of the Sr1ϪXCaXWO4 solid-solution films were independent
of the Ca content: 250Ϯ2 nm for excitation and 463Ϯ2 nm
for emission. Almost all the researchers working in this field
have shared the opinion that the blue band in CaWO4 is due
to an electron transition within undisturbed WO42Ϫ
complexes.22 Our results suggest that the energy gap related
to the blue emission in WO24Ϫ complexes is almost unaf-
fected by the change in Ca content. However, there were
variations in the intensities of the emissions: The films in the
Ca-rich region showed an extremely strong luminescence,
while the films in the Sr-rich region showed a much fainter
emission. A theoretical approach is necessary for a successful
interpretation of the optical properties of these films. How-
ever, theoretical band calculations have not been carried out
yet, due to the fact that these solids have a large number of
atoms in the unit cell.22
It is rather surprising that a complete series of crystal-
lized Sr1ϪXCaxWO4 ͑0рxр1͒ solid-solution films can be
formed even at room temperature ͑25 °C͒. Furthermore, it is
noteworthy that the present films are defect-free showing a
single blue emission and do not contain any impurity phases,
contrary to the films prepared by sputtering at higher tem-
peratures.
FIG. 4. Scanning electron micrographs of the surface ͑a͒ and cross section
͑b͒ of Sr1ϪXCaXWO4 film prepared on an anodic tungsten substrate at room
temperature in the mixed solution of Sr͑OH͒2•8H2O and Ca͑OH͒ of 0.01
2
M, respectively.
decreased with an increase of the Ca/͑SrϩCa͒ ratio in the
solution. For CaWO4 film, the values were about 15 nm from
a 100 reflection and about 55 nm from a 001 reflection,
which agree with the average size ͑about 40 nm͒ observed by
scanning electron microscopy. A typical Raman spectrum of
the Sr1ϪXCaXWO4 film is shown in Fig. 3. All samples ex-
hibited Raman spectra of the tetragonal scheelite-type
structure19 without any impurity phases. Scanning electron
micrographs in Fig. 4 show the surface and cross section of
the Sr1ϪXCaXWO4 solid-solution film. The grain size is
larger than the film thickness. This means that the initially
formed crystals grow preferentially in the horizontal direc-
tion of the substrate, which provides a better supply of the
tungsten species. As shown in Fig. 5, the important feature is
that the films exhibited only a blue emission. Such a single
luminescent feature strongly suggests that the films are
defect-free.20,21 Grasser and Scharmann observed a green
emission in addition to the blue emission at liquid nitrogen
temperature ͑Ϫ196 °C͒ in the alkaline earth tungstates with a
scheelite-type structure that contained defects. This green
emission was interpreted to be ascribed to the existence of
Schottky-defect WO3 .21 In the present film, such green
emission was not observed, but there existed only single blue
emission. The peak positions of the excitation and emission
This work was supported by a Grant-in-Aid for Scien-
tific Research No. 07405028, NEDO International Joint Re-
search Grant. The authors would like to thank M. Osada for
help with Raman spectroscopy, and M. Ishiyama for assis-
tance with x-ray photoelectron spectroscopy.
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FIG. 5. Excitation ͑a͒ and emission ͑b͒ spectra of the Sr1ϪXCaXWO4 films
at liquid nitrogen temperature. The intensities of the spectra were normal-
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starting mixed solution: xM for Sr and yM for Ca.
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