1 Introduction

Catalysts are often composed of metal and oxide components in the nano-size regimes. Design and fabrication of catalysts has always been the focus of the catalysis field. Less attention has been given to the dynamics that catalysts undergo while in catalytic reaction conditions. Temperature along with the corrosive and reactive gas pressures (and liquid environments) usually tend to alter catalysts. Morphology, redox states, and composition are all fluidic. Although catalysts are purposely tuned and created for specific reactions, in some sense, they will evolve to states that are often different from those of the original catalyst as the reaction progresses. Even though catalyst, by definition, refers to a structurally and chemically unchanged unit, catalytic processes change catalysts. Even the slightest modifications to the original structure and chemistry can alter a catalyst, varying its activity and selectivity away from the type and specifics of the reaction that it was built for.

This should not be a surprise given the strong dependence of the catalytic behavior on the electronic, chemical, and crystallographic states of the metal and/or oxide catalyst materials. The electronic, chemical, and crystallographic structures are closely related and show deviations from expected solid behavior in the nano-size regime [13]. In this regime, size dependence on catalytic activity and selectivity should be expected within a critical range between molecular and bulk limits. Size determines the electronic density of states by altering the band structure of the solid and the crystallographic shape of the catalytic surface by delimiting the outer boundaries of the catalyst material (Fig. 1a). It should also be noted that electronic and crystallographic structures can be tuned independently of size. For example, adsorbate molecules, such as reactants, intermediates or products, can alter both surface electronic states by charge transfer or crystallographic orientation and coordination upon binding. Furthermore, size indirectly establishes the kinetically most stable oxidation state of catalyst. Under net oxidizing and reducing gas atmospheres (or liquid environments) as most, if not all, catalytic reactions have, metals will be oxidized at least on the surface, or equally, metal oxides will be reduced to kinetically meta-stable phases. Particulate or grain size of the catalyst material is one of the sole factors that govern such redox processes.

Fig. 1
figure 1

a Coordination numbers given for 13-atom and 55-atom clusters close-packed with face-center-cubic (FCC) symmetry; and b distribution of various coordination sites and total coordination numbers as a function of particle size in the 1.5–15 nm range. Fraction of coordination sites were calculated by using the algorithms reported by van Hardeveld and Hartog [1]

Catalyst architecture as it applies to bi-functional or charge transfer catalysis is another factor that determines reactivity and reaction kinetics. Metal oxides often function as supports for metal catalysts or act as a co-catalyst along with the metal for the reaction. Metal oxides employed in catalytic transformations vary from inert supports like mesoporous silica (e.g. SBA-15 and MCF-17) to acidic zeolites and basic oxides of 3d-transition metals (e.g. MnO2, Fe2O3 and Co3O4), alkali metals (MgO) or lanthanides (CeO2). Then, the choice of oxide is to facilitate the direction of charge transfer and/or to introduce additional reaction sites such as to promote the bi-functional character of any particular reaction.

Likewise, the introduction of a second (or even a third) metal either alloyed with the primary metal or as separate reaction centers invoke charge transfer chemistry and bi-functional catalysis. Possible architectures for systems with more than one metal are, in the order of decreasing short range order between the components, intermetallic (i.e. ordered alloy), homogeneous random alloy, gradient alloy, core/shell and dimer hetero-aggregates (Fig. 2). The complexity exponentially increases with the number of metals and relative elemental ratios. In principle, there is an infinite number of particle architectures in compositional space which are governed by the microscopic arrangement of different metal atoms in the bulk and on the surface (as an example, see Fig. 2). As a result of such a large micro-structural space, bulk coordination and surface ensembles vary dramatically with particle architecture, as does the catalytic behavior. In general, charge transfer effects, driven by a net electronegativity difference between the metal components as predicted by Norskov’s ‘surface reactivity theory’ [4, 5], and surface ensemble effects, based upon the short-range order, are more pronounced for intermetallic catalysts. Electronic and geometric effects, induced by strain and orbital overlap as predicted by ‘near surface alloy theory’ [6, 7], are put forward fundamentally for core/shell catalysts.

Fig. 2
figure 2

Representative nano-catalyst architectures, composed of more than one component, discussed in this study: metal/oxide hybrid composites and bimetallic particles. Some alloy surface ensembles are also depicted in relation to the bimetallic architectures

Given this complex network of structure-size (or architecture) relations, it should be noted that precise and accurate knowledge of the initial states of a catalyst is necessary to develop any chemical insight into catalysts’ function during catalytic reactions in general. After all, metal and oxide nanoparticles are prepared under synthetic conditions that are different from the reaction conditions, and are kinetically trapped in the pre-catalysis forms. However, the dual effect of time and temperature acts to transform working catalysts into forms that are more stable under reactive/corrosive gas atmospheres (or liquid environments). Particle sintering and crystal phase transformations are typical results of prolonged time-on-stream operations of catalyst materials which present further complications in drawing any unambiguous conclusions concerning how catalyst materials function.

From a catalysis point of view, the control of size and phase presents an intriguing and rewarding way of tuning the desired activity and selectivity expected of any particular catalyst. Furthermore, nano-catalysts with well-defined electronic, chemical and crystallographic properties are essential to multi-path and multi-product catalytic reactions, where high activity and 100 % selectivity are targeted for particular end-products. The design and synthesis of such model catalysts, for which particle size and catalyst architecture can be fine-tuned, are essential for developing a unique understanding of active states and fundamental reaction pathways of catalytic processes that could lead to a better understanding of catalysis in general. In this respect, colloidal chemistry and other bottom-up techniques (e.g. sol–gel and solvo-thermal synthesis; e-beam and thermal evaporation; vapor deposition) offer synthetic tools and strategies to achieve the fabrication of size- and architecture-controlled nano-catalysts.

It should be noted that capping ligands are employed in colloidal synthesis to stabilize NP size and/or morphology, and they may have impact on catalyst properties, namely catalytic activity and selectivity. The documented behaviors vary from inhibitory effects, such as a surface poisoning observed for size-controlled Co NPs co-stabilized with phosphine oxide ligands during CO2/H2 reaction; [8] and promotional effects, such as a ligand-induced creation of active surface ensembles in the case of thiol-stabilized monometallic Pt and bimetallic Au–Pt NPs for hydrodesulfurization reactions [9]. Partial activity losses were also reported for Suzuki coupling [10], ethylene hydrogenation [1113], and the hydrogenative isomerization of methylcyclopentane [14] when using polymer (e.g. PVP) caps, and CO oxidation when using amine functional ligands, which were attributed to partial surface blocking effects. However, no electronic or geometric effect of surface ligands on nano-catalysts has been reported to date.

The importance of utilizing nanoparticles with monodisperse particle sizes and architectures and oxide supports/co-catalysts with controlled pore structures, surface areas, and surface functionalities as model catalysts has been discussed in the first part of this review. The subsequent sections, however, are focused on the material dynamics of such well-behaved nano-catalysts through the use of in situ tools and techniques.

The dynamic aspect of catalysis underlies the importance and necessity of in situ and in operando studies. It should be noted that the term in situ is used whenever the probe technique is employed under the reaction conditions without in-line catalytic measurements; in operando refers to simultaneous measurements of catalytic and materials properties. For in situ studies, the catalytic information comes from catalyst testing which is usually conducted in parallel scaled-up reactors under similar temperature and pressure conditions as the probe experiment. The objective of this review is to give accounts of in situ (and some in operando) experiments on model nano-catalyst systems that led to a better understanding of catalytic behaviors and trends in particular reaction processes.

This paper is organized in two sections. In the first section, in situ surface tools will be reviewed. They are classified in three categories: electronic spectroscopy, vibrational spectroscopy and electron microscopy. In the electronic spectroscopy category, X-ray absorption and photoelectron spectroscopies will be introduced as chemically sensitive surface probes. Then, sum frequency generation (SFG) vibrational spectroscopy and surface enhanced Raman techniques will be discussed in the vibrational spectroscopy category as tools that have sub-monolayer sensitivity towards immediate catalyst surfaces. Finally, transmission electron microscopy (TEM) techniques such as bright field and dark field imaging and electron diffraction will be described in relation to studies in catalysis. Along these lines, scanning transmission electron microscopy (STEM) and spectroscopic tools that use the scanning electron beam as a local probe will also be discussed. In general, the technical definitions of each tool will be given, followed by the basic components and key elements of in situ setups. Most of these tools are employed in the Somorjai group routinely to investigate the surface reactivity of model heterogeneous catalysts with bimetallic nanoparticle and metal/oxide nano-composite architectures.

In the second section of this paper, some case examples will be discussed in which the described in situ surface tools, individually or in combination, have been employed in conjunction with catalytic measurements to address structure–reactivity correlations. These case examples are grouped under four catalytic reaction categories: CO oxidation, CO2 hydrogenation, hydrogenative reforming of hydrocarbons, and heterogenized homogeneous transformations in organic liquids.

2 Probing Tools of Catalysis

Because catalysis is a surface phenomenon, the probing tools and techniques that are employed to provide structural information should exhibit a certain level of sensitivity towards surfaces or near surface regions. Furthermore, chemical sensitivity towards high-Z elements constituting catalyst and surface-adsorbed molecules should be achieved. Orientations and binding configurations of adsorbate molecules should also be addressed in order to obtain a full molecular picture of the catalyst. Additionally, structure–reactivity correlations are based on the assumption that catalysts are uniformly behaved within the probe size when bulk ensemble averages of the catalytic system are monitored; it is a matter of the spatial resolution or the probe size which will lead to identical information at the microscopic level. Hence, spectro-microscopy has a special place in our efforts to reconcile structure and catalytic behaviors with trends, and correlative spectroscopy and microscopy studies should be included within this framework. Finally, probe-matter interactions should be accounted for and ruled out properly. The probe is often a collimated light (i.e. synchrotron X-rays, lasers in IR/Vis/UV wavelengths) or electron source; or a molecule, which exhibits a unique spectral (i.e. vibrational) signature upon adsorption. Thus, the probe can, in principle, perturb catalyst surfaces in such a way as to alter the kinetics and steady-state behaviors of ongoing catalytic reactions.

2.1 Electronic, Chemical and Crystallographic Structures of Catalyst Materials via X-ray Spectroscopic Techniques

Synchrotron X-rays serve as excellent probes of electronic structure and coordination on the surface and in the near surface regions. Specifically, core level excitations from impinging soft X-rays, in the energy range of 100–1,100 eV, give rise to dipole-induced transitions at the ionization threshold which generate photoelectrons, secondary (Auger) electrons and inelastically-scattered photons (Fig. 3). Photoelectrons and Auger electrons are element specific and detection of these electrons is very surface sensitive owing to their short mean free paths in solids. Although typical penetration depths of soft X-rays at the shallow absorption edges of the elements are several hundreds of nanometers, electrons from only the top few nanometers of the surface can escape any solid. This is usually the case for L-edge absorption of 1st row (3d) transition metals such as Mn, Fe and Co; M-edge absorption of 2nd row (4d) transition metals; and N-edge absorption of 3rd row (5d) transition metals. For instance, X-rays with photon energies of the Co L3 step edge have attenuation lengths of 800 nm, defined as the length for a drop of intensity by 1/e, while electron yields are entirely registered from the topmost 2.5 nm of surfaces [15]. Furthermore, simultaneous measurement of X-ray emission provides the complimentary bulk detection.

Fig. 3
figure 3

Schematics showing the electronic principles of X-ray photoelectron spectroscopy (XPS) and X-ray absorption spectroscopy (XAS). Two modes of detection for XAS are also depicted

In addition to surface detection, the X-ray absorption process is dipole induced, so that surface selection rules apply to the transitions. As a result, the orientation and binding configurations of surface adsorbed molecules can be obtained for single crystal surfaces, and in principle preferentially oriented nano-crystalline catalysts, by tilting the sample with respect to the incoming X-ray beam. Tilt series of X-ray absorption spectra obtained in this way can reveal the relative strength of various orbital transitions with respect to the surface dipole; molecular orientation can then be deduced from this angular variation in absorption intensities. The tilt studies can be achieved using soft X-rays to measure the K edge absorption of low-Z elements such as C, N and O [1618]. Furthermore, electron yield can be detected in gas atmospheres or condensed phases (as opposed to X-ray photoelectron spectroscopy) by simply measuring the amplified compensating electron flow from earth to sample.

2.1.1 X-ray Absorption Spectroscopy

X-ray absorption gives rise to two complementary processes, which are identified as near edge X-ray absorption fine structure (NEXAFS) and extended edge X-ray absorption fine structure (EXAFS). The former technique, as the name implies, refers to the dipole-induced electronic transitions near absorption edges, which is usually 5–50 eV above the core level being excited. It is also known as X-ray absorption near edge structure (XANES), which is synonymous with NEXAFS. Generally, the shallower the core level being excited, the higher the energy resolution is because of longer core–hole lifetimes (i.e. Heisenberg uncertainty principle). Furthermore, upon X-ray absorption shallow core levels emit electrons that are highly surface sensitive. Hence, soft X-ray absorption spectroscopy is usually the preferred mode of application in catalysis for this technique. Two-dimensional nanoparticle films and adsorbate molecules at sub-monolayer coverages can be detected by using soft NEXAFS spectroscopy.

EXAFS concerns the extended energy range beyond what is defined for the near edge region. It is discerned by oscillations in the extended spectrum that arise from near neighbor interactions X-rays incident on absorber atoms give rise to wave fronts that are scattered from neighboring atoms which, in turn, give rise to interference patterns which modulate the absorption. Amplitude (in real space) and phase (in reciprocal space) of such oscillations of the absorption can be analyzed by using physically well-defined structural models to obtain the involved crystallographic variables such as coordination number, atomic distances, and thermal displacements. Because Fourier transformation, which is mathematically applied to EXAFS data to obtain the phase and amplitude, requires a summation over a large set of k-points, the EXAFS technique can only be used for X-ray absorption studies involving deeper core levels: K edge absorption for 1st and 2nd group transition metals and L3 edge absorption of 3rd group transition metals. This restricts the use of the EXAFS technique to bulk phenomena regardless of the detection mode used. Photoelectrons from shallow core levels possess high kinetic energies sufficient to travel from much deeper than near surface regions, and contribute to the background on one hand. Auger electron emission from deep core levels, on the other hand, contribute selectively to the near edge region pass the edge jump. Although the probability of Auger transitions involving shallow core levels is relatively high, more energetic secondary electrons from deeper core levels have larger escape depths rendering their contribution to the total electron yield significant. Therefore, total electron yield is not strictly confined to the near surface regions, but carries information from the bulk as well.

Nonetheless, for clusters and small nanoparticles, where bulk practically becomes surface (i.e. large surface-to-volume ratios), the EXAFS technique can be recognized as surface sensitive and thus is relevant to catalysis studies [19, 20] (see Fig. 1b). It should be noted that coordination number for close-packed metals varies steeply with particle size in the size range of interest for catalysis. For instance, coordination number jumps from an average of 7 for a 1 nm cluster, composed of 50 atoms about 80 % of which are on the surface, to an average of 11 for a 3 nm nanoparticle, where about 250 out of 800 atoms are registered on the surface, as illustrated in Fig. 1. The picture gets even more complex when more than one atom type is involved, given the large permutational space (see Fig. 2). Then, structural models can only be employed for model nano-catalysts with monodisperse particle size and architecture distributions.

All these aspects make soft X-ray absorption spectroscopy (XAS) a unique technique to study catalyst surfaces. In order to obtain an X-ray absorption spectrum, relative absorption intensities across the absorption edge of elements should be recorded. This is only possible when monochromated X-rays with tunable energies are employed; and thus, in practice, requires synchrotron radiation facilities. Soft XAS is an ultra-high vacuum (UHV) technique because of the strong interaction of X-rays with matter. The attenuation lengths of X-rays in gas atmospheres are on the order of several millimeters and much shorter in condensed matter. To prevent large signal drops while maintaining ambient gas pressures above the sample, a common strategy is to separate reaction environment from the upstream synchrotron by using windows transparent to X-rays above 100 eV. Aluminum and silicon nitride membranes are typically employed as soft X-ray windows; 100 nm thick membranes are usually mechanically strong enough to hold differential pressures while transmitting X-rays in a broad energy range with high % transmittance. In this context, reaction cells operating in static [21] or flow modes [2226] for liquids and various reactive gases can be purposely built and utilized in UHV chambers for soft XAS, as shown in Fig. 4.

Fig. 4
figure 4

a Schematics illustrating an in situ XAS cell; and b a purposely-built gas flow cell in use in the Somorjai group and c picture showing the in situ gas flow cell during operation in beamline 8.0.1 at the advance light source

2.1.2 X-ray Photoelectron Spectroscopy

Differently than XAS, XPS can use a constant, monochromated or not, photon source to excite the related core levels. Then, ejected photoelectrons are analyzed to generate photoelectron spectra. This aspect of XPS allows it to be employed as a benchtop laboratory tool. However, synchrotron radiation offers high X-ray fluxes with tunable photon energies. Combined with the fact that inelastic mean free paths of photoelectrons strongly depend on the photon energy, one can vary photon energy to map surface and near surface regions at different depths, a technique known as depth-profiling.

X-ray photoelectron spectroscopy (XPS), like soft XAS, is an UHV technique, because of the short mean free paths of photoelectrons. As opposed to XAS, photoelectrons should travel through UHV to the analyzer where they are sorted out as a function of kinetic energy that they carry. In addition, short mean free paths of photoelectrons in solids, typically ranging from several Angstroms to a few nanometers, also hinder the use of any practical window. One exception to this is the use of single- or multi-layer graphene, which is yet awaiting a successful implementation in XPS measurements.

In ambient pressure (AP) XPS, a technique that successfully overcame the inherent restrictions of traditional XPS, photoelectrons are captured before they are lost to collisions with the surrounding ambient medium by using a small aperture cone located in the proximity of the sample [2729]. Gas molecules are then differentially pumped through the aperture while photoelectrons are focused using electron lenses on to the analyzer, which is eventually pumped down to UHV [27]. By this way, ambient gas pressures in the Torr regimes are made possible in XPS measurements. Recently, another milestone in the technique came when tender X-rays in the 2,000–5,000 eV range were used to create photoelectrons from a thin solid/liquid interface, which opened up roads to unprecedented experiments for in situ and in operando studies [30].

It should also be noted that working gas pressures inside APXPS cells, although in the low Torr ranges, are of relevance to catalysis with measurable turnovers. APXPS with energy tunable synchrotron X-rays renders probing the immediate catalyst surfaces as well as the interfaces between metal and oxide support of model catalysts. Moreover, the chemical foundations in the nanoscale of surface phenomena such as wetting, encapsulation and coverage can be understood by using APXPS; and thus structure–function correlations can be derived for model nano-catalysts with fine chemical details never before observed as the catalytic reaction occurs.

2.2 Surface Orientation and Molecular Bonding via Vibrational Spectroscopy

The other extreme of the optical spectrum, specifically the far IR region, is often employed for vibrational and Raman spectroscopy. Although the excitation wavelengths range from mid UV to far IR the spectral region of interest falls in the 100–4,000 cm−1 window, where IR vibrations and Raman scattering occur. The topmost surface where catalytic reaction events take place can be distinguished by adsorbate molecules, bound to metal and/or oxide catalysts, in their activated states. Spectral isolation and identification of such states leads to the understanding of catalytic reaction pathways and even mechanisms when employed in conjunction with catalytic measurements conducted in parallel with spectroscopy. However, surface specific detection is an absolute must, given the relatively short absorption lengths of IR in the gas phase. Therefore, traditional IR and Raman techniques should be treated with caution when employed in catalytic systems. IR techniques like polarization-modulation IR reflection absorption spectroscopy (PM-IRAS) and non-linear optical techniques like SFG can be singled out as surface sensitive vibrational tools [31].

PM-IRAS is based on modulating polarization of IR light at high repetition rates compared to vibrational stretch frequencies, and has been used on model catalyst systems such as thin metal/oxide films, two-dimensional films of nanoparticles (e.g. thermally evaporated, e-beam deposited, etc.) and their combinations [32, 33]. The coupling of constructively and destructively polarized light with in phase (p-polarized) and out of phase (s-polarized) components of surface adsorbed molecules give rise to an orientation dependence governed by surface selection rules. This is achieved by illuminating the surface at grazing angles, where the intensity of outgoing p-polarized light (lp) is at a maximum, whereas the intensity of outgoing s-polarized light (ls) is not dependent on the incident angle. Hence, a surface enhancement is obtained for species with vibrational components parallel to surface normal when the IR spectrum is recorded as a plot of (lp-ls)/(ls + lp) [34].

In SFG vibrational spectroscopy, collimated and pulsed light beams (i.e. lasers) at visible and tunable mid IR wavelengths are temporally and spatially overlapped on model nano-catalysts. The light generated at summed frequencies is collected in total internal reflection geometry. The measured SFG signal is given by the electric field strengths of incident electromagnetic waves and the non-linear susceptibility. The non-linear susceptibility has both a resonant and non-resonant component. The resonant component of the non-linear susceptibility is fundamentally a sum of all bond dipoles, but for centrosymmetric environments, where a time-average of the ensemble of dipoles is in principle zero (as in bulk gas or liquid), the SFG signal cancels out. Therefore, the SFG signal is only non-zero for non-centrosymmetric media such as interfaces and surfaces, where inversion symmetry is broken. The non-resonant component of the non-linear susceptibility is, however, not well modeled, and requires control methodologies in experimentation, especially for SFG studies that involve metals, where non-resonant effects have been found to be significant.

It was found for SFG experiments that a total internal reflection geometry using a prism is best suited for maximum SFG signal output [35]. Towards this goal, entrance angles of laser beams should be carefully aligned using the prism while maintaining the temporal and spatial overlap. Short attenuation lengths of the evanescent waves, on the order of tens of nanometers, limit the probed area to near surface regions of the sample, either in contact with the prism [36] (Fig. 5) or across an ultrathin layer of aqueous electrolyte [37] that separates the sample and prism. For the reasons described above, the sample volumes employed in SFG studies are usually very small, which renders model systems like metal nanoparticles dispersed over thin films of oxides ideal.

Fig. 5
figure 5

a Sum frequency generation process, b schematic of an in situ SFG reaction cell; and c picture showing the in situ SFG gas flow cell in use in the Somorjai group

In a typical SFG setup for catalysis studies, a 1,064 nm Nd:YAG laser generating pulses in mJoules and with picosecond bandwidths is used as a seed source to pump frequency-doubled pulses in the visible spectrum (532 nm) and broadly tunable IR pulses in the 2,500–4,000 cm−1 spectral range. The oscillating visible and tunable IR pulses are synchronized and spatially overlapped at a prism with the nano-catalysts located on it or in its vicinity. A resonant SFG wave is generated wherever and whenever an evanescent wave at a given IR frequency resonates vibrationally with the adsorbate molecules.The SFG spectrum is then obtained by scanning IR frequencies in the desired spectral window. It should be noted that the resonant vibrational modes associated with the SFG signal should have both IR- and Raman-active symmetries.

It is worth mentioning that molecules chemisorbed on metal (or metal oxide) surfaces usually display net non-zero dipole moments and polarizability. This property of heterogeneous systems (i.e. solid–liquid and solid–gas) renders SFG an attractive technique for in situ/in operando studies, as highlighted in a number of studies spanning single crystals [38, 39] as well as two dimensional films of nano-catalysts [4043].

Raman inelastic scattering is a vibrational technique as well as a tool for optical phonon mode and crystal phase determinations. When used in catalysis it provides bonding information for reactant molecules, adsorbed species on catalyst surfaces, and catalysts, in particular metal oxides [44]. In the micro-Raman technique, the sample is excited with a laser source, typically a continuous wave in the visible spectrum, through the objective lens of an optical microscope. Inelastically scattered light is then collected by the same objective lens and Raman shifts are measured by using a charged coupled device after filtering out the laser line. By this method, spatial resolutions in the diffraction limit of the light can be achieved as well as high signal intensities. However, the Raman technique, inherent to its optical nature, is not surface specific.

A major breakthrough that enables the application of the Raman technique in heterogeneous catalysis, and surface studies in general, came with the resonant surface enhancement effect for coinage metals such as Au [45], Ag [46, 47] and Cu [48]; and noble metals such as Pd [49] and Rh [50, 51]. The coinage metals exhibit surface plasmons, collectively oscillating electrons localized on surfaces, when excited with the visible region of the electromagnetic spectrum. When excited with the visible light, surface plasmons become resonantly oscillating. The so-called ‘hot electrons’ due to such resonant absorption processes then enhance electromagnetic fields near the surface and decay away from the surface. As a result of this resonance enhancement, at such ‘hot spots’, the Raman process is amplified orders of magnitude compared to the non-resonant operations [52, 53]. Furthermore, enhancement factors were found to be greater when the metals are in the nanoscale and along sharp edges and corners when metal nanoparticles have unisotropic morphologies [54]. It was also found that thin dielectric coatings around these surface Plasmon resonance (SPR) active metal nanoparticles cause red shifts in the absorption spectrum and thus further facilitate the enhancement effects. This phenomenon presents tremendous opportunities for heterogeneous catalysis because the Raman scattering from the vicinity of SPR-active metals becomes statistically significant. As a result, when the active catalyst surface is located in the atomic proximity of the SPR-active metals the Raman signal can be amplified to a level that renders high sensitivity detection possible. This is the fundamental principle behind tip-enhanced Raman spectroscopy, in which Raman scattering was facilitated by an AFM tip made out of a SPR-active metal. By using the SPR enhancement phenomena, spatial resolutions on the order of tens of nanometers [55, 56] or single (adsorbate) molecule detection was reported as a proof of concept [57].

2.3 Size, Morphology and Chemical Structure Via Transmission Electron Microscopy Techniques

Transmission electron microscopy (TEM) is often employed for studying catalysts, specifically pre- and post-catalysis investigations of morphology, crystallography, and chemical states of catalysts [5863] [38]. In TEM, electrons are transmitted through the solid and produce contrast patterns based on varying degrees of transmittance through an objective lens of the primary beam (bright field imaging) or the diffracted beams (dark field imaging) across the sample. Image patterns are two dimensional projections of solid objects and can reveal morphology, atomic planes, and individual atoms in periodic arrays when the sample plane is oriented relative to the electron beam in such a way that electrons are diffracted at Braggs’ angles in the confined q-space of the high energy electron optics. Furthermore, electron diffraction patterns can be collected to obtain periodicity and even crystal phase.

2.3.1 Scanning Transmission Electron Microscopy

STEM, a spin-off technique, goes beyond the capabilities of conventional TEM and renders local structure analysis of solids possible. In STEM, the electron beam is focused to a small spot size, typically a nanometer in diameter, and is used as a local probe in the raster mode. Annular dark field (ADF) imaging is one of the techniques that can be employed in the scanning mode. ADF is achieved at short camera lengths, which requires small probe sizes. Because it is classified as a Rutherford type scattering, it is the elemental nuclei that electrons interact with, as opposed to soft electron orbitals in conventional DF imaging [64]. Therefore, ADF imaging is identified with high Z-contrast. Model catalysts are multi-element composites and are often composed of a crystalline metal sparsely dispersed on a matrix of porous and thick metal oxide. In conventional TEM, thickness and diffraction contrast contribute to image formation as Z-contrast in conventional DF, complicating analysis. However, ADF in the scanning mode decouples the effects of atomic number, thickness, and diffraction, and provides local Z-enhanced information. In this way, model catalysts can be studied with greater elemental and structural sensitivity.

It is also worth mentioning that after the transmission electron aberration-corrected microscopy (TEAM) project [65, 66] was realized, probe-corrected electron microscopes brought cluster-sized nanoparticles and even single metal site coordination complexes into the repertoire of TEM studies [67, 68]. Furthermore, aberration-corrected electron microscopes can operate at low accelerating voltages (i.e. 80 kV) and low electron dose exposures (i.e. several electrons per square Angstrom); and thus allow imaging that is free of knock-on atom displacements and ionization effects [69, 70].

It is also common practice to equip analytical tools such as energy dispersive spectroscopy (EDS) and electron energy loss spectroscopy (EELS) with the TEM operating in the scanning mode. EDS probes elemental composition for almost the entire periodic table with the exception of low Z elements, while EELS explores chemical fine structure as well as elemental composition for elements with Z < 30 [71]. Therefore, both techniques complement each other. In some aspects, EELS is reminiscent of NEXAFS, probing the electronic structure of solids such as Co, Fe and Mn; while electron energy loss fine structure (EELFS) spectroscopy [72], a technique derived from EELS, replicates the EXAFS model to obtain near neighbor bonding for elements such as O, Al and Si [71, 72]. Fundamentally, all the sought after elements of as-synthesized (or spent) catalysts such as size, morphological and geometrical shapes, phase, composition, oxidation state, and bonding can be studied in TEM.

Strong electron-matter interactions limit the TEM technique traditionally to high vacuum conditions. Environmental TEM [73], in which gas atmospheres in the Torr pressures can be dosed into the sample area in a fashion similar to APXPS, can be considered as revolutionary in the catalysis field. Recently, new developments and advances in micro-machining and membrane technologies allowed another breakthrough toward mimicking realistic catalytic environments in the TEM column. By using static and flow gas/liquid cell holders, catalysts can be studied in their working environments, either as individual nano-catalysts or composite catalyst ensembles. Then, a statistical data pool for microscopic catalytic reaction pathways can be identified as compared to the ensemble averaged macroscopic reaction pathway.

3 Case Examples of In Situ Studies of Model NP Catalysts

In situ surface techniques along with catalytic measurements play key roles in identifying the structure–reactivity properties as well as deciphering the complex catalytic behaviors and trends. When employed in studying model catalysts, of bimetallic or metal/oxide hybrid natures, in situ tools are the experimentalists’ five senses to the chemical and catalytic events as they occur. In this section, some case studies of model nano-catalysts that illustrate a correlative approach of in situ probing and catalytic measurements will be discussed. These case examples are grouped into four categories that are distinguished by the type of catalytic reaction: CO oxidation, CO2 hydrogenation, hydrogenative reforming of hydrocarbons, and heterogenized homogenous transformations in organic solvents.

3.1 Catalytic CO Oxidation over Pt/Mesoporous Metal Oxide Nano-Composite Catalysts and Pt-Based Bimetallic Nano-Catalysts

Catalytic oxidation of CO is a model reaction to evaluate catalyst activity. Pt is a model metal catalyst and shows a weak dependence of crystal shape or size in the nanoscale on catalytic turnovers to CO2, when used alone [74] or along with inert supports such as SiO2 [75, 76] and Al2O3 [77]. Likewise, oxides of 1st row transition metals such as MnO2 [78, 79], Co3O4 [79, 80], and lanthanides like CeO2 [79, 81] catalyze the CO/O2 reaction. For Pt, the reaction proceeds with CO and oxygen, atomic or molecular, chemisorbed on adjacent sites. There are more than one possible catalytic pathways proposed for the reaction over basic oxides: chemisorbed CO reacts with lattice O of the oxide metal, then O2 fills in the generated defect site; or alternatively, CO chemisorbed on an unsaturated metal center and oxygen chemisorbed on a defect site react to produce CO2. Turnovers normalized to metal centers on surfaces and apparent activation energies are quite similar for both metal and oxide type catalysts, indicating identical catalytic behavior among various catalysts for the CO/O2 reaction [82].

When combined, Pt and metal oxide composites give rise to orders of magnitude enhancements in catalytic turnovers and lowering of activation energies [8385]. This invokes either: bi-functional catalysis [86], where different reactants are activated at different catalyst sites and the reaction occurs at the interface between adjacent chemisorption sites; acid–base catalysis, which involves one-way charge transfer from metal to oxide; or some combination of both. As hard as it sounds to devise experiments to isolate the real reaction mechanism, recent in situ studies uncovered a number of previously unknown details to this synergistic chemistry. Colloidally synthesized monodisperse Pt nanoparticles supported in various metal oxides such as Co3O4, MnO2, and CeO2 with controlled physical and structural properties were chosen for this particular study [85]. The composite catalysts were then screened for catalytic oxidation of CO in both O-rich and CO-rich reaction atmospheres in the 200–250 °C range. As it will be shown, the Pt/oxide interface gave rise to more than an order of magnitude enhancement in turnovers as compared to pure Pt (supported in SiO2) and pure oxides. The enhancement factor was calculated to be about 1,000 times greater for the Pt/Co3O4 catalyst compared to the Pt/SiO2 catalyst.

In these studies, the Pt/oxide interface is broadly defined and refers to the catalytic synergy achieved as a result of the physical contact made between the metal and oxide. Catalytic turnovers at the Pt/oxide interface were calculated by first subtracting from the overall catalytic conversion the contributions of pure Pt and pure oxide catalysts and next normalizing with respect to the available Pt surface. Therefore, this method gives a lower bound for interfacial turnovers.

3.1.1 An Active CoO Phase in Contact with Pt NPs Enhances the CO Oxidation Rates

Soft X-ray absorption spectroscopy was carried out in a purposely-built gas flow cell [87] by using pelletized nano-catalysts and identical conditions as the catalytic measurements. It was found that oxide metals were significantly reduced under CO-rich (i.e. net reducing) reaction atmospheres at 250 °C (Fig. 6a, b). In the case of Pt/Co3O4 under CO-rich atmospheres and at 250 °C, the average oxidation state of cobalt determined by a least-square fitting procedure revealed CoO as by far the majority phase (a fraction of 0.9), while only a small fraction of Co3O4 was detected (Fig. 6c, d). On the contrary, only a small fraction of CoO was detected under identical reaction atmosphere at 200 °C and also under O-rich (i.e. net oxidizing) reaction atmospheres in the 200–250 °C range. Catalytic turnovers registered for the metal/oxide interface were also identical at 200 °C for both the O- and CO-rich reaction atmospheres. However, at 250 °C, where the reduction and phase transformation of cobalt oxide was most pronounced, a two-fold enhancement was obtained under the CO-rich case relative to the O-rich case (Fig. 6e, f). This clearly indicated that the active phase of cobalt oxide was CoO, not Co3O4, in sharp contrast to the common knowledge in the field prior to this work [88].

Fig. 6
figure 6

In situ Co L3 edge NEXAFS spectra measured for the Pt/Co3O4 nano-catalyst at 250 °C and in flowing a O-rich (CO:O2, 2:5); and b CO-rich (CO:O2, 5:2) reaction atmospheres. Oxidation states obtained by least square fitting of the NEXAFS spectra in c O-rich; and d CO-rich reaction atmospheres. Catalytic turnovers measured in a plug-flow reactor under e O-rich; and f CO-rich conditions [adapted with permission from An et al. [85]. Copyright: (2013) American Chemical Society]

In a prior work, colloidally synthesized bimetallic CoPt nanoparticles, having monodisperse 4 nm sizes and random alloy architectures, were deposited on silicon substrates and studied using in situ soft XAS and catalytic measurements under O-rich (1.4:1 by volume) CO/O2 reaction atmospheres (0.043–32 Torr range) and at 125 °C [87]. It was shown that as-synthesized bimetallic alloy nanoparticles, where Co and Pt atoms are randomly distributed, underwent surface segregation depending on the redox sign of the environment, either catalytically net oxidizing CO/O2 atmospheres or reducing H2 atmospheres. Co was oxidized to CoO and diffused to the surface during the CO/O2 reaction, whereas Pt segregated to the surface forming Pt-rich layers in net reducing atmospheres. Turnovers were measured and calculated under total CO/O2 (1.4:1) pressures in the 0.043 -32 Torr range and at 125 °C by using a batch reactor and the data correlated to fractions of Co2+, as in CoO, obtained under identical conditions. It was shown that a hysteresis existed for both catalytic turnovers and Co2+ fractions when the reactive gas pressures stepwise increased to 32 Torr first and then stepwise decreased back to 0.043 Torr. Therefore, it was concluded that turnovers strongly correlated with the oxidation state of Co beyond the effect of varying chemical potentials over reaction rates. Moreover, when NPs were reduced in H2 prior to dosing the CO/O2 reaction mixture, the reduction of Co2+ was kinetically induced. This depleted surfaces of catalytically active CoO, causing turnovers to drop significantly and become identical to those of the initial bimetallic alloy NPs (Fig. 7).

Fig. 7
figure 7

a ETEM BF time series recorded for a single 10 nm CoPt alloy NP in 0.1 Torr O2 and at 250 °C, indicating surface segregation of Co. b Co L3,2 electron energy loss spectra measured for a single alloy NP before and after (O2) oxidation. c Co L3,2 electron energy loss map recorded for a single NP after ex situ (air) oxidation at 400 °C, showing CoO shell [modified with permission from Xin et al. [99]. Copyright: (2014) American Chemical Society]

The overlapping results of these two works is that CoO in physical contact with Pt, regardless of how the interface formed (i.e. independent of particle architecture), has promotional effects in the CO/O2 reaction. One question, however, remained as to whether or not Co2+ centers (or reduced oxide metal sites in general) activate oxygen alone, as bi-functionality would mandate.

3.1.2 O vacancy Sites are not Actively Involved in the Oxidation of CO at the Pt/CeO2 Interface

The case of CeO2 is also worth mentioning although it shared the same general tendencies as described above. CeO2 is known to have surface defects in the form of O vacancies [89]. By using a number of synchrotron-based X-ray spectroscopic and diffraction tools in situ, it was shown that Pt decreased substantially the energy barrier for the reduction of CeO2 under H2 atmospheres in the 0.1–150 Torr range and at temperatures between 50 and 350 °C [90]. It was found that H atom spillover from the Pt surface onto the CeO2 surface generated Ce3+ and O vacancies simultaneously. Thus, the surface concentration of Ce3+, generated by CO from either a direct binding to CeO2 or a spillover at the contact regions with Pt, could be taken as a measure of O vacancies (Fig. 8a). It was found that the Pt/CeO2 nano-catalyst was more reduced, producing Ce3+, under CO-rich atmospheres than O-rich atmospheres at 250 °C (Fig. 8b). However, the Pt/CeO2 interface performed better in O-rich reaction atmospheres than in CO-rich reaction atmospheres (Fig. 8c), which indicated the greater involvement of Ce4+ sites rather than Ce3+ sites [85]. It should be noted that this was in sharp contrast with the cases of Pt/Co3O4 and Pt/MnO2 catalysts. Therefore, the O vacancy sites, because they were found in more abundance when CeO2 was reduced, could not, in principle, facilitate enhanced CO oxidation rates. This overruled the involvement of lattice defects, specifically O vacancies, which are the subject matter of the popularly known Mars van Krevelen mechanism [38] for the catalytic oxidation of CO at the Pt/CeO2 interface.

Fig. 8
figure 8

a In situ Ce M5,4 edge NEXAFS spectra measured at 250 °C for the Pt/CeO2 nano-catalyst under O-rich and CO rich atmospheres. b Fractions of CeO2 obtained by the least square fitting of the NEXAFS spectra in a. c The results of catalytic measurements under O-rich and CO-rich atmospheres and at 250 °C [Adapted with permission from An et al. [85]. Copyright: (2013) American Chemical Society]

3.1.3 More Oxyphilic Metal Acts as the Oxygen Reservoir for the Oxidation of CO at the Interface Between Metallic Pt and Metallic Sn

In a recent work, bimetallic PtSn alloy NPs were compared to pure Pt NPs, with both NPs being monodisperse (2 nm) and supported on silicon substrates, by using correlative batch reactor measurements and APXPS [91]. PtSn NPs exhibited a fourfold drop in activation barrier toward the formation of CO2 for the CO-rich (5:2 by volume) reaction mixture in the 200–300 °C range as compared to pure Pt NPs under identical conditions. Reaction order in O2 was ~0 in the 40–100 Torr range and ~0.5 in the 40–100 mTorr range, the same pressure range as APXPS studies were conducted. The pure Pt NPs had a reaction order in O2 of approximately 1.

For the APXPS measurements, photoelectrons with 250 eV kinetic energies, giving inelastic mean free paths on the order of a few layers of the topmost surface, were chosen for both Pt 4f and Sn 3d core levels. Therefore, surface specific information of oxidation states and chemical composition was obtained at the atomic level. The results indicated that the as-synthesized nanoparticles as well as the spent nanoparticles after reduction in 100 mTorr H2 and at excesses of 350 °C were randomly mixed alloys, as evidenced by XPS components ascribed to Pt(Sn) and Sn(Pt) chemical environments. Under 140 mTorr CO/O2 (5:2) reaction atmosphere and in the 200–275 °C range, the alloyed composition changed at the expanse of segregated Pt and Sn domains. This was followed by a simultaneous oxidation of Sn0 to Sn2+, as in SnO, as shown in Fig. 9. A model was proposed in complete accord with the catalytic and XPS observations: the oxidation of CO occurred along CO covered Pt surface boundary in contact with SnO via the formation of Sn0 and a vacant Pt site. The vacant site on Pt was then filled by gas phase diffusion of a CO molecule or surface diffusion of a chemisorbed CO, while SnO acted as a reservoir to provide oxygen to the reduced Sn0 sites around the Pt domains.

Fig. 9
figure 9

Sn 3d (left column) and Pt 4f APXPS spectra measured for 2 nm PtSn alloy NPs in H2 reducing, CO reducing and two CO-rich reaction atmospheres, indicating reversible changes in the chemical compositions of the topmost surfaces determined by ~250 eV photoelectrons [adapted with permission from Michalak et al. [91]. Copyright: (2014) Journal of Catalysis]

3.2 CO2 Hydrogenation over Co/TiO2 Nano-Composite Catalyst and Bimetallic Co–Pt Nano-Catalysts

While O2 as an oxidant gauges the redox behavior of the Pt-based catalysts, H2, as a stronger reductant than CO, acts on the oxyphilic metal and high valency metal oxide catalysts to alter surface properties and eventually tailor catalytic behavior. Hydrogenative synthesis of olefins, paraffins and oxygenates in the gas and liquid spectrum, from CO, Fischer–Tropsch (F–T), and/or CO2 can be classified in this category.

Co-based catalysts are generally employed for the F–T synthesis. It has been much debated what the active catalyst is. According to one widely accepted model, CoC x forms upon dissociative adsorption of CO over metallic Co, and it is this particular CoCx phase that catalyzes hydrogenation and carbon chain growth by the insertion of methylene (–CH2) groups [92]. When CO2, a mildly oxidizing molecule, is used as a carbon source under a net H2 reducing atmosphere two strongly correlated reaction steps dominate the product distribution: the reverse water gas shift reaction (rWGS), which produces CO and H2O; and F–T synthesis that produces H2O, CH4 and surface methylene groups, which lead to gas and liquid hydrocarbons [93]. The F–T synthesis is a multi-path/multi-product reaction associated with multi-channel surface diffusion and complex re-adsorption pathways.

Model nano-catalysts under simulated reaction conditions are essential for understanding the catalyst properties and associated catalytic behavior. Size-controlled model Co NPs synthesized by using modified colloidal techniques indicated a weak size dependence (threefold enhancement for larger NPs normalized to surface area) in the 3–10 nm range [8]. It was also found that the reaction was inhibited by phosphorous, residues of one particular colloidal synthesis, present at sub-monolayer coverage, therefore a modified synthetic route, free of phosphorous reagent, was also developed. Furthermore, the gas pressures (4 atm H2:CO2 3:1) and reaction temperatures (200–300 °C) were chosen such as to avoid both complete methanation and chain growth polymerization. By this way, Co nano-catalysts were studied under low conversion and chain growth regimes.

3.2.1 Support Effects Over Co NPs Deposited Inside Macroporous TiO2

In a recent work, 10 nm monodisperse Co NPs were deposited on mesoporous SiO2 and macroporous TiO2, separately; and the pelletized nano-catalysts were studied under simulated CO2/H2 conditions by using catalytic measurements and an array of synchrotron based X-ray spectroscopy and diffraction tools [94]. The objective was to capture the more active physical form and chemical state of Co for a given particle size and then to evaluate the support effects, if present. To this end, Co NPs were deliberately oxidized or reduced prior to catalytic testing, and then all steps were monitored by using soft X-ray absorption spectroscopy. It was notable that fully metallic Co, cubic phase, formed upon reduction in 150 Torr H2 at 450 °C. When oxidized in 150 Torr O2 and at 350 °C, metallic Co was converted to CoO, cubic phase. The CoO remained oxidized under ~3 atm of H2:CO2 (3:1) at 250 °C. Catalytically, CoO was superior to metallic Co by almost 10:1 when supported in TiO2, which rendered the CoO/TiO2 composite nano-catalyst superior to any such model system studied to date. It was further shown that when deposited on inert SiO2 metallic Co was more active than CoO by almost threefold, in accord with the general model that identified metallic Co as the initially active state. No spectroscopic or crystallographic evidence was, however, found that could be attributed to a CoC x phase.

This work further identified enhanced wetting of CoO on TiO2 as one potential explanation for catalytic promotion of the oxidized state. By using APXPS, it was demonstrated that the topmost surface, corresponding to inelastic mean free paths of 180 eV photoelectrons, of the CoO x /TiO2 catalyst changed dramatically (Fig. 10a, b). CoOx formed when the catalyst was treated in 100 mTorr O2 at 350 °C, and no trace of metallic Co was found when O2 was pumped out and H2 was dosed at 250 °C. Also in 100 mTorr H2 and 250 °C, CoOx occupied more space on the topmost surface regions which was ascribed to wetting of TiO2 by CoO x (Fig. 10c). When temperature was increased to 450 °C in 100 mTorr H2, Co was partially reduced. Metallic Co was then encapsulated in part by TiO2, decreasing its surface coverage and interaction with the oxide, probably as a result of the lower surface free energy of the oxide (Fig. 10d). This encapsulation of Co NPs by TiO2 must have been more pronounced under reaction pressures (i.e. more than four orders of magnitude higher in H2 when compared to APXPS) pertinent to soft XAS measurements (and catalytic testing), which detected only metallic Co in the near surface regions. Therefore, the loss of active catalyst surface and exposed CoOx/TiO2 interface, both linked to the encapsulation, must be responsible for the activity drop observed for the reduced catalyst (Fig. 10e, f).

Fig. 10
figure 10

a Co 2p and b Ti 2p APXPS spectra recorded in 100 mTorr H2 and at given temperatures.  % Co on surface calculated from the APXPS spectra under H2 atmospheres and at c 250 °C and d 450 °C. Cartoon depicts the support effects, comparing SiO2 (i.e. inert) and TiO2 substrates, as deduced from the APXPS results. Turnovers compare catalytic hydrogenation of CO2 over e oxidized CoO NPs and f metallic Co NPs supported in SiO2 and TiO2. Note that the y-axes are given to the same scales in c, d and e, f [Adapted with permission from Melaet et al. [94]. Copyright: (2014) American Chemical Society]

3.2.2 The Role of Nobler Metal in Co-Based Bimetallic Nano-Catalysts During CO2 Hydrogenation

Recently, the role of a second metal in Co-based bimetallic catalysts was put into question based on a study using in situ Soft X-ray Spectroscopy and E-TEM [95]. When Co was co-precipitated with a second metal such as Re or Pt the enhanced F–T synthesis activity obtained for the resulting catalyst, usually ill-characterized yet generally assumed to be some alloy form, is attributed to high reducibility of Co [9698]. In this work, a two-dimensional film of bimetallic CoPt alloy NPs, monodisperse 4 nm in size and 50:50 compositions, were investigated in redox atmospheres (H2 or O2) at temperatures in the 125–250 °C range. CoPt NPs performed poorly during catalytic hydrogenation of CO2 and were exclusively selective for the formation of CO (i.e. active only for the rWGS reaction). The lack of methanation reactivity and the production of CO were consistent with pure Pt NPs screened in a control run. Soft NEXAFS spectroscopy revealed easier reducibility and larger capacity of Co to remain metallic in the alloy nanoparticles compared to pure Co NPs of identical monodisperse sizes, which was attributed to a hydrogen spillover effect. The initial findings supported the generally accepted model for bimetallic F–T catalysts.

However, further investigations over model CoPt NPs using APXPS for 4 nm sizes and E-TEM for 10 nm sizes indicated that the reduction of Co was accompanied by the core/shell restructuring of the originally alloy NPs [87]. In the revisited model, Pt atoms, randomly distributed intra-particle, diffused outward forming thin Pt shells in H2 atmospheres which facilitated the reduction of Co atoms. In the mTorr O2 pressures, Pt shells screened subshell Co atoms from oxidation. As the O2 partial pressure increased beyond 100 mTorr, Co was oxidized and substituted Pt on the surface. Likewise, annular dark field images obtained in 100 mTorr H2, the same partial pressure as in APXPS studies, for individual nanoparticles (Fig. 11), showed bright surface layers and dark subsurface shells, indicating the enrichment of higher Z Pt atoms in the surface regions and Co atoms in the subsurface regions [95, 99]. Hence, TEM agreed with the APXPS results pointing to core/shell restructuring and Pt surface segregation of once alloyed nanoparticles in H2 atmospheres. Catalytically, the bimetallic CoPt NPs then behaved Pt-like as a result of the surface enrichment of Pt under net reducing atmospheres of the H2/CO2 reaction.

Fig. 11
figure 11

a ETEM BF picture of a single CoPt NP imaged in 0.1 Torr H2 and at 250 °C, showing lattice fringes: 0.22 nm for Pt(111) on the surface (red area) and 0.2 nm for Co(111) in the subsurface (green area). b STEM ADF picture of a single CoPt NP after (20 vol% H2) reduction at 400 °C. Dark band below bright surface indicates enrichment of Co in the subsurface as expected of the lower Z Co. c Co L3,2 electron energy loss map recorded after (H2) reduction at 400 °C. Note that Co shuffled back into the alloy particle as compared to the segregated particle in Fig. 7c [modified with permission from Xin et al. [99]. Copyright: (2014) American Chemical Society]

These in situ findings have implications in the design and fabrication of F–T catalysts. First, the ratios of metal components for bimetallic F–T catalysts, when chosen above the surface-to-volume ratio for any given catalyst particle, render the formation of a full monolayer of the second metal possible. For example, surface to volume ratios for nanoparticles above 10 nm are just a few percent, while the ratio exponentially increases with decreasing particle sizes. Hence, the metal loadings should be carefully chosen while considering the geometric variables of the catalyst composite. This is also why nanoparticles that are monodisperse in size and architecture are essential for heterogeneous catalysis in general. Second, because alloy architectures—composed of one (or more) oxyphilic metal(s) (e.g. Co) and one (or more) noble metals (e.g. Pt)—are kinetically metastable under synthetic F–T conditions, they are subject to core/shell restructuring where noble metal components tend to surface segregate in the thermodynamic limit. This statement is also true for any core/shell architecture with oxyphilic metal atoms comprising the shells. Then, the active particle architecture must have been overlooked; physically mixed composites of the two metal systems could well have been the active form of the bimetallic F–T catalysts.

3.2.3 Hydrogen Atom Spillover Between Pt and Co NPs When no Physical Contact was Established Between the Two

This hypothesis was put to the test in a more recent work. Two model catalyst architectures were fabricated: a mixture of individual monometallic nanoparticles supported within the same physical domain (i.e. a physical mixture); and a mixture of supported nanoparticle domains, each with only one kind of metal (i.e. a mechanical mixture) [100]. Experimentally, monometallic Co and Pt NPs, synthesized with known colloidal procedures, were either: mixed in a 30:1 mol ratio (Co:Pt) before being deposited on mesoporous silica (physical mixture); or deposited separately on mesoporous silica and the supported composites then mixed to give a 30:1 mol ratio of Co:Pt (mechanical mixture). Catalytically, both the physical and mechanical mixtures of Co and Pt NPs showed more than a fivefold enhancement in turnovers with improved selectivity toward methane formation relative to a pure Co catalyst. In 150 Torr H2 and in the 175–225 °C range, both catalyst mixtures exhibited larger fractions of metallic Co in the near surface regions, evidenced by in situ NEXAFS studies of the two-dimensional NP films at the Co L edge. As to the topmost surface by extrapolating from the surface-to-volume ratio metallic Co was found only for the Pt–Co catalyst mixtures, while the pure Co catalyst was completely oxidized. It was demonstrated that a hydrogen spillover pathway existed for the mixtures regardless of the interparticle separation between Pt and Co NPs. The H2/CO2 reaction was promoted by increased availability of atomic hydrogen either to remove surface oxides and hydroxides, to be inserted into the carbon backbone, or a combination thereof.

3.3 Hydrogenation of Unsaturated Hydrocarbons and Hydrogenative Isomerization of Methylcyclopentane

Hydrogen spillover from Pt NPs onto oxide supports have profound implications in tailoring catalytic selectivity [101]. In situ SFG vibrational spectroscopy (VS) combined with catalytic measurements can help in understanding the hydrogenative reforming reactions which usually exhibit complex reaction networks.

3.3.1 Hydrogen Atom Spillover at the Pt/TiO2 Interface During Hydrogenation of Furfural and Crotanaldehyde

Selective hydrogenation of carbonyl bonds in unsaturated aldehydes to form unsaturated alcohols has been recently demonstrated for 2 nm Pt NPs supported at a sub-monolayer coverage on e-beam evaporated TiO2 films (~50 nm) by using in situ SFG VS and catalytic measurements during hydrogenation of furfural [102] and crotanaldehyde [103]. Both molecules were found to produce more unsaturated alcohols (i.e. selective hydrogenation of the carbonyl bond) than saturated alcohols (nonselective hydrogenation of both the carbonyl bond and C=C double bond) or unsaturated aldehydes (selective hydrogenation of C=C double bond) over a Pt/TiO2 catalyst when compared to Pt NPs deposited on thermally grown SiO2. It was proposed based on in situ SFG studies under identical conditions as the catalytic testing that unsaturated aldehydes chemisorbed on Pt sites with their C=C double bonds lying parallel to the surface while C=O bonds were located upright and away from the surface. This bonding configuration led to selective hydrogenation of the C=C double bond and desorption of the saturated aldehyde, as illustrated in Fig. 12 for the hydrogenation of furfural. However, Ti3+ centers associated with O defects on the TiO2 surface acted as unique adsorption sites for the unsaturated aldehydes with their C=O bonds facing down and C=C double bonds pointing up and away from the surface. In this case, C=O bonds were selectively reduced to form alcohols by atomic hydrogen spillover from nearby Pt NP surfaces, as shown previously for Pt/CeO2 and Pt–Co hybrid nano-catalysts above.

Fig. 12
figure 12

In situ SFG spectra (left column) obtained in H2/furfural (100:1) and at 120 °C for Pt/SiO2, TiO2 and Pt/TiO2 model nano-catalysts (from top to bottom). Cartoons (right column) show the binding geometries of reactants as deduced from the SFG results and major products from catalytic measurements [adapted with permission from Baker et al. [13, 102]. Copyright: (2012) American Chemical Society]

3.3.2 Surface Diffusion of Intermediates at the Pt NP Mesoporous Zeolite Interface During Hydrogenative Isomerization of Methylcyclopentane

Spillover of reactants other than hydrogen was documented for hydrogenative isomerization of methylcyclopentane (MCP) over model Pt/mesoporous zeolite nano-catalysts by using in situ SFG [104]. For this study, 2.5 nm monodisperse Pt NPs were deposited in mesoporous zeolites of two different crystal framework structures: the BEA zeolite framework with a Si:Al ratio of 10 and the MFI zeolite framework with a Si:Al ratio of 1. Hydrogenative isomerization of methylcyclopentane was carried out in a plug-flow reactor using 10 Torr MCP, 50 Torr H2 in a balance of 700 Torr He at 150 °C. The in situ SFG VS studies were carried out under the same conditions. It was found that both Pt/zeolite nano-composite catalysts led to ring enlargement pathways, producing cyclohexane and benzene, which were not detected for the MCP/H2 reaction over either pure Pt or mesoporous zeolites. It was also noticeable that the Pt/BEA catalyst produced cyclohexane with ~70 % selectivity, while the Pt/MFI catalyst produced benzene with ~80 % selectivity. Furthermore, both catalysts exhibited an order of magnitude enhancement in turnovers normalized to either available Pt sites or zeolitic Al sites.

SFG spectra indicated for both the Pt/zeolite catalysts the presence of a methylene stretch of saturated C6 cyclics at 2,780 cm−1 and =CH2 asymmetric stretch of unsaturated C6 cyclics at 3,065 cm−1. The vibrational signatures were consistent with those of cyclohexene, and the lack of cyclohexene among the products indicated that it formed as a reactive intermediate on the catalyst surfaces at the interface between the Pt and alumina silicate support. A control run using 10 Torr cyclohexene and 50 Torr H2 in a balance of 700 Torr He led to ~70 % cyclohexane over the Pt/BEA and ~80 % benzene over the Pt/MFI. In addition both the catalysts achieved almost complete conversion, suggesting that if cyclohexene formed it would indeed hydrogenate/dehydrogenate to cyclohexane/benzene. It was proposed that an unsaturated C6 cyclic, most probably cyclohexene, was generated at the interface of the Pt and zeolites which in turn hydrogenated/dehydrogenated to the final products. Furthermore, the ratios of cyclohexene and benzene were governed by the zeolite framework type; BEA with the higher Si:Al ratio led to more hydrogenation (a factor of two) whereas MFI with the lower Si:Al ratio led to more benzene (a factor of four). SFG spectra displayed physisorbed benzene at 3,035 cm−1 only for the Pt/MFI, in accord with the higher benzene formation rate obtained for this catalyst.

3.4 Heterogenized Homogeneous Transformations in Organic Solvents

Re-adsorption contributes to product evolution in cascade catalytic reaction systems, as important a factor as the reactant spillover in other multi-path/multi-product reactions. In this respect, homogeneous hydrocarbon transformations, especially those that involve single metal sites and single reaction centers, are the most fundamental systems to look for. When carried out heterogeneously, homogeneous catalytic reactions can be understood in the surface-reactivity context; however, their kinetic investigation in the heterogeneous mode requires tools with time resolutions in the same regimes as residence times, usually in the millisecond time scale. In Fourier transformed IR where measurements in the vibrational time domain are exchanged for vibrational frequency domain, spectral acquisition can be gated with reactive gases pulsed in short time intervals on the millisecond scale [105, 106]. Therefore, FTIR can provide the instrumental time resolution necessary to monitor the history, frozen in time, of catalytic transformations. However, such short time scales are not measurable by XAS tools not even when quick XAFS [107] and energy dispersive XAFS [107, 108] techniques are employed.

In a recent work, time-on-stream reaction events in the millisecond time scales were resolved simply by using reactor geometry, reactant flow rate, and micron-sized XAS probes. For this study a capillary quartz tube of 1 mm diameter was employed where the powder catalyst was packed in a 10 mm long bed. For a linear flow rate of reactants (v) and any given distance from the origin of the catalyst bed (l), the time-on-stream of reactants is calculated by the equation, l/v. The time resolution is then obtained by the probe size and flow rate (0.5 ms for a 10 µm probe and 5 ml/h flow rate), and the shortest time-on-stream measurable is only limited by the motion of the stepped motor, which is used to translate the probe along the capillary tube or vice versa. When the X-ray probe is locked in a known distance from the origin, the collective memory of the reaction time-on-stream along the reactor bed up to that position will be stamped on the XAS spectrum regardless of the instrumental time resolution of the XAS setup, illustrated in Fig. 13. By way of trading position with time, the time evolution of the catalyst can then be monitored.

Fig. 13
figure 13

a Time series of Au L3 edge Quick NEXAFS spectra recorded in 3.5 min intervals (which sets the instrumental resolution) showing the reduction of a PhICl2 oxidized Au nano-catalyst in the batch mode. b Ratios of Au3+/Au0 calculated from a least squares fitting of the NEXAFS spectra recorded at various positions along a capillary micro-reactor during the cascade synthesis of hydropyran. Note that the time steps on the order of seconds were achieved by trading position with time for a flow rate of 5 ml/h, while the spectral acquisition times were about 20 min [adapted with permission from Gross et al. [109]. Copyright: (2014) American Chemical Society]

3.4.1 Time-On-Stream Kinetics of Au3+ Reduction During Hydropyran Synthesis

This ‘trading-position-with-time’ strategy was exploited to evaluate a silica supported, dendrimer encapsulated Au NP catalyst during a liquid phase hydropyran synthesis reaction [109]. 2 nm monodisperse Au NPs were oxidized in situ by PhICl2 present in the butanol reaction solution at stoichiometric amounts to Au. XAS displayed metallic Au without the PhICl2 oxidant. It also displayed Au3+ with the reaction solution within a 2 mm distance of the reactor bed, which was registered as a reactant time-on-stream of 5 s (Fig. 13b). Beyond this distance, Au was gradually reduced back to metallic Au which rendered the catalyst inactive for the cascade transformation. It was found that no Au3+ was present 10 mm away from the reaction origin. By using IR microscopy and a similar capillary reactor setup (two CaF2 widows separated by a 0.5 mm thick spacer), it was found for the same reaction solution in d-butanol that the hydropyran was the sole product beyond 1 mm distance from the reaction origin. Furthermore, d-butanal was observed beyond this distance, suggesting a competitive oxidation pathway as to how Au was reduced back to its metallic state.

4 Summary and Future Challenges

Colloidal nanoparticle catalysts are attractive model systems to study catalytic reactions. Tailoring physical and chemical properties of metal nanoparticles and oxide supports/co-catalysts offers an intriguing way of controlling catalyst behavior and catalytic trends. In this context, the particle size and architecture of metal nanoparticles can be varied by using colloidal chemistry to gain insight into the catalytic roles of physical and chemical variables of a catalyst. These variables are crystal shape and morphology, oxidation state, coordination, and bonding. Then, well-defined metal nanoparticles can be deposited on the choice of oxide support/co-catalyst to explore well-known support effects.

In situ surface techniques and tools are required to investigate the dynamic changes that nano-catalyst undergo as catalytic reactions occur. In situ NEXAFS TEY probes the oxidation state changes on the near surfaces of metal catalysts and oxide supports. Furthermore, coordination and bonding stem from in situ EXAFS for small nanoparticles and clusters where surface and bulk become one. Likewise, APXPS is elementally and chemically sensitive to composition changes on the near surfaces under catalytically relevant reactant pressures. In situ SFG VS provides complementary adsorbate bonding structure on the immediate surface. Intermediate species can then be inferred.

When combined with catalytic turnover and selectivity measurements in reactors built in parallel or in-line with the in situ probe setup, these techniques and tools can lead to better understanding of the catalysis and surface phenomena. As a demonstration of this correlative strategy, some case studies from the Somorjai group employing well-defined nano-catalysts of bimetallic and/or metal/oxide hybrid architectures were described in relation to support effects, surface bifunctionality, diffusion of neutral species, and charge flow. In situ studies unquestionably gave insight into the structural factors that dynamically alter catalyst surfaces. Nevertheless, there emerged other questions that require new techniques and tools to be developed and novel experimental strategies to be devised.

The support effects, on one hand, invoke strong-metal–support interactions (SMSI) which have undesired connotations of catalyst deactivation and quenching of catalytic reactivity. This was exemplified by the encapsulation of metallic Co by macroporous TiO2, which was experimentally detected using APXPS in H2 atmospheres and during net reducing atmospheres of the H2:CO2 (3:1) reaction. On the other hand, SMSI is associated with charge transfer phenomenon, where electrons or protons flowing in one direction selectively enhance certain reaction pathways. SMSI is also associated with bi-functionality, where metals and oxides activating different reactants promote catalytic activity by means of synergism. It was previously demonstrated that electrons are generated at the Schottky interface of Pt and negatively doped TiO2 films due to the CO/O2 reaction: charge flow through an external circuit was measured and correlated with catalytic turnovers [110, 111]. However, there is no study to date that unequivocally shows the charge flow between metal nanoparticles and metal oxide supports such as to control catalytic reaction channels and/or turnovers. Therefore, purposely designed and fabricated model nano-catalysts are needed in the future to bridge the existing experimental gap.

Bifunctionality is, however, the apparent reason beyond the promotional effects as demonstrated for the Pt/mesoporous metal oxide (e.g. Co3O4, MnO2 and CeO2) catalysts using soft XAS under catalytic CO oxidation conditions. It is yet not fully conceivable as to how and why some metal oxides perform superior to others. The only physical correlation found was that the redox states (i.e. in situ NEXAFS) of metal oxides respond to the redox power of the reaction atmosphere. However, no trend explains the ordering of the different oxides in terms of the measured catalytic turnovers. Hence, to a first approximation, it could be the oxides’ resistance to charge flow. It was believed that surface defects and vacancies, as illustrated for the Pt/CeO2 catalyst, could act as trap sites for charged species as to mitigate the catalytic enhancement measured. Therefore, metal oxides with well-controlled crystalline phases and defect chemistries are essential to future experiments which should be devised to generalize this unique observation to other metal oxide systems.

Reactant (i.e. neutral species) spillover can be considered in the same category as interfacial charge flow, yet there exist tools in the service of experimentalists like SFG that are best suited for monitoring the diffusion of these mobile adsorbate molecules. An unsaturated C6 cyclic intermediate, ascribed to cyclohexene, was proposed for the hydrogenative isomerization of MCP over the Pt/mesoporous zeolite catalysts based on in situ SFG vibrational spectroscopy. Also by using in situ SFG vibrational spectroscopy, selective hydrogenation of carbonyl functional groups at the Pt/TiO2 interface was traced back to hydrogen atom spillover from the Pt surface to Ti3+ sites. Likewise, the enhanced reducibility and methanation yield of Co NPs by physically distant Pt NPs, monitored by in situ soft XAS and catalytic measurements, was attributed to hydrogen atom (i) spillover from nearby Pt NPs to silica support and (ii) uptake from the silica support by Co NPs. This study also highlighted surface diffusion and adsorbate mobility as factors that govern selectivity and reaction kinetics. However, direct spectroscopic evidence of mobile hydrogen atoms is yet to be presented, as in the case of charge transfer (i.e. protons or hydrides).

In this context, time transients and kinetics of catalytic transformations should be explored in greater detail in future studies. This involves advancing instrumental time resolution on one hand and implementing strategies to diminish the need for advanced instrumentation on the other. The trading-position-with-time strategy, using micro-reactors and micron sized X-ray probes, is one that gave rise to time steps in the milliseconds regime. This concept was demonstrated by in situ NEXAFS for the time-on-stream reduction of active Au3+ species during a cascade cyclization reaction. When used with gas flows, where typical flow rates are much higher than liquid flows, the same strategy gives time sensitivity high enough to probe time-on-stream events on the order of microseconds. As a result, the flow of charged (i.e. protons) and neutral (i.e. hydrogen atoms) species can be monitored, providing that chemically sensitive tools are available. However, it should be noted that such technical limitations might remain as grand challenges in the face of in situ studies in the future. Taking an otherwise chemically sensitive tool, XPS for example, hydrogen has no photoelectron spectrum, nor does proton (electron) transfer have any spectral signature other than small core-level shifts in fractions of an electron volt, which are usually very difficult to detect even in UHV.

Finally, new instrumental techniques and design strategies are required for in situ studies of catalyst surfaces. One particular technique of interest is ion scattering, which uses ionized gas molecules as depth sensitive probes, like low energy ion scattering [112114]. When reactive gas molecules are employed as probing ion sources, like atom probe microscopy (APM), an atomically resolved layer by layer construction of catalysts can be achieved [115119]. However, the destructiveness and high vacuum requirements of ion scattering and microscopy techniques are currently detrimental to their use for in situ or in operando experiments and stand as a grand challenge for their developers.

Spectro-microscopy techniques such as TEM/EELS and AFM-Raman, which provide nanometer size local probes with high surface sensitivity, are also worth mentioning. They are technically advanced to such levels that render unique in situ and in operando studies possible. Along these lines, scanning transmission X-ray microscopy (STXM), which bridged the in situ gap between classical X-ray (absorption or photoelectron) spectroscopy and nano-spectroscopy, sets a milestone. Briefly, STXM uses diffraction zone plates and order sorting apertures (state-of-the-art X-ray optics) to focus monochromatic soft X-rays to spot sizes of about 40 nm. Nanoparticle powders and films deposited over thin silicon nitride membranes are hermetically sealed along with built-in capillary tubes and resistive micro-heaters, which allow atmospheric pressure reactive gases at elevated temperatures in a gas flow cell. Sample motion along the scanning plane is then achieved by using piezo-controlled stepper motors. By this way, elemental mapping at the absorption edge of transition metals and low-Z elements such as O and C can be obtained, in a way not much different than STEM/EELS. This has been previously demonstrated under catalytically relevant flow conditions for a Fe-based Fischer–Tropsch catalyst [120]. In the near future, the catalysis field will benefit from the involvement of such spectro-microscopy techniques in in situ/in operando studies.