Literature DB >> 32551181

The Dynamic Structure of Au38(SR)24 Nanoclusters Supported on CeO2 upon Pretreatment and CO Oxidation.

Stephan Pollitt1, Vera Truttmann1, Thomas Haunold1, Clara Garcia1, Wojciech Olszewski2,3, Jordi Llorca4, Noelia Barrabés1, Günther Rupprechter1.   

Abstract

Atomically precise thiolate protected Au nanoclusters Au38(SC2H4Ph)24 on CeO2 were used for in-situ (operando) extended X-ray absorption fine structure/diffuse reflectance infrared fourier transform spectroscopy and ex situ scanning transmission electron microscopy-high-angle annular dark-field imaging/X-ray photoelectron spectroscopy studies monitoring cluster structure changes induced by activation (ligand removal) and CO oxidation. Oxidative pretreatment at 150 °C "collapsed" the clusters' ligand shell, oxidizing the hydrocarbon backbone, but the S remaining on Au acted as poison. Oxidation at 250 °C produced bare Au surfaces by removing S which migrated to the support (forming Au+-S), leading to highest activity. During reaction, structural changes occurred via CO-induced Au and O-induced S migration to the support. The results reveal the dynamics of nanocluster catalysts and the underlying cluster chemistry.
Copyright © 2020 American Chemical Society.

Entities:  

Year:  2020        PMID: 32551181      PMCID: PMC7295362          DOI: 10.1021/acscatal.0c01621

Source DB:  PubMed          Journal:  ACS Catal            Impact factor:   13.084


A great challenge in nanocatalysis is to produce truly homogeneous, structurally well-defined, and highly active nanostructures that can serve for fundamental studies and new applications. Thiolate-protected metal nanoclusters (Mn(SR)m) with well-defined structures offer a route toward creating atomically precise and catalytically active sites,[1−4] providing model systems for atomic level studies of catalytic properties.[3,5,6] It is well-accepted that Au clusters (with <100 Au atoms) supported by metal oxides exhibit excellent catalytic activity for (low temperature) oxidation[4,7−14] and hydrogenation,[15−17] especially when compared with larger Au nanoparticles. Au clusters facilitate reactant activation due to higher adsorption energies. Nevertheless, the initially well-defined Au cluster structure may change during pretreatment and reaction, which is also affected by cluster size and the type of support material.[18−21] Previously, we have studied structural changes of Au clusters of different size, that is, Au(SC2H4Ph) (x = 25, 38, and 144, y = 18, 24, and 60) supported on metal oxides (CeO2, Al2O3, and SiO2) upon oxidative pretreatment and liquid phase reaction. In situ X-ray absorption fine structure spectroscopy (XAFS) and high-energy resolution fluorescence detected–X-ray absorption spectroscopy (HERFD-XAS) revealed higher cluster stability on CeO2 and SiO2[21−23] than on Al2O3. Here, we refine the structural picture on cluster chemistry by in situ/operando extended X-ray absorption fine structure (EXAFS) and diffuse reflectance infrared fourier transform spectroscopy (DRIFTS), to directly monitor the dynamic structure of Au38(SC2H4Ph)24 clusters on CeO2, both during ligand removal and CO oxidation. CO oxidation has been repeatedly used to assess the catalytic properties/active sites of (mainly CeO2) supported thiolated gold nanoclusters, particularly addressing ligand effects.[14,18,24−28] Two different mechanisms were proposed: (i) Mars–van Krevelen, with CO adsorbed on Au and active oxygen provided by CeO2 at the metal/oxide interface,[29] which was supported by Good et al. showing that the reaction of oxygen from the ceria lattice with CO adsorbed on gold was the rate limiting step;[30] (ii) Langmuir–Hinshelwood, with CO and O coadsorbed on neighboring Au sites.[31] Lopez Acevedo et al. explained the catalytic activity of thiolate protected gold nanoclusters with their HOMO–LUMO energy gap, which matches the binding energy of oxygen on Au.[31] Hence, for Au38(SR)24 clusters only the removal of ligands turns them into electropositive species that are able to adsorb O2. A combination of activated adsorbed and lattice oxygen provides ideal conditions for reaction with adsorbed CO. Jin and co-workers proposed that not the bulkiness of the hydrocarbon tails but the ligands at the interface between thiolated Au clusters and CeO2 inhibited CO adsorption on Au and reaction with lattice O, hence adversely affecting CO oxidation.[25] Accordingly, pretreatments removing the ligand shell should have a positive effect on activity. Nie et al.[27,28] reported for Au(SR)/CeO2 (n = 25, 38, m = 18, 24) that partial thiolate (ligand) removal led to higher activity than complete ligand removal. According to Wu et al.,[26] partial removal of thiol ligands by oxidation around 150 °C enabled CO adsorption on the exposed Au surface,[26,27] whereas full removal did not have any further effect.[26] Overall, the effect of thiolate ligands and their removal on the catalytic activity of Au nanoclusters is still controversially discussed.[1,4,14,18,21,25,30,32] Recently, we have reported a new effect, that is, migration of thiolate ligands from the Au clusters to the supporting oxide.[23] Although the assumption had been that thiolate ligands “disappeared” into the gas phase upon oxidative activation, S K-edge XAFS measurements detected that oxidized sulfur species remained on the support.[23] The redistribution and oxidation of S modified the support, which may also alter its catalytic function (e.g., by poisoning interface sites or vacancies). Herein, we performed more detailed in situ/operando EXAFS/DRIFTS and ex situ scanning transmission electron microscopy–high-angle annular dark-field imaging/X-ray photoelectron spectroscopy (STEM-HAADF/XPS) studies of structural changes of Au38(SR)24/CeO2 upon pretreatment and CO oxidation. In situ XAFS Au L3-edge spectra of Au38(SR)24/CeO2 upon different oxidative pretreatment indicated that not only ligands were removed but also that staples collapsed, depositing S atoms on the Au surface (poisoning). At higher temperature, S species migrated from the Au clusters to the support, creating bare active Au surfaces. During CO oxidation, further structural changes occurred via CO-induced Au and O-induced S migration to the support. The complex temperature dependence of these structural changes and the formation of Au–S units may explain the conflicting reports in literature on the effect of pretreatment on catalytic properties. The atomic structure of Au38(SC2H4Ph)24 was previously solved by X-ray crystallography,[33] with EXAFS confirmation thereafter.[34−36] The Au38(SR)24 nanoclusters consist of a symmetric biicosahedral structure Au23 core, which is protected by three monomeric (SR-Au-SR) and six dimeric staples (SR-Au-SR-Au-SR; Scheme ).
Scheme 1

Au38(SR)24 Nanocluster (Initial) Structure with Distances Fitted by EXAFS

As mentioned, oxidative catalyst activation is required and the structural evolution of CeO2 supported Au38(SR)24 nanoclusters were studied by Au L3-edge XAS (Figure ).
Figure 1

EXAFS fit (red) in R space of the as-prepared sample, after pretreatment (150 or 250 °C, in 5% O2 in He) and after CO oxidation reaction.

EXAFS fit (red) in R space of the as-prepared sample, after pretreatment (150 or 250 °C, in 5% O2 in He) and after CO oxidation reaction. The Artemis package[37] using the FEFF8 code[38] was applied for EXAFS data treatment, building a cluster model based on the known crystal structure. The fitted values of the three key distances are illustrated in Scheme . The AuAu distance characterizes neighboring Au atoms (e.g., those in the core). There are two different Au–S bond distances, one corresponding to Au0core-S and the other to Au+staple-S. The cluster’s structural changes upon pretreatment were evaluated via two main EXAFS parameters: R (distance) and N (coordination number of neighboring equivalent atoms). Table S1 and Figure S3 collect the fitting results, while the deduced structural changes are illustrated in Scheme .
Scheme 2

Evolution of the Au38(SR)24/CeO2 Cluster Structure Derived from EXAFS Fit, after Pretreatment at 150 or 250°C and Subsequent CO Oxidation

As expected, the number of nearest equivalent Au neighbors (NAu–Au) increased upon pretreatment (2.59 to 5.08 or 8.09), because of the increasing removal of the ligands, but EXAFS analysis still suggested that the core structure was preserved. However, the N values of Au0core-S and Au+staple-S, which are expected to continuously decrease upon pretreatment, showed a deviating behavior. Apparently, the structural changes are more complex than just a simple successive removal of (entire) ligands. When Au38(SR)24/CeO2 was pretreated at 150 °C, the AuAu and Au–S distances (R) did not change. In line with ligand removal, N of AuAu increased and N Au+staple-S strongly decreased, but N Au0core-S unexpectedly increased. The removal of the thiolate carbon backbone seems to collapse the remaining staples, creating new bonds between Au–Au but also between the outer Au atoms of the cluster core and S (Au0core-S). Pretreatment at 250 °C almost completely removed S from the cluster core, as N Au0core-S became almost zero. However, N Au+staple-S was still 0.45, indicating creation of Au+-S configurations, which can only be on the support (staples collapsed at 150 °C not reestablished at 250 °C). Figure shows catalytic CO oxidation, comparing pretreated Au38(SR)24/CeO2 with CeO2. Catalytic activity was monitored by a mass spectrometer (MS) connected to the reaction cell outlet. Au38(SR)24/CeO2 pretreated at 150 °C showed only minute activity even at 150 °C. This confirms the structural model, as Au atoms blocked by S were inaccessible for CO and O2 adsorption.
Figure 2

CO oxidation on 2 wt % Au38(SR)24 supported on CeO2 (flow: 3.3% CO, 7% O2, 89.7% He, total flow: 60 mL/min, ramp: 5 °C/min): CO2 MS traces normalized to the catalyst mass and the He signal, after different pretreatments, and for the pure support.

CO oxidation on 2 wt % Au38(SR)24 supported on CeO2 (flow: 3.3% CO, 7% O2, 89.7% He, total flow: 60 mL/min, ramp: 5 °C/min): CO2 MS traces normalized to the catalyst mass and the He signal, after different pretreatments, and for the pure support. In contrast, Au38(SR)24/CeO2 pretreated at 250 °C was active even below 40 °C, being more than 50-times more active than the catalyst sample pretreated at 150 °C (pret150). Again, this confirms the structural model of bare Au surfaces, as Au+-S species are inactive. The as-prepared Au38(SR)24/CeO2 catalyst with intact ligands was nearly inactive and also sintered, losing the cluster monodispersity; therefore, it will not be further considered here. In order to investigate reaction-induced structural changes, the samples were again characterized by EXAFS after CO oxidation (Table S1 and Figure S3). During reaction on the catalyst sample pretreated at 250 °C (pret250), the Au core structure present after pretreatment was preserved, indicated by the only slightly reduced AuAu coordination numbers, the bond distances and EXAFS fitting (minimal change of σ02Au–Au). However, N Au+staple-S decreased and N Au0core-S increased during the reaction. As S migration back to the cluster is unlikely, this suggests that (isolated) Au+staple-S converted to (agglomerated) Au0core-S on the support and/or that Au+staple-S dissociated. Additionally, more Au atoms may move to the support and merge with S species. Migration of Au atoms under reaction conditions can be explained by CO-induced atom mobility, as observed before,[39−41] which explains the decrease of N AuAu. Accordingly, S species are mobile not only during pretreatment, as shown by our previous XANES study,[23] but also during the catalytic reaction. The two Au–S species will not contribute to catalytic activity, as S is a strong poison. During CO oxidation on the less active pret150 sample with initially S-poisoned Au surfaces, S moved to the support (decreasing N Au0core-S and increasing N AuAu) and merged with CO-mobilized Au atoms (increasing N Au+staple-S). However, during reaction at 150 °C activity did not increase significantly. S may be removed from the clusters, but it will still poison the surrounding ceria. To address morphological changes, STEM-HAADF images were acquired for the “as-prepared” catalyst and the catalysts after CO oxidation (Figure S6). In all cases, Au nanoclusters of 2–4 nm size were identified. Smaller entities, like Au–S particles formed by migration of Au and S species during reaction (as indicated by N Au+staple-S) may be present as well but were beyond detection. Possible reaction-induced changes in the Au oxidation state were studied by X-ray photoelectron spectroscopy (XPS) (Figure S7). For the as-prepared sample, the Au 4f7/2 signal at 84.2 eV is characteristic of ceria supported Au clusters that are modified by metal–ligand interaction. For ligand-free Au0 nanoclusters on ceria,[42,43] a binding energy of 83.8 eV was reported by Huang et al.[23,44,45] After pretreatment and reaction, the Au 4f signals were shifted to lower binding energies. For the pret150 catalyst, the small shift agrees with the collapse of the staples, while for the pret250 sample, the −0.3 eV shift corroborates the formation of bare Au0 clusters. To monitor adsorbed species, in situ diffuse reflectance infrared Fourier transform spectroscopy (DRIFTS) was performed during CO oxidation. Figure displays temperature-dependent operando DRIFTS measurements of the highly active Au38(SR)24/CeO2 catalyst pretreated at 250 °C. Spectra were taken from room temperature to 150 °C (ramp 1 °C/min, then isothermal for 4 h).
Figure 3

Operando DRIFTS during CO oxidation on Au38/CeO2 pretreated at 250 °C, from room temperature to 150 °C (background corrected with pure CeO2 pretreated under the same conditions). (a) 2500–2000 cm–1, (b) 1600–1200 cm–1.

Operando DRIFTS during CO oxidation on Au38/CeO2 pretreated at 250 °C, from room temperature to 150 °C (background corrected with pure CeO2 pretreated under the same conditions). (a) 2500–2000 cm–1, (b) 1600–1200 cm–1. CO adsorbed on Au0 (2130 cm–1) was observed below 118 °C, corroborating clean Au surfaces (Figure S8). CO2 formation was already observed at room temperature by MS (Figure S12) and gas-phase bands between 2300 and 2400 cm–1 (Figures a and S9). In the lower wavenumber region (Figure b), the typical monodentate carbonates, frequently observed during CO oxidation and bonded to ceria, were observed via an increasing signal at 1468 cm–1. For sulfation of CeO2, Waqif et al. reported distinct IR bands of surface SO3 (or S2O7–2) and SO4 (1x S = O, 3x S–O–Ce),[46] which were also present here (Figures S10 and S11). Bulk SO4 was absent (missing bands at 1196, 1128 cm–1 in Figure S11).[46,47] Surface SO3 and SO4 increased over time, becoming more pronounced close to maximum temperature in Figure b. Thus, sulfur from Au–S species, which have migrated to the support during pretreatment, reacted to surface SO3 and SO4. The detailed evolution of the structure of Au38(SR)24 nanoclusters supported on CeO2 was monitored upon pretreatment and CO oxidation. Whereas unpretreated samples tend to sinter, oxidative pretreatment at 150 °C collapsed the staples structure. Unlike the hydrocarbon backbone, sulfur was not removed to the gas phase but remained on the Au core, thus inhibiting adsorption of CO and oxygen. Pretreatment at 250 °C fully removed S and created clean Au0 clusters with intact core structure. The removal of ligands was beneficial for CO oxidation, which is why the pret250 sample had the highest activity, being already active at room temperature. During reaction, mobile Au and S species formed additional (inactive) Au–S entities. Operando DRIFTS detected CO adsorption on Au0 below 118 °C, in addition to carbonates on the ceria support. A slow continuous transformation to SO3 and SO4 was observed (during ∼6 h), becoming more pronounced close to the maximum temperature. The current results are particularly relevant for further studies of cluster chemistry and functionality. It is important to understand the role and fate of staples/ligands and their interaction with the support, as this strongly affects catalytic performance.
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