filled 4f orbitals of Eu3+, a broad charge transfer band (CTB) appears in the excitation spectrum, significantly enhancing the absorption of excitation energy[24,25]. However, due to the limited intensity of f-f transitions in rare-earth ions, the direct excitation efficiency of Eu³⁺ is low. To address this, Gd3+ is introduced as a sensitizer, whose characteristic excitation peaks overlap with the CTB of Eu3+, enabling efficient energy absorption and transfer, thereby enhancing the luminescence efficiency of Eu3+ [26]. With its half-filled f⁷ configuration, Gd3+ exhibits ⁸S₇/₂→⁶Iⱼ and ⁸S₇/₂→⁶Pⱼ transitions that partially overlap with the CTB of Eu3+, facilitating efficient energy transfer. Li et al. demonstrated that Eu3+ emission behavior in Y₂O₃ and (Y0.75Gd0.25)2O3 revealed this overlap but lacked a mechanistic model for explanation [27]. Mancic et al. demonstrated that substituting Y3+ with Gd3+ in LnTeBO5 stabilized the lattice, reduced the charge transfer barrier, and improved luminescence intensity and thermal stability, though the thermal activation energy remained low at ~0.26 eV [28]. In this study, BYGO:Eu3+ precursor materials were synthesized via a co-precipitation method, and rapid high-temperature annealing successfully stabilized a high Gd3+ doping concentration of 40 a.t.% within the BYO lattice, far exceeding the reported limit of 12% [29]. By analyzing the characteristic emission peaks of Gd3+ and Eu3+, an energy transfer model from Gd3+→Eu3+ was established. Thermal quenching experiments demonstrated excellent thermal stability, while the consistent CCT values at elevated temperatures further confirmed that BYGO: Eu3+ phosphors are promising candidates for W-LED applications in high-temperature environments.

2. Results and Discussion

Figure 1a illustrates the synthesis process of BYGO: Eu3+ phosphors using a co-precipitation method. First, precursor solutions were prepared in specific proportions and fully dissolved. These solutions were then slowly added dropwise into an ammonium bicarbonate solution using a separatory funnel. Throughout the titration process, the solution's pH was continuously monitored with a pH meter and maintained at 10 by adding ammonium hydroxide. After titration, the mixture was stirred for an additional 6 hours to ensure a complete reaction. The resulting precipitate was washed multiple times, with the final wash performed using n-hexane to remove any residual organic impurities. The washed product was dried at 60 oC for 12 hours in an oven to obtain the precursor. This precursor was then calcined at a ramping rate of 1 oC /min to 1400 oC, held at the target temperature for 6 hours, and rapidly cooled to room temperature to yield the BYGO: Eu3+ phosphors. Figure 1b shows the SEM images of the BYGO: Eu3+ phosphors synthesized by the co-precipitation method. The phosphor particles are approximately 1 μm in size, exhibiting irregular shapes and noticeable voids between particles. These voids are attributed to the decomposition of HCO3- and CO32- in the precursor during heating [30]. The connections between particles result from the sintering process, where ~40 nm precursor particles underwent grain growth during high-temperature calcination (Figure S1). Energy-dispersive spectroscopy (EDS) mapping confirms the uniform distribution of Ba, Y, Gd, Eu, and O elements throughout the phosphors, which facilitates more efficient luminescence performance.
Figure 1c presents high-resolution transmission electron microscopy (HR-TEM) images of BYGO: Eu3+ phosphors. The particles exhibit slight aggregation, and their size aligns with the SEM results. The selected area electron diffraction (SAED) pattern reveals bright spot rings, indicating high crystallinity and confirming the formation of a polycrystalline BYO host structure consistent with JCPDS No.038-1377. In the HRTEM images of the optimized nanoscale samples, distinctive lattice fringes are observed with an interplanar spacing of 3.094 Å, closely matching the standard value of 2.7954 Å for the (1 0 7) crystal plane of the Ba3Y4O9 host. However, the spacing is increased by ~0.1186 Å, indicating a lattice expansion of approximately 4.0%. This expansion results from the substitution of Y3+ ions with larger Gd3+ and Eu3+ ions in the BYO lattice. Figure 1d displays the XRD patterns of undoped and doped BYO samples. All patterns match well with the standard Ba3Y4O9 data, with no additional diffraction peaks observed, confirming that the dopant ions were fully incorporated into the BYO lattice without forming impurity phases. The magnified main peak detail on the right further reveals that, with the doping of Eu³⁺ and Gd³⁺, all diffraction peaks shift toward smaller angles, accompanied by a deterioration in crystallinity. This indicates that the excessive substitution of the original lattice Y³⁺ ions by the larger Gd³⁺ and Eu³⁺ ions leads to lattice expansion and structural changes.
Figure 2a presents the PLE spectra of Eu3+-doped BYO and BYGO systems, showing two primary components. The first component is a broadband excitation peak centered at 258 nm (CTB), spanning the 220–330 nm short-wavelength region. This peak arises from the charge transfer transition of electrons from the 2p orbitals of O2- to the empty 4f orbitals of Eu3+, forming an excited state [24]. The second component consists of several sharp excitation peaks in the 313–538 nm long-wavelength region, corresponding to the 4f-4f transitions of Eu3+. These include ~363 nm (7F05D4), ~385 nm (7F05G4), ~395 nm (7F05L6), ~417 nm (7F05D3), ~465 nm (7F05D2), and ~538 nm (7F05D1) [31]. Among these, the CTB intensity is significantly higher than that of the intra-4f transitions, indicating that CTB excitation is the most effective method to achieve fluorescence in the Eu3+-doped BYO system. Notably, the peak at 394 nm (7F05L6) exhibits the highest intensity among the 4f-4f transitions [32]. This hypersensitive transition is highly dependent on the strength of the crystal field, meaning even minor variations in the local structure or surrounding environment of Eu3+ can significantly affect its intensity. Additionally, two extra peaks at 275 nm and 315 nm appear in the BYGO system, attributed to the 8S7/26IJ and 8S7/26PJ transitions of Gd3+. The 275 nm peak overlaps with the CTB, enabling efficient energy transfer from Gd3+→Eu3+ [33]. Figure 2b shows the PL spectra of Eu3+-doped BYO and BYGO systems under 258 nm (CTB) excitation. Six emission peaks are detected, with the most prominent one at ~612 nm (5D07F2), which corresponds to an electric dipole transition [34]. This transition is highly sensitive to lattice asymmetry due to the symmetry-breaking effect of the 4f orbitals in non-centrosymmetric environments. The split peaks in the orange region (~589 nm, ~595 nm, and ~601 nm) result from the magnetic dipole transition (5D07F1), which occurs in centrosymmetric environments. The asymmetry of the Eu3+ local environment is reflected in the intensity ratio (IR/O) of the 5D07F2 and 5D07F1 transitions. In the BYO system, the IR/O value is 2.92, indicating a highly asymmetric local environment for Eu3+ ions. In the BYGO system, the IR/O ratio increases slightly (~3.06), attributed to the lattice expansion caused by the larger ionic radius of Gd3+ (~1.053 Å, CN=8) compared to Y3+ (~1.040 Å, CN=8), which enhances asymmetry. Additionally, as a common sensitizer, Gd3+ significantly enhances Eu3+ emission, increasing the overall PL intensity of BYGO by ~135% compared to BYO under identical conditions (Figure S2). The inset shows the emission intensity trend for different Eu3+ doping concentrations, consistent with previously reported studies [35].
Figure 2c evaluates the quantum efficiency (QE), a critical parameter determining phosphor brightness (see Note S1 for QE calculation). For BYO and BYGO systems, the maximum QE is achieved at the quenching concentration (~5% Eu3+), reaching ~55% and ~86%, respectively (Figure S3). The QE trends align with those of the PL intensity, confirming that doping concentration strongly influences luminescence properties. In the Gd3+/Eu3+ co-doped systems, Martins et al. measured a quantum efficiency (QE) of 48% in Y2O3 [36], while Liu et al. reported a QE of 70.6% in LiGd0.5Eu0.5MgWO6 [37], both of which are lower than that of BYGO system.
To confirm the substitution of Y3+ by Gd3+ in the BYO lattice, Figure 2d-f presents the Rietveld refinement results for BYO, BYO: 5% Eu3+, and BYGO: 5% Eu3+, analyzed using Topas software. Comparative analyses of the structural parameters are summarized in Table S1, with refinement parameters detailed in Tables S2–S4. The results confirm that the ionic radii of Gd3+ (~0.938 Å, CN=6; ~1.053 Å, CN=8) and Eu3+ (~0.950 Å, CN=6; ~1.066 Å, CN=8) are larger than that of Y3+, making excessive doping prone to introducing impurity phases. However, the use of chemical co-precipitation and rapid cooling at 1350 oC effectively traps impurity ions within the lattice, reducing their escape probability. Calculations indicate that ~4.9 at.% Eu3+ and ~38.15 at.% Gd3+ successfully replaced Y3+ sites, with the lattice volume expanding by ~3.19%. This conclusion is consistent with the lattice expansion observed in the TEM results (Figure 1c).
Excessive doping of Gd3+ not only influences the lattice sites but also modifies the original luminescence mechanism in the BYO: Eu3+ system [36]. To investigate the role of Gd3+ as a sensitizer in enhancing luminescence in the BYGO: Eu3+ system, PLE spectra were measured using the characteristic emission wavelength of Gd3+ at ~315 nm as the monitoring wavelength, as shown in Figure 3a(i). The spectra reveal a distinct excitation peak at ~275 nm corresponding to the 8S7/26Pj transition, along with additional peaks at ~244 nm and ~252 nm, attributed to the 8S7/26Ij transitions. These peaks are absent in the PLE spectra of BYO: 5% Eu3+, confirming that they are directly related to the presence of Gd3+. Figure 3a(ii) demonstrates a positive correlation between peak intensity and Gd3+ concentration, but when the Gd3+ content exceeds 40%, a phase transition occurs in the BYGO system, as shown in Figure S4, establishing 40% as the maximum doping level to maintain the pure-phase structure. PL spectra under different monitoring wavelengths are presented in Figure 3b. For BYO: 5% Eu3+, the PL intensity is weak when excitation wavelength at 275 nm, as this wavelength lies within the CTB excitation range of Eu3+. In contrast, the PL spectrum of BYGO: 5% Eu3+ shows not only the characteristic emission peaks of Eu3+ but also a strong emission peak at ~315 nm corresponding to the 6Pj8S7/2 transition of Gd3+. This indicates that a significant portion of the ultraviolet energy absorbed by the system is released as Gd3+ emission, while only a small fraction is transferred to Eu3+ through energy transfer, as shown in Figure 3b(i). When the monitoring wavelength is shifted to 258 nm (Figure 3b(ii)), the Gd3+ emission peaks are nearly absent, leaving only the strong characteristic emissions of Eu3+. This suggests that under 258 nm excitation, nearly all energy in the system is efficiently transferred to Eu3+.
Based on the Judd-Ofelt theory, the energy transfer mechanism in the BYGO: Eu3+ system is depicted in Figure 3c. At an excitation wavelength of 275 nm, the BYO: Eu3+ system shows weak emission because, although this wavelength is not the optimal excitation wavelength, it still falls within the CTB region of Eu3+, allowing for low-efficiency photon absorption. In contrast, the BYGO: Eu3+ system exhibits a sharp and intense ultraviolet emission (~315 nm). This energy corresponds to the transition of Gd3+ from the 8S7/26IJ energy level, with a portion of the energy transferred to Eu³⁺, as the 6Iⱼ level overlaps with Eu3+’s CTB. Additionally, some Gd3+ ions undergo the 6IJ6PJ transition, and the energy difference generated in this process is suitable for Eu3+’s 5D0 energy level absorption, promoting the characteristic Eu3+ emission [38]. Therefore, as shown in Figure 3b i, the emission intensity of BYGO: Eu3+ at 612 nm is stronger than that of BYO: Eu3+. At an excitation wavelength of 258 nm, the BYO: Eu3+ system directly absorbs photon energy, with electrons transitioning from the ground state ⁷F₀ to the CTB and subsequently relaxing non-radiatively to the 5D0 excited state. This is followed by a radiative transition to the 7FJ (J = 0, 1, 2, 3, 4) states, emitting orange-red light. In the BYGO: Eu3+ system, electrons transition from the 8S7/26DJ, with energy transfer occurring through multiple Gd3+ ions in the lattice, concentrating the excitation energy onto a few high-energy Gd3+ ions. These high-energy Gd3+ ions then efficiently transfer energy to Eu³⁺. The better energy level matching between high-energy Gd³⁺ and Eu³⁺ significantly enhances the energy transfer efficiency from Gd3+→Eu3+. Therefore, in Figure 3b ii, the characteristic emission of Gd3+ is nearly absent, and only the intense Eu³⁺ emission is observed. These processes work synergistically, achieving efficient energy transfer from Gd3+→Eu3+ [39].
Phosphor materials are often required to perform under diverse operational environments, with thermal stability being a critical factor, especially at elevated temperatures [40,41]. Higher temperatures intensify lattice vibrations, increase non-radiative relaxation pathways, and lead to reduced luminescence efficiency and fluorescence lifetime, culminating in thermal quenching [42]. However, the incorporation of substantial amounts of Gd3+ has been shown to effectively mitigate these issues. As demonstrated in Figure 4a, the temperature-dependent PL spectra of BYO: Eu3+ and BYGO: Eu3+ phosphors reveal that at 300 K, the emission intensity of BYO is 53.52% of BYGO. As the temperature increases to 450 K, this ratio decreases to 20.14%, indicating that BYO exhibits a faster decline in emission intensity. Within the practical operating temperature range for LEDs (~400 K), the emission intensity of BYGO retains 59.56% of its initial value at 300 K, whereas BYO retains only 20.26%, clearly highlighting the improved thermal stability conferred by Gd3+ doping. To investigate the underlying mechanism, the temperature-dependent fluorescence decay lifetimes of BYO: Eu3+ and BYGO: Eu3+ phosphors were measured, as shown in Figure 4b. The fluorescence lifetime (τ) was calculated using the method outlined in Note S2. As the temperature increases from 300 K to 450 K, under the detection conditions of an excitation wavelength of 258 nm and an emission wavelength of 612 nm, the τ of BYO: 5% Eu3+ decreases significantly from ~1.038 ms to ~0.774 ms. In contrast, under the same detection conditions, the τ of BYGO: 5% Eu3+remains relatively stable at ~0.744 ms. In the undoped BYO: Eu3+ system, 2p electrons of O²⁻ transfer energy to Eu3+ through the CTB, exciting its 4f states [43]. The energy is subsequently dissipated via phonon-mediated non-radiative relaxation, a process that becomes increasingly pronounced at higher temperatures, leading to shorter excited-state lifetimes and diminished radiative efficiency. In contrast, the introduction of Gd3+ induces lattice expansion and increases structural asymmetry, effectively reducing lattice stress and defect density, thereby suppressing multi-phonon relaxation. Furthermore, the efficient energy transfer pathway from Gd3+ to Eu3+ enhances Eu3+ emission intensity while minimizing non-radiative relaxation [44]. This mechanism ensures that the BYGO system exhibits superior fluorescence lifetime stability at elevated temperatures, significantly mitigating thermal quenching effects.
The thermal activation energy (Ea), calculated using the Arrhenius equation, provides a quantitative measure of thermal quenching resistance. As shown in Figure 4c, the Ea of BYO: 5% Eu3+ is 0.1688 eV, while that of BYGO: 5% Eu3+ increases significantly to ~0.3051 eV. This value surpasses those reported for many red phosphors (see Table S5), underscoring the enhanced thermal stability of the BYGO system due to Gd3+ doping.
To further investigate the effect of Gd3+ doping on luminescent properties, Figure 4d illustrates the CIE chromaticity coordinates of BYO: 5% Eu3+ and BYGO: 5% Eu3+ at different temperatures. As the temperature increases, the CIE coordinates of BYO: 5% Eu3+ exhibit significant shifts, moving from the red region at (0.6382, 0.3258) to the orange region at (0.5951, 0.3008). This change is attributed to intensified lattice expansion at elevated temperatures, where the 5D07F2 electric dipole transition at 612 nm, being more sensitive to the local coordination environment, undergoes faster thermal quenching compared to the 5D07F1 magnetic dipole transition at ~538 nm. In contrast, BYGO: 5% Eu3+ maintains stable CIE coordinates at (0.6524, 0.3471) across the entire temperature range, benefiting from a more stable lattice structure and reduced influence of phonon energy on energy transfer. The CCT values, calculated using the method detailed in Note S4 and summarized in Table S6, further corroborate this stability. The CCT of BYO: 5% Eu3+ varies between 3161 K and 3468 K, while BYGO: 5% Eu3+ consistently achieves a lower CCT of approximately 2700 K, which is favorable for improved color rendering [45]. These findings indicate that Gd3+ doping not only enhances luminescence intensity and efficiency but also significantly improves lattice stability and thermal resistance. Such advancements provide a novel design approach for lighting applications in dynamic and high-temperature environments.
Figure 1a Synthesis process of BYGO: Eu3+ phosphor. Figure 1b FE-SEM and EDS Mapping of BYGO: Eu3+ phosphor. Figure 1c FE-TEM analysis of BYGO: Eu3+ phosphor. Figure 1d XRD pattern of BYGO: Eu3+ phosphor, with an enlarged detail of the main peak on the right.
Figure 2a Comparison of the PLE spectra of BYO: Eu3+ and BYGO: Eu3+. Figure 2b Comparison of the PL spectra of BYO: Eu3+ and BYGO: Eu3+. Figure 2c Comparison of the quantum efficiency (QE) of BYO: 5% Eu3+ and BYGO: 5% Eu3+. Figure 2 d, e, f XRD patterns of BYO, BYO: Eu3+, and BYGO: Eu3+, respectively, refined using the Topas software.
Figure 3a Comparison of PLE spectra with an excitation wavelength of 315 nm, i) comparison of the PLE spectra of BYO: 5% Eu3+ and BYGO: 5% Eu3+, ii) comparison of PLE spectra with a fixed doping of 5% Eu3+ while varying the Gd content. Figure 3b comparison of the PL spectra of BYO: 5%Eu3+ and BYGO: 5% Eu3+ at different excitation wavelengths, i) comparison of PL spectra at a excitation wavelength of 275 nm, ii) comparison of PL spectra at the normal excitation wavelength of 258 nm. Figure 3c Schematic diagram of energy transfer in the BYGO: 5% Eu3+ system.
Figure 4a Comparison of photoluminescence (PL) spectra of BYO: 5% Eu3+ and BYGO: 5% Eu3+ at different temperatures. Figure 4b Comparison of PL spectra of BYO: 5% Eu3+ and BYGO: 5% Eu3+ at different temperatures. Figure 4c Thermal quenching activation energy of BYO: 5% Eu3+ and BYGO: 5% Eu3+. Figure 4d CIE color coordinates of BYO: 5% Eu3+ and BYGO: 5% Eu3+ at different temperatures.

3. Materials and Methods

Barium nitrate (Ba(NO3)2, 99.999%), yttrium nitrate hexahydrate (Y(NO3)3·6H2O, 99.99%), gadolinium nitrate hexahydrate (Gd(NO3)3·6H2O, 99.99%), and europium nitrate hexahydrate (Eu(NO3)3·6H2O, 99.99%) were procured from Alfa Aesar (China) Chemical Co., Ltd. Ammonium bicarbonate (NH4HCO3, 99.995%), n-hexane (C6H14, UV/VIS spectroscopy grade), and absolute ethanol (CH₃CH₂OH, 99.8%) were supplied by Shanghai Aladdin Biochemical Technology Co., Ltd. All reagents were of analytical grade and used as received without further purification.
For each synthesis of the BYGO: Eu3+ precursor, stoichiometric amounts of nitrate salts were precisely weighed according to their atomic ratios and dissolved in ultrapure water to prepare 250 mL of solution. This solution was slowly added dropwise into an ammonium bicarbonate solution while maintaining a constant pH of 10 by the controlled addition of dilute ammonium hydroxide. After the titration, the suspension was stirred continuously for 6 hours to ensure complete homogenization. The resulting precipitate was washed thoroughly with deionized water and n-hexane to remove impurities, followed by drying at 65 oC for 6 hours to obtain the precursor powder. The dried precursor was calcined in a muffle furnace (Nabertherm LHT 08-18, Germany) at a heating rate of 1 oC/min. The temperature was raised to 1350 oC and maintained for 5 hours. At the end of the calcination process, the phosphor samples were extracted from the furnace at 1350 oC and rapidly cooled to room temperature to facilitate phase transformation. The cooled phosphor powders were ground finely using an agate mortar and pestle and then sieved through a 1000-mesh stainless steel sieve (15 μm pore size) to achieve uniform particle size distribution.
The surface morphology of the phosphor materials was examined using a field emission scanning electron microscope (FE-SEM, Hitachi SU-70) equipped with an energy-dispersive spectroscopy (EDS) system operated at an accelerating voltage of 5 kV to analyze elemental composition. The nanoscale characteristics and lattice spacings of the samples were further analyzed by field emission transmission electron microscopy (FE-TEM, JEM-F200, JEOL). Selected area electron diffraction (SAED) patterns were also acquired using the TEM's integrated detector. X-ray diffraction (XRD) analysis of all samples was performed using a Rigaku SmartLab XRD system. Scans were conducted from 10o to 90o in 2θ, with a step size of 0.02o and a scanning speed of 0.05 seconds per step under ambient conditions (Cu Kα radiation, λ = 1.5412 Å). Structural refinement of the XRD data was carried out using the Le Bail method with Topas3 software to determine the crystal structure. Photoluminescence (PL) emission, photoluminescence excitation (PLE), and fluorescence decay curves were recorded using an Edinburgh Instruments FLS-1000 fluorimeter. Quantum efficiency (QE) was measured using a Horiba DeltaFlex instrument equipped with a 260 nm NanoLED laser, enabling precise evaluation of the phosphor's photoluminescent properties.

4. Conclusions

A series of BYO: Eu3+ phosphors were synthesized via co-precipitation, and doping with ~40% Gd3+ led to significant improvements in both luminescent performance and thermal stability. Structural analysis confirmed that Gd3+ substitution for Y3+ caused a lattice expansion of approximately 4.0%, which enhanced the energy transfer from Gd3+ to Eu3+, resulting in increased Eu3+ emission intensity. The quantum efficiency of BYGO: 5% Eu3+ reached ~86%, notably higher than the ~55% observed for BYO: 5% Eu3+. Thermal activation energy (Ea) for BYGO: Eu3+ was calculated to be ~0.3051 eV, significantly surpassing the ~0.1688 eV for BYO: Eu3+, indicating improved resistance to thermal quenching. Even at elevated temperatures (300 K to 450 K), BYGO: Eu3+ maintained a stable fluorescence lifetime (~0.744 ms) and a consistent color temperature (~2066 K), reflecting enhanced high-temperature color stability. These findings demonstrate that Gd3+ doping substantially improves the thermal and optical properties of the BYGO: Eu3+ system, making it highly promising for high-temperature applications in LED lighting and display technologies.

Supplementary Materials

The following supporting information can be downloaded at: Preprints.org, Figure S1: title; Table S1: title; Video S1: title. Figure S1 FE-SEM images of a single BYGO: 5% Eu3+ precursor (a) and the same precursor after calcination at 1350°C (b), showing significant morphological changes due to thermal treatment; Figure S2 Comparison of emission intensity between Eu3+-doped BYO and BYGO systems; Figure S3 Comparison of QE between BYO: Eu3+ and BYGO: Eu3+; Figure S4 XRD of Ba3Y2Gd1.8Eu0.2O9; Table S1 Crystal structure data interpretation of Ba3Y4O9, Ba3Y3.8Eu0.2O9 and Ba3Y2.2Gd1.6Eu0.2O9 phosphor with reference to standard Ba3Y4O9 host at room temperature 25 oC; Table S2 Diverse atomic parameters together with the refined atomic positions of Ba3Y4O9 phosphor; Table S3 Diverse atomic parameters together with the refined atomic positions of Ba3Y3.8Eu0.2O9 phosphor; Table S4 Diverse atomic parameters together with the refined atomic positions of Ba3Y2.2Gd1.6Eu0.2O9 phosphor; Table S5 Comparison of activation energy of the BYGO phosphor with some previously reported phosphors; Table S6 Colour temperature statistics of the samples; Note.S1 Quantum yields; Note S2 Decay time; Note S3 Activation Energy; Note S4 Colour temperature.

Author Contributions

Conceptualization, Dong Zhu and Youming Lu; methodology, Chunfeng Wang; software, Shun Han; validation, Peijiang Cao, Dong Zhu and Yuxiang Zeng; formal analysis, Dong Zhu and Youming Lu; investigation, Peijiang Cao; resources, Chunfeng Wang and Deliang Zhu; data curation, Dong Zhu and Youming Lu; writing—original draft preparation, Dong Zhu and Youming Lu; writing—review and editing, Dong Zhu and Youming Lu; visualization, Zhu and Yuxiang Zeng; supervision, Wenjun Liu; project administration, Deliang Zhu; funding acquisition, Youming Lu All authors have read and agreed to the published version of the manuscript.

Funding

This work was supported by the National Natural Science Foundation of China (Grant No. 52372154, 12074263, 51872187, and U22A2077), the Natural Science Foundation of Guangdong Province (Grant No. 2021A1515012013), the Shenzhen Science and Technology Innovation Commission (Grant No. JCYJ20240813142628038, JCYJ20220809152330002, JCYJ20180305124701756, JCYJ20180508163404043, JCYJ2018030507182248925), and the Shenzhen High-End Talent Scientific Research Program.

Informed Consent Statement

Informed consent was obtained from all subjects involved in the study.

Data Availability Statement

The original contributions presented in this study are included in the article/supplementary material. Further inquiries can be directed to the corresponding authors.

Conflicts of Interest

The authors declare no conflicts of interest.

Abbreviations

The following abbreviations are used in this manuscript:
W-LEDs White light-emitting diodes
BYO Ba3Y4O9
BYGO Ba3(Y0.6Gd0.4)4O9
CCT Correlated color temperature
CTB Charge transfer band
PL Photoluminescence
PLE photoluminescence excitation
QE Quantum efficiency
FE-SEM Field emission scanning electron microscope
EDS energy-dispersive spectroscopy
FE-TEM Field emission transmission electron microscopy
SAED Selected area electron diffraction
XRD X-ray diffraction
Ea Activation energy

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Figure 1. Synthesis and characterization of BYGO: Eu3+.
Figure 1. Synthesis and characterization of BYGO: Eu3+.
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Figure 2. Optical characterization of BYGO: Eu3+ phosphor.
Figure 2. Optical characterization of BYGO: Eu3+ phosphor.
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Figure 3. Energy transfer in BYGO: Eu3+ phosphor.
Figure 3. Energy transfer in BYGO: Eu3+ phosphor.
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Figure 4. Comparison of luminescent properties of BYO: 5% Eu³⁺ and BYGO: 5% Eu³⁺ at different temperatures.
Figure 4. Comparison of luminescent properties of BYO: 5% Eu³⁺ and BYGO: 5% Eu³⁺ at different temperatures.
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