The interactions of gas molecules with metal oxides used
as catalysts
or support materials in heterogeneous catalysis are highly intriguing.
It is of great importance to gain detailed insight into the complex
and often dynamic behavior of oxide particles under operando conditions.
In this study, the understanding of CO interactions with cerium oxide
surfaces is advanced by bridging the so-called materials and pressure
gaps. This is accomplished by studying the influence of different
types of materials, pressures, and temperatures by using different
infrared spectroscopies as the primary investigation tool. Whereas
low-temperature CO adsorption (<80 K) on various well-defined CeO2 single crystal surfaces yields distinct vibrational bands
that can be assigned to different adsorption sites on fully stoichiometric
and also on reduced surfaces using validated ab initio calculations,
strong gas-phase contributions turn the interpretation of results
obtained for powders under operando conditions into a major challenge.
By using a combination of UHV-IRRAS, in situ transmission infrared
spectroscopy, and operando DRIFTS measurements, the reference data
obtained for single-crystal surfaces under UHV conditions could be
used to assign the features observed in spectra obtained for powder
materials. In the next step, the different CO vibrational bands were
used to monitor surface structural changes occurring at elevated pressures
and temperatures. An increase in the concentration of Ce3+ species as a result of CO-induced reduction could be directly demonstrated
even at low (300 K) temperatures. Our results demonstrate important
progress toward the noninvasive, nondestructive characterization of
real catalysts under operando conditions.