2.3. Luminescent properties
The photoluminescence excitation (PLE) spectra of the Eu
3+ doped glasses are displayed in
Figure 5. All data were obtained at room temperature by monitoring the most intensive characteristic emission of Eu
3+ ions at 613 nm wavelength, corresponding to
5D
0 →
7F
2 transition. From
Figure 5 it can be observed that the PLE spectra consist of broad continuous band ranging from 220 to 350 nm and narrow - peaks in 350 - 600 nm wavelength range. Generally, the excitation broadband in the ultraviolet region arises due to the ligand - to - metal charge transfer (LMCT) from O
2– ligand to W
6+/Mo
6+ ions in WO
n groups (WO
n = WO
4 and WO
6) and MoO
n groups (MoO
n = MoO
4) of the glass matrix as well as from O
2– ions to Eu
3+ ions, i.e. electron transfer from the 2p orbital of O
2– to the empty 4f orbital of Eu
3+ [
30,
31,
32,
33,
34]. As it is seen from the
Figure 5, in the PLE spectrum of the glass x = 50, two maxima of the LMCT band are observed – one at about 260 nm and the other at about 325 nm. Considering the previous assignements of PLE peaks of Eu
3+ ions [
34,
35], the bands at around 260 nm and 325 nm in the excitation spectra obtained would be assigned mainly to the O
2–→ Eu
3+ and O
2–→W
6+/Mo
6+ LMCT transitions, respectively.The stronger intensity of the band at around 260 nm compared to the band at around 325 nm suggests that the O
2–→ Eu
3+ LMCT is taking place largely in the glass x = 50.
The presence of the excitation band of MoO
n and WO
n groups, recorded at the emission wavelength of Eu
3+ at 613 nm suggests the existence of non - radiative energy transfer from glass matrix to the active rare earth ion [
34,
36]. As can be seen, the intensity of this band highly depends on the WO
3 concentration and increases with the increasing of WO
3 content, suggesting that the energy transitions O
2– → W
6+, in comparison to O
2– → Mo
6+, largely influence the intensity of the charge transfer absorption band of host matrix. Thus, it can be assumed that WO
3 will contribute predominantly to the non - radiative energy transfer to the Eu
3+ active ions and the glasses containing significant tungsten oxide concentrations will exhibit the most intense emission. This process is known as host sensitized luminescence.
The excitation spectra also show several peaks between 350 - 600 nm wavelength range, assigned to the f - f intra - configurational forbidden transitions of Eu
3+ from the ground state (
7F
0) and from the first excited state (
7F
1):
7F
0 →
5D
4 (363 nm),
7F
1 →
5L
7 (383 nm),
7F
0 →
5L
6 (395 nm),
7F
0 →
5D
3 (412 nm),
7F
0 →
5D
2 (463 nm),
7F
0 →
5D
1 (523 nm),
7F
1 →
5D
1 (531 nm) and
7F
0 →
5D
0 (577 nm) [
37], of which the
7F
0 →
5L
6 (395 nm) transition is the most intensive and was considered as an excitation wavelength to record the emission spectra. Compared to the LMCT, the f - f transitions are stronger and their intensity increases, as the concentration of WO
3 increases, which is advantageous for achieving appropriate excitation by near - UV and blue LED chips, since in general the intensity of these Eu
3+ transitions is weak due to the fact that they are forbidden by the Laporte`s selection rule [
38].
The photoluminescence emission (PL) spectra of Eu
3+ - doped glasses, recorded under the most intensive Eu
3+ excitation at 395 nm light are shown in
Figure 6. The characteristic emission peaks originated from the radiative transitions of Eu
3+ ions from the
5D
0 excited state to the lower - lying
7F
0,
7F
1,
7F
2,
7F
3,
7F
4 ground states are observed at 580 nm, 593 nm, 613 nm, 652 nm and 702 nm, respectively. The dominant luminescent band is located at 613 nm. From
Figure 6 it is clear that the emission intensity strongly depends on the WO
3 concentration and increases considerably as its content increases. This observation may be due to the occurring non-radiative charge transfer from glass host to the active Eu
3+ ion. Evidence for the existence of the energy transfer is the absence of the characteristic broad emissions of WO
3 and MoO
3 in the spectral range 400 - 600 nm [
39,
40] arising from the fact that the energy absorbed by the tungstate and molybdate groups has transferred non - radiatively to the active Eu
3+ ion.
Among all the observed emission transitions, 5D0→7F2 transition is identified as electric dipole (ED) and is forced by the crystal field environment in the vicinity of the Eu3+ ions, while 5D0→7F1 transition is allowed magnetic dipole (MD) in nature, independent of host matrix.
When Eu
3+ ions are embedded in sites with inversion symmetry, the
5D
0→
7F
1 magnetic dipole transition will dominate; on the contrary, when a Eu
3+ ion site is noncentrosymmetric, the
5D
0→
7F
2 electric dipole transitions will be the strongest in the emission. As a result, the luminescence intensity ratio (R) between electric (
5D
0→
7F
2) and magnetic (
5D
0→
7F
1) dipole transitions can be used as a probe to the nature of the site and symmetry of the coordination sphere and provide valuable information about the local symmetry around the rare earth ion, the strength of covalent bonding between Eu
3+ and its surrounding ligands and the emission intensity. The higher the value of R, the more distortion from inversion symmetry is observed, as well as higher covalency between Eu
3+ and O
2– ions and increased emission intensity [
37,
41,
42]. The calculated intensity ratios R (7.09-7.82) of the obtained glasses (
Table 2) are higher than those of previously synthesized by us glasses [
20,
43,
44,
45,
46] and than other Eu
3+ doped oxide glasses reported in literature [
47,
48,
49,
50,
51,
52,
53], as well as the commercially available red phosphors Eu
3+:Y
2O
3 [
54,
55] and Eu
3+:Y
2O
2S [
56] suggesting that the synthesized samples are characterized with more asymmetry in the vicinity of Eu
3+ ions, stronger Eu - O covalence, and an enhanced emission intensity. From
Table 2 it also could be seen that, the value of asymmetric ratio is increasing as the WO
3 content increases and as a result stronger luminescence is observed.
Additional evidence of the low site symmetry in the vicinity around the active Eu
3+ ions is the presence of the
5D
0 →
7F
0 transition, which is strictly forbidden and according by Binnemans, appears in emission spectra when Eu
3+ ions are located in sites with C
2v, C
n or C
s symmetry [
37]. To further examine the symmetry of the Eu
3+ sites, the
5D
0 →
7F
1 transition is considered, which displays splittings. This implies that the symmetry of the Eu
3+ sites in the studied glasses are C
2v or lower [
57].
The observed optical properties are discussed on the basis of the glass structural features. The most intensive Eu3+ emission peak, corresponding to the hypersensitive 5D0 → 7F2 transition, along with the high values of the luminescent ratio R, evidence that Eu3+ ions are located in low site symmetry in the host matrix. This emission peak intensity and the R values of investigated glasses increases with the increasing WO3 concentration indicating that the substitution of MoO3 with WO3 contributes to the creation of a more distorted and rigid glass structure that lowers the site symmetry of the rare-earth ion and improves its photoluminescence behavior. Furthemore, the increasing intensity of the band at 613 nm (5D0 → 7F2 transition) with increasing WO3 concentration indicates that the WO3 contributes predominantly to the non - radiative energy transfer to the Eu3+ active ions (host sensitized luminescence). Thus, WO3 is more appropriate component than MoO3 for enhancing the luminescent intensity of the doped Eu3+ ion.