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Adsorption Sites on Oxide Surfaces
The general objective of this project is to develop models and
techniques to characterize the chemical properties of special surface
sites associated with oxidation catalysis. Metal oxide surfaces
are emulated by oxygen overlayers and by oxide films prepared in situ
by oxidation of metal surfaces. For instance, in one past study
both the promoting role of argon ion bombardment [J. C. de
Jesús, P. Pereira, J. Carrazza and F. Zaera, Surf. Sci. 369
(1996) 217] and the effect of water on the oxidation of nickel films
were studied [J. C. de Jesús, J. Carrazza, P. Pereira and F.
Zaera, Surf. Sci. 397 (1998) 34]. The resulting surfaces are then
characterized by a combination of physical (XPS, AES, SIMS, LEED
and ISS) and chemical (TPD titration) methods in order to determine the
stoichiometry of the surface, the oxidation state of the constituent
elements and the electronic properties of given sites, and to establish
correlations between the presence of specific defect sites on the
surface (such as oxygen vacancies, unique oxidation states or special
coordinations) and chemical activity.
Chemical methods have proven particularly powerful for the detailing of
specific surface sites with unique chemical (and potentially catalytic)
properties. We have over the years focused on the study of
oxygen-treated nickel surfaces as prototypical of many metal
oxides. Specifically, we have taken advantage of the several
ordered layers that form upon oxygen adsorption on the (110) plane of
late transition metal single-crystals. Particular oxidation states on
the surface were first probed by titration experiments using carbon
monoxide [H. Öfner and F. Zaera, J. Phys. Chem. B 101 (1997)
9069]. Indeed, CO TPD proved to be a particular useful local
probe for the investigation of defective NiO surfaces, since its
adsorption energy varies by over 20 kcal/mol in going from a metallic
Ni(110) clean surface to NiO, in a way that correlates roughly with the
number of oxygen atoms directly coordinated to the nickel atom.
This is illustrated by the data shown in the figure below. The
CO-probing experiments also revealed that Ar+ bombardment of thin NiO
films leads to the formation of Ni-O phases similar to those found
during the early oxidation stages of the Ni metal surface.

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Example of the use of small molecules as
chemical probes for the titration of specific surface sites.
Shown in this figure are CO TPD spectra from a Ni(110) crystal covered
with different coverages of oxygen atoms. Discrete temperature
changes on the order of 100 K are seen as the oxygen coverage is
increased, in a way that correlates with the number of oxygen atoms
coordinated to the nickel atom being probed, and, more indirectly, to
its oxidation state.
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Ammonia, although it displays far more complex surface
chemistry, can also be used as a probe molecule, in this case to
identify hydrogen-bonding and acidic surface sites. Initial
studies on the reactivity of ammonia on clean Ni(110) surfaces by TPD
indicated limited decomposition to NH2(ads) at about 300 K, further
dehydrogenation to NH(ads) and N(ads) at around 380 K, and some
NH2(ads) + H(ads) recombination to NH3(g) at ~360 K [D. Chrysostomou,
J. Flowers, and F. Zaera, Surf. Sci. 439 (1999) 34]. More to the
point of this project, it was shown that the dissociative pathway can
be enhanced by surface oxygen and/or hydroxo groups, as indicated by
the TPD and XPS data shown below [H. Guo, D. Chrysostomou, J. Flowers
and F. Zaera, J. Phys. Chem. B 107(2003) 502; H. Guo and F. Zaera,
Surf. Sci. 524 (2003) 1]. Of particular interest in this case is
the new high-temperature (~400 K) desorption state observed at
intermediate oxygen coverages. Our work, as well as that of
others, strongly suggest that ammonia dissociates easily below 400 K,
and that the chemistry observed in that high-temperature state may
involve NH2 (and perhaps NH) surface intermediates. We propose a
facile interchange along the NH3(ads) + O(ads) -> NH2(ads) + OH(ads)
-> NH(ads) + H2O(ads) reaction coordinate, similar to that seen with
water [H. Guo and F. Zaera,Catal. Lett. 88 (2003) 95].

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Evidence for the high reactivity of some
surface oxygen atoms towards ammonia activation on partially oxidized
Ni(110) surfaces. Left panel: sequence of N 1s X-ray
photoelectron spectroscopy (XPS) data for ammonia coadsorbed with
oxygen as a function of temperature illustrating the facile interchange
of hydrogen atoms between the two species. Rapid interconversion
between ammonia and water is attained via the formation of NH2, NH, and
OH surface intermediates. Right panel: sequence of TPD traces for
ammonia desorption from Ni(110) surfaces treated with different amounts
of oxygen. A new high-temperature state is seen above 400 K at
the intermediate oxygen doses associated with O atoms at the end of
O–Ni–O surface chains (see diagram). These oxygen atoms are
believed to be particularly active towards the abstraction of hydrogen
atoms from adsorbed ammonia, the step responsible for the reactions
indicated in the left panel. These experiments exemplify the
importance of specific local ensembles of surface atoms in defining
sites for selective catalysis.
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Chemical probes have been complemented with physical spectroscopic
methods to better identify potential catalytic sites. In one
approach, ion scattering (ISS, or LEIS) has been used in conjunction
with TPD and XPS for the study of the adsorption of hydrogen, oxygen,
ethyl iodide, and 2-propyl iodide on Ni(100) [N. R. Gleason and F.
Zaera, Surf. Sci. 385 (1997) 294]. In all those systems the
decrease in the Ni ISS signal intensity seen during the uptake could be
explained by shielding of the Ni surface atoms by the adsorbate.
In addition, since the ISS data could be correlated nicely with results
from other techniques, the conclusion was reached that matrix effects
and changes in neutralization probabilities (due to variations in work
function) were negligible for the systems studied here.
Additional ISS studies on the adsorption of 2-propyl iodide on
oxygen-precovered Ni(100) indicated that those molecules bond
preferentially to Ni, not O, sites [N. R. Gleason and F. Zaera, J.
Catal. 169 (1997) 365].

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Illustration of the use of ion scattering
spectroscopy (ISS) for the identification of adsorption sites in
complex systems. The data in the main frame correspond to the ISS
spectra obtained after different uptakes of 2-propyl iodide on
O/Ni(100) surfaces prepared by adsorption of 3.0 L of O2 at 300
K. The inset, which shows the ISS peak areas normalized to the
signal of the Ni and O peaks for the surface with 0.0 L 2-C3H7I,
highlights the fact that the alkyl iodides prefer to adsorb on the
metal sites.
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More recently, we have coupled the
use of Xe with other adsorbates as probes for minority surface
sites. Xe is quite inert, but, thanks to his high polarizability,
highly sensitive to its local electronic environment. This can be
detected by changes in the binding energy of the Xe
photoelectrons. The Figure below illustrates how this so-called
PAX spectroscopy works. The left panel displays typical Xe 3d5/7 XPS
data obtained for xenon adsorbed on Ni(110) in equilibrium with
increasing gas-phase Xe pressures, and the right panel summarizes the
data recorded for clean, sputtered, and oxygen-treated surfaces.
Red shifts of up to 1.0 eV in binding energy are seen here in all three
cases, a direct manifestation of the sequential adsorption of xenon on
sites with increasing local electrostatic potentials. Moreover,
each sample starts at a different initial value, pointing to the
different nature of the initial adsorption sites in each case.
For instance, it is seen from the data that sputtering of the surface
leads to the production of more unsaturated surface nickel atoms with a
higher local work function. Finally, the different Xe uptakes
observed as a function of pressure in each of the reported cases
indicates clear differences in the distribution of sites.
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Data from X-ray photoelectron
spectroscopy of adsorbed xenon (PAX) experiments for the
characterization of Ni(110) single-crystal surfaces. Left:
Differential Xe 3d5/2 XPS signals from clean Ni(110) versus equilibrium
Xe pressure. Not only the xenon uptake increases with increasing
pressure, as expected, but the XPS peak position also shifts,
indicating adsorption on different local environments. Right: Xe
surface coverage (open symbols) and 3d5/2 XPS binding energy (filled
symbols) as a function of Xe pressure for clean (circles), sputtered
(squares) and oxygen-dosed (triangle) surfaces. 0.1 L of O2 was
dosed at 400 K in the latter case to obtain a low (<10%) coverage of
atomic oxygen on the Ni(110). Significant drops in binding energy
are seen in all three cases with increasing pressures, suggesting a
sequential population of surface sites with increasing local work
functions. In addition, the different shapes of the uptake curves
points to different distributions of sites in each case.
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The high polarizability of xenon also leads to important
changes in its adsorption energy by the local surface surroundings, and
that energy can be easily measured by TPD. The power of Xe TPD
for the identification of unique surface sites is illustrated by the
data below for atomic oxygen adsorbed on Ni(110). Notice in
particular the increase in Xe desorption temperature seen at low oxygen
coverages (left panel), which we believe is associated with a highly
mobile oxygen atomic species at the end of incomplete –Ni–O surface
rows. That high-temperature Xe peak disappears and is replaced by
a weaker state after oxygen exposures above 0.5 L, and increasing xenon
doses on the low-coverage surfaces also brings up that second
adsorption mode.

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Xe TPD spectra used for the
characterization of O-Ni(110) single-crystal surfaces.
Left: Xe TPD traces obtained after 0.6 L Xe exposures on Ni(111)
treated with various O2 predoses at 400 K. The formation of a new
adsorption site after 0.1 - 0.2 L O2 treatments is signified by the
distinct new high-temperature peak about 100 K. Right: Xe TPD
data versus Xe exposure for a 0.2 L O2 predose. In this case
saturation of peak at 100 K, presumably from Xe adjacent to oxygen
atoms in an active –Ni–O environment, is followed by the growth of a
second feature around 75 K, perhaps the result of a structural change
in the remaining of the surface.
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Ultimately, our interest is to correlate the existence of specific
surface ensembles with specific reactions. In particular, we have
come to conclude that the terminal oxygen atoms in the –Ni–O rows that
form on (110) planes of late transition metals are particularly active
towards hydrogen-transfer reactions. This is shown in the figure
below for the cases of ammonia hydrogen exchange and methyl
hydrogenation steps. In both cases the optimum reactivity is seen
after oxygen doses somewhere between 0.1 and 0.3 L, the exposure range
that leads to the formation of the unique sites identified by the high
Xe desorption temperature. Interestingly, oxidation of both
methyl and methylene groups to formaldehyde does require much higher
oxygen coverages. We have also observed that while ammonia
appears to adsorb on the unsaturated-oxygen sites even at low
temperatures, carbon monoxide does not: the high-temperature Xe TPD
peak is blocked right away by NH3 pre-adsorption, but prevails even
after significant predoses of CO.

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Correlation between the physical
characteristics of O-Ni(110) surfaces with different oxygen coverages
and their reactivity toward methyl hydrogenation and ammonia
hydrogenation-dehydrogenation. Plotted in the main frame are the
TPD yields for methane production from methyl iodide (the precursor for
surface methyl groups) and for ammonia recombination. In both
cases the data show particularly high activity in the 0.1 - 0.3 L O2
exposure range corresponding to the formation of uniquely row-end –Ni–O
unsaturated oxygen atoms. Those sites are identified directly by
the high-temperature Xe TPD peak shown in the inset.
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Researchers
Funding:
Equipment: |
Dr. Hansheng Guo, Mr. Min Shen
Department of Energy - Basic Energy Sciences
UHV Chambers # 2 and # 3
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Last modified on July 28, 2005
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