DOI:
10.1039/D5QI00395D
(Research Article)
Inorg. Chem. Front., 2025,
12, 3663-3671
Achieving tunable ultra-broadband NIR emission originating from the two-site occupation of Cr3+ ions in Mg3Ga2SnO8:Cr3+†
Received
9th February 2025
, Accepted 8th March 2025
First published on 21st March 2025
Abstract
Near-infrared phosphor-converted light-emitting diodes (NIR pc-LEDs) are considered promising light sources for a variety of applications due to their cost-effectiveness, broadband emission, compact size, and high output power. The key to developing high-performance NIR pc-LEDs lies in the design of phosphors. In this study, we report a NIR Mg3Ga2SnO8:Cr3+ (MGS:Cr3+) phosphor synthesized via a traditional high-temperature solid-state method. Under 450 nm excitation, MGS:Cr3+ exhibited an intense tunable ultra-broadband NIR emission. By adjusting the concentration of Cr3+ ions, the full width at half maximum (FWHM) of the spectrum was observed to be broadened from 151 to 223 nm, while the peak wavelength shifted from 715 to 833 nm. Crystal structure analysis, low-temperature spectra, and fluorescence decay curves revealed that these fascinating tunable characteristics originated from the two-site occupation of Cr3+ ions. Additionally, the presented phosphor exhibited an impressive internal quantum efficiency (IQE = 57.8%) and superior photoluminescent thermal stability (I423 K/I303 K = 50%). Moreover, the fabricated NIR pc-LED devices based on the MGS:0.08Cr3+ and MGS:0.02Cr3+ samples proved their potential in night vision imaging, non-invasive detection, and plant growth illumination applications.
1. Introduction
Due to the invisibility and penetration ability of NIR light, NIR light sources have found wide applications across various fields, such as night vision imaging, plant growth illumination, non-invasive detection, remote control technology, and compositional analysis, in recent decades.1–6 The emerging smart devices require NIR light sources with a range of advantages, including miniaturization, broadband emission, and high thermal stability.7–10 However, NIR traditional light sources like incandescent lamps and tungsten lamps are constrained by their short lifespan, large size, long response time, and poor efficiency. The AlGaAs LEDs are considered a new-generation NIR light source and offer the advantages of high efficiency and compact size. However, their high cost and inherently narrowband emission have hindered their application, especially in meeting the requirements of broad wavelength coverage for compositional analysis.11–13 NIR pc-LEDs are considered exceptional NIR light sources owing to benefits of broadband emission, high efficiency, compactness, and high thermal stability.
Given the varying requirements of NIR spectra in different application fields, the development and design of phosphors with adjustable FWHM and peak wavelengths become particularly crucial. As Cr3+ ions possess a range of advantages, including high quantum efficiency, tunable emission bands, high absorption efficiency, and compatibility with blue LEDs, they have been considered promising NIR luminescent centers.14–17 Currently, the reported narrowband NIR phosphors include BaGd2Al2Ga2GeO12:Cr3+,18 ZnAl2O4:Cr3+,19 and LiAlSiO4,20 demonstrating potential applications in plant growth illumination. Alternatively, broadband emission NIR phosphors have a wider range of applications. To date, various strategies have been reported to achieve broadband emissions. By constructing multi-site luminescent centers, ultra-broadband emission can be realized. The relevant reports include La2MgZrO6:Cr3+,21 K4Ga3Ta(PO4)6:Cr3+,22 and La3Ga5GeO14:Cr3+.23 A strategy involving the introduction of an additional luminescent center to establish energy transfer and broaden the emission band has been proposed. Typical reports include Mg7Ga2GeO12:Ni2+,Cr3+,24 MgO:Cr3+,Ni2+,25 La2MgHfO6:Cr3+,Yb3+,26 KAlP2O7:Cr3+,Yb3+,Er3+,27 and Y3ScAl4O12:Cr3+,Nd3+.28 The emission band broadening can be obtained by employing crystal field engineering, and the notable examples are Gd3(MgxGa5−2xGex)O12:Cr3+,29 Y(Ga,Al)3(BO3)4:Cr3+,30 and Gd3YxInxGa5−2xO12:Cr3+.31 Additionally, it has been reported that broadband emission can be achieved through co-doping Cr3+ and Cr4+ ions, such as Mg2GeO4:Cr3+,Cr4+.32 However, the development of highly efficient NIR phosphors with tunable broadband emission remains a significant challenge.
In this work, a series of MGS:xCr3+ (x = 0.02, 0.04, 0.06, 0.08, 0.10, and 0.14) phosphors were developed. The low-temperature emission and excitation spectra, crystal structure, and fluorescence decay curves confirmed the presence of two kinds of luminescent centers (Cr(I) and Cr(II)). By adjusting the concentration of Cr3+ ions, the FWHM was effectively tuned over a wide range from 151 to 223 nm, and the peak wavelength was shifted from 715 to 833 nm. This remarkable tunability is due to the energy transfer from the 2E states of Cr(I) to the 4T2 states of Cr(II). The ultra-broadband NIR phosphor MGS:0.08Cr3+ exhibits superior thermal stability, maintaining 50% of its room-temperature emission intensity even at 423 K, alongside an impressive IQE of 57.8%. Moreover, the NIR pc-LEDs based on MGS:0.02Cr3+ and MGS:0.08Cr3+ demonstrated a high NIR output power of 24.7 and 27.8 mW (100 mA) and remarkable photoelectric conversion efficiency of 14.4 and 16.4% (10 mA). Notably, high-performance pc-LEDs served as NIR light sources for plant growth illumination, night vision imaging, and non-invasive detection applications, achieving significant performance.
2. Results and discussion
2.1. Structural analysis
The XRD analysis is used to determine the phase purity and crystal structure of samples. The representative XRD patterns of the MGS:xCr3+ samples and the standard card (Mg2TiO4 ICSD-24232) are presented in Fig. 1a. It is evident that all the XRD patterns of samples match well with the standard card without any additional diffraction peaks of impurities, indicating the successful synthesis of the MGS:xCr3+ pure phase. Fig. 1b illustrates the crystal structures of MGS. MGS is composed of two types of polyhedra: [MgO4] tetrahedron and [Mg/Ga/SnO6] octahedron. Cr3+ and Ga3+ ions have the same electronic valence, Cr3+ ions (r[CN=6] = 0.615 Å), Ga3+ ions (r[CN=6] = 0.62 Å), and Sn4+ ions (r[CN=6] = 0.69 Å) have similar ionic radii, Cr3+ ions replace Ga3+ and Sn4+ ions in the octahedral sites. The refinement results and crystal structure information of MGS:0.08Cr3+ are presented in Fig. 1c. The refinement gives Rwp = 9.51% and Rp = 6.69. All the reliability parameters are below 10%, confirming that the samples possess good phase purity. The detailed refined crystallographic and structure parameters are summarized in Table S1.† XPS is used to detect the surface elemental composition and valence states of ions. As shown in Fig. 1d, the signals of Mg2+, Ga3+, Sn4+, O2−, and Cr3+ ions are shown in the XPS spectrum. Fig. 1e presents the scanning electron microscopy (SEM) image and energy-dispersive X-ray spectrometry (EDS) patterns for an in-depth analysis of the microstructure and elemental composition of MGS:0.08Cr3+. The SEM image highlights the particles featuring irregular shapes and a smooth surface, indicative of crystallization within the sample. Meanwhile, the EDS patterns confirm a uniform distribution of Mg, Ga, Sn, O, and Cr across the obtained samples. These results validate the successful synthesis of the MGS:Cr3+ samples.
 |
| Fig. 1 (a) XRD patterns of MGS:xCr3+ and Mg2TiO4 (ICSD-24232). (b) Crystal structures of MGS. Rietveld refinement (c) and XPS spectrum (d) of MGS:0.08Cr3+. (e) SEM image and the corresponding elemental mappings of MGS:0.08Cr3+. | |
2.2. Photoluminescent properties
The diffuse reflection (DR) spectra of the undoped MGS and MGS:0.08Cr3+ samples are presented in Fig. 2a to study the absorption of the materials. Compared with the DR spectrum of undoped MGS, the DR spectrum of MGS:0.08Cr3+ shows two additional bands, which are related to the 4A2 → 4T1 and 4A2 → 4T2 transitions of the Cr3+ ions. This implies that the Cr3+ ions are successfully introduced into MGS. The optical band gap of undoped MGS can be determined through the Kubelka–Munk function:33 | [F(R)hv]2 = A(hv − Eg) | (2) |
F(R) is the absorption, R represents the diffuse reflectance, A refers to the absorption constant, and hv and Eg are the photon energy and optical bandgap, respectively. Based on the above equations, the fitting result of the undoped MGS is calculated to be 5.1 eV (Fig. S1†). The excitation and emission spectra of MGS:0.08Cr3+ at room temperature are measured and shown in Fig. 2b. The excitation spectrum reveals two discernible bands distributed within the 350 to 700 nm range. These bands originate from the 4A2 → 4T1 and 4A2 → 4T2 transitions of the Cr3+ ions. It can be seen that the emission spectrum shows an intense ultra-broadband NIR emission in the range of 600 to 1200 nm with a FWHM of 212 nm under a 450 nm excitation. To further investigate the origin of the ultra-broadband emission and the luminescent centers, the emission spectrum of the MGS:0.08Cr3+ sample at 7 K was tested, as shown in Fig. 2c. Evidently, the emission spectrum exhibits two band structures comprising a narrowband and a broadband. The fluorescence decay curves obtained by monitoring at 713 and 900 nm at 7 K are shown in Fig. 2d. The photoluminescent lifetime of the Cr3+ ions are calculated as follows:34 |  | (3) |
I(t) is the emission intensity of Cr3+ ions at time t. Notably, the decay curve at 713 nm exhibits a millisecond-scale lifetime (1.72 ms), which is characteristic of the 2E → 4A2 transition of the Cr3+ ions. However, the decay curve at 900 nm displays a microsecond-scale lifetime (0.18 ms/180 μs), indicative of the 4T2 → 4A2 transition of the Cr3+ ions. These indicate that the emission spectrum of MGS:Cr3+ is related to the 2E and 4T2 states of the Cr3+ ions. The photoluminescent properties are determined by the luminescent centers. To investigate the luminescent centers in MGS:Cr3+, a series of low-temperature excitation and emission spectra were tested and recorded in Fig. 2e and f. Fig. 2e shows the normalized spectra obtained by monitoring different wavelengths. They exhibit dissimilar profiles. Furthermore, the normalized emission spectra obtained under different excitation wavelengths in Fig. 2f also do not perfectly overlap. These suggest that the broadband and narrowband emissions originate from two kinds of luminescent centers.
 |
| Fig. 2 (a) Diffuse reflectance spectra of undoped MGS and MGS:0.08Cr3+. (b) Excitation and emission spectra of MGS:0.08Cr3+. (c) Emission spectrum obtained under a 450 nm excitation at 7 K. (d) Fluorescence decay curves monitored at 713 and 900 nm for MGS:0.08Cr3+ at 7 K. Excitation (e) and emission (f) spectra of MGS:0.08Cr3+ at 7 K. | |
The emission spectra of Cr3+ ions are deeply influenced by the crystal field strength. Owing to the lack of shielding from the outer electron shells, the valence electrons of the Cr3+ ions undergo d–d transitions, rendering them highly susceptible to variations in the crystal field strength. Typically, when the Cr3+ ions are in a weak crystal field environment, the emission spectrum exhibits a broad band. Conversely, when the Cr3+ ions are in a strong crystal field environment, the emission spectrum shows a narrow band. According to the equation:35
|  | (4) |
Here, Dq is the crystal field strength parameter, and R is the distance between the central atom and the ligand. r is the radius of the 3d-wave function. Z represents the charge of the anion, and e is the charge of the electron. Based on the relationship between Dq and 1/R5, it is inferred that the narrowband emission originates from the Cr3+ ions replacing the smaller Ga3+ ions in a strong crystal field environment, while the broadband emission arises from the Cr3+ ions replacing the larger Sn4+ ions in a weak crystal field environment. The luminescent centers associated with the narrowband and broadband emissions are labeled as Cr(I) and Cr(II) in Fig. 2f, respectively.
2.3. The tunable ultra-broadband NIR emission and thermal stability
Different concentrations of Cr3+ ions were introduced to optimize the photoluminescent properties of MGS:Cr3+. Fig. 3a presents a series of emission spectra with varying concentrations, revealing notable changes in intensity. Fig. 3b summarizes the variation trends of the FWHM and peak wavelength of the emission spectra for samples with different concentrations. As the concentration increases, the FWHM broadens from 151 nm at x = 0.02 to 223 nm at x = 0.14, and the peak wavelength shifts from 715 nm at x = 0.02 to 833 nm at x = 0.14. These phenomena arise from the shortened distance between adjacent Cr3+ ions as the concentration is elevated, leading to enhanced interactions. The probability of the energy transfer from the 2E states of Cr(I) to the 4T2 states of neighboring Cr(II) results in the attenuation of the narrowband emission intensity and the enhancement of the broadband emission intensity. Thus, the emission spectra exhibit a transition from narrowband dominance at lower concentrations to broadband dominance at higher concentrations, and the peak wavelength shifts from shorter to longer wavelength regions. The increase in broadband emission intensity outweighs the decrease in the narrowband emission intensity, leading to an overall enhancement in the total emission intensity. When the concentration is further elevated, the emission intensity diminishes monotonously, which is attributed to concentration quenching. As the concentration of Cr3+ ions increases, the distance between the adjacent activators decreases. It results in a greater probability of energy transfer from luminescent centers to quenching centers, leading to increased energy loss and a subsequent reduction in emission intensity. As shown in Fig. 3c, the IQE, absorption efficiency (AE), and external quantum efficiency (EQE) of the MGS:0.08Cr3+ sample are evaluated and determined to be 57.8%, 35.3%, and 20.4%.
 |
| Fig. 3 (a) Concentration-dependent emission spectra of MGS:xCr3+. (b) FWHM and the peak wavelength of MGS:xCr3+. (c) Quantum efficiency graph of MGS:0.08Cr3+. (d) Normalized photoluminescent lifetime at 713 and 900 nm of MGS:xCr3+ samples. (e) Normalized emission spectra of MGS:0.08Cr3+ at different temperatures. (f) Schematic of the electron population at lower and higher temperatures. (g) Temperature-dependent emission spectra of MGS:0.08Cr3+ sample at different temperatures. (h) Normalized intensities at different temperatures. (i) Mechanism for thermal quenching in MGS:Cr3+. | |
To further investigate concentration quenching, fluorescence decay curves at 713 nm and 900 nm were monitored for samples with different concentrations (Fig. S2 and S3†). The photoluminescent lifetimes are calculated and listed in Table S2.† With the increase in Cr3+-concentration, the photoluminescent lifetimes at 713 and 900 nm shorten, dwindling from 0.37 and 0.18 ms at x = 0.02 to 0.08 and 0.08 ms at x = 0.14. This is attributed to the gradual strengthening of the concentration quenching effects. Fig. 3d presents the variation trends of the normalized photoluminescent lifetime at 713 and 900 nm in the emission spectra of samples with different Cr3+ ion concentrations. As the concentration is elevated, the photoluminescent lifetime at 713 nm decreases rapidly. This phenomenon can be attributed to the enhanced energy transfer from the 2E states of Cr(I) to the 4T2 states of Cr(II) between adjacent Cr3+ ions, as mentioned earlier. The photoluminescent lifetime at 900 nm initially decays slowly and then more rapidly as the concentration increases. This phenomenon can be explained by the energy transfer from Cr(I) compensating for losses at lower concentrations, while the concentration quenching becomes dominant when the energy transfer is weaker at higher concentrations.
A series of emission spectra for MGS:0.08Cr3+ from 12 to 298 K were measured and are presented in Fig. S4† and Fig. 3e. During the transition from lower to higher temperatures, the emission spectra exhibit a series of continuous changes. The intensity of the narrowband emission gradually decreases while the intensity of the broadband emission progressively increases. At room temperature (RT), the emission spectrum is predominantly characterized by broadband emissions. The mechanism of the dynamic changes in the spectra during the heating process can be well understood through the schematic diagram shown in Fig. 3f. At lower temperatures, electrons populate the 2E states of Cr(I), and the 4T2 states of Cr(II) undergo radiative transitions back to the 4A2 states, accompanied by intense narrowband and broadband NIR emissions, respectively. As the temperature rises, some electrons at the 2E state of Cr(I) thermally migrate to the 4T2 state of Cr(I). Then, they return to the 4A2 state through radiative transition, generating a broadband emission in the vicinity of 730 nm. Some electrons transfer energy to Cr(II). The electrons of Cr(II) are excited to the 4T2 state and then return to the 4A2 state. This ultimately leads to an enhanced intensity of broadband emission and a weakened intensity of narrowband emission. When the temperature reaches 195 K, the broadband emission intensities of Cr(I) and Cr(II) are approximately the same, and the FWHM reaches its maximum value.
Blue LEDs generate heat during operation, which significantly impacts phosphors with poor thermal stability, leading to pronounced thermal quenching. Consequently, the performance of NIR devices is diminished. Therefore, developing phosphors with exceptional thermal stability can prevent severe thermal quenching, ensuring the efficient luminescence of high-performance NIR devices. Superior resistance to thermal quenching enables more energy to be converted into light rather than heat at elevated temperatures, thereby minimizing energy loss during the conversion process. It also ensures that NIR devices achieve higher output power and maintain optimal performance under demanding conditions. The photoluminescent thermal stability of NIR phosphors serves as a criterion in assessing their practical application performance. Fig. 3g presents the contour map of the temperature-dependent emission spectra in the temperature range from 303 to 483 K. As the temperature increases, the emission intensity gradually decreases. As shown in Fig. 3h, it can be observed that the emission intensity at 423 K retains 50% of the value at 303 K. As shown in Table S3,† the presented phosphor MGS:Cr3+ demonstrates higher thermal stability compared with previously reported phosphors with a FWHM greater than 200 nm, demonstrating the high performance of MGS:Cr3+.
Fig. 3i illustrates the mechanism of thermal quenching of two kinds of luminescent centers in MGS:Cr3+. At lower temperatures, as expected, electrons in the 4T2 and 2E states of Cr(I) and Cr(II) return to the 4A2 states via radiative transitions accompanied by narrowband and broadband NIR emissions, respectively. When the temperature increases, the electrons at the 4T2 states of Cr(I) and Cr(II) are thermally activated, overcoming the energy barrier and transferring to the intersection of 4T2 and 4A2 states, then back to the ground states via non-radiative transitions. Meanwhile, Cr(I) continuously supplies energy to Cr(II). It is observed that the emission intensity of Cr(I) decays rapidly compared with Cr(II). These factors led to a decrease in the overall intensity of NIR emission.
2.4. Fabrication of the NIR pc-LED
High-performance pc-LED devices were fabricated by mixing 0.5 g of the prepared MGS:Cr3+ samples with transparent silicone resin in a 1
:
1 ratio, followed by applying this mixture onto 450 nm blue chips. Representative samples MGS:0.02Cr3+ and MGS:0.08Cr3+ were utilized as narrowband and broadband NIR phosphors, respectively, for the pc-LED1 and pc-LED2 fabrication. The performance of these devices is evaluated and presented in Fig. 4a and c. As the current is incrementally elevated from 10 to 200 mA, the electroluminescence (EL) spectra exhibit a continuous enhancement in intensity while maintaining a consistent spectral shape throughout the process. The inset photographs depict the on and off states of the NIR pc-LEDs. Fig. 4b and d illustrate the output power and photoelectric conversion efficiency under various driving currents. As the driving current increases, the output power initially rises and then declines, which correlates with the efficiency roll-off in commercial blue LEDs under high drive currents. The high output power enables NIR devices to be integrated into compact systems, eliminating the need for bulky power supplies. Furthermore, the impressive high photoelectric conversion efficiency signifies reduced energy loss and enhanced energy utilization. At a driving current of 100 mA, the NIR pc-LED1 and NIR pc-LED2 exhibit high NIR output power of 24.7 and 27.8 mW and impressive photoelectric conversion efficiency of 14.4 and 16.4%. The detailed EL testing results are provided in Tables S4 and S5.†
 |
| Fig. 4 EL spectra of the pc-LED1 (a) and pc-LED2 (c) at varying currents. Photoelectric conversion efficiency and output power of pc-LED1 (b) and pc-LED2 (d). | |
2.5. High-performance NIR pc-LEDs for application
Light is a crucial environmental factor that regulates plant photosynthesis, metabolism, and gene expression. According to the absorption spectra of plant pigments, the phytochromes PFR absorb light at 730 nm. Inspired by the spectral characteristics and high performance of the device, the potential of pc-LED1 as a light source for plant growth was tested. The electroluminescence spectrum shows significant overlap with the absorption spectra of phytochromes PFR (Fig. 5a). This result suggests that the MGS:0.02Cr3+ phosphor holds potential applications in indoor plant growth illumination. To assess the potential of this NIR pc-LED2 as a light source for night vision imaging and non-invasive detection, a series of validation tests were conducted. Fig. 5e, b and f display images of a toy captured in white light, darkness, and NIR light conditions. When the white light is turned off, the contours of the toys are indiscernible to the naked eye, and photographs taken with an NIR camera show darkness (Fig. 5b) with no observable toy. When the pc-LED2 is illuminated as the NIR light source and used to capture the scene with the NIR camera, a clear, vivid toy is recorded in the photograph (Fig. 5f). Non-invasive detection is of paramount importance in both industrial and agricultural sectors. Under white light, the chips on the ID card and SIM card are not directly observable (Fig. 5c and d). When the cards are placed between the NIR camera and pc-LED2, the captured images clearly reveal the chip positions and their intactness (Fig. 5g and h). These demonstrate its potential for application in night vision imaging and non-invasive detection.
 |
| Fig. 5 (a) EL spectrum of LED1 and absorption spectra of phytochromes PFR. Toy under white light (e), darkness (b), and NIR pc-LED1 (f). ID card (c) and SIM card (d) under white light. ID card (g) and SIM card (h) under NIR light. | |
3. Conclusion
In summary, the tunable ultra-broadband NIR phosphor MGS:Cr3+ was successfully synthesized via a high-temperature solid-state reaction method. MGS:Cr3+ exhibits customizable ultra-broadband emission with tunable FWHM (151 to 223 nm) and peak wavelengths (715 to 833 nm). This notable characteristic is attributed to the controlled energy transfer from luminescent centers Cr(I) to Cr(II). MGS:0.08Cr3+ exhibits excellent superior stability (50%) and a good IQE of 58.8%. Finally, the optimized NIR pc-LEDs based on MGS:0.02Cr3+ and MGS:0.02Cr3+ samples demonstrated their potential as light sources for applications in night vision imaging, non-invasive detection, and plant growth lighting.
Author contributions
Pengcheng Luo: conceptualization, data curation, formal analysis, investigation, methodology, and writing – original draft; Dashuai Sun: supervision and writing – review; Zeyu Lyu: project administration, resources; Mingxiang You: data curation and software; Zheng Lu: data curation; Xiaowei Zhang: data curation; Luhui Zhou: data curation; Hongpeng You: funding acquisition, project administration, resources, supervision, and writing – review & editing.
Data availability
The data supporting this article have been included as part of the ESI.† More raw data are available from the corresponding author on reasonable request.
Conflicts of interest
There are no conflicts to declare.
Acknowledgements
This work is financially supported by the National Key Research and Development Program (Grant No. 2022YFC2905201), the National Natural Science Foundation of China (Grant No. 52072363 and 22305250), and the research fund of Key Laboratory of Rare Earths, Chinese Academy of Sciences.
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