Oxide-supported Rh catalysts are important components
of commercial
three-way catalysts for pollution abatement. Despite their universal
application, many mysteries remain about the active structure of Rh
on oxide supports as these materials often contain a mixture of nanoparticles
and single-atom Rh species on the same support, even after aging.
Probe molecule Fourier transform infrared (FTIR) spectroscopy in this
work shows that atomically dispersed Rh on γ-Al2O3 prefer to strongly bind CO when exposed to NO and CO mixtures
and that light-off of NO reduction occurs at temperatures similar
to CO desorption, suggesting that the first and rate-determining step
in NO–CO reactions may be the desorption of CO from single-atom
Rh dicarbonyl complexes, Rh(CO)2. Two sets of symmetric
and asymmetric stretching frequencies associated with distinct Rh(CO)2 species are observed in FTIR spectra at 2084/2010 and 2094/2020
cm–1. During temperature ramps, the latter pair
of bands at 2094/2020 cm–1 converts to the 2084/2010
cm–1 bands at 463 K before all symmetric and asymmetric
bands disappear at 573 K. Bands then appear in the range of 1975–1985
cm–1 associated with Rh monocarbonyl, Rh(CO), species
upon the disappearance of the 2084/2010 cm–1 bands,
suggesting that CO desorbs sequentially from Rh(CO)2 by
forming Rh(CO) intermediates. Combined DFT and FTIR experiments suggest
that local OH coverage on the γ-Al2O3 surface
distinguishes the two Rh(CO)2 species: the higher frequency
species resides on a less hydroxylated region and migrates to a more
hydroxylated region at higher temperatures, causing the CO vibrational
frequency to decrease by ∼10 cm–1. CO desorption
occurs from this Rh(CO)2 structure with high local OH coverage,
consistent with the DFT predicted trend of CO binding energies. Because
of the coincidence of CO desorption with the light-off of NO reduction,
local support hydroxylation of atomically dispersed Rh1/γ-Al2O3 catalysts likely affects both
the Rh structure after CO desorption and the kinetics of NO reduction,
studies of which are enabled by the Rh(CO)2 model developed
here.