Alexander
Simanenko
a,
Jan
Škvára
b,
Pankaj Kumar
Samal
b,
Evanie
Franz
a,
Robert
Hübsch
a,
Tomáš
Skála
b,
Nataliya
Tsud
b,
Sascha
Mehl
c,
Daniel
Schauermann
a,
Viktor
Johánek
b,
Josef
Mysliveček
b,
Olaf
Brummel
a,
Yaroslava
Lykhach
*a and
Jörg
Libuda
a
aInterface Research and Catalysis, ECRC, Friedrich-Alexander-Universität Erlangen-Nürnberg, Egerlandstraße 3, 91058 Erlangen, Germany. E-mail: yaroslava.lykhach@fau.de
bCharles University, Faculty of Mathematics and Physics, Department of Surface and Plasma Science, V Holešovičkách 2, Prague, 18000, Czech Republic
cElettra-Sincrotrone Trieste SCpA, Strada Statale 14, km 163.5, Basovizza-Trieste, 34149, Italy
First published on 14th April 2025
The stabilities of monometallic Rh and Pd nanoparticles and bimetallic Pd–Rh core–shell nanoparticles supported on Co3O4(111) thin films grown on Ir(100) were investigated with respect to the oxidation state and dissolution in alkaline electrolyte under the conditions relevant for electrochemical ethanol oxidation. Towards this aim, the well-defined model systems were characterized by means of synchrotron radiation photoelectron spectroscopy coupled with an ex situ emersion electrochemical cell (EC-SRPES) and scanning tunneling microscopy (STM). We found that the electronic metal–support interaction (EMSI) has a strong influence on the oxidation state of Rh, resulting in a strong oxidation and anchoring of the oxidized Rh3+ species on the surface of Co3O4(111). Consequently, the EMSI prevents the dissolution of Rh into the electrolyte regardless of the potential range. In contrast, it has no effect on the oxidation state and dissolution of Pd in the potential range of 0.3–1.1 VRHE. However, extending the potential range to 0.3–1.5 VRHE results in a stronger dissolution of Pd due to the reversible oxidation/reduction of Pd, which is enhanced in the presence of the EMSI. Most importantly, the magnitude of the EMSI and, thus, the extent of noble metal oxidation, can be effectively controlled by the nature of the metal/Co3O4(111) interface in the bimetallic Pd–Rh core–shell nanoparticles.
Based on our recent study, the oxidation state and stability of the monometallic Pd/Co3O4(111) system in alkaline environment is strongly influenced by the size and the shape of Pd nanoparticles that are directly controlled by the EMSI.34 In the limit of small Pd nanoparticles, a larger magnitude of the EMSI leads to stronger dissolution. This effect is suppressed for Pd nanoparticles thicker than one atomic layer.34 The benefit of the EMSI for the Pd/Co3O4(111) system is a shift of the onset of oxidation of cylinder-shaped Pd nanoparticles on Co3O4(111) to higher potentials with respect to hemisphere-shaped Pd nanoparticles on HOPG.34 However, above the onset of oxidation, the extent of oxidation of Pd nanoparticles was considerably higher in the presence of the EMSI in the Pd/Co3O4(111) model system.34
In this paper, we systematically investigated the electrochemical stability of the monometallic Rh/Co3O4(111) and Pd/Co3O4(111) model catalysts and the bimetallic Pd–Rh core–shell nanoparticles supported on the well-ordered Co3O4(111) films grown on Ir(100) as a function of chemical composition and the nature of the metal/oxide interface. Towards this aim, we monitored the oxidation states of Rh, Pd and Co atoms before and after potential cycling under the conditions relevant for the electrochemical oxidation of ethanol by means of synchrotron radiation photoelectron spectroscopy coupled with an ex situ electrochemical cell (EC-SRPES). Our findings reveal the critical role of the EMSI in stabilizing the bimetallic core–shell nanoparticles in electrochemical environment and provide valuable insights into the related phenomena.
The Co3O4(111) film was prepared on Ir(100) based on a multi-step procedure35–37 that has been used in other works.32–34 The Ir(100) single crystal (MaTecK, 99.99%) was first cleaned by Ar+ sputtering (300 K, 60 min), followed by annealing in UHV (3 min), then in an oxygen atmosphere (1 × 10−7 mbar, SIAD, 99.999%, 3 min), and again in UHV (3 min) at 1200 K until no traces of carbon or other impurities were found in the photoelectron spectra and a sharp Ir(100) (5 × 1) pattern was observed by LEED. Subsequent annealing of the Ir(100) crystal in an oxygen atmosphere (5 × 10−7 mbar, 1200 K, 5 min) yielded the (2 × 1)−O reconstruction. An epitaxial Co3O4(111) film was then grown on the (2 × 1)−O/Ir(100) surface by PVD of Co metal (Goodfellow, 99.99%) in an oxygen atmosphere (2 × 10−6 mbar) at 273 K, followed by annealing in oxygen (2 × 10−6 mbar) at 523 K for 20 min, followed by annealing in UHV at 680 K for 3 min. This method yielded a continuous, stoichiometric Co3O4(111) film with a thickness of 6.0 nm, as determined from the attenuation of the Ir 4f core level intensity. LEED observations on the prepared films confirmed the epitaxial growth of Co3O4(111) (see Fig. 1a).
The monometallic Pd/Co3O4(111) and Rh/Co3O4(111) model catalysts were prepared by PVD of Pd (MaTecK, 99.9%) and Rh (Goodfellow, 99.9%) metals, respectively, on Co3O4(111)/Ir(100) at 300 K in UHV. The nominal thicknesses of the Pd and Rh films, determined from the attenuation of the Co 2p core level intensity, were 0.39 nm and 0.42 nm, respectively. The Pd and Rh thicknesses, expressed in terms of monolayers (ML), were 1.73 ML and 1.92 ML, respectively, where 1 ML corresponds to 0.225 nm (Pd) and 0.219 nm (Rh).
The bimetallic Pd–Rh core–shell nanoparticles were prepared by subsequent PVD of 1 ML of Pd and 1 ML of Rh metals, or vice versa, on Co3O4(111)/Ir(100) at 300 K in UHV. We denote the resulting core–shell nanoparticles as Pd@Rh/Co3O4(111) and Rh@Pd/Co3O4(111) based on the broadly accepted definition for the core@shell nanoparticles, where the core is an inner metal and the shell is an outer metal.38 The nominal thickness of the core metal was determined from the attenuation of the Co 2p core level intensity, while the nominal thickness of the shell metal was determined from the attenuation of the core level intensity of the core metal.
A specially designed EC cell was connected to the analysis chamber via a buffer chamber and a load lock system. The setup allowed sample transfer between the EC cell and the analysis chamber without exposure to air. A detailed description of the EC setup can be found in our previous publication.29 We used the sample, a gold wire (HMW Hauner, 99.99%), and a commercial Ag/AgCl (ALS, 3 M NaCl, 0.195 VNHE) as the working electrode (WE), counter electrode (CE), and reference electrode (RE), respectively. All glassware, Teflon equipment, and gold wire were soaked overnight in a solution of Nochromix (Sigma-Aldrich) and concentrated sulfuric acid (Merck, EMSURE, 98%). Prior to the experiment, all equipment was rinsed five times with ultrapure water (Milli-Q Synergy UV, 18.2 MΩ cm at 25 °C, TOC < 5 ppb) and then boiled three times in Milli-Q water for 30 min. Gold wire was annealed in the flame of a Bunsen burner and then rinsed with ultrapure water.
The EC voltammograms were acquired upon immersion of the samples in 0.2 M ethanol (C2H5OH, Merck LiChrosolv, 99.9%) containing aqueous (Milli-Q Synergy UV, 18.2 MΩ cm at 25 °C, TOC < 5 ppm) electrolyte of 0.1 M potassium phosphate buffer (K2HPO4, Merck Suprapur, 99.99%; KH2PO4, Merck Suprapur, 99.99%; KOH, Alfa-Aesar, 99.98%) at pH 10. Prior to the experiment, the electrolyte was thoroughly degassed with Ar (Linde, 6.0). The EC measurement was performed by establishing a constant flow of electrolyte at the top of the capillary in the EC cell. The sample was then moved to the capillary under potential control and brought into contact with the electrolyte in a hanging meniscus geometry. The sample was then treated under the conditions of the EC experiments specified below. The potentials were controlled using a potentiostat Gamry Reference 600. The scan rate for all voltammograms was 20 mV s−1. After emersion, the sample was retracted, rinsed with degassed ultrapure water, and transferred to the analysis chamber for SRPES characterization.
Core level spectra were obtained at photon energies of 410 eV (C 1s, Pd 3d, Rh 3d), 550 eV (Pd 3d, Rh 3d), 650 eV (O 1s, Pd 3d, Rh 3d), 810 eV (Pd 3d, Rh 3d), and 930 eV (Pd 3d, Rh 3d). Valence band spectra were acquired at photon energies of 60 eV and 115 eV. In addition, Al Kα radiation (1486.6 eV) was used to measure the Co 2p and Ir 4f core levels. The binding energies in the spectra were calibrated with respect to the Fermi level. All spectra were acquired with a constant pass energy and an emission angle of the photoelectrons of 0° or 20° with respect to the sample normal while using synchrotron radiation or the X-ray source, respectively.
The total spectral resolution values were 200 meV (60–115 eV), 350 meV (410 eV), 500 meV (550 eV), 650 meV (650 eV), 850 meV (810 eV), and 1 eV (930 eV). The KolXPD fitting software was used to process the obtained data and analyze the spectra.39 The spectral components in the Pd 3d and Rh 3d core level spectra were fitted with an asymmetric Doniach–Šunjić function convoluted with a Gaussian profile after subtraction of the Shirley background. The Pd 3d and Rh 3d core level spectra were fitted using a spin–orbit splitting of 5.3 and 4.7 eV, respectively. A fixed branching ratio of 1.5 was used for the Pd 3d core level spectra. The Coster–Kronig effect, which leads to a broadening of the Rh 3d3/2 component compared to Rh 3d5/2, was considered in the fitting of the spectra. Specifically, the Rh 3d core levels were fitted with two asymmetric Doniach–Šunjić functions convoluted with a Gaussian profile, keeping the branching ratio between the peak areas at 1.5. The selected fitting parameters for Pd 3d and Rh 3d spectra obtained from as-prepared model systems are given in ESI, section S1.† The Co3+/Co2+ concentration ratio of the Co3O4(111) was determined from the intensities of the corresponding Co3+ and Co2+ features in the valence band spectra obtained with high surface sensitivity. More details about this method are given elsewhere.32,40
Well-ordered Co3O4(111) thin films were grown on a clean Ir(100) substrate (MaTecK). The clean (5 × 1)−Ir(100) surface was obtained by repeated cycles of ion sputtering followed by annealing at 1330 K in UHV for 3 min, than in 1 × 10−7 mbar O2 for 3 min, and, finally, in UHV for 3 min. Afterwards, the (5 × 1) reconstruction was lifted by annealing at 1270 K in a background pressure of 5 × 10−7 mbar O2 (Linde, 99.999%) yielding the (2 × 1)−O/Ir(100) structure. Co (Alfa Aesar, 99.995%) was deposited onto (2 × 1)-O/Ir(100) in the background O2 atmosphere of 1.5 × 10−6 mbar at 300 K from an electron-heated Ta crucible. After Co deposition, the layer was further oxidized in 2 × 10−6 mbar of O2 for 60 min at 680 K. To achieve the final Co3O4(111) ordering, annealing in UHV at 720 K was performed. The layers were prepared with a nominal thickness of approximately 5.0 nm as determined by a quartz crystal microbalance (QCM) and by attenuation of the Ir 4f XPS signal. The crystallinity of the Co3O4(111) films was verified by means of LEED and STM (ESI, section S2†). The Rh/Co3O4(111), Pd/Co3O4(111), Rh@Pd/Co3O4(111), and Pd@Rh/Co3O4(111) model systems were prepared by the deposition of Rh and Pd metals on the as-prepared Co3O4(111) film from the electron-heated Rh and Pd wires (Goodfellow, 99.99%) in UHV at 300 K. The nominal thickness of the deposited Rh, Pd, Rh@Pd, and Pd@Rh films was determined by means of a QCM. Specifically, the nominal thicknesses of Rh and Pd films in the Rh/Co3O4(111) and the Pd/Co3O4(111) model systems were 0.42 nm and 0.43 nm, respectively, which corresponds to 1.9 ML coverage for both systems. The nominal thicknesses of the core and shell metals in the Rh@Pd/Co3O4(111) were 0.17 nm and 0.19 nm, respectively. The nominal thicknesses of the core and shell metals in the Pd@Rh/Co3O4(111) were 0.19 nm and 0.17 nm, respectively. STM imaging was performed at 300 K using electrochemically etched W tips. STM images were obtained at tunneling voltages and currents of 2.0 V and 0.2–0.35 nA, respectively.
The well-defined model systems are shown schematically in Fig. 1a. The detailed description of the preparation procedures is given in Experimental. The analysis of the electronic structure and morphology of the model systems requires analytical methods which provide high surface sensitivity.41 Methods based on X-ray or electron beam transmission are not suitable due to the low noble metal content and the presence of the bulk metal single crystal substrates. After preparation, the model systems were subjected to the SRPES characterization before and after the series of cyclic voltammetry (CV) procedures in 0.2 M ethanol solution in phosphate buffer (pH 10). The experimental approach is schematically shown in Fig. 1b. The first CV series involved 5 cyclic voltammograms in a potential range of 0.3–1.1 VRHE. This potential range is based on the stability region of Co3O4(111)42 and Pd nanoparticles34 with respect to dissolution and oxidation and represents the typical potential range for ethanol oxidation.43 The second CV series involved 5 voltammograms in the potential range of 0.3–1.5 VRHE followed by 5 voltammograms in the range of 0.3–1.1 VRHE. Typical voltammograms obtained in the potential regions of 0.3–1.1 VRHE and 0.3–1.5 VRHE during the first and the second CV series obtained from the Pd/Co3O4(111) model system are shown in Fig. 1b. Note that the potential range of 0.3–1.5 VRHE includes the regions of partial hydroxylation of Co3O4(111)44 and Pd oxidation.34 Therefore, cycling in the potential range of 0.3–1.5 VRHE involves reversible oxidation and reduction of the catalyst which may potentially trigger restructuring,25,27 chemical reordering in the supported nanoparticles,27 as well as partial dissolution of the noble metals.26 Note that Co3O4(111) film is stable with respect to dissolution in the ranges of both CV series with the rates of Co dissolution well below the detection limit of inductively coupled plasma-mass spectrometry (ICP-MS).29,42
The EMSI in both systems yields a minor fraction of oxidized species incorporated in the oxide or at the metal/oxide interface.32,33 Earlier, we identified the partially oxidized Pdδ+ aggregates in combination with PdOx clusters and atomically dispersed Pd2+sol species in the Pd/Co3O4(111) system,32 and atomically dispersed Rh3+ species in the Rh/Co3O4(111) system.33 Typically, the Pdδ+/Pd2+ aggregates and atomically dispersed Pd2+sol species are strongly attenuated by metallic Pd0 nanoparticles at high coverages.32 As a result, these species are hardly visible in the Pd 3d spectra obtained with surface sensitive photon energies (see Fig. 2a, bottom spectrum) but can be still detected using higher photon energies32 (see ESI, section S3†). In contrast, the contribution from atomically dispersed Rh3+ species is well-resolved in the Rh 3d spectrum at 308.2 eV (Rh 3d5/2). The STM images obtained from the Pd/Co3O4(111) and Rh/Co3O4(111) model systems revealed the growth of well-dispersed Pd and Rh nanoparticles (Fig. 2, side panels). In our previous studies we investigated the morphologies of the Pd and Rh nanoparticles in a great detail.32,33 Basically, both Pd and Rh nanoparticles acquire cylindrical shapes on Co3O4(111), but differ strongly with respect to the average size and the density of supported nanoparticles. Specifically, Pd nanoparticles have average diameter of 5–6 nm and the particle density of 2.7 × 1012 cm−2. In contrast, the Rh nanoparticles have an average diameter of 3.3 nm and the particle density is 7.3 × 1012 cm−2. The observed morphologies are consistent with different magnitude of the EMSI in two systems.33 Namely, the larger magnitude of the EMSI in Rh/Co3O4(111) model system yields the nanoparticles of smaller size at higher particle density with respect to the Pd/Co3O4(111) model system. Nevertheless, the heights of the Pd and Rh nanoparticles are similar, i.e. 3–4 ML.33 Note that the height is the most important parameter determining the extent of oxidation of the Pd nanoparticles supported on Co3O4(111) under electrochemical conditions.34
After the first CV series, we observed a decrease in the total intensity of the Pd 3d spectra (Fig. 2a, middle spectrum and Fig. 2c) accompanied by a shift of the metallic Pd0 contribution by 0.3 eV toward higher binding energies. After the second CV series, we observed much stronger decrease of the Pd 3d intensity (Fig. 2a, top spectrum and Fig. 2c). The corresponding shift of the Pd0 contribution can be explained by adsorption of carbonaceous residues after electrochemical experiments.34 However, the decrease of the total Pd 3d intensity after the first and the second CV series cannot be explained solely in terms of the attenuation. In particular, the loss of Pd due to dissolution in electrolyte has to be taken into consideration. Towards this aim, we performed the analysis of the total Pd 3d intensities obtained with different photon energies before and after CV series (SRPES method, see ESI, section S4†). We validated the SRPES method based on the comparison of the amounts of dissolved noble metal determined by SRPES and online ICP-MS using identical samples subjected to similar electrochemical treatments. The fraction of dissolved metal was calculated using a Python script (see ESI, section S4†). The corresponding approach allowed us to estimate the thickness of the carbonaceous deposits and the amount of dissolved Pd. We estimated that about 7% of Pd is dissolved into electrolyte and about 0.31 nm thick amorphous carbon layer is deposited onto Pd nanoparticles after the first CV series. After the second CV series, 20–25% of Pd is dissolved and 0.52 nm of amorphous carbon film is deposited onto Pd nanoparticles with respect to as-prepared system. Stronger dissolution of Pd after the second CV series is consistent with a larger extent of Pd oxidation due to cycling in the range of 0.3–1.5 VRHE. Earlier we have shown that Pd nanoparticles are strongly oxidized at 1.5 VRHE due to the EMSI effect.34 Nevertheless, the absence of stable palladium oxides in the Pd 3d spectra after the first and the second CV series suggests that the reversible oxidation/reduction of Pd is a fast process and the metallic state is fully recovered after cycling.
Interestingly, we observed very different behavior in the Rh/Co3O4(111) model systems under similar conditions. After the first CV series, the oxidized Rh contribution increased strongly at the expense of the metallic Rh0 contribution (Fig. 2b, middle spectrum and Fig. 2d). In addition, the binding energies of the oxidized and metallic Rh0 contributions shifted by 0.5 and 0.3 eV, respectively, toward the higher binding energy. These shifts were not accompanied by the shifts of the Co 2p or O 1s contributions (see ESI, section S5†). After the second CV series, we observed further oxidation of Rh and a shift of the oxidized and metallic Rh0 contributions to 309.3 eV (Rh 3d5/2) and 307.9 eV (Rh 3d5/2), respectively. Noteworthy, the shift of the oxidized Rh 3d contribution is about 1.0 eV with respect to the corresponding Rh 3d component in as-prepared Rh/Co3O4(111) system. However, at this time, the shift of the oxidized Rh contribution is accompanied by the similar shifts of the Co 2p and O 1s core level spectra (see ESI, section S5†). Generally, this observation suggests a different nature of the oxidized Rh species formed after the first and the second CV series. In this respect, similar shifts of the oxidized Rh 3d and Co 2p and O 1s contributions suggests that oxidized Rh species got integrated into the Co3O4(111) substrate. Note, if oxidized Rh 3d contribution is not accompanied with a similar shifts of the Co 2p and O 1s, it means that oxidized Rh is decoupled from the Co3O4(111) substrate.
With respect to the nature of the oxidized Rh species formed after the first and the second CV series, we refer to the Pourbaix diagram.26 Accordingly, the formation of stable Rh2O3 takes place in the potential range of 0.84–1.79 VRHE in alkaline electrolyte, whereas RhO2 forms above 1.79 VRHE.26 Taking into account the chemical shifts, we assume that after the first CV series, Rh nanoparticles are oxidized at the top forming a Rh2O3-like oxide. In contrast, the oxidized Rh species formed after the second CV series represent atomically dispersed Rh3+ species anchored at the Co3O4(111) substrate in combination with some Rh2O3-like oxide. We note that the Rh3+ species in the form of Rh2O3-like oxide and the Rh3+ species anchored at the Co3O4(111) substrate cannot be resolved reliably due to the similar binding energies.33,45 Therefore, we label the corresponding contributions as Rh3+/RhOx.
Finally, we associate the binding energy shifts of the Rh0 contribution after the first and the second CV series to a particle size effect.46,47 This assignment is consistent with the decreasing size of metallic Rh0 core due to oxidation or disintegration and anchoring of Rh3+ and formation of RhOx species on the Co3O4(111) substrate. Most interestingly, despite the strong oxidation, the decrease of the total intensity of the Rh 3d spectra after the first and the second CV series is rather small. However, we cannot estimate the extent of Rh dissolution in the Rh/Co3O4(111) system due to unknown morphology of the catalyst after CV series. Still, based on the total Rh 3d intensities, we conclude that the extent of Rh dissolution is considerably smaller in comparison to the Pd/Co3O4(111) system.
With respect to the EMSI in the Pd/Co3O4(111) and Rh/Co3O4(111) model systems, we analyzed the oxidation state of the Co3O4(111) support. The Co3+/Co2+ ratios calculated from the heights of the corresponding Co3+ and Co2+ features in the valence bands obtained with photon energy of 60 and 115 eV are shown in Fig. 2e and f. Note that the Co3+/Co2+ ratios obtained with photon energy of 60 and 115 eV correspond to the surface and sub-surface sensitivities, respectively, due to the different inelastic mean free paths (IMFP) of the corresponding photoelectrons.48 The most important differences between the Pd/Co3O4(111) and the Rh/Co3O4(111) model systems concern the evolution of the Co3+/Co2+ ratios obtained with the highest surface sensitivity (photon energy 60 eV). First, in both as-prepared systems, the Co3+/Co2+ ratios are similar. This suggests a similar magnitude of the charge transfer at the metal/oxide interface which corresponds roughly to the reduction of 50% of Co3+ cations in the second cationic layer of the Co3O4(111) substrate.32 Interestingly, the Co3+/Co2+ ratio remains virtually unchanged on Pd/Co3O4(111) after the first and the second CV series. In contrast, the Co3+/Co2+ ratio significantly decreases for Rh/Co3O4(111) after the first and the second CV series. The total drop of the Co3+/Co2+ ratio by as much as a factor of 2 in Rh/Co3O4(111) corresponds to the reduction of nearly 100% of the Co3+ cations in the second cationic layer of the Co3O4(111) substrate.32 The observed differences in the evolution of the Co3+/Co2+ ratios in two model systems suggest that the Co3O4(111) substrate actively participates in anchoring of the oxidized Rh species and, thus, prevents Rh dissolution into electrolyte. Nevertheless, based on the comparison of the Co3+/Co2+ ratios obtained with different photon energies, we assume that the reduction of Co3O4(111) is limited to the surface, while the sub-surface region remains nearly unaffected. This observation suggests that the structure of the Co3O4(111) film is largely preserved during cycling.
Additionally, we explored the depth distribution of the Rh species in the Rh/Co3O4(111) model system by the analysis of the Rh 3d spectra obtained with different photon energies between 410 and 930 eV (see ESI, section S6 and Fig. S6†). We verified that after the first CV series, the RhOx species are distributed at the surface and cover the metallic Rh0 nanoparticles. In contrast, after the second CV series, both the oxidized and metallic Rh0 species are distributed at the surface and do not attenuate the contributions of each other.
The dominant species in both the Rh-core and Pd-shell are metallic Rh0 and Pd0 associated with the main contributions at 307.1 eV (Rh 3d5/2) and 335.3 eV (Pd 3d5/2), respectively. A minor contribution from the atomically dispersed Rh3+ emerges at 308.2 eV (Rh 3d5/2). The STM image obtained from the as-prepared Rh@Pd/Co3O4(111) model system reveals formation of nanoparticles. Earlier, we characterized the morphology of supported Rh@Pd nanoparticles in a great detail.33 We found that the average diameter of the Rh@Pd nanoparticles is 3.0 nm and the density is 7.7 × 1012 cm−2. The observed morphology of the Rh@Pd nanoparticles is similar to the one observed for monometallic Rh nanoparticles. Surprisingly, already after the first CV series, we observed substantial binding energy shifts of the Rh0 and oxidized Rh contributions by 0.7 and 1.0 eV toward higher binding energies, reaching 307.8 eV (Rh 3d5/2) and 309.2 eV (Rh 3d5/2), respectively. In the Pd 3d spectrum, a minor contribution from the Pd2+ state at 337.5 eV (Pd 3d5/2) appeared together with a 0.5 eV shift in the binding energy of the Pd0 contribution toward higher binding energies. Noteworthy, the shift of the oxidized Rh contribution is accompanied by similar shifts of the Co 2p and O 1s core levels (see ESI, section S5†). This observation suggests atomic dispersion and anchoring of the oxidized Rh3+ species on the Co3O4(111) substrate already after the first CV series. This suggestion is in line with the decrease of the Co3+/Co2+ ratios (Fig. 3e).
After the second CV series, no changes in the oxidation state of the Rh@Pd/Co3O4(111) model system were observed. The observed scenario suggests that the Rh@Pd/Co3O4(111) model system is more prone to oxidation than the monometallic Rh/Co3O4(111) and Pd/Co3O4(111) model systems. With respect to the total Rh 3d and Pd 3d intensities, we found that the Rh 3d intensity decrease is minor, whereas the Pd 3d intensity decreases significantly after the first and the second CV series. This observation suggests that the dissolution of the Rh-core is significantly suppressed whereas Pd-shell is prone to dissolution. We performed a similar analysis of the total Pd 3d intensities as in the case of monometallic Pd/Co3O4(111) (see ESI, section S4†). We estimated that about 30% and 50% of Pd-shell dissolves into electrolyte after the first and the second EC series, respectively. The analysis of the depth distribution of the Rh species in the Rh@Pd/Co3O4(111) model system revealed that the Rh3+ species are located mainly at the surface of the catalyst (see ESI, section S6 and Fig. S7†).
Finally, we focus on the Pd@Rh/Co3O4(111) model system, where Pd@Rh core@shell nanoparticles have the Pd-core in the direct contact with the Co3O4(111) substrate (Fig. 4). The Rh 3d and Pd 3d spectra obtained from the as-prepared Pd@Rh/Co3O4(111) model system are shown as bottom spectra in Fig. 4a and b, respectively. The dominant species in both the Pd-core and Rh-shell are metallic Pd0 and Rh0 that give rise to the main contributions at 335.3 eV (Pd 3d5/2) and 307.1 eV (Rh 3d5/2), respectively. A minor contribution from the atomically dispersed Rh3+ emerges at 308.2 eV (Rh 3d5/2). The STM image obtained from the as-prepared Pd@Rh/Co3O4(111) model system reveals formation of nanoparticles. Earlier, we characterized the morphology of supported Pd@Rh nanoparticles in great detail.33 Generally, we found that the average diameter and the density of the Pd@Rh nanoparticles are identical to these observed for Rh@Pd nanoparticles, which correspond to 3.0 nm and the density is 7.7 × 1012 cm−2, respectively.
However, in contrast to the Rh@Pd/Co3O4(111) model system, we observed a significant suppression of oxidation of both Pd-core and Rh-shell after the first CV series. Still, the Rh0 and oxidized Rh contributions shifted by 0.2 and 0.6 eV toward higher binding energies, reaching 307.3 eV (Rh 3d5/2) and 308.8 eV (Rh 3d5/2), respectively. The Pd0 contribution shifted by 0.1 eV toward higher binding energies. Noteworthy, the shift of the oxidized Rh contribution is not accompanied by similar shifts of the Co 2p and O 1s contributions (see ESI, section S5†). Therefore, in correspondence with our previous observation discussed above, we associate the corresponding scenario with the formation of RhOx which is predominantly not in contact with Co3O4(111). Nevertheless, the decrease of the Co3+/Co2+ ratio suggests that a fraction of oxidized Rh species must be also anchored at the Co3O4(111) surface (Fig. 4e). Most importantly, we relate the significant suppression of oxidation of Rh-shell to the lower magnitude of the EMSI due to decoupling of Rh and Co3O4(111) at the interface using the metallic Pd-core as a buffer layer.
After the second CV series, we observed a significant increase of the oxidized Rh contribution at the expense of the Rh0 contribution accompanied by its shift to 309.1 eV (Rh 3d5/2). In addition, a minor contribution of Pd2+ at 337.5 eV (Pd 3d5/2) appeared in the Pd 3d spectrum. Noteworthy, the shift of the oxidized Rh component is accompanied by smaller shifts of the Co 2p and O 1s contributions (see ESI, section S5†). Still, we observed a further decrease of the Co3+/Co2+ ratio, suggesting an increase in the fraction of oxidized Rh species anchored at the Co3O4(111) surface (Fig. 4e). This observation suggests the predominant formation of RhOx over the Pd-core and partial anchoring of Rh3+ species at the surface of Co3O4(111). Additionally, we attribute the appearance of the Pd2+ contribution to the formation of PdO oxide.
With respect to the dissolution of the Pd@Rh nanoparticles, we observed a decrease in the total Rh 3d and Pd 3d intensities by a factor of 2 only after the first CV series. After the second CV series, the total intensity of the Rh 3d core level slightly increased, while the total Pd 3d intensity remain virtually unchanged. We speculate that the effect is caused by a slight expansion of the Rh-shell due to oxidation and distribution of the Rh3+ over the surface of Co3O4(111).
The analysis of the depth distribution of the Rh species in the Pd@Rh/Co3O4(111) model system revealed that the oxidized Rh species are located at the surface of the catalyst (see ESI, section S6 and Fig. S8†).
(b) Bimetallic Pd–Rh nanoparticles: the EMSI has the largest impact on the Rh@Pd core@shell nanoparticles when the Rh-core is in direct contact with Co3O4(111). It results in a strong oxidation and anchoring of a large fraction of oxidized Rh3+ species at the surface of the Co3O4(111). This prevents dissolution of Rh-core into electrolyte but leads to minor oxidation and stronger dissolution of Pd-shell. The impact of the EMSI is minimized for the Pd@Rh nanoparticles, where Pd-core is in direct contact with Co3O4(111). The Pd@Rh nanoparticles are less prone to oxidation and dissolution in comparison to the Rh@Pd nanoparticles. Specifically, Rh-shell in the Pd@Rh nanoparticles gains a higher stability with respect to oxidation in comparison to monometallic Rh nanoparticles.
(d) Bimetallic Pd–Rh nanoparticles: the structure and the oxidation state of the Rh@Pd nanoparticles formed after the first CV series remains stable thereafter. The Pd@Rh nanoparticles remain stable with respect to dissolution but the Rh-shell gets strongly oxidized.
The findings of our study demonstrate the potential of the EMSI to stabilize noble metals against dissolution into electrolytes. However, it is imperative to regulate its magnitude to prevent excessive oxidation of the supported metals under electrochemical conditions. The rational design of multifunctional core@shell nanoparticles offers a promising avenue for enhancing the efficiency of noble metal utilization in electrocatalysis.
Footnote |
† Electronic supplementary information (ESI) available: Fitting parameters for Pd 3d and Rh 3d core levels, STM image of Co3O4(111) film, Pd 3d spectra obtained from Pd/Co3O4(111) using different photon energies; analysis of dissolution and carbon deposition after CV series, validation of the method, Python script, Co 2p and O 1s obtained from Pd/Co3O4(111), Rh/Co3O4(111), Rh@Pd/Co3O4(111), and Pd@Rh/Co3O4(111); IMFPs of Rh 3d and Pd 3d photoelectrons in Pd, Rh, and Co3O4 excited with different photon energies; analysis of the depth distribution of Rh species in Rh/Co3O4(111), Rh@Pd/Co3O4(111), and Pd@Rh/Co3O4(111). See DOI: https://doi.org/10.1039/d5nr00413f |
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