J. Chem. Phys., Vol. 116, No. 11, 15 March 2002
Adsorption and reaction of sulfur dioxide
4699
Despite the conclusions reached by the latter investiga-
tion, further work is needed to determine the local distribu-
tion of surface species following the interaction of SO2(g)
with the Cu͑110͒ and Cu(110)-p(2ϫ1)-O surfaces. In this
paper we report the results of a coordinated study of the
reaction of SO2(g) with clean and oxygen-covered Cu͑110͒
by STM, XPS, and TPRS. The mechanism of the reaction
and the distribution of structures produced by the reaction
products are clarified.
of the foil. The temperature was monitored by a Chromel-
Alumel thermocouple spot welded to the Ta foil at a location
directly behind the crystal. The surface was cleaned by three
sputter-anneal cycles, with the first anneal done in an O2
atmosphere at 10Ϫ7 Torr. Surface cleanliness and composi-
tion were probed with XPS using nonmonochromatic MgK␣
x-rays. The photoelectrons were collected normal to the sur-
face by the energy analyzer utilizing a 25 eV pass energy.
Binding energies were calibrated with respect to the Au 4f
peak ͑84.00 eV͒ and referenced to the Cu(2p3/2) peak.
The purity of the SO2(g) ͑Praxair, 99.98%͒, O2(g)
͑16O2 , Praxair, 99.999%͒, 18O2(g) ͑MSD Isotopes, 97.7%͒,
and D2S(g) ͑Cambridge Isotope Laboratories, 98%͒ were
monitored with the QMS during dosing; all gases were dosed
from the background. Exposures are reported in units of
Langmuir (1 Lϭ10Ϫ6 Torr s). Typical SO2(g) dosing pres-
sures were on the order 1ϫ10Ϫ8 Torr. The p(2ϫ1) oxygen
overlayer at 0.24 monolayer ͑ML͒ coverage was prepared by
dosing 1.5 L (1ϫ10Ϫ8 Torr, 2.5 min͒ of O2(g) at 450 K,
yielding p(2ϫ1) oxygen islands separated by the uncovered
Cu surface.
II. EXPERIMENT
Most experiments were performed in an ultrahigh
vacuum chamber equipped with STM, low energy electron
diffraction ͑LEED͒, Auger electron spectroscopy ͑AES͒, and
temperature-programmed reaction spectroscopy ͑TPRS͒. The
chamber was equipped with a sputter ion gun and stainless
steel gas dosers. The system exhibited a base pressure of 2
ϫ10Ϫ10 Torr following cleaning, which rose to approxi-
mately 5ϫ10Ϫ10 Torr during experiments.
The homemade ‘‘Johnnie Walker’’ type STM employed
utilizes RHK STM 100 control electronics and a Pt/Ir tip.
The tip was cleaned via induced field evaporation onto a
gold surface ͑ϳ4 A, 15 min͒ prior to imaging.
III. RESULTS AND DISCUSSION
Scan dimensions were calibrated using the
Cu(110)-p(2ϫ1)-O structure.9 All images were processed
with x-offset and x-slope subtraction.
A. Surface characterization
1. XPS
The Cu͑110͒ crystal used was aligned to within 0.5° of
the ͑110͒ plane using Laue backscattering and was mechani-
cally polished down to 0.3 m alumina paste. The crystal
was cleaned in vacuum by three Ar ion sputter ͑2 A, 500
eV, 15 min at 600 K͒ and anneal ͑800 K, 10 min͒ cycles,
with the first anneal done in an oxygen atmosphere (1
ϫ10Ϫ7 Torr) to cleanse the surface of impurities observed in
STM images. Both sharp p(1ϫ1) LEED patterns and sub-
sequent high-resolution STM images were used to assess the
degree of surface cleanliness and order. The crystal could be
cooled to 120 K with liquid nitrogen and heated to 1100 K
by electron bombardment to the back of the crystal. The
temperature was monitored by a Chromel-Alumel thermo-
couple spot welded to a Ta foil in direct contact with the
back of the crystal. The STM ramp housing the crystal and
the STM scan head were allowed to thermally equilibrate
prior to STM measurements.
Separate XPS and TPRS measurements were made in a
second UHV system consisting of interconnected preparation
and analysis chambers. The analysis chamber exhibited a
base pressure of 3ϫ10Ϫ10 Torr and was equipped with
LEED optics, a Perkin-Elmer 04-548 dual anode x-ray
source, an EA-10-plus hemispherical energy analyzer from
SPECS, and a UTI 100c quadrupole mass spectrometer
͑QMS͒ used for TPRS measurements. The ionizer of the
QMS was enclosed in a glass cap with a small hole facing
the crystal surface. A computer coupled to the QMS was
used to record TPR-spectra. The preparation chamber
reached a base pressure of 6ϫ10Ϫ10 Torr and was equipped
with a sputter ion gun and stainless steel gas dosers. The two
chambers were isolated from each other during experiments.
In this system the crystal was supported on a Ta foil and
heated resistively via two Ta wires spot-welded to the back
XPS measurements following adsorption and reaction of
SO2(g) with the Cu͑110͒ surface are shown in Fig. 1͑a͒ and
summarized in Table I.10–17 Except for adsorption and mea-
surement at 240 K, all spectra were taken at room tempera-
ture following anneal to the specified temperature. An O(1s)
spectrum obtained for a saturated p(2ϫ1)-O overlayer at
0.5 ML coverage and a S(2p) spectrum obtained for S(a)
following decomposition of D2S are shown at the top of the
figure for reference. The position of the sulfur S(2p) XPS
signal is consistent with that observed by Roberts and co-
workers in their investigation of H2S(g) reaction on
Cu͑110͒.
Due to the absence of a feature for atomic sulfur, the
S(2p) doublet observed following adsorption at 240 K is
attributed to molecularly adsorbed SO2 . The binding ener-
gies observed are very close to those previously reported for
weak molecular adsorption of SO2 on Ag͑110͒, but are some-
what different from the measured values for Ni, for which
stronger interactions would be expected ͑Table I͒. From the
molecularly adsorbed state the ratio of the photoionization
cross-sections of O(1s) and S(2p) was determined to be
1.60, which is within 3% of the theoretical value of 1.64
determined by Scofield.18 The x-ray photoelectron spectrum
of SO2(a) does not change significantly with temperature
below 300 K.
After the surface is annealed to 324 K the x-ray photo-
electron spectrum is marked by the presence of S(2p) dou-
blets at 161.4 eV and 166.2 eV. The S(2p) peak at 161.4 eV
coincides with that for atomic sulfur, which is evident by
comparison to the reference spectrum for S(a) ͓Fig. 1͑a͔͒.
The O(1s) peak observed after heating to 324 K is shifted by
0.8 eV from that for a p(2ϫ1) oxygen overlayer ͓Fig. 1͑a͔͒.
We attribute this O(1s) peak and the S(2p) doublet at 166.2
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