2694
D.E. Starr et al. / Surface Science 600 (2006) 2688–2695
could be formed. In the low temperature regime
(
ꢀ1000 K), the thin carbon film is graphitic in nature. At
higher temperatures, thicker carbon films, exposing carbon
nanowires and curved graphitic layers, are observed. We
suggest that the structure of the carbon film on Pt is the re-
sult of the complex interplay of carbon dissolution/segrega-
tion and therefore may depend on other parameters such as
heating/cooling rates as well. The difference in the struc-
tures of the LT and HT film may explain the different reac-
tivity towards oxygen as previously observed [17].
The carbon films exhibited a surface with a high density
of defects, however, gold species vapor deposited on these
films are found to interact only weakly with the carbon film
supports such that only relatively large ꢀ10 nm particles
were observed by STM at room temperature. This is in con-
trast to Au deposited on various oxide films under the same
conditions, where much smaller particles were stable upon
heating to 500 K. Therefore, the STM data indicate a weak
interaction of metallic gold with carbon substrates, inde-
pendent of the nature and defect structure of the carbon.
Our TPD studies showed that the CO adsorption behav-
ior (desorption temperature, adsorption capacity) is very
similar to that observed for various gold/oxide systems
studied in our group. These results fully support the con-
clusion [6,7] that CO adsorption on gold is essentially inde-
pendent on the nature of support used, however, the
support may influence stability of the smallest Au species
towards sintering.
Fig. 6. In situ Au4f spectra obtained for Au deposited on the HT film
upon stepwise heating in vacuum from 300 to 1000 K. Inset shows the
intensity ratio of Au4f and C 1s signals as a function of the annealing
temperature.
tion of gold with the carbon supports is weaker than with
the oxide surfaces, and that this interaction is not affected
by the nature of the carbon support (LT vs HT film).
Fig. 5c and d presents CO TPD spectra for the two Au/
C surfaces. These spectra are very similar to those we have
observed for Au particles on oxide films [6,7]. As deposited
at 120 K Au species adsorb CO much stronger than do an-
nealed Au particles (Tdes ꢀ 235 K vs ꢀ185 K). In addition,
the CO adsorption capacity drops upon annealing. Both
observations indicate the adsorption of CO takes place
only on low-coordinated Au surface atoms, which decrease
in number upon heating and concurrent sintering. In sum-
mary, these results fully support our previous conclusions
that CO adsorption on gold is essentially independent on
the nature of support used, however, the support may influ-
ence the stability of the smallest Au species, which in turn
depends on the Au/support interaction [3].
Acknowledgments
We acknowledge the Russian National Program
‘
(
‘Development of the Scientific Potential of High School’’
grant UR 05.01.206).
XPS measurements were also conducted for ꢀ0.05 ML
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