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L.E. Muresan et al. / Journal of Alloys and Compounds 755 (2018) 135e146
Fig. 12. The chromatic coordinates of CYSO and CLSO samples under excitation with 235 nm (a) and 303 nm (b).
at 240 nm attributed to 4f8 /4f75d1 transition in Tb3þ. The low
crystallinity of sample and presence of Y2O3 phase may explain the
broadened band that gathers several overlapping bands. Through
Gaussian curve-fitting, these bands are observed at 233 nm,
244 nm and 260 nm (see Fig. 9 a). Comparing the excitation spectra
of CYSO fired at 800 ꢀC with that of Y2O3:Tb, it is obvious that band
at 240 nm brings together components arising from the accom-
modation of Tb3þ in C2, C3i sites of Y2O3 (bands at 244 nm, 260 nm)
and C3, Cs sites in hexagonal Ca2Y8(SiO4)6O2 lattice (band at
233 nm) [13,46]. In case of CLSO sample fired at 800 ꢀC, the small
broad band at 273 nm is due to Tb3þ spin forbidden f-d transition in
La2O3. Further increase of temperature up to 1100 ꢀC significantly
changes the shape of the excitation spectrum by shifting the
240 nm band toward lower wavelength (233 nm) indicating the
formation of Tb3þ luminescent centers in apatite lattice (spin
allowed f-d transitions). Moreover, the two bands with maxima at
274 nm and 303 nm, which are extended into a large spectral
domain may hidden other bands observed in Y2O3:Tb while the
shoulder at 246 nm (seen as an intense band in Y2O3:Tb) become
more evident with the increase of firing temperature. The very
small forbidden fef transitions of Tb3þ are observed in the range
350e450 nm for CYSO samples, but not for CLSO samples (Fig. 9).
The spin allowed f-d transition of Tb3þ in CLSO sample presents a
small shift from 230 nm to 235 nm due to some lattice distortions
caused by the heating process.
The highest excitation peak centered at 235 nm was fixed as
excitation wavelength for recording the emission spectra. Fig. 10
illustrates the emission spectra of apatite (CYSO and CLSO sam-
ples) and oxide phosphors (Y2O3:Tb, La2O3:Tb). The emission
spectra of samples consist of several peaks from 350 nm to 650 nm
with a prominent green emission at 545 nm and 551 nm due to
5D4-7F5 transition. The emission lines at 380 nm, 416 nm, 437 nm,
458 nm are from 5D3-7F6,5,4 transitions, those from 487 nm to
495 nm are attributed to 5D4-7F6, while lines at 585 nm, 592 nm and
625 nm are the results of 5D4-7F4,3 transitions.
A quick observation of PL spectra reveals that the blue emission
dominates in CLSO samples, while green emission is dominant in
case of CYSO samples. This suggests that terbium ions occupy sites
with different symmetry in CYSO and CLSO samples. Furthermore,
correlation with XRD data leads to an interesting observation. Even
though CLSO samples exhibit higher phase purity than CYSO
samples, the PL emission is up to 4 times smaller. This behaviour
can be explained by the incorporation degree of Tb3þ in the ma-
terial during both precipitation process and thermal treatment
stage. In order to make some correlations regarding the emission
intensity and incorporation of Tb3þ in the apatite lattice, the ICP-
OES measurements were performed. Fig. 11 depicts the variation
of emission intensity and the real amount of cations (Ca2þ, Y3þ
,
La3þ, Tb3þ) in phosphor samples with firing temperature.
As a general trend, emission intensity increase with firing
temperature due to improvements of powders crystallinity and
Tb3þ incorporation degree from 0.101 mol to 0.121 mol for CYSO
samples and from 0.108 mol to 0.115 mol for CLSO samples. During
the thermal treatment more and more Tb ions accommodate in the
apatite lattice enhancing the probability of radiative transitions. It
is also observed that the Tb amount in CLSO samples is smaller than
in CYSO samples, this being a possible explanation for the lower PL
intensity of CLSO samples. According with ICP-OES results, we can
say that CYSO samples are closed to theoretical formula
-
Ca2Y7.88Tb0.12(SiO4)6O2 with values for Y3þ and Ca2þ slowly higher
than the theoretical ones, which can be explained by the presence
of Y2O3 as secondary phase in concordance with XRD results. As for
CLSO samples the real amount of Ca2þ is half from the theoretical
values, which indicate that the stoichiometry of the final product is
modified due to un-reacted or redissolved cations. The deviation
from the theoretical composition is expected since the precipita-
tion is an extremely complex process involving a large variety of
ions (Ca2þ, Y3þ, La3þ, Tb3þ) having different precipitation rates and
different solubility products (KCa(OH)2 ¼ 5 ꢂ 10ꢁ6
;
KLa(OH)
¼ 2 ꢂ 10ꢁ21; KY(OH)3 ¼ 1 ꢂ 10ꢁ22) [49]. On the basis of the emission
3
spectra, the chromatic coordinates of CYSO and CLSO phosphors
were calculated and presented in Fig. 12.
It can be observed that CYSO samples are grouped in the green
region of the map, while CLSO samples are situated in the turquoise
region either the excitation is 235 nm (Fig.12a) or 303 nm (Fig.12b).
On the other hand, the firing temperature seems to generate
important color shifts. From Fig. 12a, it is clear that the emitting
color is changed from greenish to turquoise as the firing tempera-
ture increases and the CIE coordinates varies from (0.2137, 0.329) to
(0.260, 0.565). Under 303 nm excitation the color shift is not so