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M. Womes et al. / Solid State Communications 131 (2004) 257–260
help of the calculated DOS from Ref. [6]. This approach is
based on the assumption of a sufficient screening of the core
hole created by the absorption process. The presence of a
core hole affects mainly transitions in the vicinity of the
absorption threshold, where the kinetic energy of the photo-
excited electron is lowest. These transitions are shifted
towards lower energies, while spectral features at higher
transition energies are rather unaffected. In the present case
core hole effects on peak positions turned out to be
negligible so that the experimental spectra are directly
comparable to densities of states calculated for the
electronic ground state. This same procedure has previously
been applied with success to the spectra of FeS and FeS2
[10] and allows a coherent interpretation of all spectral
features and to establish an experimental picture of the
conduction band structure over a range of approximately
30 eV above EF:
2. Experimental
Polycrystalline In2S3 was synthesised by direct reaction
of a stoichiometric mixture of the elements in an evacuated
silica tube at 1050 8C during 2 h followed by a first
annealing at 800 8C during 4 days and a second annealing
at 450 8C for 3 h. The reaction led to a reddish powder which
X-ray powder diffraction showed to be the pure a-In2S3
spinel phase. X-ray absorption spectra were recorded at the
SuperACO (sulphur) and DCI (indium) storage rings of
LURE, Orsay. All spectra were recorded in transmission
geometry on finely ground powders sieved to 5 mm and
deposited on a microporous membrane. The deposits were
obtained by dispersing the powder in cyclohexane followed
by filtering the solvent through the membrane. The
beamlines were equipped with Si(111) double crystal
monochromators, which were calibrated by setting the
maximum of the S K edge white line in FeS2 to 2472.1 eV
[11] and the first inflection point on the K edge of a Ti metal
foil to 4966.0 eV [12]. The spectral resolution is limited by
the broadening caused by the monochromator (0.3 eV at
2.5 keV, 1.5 eV at 4 keV) and by the finite life time of the
core hole (0.59 eV for S 1s, 3 eV for In 2s and 2p [13]).
Fig. 1. X-ray spectra of In2S3 recorded at the S K, In L1 and In L3
absorption edges, aligned on a common energy scale together with
calculated DOS from Ref. [6].
the distinguishable bands in terms of atomic origin and final
state symmetry as deduced from the spectra and with their
position relative to the top of the valence band as determined
from Fig. 1.
The calculated DOS shows that the In 5p states are split
into two bands from octahedral indium, reflecting the
aforementioned distortion on the B-sites, plus a third, single
band from tetrahedral indium, in agreement with the local Td
symmetry on A-sites. The appearance of unoccupied In 5s
states is consistent with the formal electron configuration
[Kr] 4d10 5s0 5p0 of In3þ. The distribution of In 5s states is
not affected by distortions on lattice sites. The density of
vacant S 3p states shows two structures a and b. Comparison
with the In DOS allows to attribute a and b to sulphur 3p
states hybridised with In 5s and 5p states, respectively.
Structure b comprises S 3p states mixed with all three In p
bands. Their individual contributions are smeared out by the
Gaussian broadening function applied to the calculated
DOS. They give in their sum a single, large band, which is
asymmetrically broadened towards lower energies in
agreement with the shape and the position of the In p
bands. The experimental S K edge spectrum shows two
intense structures, a narrow peak at lower energy and a
broader, asymmetric peak at higher energy, which can be
attributed to transitions to bands a and b, respectively. Their
maxima are separated by 4.2 eV, in good agreement with the
calculated energy difference a 2 b of 3.9 eV. The good
agreement between the theoretical value, calculated for the
3. Results and discussion
Fig. 1 shows the S K, In L1, and In L3 edge X-ray
absorption spectra together with the calculated sulphur p
and indium s and p DOS, convoluted with a Gaussian
function to simulate experimental broadening [6]. The zero
of the common energy scale has been chosen at the top of
the valence band as determined in Ref. [7]. Table 1 lists all
spectral features discussed in the following with their
absolute energies at which they appear on the X-ray
absorption spectra. The table gives also the composition of