Ru1/MO2 SAC model preparation and single-atom structure confirmation
Ru1/MO2 SACs were prepared following the same protocol to minimize variables (Fig. S1). The supports were first annealed at 450 oC to stabilize their surfaces (Fig. S2), and then their aqueous mixtures with RuCl3 (0.04 wt% Ru) were frozen with liquid N2 and dried with vacuum freeze-drying. The powder precursors were then calcined in air at 400 oC and washed with ammonia water to yield Ru1/MO2 SACs (Fig. S3).
Atomic dispersions of Ru were confirmed with aberration-corrected scanning transmission electron microscopy (Ac-STEM) and extended X-ray absorption fine structure (EXAFS)11. The isolated brighter spots in STEM image indicate atomic dispersions of Ru atoms (Fig. 1a). R-space EXAFS results display clear Ru-O but rare Ru-Ru bonds (Fig. 1b, S4), further confirming the atomic dispersions of Ru on MO2 supports. Mean coordination numbers (CN) of Ru1 are fitted to be 4.9 on TiO2, 5.0 on SnO2, and 5.0 on MnO2 (Table S1). This indicates that Ru atoms display square-pyramidal coordination configurations on MO2 supports (Fig. 1c).
Revealing Ru1-MO2 interaction trends and electronic-level principles
The primary SASI issue deals with M1-support interaction mechanisms through surface coordination bonds and the effects on the stabilization and charging states of M1 atoms. We probe the electronic-level mechanisms of Ru1-MO2 interactions with X-ray absorption near-edge structure (XANES) at Ru L3 edge. In octahedral [MO6] ligand fields, d orbitals split into π-type t2g and σ-type eg states25, and will further split in square-pyramidal [MO5] configurations like Ru1/MO2 SACs (Fig. 1c). L3-edge spectra result from 2p3/2→nd dipole electron transition, and thus can probe the splitting degrees and bonding states of valence nd orbitals24. Ru L3-edge spectra display clear differences among Ru1/MO2 SACs (Fig. 1d). In contrast, K-edge XANES data, resulting from 1s→5p electron transitions, do not show significant differences (Fig. S5). The difference indicates that Ru1/MO2 SACs display similar bonding states for 5p orbitals, but different for 4d orbitals.
The altered peak positions and widths of L3 lines reflect varied coupling strengths between Ru4d and O2p orbitals (Fig. 1d)24,25. Peak position increases following Ru1/TiO2 (2,842.5 eV) ≈ Ru1/SnO2 (2,842.6 eV) < RuO2 (2,843.2 eV) < Ru1/MnO2 (2,844.1 eV). This trend indicates that Ru1 shows the highest valence state on MnO2 and lowest on TiO2. Meanwhile, peak width also increases following Ru1/TiO2 < Ru1/SnO2 < RuO2 < Ru1/MnO2, which also indicates different Ru4d-O2p coupling degrees. The clearly split t2g and eg states suggest more Ru4d-O2p overlaps in RuO2 and on MnO2, while Ru-O coupling is even stronger for Ru1/MnO2. In contrast, the narrower L3 lines on TiO2 and SnO2 mean weaker Ru4d-O2p overlaps and more localizations of Ru4d orbitals. The L3 line of Ru1/TiO2 is further narrower than that of Ru1/SnO2, suggesting that Ru4d-O2p coupling on TiO2 are even weaker than on SnO2. Such different orbital couplings can further lead to varied filling degrees of Ru4d orbitals. The electron densities in Ru4d orbitals increase following Ru1/MnO2 < Ru1/SnO2 < Ru1/TiO2, opposite to the trend of Ru-O coupling strength.
Support effects on Ru1-MO2 binding strengths intrinsically result from different Osl reactivity or oxide reducibility13,30. We characterized the reducibility of TiO2, SnO2, and MnO2 supports with H2 temperature-programed reduction (H2-TPR, Fig. 1e). H2 uptakes show that the reducibility increases following TiO2 < SnO2 < MnO2, consistent with the trend of Ru1-MO2 binding strength. In addition, as oxide reducibility can be measured by the formation energy of oxygen vacancy (EVo), we further studied the correlation of Ru1-MO2 binding energy with EVo through calculations based on density functional theory (DFT) 13. Calculated results (Fig. 1f) show that lower EVo leads to stronger Ru1-MO2 binding with MnO2, while the weakest with TiO2. H2-TPR and calculation results therefore indicate that Osl reactivity fundamentally determines Ru1-MO2 binding strengths. Such varied Ru1-MO2 interactions further alter the extension and filling degrees of 4d orbitals and charging states of Ru1 atoms.
Revealing CO-Ru1/MO2 adsorption trends and electronic-level principles
The second SASI issue deals with adsorbate-M1 adsorption features and mechanisms. We use CO as a model molecule to probe the interaction trend and electronic mechanisms of CO-Ru1 adsorptions. CO coordinates to M1 sites through M-C bonds (Fig. 2a), and the bonding strength is synergistically enhanced by the back donations of electrons from d orbitals to CO’s π*-type lowest unoccupied molecular orbitals (LUMO, Fig. 2b)17. CO-M bonding strength therefore positively correlates to the filling degrees of d orbitals. We characterized CO adsorption on Ru1/TiO2 and Ru1/SnO2 with diffuse reflection infrared Fourier transformation spectra (DRIFTS) at -140 oC (Fig. 2c). No signal could be collected for Ru1/MnO2 owing to the dark color of MnO2. C-O stretching modes locate at 2,128 cm− 1 for Ru1/TiO2 and 2,152 cm− 1 for Ru1/SnO2. This difference means weaker C-O but stronger Ru-C bonds on Ru1/TiO2. Therefore, CO adsorbs more strongly on Ru1/TiO2 than on Ru1/SnO2, further verifying more localization of Ru4d orbitals on TiO2 than on SnO2 as revealed from L3 lines.
We further confirmed CO-Ru1 interaction trends through DFT calculations (Fig. 2d). Calculated CO-Ru1 adsorption energies are 0.65 eV on MnO2, 1.23 eV on SnO2, and 1.72 eV on TiO2. The corresponding Ru1-C bond lengths are 2.04, 2.03, and 1.90 Å. The greatest adsorption energy and least Ru1-C bond length indicate the strongest adsorption of CO with Ru1/TiO2. This calculated Ru1-CO adsorption trend is consistent with DRIFTS results.
The electronic mechanisms of Ru1-MO2 binding and CO-Ru1 adsorption were further analyzed from the changes in the distribution states of Ru4d orbitals and electron densities. Calculated partial densities of states (PDOS, Fig. 2e) of Ru4d orbitals and CO’s π states show clear overlaps between CO’s HOMOs and Ru4d states. This indicates effective adsorptions of CO by Ru1/MO2 SACs. Meanwhile, the different overlapping degrees further indicate different coupling strengths24. Ru1/TiO2 displays the greatest d-π overlap, while Ru1/MnO2 the least. This means that CO can form stronger coordination bonds with Ru1/TiO2. These calculated interaction trends agree with the experimental trends.
The direct effect of CO adsorption is to redistribute the bonding states of Ru4d orbitals, because the nature of forming new bonds and breaking old bonds is to redistribute valence orbitals31. In the [MO5] ligand fields of Ru1/MO2 SACs, Ru4d states mainly couple with the 2p orbitals of Osl atoms, while CO adsorption occurs through overlapping its frontier orbitals with Ru4d orbitals. This interaction polarizes Ru4d states from Fermi levels in Ru1/MO2 SACs into surface coordination bonds around 3.5 eV (Fig. 2e)24. This orbital redistribution effect can be further confirmed by the altered charging states of Ru1 sites13. For Ru1/MO2 SACs, the electron densities apparently accumulate within Ru-Osl bonds but deplete on the surfaces, meaning preferential couple of Ru4d to O2p orbitals. After CO adsorption, the electron densities of Ru-Osl bonds notably decrease for the three Ru1/MO2 SACs; instead, CO-Ru bonds show accumulated electron densities. These changes reveal state redistributions of Ru4d orbitals from Ru-Osl to CO-Ru bonds. In this redistribution-based physicochemical model, CO and Osl are competitive to overlap Ru4d orbitals. Therefore, CO adsorption strength depends on the redistribution tendency of Ru4d orbitals, which are further confined by Ru1-MO2 interactions24.
Revealing catalytic trends of CO oxidation by Ru1/MO2 SACs
The third SASI issue deals with how M1-support and adsorbate-M1 interactions affect SAC’s catalytic performances. The goal is to reveal the roles of M1 and supports in catalytic processes. Here we use CO oxidation as a model reaction to probe the catalytic features and trend of Ru1/MO2 SACs. Temperature-dependent CO conversions catalyzed by Ru1/MO2 and MO2 supports display three features (Fig. 3a). First, Ru1 can enhance CO oxidation, particularly on TiO2 and SnO2. The onset temperature (Tonset) decreases from 260 to 180 oC for TiO2 and from 240 to 160 oC for SnO2. At 260 oC CO conversion increases from 0.0–47.3% for TiO2 and 3.0–100% for SnO2. The enhancement effect of Ru1 on MnO2 is less significant owing to the high intrinsic activity of MnO2. Second, Ru1/MO2 SACs show support-dependent activities. Both Tonset and T100% increase as Ru1/MnO2 < Ru1/SnO2 < Ru1/TiO2. This trend means that Ru1/MnO2 shows the highest activity while Ru1/TiO2 the lowest. Third, the activity trend is opposite to CO-Ru1 adsorption strength, but consistent with support reducibility. This feature suggests that CO-Ru1 adsorption strength does not dominate the catalytic activities of Ru1/MO2 for CO oxidation, while Osl reactivity should play critical roles.
We reveal the catalytic mechanisms with DFT calculations. CO oxidation follows Mars-van-Krevelen (MvK) mechanism by SACs (Fig. 3b)15,17. This approach involves CO adsorption at M1 sites to yield *CO species (i→ii), combination of *CO with Osl to release CO2 and yield VO (iii→v), adsorption of O2 and CO to release CO2 and restore VO (vi→viii→i)4,15.
Calculated CO-Ru1 adsorption energies are − 1.72 eV on TiO2, -1.22 eV on SnO2, and − 0.65 eV on MnO2; however, Ru1/MnO2 is the most active for CO oxidation. The strongest CO adsorption on Ru1/TiO2 does not lead to the highest activity, thus CO adsorption is not the rate-determining step. This may be because CO adsorption from the gas phase is a spontaneous and rapid process and does not need activation. Instead, the activation of Osl to release CO2 should control the whole reaction rates, because the reaction of *CO + Osl → CO2 + VO needs to break multiple Osl-M bonds.
Osl-support binding strength intrinsically determines Osl reactivity and reducibility of oxide supports, and can be measured with the formation energy of VO (EVo)13. Calculated EVo are − 0.87 eV for TiO2, -2.13 eV for SnO2, and − 3.40 eV for MnO2 when coupling to CO oxidation (v). The activation energies (Ea) to form VO are 1.21 eV for Ru1/TiO2, 0.41 eV for Ru1/SnO2, and 0.35 eV for Ru1/MnO2 (iv→v). Both the thermodynamic (EVo) and kinetic (Ea) energies favor the reaction of *CO with Osl on Ru1/MnO2. Therefore, for CO oxidation, Ru1 sites mainly capture CO molecules from the gas phase to form *CO, while support reducibility intrinsically determines the catalytic activity owing to the consumption of Osl through breaking multiple Osl-M bonds.