H.Z. Tao et al. / Solid State Communications 137 (2006) 408–412
411
the bigger weight of In compared with Ga. Furthermore,
considering the less force constant of In-S bonds compared
with Ga–S ones, the A1g mode of InS tetrahedra should locate
Now let us see the spectral evolution of the (1Kx) GeS2–
xIn S glasses (xZ0–0.3). Firstly, the clear evolution of the
region 270–320 cm from a small shoulder to a distinct peak at
2
3
K1
4
K1
K1
at the lower wave number than 315 cm . So it is rational to
K1
306 cm
gives the direct proof about the existence of InS4
attribute the additional peak at 306 cm
stretching vibration of InS tetrahedra.
to the symmetric
tetrahedra within the Ge–In sulfide glassy net. In addition,
following the addition of In S , the similar transformation of the
4
2 3
K1
region 225–255 cm from a small prominence to a dominating
According to the analysis about the Raman spectra of
inverse and partially inverse indium sulfide spinels, Lutz
et al. [7] ascribed the bands in the range 240–255 to the A1g
breathing mode based on the facts that the intensity of this
band increases with increase in the degree of inversion of
K1
K1
peak at 245 cm within the region 200–270 cm indicates
another coordination surroundings of In atoms, viz. InS6
octahedra. And the weaker scattering strength of the prominence
K1
K1
at 245 cm compared with that of another one at 306 cm
manifests itself that the added indium exists mainly in the form of
the spinels. So it is reasonable to ascribed Raman peak at
K1
2
45 cm
to the symmetric stretching vibrating of InS6
InS tetrahedra. Secondly, the incremental quantity of the ethane-
4
octohedra.
. Discussion
The Raman spectrum of the compound GeS glass in Fig. 1
like units S In–InS with the addition of In S within the glassy
3
3
2 3
net can be confirmed by the gradual enhancement of the
K1
characteristic bands at about 150 and 225 cm together with
K1
the slowly broadening of the main peak at 340 cm toward
4
lower wave number aspect originated from another diagnostic
K1
2
(
can be distinctly observed at 115, 340 (A ), 370 (A ) and
0) is similar to those reported previously [11–13]. Four bands
c
band at 321 cm of the S In–InS units. Thirdly, the far weaker
3 3
K1
intensity of the prominence of the band at about 225 cm
K1
compared with that of another one at 255 cm gives us the
1
1
K1 K1
31 cm . The broad band at 115 cm , superimposed on the
4
high frequency tail of the boson peak, was ascribed ordinarily
information that the ethane-like units S
being more preferentially than another similar units S
when sulfur is deficient due to the addition of In . And the
Ge–GeS
comes into
3
3
to the bond bending motions of S atoms in GeS tetrahedra,
4
3
In–InS
3
while Kotsalas, etc. [11] suggested that considerable contri-
bution to this band may arise from intermolecular displace-
ments of whole GeS structural units. The bands at 340 and
S
2 3
K1
gradually widening of the main peak at 340 cm toward the
higher wave number aspect from sample 0–9 can be explained
from the gradual enhancement of another characteristic band at
4
K1
3
undoubtedly to the A symmetric stretching vibrations of GeS4
70 cm are strongly polarized and the former is attributed
K1
about 360 cm [12] of the ethane-like units S Ge–GeS . Lastly,
3 3
1
tetrahedra, while the latter is due to the symmetric stretch
vibrations of S atoms in bridges of edge-sharing (GeS
the descending scattering intensity by inchmeal of the shoulder at
K1
)
/2 4
370 cm isduetothedescendingamountofbridgedunits Ge
originated from the increasingly enhanced quantity of other units
(e.g. InS and InS , etc.) following the addition of In
2 6
S
1
K1
tetrahedra. The shoulder at 431 cm is relatively depolarized
c
(
to the A and A bands) and generally recognized to be due to
1
4
6
S .
2 3
1
the S–S and/or multi-sulfur bonds although there were some
controversies [14]. And this gives a probable existence of small
S–S chains in g-GeS2 either as separate molecular units
5. Conclusion
(
inhomogeneities) or as interconnecting units between GeS
4
K1
The Raman scattering and FTIR transmission spectra of the
prepared polycrystalline In S that belongs to the defect spinel-
type structure was reported. The additional peaks at 306 and
units. In addition, the very weak Raman band at 255 cm (can
be attributed to the vibrational mode of the ethane-like units
S Ge–GeS ; and only can be seen clearly through local
2
3
3
3
K1
245 cm
vibrating of InS and InS microstructural units respectively.
were attributed to the local symmetric stretching
magnification of Raman spectra) give another proof that the
microstructure of the stoichiometric GeS2 glass does not
consist only of GeS tetrahedra.
4
6
The inhomogeneous nature of sample 10 (0.65GeS2–
.35In S ) was clearly confirmed by the Raman scattering
4
0
2
3
According to the Fig. 1, the spectrum 1 exactly corresponds
to the Raman spectra of the prepared polycrystalline In2S3
which further verified the result of the XRD analysis. As to the
spectrum 4, the characteristic bands of the S In–InS ethane-
measurement. Based on the spectral evolution of the (1Kx)
GeS –xIn S glasses, the following micro-structural infor-
mation can be deduced:
2
2 3
3
3
like units can be clearly distinguished based on the distinct
K1
(
1) The added indium exists mainly in the form of InS4
tetrahedra together with a small quantity of InS octahedra
broad peak at about 153 cm
shoulders at about 226 and 321 cm
together with the small
K1
6
[15]. In addition, the
is due to the symmetric stretching
K1
within the glassy network.
2) With the addition of In S , the ethane-like units S Ge–
K1
main peak at 340 cm
mode of GeS and the small prominence at about 255 cm
(
2
3
3
4
GeS are more preferentially formed than the similar S In–
3
3
can be ascribed to the vibrating of the S Ge–GeS ethane-like
3
3
InS units.
3
K1
units. Furthermore, the bands at 306 and 244 cm
attributed to the symmetric stretching vibrations of InS and
can be
Acknowledgements
4
InS6 units, respectively, based on the above-mentioned
ascription. Lastly, the spectra 2 and 3 are intervenient between
the spectrum 1 and 4.
This work was partially funded by the National Natural
Science Foundation of China (No. 50125205), the Opening