Tunable Luminescence and Energy Transfer of Sr₃B₂O₆:Ce³⁺, Sm³⁺ Phosphors with Potential Anti-Counterfeiting Applications

Abstract

Sm³⁺ and Ce³⁺ singly doped and Sm³⁺ and Ce³⁺ co-doped Sr₃B₂O₆ phosphors are prepared via a high-temperature solid-state reaction method. The crystal structure and phase purity are characterized by X-ray diffraction (XRD) analyses. The Sm³⁺-doped sample displays an emission in the orange-red region, with the strongest emission line at about 648 nm and possessing a good luminescence thermal stability between 78 and 500 K. With the increase in the Sm³⁺ content, the concentration quenching is observed due to the cross-relaxation (CR) processes among the Sm³⁺ ions. Upon 340 nm excitation, the Ce³⁺-doped phosphor presents a broad emission band in the blue region with a maximum at about 420 nm, which overlaps well with the ⁶H_5/2 → ⁶P_3/2 excitation line of Sm³⁺ and implies the possible energy transfer from Ce³⁺ to Sm³⁺. The spectral and decay measurements of the Ce³⁺ and Sm³⁺ co-doped samples are conducted and the Inokuti–Hirayama (I-H) model is adopted to analyze the luminescence decay dynamics of the donor Ce³⁺. Owing to the evident sensitization of the Sm³⁺ by the Ce³⁺ ions, the co-doped samples exhibit color variation under different wavelength excitations, endowing them with potential applications in optical anti-counterfeiting.

1. Introduction

Lanthanide-activated luminescence materials with stimuli-responsive emission outputs have attracted increasing attention due to their potential applications in optical anti-counterfeiting and information security fields [1,2,3,4,5,6]. To pursue the superior performances of feasibility and reliability for applications, there is a necessity for the constant exploration of novel phosphors with an easy trigger and an abundant color evolution. Recently, the excitation-wavelength-responsive lanthanide-activated phosphors including upconversion [1] and downshifted phosphors [2] have emerged as important alternatives owing to the feature of a convenient excitation trigger [7,8], when compared to other stimuli methods such as temperature [9], pressure [10], and so on. With the merit of high emission efficiency, the downshifted lanthanide-activated phosphors significantly promote the performances of optical anti-counterfeiting and information security applications. To further expand their color evolution range with the trigger of excitation wavelength, a feasible way is by simply co-doping two or more different lanthanide ions with distinct emission colors into a suitable host compound. Thus, the emission color and the excitation wavelength may be tuned and expanded by virtue of the possible energy transfer among these lanthanide ions.

Sm³⁺ ions usually display strong 4f-4f absorption lines at about 400 nm in most compounds, which match well with the commercially available light-emitting diode (LED) chips. Meanwhile, Sm³⁺-doped phosphors usually exhibit an intense emission in the orange-red region. Therefore, it is easy to achieve monochromatic anti-counterfeiting with a commercial 400 nm LED chip by choosing Sm³⁺ ions as activators.

In addition, the energy of the parity-allowed 4f-5d transition of Ce³⁺ is evidently affected by the host crystal field and electron–phonon coupling, due to its outer-lying 5d orbitals. The emission of Ce³⁺ is found to vary from UV to the red region [11,12,13] in different types of host compounds. It can be deduced that if Ce³⁺ ions display a blue-violet emission around 400 nm in a well-selected host compound, then Ce³⁺–Sm³⁺ energy transfer (ET) may occur, and it is possible to realize a wide range of luminescence tuning from a blue-violet emission of Ce³⁺ to an orange-red emission of Sm³⁺ under different excitation conditions, by utilizing their different emission colors and the potential ET effect.

Based on the above considerations, we chose Sr₃B₂O₆ (abbreviated as SBO hereafter) as a host compound in this paper due to its simple synthesis condition, good physicochemical stability [14] and one kind of Sr²⁺ site for lanthanide occupation. The influence of temperature and concentration on Sm³⁺ luminescence and the energy transfer dynamics between the Ce³⁺ and the Sm³⁺ in the SBO host were studied. The results reveal the emission color-tunability of the co-doped samples upon different excitation wavelengths and demonstrate their potential applications in optical anti-counterfeiting. This work provides a simple strategy and a candidate material towards excitation-wavelength-responsive optical anti-counterfeiting.

2. Materials and Methods

A series of Sm³⁺ and Ce³⁺ singly doped (Sr_3−2xSm_xNa_xB₂O₆, x = 0.005, 0.01, 0.02, 0.03, 0.05, 0.10, SBO:xSm³⁺; Sr_2.98Ce_0.01Na_0.01B₂O₆, SBO:0.01Ce³⁺) and Ce³⁺ and Sm³⁺ co-doped samples (Sr_2.98−2yCe_0.01Sm_yNa_0.01+yB₂O₆, y = 0.005, 0.01, 0.02, 0.03, 0.05, 0.10, SBO:0.01Ce³⁺, ySm³⁺) were prepared via a high-temperature solid-state reaction method using SrCO₃ (Analytical Reagent, A. R.), H₃BO₃ (A. R.), Na₂CO₃ (A. R.), Sm₂O₃ (99.99%) and/or CeO₂ (99.99%) with stoichiometric ratios as reactants. The raw materials were fully ground in agate mortars, then transferred into corundum crucibles and heated at 1423 K for 6 h in a reductive H₂-N₂ (5–95%) ambience. After cooling down to room temperature (RT) naturally in the furnace, the products were re-ground for further characterizations.

The phase purity of the powder samples was checked by X-ray diffraction (XRD) measurements on a RIGAKU D-MAX 2200 VPC X-ray diffractometer (Tokyo, Japan) with Cu Kα radiation (λ = 1.5418 Å) at an operating condition of 40 kV and 26 mA. The XRD data were collected over a 2θ range of 10–80° with a scanning rate of 10°/min. The high-quality XRD data of the SBO:0.005Sm³⁺ for Rietveld refinement were recorded over a 2θ range from 10° to 110° at an interval of 0.02° using a Bruker D8 ADVANCE X-ray diffractometer (Billerica, MA, USA) with Cu Kα radiation (λ = 1.5418 Å) at 35 kV and 35 mA. Rietveld refinement was performed with the TOPAS-academic V4.1 program [15]. The morphology of the SBO:0.005Sm³⁺ sample was characterized with an FEI Quanta 400 FEG scanning electron microscope (SEM) (Lincoln, NE, USA). The photoluminescence (PL) spectra and luminescence decay curves at RT and varied temperatures were measured on an Edinburgh FLS 1000 combined spectrometer equipped with a PMT detector (Livingston, UK). A 450 W Xe900 xenon lamp was used as an excitation source of steady-state PL measurements; a 340 nm pulsed light-emitting diode (EPLED, Edinburgh Instruments) was used to collect the luminescence decay curves of Ce³⁺, while a 60 W μF900 flash lamp with a pulse width of 1.5–3.0 μs and a pulse repetition rate of 20 Hz was used to record the luminescence decay curves of the Sm³⁺ in a microsecond range. The temperature-dependent luminescence measurements in 78–500 K were performed with an Oxford Optistat DN cryostat (Abingdon, UK), and the sample temperature was controlled by a MercuryiTC temperature controller. Sample images upon UV excitation were taken with an Apple iPhone 8 Plus mobile phone at a normal condition.

3. Results and Discussion

3.1. Crystal Structure, Morphology and Phase Purity

The SBO crystallizes in a trigonal system with a space group of R-3c (No. 167) [16]. There is only one kind of Sr²⁺ site in the SBO, which coordinates with eight oxygen ions to form a dodecahedron geometry with C₂ symmetry, as shown in Figure 1a. Each B³⁺ ion coordinates with three oxygen ions to form a [BO₃]³⁻ planar triangle. Due to the similar ion radii of Sr²⁺ and lanthanide dopants, as well as the charge compensator Na⁺ (coordination number, C. N. = 8, r(Sr²⁺) = ~1.26 Å, r(Ce³⁺) = ~1.14 Å, r(Sm³⁺) = ~1.08 Å, r(Na⁺) = ~1.18 Å) [17], the Ce³⁺, Sm³⁺ and Na⁺ ions are expected to occupy the Sr²⁺ sites. Rietveld refinement of the SBO:0.005Sm³⁺ sample is performed and shown in Figure 1b. The values of R_p (~6.58%), R_wp (~4.66%) and R_B (~3.50%) indicate a reliable refinement result. The refined lattice parameters are a = b = 9.044(1) Å, c = 12.572(1) Å, γ = 120°, V = 890.6(1) ų and Z = 6, and other related parameters are listed in

Table 1. Refined parameters of SBO:0.005Sm³⁺ sample.

Atom	x	y	z	Occ.	Biso
Sr	0.3554(1)	0	0.2500	0.9966	1.1227(13)
Sm	0.3554(1)	0	0.2500	0.0017	1.3435(13)
Na	0.3554(1)	0	0.2500	0.0017	0.9375(21)
B	0	0	0.1185(8)	1	1.3979(20)
O	0.1601(4)	0.0118(5)	0.1156(2)	1	1.1704(42)

. The average Sr²⁺/Sm³⁺-O²⁻ bond length is about 2.634(4) Å, while the adjacent distance of the nearest Sr²⁺ ions is evaluated at about 3.594 Å. Figure 1c display the SEM image of the SBO:0.005Sm³⁺ sample. Agglomerate particles with irregular shapes and an average size of several microns are observed. Some representative XRD patterns of the host compound and the singly or doubly doped samples are displayed in Figure 1d. The patterns of the un-doped host and doped samples match well with that of the theoretical result calculated with the Crystallographic Information File (CIF) of the SBO [16]. Furthermore, the lattice parameters of the representative samples are also calculated via Rietveld refinement as tabulated in

Table 2. Calculated lattice parameters of doped samples.

Samples	SBO:0.01Ce3+	SBO:0.10Sm3+	SBO:0.01Ce3+, 0.10Sm3+
a (Å)	9.042(1)	9.039(2)	9.038(2)
c (Å)	12.570(3)	12.567(3)	12.565(3)
V (Å3)	890.3(2)	889.5(1)	889.2(3)

. They clearly show the lattice shrinkages with different degrees, which depends on the doping ionic size and concentration. These results imply the successful doping of lanthanides into the SBO host lattice.

3.2. Luminescence Properties of Sm³⁺ in SBO Host

Figure 2a displays the excitation and emission spectra of the SBO:0.005Sm³⁺ at RT. When monitoring the emission wavelength at 648 nm, some sharp line-like excitation peaks can be observed in the range of 250–480 nm, which are attributed to the transitions from the ⁶H_5/2 ground state to higher 4f levels of Sm³⁺. The dominant peak at about 402 nm is assigned to the ⁶H_5/2 → ⁶P_3/2 transition of the Sm³⁺ ion [18]. Upon 402 nm excitation, one can identify about three relatively intensive sharp peaks in the emission spectra in Figure 2a, which can be aligned as ⁴G_5/2 → ⁶H_J transitions of the Sm³⁺ for J = 5/2 (~564 nm), 7/2 (~599 nm) and 9/2 (~648 nm), respectively [19]. The strongest emission peak of the Sm³⁺ in our case is located at 648 nm originating from the ⁴G_5/2 → ⁶H_9/2 electric–dipole transition, similar to the results in YVO₄ [20,21], Sr₂CaMoO₆ [22] and Ca₂GdNbO₆ [23] with asymmetric cationic environments, but is different with some cases where the Sm³⁺ sits at high-symmetrical sites [24,25,26]. The luminescence of the SBO:0.005Sm³⁺ displays exponential decay with a lifetime of about 1.83 ms, as shown in Figure 2b.

In order to study the temperature-related luminescence properties of Sm³⁺, we measured the emission spectra as well as the decay curves of the SBO:0.005Sm³⁺ at 78–500 K as given in Figure 2c,d. The spectral profiles at different temperatures nearly remain identical, although a slight thermal broadening is observed. The peak intensity (relative height) at 648 nm in the inset of Figure 2c shows a decline from 78 to 500 K, where the peak intensity at 500 K remains at 22.5% of that at 78 K. However, the overlapped exponential decay curves in Figure 2d manifest the good thermal stability of the Sm³⁺ 4f-4f luminescence. The discrepancy between the results obtained from luminescence intensity and luminescence decay measurements is mainly due to the complicated factors attributed to the spectral measurements, such as the temperature-dependence of absorption strength, energy migration and reabsorption [27]. Decay measurement seems to provide a more reasonable insight into the thermal-quenching behavior. The thermal quenching of Sm³⁺ is mainly related to the multi-phonon relaxation (MPR) process [28] where several phonons synergistically depopulate the higher-lying excited electrons of the Sm³⁺, as depicted in Figure 2e. The MPR process of Sm³⁺ depends on the energy gap (ΔE) between ⁴G_5/2 and ⁶F_11/2 (~7400 cm⁻¹), as well as the effective phonon energy (ℏω ~ 900 cm⁻¹ in Sr₃B₂O₆ in [29]. The number of phonons (p) is derived by p = ΔE/ℏω. The good thermal stability of Sm³⁺ in our case indicates the ineffective MPR process that requires too many phonons (~8) to bridge the energy gap between the two energy levels.

The concentration-dependent emission spectra of the SBO:xSm³⁺ (x = 0.005, 0.01, 0.02, 0.03, 0.05, 0.10) are presented in Figure 3a. The emission profile does not change with increasing dopants, while the intensity comes to a maximum when x = 0.02 and slightly decreases above this concentration as shown in the inset. The luminescence decay curves of the SBO:xSm³⁺ are also measured and shown in Figure 3b. At a low concentration (x = 0.005, 0.01), the decay curves stay mono-exponential but they deviate gradually from the exponential form at higher concentrations, indicating that concentration quenching happens in the concentrated samples. The average lifetime values of the samples are then obtained via the following equation [30]:

$$\tau ={{\displaystyle \int }}_0^{\infty }\frac{I\left(t\right)}{I\left(0\right)}dt$$

(1)

where I(0) and I(t) denote the luminescence intensity when time is 0 and t, respectively. The average lifetime values are listed in the legend of Figure 3b and are shortened with the increase of the Sm³⁺ concentration. When dopants increase, the Sm³⁺-Sm³⁺ interaction distance is shortened, and the dense energy levels of the Sm³⁺ endow them with some resonant non-radiative channels to quench the luminescence of the Sm³⁺ via a cross-relaxation (CR) process. Some CR channels of the Sm³⁺, such as [⁴G_5/2, ⁶H_5/2] → [⁶F_11/2, ⁶F_5/2], [⁴G_5/2, ⁶H_5/2] → [⁶F_5/2, ⁶F_11/2], [⁴G_5/2, ⁶H_5/2] → [⁶F_9/2, ⁶F_9/2], and so on, have been reported and schematized in Figure 2e [22,24,31,32].

To further study the CR mechanism of Sm³⁺ in the SBO host, we applied the Inokuti–Hirayama (I-H) model to analyze the luminescence decay curves of the Sm³⁺-doped samples as shown in the following equation [33]:

$$\frac{I\left(t\right)}{I\left(0\right)}=exp\left[-\left(\frac{t}{{\tau }_0}\right)-\frac{4\pi }{3}{C}_{\mathrm{A}}\Gamma \left(1-\frac{3}{S}\right){\left(C_{\mathrm{DA}}\right)}^{3/S}{t}^{3/S}\right]$$

(2)

where I(t) denotes the intensity at a given time t, I(0) is the initial intensity, τ₀ is the intrinsic lifetime of Sm³⁺ (~1.83 ms), and C_A is doping concentration of Sm³⁺. C_DA is the ET microparameter. Γ(x) is the gamma function and S expresses the multipolar interaction (6 for electric dipole-dipole (EDD) interaction, 8 for electric dipole-quadrupole (EDQ) and 10 for electric quadrupole-quadrupole (EQQ)). The energy transfer probability P_DA can be expressed with the following equation:

$$P_{\mathrm{DA}}=C_{\mathrm{DA}}^{\left(S\right)}/R^S$$

(3)

where R is denoted as the distance between ions. When P_DA = 1/τ₀, where the ET rate of donor ion equals to its own radiation rate, the obtained R is defined as ET critical distance (R_c). The fitted results are compiled in

Table 3. Relevant parameters in I-H model analysis.

Sm3+ Concentration	CA (×1025 m−3)	CDA (×10−53 m6/s)	Radj2
0.01	6.742	2.740	0.9975
0.02	13.48	3.338	0.9978
0.03	20.23	3.856	0.9974
0.05	33.71	4.542	0.9973
0.10	67.42	4.175	0.9973
average	-	3.730	-

. When S is set to be 6, the best fitting quality can be obtained, indicating that the main interaction type of CR in Sm³⁺ ions is EDD interaction, similar to the result in [34,35]. The averaged C_DA value is ~3.730 × 10⁻⁵³ m⁶/s, and the corresponding R_c is calculated to be about 6.40 Å.

3.3. Luminescence Properties of SBO:0.01Ce³⁺ Sample

Figure 4a shows the highest-height normalized excitation and emission spectra of a diluted sample SBO:0.01Ce³⁺ at RT. Monitoring 420 nm emission, one can observe three broad bands over a range of 250–380 nm, which are assigned as the transitions from 4f ground state to 5d_i (i = 1, 2, 3) excited states of Ce³⁺ in descending order in wavelength. Upon 340 nm excitation, Ce³⁺ exhibits a broad emission band with a maximum at ~420 nm, consistent with the reported result in [36,37]. The Commission Internationale de l’Eclairage (CIE) chromaticity coordinates are calculated as (0.157, 0.031), lying in the blue-violet region as shown in the inset of Figure 4a. The luminescence decay curve in Figure 4b displays an exponential feature, and the lifetime of the Ce³⁺ emission is fitted to be ~38.2 ns.

3.4. Luminescence of Sm³⁺, Ce³⁺ Co-Doped Samples and Ce³⁺-Sm³⁺ ET Dynamics

Figure 5a shows the highest-height normalized excitation and emission spectra of SBO:0.01Ce³⁺ and SBO:0.005Sm³⁺ at RT. A spectral overlap of the Ce³⁺ emission and the Sm³⁺ excitation over a range of 365–550 nm can be observed, suggesting the possibility of ET from Ce³⁺ to Sm³⁺. Figure 5b displays the spectral difference of the Sm³⁺ singly doped and the Ce³⁺ and Sm³⁺ co-doped sample. Upon excitation at 340 nm where Ce³⁺ can be efficiently excited but the absorption of Sm³⁺ is very weak, the Sm³⁺ singly doped sample has a similar emission spectrum, but an evidently weaker signal compared to that in Figure 2a. In the Ce³⁺ and Sm³⁺ co-doped case, both the emission of Ce³⁺ and Sm³⁺ can be observed. Under 340 nm excitation, the intensity of Sm³⁺ shows a 10-fold enhancement compared to the singly doped one, indicating the ET from Ce³⁺ to Sm³⁺ greatly sensitizes the luminescence of Sm³⁺.

When further increasing the Sm³⁺ concentration in the SBO:0.01Ce³⁺, ySm³⁺ (y = 0.005–0.10) samples, Ce³⁺ emission decreases with increasing y values except for the outlier SBO:0.01Ce³⁺, 0.01Sm³⁺, which may be due to an experimental error, as shown in Figure 5c. One can also notice that there is a V-shaped notch in the Ce³⁺ emission spectra at 402 nm, as marked with a dashed rectangle because of the absorption of Sm³⁺ [18]. The reduction in Ce³⁺ intensity is mainly due to the ET from Ce³⁺ to Sm³⁺. This can be also confirmed by the Ce³⁺ decay curves in Figure 5d after ruling out the concentration quenching of Ce³⁺ in the SBO host, which was studied in our previous work [37].

The Sm³⁺ emission intensity in Figure 5c shows an increase when y = 0.005–0.05, and then decreases. Two opposite effects, the Ce³⁺-Sm³⁺ ET and the Sm³⁺-Sm³⁺ CR, jointly affect the luminescence intensity of Sm³⁺ in the co-doped samples. The ET enhances the Sm³⁺ luminescence while the CR weakens it. At low concentrations, the ET effect plays a more important role, so the Sm³⁺ emission intensity increases with the increasing doping contents. Then, the CR becomes dominant in highly-doped samples where the ET seems insufficient to offset the CR, thus leading to a decline in Sm³⁺ emission. The luminescence decay curves of Ce³⁺ in co-doped samples (Figure 5d) gradually deviate from exponential, and their average lifetime values obtained via Equation (1) are also shortened from 37.5 ns (y = 0.005) to 26.4 ns (y = 0.10) (see the legends in Figure 5d), indicating that the ET from Ce³⁺ to Sm³⁺ accelerates the depopulation process of the Ce³⁺ excited electrons. The I-H model is also utilized to analyze the decay properties of the Ce³⁺. The fitted result and relevant parameters are displayed in Figure 5d and

Table 4. Relevant parameters in I-H model analysis in Ce³⁺ and Sm³⁺ co-doped samples.

Sm3+ Concentration	CA (×1025 m−3)	CDA (×10−49 m6/s)	Radj2
0.005	3.371	0.8791	0.9978
0.01	6.742	2.424	0.9983
0.02	13.48	1.393	0.9983
0.03	20.23	2.359	0.9978
0.05	33.71	4.089	0.9984
0.10	67.42	2.464	0.9982
average	-	2.268	-

. When S is set to be 6, we obtain the best fitting, showing that the main multipolar interaction in the Ce³⁺-Sm³⁺ ET process is EDD type [38,39]. The average C_DA in the Ce³⁺-Sm³⁺ ET process is ~2.268 × 10⁻⁴⁹ m⁶/s.

3.5. Color Variation under Different Excitation Conditions of Samples and Their Potential Anti-Counterfeiting Applications

With the distinguished emission colors of the Ce³⁺ and the Sm³⁺ as well as their ET effect, color variation under different excitation wavelengths in the co-doped samples can be anticipated. Figure 6a exhibits luminescent images of the SBO:0.02Sm³⁺ and the SBO:0.01Ce³⁺, 0.02Sm³⁺ upon 340, 365 and 402 nm excitation of xenon lamp at RT. Monochromatic emission from Sm³⁺ is observed in the SBO:0.02Sm³⁺ sample with different excitation wavelengths. For the SBO:0.01Ce³⁺,0.02Sm³⁺ sample, one can observe a color evolution from violet-blue, sky-blue to orange-reddish color under 340, 365 and 402 nm excitation, respectively. At 340 and 365 nm excitation, Ce³⁺ can be efficiently excited and the Sm³⁺ orange-reddish emission can be greatly enhanced in virtue of the ET. Hence, the sample display is a mixed color of Ce³⁺ and Sm³⁺. When exciting at 402 nm where Sm³⁺ has a strong excitation peak but Ce³⁺ shows no absorption, only the characteristic red emission of Sm³⁺ is observed. The color tunability of the co-doped samples upon different excitation conditions may be applied in optical anti-counterfeiting. Figure 6b shows the anti-counterfeiting application demonstration using the SBO:0.02Sm³⁺ and the SBO:0.01Ce³⁺, 0.02Sm³⁺ samples. A patterned quartz glass substrate was first prepared via a laser printing and corrosion procedure, as introduced in our previous works [40,41]. The corresponding sample powders are filled into the substrate to form the pattern. Upon 365 nm commercial UV lamp excitation, the two samples display a red and violet-blue pattern of “SUN YAT-SEN UNIVERSITY”, respectively, resembling the result in Figure 6a. Furthermore, when we used a commercial 405 nm LED lamp and a 495 nm filter to eliminate the intensive excitation light, and both the two samples exhibited an orange-reddish pattern originating from the Sm³⁺ luminescence. These results manifest their potential applications in optical anti-counterfeiting.

4. Conclusions

The Sm³⁺ and Ce³⁺ singly doped and Sm³⁺ and Ce³⁺ co-doped SBO samples were prepared via a conventional high-temperature solid-state reaction method. XRD patterns of the doped samples reveal their single phase of the SBO. Upon 402 nm excitation, the Sm³⁺ singly doped sample exhibits an orange-reddish emission at about 648 nm, which is assigned as the ⁴G_5/2 → ⁶F_9/2 transition and possesses a radiative lifetime of ~1.83 ms. The Sm³⁺ luminescence maintains good thermal stability up to 500 K with identical temperature-dependent decay curves. Concentration quenching occurs in samples with high dopants, which is due to the CR process of Sm³⁺ ions. I-H model analysis reveals that the main mechanism of the CR is EDD interaction with C_DA ~3.730 × 10⁻⁵³ m⁶/s and a critical interaction distance of ~6.40 Å. The Ce³⁺ doped sample SBO:0.01Ce³⁺ displays a broad emission band in the blue region at ~420 nm with a lifetime of ~38.2 ns. A spectral overlap between Ce³⁺ emission and Sm³⁺ excitation is observed, manifesting a possible ET from Ce³⁺ to Sm³⁺. Upon 340 nm of the Ce³⁺ 4f-5d transition in the co-doped samples, the Sm³⁺ luminescence is remarkably enhanced, and the decay curves of the Ce³⁺ in co-doped samples deviate from exponential features, which verify the Ce³⁺-Sm³⁺ ET. The I-H analysis on decay curves of the Ce³⁺ luminescence indicates the main EDD interaction type in the ET process from Ce³⁺ to Sm³⁺. With tunable luminescence upon different wavelength conditions, the Ce³⁺ and Sm³⁺ co-doped SBO samples are regarded as promising candidates for optical anti-counterfeiting.