Introduction

At present, LEDs which can convert power into light via the electrons and holes recombination radiating visible light have been integrated into every aspect of our lives and works. For instance, colorful LEDs are applied to backlight panel for displays and projectors, or as a kind of interior decorative material; white emission LEDs (w-LEDs) are widely used in indoor and outdoor illumination for replacing traditional incandescent due to their excellent characteristics: high luminescent efficiency, brightness, lower power consumption, long operation time, lower manufacture costs, high chemical stability and eco-friendly features etc1,2,3. So far, there have been two kinds of method to get white light emission. One is that combination GaN/InGaN blue ships with YAG:Ce3+ yellow emission phosphors, in which white light is composed of blue light and yellow light with cold color temperature owing to lack of red emission4,5. The other one is based on UV/n-UV chips triple color (red, green and blue) compounds white emission, of which color rendering index is better than the former, but trade-off luminescent efficiency, different decay situations, complex assembly processes and costs expensive are primary reasons for restricting its development6,7. Therefore, the development of a single phase phosphors with white light emission turns into a solution.

Apatite, chemical formula is M10[TO4]6Z2, where M stands cation site with +1, +2 or +3 charges (can be occupied by K+, Na+, Ca2+, Sr2+, Ba2+, Pb2+, Mn2+, La3+, Y3+, Ce3+ etc.), and [TO4] represents anion group (can be replaced by [SiO4], [PO4], [GeO4], [MnO4], [VO4], [AsO4], [SO4] etc.), and Z is anion with −1 or −2 charges generally being O2−, OH and halogen ions8,9. Apatite phase possesses complicated structure, in which exists two kinds of independent M cation sites where [MO9] nine-fold coordinated polyhedron with C3 point symmetry and [MO6Z] seven-fold coordinated polyhedron with CS point asymmetry, contributing to achieve different kinds emission of the same rare earth ion10,11. Until now, a several of apatite type phosphors with white light emission were reported, such as Ca9La(PO4)5(SiO4)F2:Dy3+12, Ba10(PO4)6O:Eu2+,Tb3+/Li+13, Mg2Y8(SiO4)6O2:Ce3+/Mn2+/Tb3+14, Ca5(PO4)3Cl:Dy3+,Li+/Eu3+15 etc. Recently, rare earth element dysprosium has been given intensively attentions and investigated in terms of their unique photoluminescence properties in luminescent materials. Dy3+ ion single-doped phosphors can emit near white light, and need to combinate red emission to get better white light emission, such as Sm3+, Eu3+, Mn2+ etc16,17,18.

Here, we synthesized Ca2La8(SiO4)6O2:Dy3+/Sm3+ phosphors with pure apatite structure for the first time. Traditional solidstate method was employed there. And crystallographic structure and morphology were characterized by using XRD, SEM, FT-IR, while photoluminescence spectra, quenching effect, energy transfer effect and fluorescence lifetimes were measured and analyzed. In addition, temperature dependent spectra also were measured, which indicated excellent thermal stability of 8% emission intensity decrease at 150 °C. The optimal white light emission at (0.309,0.309) with CCT 6848 K, belonging to cold white light, could be suitable applied in commercial w-LEDs application.

Experimental

Materials and synthesis

The solid state method was employed in synthesis of a series of Ca2La8-x-y(SiO4)6O2:xDy3+/ySm3+ phosphors, and the chemicals CaCO3, La2O3, SiO2, Dy2O3, Sm2O3 all are analytic grade purity and purchased by Aladdin Industrial Corporation. Typically, as synthesis of Ca2La7.6(SiO4)6O2:0.20Dy3+/0.20Sm3+ phosphors, marked as CLSO:0.20Dy3+/0.20Sm3+, firstly weighing and mixing raw materials with stoichiometric ratio and then grinding for nearly 10 min at agate mortar. Next the mixture was placed into an alumina crucible and pre-sintered at 1000 °C for 1 h and annealed at 1500 °C for 4 h. Finally, as-synthesized samples naturally cooled to room temperature and ground into powder for measurement.

Measurement and characterization

The XRD patterns of all as-synthesized samples were measured by X-ray powder diffractometer (D8 Advance, Bruker Corporation, Germany) with Cu-Kα radiation λ = 0.15406 nm under the condition of 40 KV and 30 mA, and the range from 10° to 80°. The SEM images were identified by high resolution field emission scanning electron microscope (JSM-7001F). The FT-IR patterns were identified on Fourier transform infrared spectrometer (Spectrum 100, Perkinelmer). The PL and PLE spectra at room temperature were recorded by fluorescence spectrometer (Hitachi F-4600) with a excitation resource xenon lamp (400 V, 150 W), and a 400 nm cut-off filter was used. The decay curves were measured by a spectro-fluorometer (Horiba, Jobin-Yvon TBXPS). Above of measurements are under room temperature. The temperature-dependence spectra were recorded on a spectro-fluorometer (Horiba, Jobin-Yvon Fluorolog-3 FL3-21), combined with a self-made heating attachment and a computer-controlled electric furnace (Tianjin Orient KOJI Co. Ltd, TAP-02).

Results and Discussion

Structure and morphology

Figure 1(A) shows the XRD patterns of CLSO host and CLSO:0.20Dy3+, CLSO:0.20Dy3+/0.20Sm3+ phosphors. As observed, there are similar XRD patterns for the CLSO host and doped samples. And no impurity phase peaks appear, which indicates that rare earth ions substitute the host lattice causing little changes in crystal structure, due to ion radii of Dy3+ (r = 0.97 Å for CN = 7 and r = 1.08 Å for CN = 9)and Sm3+ (r = 1.02 Å for CN = 7 and r = 1.13 Å for CN = 9)are close to that of La3+ (r = 1.10 Å for CN = 7 and r = 1.22 Å for CN = 9)of the CLSO host12,19,20. JADE6.5 software was utilized to analyze these XRD patterns, based on Scherrer’s equation and lattice strain theory, and analysis results, shown on Table 1, demonstrate all samples belonging to hexagonal apatite structure and space group P63/m. The calculated values of CLSO host are little different from that JCPDS No.29-0337 given, and as RE3+ ions doped there is an irregular decrease in cell parameter and unit cell volume (more cell parameters see Supplementary Tables S1S3), owing to in theoretical prediction impurity Dy3+ or Sm3+ ions should only occupy La3+ ions lattice resulting in a regular decrease as impurity RE3+ ions concentration increases in CLSO host crystal structure, but the actual situation exists some difference with theories. During the synthesis process, thermal diffusion being a stochastic and uncontrollable process, though ion radius of Dy3+ or Sm3+ is close to that of La3+ and more suitable to substitute La3+, there still a few part of Ca2+ are replaced by impurity ions and will generate a Ca2+ vacancy when an impurity RE3+ ion with +3 charges occupies a Ca2+ ion lattice point with +2 charges, bringing about irregular lattice distortion.

Figure 1
figure 1

(A) The XRD patterns of CLSO host and CLSO:0.20Dy3+, CLSO:0.20Dy3+/0.20Sm3+ samples and the standard card JCPDS #29-0337 Ca2La8(SiO4)6O2 shown as a reference. (B) The FT-IR spectroscopy of as-synthesized CLSO host, CLSO:0.20Dy3+, CLSO:0.20Dy3+/0.20Sm3+ samples.

Table 1 Space group, cell parameters, and unit cell volume of compounds.

FT-IR pattern of the CLSO host and Dy3+, Sm3+ doped phosphors are shown on Fig. 1(B). As shown, the doped phosphors’ curves are slightly different from the CLSO host, with same absorption peaks at 924 cm−1 and 600–400 cm−1, indicated that dopant will generate negligible influence in term of host crystal structure, completely consistent with XRD analysis results mentioned above. According to the literature21, [SiO4] tetrahedron vibration absorption peaks located on 1100–900 cm−1 and 600–400 cm−1, respectively correspond to the asymmetric Si-O bond stretching modes and the [SiO4] silica tetrahedron bending modes. In this host, the asymmetric stretching of Si-O bond produces an absorption peak of which wavenumber is 924 cm−1, and a multiple absorption peak at 538–400 cm−1 should be assigned to silica tetrahedron bending. Figure 2 shows the SEM images of CLSO:CLSO:0.20Dy3+/0.20Sm3+ sample, and from picture A to picture D magnification are 1.5 K X, 7.00 K X, 16.00 K X and 24.00 K X, respectively. As we observed in images, sample particles have no fixed shape, belonging to gravel-like morphology with particle size from 1 μm to 10 μm.

Figure 2
figure 2

SEM images of CLSO:0.20Dy3+/0.20Sm3+ with different magnification.

Photoluminescence spectra

The PL spectra of CLSO:xDy3+ (x = 0.04, 0.08, 0.12, 0.16, 0.20, 0.24, 0.28 and 0.32) excited at 349 nm are presented in Fig. 3(A), which demonstrate that intensity of emission at 479 nm and 573 nm depend on Dy3+ doping concentration. Two emission peaks shown on Fig. 3(A), of which peak center at 479 nm and 573 nm correspond to 4F9/2 − 6H15/2 and 4F9/2 − 6H13/2 transition respectively, and there is a very low intensity emission at 664 nm corresponding to 4F9/2 − 6H11/2 transition not shown22.It is clearly found that the emission intensity at 479 nm and 573 nm both increase first, and when 0.20 concentration of Dy3+ them reache a maximum, and then decrease as the concentration increasing unceasingly owing to the concentration quenching effect23. According to Van Uitert reported24, the electric multi-polar interaction type dominating energy transfer between adjacent Dy3+ ions of sensitizers and activators, could be estimated by using following Eq. (1):

$$\frac{I}{x}=k{[1+\beta {(x)}^{\theta /3}]}^{-1}$$
(1)

where x refers to the activator Dy3+ ion concentration, I/x represents the emission intensity per activator concentration, k and β are constants for host lattice25. Dipole-dipole, dipole-quadrupole, quadrupole-quadrupole interactions respectively correspond with the values of θ = 6, 8, 10. The above Eq. (1) could equivalently transform into Eq. (2), as follows:

$$aLg(\frac{I}{x})=-\,\frac{\theta }{3}Lg(x)+R$$
(2)

where R is a constant related to k and β. Figure 3(B) shows the fitting line of Lg(I/x) versus Lg(x) in CLSO:xDy3+ phosphors with different wavelength at 479 nm and 573 nm respectively beyond the quenching concentration. It is clearly found that the fitting curves of Lg(I/x) versus Lg(x) are well matched with relatively linear correlation and the slopes were confirmed to be −1.99 and −1.85, corresponding with 4F9/2 − 6H15/2 and 4F9/2 − 6H13/2 transition respectively. Therefore, θ which equals the value of slope multiplied by −3, and are 5.97 and 5.55 respectively. Both of the θ values obtained are closest to 6, meaning that dipole-dipole interaction between Dy3+ ions dominants in energy transfer process, consistent with Liu et.al.12 Sm3+ doped CLSO phosphors also have been studied (see Supplementary Figs S1 and S2), and dipole-dipole interaction is proved.

Figure 3
figure 3

(A) The PL spectra of CLSO:xDy3+ (x = 0.04–0.32) phosphors on Dy3+ doping content (x), inserted graph plots intensity at 479 nm and 573 nm versus Dy3+ doping concentration. (B) The fitting line of Lg(I/x) versus Lg(x) in CLSO:xDy3+ phosphors.

In addition, CLSO:0.20Dy3+/ySm3+ phosphors PL spectra, y varying from 0 to 0.32, were measured, and shown on Fig. 4. It can be clearly observed that with Sm3+ ion doping concentration increasing, the characteristic peaks intensity of Dy3+ at 479 nm and 573 nm both show gradually decreasing due to existence of Dy3+ → Sm3+ energy transfer in Dy3+/Sm3+ co-doped CLSO phosphors system. However, peak at 601 nm which is the characteristic emission of Sm3+ ion in CLSO system, do not exhibit an obvious increase (Fig. 4a,c)with its concentration increasing that is different from Sm3+ single doped CLSO spectra (see Fig. S1). And there two hypotheses proposed, the first one is that absorption and emission efficiency of Dy3+ at 365 nm wavelength both are much higher than those of Sm3+ in CLSO system, the other one is that in the system maybe exist Sm3+ → Dy3+ and Sm3+ → Sm3+ non-radiative energy transfer phenomenon too.

Figure 4
figure 4

The PL spectra of CLSO:0.20Dy3+/ySm3+ (y = 0 − 0.32)phosphors, (a,b) are partial enlargement of the spectra, (c) depicts emission intensity variation at 479 nm, 573 nm and 601 nm in pace with Sm3+ ion concentration increasing.

Energy transfer

The spectra appear variation phenomenon along with Sm3+ ion doping concentration increasing because energy transfer effect dominants. To further understand the energy transfer processes, the PL and PLE spectra, interaction type, critical distance and energy transfer efficiency all were investigated. Figure 5(A) shows the PL spectra of single doped CLSO:Dy3+ and CLSO:Sm3+ phosphors at 365 nm excitation, and the PLE spectra of them monitored at 573 nm and 601 nm respectively. emission peaks center of CLSO:Sm3+ appear at 566 nm, 601 nm and 650 nm caused by the electronic energy level transition of 4G5/2 → 6H5/2, 4G5/2 → 6H7/2 and 4G5/2 → 6H9/2, respectively22. From Fig. 5(A), it can be seen that the PL spectrum (blue line) at 479 nm of Dy3+ overlap with the PLE spectrum (purple line) at 476 nm of Sm3+ proving existence of Dy3+ → Sm3+ energy transfer, and also overlap with the green line PLE spectrum monitored at 579 nm of Dy3+ revealing Dy3+ → Dy3+ energy transfer. Emission peak at 566 nm and emission peak at 579 nm overlapped is the cause of characteristic peak at 566 nm not shown on PL spectra of Fig. 4.

Figure 5
figure 5

(A) The PL and PLE spectra of CLSO:Dy3+ and CLSO:Sm3+ phosphors. (B) The linear fitting of ISO/IS of Dy3+ versus Cn/3 in CLSO:0.20Dy3+/ySm3+ (y = 0–0.32) phosphors. (C) The plotting of ηT versus Sm3+ ion concentration. (D) Decay curves of Dy3+ in CLSO:0.20Dy3+ phosphor excited at 365 nm monitored at 479 nm (I) and 573 nm (II); (III) decay curve of Sm3+ in CLSO:0.20Sm3+ phosphor excited at 365 nm monitored at 601; decay curves of CLSO:0.20Dy3+/0.20Sm3+ phosphor excited at 365 nm monitored at 479 nm (IV), 573 nm (V) and 601 nm (VI).

According to the Dexter’s multipolar interaction energy transfer formula26, as follows:

$$\frac{{\eta }_{S0}}{{\eta }_{S}}\propto {C}^{n/3}$$
(3)

where ηS0, ηS are the luminescence quantum efficiencies of Dy3+ in the absence and presence of Sm3+ respectively, and C stands the total concentration of doping ions, which equals 0.20(Dy3+) + y(Sm3+). The values of n = 6, 8, 10 correspond with dipole-dipole, dipole-quadrupole, quadrupole-quadrupole interactions, respectively. Owing to the values of ηS0 and ηS are hard to measure and ηS0S approximately equals IS0/IS, which stands emission intensity of Dy3+ with/without Sm3+ ion existence, formula (3) can be convert into following formula:

$$\frac{{I}_{S0}}{{I}_{S}}\propto {C}^{n/3}$$
(4)

The relationship between IS0/IS and Cn/3 based on formula (4) are plotted in Fig. 5(B). It can be found that when n value takes 10, the value of linear fitting coefficient R2 is biggest and linear behavior is best, therefore it reveals Dy3+ → Sm3+ energy transfer via quadrupole-quadrupole interaction mechanism, which is consistent with others’ previous investigation27.

With the increase of Sm3+ dopant content, the emission spectra intensity of Sm3+ activators were observed to increase slightly whereas PL spectra intensity of Dy3+ sensitizers simultaneously occur significantly decreasing. The energy transfer efficiency ηT from Dy3+ to Sm3+ can be calculated by following equation28:

$${\eta }_{T}=1-\frac{{I}_{S}}{{I}_{S0}}$$
(5)

Figure 5(C) shows the plotting of ηT versus Sm3+ ion concentration. As it shown, the energy transfer efficiency increases in pace with Sm3+ ion concentration increasing, and When Sm3+ ion concentration is 0.32, the efficiency can reach to 74.72%. and it can be estimated that the critical concentration when energy transfer efficiency is 50%, approximately equals 0.336.

According to the Dexter-Schulman theory the critical concentration will be higher if the energy transfer probability is lower. And the energy transfer probability depends on the distance between sensitizers and activators ions. Therefore, the Dy3+ → Sm3+ energy transfer probability depending on the distance between Dy3+ and Sm3+, on the basis of Blasse’s expression29, the critical distance (RC) of energy transfer can be calculated by Eq. (6), as follows:

$${R}_{{\rm{c}}}=2{(\frac{3V}{4\pi {x}_{{\rm{c}}}{\rm{N}}})}^{1/3}$$
(6)

where V stands the volume of the crystallographic unit cell, and xc the critical concentration, and N the number of lattice sites which can be occupied by dopant ions in the unit cell and N = 1. Substituting V, xc and N into Eq. (6), it is found that the critical distance RC equals 14.809 Å in CLSO:0.20Dy3+/0.20Sm3+ phosphors. And similar values are found in other systems27,30. Therefore, when distance between rare earth ions R < 6 Å, there exchange interaction dominants in energy transfer processes31 while quadrupole-quadrupole interaction contributes to those processes when 6 Å < R < 14.809 Å in CLSO:0.20Dy3+/0.20Sm3+ phosphor.

Decay curves

To further understand the de-excitation and Dy3+ → Sm3+ energy transform processes, decay curves of CLSO:Dy3+, CLSO:Sm3+ and co-doped CLSO:Dy3+/Sm3+ phosphors are measured for 4F9/2 level of Dy3+ ions and 4G5/2 level of Sm3+ ions, and shown on Fig. 5(D). Red lines all are fitting lines and fitting index R2 value also are shown on Fig. 5(D). All samples are excited at 365 nm wavelength with different monitored wavelength, and it can be found that all of decay curves can be successfully fitted with a typical second order exponential decay equation32 as follows:

$$I({\rm{t}})={I}_{0}+{A}_{1}\exp (\,-\,{\rm{t}}/{\tau }_{1})+{A}_{2}\exp (\,-\,{\rm{t}}/{\tau }_{2})$$
(7)

where I(t) represents at time t the luminescence intensity and I0 is the initial luminescence intensity, A1 and A2 are decay constants, τ1 and τ2 respectively stand slow and rapid lifetimes for exponential components. Besides, the effective time (τ*) can be calculated as following equation:

$${\tau }^{\ast }=({A}_{1}{\tau }_{1}^{2}+{A}_{2}{\tau }_{2}^{2})/({A}_{1}{\tau }_{1}+{A}_{2}{\tau }_{2})$$
(8)

Hereafter, the effective lifetimes of 4F9/2 level of Dy3+ in CLSO:0.20Dy3+ phosphor are calculated to be 327.58 μs (479 nm) and 336.74 μs (573 nm), and those in CLSO:0.20Dy3+/0.20Sm3+ phosphor are calculated to be 3.88 μs (479 nm) and 32.44 μs (573 nm); and the effective lifetime of 4G5/2 level of Sm3+ in CLSO:0.20Sm3+ phosphor at 601 nm is found to be 697.07 μs and that in CLSO:0.20Dy3+/0.20Sm3+ phosphor is 22.89 μs. It can be obviously observed that the lifetimes of Dy3+ and Sm3+ have a sharp decrease, considering that the distance between Dy3+ and Dy3+, Dy3+ and Sm3+, Sm3+ and Sm3+ decreases with dopant concentration increasing, causing the probability of energy transfer to luminescent killer sites rising. The lifetime decrease of Dy3+ in co-doped phosphor owing to existing Dy3+ → Sm3+ non-radiative energy transfer because of the overlap between peak at 479 nm of emission spectra of Dy3+ and peak at 476 nm of excitation spectra of Sm3+, interestingly, the lifetime of Sm3+ also appear a sharp decline for the reason that there may exist Dy3+ ↔ Sm3+ bilateral non-radiative energy transfer, consistent with the second hypothesis mentioned above in spectra section.

Temperature dependent PL spectra

To further investigate the possible practical application under high power condition, the temperature dependent photoluminescence spectra of CLSO:0.20Dy3+/0.20Sm3+ phosphor ranging from 303 K to 418 K have been measured at excitation wavelength of 365 nm shown on Fig. 6(A). With temperature increasing from room temperature 303 K to 423 K, it depicts that there is no change occurring in terms of the position and shape of the emission spectra while just the intensity of the emission spectrum decreases. When temperature turns up to 423 K the emission intensity decreases about 8%, compared with that at room temperature 303 K,, which indicates that the CLSO:0.20Dy3+/0.20Sm3+ phosphor exhibits excellent thermal stability for potential w-LED application.

Figure 6
figure 6

(A) Temperature dependent PL spectra of CLSO:0.20Dy3+/0.20Sm3+ phosphor in the range of 303–423 K. (B) The chromaticity diagram of CLSO:0.20Dy3+ (0.286,0.312) and CLSO:0.20Dy3+/0.20Sm3+ (0.309,0.309) phosphors, and digital photograph shows that “FU” and “JIE” are spelled using CLSO:0.20Dy3+ and CLSO:0.20Dy3+/0.20Sm3+ phosphors at 365 nm excitation respectively.

CIE color coordinate and correlated color temperature

The the Commission Internationale de L’Eclairage (CIE) color coordinate and correlated color temperature (CCT) are two important indicators directly inspecting accurate color emission, color purity and its temperature of phosphors. These CIE chromaticity coordinates were calculated based on their PL spectrum, and the results are shown on Table 2 with CCT. The correlated color temperature can be estimated by following McCamy empirical formula27,33:

$${\rm{CCT}}=-\,{\rm{449}}{n}^{3}+3525{n}^{2}-6823n+5520.33$$
(9)

where n equals (x − xe)/(y − ye), and the chromaticity epicenter (xe, ye) is (0.3320,0.1858). All of CCT of CLSO apatite phosphors are over 5000 K, which is boundary temperature, CCT of white light emission less than 5000 K named warn white light used for household lighting or appliances and conversely clod white light more suitable for commercial application for lighting purposes. From Table 2, it can be observed that CLSO:0.20Dy3+/0.20Sm3+ apatite phosphor exhibits better chromaticity coordinate than others at 365 nm excitation, being closet to the ideal white light emission point (0.333,0.333). Figure 6(B) shows the chromaticity diagram of CLSO:0.20Dy3+ and CLSO:0.20Dy3+/0.20Sm3+ phosphors excited at 365 nm, which are consistent with display light emission in the insert digital photograph, of which “FU” spelled by CLSO:0.20Dy3+ phosphor and “JIE” spelled by CLSO:0.20Dy3+/0.20Sm3+ phosphors at 365 nm excitation as well. Those emission characteristics our CLSO:Dy3+/Sm3+ phosphors demonstrated indicate that they can use for commercial w-LEDs application.

Table 2 Table of the comparison of the CIE color coordinates (x,y) and CCT (K) of CLSO:0.20Dy3+/ySm3+ (y = 0–0.32) phosphors excited at 365 nm.

Conclusion

In this article, a series of CLSO:Dy3+/Sm3+ were synthesized by high temperature solid state method, and all as-synthesized phosphors are pure apatite structure and gravel-like morphology with particle size ranging 1–10 μm. In single doped CLSO:Dy3+ phosphors, the characteristic peaks of Dy3+ occur at 479 nm, 573 nm and 664 nm due to 4F9/2 − 6H15/2, 4F9/2 − 6H13/2 and 4F9/2 − 6H11/2 transition, respectively. Moreover, Dy3+ − Dy3+ dipole-dipole interaction primarily contributes to emission quenching effect and quenching concentration at 0.20 Dy3+ ion concentration. In co-doped CLSO:Dy3+/Sm3+ phosphors the luminescence spectra confirmed that existence of Dy3+ → Sm3+ energy transfer phenomenon via quadrupole-quadrupole interaction with the critical distance 14.809 Å. Energy transfer efficiency can up to 74.72% with Sm3+ ion doping concentration increasing. Decay curves reveal that Dy3+ → Sm3+ energy transfer result in lifetimes of 4F9/2 level of Dy3+ having a sharp decrease, and it also occur a sharp lifetime decay of 4G5/2 level of Sm3+ due to there may exists Dy3+ ↔ Sm3+ bilateral non-radiative energy transfer. Our CLSO:0.20Dy3+/0.20Sm3+ apatite phosphor exhibits cold white light emission with CIE chromaticity coordinate (0.309,0.309) and CCT 6848 K. In addition, CLSO:0.20Dy3+/0.20Sm3+ phosphor demonstrates excellent thermal stability and at 423 K emission intensity still is 92% of that at room temperature. These characteristics reveal CLSO:Dy3+/Sm3+ can be a potential candidate for commercial w-LEDs devices.