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1881
short range order in the lattice, leading to higher energy
transitions. At 600 1C, one more small peak was necessary to fit
the emission band, with energy of 2.47 eV (502 nm), being
ascribed to a green emission. For this sample, the highest
contribution for the emission band comes from the orange
emission, while the other samples have a higher contribution of
the green emission.
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6] E. Longo, E. Orhan, F.M. Pontes, C.D. Pinheiro, E.R. Leite, J.A. Varela, P.S. Pizani,
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Orhan et al. [19,20] performed theoretical studies for the
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disordered structures of CaWO
4
and SrWO
tungsten atoms (W*) by 0.3 A away from oxygen atoms (O*), in
order to break the bonds, thus creating truncated WO clusters. In
4
, by displacing two
[8] Z.R. Silva, J.D.G. Fernandes, D.M.A. Melo, C. Alves, E.R. Leite, C.A. Paskocimas,
˚
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A 78 (2004) 355–358.
3
both theoretical studies of tungstates, the authors ascribed the
bottom of the conduction band to W* (5d) orbitals, whereas the
top of the valence band was occupied by O* (2p), with the bonded
O (2p) orbitals lying at a lower energy position within the valence
band.
Accordingly, the authors suggest that the presence of various
bands in the PL spectra of the CWO thin films is related to these
orbitals. The highest energy bands, green and yellow, may be due
to the radiative decay occurring from the W* (5d) orbitals to the O
[
[
[
[
[
11] G. Blasse, B.C. Grabmaier, Luminescent Materials, Springer, Berlin, Heidelberg,
1994.
12] M. Nikl, P. Bohacek, E. Mihokova, N. Solovieva, A. Vedda, M. Martini, G.P. Pazzi,
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[
[
[
(
2p), while the decay corresponding to the lowest energy, red
band, would be from W* (5d) to O* (2p) [19].
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5
. Conclusions
[19] E. Orhan, M.A. Santos, M.A.M.A. Maurera, F.M. Pontes, A.G. Souza, J. Andr e´ s,
A. Beltran, J.A. Varela, P.S. Pizani, C.A. Taft, E. Longo, J. Solid State Chem. 178
(
2005) 1284–1291.
The polymeric precursor method was successfully employed in
[20] E. Orhan, M. Anicete-Santos, M.A.M.A. Maurera, F.M. Pontes, C.O. Paiva-
Santos, A.G. Souza, J.A. Varela, P.S. Pizani, E. Longo, Chem. Phys. 312 (2005)
the synthesis of powder samples from the Ca
x
Sr1ꢀxWO (0pxp1)
4
1
–9.
system, producing fine single phase powders at a relatively low
temperature. A disordered material was obtained for the heat
treatment temperatures up to 400 1C. Starting from 500 oC, the
[
21] M. Anicete-Santos, E. Orhan, M.A.M.A. de Maurera, L.G.P. Sim o˜ es, A.G. Souza,
P.S. Pizani, E.R. Leite, J.A. Varela, J. Andr e´ s, A. Beltr a´ n, E. Longo, Phys. Rev. B 75
(2007) 165105/1–165105/11.
22] D.S. Gouveia, A.G. Souza, M.A.M.A. Maurera, C.E.F. Costa, I.M.G. Santos, S.
Prasad, J.G. Lima, C.A. Paskocimas, E. Longo, J. Therm. Anal. Calorim. 67 (2002)
%
[
crystallization of the system takes place. The most intense room
temperature PL emission (600 1C) was obtained for the structure
that is neither highly disordered (400 and 500 1C), nor completely
ordered (700 1C).
4
59–464.
[23] D.S. Gouveia, R. Rosenhaim, M.A.M.A. Maurera, S.J.G. Lima, C.A. Paskocimas,
E. Longo, A.G. Souza, I.M.G. Santos, J. Therm. Anal. Calorim. 75 (2004)
453–460.
As for the influence of composition on the optical bandgap, at
[
[
[
24] S.L. Porto, M.R. Cassia-Santos, I.M.G. Santos, S.J.G. Lima, L.E.B. Soledade, A.G.
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25] F.M. Pontes, S.H. Leal, M.R.M.C. Santos, E.R. Leite, E. Longo, L.E.B. Soledade, A.J.
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26] S.C. Souza, I.M.G. Santos, M.R.S. Silva, M.R. C a´ ssia-Santos, L.E.B. Soledade, A.G.
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6
00 1C, the highest short and long range disorder was observed for
, the same compositions that displayed the highest
Ca0.6Sr0.4WO
4
photoluminescent emission. This result corroborates the role of
disorder in the PL phenomenon.
The PL emission spectra could be separated into three of four
Gaussian curves, with a red, red/orange and green emission. The
lower wavelength peak is placed at around 540 nm, and the higher
wavelength peak at about 700 nm. Similar results were reported
[27] F.M. Pontes, M.A.M.A. Maurera, A.G. Souza, E. Longo, E.R. Leite, R. Magnani,
M.A.C. Machado, P.S. Pizani, J.A. Varela, J. Eur. Ceram. Soc. 23 (2003)
3001–3007.
[28] T.T. Basiev, A.A. Sobol, Y.U.K. Voronko, P.G. Zverev, Opt. Mater. 15 (2000)
205–216.
[
[
[
[
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30] F.D. Hardcastle, I.E. Wachs, J. Raman Spectrosc. 26 (1995) 397–405.
31] D.L. Wood, J. Tauc, Phys. Rev. B 5 (1972) 3144–3151.
32] J.A. Groenink, G. Blasse, J. Solid State Chem. 32 (1980) 9–20.
4
in the literature for CaWO .
Acknowledgments
[33] Z. Lou, M. Cocivera, Mater. Res. Bull. 37 (2002) 1573–1582.
[
[
[
34] M. Nikl, P. Strakova, K. Nitsch, V. Petricek, V. Mucka, O. Jarolimek, J. Novak, P.
Fabeni, Chem. Phys Lett. 291 (1998) 300–304.
This work was supported by the Brazilian funding programs
PRONEX/CNPq/ Fapesq and PADCT/CNPq/MCT.
35] M. Martini, G. Spinolo, A. Vedda, M. Nikl, K. Nitsch, V. Hamplova, P. Fabeni,
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Pizani, L.G.P. Sim o˜ es, L.E.B. Soledade, A.G. Souza, I.M.G. Santos, J. Solid State
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