K.-M. Schindler et al. / Surface Science 603 (2009) 2658–2663
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the bulk structure of NiO were found. The reason for this discrep-
ancy remains unclear. For a 15 ML thick layer of CoO on Ag(001)
bulk like properties have been found in photoemission and Auger
electron diffraction [13], similar to NiO. On Au(111) a 10 ML thick
CoO(111) film also showed bulk-like angle-resolved photoemis-
sion spectra [14]. Very recently, Torelli et al. showed with a grazing
incidence X-ray diffraction (GIXD) study that CoO films grow
pseudomorphically up to a thickness of 5 ML and gradually relax
to the bulk lattice with increasing thickness [16].
the (10) and (11) reflections. The arrows indicate the unit cell of
the reciprocal lattice and point to the (10) diffraction spots. The
orientations of the two patterns are identical, which shows how
well defined the CoO layer is oriented relative to the Ag(001) sub-
strate with fourfold rotational symmetry. The spots of the CoO
layer are broader than the ones from the Ag(001) surface. Obvi-
ously, the long range order in the CoO film is less perfect than that
of the Ag(001) surface. In summary, the LEED pattern shows that
our preparation results in a film comparable to the ones investi-
gated previously and that the deposition of Co in an O2 atmosphere
has resulted in a film of cobalt oxide growing pseudomorphically
on the Ag(001) substrate.
2. Experiment
Fig. 2 shows the experimental LEED I(V) curves of the clean
Ag(001) surface and the 4 ML thick CoO film on Ag(001). The
two sets of curves are completely different, which is most promi-
nently seen at energies, where a spot of the LEED pattern has max-
imum intensity for one system and minimum intensity for the
other system. Example energies are 80 eV, 115 eV and 225 eV for
the (10) diffraction spot, 120 eV, 145 eV, 230 eV, 290 eV and
330 eV for the (11) spot and 250 eV and 300 eV for the (20) spot.
Obviously, the majority of well ordered Ag(001) parts of the sub-
strate are covered by a uniform layer of CoO thick enough, so that
electrons scattered in the Ag substrate do not reach the surface.
This is in line with previous findings of a nearly layer-by-layer
growth mode of the ultra thin film of CoO. The absence of
Ag(001) LEED spots, however, does not preclude the presence of
small or disordered patches of Ag protruding through the CoO film,
since the scattering of electrons would not result in a diffraction
pattern. However, it has been shown with scanning tunneling
microscopy (STM) that such Ag protrusions are absent in films pre-
pared under these conditions (deposition rate, oxygen partial pres-
sure and most importantly substrate temperature) [6].
A comparison of the LEED I(V) curves from the film and from the
(001) surface of a CoO single crystal gives additional evidence that
the preparation conditions give CoO with rocksalt structure and no
other oxide phase, which cannot a priori be excluded. Fig. 3 com-
pares the (11), (20) and (21) I(V) curves of the cobalt oxide film
on Ag(001) and the (001) surface of a CoO single crystal as pub-
lished [2]. The similarity of the two sets of curves confirms that
the oxide in the film is actually CoO with rocksalt structure. Com-
paring the experiments of the two systems (bulk and thin film) re-
veals another advantage of thin films of insulating materials. In the
case of the bulk single crystal charging effects prevented the
recording of I(V) curves below 170 eV [2], whereas in the case of
the thin film, charges created in the film present no problem as
they are easily transferred to the metallic Ag substrate. As a result
the intensity of the (10) spot could be recorded from an energy as
low as 30 eV, as evident from Fig. 2. For all spots together about 6
additional intensity maxima could be included in the data analysis.
The additional low-energy parts of all spots sum up to 250 eV, a
substantial part of the whole dataset.
Experiments were performed in a standard UHV chamber (Omi-
cron Full Lab) with a base pressure below 5 ꢁ 10ꢂ9 Pa (5 ꢁ 10ꢂ11
mbar). The Ag(001) sample had previously been used for numer-
ous investigations. Therefore, the success of preparations regarding
cleanliness and long-range order of this crystal had been checked
extensively with different methods, including scanning tunneling
microscopy (STM). Prior to the investigations described here, the
Ag sample was prepared by several cycles of Arþ ion sputtering
(600 eV ion energy and typically 2 l
A=m2 ion current) and anneal-
ing at 600 K until sharp LEED spots were obtained.
CoO films were prepared by reactive evaporation of Co metal
from a Knudsen cell in an oxygen atmosphere of 10ꢂ4 Pa (10ꢂ6
mbar) similarly as described previously [13,15]. The deposition
rate was 0.2 ML of CoO per minute as determined using a quartz
microbalance. In order to reduce the roughness of the film, the
Ag substrate was kept at
evaporation.
a temperature of 470 K during
Normal incidence low-energy electron diffraction I(V) curves
were recorded at room temperature with a standard 4-grid LEED
optics (Omicron), a video camera and the Erlangen LEED software.
The orientation of the sample in front of the LEED optics was ad-
justed until minimal differences between symmetry equivalent
beams were achieved. The agreement between the beams was
quantified in terms of Pendry’s r-factor Rp [17]. The orientation of
the sample was adjusted for normal incidence of the electron beam
until an r-factor of below 0.1 was achieved.
3. Multiple scattering calculations
Multiple scattering calculations were performed using the sym-
metrized automated tensor LEED package (SATLEED) of Barbieri
and van Hove [18]. The structure determination of the ultrathin
film of CoO on Ag(001) is based on five independent I(V) curves
with beam indices (1,0), (1,1), (2,0), (2,1), (2,2), energy ranges
from 30 to 400 eV and a total energy range of 1025 eV. Phase shifts
up to an lmax of 9 were derived from the Barbieri–van Hove phase
shift package. The imaginary part of the inner potential was fixed
to 5 eV, the real part was initially set to 10 eV and optimized in
the search procedure. The Debye temperatures of Co, O, and Ag
were initially set to 385, 500, and 225 K, respectively. After a best
fit model has been determined with the Debye temperatures kept
at these values, a second pass of optimization including the Debye
temperatures has been performed. The structural parameters re-
mained basically unchanged in this second pass. However, the er-
ror bars of structural parameters became smaller due to an
increased sensitivity on structural changes.
Unfortunately, no LEED I(V) curves have been published for
other cobalt oxides, in particular Co3O4, the next stable bulk phase
with some Co in the oxidation state 3þ. However, Co3O4 can safely
be excluded by considering the details of its structure, since its spi-
nel structure differs strongly from the rocksalt structure of CoO.
First of all, each side of the unit cell of Co3O4 is about two times
as long as those of CoO, which at least should give rise to a unit cell
doubling and a (2 ꢀ 2) superstructure or an even more complex
pattern. Secondly, there are differences in the Co and O sublattices.
However, it is sufficient to discuss the Co sublattice, since the dif-
ferences are larger than in the O sublattices and the scattering fac-
tors of Co are higher than those of O. The first difference is that the
number of Co atoms in octahedral sites in Co3O4 is only half of that
in CoO. Secondly, an additional quarter of Co atoms occupies tetra-
hedral sites in Co3O4, whereas such sites are not at all occupied in
4. Results and discussion
Fig. 1 shows the LEED patterns of a clean Ag(001) surface and a
CoO film on Ag(001). For easier comparison both patterns have
been recorded at an electron energy of 75 eV and with the sample
at the same position. The bright spots of the patterns correspond to