The
characteristics of small cerium oxide and gold–cerium
oxide clusters were investigated as models for gold attachment to
various defect sites on a ceria surface. Photoionization efficiency
(PIE) spectra of gas phase Ce3O
n
(n = 0–4) and AuCe3O
n
(n = 0–3) clusters were
recorded and compared to spectral simulations based on DFT calculations.
Calculated structures and PIE spectra for the Ce3O5,6 and AuCe3O4–6 clusters are
also presented; however, these species were not detected during photoionization
experiments. Addition of an Au atom to Ce3 was found to
increase the energy of the ionization onset by ∼0.4 eV, whereas
addition of one or more oxygen atoms decreases the onset by ∼0.25
eV. The optimized AuCe3O
n
(n = 0–4) cluster geometries correlate with Au atoms
adsorbed to oxygen vacancy sites while the AuCe3O5 and AuCe3O6 clusters are consistent with Au
adsorption to CeO3 and CeO2 vacancies, respectively.
The interactions between the cerium oxide cluster surface and the
adsorbed Au atom were found to strongly depend on the nature the of
the adsorption site. Au adsorbed to O vacancies are negatively charged
with a Ce → Au charge transfer, whereas Au adsorbed to CeO2 and CeO3 vacancies have a reversed Au →
Ce charge transfer, resulting in a positively charged Au atom. Au
adsorption to the Ce3O
n
clusters
has the effect of (i) reducing the differences in the HOMO energies
of the AuCe3O4, AuCe3O5, and AuCe3O6 clusters and (ii) lowering the
binding energy of oxygen atoms for all AuCe3O
n
(n = 1–6) clusters. Au adsorption
appears to have a minimal effect on CeO2 vacancy formation,
although CeO2 vacancies were calculated to form more readily
than O vacancies on both the Ce3O
n
and AuCe3O
n
clusters.
The low energy fragmentation calculated for the Ce3O5,6 and AuCe3O4–6 clusters, via
loss of either Au, O, or CeO2, could potentially make photoionization
experiments unfeasible since these clusters may simply dissociate
when exposed to high energy photons above the ionization threshold.