The hydrothermal method and properly selected synthesis conditions enable obtaining nanoparticles (NPs) composed of GdBO3 doped with 18%Yb3+, 1%Ho3+, and various concentrations of Ce3+ ions. The desired structure of the NPs was obtained in situ under hydrothermal conditions, and it was unnecessary to calcinate the product to achieve the desired monoclinic structure of NPs or precipitate the precursor before the hydrothermal reaction, as often suggested in the literature 37. The as-precipitated product was dried at 80°C for 24 hours. However, to enhance the NPs' crystallinity and simultaneously achieve a more intense emission, samples were annealed at 525°C and 925°C. The calcination temperature was estimated based on TGA analysis (Fig. 1) and also literature reports. At about 525°C, borates start to transform into stable high-temperature forms, and 925°C is the point at which the most stable form of borates is expected 31.
The ICP-MS analysis revealed disparities in the actual concentrations of Ce3+ ions and partially of Yb3+ ions within the prepared NPs compared to the intended values (Supplementary Table S1). The reaction conditions were identical; hence, the ultimate product composition was influenced by additional factors. This discrepancy could stem from variations in the ionic radii among Ln3+ ions and the solubilities of RE-borates 38–40. Specifically, the comparatively lower solubility of GdBO3, YbBO3, and HoBO3 (precipitating faster than CeBO3) may contribute to the significantly reduced concentration of Ce3+ ions in the resultant materials, diverging from the anticipated levels based on the quantities of reagent salts added. Furthermore, the larger ionic radii of Ce3+ ions compared to the other Ln3+ ions (Gd, Yb, Ho) impede the effective exchange of Gd3+ ions within the matrix.
Although Ce3+ and Ho3+ ions possess the most similar ionic radii, a surplus of Ce3+ ions is necessary to incorporate them into the gadolinium borate structure. While RE-based compounds are typically isostructural, deviations from this trend frequently manifest at the gadolinium stage41. Consequently, borates featuring Gd, Yb, and Ho are more favorable than those incorporating Ce. The XRD patterns of the GdBO3-doped NPs match well with reference pattern COD 701884130 and the crystal structure was identified as monoclinic C2/c (Fig. 2a, b). No other phases or impurities were detected, consistent with the basic parameters of GdBO3. The only observed changes were that, with increased calcination temperature, the XRD lines became more intense, sharp, and narrow. This corresponds to higher crystallinity and a larger average grain size of the product. In addition, the intensities of diffraction lines positioned at approximately 20° and 27° exhibited exceptional increase relative to other diffraction lines. They displayed significantly greater intensity than the same XRD lines observed on patterns for samples subjected to those dried at 80°C. This phenomenon may be attributable to preferential
crystal growth along one or two specific crystallographic axes. This observation aligns with TEM images, which depict a nearly two-dimensional morphology of the NPs, characterized by a flattened plate-like structure (Fig. 3)42. The monoclinic structure of the NPs, which is schematically performed in Fig. 2b, confirms that eight neighboring atoms surround two gadolinium ions. Furthermore, the boron atoms are 4-coordinated in tetrahedral BO4 groups, which form three-membered rings comprising polyborate B3O99− units. The coordinating oxygens are divided into two types: terminal oxygens form a trigonal antiprism around Gd3+ ions while bridging oxygens connect the cations 30. Then, the TEM images of the GdBO3 doped with 18%Yb3+, 1%Ho3+, and 0.15%Ce3+ (Fig. 3) unveil noticeable variations in the average grain size and morphology of the NPs under different temperature treatments. Specifically, drying at 80°C followed by annealing at 525°C and 925°C results in distinct product characteristics. The dried samples present the most irregular morphology. They consist of two phases: bigger particles and a significant amount of very small particles, which look like nucleation seeds. A higher calcination temperature is needed for a more crystalline and homogenous product. The morphology is non-uniform for each NP but can be described as a thin flake. The average grain size of NPs dried at 80°C is ~ 70 nm, calcinated at 525°C is ~ 30 nm, and at 925°C is ~ 102 nm. The particles show noticeable agglomeration, a common occurrence in materials prepared by hydrothermal methods. However, the material's morphology is suitable for potential applications like anticounterfeiting tags and modifying paper or cellulose fibers.
Figure 4 presents the up-conversion spectra of GdBO3:18%Yb3+/1%Ho3+/x%Ce3+ (x = 0; 0.1; 0.15; 6.5; 13) under NIR 972 nm excitation, showing dependency of the particular emission bands intensity on various Ce3+ concentration. It should be noted that neither ytterbium nor cerium ions have 4f levels corresponding to green and red emissions. The spectra consist mainly of both typical Ho3+ bands, namely 5S2/5F4 → 5I8 in the green region at 537 nm and 5F5 → 5I8 in the red range, with the maximum at 647 nm. A band related to the transition 5F4/5S2 → 5I7 at 753 nm can also be depicted. The emission spectra show that the intensity of the red and the green bands is comparable regarding each sample prepared. However, a more detailed analysis of the red-to-green band intensity ratio shows slight changes as the concentration of Ce3+ ions varies. Moreover, the influence of Ce3+ ions on overall luminescence intensity is decreasing, especially starting from the sample with higher Ce3+ concentration, namely 6.5%. The observed phenomenon stems from the energy transfer between Ho3+ and Ce3+ ions, which can affect the transition pathways within the emission of the prepared NPs9,34. To investigate the dependency of the R/G ratio on Ce3+ ion doping, the area of the red and green band was determined and compared, which is presented accordingly in Fig. 4 (insert). The R/G intensity ratio of up-conversion emission spectra decreases from 1.8 to 0.62 with increasing concentration of cerium ions. Changes in color emission are observed as a shift from the yellow-green spectral region (for 0% Ce3+ concentration) towards the green region with an increase in Ce3+ concentration to 13%. In this study, the correlated color temperature (CCT) was calculated using the McCamy equation based on the CIE (1931 Commission Internationale de l’Eclairage) chromaticity coordinates, x, and y, while visualizing the color emission on chromaticity diagrams and schemes. The CCT was calculated by using the Eq. 43:
$$\varvec{C}\varvec{C}\varvec{T}= -{437\varvec{n}}^{3}+{3601\varvec{n}}^{2 }-6861\varvec{n}+5514.31$$
$$\varvec{n}=\frac{(\varvec{x}- {\varvec{x}}_{\varvec{e}})}{(\varvec{y}- {\varvec{y}}_{\varvec{e}})}$$
where: xe = 0.3320, ye = 0.1858, and x and y are the color coordinates.
The results are presented in Fig. 5, where one can observe an increase in color temperature from 4345K to 5442K with the increase in Ce3+ concentration.
The unusual changes in the red-to-green (R/G) ratio, characterized by a decreasing trend contrary to the typical increase, prompted an investigation into the mechanism of UC processes. As the concentration of Ce3+ ions increases, the red and green emission bands continuously decrease, suggesting the involvement of ET between Ho3+ and Ce3+ ions. Specifically, the green emission arises from the population of the 5F4 and 5S2 states through two distinct ET pathways from Yb3+ to Ho3+ ions (ET1 and ET2, Fig. 6). However, the population of the red 5F5 level necessitates nonradiative relaxation from 5F4, 5S2 to 5F5, and 5I6 to 5I7, implying a longer time to obtain the red emission. The energy gap between the 2F7/2 - 2F5/2 levels of Ce3+ ions aligns well with the energy difference between 5I6 - 5I7 and 5F4,5S2-5F5 levels of Ho3+ ions, facilitating the promotion of these energy levels and concurrent red emission. Nevertheless, the intensities of the green and red emission bands decrease with increasing Ce3+ concentration, indicating competition between ETs from Yb3+ to Ho3+ and back ET (bET) from Ho3+ to Yb3+. Upon establishing the optimal concentration of Yb3+ ions, ET transfer promotes red emission, while bET enhances green emission. In our samples, the transition towards the green region suggests that the enhancement of red emission by cross-relaxation (CR) from Ce3+ to Ho3+ ions and ET from Yb3+ to Ho3+ is outweighed by bET from Ho3+ to Yb3+.
Comparatively, in the case of samples performed in this article, inversely compared to the samples doped with Yb3+, Ho3+, and Ce3+ ions in a molybdate matrix 34, there is an insufficient concentration of Yb3+ ions to populate the Ho3+ ions’ red emitting level, leading to the dominance of bET and resulting in green emission. With a higher concentration of Yb3+, the color tends towards yellowish due to increased participation of the red color; however, decreased Yb3+ concentration, consistent ICP-MS results, leads to the dominance of bET mechanisms, rendering the Ho3+ red level inadequately pumped by Yb3+. Concurrently, CR processes from Ho3+ to Ce3+ quench the red emission as Ce3+ concentration increases. These processes collectively contribute to the atypical behavior of tunability, shifting the color from yellowish to green with increasing Ce3+ concentration in the samples prepared. The atypical red-to-green (R/G) ratio changes, indicating a decreasing trend contrary to the typical increase, prompted us to analyze the UC process mechanism. The emission bands decrease continuously, together with increasing concentration of Ce3+ ions. It indicates that the ET between Ho3+ and Ce3+ ions must be responsible. The 5F4 and 5S2 states are mainly populated by two different types of ET from Yb3+ to Ho3+ ions, what resulted in green emission. However, the population red 5F5 level requires nonradiative relaxation from 5F4, 5S2 to 5F5, and 5I6 to 5I7. It means that red emission is populated in a longer time. The energy gap between 2F7/2 - 2F5/2 of Ce3+ ions matches well with the energy between 5I6 - 5I7 and 5F4,5S2-5F5 of Ho3+ ions, which can result in the promotion of these energy levels and at the same time the red emission. However, the emission intensity of the green and red emission bands decreases with increasing Ce3+ concentration, so the ET from Yb3+ to Ho3+ must compete with back ET from Ho3+ to Yb3+. When the optimal concentration of the Yb3+ ions in samples is established, the ET transfer can promote the red emission, and at the same time, BET enhances the green emission. Here, in the case of our samples, the color changes into green region suggest that the enhancement of red emission by ET from Ce3+ to Ho3+ and ET from Yb3+ to Ho3+ loses with BET from Ho3+ to Yb3+. Compared to the results observed for the molybdate matrix doped with Yb3+, Ho3+, and Ce3+, in our case, there are too few Yb3+ ions to populate the Ho red emitting level, and the BET dominates, resulting in green emission34. When there is more Yb3+ - the color is more yellowish. Hence, the participation of the red color is higher, but when the Yb3+ decreases (which is in accordance with ICP-MS results), the BET mechanism wins and pumping by Yb3+, the Ho3+ of the red level is not sufficient. At the same time, the cross-relaxation processes (CR) from Ho3+ to Ce3+ quench the red emission while the Ce3+ concentration increases. All these processes result in untypical tunability behavior and shift from yellowish to green color with increased Ce3+ concentration in the performed samples.
Supplementary Fig. S2 performs excitation spectra with quite narrow bands with a maximum at 972 nm, which are assigned to the 2F7/2 → 2F5/2 transition, related to the energy absorption by Yb3+ ions. The narrow shape of the band is an effect of a low crystal field around Yb3+ ions, which is characteristic for this type of crystal borates structure44. However, does the observation of the 2F7/2 → 2F5/2 transition band confirm the energy transfer from Yb3+ to Ho3+ ions leading to the emission in the visible range. Consequently, the intensities of excitation peaks are Ho3+/Ce3+/Yb3+ is changing adequately to the concentration of Ho3+/Ce3+/Yb3+, which is in agreement with the emission spectra shown.