Open Access Article
Rishi Verma
*,
Gunjan Sharma
,
Rohit Bansal
,
Charvi Singhvi
,
Saideep Singh
and
Vivek Polshettiwar
*
Department of Chemical Sciences, Tata Institute of Fundamental Research, Mumbai, 400005, India. E-mail: rishi.verma@tifr.res.in; vivekpol@tifr.res.in
First published on 21st May 2026
Photocatalysis stands at the forefront of efforts to address global challenges in sustainable energy and environmental remediation. In this review, we critically examine the two major classes of heterogeneous photocatalysts-plasmonic materials and semiconductors-highlighting their fundamental distinctions, catalytic mechanisms, and potential for driving light-induced chemical transformations. We first explore the fundamentals of plasmonic materials and semiconductors, highlighting key distinctions and overlaps in their photophysical properties, elucidating how these differences govern their photocatalytic performance and reaction pathways. This review further explores practical examples of photocatalytic reactions, including CO2 reduction, N2 reduction, and dry reforming of methane (DRM), illustrating the versatility, catalytic efficiency, and inherent limitations of each class of materials. Additionally, we explore the excited-state dynamics of both plasmonic and semiconductor materials, with a focus on the underlying mechanisms that govern charge carrier behavior under light excitation. This review provides an overview of the present state of plasmonic and semiconductor photocatalysis, while also highlighting promising directions for future advancements. By exploring synergistic strategies that bridge these two classes of materials, it aims to unlock new pathways for light-driven chemical transformations, ultimately advancing catalytic performance for sustainable energy and environmental applications.
Over the past few decades, significant progress has been made in developing materials capable of efficiently absorbing sunlight and driving chemical transformations. However, the challenge of improving catalytic efficiency remains, especially when dealing with complex multi-electron processes like CO2 reduction or water splitting. The efficiency of a photocatalyst is highly dependent on the material's ability to interact with light, separate charge carriers, and drive specific reactions. Therefore, designing materials with optimal light absorption, charge transfer, and catalytic properties is crucial for the high efficiency of photocatalysts.1–6
With the advent of nanotechnology, new opportunities have arisen to engineer photocatalysts that can manipulate light and charge carrier dynamics at the nanoscale. Among the various photocatalytic systems that have been explored, two major categories have stood out: semiconductors,7–150 and plasmonic photocatalysts.151–435 These two classes of materials are often studied in isolation and are governed by fundamentally different photophysical principles with direct consequences for catalysis. While other classes, such as molecular photocatalysts, metal complexes, and biological systems like photosystems used in photosynthesis, are also highly relevant, this review focuses on semiconductors and plasmonic materials, as these two classes have emerged as the most extensively studied solid-state platforms for heterogeneous photocatalysis. Semiconductors and plasmonic metals differ not only in how they absorb light but also in how they manage and utilize the resulting excited states. Semiconductors rely on band-to-band transitions that generate relatively long-lived electron–hole pairs. Plasmonic materials, in contrast, exploit collective electron oscillations that lead to intense light–matter interactions, ultrafast carrier generation, and localized field effects. These distinct pathways set the stage for fundamentally different catalytic behaviors, motivating a careful side-by-side comparison.
This dichotomy highlights why a direct comparison is timely. A discussion on excitation mechanisms, carrier relaxation dynamics, and catalytic performance across both systems can clarify how their distinct photophysics translate into performance. It also provides design principles for next-generation catalysts that aim to integrate the long carrier lifetimes of semiconductors with the strong light–matter interactions of plasmonic nanostructures.
Semiconductor-based photocatalysts have been a foundation of photocatalytic research since the pioneering work on TiO2 for water splitting by Fujishima and Honda in 1972.7 Semiconductors, such as TiO2, ZnO, CdS, and BiVO4, are known for their ability to absorb photons and generate electron–hole pairs that can subsequently participate in redox reactions at the catalyst surface. Upon photon absorption, an electron is excited from the valence band to the conduction band, leaving behind a hole. These charge carriers (electrons and holes) can migrate to the surface and participate in oxidation and reduction reactions, enabling processes like water splitting and CO2 reduction. The efficiency of semiconductor photocatalysts is highly dependent on factors such as the band gap, light absorption properties, charge carrier mobility, and the ability to suppress charge carrier recombination.13,17,137
Despite their widespread use, semiconductor-based photocatalysts face persistent challenges in harvesting solar energy efficiently. Many, such as TiO2, are mainly active under ultraviolet (UV) light, which accounts for only ∼5% of the solar spectrum.22 Even when visible-light excitation occurs in certain semiconductors, it often produces less energetic charge carriers, limiting photocatalytic efficiency.28 Their relatively low absorption coefficients further restrict overall light harvesting.137 To address these issues, extensive strategies such as doping, defect engineering, and heterojunction formation have been explored to extend absorption into the visible region and enhance electron and hole separation.44,62 Emerging designs, including 2D semiconductors, quantum dots, and core–shell nanostructures, show promise in improving light absorption and charge dynamics, thereby advancing the potential of semiconductor photocatalysts for scalable applications.10,11
On the other hand, plasmonic photocatalysis has attracted significant attention for its ability to harvest visible light through localized surface plasmon resonance (LSPR) in metal nanoparticles such as Au, Ag, Al, and Cu. Plasmonic nanoparticles can generate highly energetic charge carriers and strong local electromagnetic fields, enabling selective and efficient photocatalytic transformations.151 They have been widely explored for reactions such as CO2 reduction, water splitting, and nitrogen reduction.155,186,404 However, plasmonic systems also face challenges, particularly related to the relatively short lifetimes of excited charge carriers (hot electrons) and the difficulty in controlling charge transfer processes.152,161 Moreover, the scalability of plasmonic materials, given their reliance on precious metals, presents another challenge for widespread commercial use. Despite these hurdles, the unique ability of plasmonic photocatalysts to drive reactions under visible light and their tunable properties make them an exciting area of research with significant potential for future energy applications.
Thus, despite advances in photocatalyst design, both semiconductor and plasmonic systems face intrinsic limitations that hinder large-scale application. A comparative analysis of these two approaches is therefore crucial to highlight their respective strengths, limitations, and opportunities for synergistic innovation. In this review, we present a comprehensive comparison of plasmonic and semiconductor photocatalysts, focusing on their fundamental properties, including excitation mechanism, charge carrier dynamics, and excited-state lifetimes. We examine the distinct mechanisms by which these materials absorb and harness light, highlighting how these differences influence their photocatalytic efficiency and reaction pathways. Additionally, we highlight key photocatalytic applications, including CO2 reduction, N2 reduction, and dry reforming of methane (DRM), where both plasmonic and semiconductor photocatalysts have demonstrated their potential. By discussing the strengths and limitations of each system, we aim to identify promising avenues for future research and development, ultimately guiding the design of more efficient and sustainable photocatalytic materials for energy and environmental applications.
To comprehend these phenomena, it is essential to understand the underlying electronic structure of solids. Detailed mathematical treatments of band structure, density of states, momentum conservation, and the Fermi level are well established in solid-state physics texts and are therefore beyond the scope of this review.436–439 Here, we provide only a brief introduction to establish a conceptual basis for the discussion that follows. The energy bands in a material dictate the range of energy of electron occupation, with the band gap defining the energy gap between the conduction band and valence band. The band gap also dictates the photon energy required to generate electron–hole pairs. The Fermi level represents the electrochemical potential of electrons in the material, equivalently, the energy at which the Fermi-Dirac occupation probability equals one-half. In metals, it coincides with the highest occupied electronic state at absolute zero; in semiconductors, it lies within the band gap, and its precise position is determined by the doping level and temperature. Momentum conservation determines the efficiency of optical transitions, while the density of states (DOS) governs the availability of electronic states for excitation.436–439 Together, these fundamental aspects of electronic structure determine the photophysical responses of semiconductors and plasmonic materials, including both their commonalities and distinctions.
The electron–hole pairs generated through light excitation in semiconductors catalyze a variety of chemical reactions. The entire process, from the moment excitons are generated to when the charges participate in redox chemistry, can be delineated into three distinct stages:
(1) Photoexcitation: this initial stage involves the absorption of light by the semiconductor, resulting in the generation of excitons.
(2) Charge separation and diffusion: following photoexcitation, the excited charges (electron–hole pairs) must be effectively separated and diffused to the catalyst surface. Minimizing electron–hole recombination during this stage is critical to ensure that a greater number of charge carriers reach the surface.
(3) Charge utilization for redox reactions: in the final stage, the separated charges participate in redox reactions at the catalyst surface. To attain high efficiency in these reactions, it is essential to not only maintain a high charge carrier density but also promote stronger surface adsorption and activation on the catalyst, facilitating the efficient coupling of surface charges with targeted reduction or oxidation reactions.
To optimize the charge generation step, researchers are focused on developing catalysts capable of absorbing a broader spectrum of solar energy, thereby maximizing the number of photons converted into electron–hole pairs. However, having a high density of charge carriers on the surface does not guarantee efficient redox reactions. Enhancing the molecular-level catalytic activity and selectivity is essential for effective surface reactions.
The ability of photogenerated electrons and holes to take part in reduction and oxidation is mainly determined by the relative positions of the conduction band minimum (CBM) and the valence band maximum (VBM). For an overall photocatalytic reaction to proceed, the CBM must lie at a higher energy than the reduction potential of the target species, while the VBM must lie at a lower energy than the oxidation potential of the corresponding species (Fig. 1a). If either of the band edges (CBM or VBM) fails to meet this criterion, sacrificial agents must be employed as alternative electron acceptors or donors to facilitate the required half-reaction.14
In pristine semiconductor photocatalysts, charge carrier generation, migration, and surface reactions occur on the same material, but each stage faces intrinsic limitations. Wide-band gap semiconductors (e.g., TiO2) are limited to UV absorption (∼5% of the solar spectrum), while narrow-band gap materials (e.g., CdS, Fe2O3) harvest visible light but often exhibit weaker redox potentials due to unfavorable band-edge positions.11 Once generated, electrons and holes frequently recombine during migration because separation lacks a strong driving force. At the surface, slow reaction kinetics and limited catalytic activity further reduce efficiency, while accumulated charges may even degrade the semiconductor.11,14 One important factor modulating charge dynamics is band bending at semiconductor surfaces and interfaces. Fermi-level equilibration between bulk and surface, or between different crystal facets, induces space charge regions and internal electric fields. These fields can steer electrons and holes toward different reaction sites, partially improving separation.11 Facet engineering, ferroelectric polarization, dipole fields, and junction formation (metal–semiconductor or semiconductor–semiconductor) provide additional routes to enhance charge carrier separation. A more comprehensive discussion of these interfacial effects and their role in modulating charge dynamics can be found in a previous review.11
The LSPR arises when light interacts with metal nanoparticles smaller than the incident wavelength, inducing collective oscillations of surface electrons. The decay of these oscillations generates energetic hot carriers and heat on ultrafast timescales (Fig. 1b).151,152 The optical response of plasmonic nanoparticles can be tuned by their size and shape, enabling efficient sunlight absorption and energy conversion. Hot electrons generated during LSPR dephasing can either transiently activate adsorbed molecules on the metal surface without permanent transfer or undergo plasmon-mediated electron transfer (PMET) to nearby semiconductors or molecules, driving reactions such as water splitting, CO2 reduction, and organic transformations.152,155 The relaxation of hot carriers occurs through electron–electron and electron–phonon scattering, leading to heat dissipation, which can also catalyze reactions on metal surfaces. In addition, LSPR creates intense near-field enhancements at particle edges or junctions, amplifying light absorption and scattering to boost catalytic efficiency.152 Understanding these ultrafast carrier dynamics and their coupling with reactants is crucial for designing efficient plasmonic photocatalysts.151,157,170
The strength of these interactions is quantified through the absorption and scattering cross-sections, which depend on the polarizability. The scattering cross-section increases with the sixth power of the particle radius, while the absorption scales with the third power, making absorption dominant for smaller particles.436–439 These relationships are given by:
![]() | (1) |
![]() | (2) |
The effectiveness of hot electron generation depends on efficient electron-surface interactions, which are promoted in systems with surface features that disturb translational symmetry, enhancing electron scattering and photon absorption. The subsequent generation of thermalized electrons through electron–electron scattering depends on the scattering rates, while the conversion of light energy to heat is governed by the electron–phonon scattering processes. Both processes are strongly influenced by the size of the metal nanoparticles. Smaller nanoparticles exhibit increased electron-surface interactions, raising the probability of hot electron generation and improving electron-driven catalysis. In contrast, larger nanoparticles more readily channel absorbed energy into lattice heating, leading to more pronounced photothermal effects, because reduced surface scattering and longer electron mean free paths favor bulk electron–phonon energy transfer over hot-carrier extraction.151
In summary, the photophysical foundations of these two material classes are defined by their distinct electronic structures: the discrete band gap of semiconductors and the collective electronic oscillations of plasmonic metals. While semiconductors drive catalysis through the generation and separation of relatively long-lived electron–hole pairs governed by band-edge potentials, plasmonic materials operate through the ultrafast generation of high-energy hot carriers and the creation of intense localized electromagnetic fields. By defining the specific stages of carrier generation, migration, and utilization, it becomes clear that the efficiency of these systems is intrinsically linked to their unique energy-relaxation timescales and optical cross-sections. Establishing this conceptual framework is a prerequisite for understanding how these materials can be tailored to meet the specific thermodynamic and kinetic requirements of complex chemical transformations.
Having established the fundamentals of semiconductors, excitons, and plasmonic excitation, we now turn our attention to practical applications. In the following sections, we will explore the similarities and differences in plasmonic and semiconductor systems and how these properties facilitate catalysis in significant reactions, including nitrogen reduction, CO2 reduction, and dry reforming of methane. Finally, we will conclude with ultrafast studies on semiconductor and plasmonic materials, thereby linking the photophysical aspects previously discussed with observed catalytic phenomena in the literature across various reactions.
Understanding these distinctions requires examining the microscopic processes that govern light–matter interactions, where classical and quantum effects dictate how absorbed energy is utilized. This section highlights the contrasting strengths and limitations of semiconductors and plasmonic materials, highlighting why their performance in photocatalysis differs fundamentally. A comparative evaluation of these two classes of photocatalysts thus provides insights into their mechanisms and potential applications.
This collective oscillation of conduction electrons arises from the intrinsic dielectric response of metals, which is strongly dependent on their free carrier density. When the frequency of incident light matches the natural oscillation of these electrons, a resonance condition is established. Under these conditions, the nanoparticle exhibits robust light–matter coupling, resulting in absorption and scattering cross-sections that can exceed the particle's geometric cross-sectional area by one to two orders of magnitude. This unique property results in the extraordinary optical response of plasmonic nanostructures and sets them apart from conventional semiconductors.
This collective excitation is short-lived, typically dephasing within 1–10 fs through Landau damping, wherein the coherent plasmon oscillation decays into excited charge carriers. The resulting hot carriers possess a broad, non-thermal energy distribution that extends well above the Fermi level (Fig. 1b). Such a wide energetic spread is often regarded as one of the defining advantages of plasmonic systems, as unlike semiconductor photoexcitation, where a single photon generates a single electron-hole pair at a specific energy, the collective nature of plasmon excitation yields hot carriers distributed across a broad range of energies from a single plasmon decay event.160,171,181
In contrast to plasmonic systems, semiconductor photoexcitation is governed by discrete optical transitions between well-defined electronic bands. Each absorbed photon generates a single electron–hole pair (or exciton) with specific energy and momentum, rather than a broad, collective excitation involving multiple electrons (Fig. 1a).137 This distinction arises from the band structure, which imposes strict energy thresholds and allows only certain transitions. Momentum conservation further shapes absorption behavior: direct band gap semiconductors allow efficient vertical transitions in momentum space, whereas indirect band gap materials require phonon assistance, leading to weaker absorption and distinct edge characteristics.137
In semiconductors, the energy landscape is more discrete and predictable (Fig. 2b). Each absorbed photon produces carriers with specific energies that can be directly aligned with the redox potentials of targeted reactions, offering a level of precision absent in plasmonic systems.53,139 Furthermore, the coulombic attraction between electrons and holes introduces spatial correlation, giving rise to excitons with characteristic sizes and lifetimes. Free charge carriers in inorganic semiconductors can persist from nanoseconds to microseconds before recombination, depending on trap density, doping, and dimensionality, a timescale that is orders of magnitude longer than the femtosecond dynamics of plasmonic hot carriers.
By contrast, semiconductor absorption is generally modest in intensity but offers distinct advantages. Near their band edge, semiconductor nanoparticles typically exhibit extinction coefficients in the range of 104–106 M−1 cm−1.107 While lower than plasmonic resonances, this absorption spans broader spectral ranges and is more strongly dictated by the band structure, yielding predictable energy thresholds and stable optical responses under varying surrounding conditions. Plasmonic nanomaterials exhibit absorption that is highly sensitive to their surrounding environment, with the peak position shifting as the dielectric properties of the medium change.152,154
Plasmonic nanoparticles generate intense electromagnetic fields, creating a localized intense electric field region that can enhance electric field intensity by factors of 102 to 103 compared to the incident light (Fig. 1b and c).151,152 This near-field enhancement emerges from the coherent oscillation of surface electrons, which creates regions of concentrated electromagnetic energy in the immediate vicinity of the nanoparticle surface. Unlike the uniform fields of plane waves, plasmonic near-fields are highly inhomogeneous, with intensity enhancement factors that can reach values of 104 to 106 at specialized locations called hotspots.151,159 These hotspots represent electromagnetic singularities where field enhancement reaches its maximum intensity. They typically occur at sharp features such as particle tips, edges, and corners where charge accumulation is highest, or in narrow gaps between closely coupled nanoparticles where fields from multiple sources constructively interfere.151,159 The spatial extent of plasmonic field enhancement decays extremely rapidly with distance from the nanoparticle surface. In most cases, the effect is confined to just 5–10 nanometers, creating an intensely localized activation zone. Molecules within this zone experience intense field enhancement, while those just slightly farther away remain virtually unaffected.158 This distance dependence has profound implications for catalytic selectivity. The plasmonic enhancement zone acts like a molecular spotlight, selectively activating surface-bound species while leaving solution-phase molecules untouched (Fig. 1b and c). This spatial selectivity can be exploited to control reaction pathways, enhance weak molecular transitions that would otherwise be optically inactive, and create catalytic hot zones with precisely defined dimensions.
Semiconductor photocatalysts operate with an entirely different field paradigm, generating built-in electric fields through band bending phenomena that extend much deeper into the material and persist even in the absence of illumination.16,25,26 When a semiconductor surface is exposed to an environment with a different chemical potential, charge redistribution occurs to achieve electrochemical equilibrium, creating space charge regions with associated static electric fields. The formation of these internal electric fields through band bending is a fundamental characteristic of the semiconductor systems, as shown by the example of upward and downward bending in an n-type semiconductor system (Fig. 3). While shown for an n-type semiconductor, similar electric fields also exist across various doping profiles and junction types in semiconductor systems.11 While these fields are generally weaker than plasmonic hotspots, they extend over much larger distances, depending on the doping concentration and surface conditions. These built-in fields serve multiple functions in semiconductor photocatalysis. They drive photogenerated electrons and holes in opposite directions, reducing recombination probability and enhancing charge separation efficiency. They modulate surface reactivity by altering the energetic positions of surface states, affecting both adsorption energies and reaction kinetics. They also create junction potentials at interfaces between different materials, providing additional driving forces for charge transfer and separation.11 Unlike the dynamic, light-dependent fields in plasmonic systems, semiconductor built-in fields are largely static, changing only slowly with variations in surface chemistry, temperature, or surrounding conditions.
In semiconductors, molecule coupling is primarily governed by energetic alignment with the band edges, whereas in plasmonic systems, coupling depends on both the energy of hot carriers and resonant interactions with the local electromagnetic field. The key requirement is that molecular energy levels align appropriately with semiconductor band edges to enable efficient charge transfer (Fig. 1a). CBM must lie at a higher electronic energy than the reduction level of the target species, while the VBM must lie at a lower electronic energy than the corresponding oxidation level.7,8,23 Surface states often serve as intermediates in semiconductor-molecule charge transfer, providing stepping stones that facilitate electron or hole transfer even when direct band-to-molecule transitions are energetically unfavorable. These surface states can be intrinsic features of the semiconductor crystal structure or extrinsic states created by surface defects, adsorbates, or chemical modifications. The built-in electric fields in semiconductors also influence molecular coupling by polarizing adsorbed species and stabilizing charged transition states.8,11 Thus, while plasmonic and semiconductor systems exhibit distinct temporal, spatial, and energetic behaviors, they operate through fundamentally related mechanisms of molecule–material interaction.
Semiconductor photocatalysts operate within their catalytic capabilities that are fundamentally constrained by the fixed positions of their band edges, which set absolute limits on the reducing and oxidizing power of photogenerated carriers (Fig. 1a).8,11 The thermodynamic driving force for each process scales with the energy difference between the band edge and the redox potential:
. This creates a rigid framework that determines which reactions are possible and which are forbidden. This thermodynamic constraint manifests in several practical limitations that have limited semiconductor photocatalysis. Wide-band gap semiconductors like titanium dioxide possess band edges positioned at highly favorable potentials for both water reduction and oxidation, making them excellent photocatalysts for water splitting. However, their large band gaps (3.2 eV for anatase TiO2) restrict them to ultraviolet absorption, capturing less than 5% of the solar spectrum and severely limiting their practical efficiency.20–22 Conversely, narrow-band gap semiconductors can harvest visible light but often suffer from unfavorable band edge positions. Materials like iron oxide (α-Fe2O3) absorb strongly in the visible region but possess a conduction band minimum that is insufficiently negative (vs. NHE) to reduce protons to H2 without an external bias or sacrificial electron donors.21 This fundamental trade-off between spectral coverage and thermodynamic driving force represents one of the central challenges in semiconductor photocatalyst design. The situation becomes even more complex when considering practical reaction conditions. Practical catalytic processes require overpotentials beyond the thermodynamic minimum to achieve reasonable reaction rates, further constraining the available energy window. Additionally, for metal oxide semiconductors, band edge positions shift by approximately −59 mV per pH unit due to surface protonation equilibria, a Nernstian response that creates pH-dependent constraints on thermodynamic driving forces.8,14
Plasmonic photocatalysts operate under an entirely different energetic paradigm. Rather than being constrained by fixed band positions, plasmonic systems generate hot carriers with a broad energy distribution that can potentially access multiple reaction pathways simultaneously (Fig. 2a).152,181,203 This energetic flexibility represents both plasmonics' greatest strength and its most significant challenge. The energy distribution extends well above the Fermi level, potentially reaching energies of several electron volts and enabling access to reaction pathways that would be kinetically challenging under equilibrium conditions. The LSPR frequency can be tuned across the visible and near-infrared spectrum through careful control of nanoparticle size, shape, and composition, enabling spectral matching with target reactions or optimization for specific solar irradiation conditions.151 This tunability extends to the hot carrier energy distribution itself, which can be modified through plasmon–molecule coupling or by engineering the local electromagnetic environment. However, this energetic freedom comes at a steep price. The broad energy distribution means that only a small fraction of hot carriers possesses the precise energy needed for any specific reaction, leading to inherent inefficiencies in energy utilization. Moreover, the rapid thermalization of hot carriers through electron–electron and electron–phonon scattering creates a fierce competition between energy utilization and energy dissipation.165
Plasmonic energy conversion, in contrast, operates in highly non-equilibrium, transient regimes where different processes occur on vastly different timescales. Plasmon excitation and dephasing occur within femtoseconds, hot carrier generation proceeds on timescales of 1–100 femtoseconds, thermalization occurs within picoseconds, and chemical reactions may require nanoseconds to microseconds for completion.154,161,165 This temporal mismatch creates fundamental challenges in energy utilization that cannot be addressed through conventional optimization approaches. The transient nature of plasmonic processes demands entirely different optimization strategies focused on accelerating beneficial processes or slowing detrimental ones. Hot carrier injection must be accelerated through improved energy alignment and stronger coupling.161,230 Thermalization can be slowed through quantum confinement effects or by creating energy bottlenecks in the electronic structure. Chemical reactions can be accelerated through field enhancement or by pre-activating reactant molecules through surface chemistry. Efficient transfer of hot electrons can be achieved by creating “antenna–reactor” catalysts.220,248
A semiconductor typically operates under a quasi-steady-state population under continuous illumination, where photoexcitation generates electron–hole pairs that can be spatially separated by built-in electric fields or junctions. These moderate fields, combined with surface states, can stabilize charged transition states or provide alternative reaction pathways with slightly lowered activation barriers.32,54 Plasmonic systems, while relying on the same fundamental electron transfer principle, can provide additional, transient contributions due to intense local electromagnetic fields and thermal effects.170 Hot carriers can directly populate antibonding orbitals, while near-field enhancements and transient local heating can temporarily increase the effective energy available to adsorbed molecules. Vibrational excitation may also play a role, enhancing certain molecular motions and subtly steering reactions toward specific pathways.253,286
In essence, the underlying electron-transfer mechanism is shared between semiconductors and plasmonics. The apparent differences largely arise from the magnitude, localization, and temporal profile of the excitation: plasmonic systems often provide higher-energy, ultrafast, and spatially concentrated stimuli, whereas semiconductors offer more moderate but sustained activation.
When semiconductor dimensions shrink to approach the exciton Bohr radius, which ranges from ∼1 nm (e.g., ZnO) to over 30 nm (e.g., InAs, PbS) depending on the material, quantum confinement effects begin to dominate, fundamentally restructuring the electronic landscape and optical properties. This quantum size effect represents one of the most powerful tools in semiconductor photocatalyst design, enabling precise control over band gaps, absorption spectra, and redox potentials through simple size manipulation.10 The implications of quantum confinement extend far beyond simple spectral tuning. Size reduction increases the overlap between electron and hole wavefunctions, enhancing oscillator strength and improving light absorption efficiency.10 The density of states transforms from continuous (3D bulk) to increasingly discrete (2D, 1D, 0D), creating atomic-like energy levels in the smallest nanocrystals (Fig. 4). Most importantly for photocatalysis, quantum confinement shifts band edge positions, enabling fine-tuning of redox potentials to match specific reaction requirements.10
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| Fig. 4 Schematic representations of the density of states (DOS) as a function of energy for semiconductor crystals in different dimensions: (a) 3D bulk, (b) 2D, (c) 1D, and (d) 0D. | ||
This size-energy connection provides semiconductor photocatalysts with remarkable design flexibility. A single material composition can be optimized for different reactions simply by controlling particle size during synthesis. Larger particles provide stronger light absorption and lower band gaps for visible light harvesting, while smaller particles offer higher energy carriers and more favorable redox potentials for challenging reactions. The ability to independently tune spectral response and energetic driving force represents one of semiconductor photocatalysis's greatest advantages. However, quantum confinement also introduces new challenges. Smaller particles exhibit increased surface area-to-volume ratios, leading to higher densities of surface defects that can act as recombination centers. The discrete energy levels in quantum dots can create energy bottlenecks that impede charge transport and extraction. Surface chemistry becomes increasingly important as surface atoms constitute larger fractions of the total particle, potentially altering electronic structure and catalytic behavior in unpredictable ways.
Plasmonic nanoparticles exhibit size-dependent properties that can be understood within classical electrodynamics for particles larger than approximately 2 nanometers. Unlike the quantum mechanical origins of semiconductor size effects, plasmonic size dependence emerges from classical electromagnetic phenomena, including retardation effects, surface scattering, and the balance between radiative and non-radiative decay pathways.151 As plasmonic particles grow larger, several competing effects come into play. Retardation effects become significant when particle dimensions approach the wavelength of light, causing red shifts in LSPR frequency and changes in field distribution patterns. Radiative damping increases with particle size, becoming the dominant loss mechanism for particles larger than approximately 100 nanometers. While this radiative loss reduces the local field enhancement, it can actually improve far-field scattering efficiency, making larger particles more effective for light-scattering applications. For smaller particles below approximately 10–20 nm, where particle dimensions become comparable to or smaller than the bulk electron mean free path (∼38 nm for Au, ∼52 nm for Ag), surface scattering becomes increasingly important, contributing additional damping.151 This surface scattering broadens LSPR linewidths and can shift resonance frequencies, but it also enhances hot carrier generation by increasing the probability of electron-surface interactions that break momentum conservation. The optimization of plasmonic particle size represents a delicate balancing act between competing factors. Intermediate sizes (50–80 nm for gold) often provide optimal field enhancement by balancing strong absorption with manageable damping losses. Smaller particles favor hot carrier generation and chemical interface damping, while larger particles excel in far-field applications and radiative processes. Unlike semiconductors, where quantum confinement provides a clear size–property relationship, plasmonic optimization requires careful consideration of the specific application and the relative importance of different enhancement mechanisms.
This exploration of fundamental comparison between semiconductor and plasmonic photocatalysts reveals not competing paradigms, but complementary approaches to solar energy conversion that can be synergistically combined to transcend the limitations of either system alone. Semiconductors offer the precision of quantum mechanics, discrete energy levels, predictable thermodynamics, and long-lived charge carriers that enable sustained catalytic processes. Plasmonic systems provide the power of collective excitation, intense electromagnetic fields, thermal effects, broad energy distributions, and ultrafast dynamics that can access high-barrier reactions and utilize the full solar spectrum. It should be noted, however, that these distinctions represent general trends rather than rigid boundaries, and exceptions exist where systems display properties that extend beyond this broad framework. The path forward lies not in choosing between these approaches, but in understanding how their distinct strengths can be combined to create architectures that combine controlled charge dynamics with strong optical field enhancement. The following sections will explore how these fundamental principles translate into catalytic applications and examine the emerging strategies for creating next-generation photocatalytic systems that integrate plasmonic and semiconductor functionalities.
From a fundamental chemical perspective, these three reactions serve as the ultimate benchmarks for catalytic performance because they involve the activation of some of the strongest chemical bonds found in nature. The thermodynamic stability of the C
O bond in CO2, the C–H bond in CH4, and the formidable N2 triple bond (941 kJ mol−1) creates kinetic barriers that are largely insurmountable for traditional catalysts at ambient temperatures. Mastering these transformations requires more than simple energy transfer; it demands the precise management of multi-electron and multi-proton pathways. These molecules, therefore, represent the most rigorous test of a photocatalyst's ability to manipulate high-energy transition states and control product selectivity in stable molecular species.
Furthermore, these reactions provide an ideal platform for comparing the distinct operational regimes of semiconductor and plasmonic architectures. Driving these high-barrier transformations necessitates winning the temporal race against charge relaxation, utilizing strategies such as hot-carrier injection, localized near-field enhancement, and defect-mediated molecular activation. By examining the nuances of CO2 reduction, DRM, and N2 reduction, we can evaluate how different photocatalytic systems utilize excited charge carriers to override traditional thermal limits.
The sunlight-driven reduction of CO2 by H2O is particularly promising for scalable energy storage and carbon-neutral production of high-energy fuels, with O2 as the by-product.440,450 However, this process is challenged by low efficiency and poor product selectivity, especially for high-value chemicals. Low efficiency is often due to the use of wide-band gap semiconductors that absorb only ∼4% of the solar spectrum (UV light) and suffer from high charge carrier recombination rates. An alternative reducing agent to H2O is molecular H2, which has a lower oxidation potential and helps avoid these issues.451,452
To improve the charge transfer efficiency in CO2 reduction, various strategies have been developed, such as cocatalyst loading, heterojunction fabrication, interface activation, and surface catalytic site engineering. Engineering surface catalytic sites can extend light absorption, improve the separation of photogenerated electrons and holes, and thus facilitate surface redox reactions. For example, introducing spatially separated catalytic sites (cocatalyst) can enhance charge carrier transfer and surface redox reactions (Fig. 5a). Li et al.453 prepared copper–cobalt dual catalytic site porous TiO2, where Cu sites acted as reductive sites and Co sites as oxidative sites. The spatial separation of reactive sites on TiO2's surface significantly promoted charge separation during catalytic reactions.
Fabricating heterostructure catalysts with favorable band alignment is also effective for achieving broad spectral responses and efficient charge separation. Depending on charge transfer directions, heterostructure catalysts are categorized as p–n junctions or Z-schemes.454–458 In a p–n junction, photo-generated electrons are injected into the component with a lower CB edge, while photo-generated holes migrate to the component with a higher VB edge (Fig. 5b). In contrast, in a Z-scheme architecture, photo-generated electrons in the component with a lower CB edge recombine with holes in the component with the higher VB edge, either directly or indirectly, using a conductive intermediate or reversible redox shuttle (Fig. 5c).
Moreover, heterogeneous photocatalytic CO2 reduction can also be carried out over metal catalysts like gold, silver, copper, and bismuth, mainly due to the LSPR effect.459–461 Hot charge carriers are formed through intraband s-to-s or interband d-to-s transitions after the decay of LSPR (Fig. 5d). Both the local heat and hot charge carriers can contribute to CO2 reduction.
Different strategies have been carried out to increase the lifetime of these charge carriers in both semiconductor and plasmonic photocatalysts. In oxide semiconductors, defect creation in the form of O vacancies offers dual advantages by offering trap sites for electrons and introducing mid-gap states, broadening the absorption spectrum of the semiconductors. For CO2 reduction, they can be critical for activating CO2 molecules or can help in stabilizing semiconductor and cocatalyst interfaces by special phenomena like strong metal–support interactions (SMSI). For example, black TiO2 with dual active sites (Ni NPs and oxygen defects) was synthesized by Chen et al.462 Surface dual sites acted as the binding sites of the CO2 molecule and lowered its activation energy, while oxygen defect sites also trapped the electron and narrowed the band gap of TiO2, collectively resulting in an 18-times higher acetaldehyde production than that catalyzed by P25. One such study by Ozin et al.463 focuses on the exploitation of O vacancy defects in In2O3 semiconductor nanoparticles for photothermal CO2 hydrogenation (Fig. 6). The pale yellow In2O3 powder was converted to pitch-black by controlling its non-stoichiometry through hydrogen treatment at elevated temperatures (Fig. 6a). The optical reflectance spectra (UV-Vis-NIR) for S1–S4 showed a trend of gradually increasing absorption, broadening and red shifting of the ultraviolet absorption edge into the visible region with higher temperatures of the hydrogenation (Fig. 6b). High resolution transmission electron microscopy (HRTEM) confirmed the formation of these heterostructures having amorphous indium oxide In2O3−x interfaced with crystalline indium oxide In2O3 (Fig. 6c and d), which enabled the photothermal reverse water gas shift (RWGS) reaction with 100% selectivity. X-ray photoelectron spectroscopy (XPS) analysis revealed that oxygen vacancies increased with hydrogenation temperature, with S2, S3, and S4 corresponding to In2O2.8, In2O2.7, and In2O2.63, respectively (Fig. 6e). The black In2O3−x/In2O3 exhibited a CO production rate nearly three orders of magnitude higher than the yellow In2O3 under light, reaching 1874.62 µmol h−1 m−2 (Fig. 6f). Based on the enclosed thermocouple, the temperatures of S1–S3 are lower than 50 °C, and about 160 °C for S4. The local temperatures of all samples were estimated from the conversion of CO2 to CO (yield, ppm), where S4 was found to be 262 °C in contrast to S1–S3 which were found to have much lower local temperatures (Fig. 6g). The effect of oxygen vacancies on CO2 binding was analyzed using in situ diffuse reflectance infrared Fourier transform spectroscopy (DRIFTS) where a reaction pathway involving the CO2 insertion and regeneration of oxygen vacancies was proposed (Fig. 6h). Photoconductivity measurements under vacuum and experimental conditions for S1 and S4 were performed to study the dynamics of photoexcited carriers.
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Fig. 6 Photocatalytic CO2 hydrogenation over single-component In2O3−x. (a) Color changes from pale yellow to grey to black observed on hydrogenating stoichiometric In2O3 at 200, 300, 400 °C to form non-stoichiometric In2O3−x with monotonically increasing values of x with temperature, (b) optical reflectance spectra (UV-Vis-NIR), (c) STEM, and (d) HRTEM images of S4 at different magnifications. A dashed green circle indicates an amorphous phase, yellow arrow indicates the measured lattice spacing and the red square indicates the imaged position, (e) high-resolution O 1s core level XPS spectrum of S4, (f) photocatalytic CO2 hydrogenation in a batch reactor. (g) Catalytic performance for S4 in a flow reactor at different temperatures, both with and without light irradiation, inset is the enlarged view of the catalytic performance for 200, 225, and 250 °C, (h) in situ DRIFTS spectra of S4 obtained under both H2 and CO2 (1 : 1) with increased temperatures, (i) photocurrent saturation and decay plot, (j) corresponding in situ I–V plot, (k) the In2O3−x/In2O3 heterostructure showing the In(III)′, [O] electron-trapping and O′ hole-trapping mid-gap energy states near the CB and VB edges, respectively. Reproduced with permission from ref. 463. Copyright 2020 Springer Nature. | ||
The much faster photo-saturation of the excited electrons for S4 implied a stronger optical absorbance for S4 than S1. While the light was off, the photocurrents of S1 and S4 slowly decayed, with S4 requiring a much longer decay time than S1, which implied a higher population of oxygen vacancy traps for photoelectrons (Fig. 6i). The longer lifetime of the detected photoelectrons also meant a higher probability for the photoexcited electrons to participate in the reaction and thereby results in a better catalytic performance for S4. The same trend was observed under vacuum conditions, and the resulting I–V plot further confirmed the prolonged lifetime of photoexcited electrons for S4 (Fig. 6j). The oxygen vacancies [O] and coordinately unsaturated indium In′ sites and oxygen O′ sites in In2O3−x existed as mid-gap defect states in the band gap of In2O3.107,464 These states were shown to be respectively situated near the oxide-based valence band and indium-based conduction band, with the charge-balancing electrons occupying mid-gap states and aiding in the separation of electron–hole pair and therefore facilitating photochemical conversion of CO2 to CO (Fig. 6k).
It should be noted that the nature of defect sites is critical to determine the selectivity of the reaction, as it can change the charge carrier dynamics as well as the surface activity. In another report, when the defects were introduced in In2O3 using NaBH4 instead of thermal treatment in an H2 environment, the catalyst was hydroxy-terminated, leading to shifting the reaction pathway towards methanol.465
To enhance the efficiency of single-component semiconductors, various strategies such as forming heterojunctions between semiconductors and loading metal cocatalysts are employed. In a study by Li et al.,466 graphdiyne (GDY)-modified In2O3 hybrid photocatalysts (denoted as GDY-IO) were synthesized using simple electrostatic attraction and thermal annealing methods (Fig. 7a). The GDY-IO composites not only showed significantly improved photocatalytic activity in the production of CO and CH4 but also enabled the formation of C2+ hydrocarbons (such as C2H4, C2H6, C3H6, and C3H8) under atmospheric conditions. The introduction of GDY promoted the separation of excited carriers and enhanced the adsorption and activation of CO2, which significantly lowered the kinetics barrier for CH* formation and favored hydrogenation and C–C coupling processes. TEM analysis revealed that the intimate two-phase interfacial contact between highly crystallized In2O3 and the amorphous GDY region (Fig. 7b and c) effectively improved interfacial charge transfer during the photocatalytic reaction.
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| Fig. 7 Photocatalytic CO2 hydrogenation over GDY-IO utilizing heterojunction. (a) Schematic illustration of the synthetic process for GDY-IO composites, (b) TEM and (c) HRTEM images of 0.4% GDY-IO composites, (d) high-resolution In 3d spectra and (e) O 1s spectra of In2O3 and 0.4% GDY-IO composite, (f) UV-Vis DRS spectra of In2O3, GDY, and GDY-IO composites, (g) density of states of In2O3 before and after contact with GDY, (h) products of photocatalytic CO2 reduction on various catalysts, (i) time-resolved photoluminescence observed from selected red frames on single In2O3 particle, single 0.4% GDY-IO particle, and single 0.4% GN-IO particle, (j) transient photocurrent response curves, (k) schematic diagram for the electron transfer and the formation of built-in electric field between In2O3 and GDY upon their contact, and the holes transfer between In2O3 and GDY after light irradiation. Reproduced with permission from ref. 466. Copyright 2024 Elsevier. | ||
High-resolution In 3d XPS spectra of In2O3 showed two peaks corresponding to In 3d5/2 and In 3d3/2. Notably, after coupling GDY with In2O3, these In 3d peaks shifted to higher binding energies compared to those of pristine In2O3 (Fig. 7d). A similar shift was observed in the O 1s spectra, indicating electron transfer from In2O3 to GDY upon contact (Fig. 7e). Furthermore, electron paramagnetic resonance (EPR) signals at the g-value of 2.003, along with O 1s XPS, demonstrated that the GDY-IO possessed a higher concentration of oxygen vacancies (Ov) than pristine IO. Notably, heterojunction fabrication between GDY and IO helped to improve the visible light absorption of In2O3 (Fig. 7f). Additionally, a significant decrease in the integrated density-of-states (DOS) in In2O3 after contact with GDY was observed, implying accelerated electron mobility from In2O3 to GDY (Fig. 7g).
The pristine In2O3 catalyzed both the RWGS reaction and the methanation reaction, producing CO and CH4 as primary products. Interestingly, the GDY-IO composites exhibited a different product distribution under the same reaction conditions, generating not only CO and CH4 but also C2+ hydrocarbons (C2H4, C2H6, C3H6, and C3H8) during the photocatalytic process (Fig. 7h). The GDY-IO composites showed negligible thermal effects since the photocatalytic performance tests were conducted at room temperature, with the final bulk reaction temperature below 120 °C.
The combination of GDY with In2O3 led to the weakest photoluminescence (PL) emission peak, likely due to the increased concentration of oxygen vacancies introduced by GDY, which provided more traps for capturing electrons and preventing electron–hole recombination. Consequently, the GDY-IO sample exhibited a longer transient fluorescence lifetime (∼11 ns) compared to pristine In2O3 (∼5.1 ns) and GN-IO (∼8.5 ns) (Fig. 7i). Transient photocurrent response (Fig. 7j) and electrochemical impedance tests collectively indicated that the introduction of GDY indeed facilitated charge carrier separation. The combined in situ DRIFTS and density functional theory (DFT) results demonstrated that introducing GDY into In2O3 enhanced CO2 adsorption and activation, leading to electron enrichment on the In2O3 surfaces near the oxygen vacancies, which together stabilize reaction intermediates and promote C–C coupling reactions.
Based on these observations, an electron transfer mechanism was deduced (Fig. 7k). When In2O3 and GDY were in contact, electrons transferred from In2O3 to GDY to reach the same Fermi level, creating a built-in electric field. Under light irradiation, the photogenerated holes from In2O3 were driven to transfer to GDY by the built-in electric field, while the photogenerated electrons were captured by the abundant surface oxygen vacancies in In2O3. As a result, the separation and transfer of photogenerated carriers in the GDY-IO composite are significantly improved. Most importantly, the photogenerated electrons in In2O3 migrated and accumulated at the surface oxygen vacancies, providing a high surface charge density to overcome the C
O activation and C–C coupling energy barriers, facilitating the transformation of CO2 into C2+ hydrocarbons.
To enhance charge separation in photocatalysts, in addition to strategies like defect creation and heterojunction fabrication, noble metal loading is a simple and effective method. The nature of metal-support interfaces and their electronic structure critically governs photocatalytic activity through strong metal-support interactions, plasmon-driven light-matter coupling, and charge-carrier trapping and transport dynamics in heterogeneous systems.467–470 In a study by Liu et al.,467 a series of TiO2-supported palladium photocatalysts were synthesized using a glucose reduction method (Fig. 8). These photocatalysts exhibited high activity for the photocatalytic hydrogenation of CO2, with a notable selectivity towards CH4 formation. Pure TiO2 consisted of spherical aggregates of small subparticles, uniform in size and shape, with nanoparticles averaging 30–40 nm in diameter. High-resolution TEM images revealed that palladium nanoparticles had a diameter of 3 nm, with lattice spacings corresponding to the (004) plane of anatase TiO2 and the (200) plane of Pd (Fig. 8a). As Pd loading increased, the samples exhibited improved optical responses, with absorbance in the 380–700 nm range significantly higher than that of pure TiO2, attributed to the LSPR of Pd nanoparticles (Fig. 8b). The band gap energy of pure TiO2 was estimated at 3.27 eV, but after Pd loading, the absorption edge shifted, reducing the Eg value to 3.06 eV for 1.5 wt% Pd/TiO2 (Fig. 8c). The photoluminescence intensity decreased with increasing palladium loading (up to 1.0 wt%), indicating improved charge separation and reduced recombination of photogenerated charges on the Pd-loaded TiO2 surface (Fig. 8d). However, for Pd loadings above 1.0 wt%, PL intensity increased again, which was attributed to the formation of new recombination centers by excess palladium. XPS spectra revealed that PdO was also formed during catalyst preparation and storage, with a slight shift in the PdO peaks for the used catalyst (Fig. 8e), possibly due to the formation of Pd–C, as suggested by the increased C 1s area. When photocatalytic CO2 hydrogenation was performed under batch conditions, CH4 was the main product, along with some CO and C2H6. The yields of these products increased with Pd loading up to 1.0 wt%, with the highest yields of CH4, CO, and C2H6 being 355.62, 46.35, and 39.69 µmol g−1, respectively, after 3 hours of irradiation (Fig. 8f). Excessive Pd loading reduced yields, possibly due to new recombination centers or a shielding effect that inhibited light harvesting.
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| Fig. 8 Photocatalytic CO2 hydrogenation over Pd/TiO2 semiconductor-cocatalyst system. (a) HRTEM image of Pd/TiO2, (b) UV-Vis absorption spectra of TiO2 and Pd-loaded TiO2 samples, (c) plot of (αhν)2 vs. photon energy (hν) for the direct optical band gaps of TiO2 and Pd-loaded TiO2, (d) PL spectra of TiO2 and Pd/TiO2 measured at an excitation wavelength of 325 nm, (e) X-ray photoelectron spectra of 1.0 wt% Pd/TiO2 catalyst Pd 3d region, (f) relationship between the products and the loading amount of Pd after irradiation for 3 h, (g) change in temperature with irradiation time, (h) relationship between the yield of CH4 and the reaction time using 1.0 wt% Pd/TiO2 catalyst with different light sources, (i) schematic illustration of charge transfer over Pd/TiO2 during the photoreaction. Reproduced with permission from ref. 467. Copyright 2017 American Chemical Society. | ||
To investigate the effect of light, experiments were conducted in the dark at 130 °C, which corresponded to the temperature reached under light illumination (Fig. 8g), and under visible light yielded only small amounts of CH4, indicating that Pd-loaded TiO2 was primarily active under UV light (Fig. 8h), as supported by UV-Vis spectra. These findings demonstrated that the photocatalytic hydrogenation of CO2 was driven by a synergistic effect between the metal and the support. Based on these observations, a reaction mechanism was proposed: Upon UV light exposure, TiO2 absorbed energy greater than or equal to its band-gap energy, generating photogenerated electron–hole pairs. Electrons in the CB and holes in the VB were partially transferred to the surface, where the electrons migrated to adjacent Pd nanoparticles. These electrons combined with chemisorbed CO2 to form CO2−, enhancing charge separation and inhibiting recombination. The holes in the VB of TiO2 were captured by reactive atomic hydrogen, forming H+, which was dissociated at Pd sites by combining with electrons. Activated CO2 molecules at Pd sites reacted with H+ and electrons to produce the intermediate Pd–C
O. This intermediate could either desorb as CO or further react with dissociated H to form Pd–C, which then reacted with more H species to produce CH4 (Fig. 8i).
Photo-thermal catalysis, which relies on the simultaneous action of light and heat, inevitably exposes materials to high temperatures where several intrinsic limitations arise. As discussed earlier in Section 3.2, efficient charge separation can be achieved due to the presence of a built-in electric field within semiconductor materials. However, under elevated temperatures (>300 °C), accelerated lattice vibrations induce thermal quenching of photogenerated carriers, structural stability becomes compromised, and surface-defect-mediated recombination is significantly intensified. Ferroelectric semiconductors offer a potential solution because their spontaneous polarization provides an internal electric field that can drive carrier separation, yet this advantage weakens at high temperatures due to inherently limited polarization strength and polarization collapse near the Curie temperature. These challenges require the need for strategies that stabilize ferroelectric polarization and suppress both bulk and surface recombination under harsh photo-thermal operating conditions. In a recent study by Kuang et al.,70 the authors harnessed the same built-in electric field of a semiconductor material to increase the efficiency of the photo-thermal CO2 hydrogenation reaction. In their work, they used a ferroelectric PbTiO3 material that has a spontaneous polarization in it, and they did surface modification to increase the polarization effect to their advantage. They first synthesized cuboidal PbTiO3 nanoparticles (PTO) by hydrothermal synthesis (Fig. 9a). The morphological and crystallinity characterizations of PTO revealed a brick like structure with exposed {001} facets on its top/bottom surfaces and {100} facets on the other four lateral facets. The intrinsic ferroelectric polarization electric field of PTO is oriented along the [001] direction (c-axis), hence the polarization direction of the synthesized PTO was perpendicular to its top/bottom surfaces (Fig. 9b). The measured ferroelectric characteristics of the PTO was found out to be, d33 = 38.2 pm V−1 with characteristic butterfly-shaped amplitude hysteresis and a phase reversal by piezoelectric force microscopy (PFM) (Fig. 9c). The COMSOL simulation model simulated the polarization electric field strength of PTO (Fig. 9d), suggesting a electric field of up to 0.7 × 10−2 V can be spontaneously generated within PTO. This spontaneous polarization electric field in PTO directed the photogenerated carrier toward opposite polarity (001) crystal surfaces, thereby inhibiting the carrier recombination in the bulk phase.70
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| Fig. 9 Ferroelectric polarization and surface engineering for enhanced photo-thermal CO2 hydrogenation. (a) TEM image, (b) schematic of the direction of polarization electric field, (c) amplitude and phase hysteresis loops, (d) COMSOL simulated polarization electric field, of pure PTO, (e) amplitude and phase hysteresis loops of 2%-PTPO, (f) thermal (400 °C)/photo-thermal coupled (400 °C, light intensity = 20 mW cm−2) CO2 hydrogenation performance of pure PTO and x%-PTPO (x = 1, 2, 3), (g–i) TRPL spectroscopy of pure PTO, 2%-PTPO, and PR-Au/MnOx-2%-PTPO, respectively, (j) thermal (400 °C)/photo-thermal coupled (400 °C, light intensity = 20 mW cm−2) catalytic CO2 hydrogenation performance of PR-Au/MnOx-2%-PTPO and its control samples, (k) continuous photo-thermal coupled catalytic CO2 hydrogenation testing of PR-Au/MnOx-2%-PTPO. Reproduced with permission from ref. 70. Copyright 2025, Wiley-VCH GmbH. | ||
However, the next challenge was to enhance and preserve this polarization at high temperatures. To achieve this goal, the authors doped Pt into the PTO by adding Pt precursor in the hydrothermal synthesis of PTO, forming PTPO. The choice of Pt was based on its ionic radius, which closely matches Ti4+ and allows substitution-induced lattice distortion to enhance polarization, as well as its electronic configuration, which introduces additional energy states that promote charge localization and provide multiple transport pathways for photogenerated carriers. Pt doping was found to leave the brick-like morphology and textural properties of PTO largely unchanged, yet it introduced notable structural and electronic modifications. XRD and EPR analyses collectively showed that Pt2+ substitutes Ti4+ sites in the [TiO6] octahedra and simultaneously generates oxygen vacancies, leading to lattice distortion along the polar c-axis. This distortion is most pronounced at 2% Pt, which correlates with the strongest enhancement of ferroelectric polarization. PFM measurements show an increase in the effective piezoelectric coefficient from 38.2 pm V−1 in pure PTO to 57.2 pm V−1 in 2%-PTPO, confirming polarization amplification (Fig. 9e). In addition, Pt-induced impurity states cause a red-shift in optical absorption and reduce the band gap, while preserving the n-type semiconductor nature of PTO.
The PTPO and PTO were then tested for CO2 hydrogenation reaction in flow. Catalytic testing showed that Pt doping had virtually no effect on the thermocatalytic CO2 hydrogenation performance, with Pt-doped PTO and pristine PTO exhibiting nearly identical activity under heat-only conditions (Fig. 9f). However, under photo-thermal operation, Pt doping produced a pronounced enhancement, with 2%-PTPO delivering the highest CO2 conversion efficiency of 66.7 mmol g−1 h−1 CO and 3.6 mmol g−1 h−1 CH4, a 2.2-fold enhancement in electron transfer efficiency compared to pure PTO (Fig. 9f). Since thermocatalysis depends mainly on surface chemistry, the unchanged thermal performance indicates that Pt does not significantly alter surface-active sites. In contrast, the improvement under photo-thermal conditions reflects Pt-induced polarization amplification, which promotes more efficient photogenerated carrier separation.
While Pt doping enhanced internal polarization, the lack of active surface sites and the prevalence of surface carrier recombination remain significant bottlenecks. To address these, the authors leveraged the intrinsic ferroelectric properties of 2%-PTPO to drive the facet-selective photodeposition of dual cocatalysts. By utilizing the spontaneous polarization of the PTO matrix, photogenerated electrons and holes were directionally migrated to opposing {001} facets, allowing for the spatial isolation of Au nanoparticles (electron traps) and MnOx nanosheets (hole traps). This strategic placement transformed the crystal into a spatially isolated redox system, preventing the recombination of charge carriers at the surface. The synergy between Pt doping and dual-cocatalyst loading significantly optimized the thermodynamic and kinetic profiles of the catalyst. DFT calculations and in situ XPS confirmed that the inclusion of Au and MnOx not only lowers the CO2 adsorption energy, from −0.27 eV in pure PTO to a much more favorable −2.57 eV in the dual-loaded system, but also acts as a powerful driving force for charge transfer. Comprehensive carrier dynamics studies, including in situ Kelvin probe force microscopy, time-resolved photoluminescence (TRPL), and temperature-dependent PL, provide quantitative evidence for this enhanced performance.
Photoluminescence spectroscopy revealed that the exciton binding energy, a key indicator of recombination probability, dropped dramatically from 216.7 meV in pure PTO to just 103.6 meV in the PR-Au/MnOx-2%-PTPO system. This reduction was mirrored in the TRPL data, where the average carrier lifetime increased from 5.6 ns to 14.8 ns (Fig. 9g–i). Furthermore, in situ XRD and high-temperature catalytic testing demonstrated that Pt doping elevates the Curie temperature from 550 °C to 650 °C. This ensured that the material retains its crucial ferroelectric tetragonal phase at elevated reaction temperatures, maintaining the polarization-led carrier separation necessary for high-efficiency solar-to-fuel conversion.
The catalytic performance of the PR-Au/MnOx-2%-PTPO system demonstrated the practical success of this bulk-surface engineering strategy, particularly in demanding high-temperature environments. At 400 °C, the optimized catalyst achieved a remarkable photo-thermal coupled CO2 conversion rate of 140.8 mmol g−1 h−1, significantly outperforming its mono-cocatalyst and unmodified counterparts while maintaining exceptional structural integrity over a 24-hour stability test (Fig. 9j and k). Most notably, the catalyst excels where traditional ferroelectrics fail; while pure PTO experienced a decline in photo-activity at 550 °C due to a ferroelectric-to-paraelectric phase transition, the Pt-doped samples retain their tetragonal phase and spontaneous polarization up to 650 °C. Consequently, at 550 °C, PR-Au/MnOx-2%-PTPO delivers a CO2 conversion rate of 235.7 mmol g−1 h−1 for CO, nearly double the efficiency of its purely thermal catalytic performance, proving that Pt doping effectively extends the operational temperature window for ferroelectric-enhanced catalysis.
Ultimately, this study highlights how the built-in electric field, as a fundamental property inherent to a material's crystal structure and electronic alignment, can be precisely exploited to overcome the most persistent kinetic challenges in complex chemical reactions. It underscores that by tailoring internal polarization alongside surface architecture, one can harness the internal electronic forces of ferroelectrics to drive high-performance solar-to-fuel conversion.70
Apart from acting as cocatalysts and increasing the electron–hole separation in semiconductors, metals can also act as light harvesters and form hot charge carriers through LSPR, which can further boost the catalytic performance. In a study by Liu et al.,471 plasmonic Rh nanoparticles demonstrated significant photocatalytic properties by reducing activation energies and exhibiting strong product photo-selectivity in CO2 hydrogenation reactions (Fig. 10). This design exemplifies a supported plasmonic metal on an insulating oxide, where the metal nanostructures function as bifunctional centers for both photon harvesting and surface catalysis. The Rh photocatalyst, consisting of 37 nm Rh nanocubes (Fig. 10a) dispersed on Al2O3 with a 1.02% mass loading (Rh/Al2O3), showed that under mild illumination, the activation energies for CO2 hydrogenation were lowered by approximately 35% compared to thermal activation energies (Fig. 10e and f). Specifically, the selectivity for CH4 over CO was remarkably enhanced, achieving over 86% under blue light and more than 98% under UV light, with reaction rates doubling the thermocatalytic rates at 350 °C.
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Fig. 10 Plasmon driven selectivity for CO2 hydrogenation over Rh/Al2O3 photocatalyst. (a) TEM images of the Rh/Al2O3 photocatalyst. Scale bar, 100 nm (inset: 25 nm), (b) extinction spectra of rhodium nanocubes, (c) selectivity towards CH4 of the thermo- (black circles) and photocatalytic reactions under ultraviolet (365 nm, red squares) and blue (460 nm, blue triangles) illumination as a function of temperature under H2-rich (CO2 : H2 = 1 : 5.5, solid symbols) and H2-deficient (CO2 : H2 = 1 : 3.1, open symbols) conditions. (d) rates of CH4 photo-production as a function of ultraviolet light intensity at 623 (black squares) and 573 K (red circles). (e) Thermocatalytic reaction rates of CH4 (black squares) and CO (red circles) production on Rh/Al2O3 as a function of temperature, (f) photoreaction rates for CH4 production on Rh/Al2O3 under 1.18 (black squares), 0.59 (red circles) and 0.24 W cm−2 (blue triangles) ultraviolet illumination as a function of temperature, (g) rates of CH4 (green) and CO (black) production at 623 K on Rh/Al2O3 or Au/Al2O3 (solid lines) and Al2O3 (dotted lines) under dark and ultraviolet illumination at 3 W cm−2, (h) the thermocatalytic reaction activates both CO–Rh bonds and CH–O bonds to produce CO and CH4, respectively. Reproduced with permission from ref. 471. Copyright 2017 Springer Nature. | ||
The Rh nanocubes, with precisely tunable size and LSPR wavelength, had sharp corners that concentrated light and liberated hot carriers. The study found that the LSPR of Rh nanocubes, which was 334 nm (3.71 eV) in ethanol, was broadened and blue-shifted when placed on porous Al2O3 (Fig. 10b). Unlike Au nanoparticles, which produced only CO regardless of illumination, Rh nanoparticles exhibited high selectivity towards CH4 production only under illumination (Fig. 10g). This difference arose because the weaker oxygen binding on Au surfaces prevented C–O bond cleavage in CHO intermediates, whereas the stronger O adsorption energy on Rh stabilized these intermediates and enabled their dissociation toward CH4 formation.471
Dark thermocatalytic reactions on Rh nanoparticles showed moderate selectivity with a CH4 ratio of approximately 60
:
40 across different temperatures and reaction rates. However, under UV illumination, the CH4 production rate was significantly enhanced, with a photo-selectivity exceeding 95% (Fig. 10c). This high selectivity persisted even under H2-deficient conditions during illumination but dropped in the dark, indicating that the selective production of CH4 was driven by light rather than thermal effects or excess H2.
The study confirmed that the high photo-selectivity was not due to local heating but was attributed to the selective activation of CHO intermediates by plasmon-generated hot electrons. Under UV illumination at ∼1 W cm−2, the reaction rate showed a super-linear dependence on light intensity, with an exponent of n = 2.1 at 623 K and 2.4 at 573 K, suggesting multiple excitations of vibrational modes by hot electrons (Fig. 10d). The reaction kinetics of CO2 hydrogenation on Rh and Au photocatalysts were investigated, revealing that the activation energy (Ea) for CH4 production under UV light was reduced to 50.4 kJ mol−1 compared to 78.6 kJ mol−1 under thermocatalytic conditions. This reduction in Ea was also observed for CO production on the Au photocatalyst, decreasing from 55.8 kJ mol−1 in the dark to 39.5 kJ mol−1 under visible light.
They concluded that the transfer of hot electrons from plasmonic metal nanoparticles to specific intermediates selectively activates certain reaction pathways by interacting with anti-bonding orbitals, thus providing a method to control the selectivity of catalytic processes. In contrast, in thermocatalytic reactions, phonons activate both CHO and CO intermediates, leading to comparable production rates of CH4 and CO on the ground-state reaction coordinate (Fig. 10h).
The previous study demonstrated that the plasmonic resonance of Rh nanoparticles is confined to the UV region. However, red-shifting the plasmonic resonance further into the visible region could enhance the photocatalyst's effectiveness within the solar spectrum. Assembling plasmonic nanoparticles into closely packed clusters to create ‘hot spots’ through plasmonic coupling is one approach that could lead to more selective and efficient CH4 production from CO2 hydrogenation, even under direct or mildly concentrated sunlight.
Conventional plasmonic nanocatalysts have intense but narrow absorption spectra. In our lab, we focus on developing antenna–reactor systems using a unique broadband-absorbing ‘black gold’226 to enhance plasmonic absorption and broaden the absorption profile in the visible region through plasmonic coupling and ‘hot spot’ formation. We designed dendritic plasmonic colloidosomes (DPC) of Au loaded with nickel sites (DPC-C4-Ni)248 (Fig. 11). This design is an example of antenna–reactor geometry where plasmonic metal functions as a light harvester and the other metal functions as an active site for catalysis. DPC-C4-Ni was synthesized by loading Au nanoparticles on dendritic fibrous nanosilica (DFNS) over four cycles (Fig. 11a). DPC-C4-Ni absorbed broadband light from the solar spectrum (Fig. 11b) and generated intense localized hot spots with strong electric fields, as shown by the finite difference time domain (FDTD) simulations (Fig. 11c). When DPC-C4-Ni was illuminated with visible light, it became highly catalytically active, enabling CO2 hydrogenation using solar energy (Fig. 11e). We conducted CO2 hydrogenation reactions at various light intensities and temperatures, observing a superlinear dependence of CO production on light intensity with a power law exponent of 5.6. This behavior was characteristic of multielectron-driven plasmonic reactions. The apparent activation energy (Eapp) for the reaction under light was 21.3 ± 2.1 kJ mol−1, significantly lower than the Eapp of 65.8 ± 2.6 kJ mol−1 in the dark, indicating a substantial decrease in the activation energy barrier (Fig. 11d). The observed photo enhancement in CO production also suggested the involvement of a nonthermal pathway in CO2 hydrogenation, with the thermal effect playing a minimal role.
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| Fig. 11 Photocatalytic CO2 hydrogenation over black gold-Ni antenna–reactor system. (a) TEM image of DPC-C4-Ni, (b) UV-DRS spectrum of DPC-C4 and DPC-C4-Ni, (c) electric field intensity (V m−1) in DPC-C4-Ni using FDTD simulation, (d) Arrhenius plot for Eapp of the CO2 hydrogenation in the dark and light, (e) production rate of CH4 and CO in light at various intensities and in dark at different temperatures, (f) schematic of direct vs. indirect energy transfer processes that can result in hot-electron population in a Ni reactor, (g) KIE for CO2 hydrogenation, measured in dark and light, (h) kinetic trace extracted at the maximum of the winglet for both samples, (i) kinetic trace extracted at the minimum of bleach observed at around 410 nm for DPC-C4-Ni. Reproduced with permission from ref. 248. Copyright 2023 American Chemical Society. | ||
This hypothesis was further supported by an increase in the kinetic isotope effect (KIE), the ratio of photocatalytic rates for the 12CO2 and 13CO2 isotopes (Fig. 11g). The enhanced KIE was a distinct signature of the nonthermal activation of reactions. In DPC-C4-Ni, the hypothesis was that the hot electrons were either generated in Ni after LSPR decay (a direct mechanism) or charges were transferred from Au to Ni (an indirect mechanism) (Fig. 11f). A fraction of these hot electrons interact with reactant CO2, activating it and lowering the activation energy barrier. Additionally, during the damping of black gold LSPR, electrons in the nickel d-band could be excited to higher energy levels (hot electrons), and hot-electron transfer from Au to Ni could occur, filling the Ni d-band.
To study the involvement of hot electrons and their transfer mechanism to Ni sites, we performed ultrafast transient absorption spectroscopy (TAS) measurements. The formation of hot carriers and elastic electron–electron scattering was observed, with estimated processes occurring at 302 ± 63 fs and 419 ± 107 fs for DPC-C4 and DPC-C4-Ni, respectively (Fig. 11h). The first decay, related to electron–phonon scattering time, was estimated to be 2.16 ± 0.11 ps for DPC-C4 and 1.64 ± 0.12 ps for DPC-C4-Ni. The reduced electron–phonon lifetime in DPC-C4-Ni suggested changes in the plasmon electronic structure consistent with hot carrier transfer from Au to Ni. A negative signal centered at 410 nm in the DPC-C4-Ni sample, absent in DPC-C4, corresponded to the Ni d–d transitions (Fig. 11i). The negative signal indicated a decrease in empty states in the Ni d-band, consistent with hot-electron donation from Au to Ni. These findings suggested that the indirect hot-electron generation mechanism played a dominant role in Ni's electronic changes and, consequently, its catalytic behavior.248
As discussed in the earlier example of DPC-C4-Ni, one way to enhance the catalytic activity of plasmonic nanostructures is to integrate plasmonic metals with catalytically active metals to form antenna–reactor bimetallic heterostructures.181,472–476 Another example of such a strategy is a study by Xie et al.477 in which the authors explored surface-alloyed Au@AuRu plasmonic nanoparticles loaded on graphitic carbon nitride (g-C3N4) to create a bimetal-semiconductor heterojunction (Au@AuRu/g-C3N4) (Fig. 12). This catalyst was designed for efficient hot-electron-induced CO2 hydrogenation under mild conditions. By doping a low content of catalytically active Ru atoms into the surface of Au nanoparticles (Fig. 12a–c), the production selectivity was significantly enhanced, shifting from 63.1% CO to 98.4% CH4 (Fig. 12e). The efficiency of CO2 methanation reached 103 µmol g−1 h−1 under light at 150 °C, far exceeding its performance in dark reactions (Fig. 12d) and surpassing that of reference catalysts Au/g-C3N4 and Au@Ru/g-C3N4 (Fig. 12e).
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| Fig. 12 Photocatalytic CO2 hydrogenation over Au@AuRu/g-C3N4 plasmon–semiconductor hybrid. (a) Schematic illustration of different metal NPs supported on g-C3N4, (b) TEM image of Au@AuRu/g-C3N4, (c) atomic-resolution HAADF-STEM image of Au@AuRu NPs. (d) Production rates over Au@AuRu/g-C3N4 in the dark and under irradiation at different temperatures for 4 h, (e) production rates over different catalysts at 150 °C under illumination, (f) production rates obtained by the prepared catalysts under the light of different wavelengths (UV: λ < 400 nm, Vis: 400 nm < λ < 650 nm), (g) the production rates of Au@AuRu/g-C3N4 at 150 °C under different light powers, (h) CO2-TPD curves of g-C3N4, Au/g-C3N4, Au@AuRu/g-C3N4, and Au@Ru/g-C3N4, (i) normalized transient absorption kinetics traces for Au/g-C3N4, Au@AuRu/g-C3N4, Au@AuRu/ZrO2, Au@AuRu/SiO2, and g-C3N4, (j and k) schematic illustration of hot electron injection and catalytic process. Reproduced with permission from ref. 477. Copyright 2022 Elsevier. | ||
The photothermal CO2 hydrogenation performance of Au@AuRu/g-C3N4 at low temperatures surpassed that of noble metal (Au, Pd, Rh, Ru) and oxide (In2O3)-based photocatalysts reported in the literature. The production rate under visible light (400 nm < λ < 650 nm) was superior to that under ultraviolet light (λ < 400 nm), demonstrating that the LSPR effect of Au plays a crucial role in promoting CO2 conversion (Fig. 12f). This was also evident from the light intensity dependence study (Fig. 12e). Hydrogen temperature-programmed desorption (H2-TPD) and CO2/CO desorption experiments were conducted to evaluate the adsorption capacities of various catalysts. Ru-modified Au@AuRu/g-C3N4 and Au@Ru/g-C3N4 showed enhanced H2 adsorption and dissociation, as well as stronger CO2 and CO adsorption compared to their counterparts, facilitating efficient CO2 conversion to CH4. g-C3N4 was also found to adsorb CO2 weakly (∼91 °C) (Fig. 12h).
Transient absorption spectroscopy was employed to provide direct evidence of electron transfer from Au@AuRu NPs to g-C3N4 (Fig. 12i). Unlike Au/g-C3N4, Au@AuRu/g-C3N4 exhibited a slower electron injection process after 15 ps, attributed to the surface states in the AuRu shell retaining electrons for a longer duration before injecting them into the semiconductor. At 1 ns, the residual electron signal in Au@AuRu/g-C3N4 was 69.39% of the initial value, while this ratio for Au/g-C3N4 was only 33.17%. This indicated that hot electrons generated by Au were transferred to the AuRu shell and then injected into g-C3N4 in Au@AuRu/g-C3N4, prolonging the lifetime of the plasmon-induced electrons and enhancing the catalytic reaction (Fig. 12j). The accumulated hot electrons on g-C3N4 promoted the activation of CO2 adsorbed on the metal/semiconductor interfaces. Based on in situ DRIFT results, CO2 was converted into CO, which was then adsorbed on the metal surface for further hydrogenation to form CH4 (Fig. 12k).477
Light-driven chemical transformations on plasmonic nanostructures have traditionally utilized noble metals like Ag and Au due to their efficient plasmonic properties in the visible range. However, given the high cost and scarcity of these metals, there have been efforts to explore more abundant alternatives such as Al, Cu, and Fe. A significant challenge with these metals is their tendency to form oxide layers due to spontaneous oxidation, and their plasmon resonances often lie in the UV region, unlike the visible plasmonic resonances of Au, Ag, and Pt.
Halas et al.238 developed a notable plasmonic Al@Cu2O antenna–reactor heterostructure using earth-abundant materials, aiming to harness charge-carrier generation for the catalytic conversion of CO2 into CO under milder conditions compared to purely thermally driven processes (Fig. 13). This study highlighted Al as a plasmonic antenna that enhances reactivity on adjacent materials, in this case, the semiconducting oxide Cu2O. The Al@Cu2O heterostructure showed better external quantum efficiencies (EQE) for CO formation. In contrast, increasing irradiation intensities on pure Cu2O did not improve EQE, highlighting the unique advantage of the plasmonic Al core. A combination of experimental investigations and theoretical simulations was employed to distinguish the respective roles of plasmon-induced charge carrier generation and photothermal heating in driving the photocatalytic reverse water–gas shift reaction (rWGS) on Al@Cu2O.
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| Fig. 13 Photocatalytic CO2 hydrogenation over plasmon–semiconductor antenna–reactor Al@Cu2O. (a) High-resolution TEM image of Al and of Al@Cu2O nanoparticles, scale bar: 20 nm, (b) the impact of visible light intensity on the rate of CO formation on photocatalysts prepared from Cu2O, Al NCs and Al@Cu2O, (c) the overall rate of products formation as a function of applied temperature in purely thermal-driven (light off) rWGS for oxide supported Al NCs and Al@Cu2O (unfilled data points). For comparison, the reaction rates during the light-induced process (10 W cm−2) are shown at the corresponding recorded temperatures for oxide-supported Al NCs and Al@Cu2O (filled data points), (d) the measured EQE as a function of illumination wavelength for oxide-supported Al@Cu2O compared to Al vs. illumination wavelength, (e) numerically calculated local electric field strength |E(r)|2 in Al core (left axis) and Cu2O shell (right axis), (f) energy band diagram of Al@Cu2O for plasmon-mediated carrier generation for injection into unoccupied state of CO2 for C–O bond activation. Reproduced with permission from ref. 238. Copyright 2017 Springer Nature. | ||
Electron microscopy and elemental analysis revealed that the pristine Al nanocrystals (Al NCs) had a nominal diameter of 100 nm (Fig. 13a). To form the plasmonic antenna–reactor nanoparticles, a ∼15 nm thick Cu2O shell was grown around the Al core, which was separated from the Al metal by a 2–4 nm self-limiting amorphous Al2O3 layer. The UV-Vis-NIR extinction spectrum showed a dipolar plasmon mode at 465 nm for pristine Al NCs, which shifted to ∼550 nm after the Cu2O shell growth. The rate of CO formation catalyzed by Al@Cu2O was significantly higher than that of Cu2O and pristine Al without the reactive Cu2O shell, especially under higher illumination intensities (Fig. 13b). The study also investigated the steady-state heating of the photocatalysts under illumination using high-resolution spatial and temporal mapping of temperature variations. At a maximum visible light intensity of 10 W cm−2 in air, the Al NCs/γ-Al2O3 catalyst surface reached temperatures upwards of 175 °C. Despite this heating, the photocatalytic rWGS on Al@Cu2O was characterized by higher product selectivity and yields under illumination at comparable temperatures (Fig. 13c). Notably, the average steady-state surface temperature of 175 °C was below the 200 °C onset temperature for product formation in thermal-driven rWGS, yet it achieved a significantly higher overall reaction rate.
Further analysis revealed that coating Al NCs with a Cu2O shell substantially enhanced EQE, particularly around the dipolar plasmon resonance at ∼570 nm (Fig. 13d). The wavelength-dependent CO formation was compared with local electric field enhancement, calculated by finite element method (FEM) (Fig. 13e). The study demonstrated that the rate of carrier generation from plasmon decay was directly proportional to the plasmon-induced internal electric field enhancement. The Finite Element Method (FEM) simulations showed that the calculated electric field enhancement (|E(r)2|) in both the Al core and the Cu2O shell qualitatively matched the measured EQE spectrum (Fig. 13e). The twin mechanisms of carrier generation, direct or indirect energy transfer, both contributed to enhanced hot-carrier densities for chemical transformations. To isolate the influence of the plasmonic core, a model structure was created where the Al core was replaced with a dielectric Al2O3 sphere of the same size. In this scenario, the local electric field enhancement in the Cu2O shell did not reproduce the experimental EQE spectrum, validating the role of the Al antenna in carrier generation through plasmon decay.
The higher efficiency of light-assisted rWGS on Al@Cu2O compared to pristine Al NCs was attributed to the concurrent enhancement in surface catalytic activity and carrier generation rates. The energy diagram and schematic of the proposed elementary steps for plasmon-induced carrier-assisted rWGS on Al@Cu2O were illustrated (Fig. 13f). The negative electron affinity of CO2 posed a challenge for electron injection to form CO2−, the first and most difficult step in CO2 activation. However, CO2 adsorption on Cu2O surfaces led to charge redistribution, reducing the energy barrier for transient electron transfer to unoccupied states of adsorbed CO2, thus facilitating CO2 activation.
The study concluded that the unique selectivity observed during light-induced processes on Al@Cu2O could be explained by plasmon-induced selective C–O bond activation and nonthermal desorption of CO from reactive surface sites. Although a 2–4 nm amorphous Al2O3 shell enveloped the Al core, hot-carrier tunneling to the oxide surface remained feasible, facilitated by the abundant defect states within the Al2O3 layer. The study provided evidence for this hot-carrier tunneling mechanism through the direct dissociation of adsorbed CO2 on pristine Al NCs under visible light at ambient conditions.
Overall, this work demonstrated that the efficiency of resonance energy transfer in plasmon-enhanced photocatalysis primarily depends on the overlap between the LSPR absorption of the plasmonic metal and the optical transitions in the nearby semiconductor. Two mechanisms for resonance energy transfer were discussed: near-field enhancement associated with radiative plasmon decay and dipole–dipole coupling in non-radiative plasmon-induced resonance energy transfer (PIRET). While the FEM simulation results were interpreted in the context of near-field enhancement, the study acknowledged the plausibility of PIRET as well.238
Plasmonic catalysts have shown immense promise in CO2 conversion processes; however, their widespread application is significantly hindered by a heavy reliance on noble metals like Au and Ag. To find more sustainable alternatives, many researchers have pivoted toward Al and Cu, as both metals exhibit strong LSPR in the visible range. Yet, these non-noble alternatives suffer from poor stability and are notoriously prone to oxidation, which degrades their catalytic efficacy over time. In a recent study, Ye et al.162 addressed this fundamental stability-performance trade-off by developing an alloy-based catalyst utilizing Cu and Ru. By strategic alloying, they not only mitigated the oxidation issues inherent to copper but also harnessed the resulting system for the efficient photothermal conversion of CO2 specifically into methanol. This system represents a bimetallic plasmonic alloy or alloy-based antenna–reactor, where the electronic coupling between a plasmonic metal and a transition metal is strategically utilized to enhance both catalytic stability and selectivity.
The synthesis of the CuRu catalysts was performed using a wet impregnation–precipitation method on a MgAl2O4 support prepared via lyophilization, resulting in highly dispersed metal species that were initially invisible to XRD but clearly resolved through HAADF-STEM. The HAADF-STEM images reveal bright contrast regions corresponding to CuRu alloy nanoparticles uniformly distributed across the support (Fig. 14a). To resolve the local atomic environment, Wavelet-Transformed EXAFS (WT-EXAFS) was employed; the 2D contour plots distinguished a dominant Cu–O coordination at 1.5 Å and a Cu–Ru/Cu signal at 2.2 Å, revealing a sophisticated electronic coupling where Cu exists in a partially oxidized state (Cuδ+) stabilized by metallic Ru (Fig. 14b–e). This synergy was further validated by in situ irradiated XPS and CO-DRIFTS, which show a light-induced electron transfer from Ru to Cu, effectively “pumping” electrons to maintain the active metallic Cu0 state and preventing deactivation. Consequently, the alloy exhibits a LSPR band at ∼590 nm that not only broadens light absorption but also facilitates a potent photothermal conversion, providing the localized thermal energy and electronic environment necessary for the selective hydrogenation of CO2 to methanol under mild conditions.
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| Fig. 14 Structural and performance characterization of the RuCu alloy catalyst for photothermal CO2 hydrogenation. (a) HAADF-STEM image of Ru0.1Cu1-MgAl2O4, (b–e) WT-EXAFS contour plots of activated Ru0.1Cu1-MgAl2O4, in comparison with Cu2O, Ru foil which were used as reference materials, (f) thermal catalytic performance of the RuxCuy-MgAl2O4 catalyst, (g) photothermal catalytic performance of the RuxCuy-MgAl2O4 catalyst, (h and i) In situ DRIFTS obtained for activated Ru0.1Cu1-MgAl2O4 catalytic hydrogenation of CO2, (j) schematic illustration of intermediate adsorption and conversion on RuCu catalytic sites during CO2 hydrogenation. Reproduced with permission from ref. 162. Copyright 2026 Wiley-VCH GmbH. | ||
The catalytic evaluation of the RuxCuy-MgAl2O4 system highlighted the transformative impact of the RuCu alloy on both activity and selectivity, particularly when transitioning from purely thermal to photothermal conditions. While thermal catalysis yields were comparatively low (Fig. 14f), the Ru0.1Cu1 catalyst demonstrated superior performance under visible light (640 µL g−1 h−1), significantly outperforming its monometallic counterparts in the selective hydrogenation of CO2 to methanol (Fig. 14g). To understand the surface kinetics driving this selectivity, in situ DRIFTS was employed to monitor the intermediates under reaction conditions. The vibrational bands of *HCOO at 1593 and 2961 cm−1 were observed, while peaks at 1489, 2851, and 2922 cm−1 were attributed to methoxy species (*CH3O) (Fig. 14h and i). These results confirmed a stepwise hydrogenation pathway from CO2 to CH3OH via formate and methoxy intermediates (Fig. 14j). Furthermore, the catalyst showcased exceptional long-term stability, maintaining its production rate over a 60-hour continuous test, which was attributed to the Ru to Cu electron transfer that preserves the Cu sites in their reduced, active form against oxidative poisoning. Ultimately, the mechanism was driven by the Cu LSPR-induced photothermal effect, which supplied localized heat to lower the activation barrier, while the RuCu electronic synergy manages the surface intermediates to ensure high methanol selectivity and sustained durability.
This study demonstrated that the RuCu alloy system successfully bypasses the inherent instability of copper-based plasmonics through strategic electronic coupling. By leveraging the synergistic antenna–reactor geometry, the results highlight that the reactor metals in such configurations do not merely serve as active catalytic sites but play a critical role in stabilizing the plasmonic metal against oxidative deactivation.162
The photocatalytic conversion of CO2 with H2O involves two critical half-reactions: the reduction of CO2 by photogenerated electrons and protons, and the oxidation of H2O by photogenerated holes. Strategies like doping, defect engineering, and heterostructure fabrication have been employed to enhance the efficiency of conventional semiconductors.527–536 For instance, Xie et al.527 reported atomically thin layers of sulfur-deficient CuIn5S8 with charge-enriched Cu–In dual sites, demonstrating near 100% selectivity for CH4 production from CO2 under visible light (Fig. 15). The CuIn5S8 single-unit-cell layers achieved a CH4 evolution rate of 8.7 µmol g−1 h−1, attributed to the formation of a highly stable Cu–C–O–In intermediate. The defects in the catalyst design acted as trapping sites for photogenerated electrons or holes, thereby improving carrier separation. The atomically thin 2D layers provided abundant low-coordinated dual-metal sites, allowing simultaneous M–C and M–O bond formation, stabilizing intermediates, and enhancing reaction selectivity towards CH4. High-resolution transmission electron microscopy (HRTEM) (Fig. 15a) showed the high orientation along the [001] projection, and atomic force microscopy (AFM) confirmed single-unit-cell thickness (∼1.07 nm). The defects were characterized by electron spin resonance (ESR) signal (g = 2.003) (Fig. 15b) and an upshift in the S 2p XPS peak, indicating the presence of S vacancies (Fig. 15c). The electronic band structures of VS-CuIn5S8 were analyzed using synchrotron radiation photoemission spectroscopy (SRPES) (Fig. 15d), and UV-Vis spectra (Fig. 15e) revealed suitable band gaps and band edge positions for CO2 reduction and O2 evolution under visible light (Fig. 15f). Compared to pristine CuIn5S8, the sulfur-deficient layers exhibited a 5.4-fold increase in CH4 evolution rate and near 100% selectivity for CH4 over CO (Fig. 15g). VS-CuIn5S8 showed enhanced visible-light absorption, higher surface photovoltage (SPV) peak intensity (Fig. 15i) as well as lower PL peak intensity relative to the pristine CuIn5S8 single-unit-cell layers. The time-resolved fluorescence spectra showed extended carrier lifetimes, indicating improved charge separation (Fig. 15h). In situ Fourier transform infrared spectroscopy (FTIR) highlighted that CO intermediates on VS-CuIn5S8 surfaces were rapidly protonated to CHO*, preventing CO desorption and favoring CH4 formation. DFT calculations demonstrated that charge-enriched Cu–In dual sites stabilized COOH* intermediates more effectively than Cu single sites, reducing energy barriers and enabling spontaneous protonation to CH4. This work highlighted the potential of rationally designed defect-engineered atomically thin semiconductor sheets with dual-metal sites to modulate reaction pathways, improving the activity and selectivity of CO2 photoreduction.527
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| Fig. 15 Photocatalytic CO2 reduction to CH4 mediated by vacancy-rich atomically thin CuIn5S8 layers. (a) HRTEM image showing the interplanar distances, and the corresponding dihedral angle, (b) EPR spectra, in which the signal at g = 2.003 corresponds to the S vacancies, (c) XPS spectra of S 2p for the VS-CuIn5S8 single-unit-cell layers and the pristine CuIn5S8 single-unit-cell layers, (d) SRPES valence-band spectra, in which valence-band maxima are located at 2.04 and 2.46 eV below the Fermi level, (e) UV-Vis diffuse reflectance spectra. (inset) Obtained band gaps of 1.92 eV and 2.06 eV, (f) schematics illustrating the electronic band structures, (g) products of photocatalytic CO2 reduction for the VS-CuIn5S8 single-unit-cell layers (red bars) and the pristine CuIn5S8 single-unit-cell layers (blue bars), (h) fluorescence emission decay spectra, (i) surface photovoltage (SPV) spectra of VS-CuIn5S8 single-unit-cell layers and the pristine CuIn5S8 single-unit-cell layers. Reproduced with permission from ref. 527. Copyright 2019 Springer Nature. | ||
Among semiconductors, metal oxyhalide ultrathin nanosheets (UTNs) are particularly promising for CO2 reduction due to the unique heterogeneity in their crystal structure. These materials feature both covalent metal–oxygen bonding and soft ionic metal–halide bonding coexisting within a two-dimensional layer. This arrangement creates an anisotropic charge distribution between the metal–oxygen layer and metal–halogen slices, resulting in a preferentially oriented internal electric field within the 2D metal oxyhalide layer.489,504,528
When defect engineering is applied to selectively disrupt halide or oxygen atoms, it induces a synergistic effect by exposing unsaturated surface metal atoms and enhancing the internal electric fields. This coupling significantly improves charge separation efficiency and catalytic performance in metal oxyhalide UTNs. Zhang et al.528 explored van der Waals gaps (VDWGs) and defects for photocatalytic CO2 reduction and reported an efficient pure water CO2-to-CO conversion using sub-3-nm-thick BiOCl nanosheets enriched with van der Waals gaps on their two-dimensional facets (Fig. 16). Unlike bulk BiOCl, these atomic layers with abundant VDWGs showed significantly reduced exciton binding energy (from 137 to 36 meV) and a 50-fold increase in charge separation efficiency. VDWGs facilitated the formation of VDWG-Bi-VO˙˙-Bi defect sites, which optimized CO2 activation, *COOH splitting, and *CO desorption. This system achieved a photocatalytic CO2 reduction (PCR) rate of 188.2 µmol g−1 h−1 under visible light in pure water without requiring cocatalysts, hole scavengers, or organic solvents (Fig. 16g and h). The nanosheets, with 99% VDWG exposure achieved through gas-phase exfoliation, demonstrated enhanced electron–hole separation due to weakened exciton binding and the formation of active VDWG-Bi-VO˙˙-Bi sites (Fig. 16a–d). Positron annihilation spectroscopy (PAS) showed a lifetime of 195 ps (Fig. 16e), EPR showed a peak centered at g = 2.004 (Fig. 16f), and X-ray absorption near-edge structure (XANES) revealed an additional peak centered at 529.6 eV (Fig. 16i), confirming the presence of VDWG-Bi-VO˙˙-Bi defects, which were positively proportional to VDWGs coverage percentage. This defect structure enhanced CO2-to-CO conversion, with a stoichiometric CO
:
O2 evolution ratio of ∼2.14
:
1 (Fig. 16g and h). Steady-state PL measurements across temperatures demonstrated reduced exciton binding energy (Eb) due to high VDWG coverage, which facilitated charge carrier separation and suppressed recombination (Fig. 16j and k). The VDWGs offered channels along which electrons and holes can diffuse and then separate. In addition, the VDWGs-dominated surfaces possess abundant unsaturated atoms or architectures that can efficiently trap electrons or holes to inhibit their recombination. Time-resolved PL measurements showed a 20.7-fold longer charge carrier lifetime for BOC-VDWGs-AL compared to conventionally exfoliated nanosheets (Fig. 16l). Similarly, an 11.5-fold higher photocurrent (Fig. 16m) and a smaller electrochemical impedance arc evidenced efficient bulk charge carrier separation with high VDWG coverage (Fig. 16n).
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| Fig. 16 Photocatalytic CO2 reduction to CO over van der Waals gap-rich BiOCl atomic layers. (a) TEM image, (b) dark-filed STEM image and elemental mappings, (c) aberration-corrected HAADF-STEM image, (d) intensity profiles (taken along the lines of c) of BOC-VDWGs-AL, (e) PAS, (f) EPR, (g) yield of O2 detected during pure-water PCR photocatalyzed by BOC-VDWGs-AL, as well as the calculated yield ratio of CO to O2, (h) comparison of CO-evolving rate of BOC-VDWGs-AL, CBOC-VDWGs, and BOC-VDWGs-76, all under visible light in the presence of pure-water and CO2, (i) O K-edge XANES of BOC-VDWGs-AL, CBOC-VDWGs, and BOC-VDWGs-76, (j) PL of BOC-VDWGs-AL, (k) comparisons of Eb and VDWG coverage percentage of BOC-VDWGs-AL, CBOC-VDWGs, and BOC-VDWGs-76, (l) time-resolved PL of BOC-VDWGs-AL and BOC-VDWGs-76, (m) transient photocurrent responses and (n) bulk charge separation efficiencies of BOC-VDWGs-AL, CBOC-VDWGs, and BOC-VDWGs-76, (o) UV-visible absorption spectra, (p) plots of (αhν)1/2 versus energy (hν) for the band-gap energies, (q) band structure alignments of BOC-VDWGs-AL and BOC-VDWGs-76. Reproduced with permission from ref. 528. Copyright 2021 Springer Nature. | ||
The VDWG-Bi-VO˙˙-Bi defect also imparted BiOCl, which is normally photoactive only under ultraviolet light, with optical absorption across the entire visible light spectrum (Fig. 16o). This occurs because VDWG-Bi-VO˙˙-Bi introduces intraband states between the conduction and valence bands, narrowing the band gap and enabling the absorption of long-wavelength visible-light photons (Fig. 16p). Ultraviolet photoelectron spectra (UPS) revealed that BOC-VDWGs-AL possesses a valence band maximum of 2.21 eV, providing sufficient potential to photo catalytically oxidize H2O into O2 (Fig. 16q).
These findings highlight the transformative role of VDWGs in ultrathin BiOCl nanosheets. The high VDWG coverage enabled ultralow Eb and catalytically active VDWG-Bi-VO˙˙-Bi sites, achieving superior PCR performance using visible light, pure water, and CO2. This innovative VDWG engineering approach adds a new dimension to the optimization of layered photocatalysts, surpassing traditional strategies like defect engineering, doping, or single-atom loading.528
Compared to monometallic oxyhalides, bimetallic oxyhalides remain relatively underexplored. In a recent study, Chen et al.529 employed a novel top-down wet-chemistry desalination approach to remove the alkali-halide salt layer within the complex bulk precursor structure of Pb0.6Bi1.4Cs0.6O2Cl2 (PBCOC) (Fig. 17). This process successfully produced a new two-dimensional ultrathin bimetallic oxyhalide, Pb0.6Bi1.4O2Cl1.4 (PBOC). The desalination process, achieved via simple ultrasonication in deionized water, dissolved the Cs–Cl layer (Fig. 17a), delaminating the parental PBCOC structure into ultrathin PBOC layers. Scanning electron microscopy (SEM), scanning transmission electron microscopy (STEM), and energy dispersive spectroscopy (EDS) analyses validated the reduced Cs and Cl concentrations (to 0.05% and 21.73%, respectively), indicating successful leaching (Fig. 17b). STEM imaging revealed a layered ABBA stacking arrangement in PBOC, with mirror-symmetry-mediated stacking interactions and van der Waals bonding between layers (Fig. 17c).
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| Fig. 17 Photocatalytic CO2 reduction over desalinated bimetallic oxyhalide (Pb0.6Bi1.4O2Cl1.4). (a) Schematic illustration of ultrathin PBOC layers synthesis from PBCOC via desalination strategy, (b) STEM-EDS elemental-mapping images and the corresponding element atomic concentrations, (c) atom-resolved inverse FFT BF-STEM images, with the labeled zone axis, (d) UV-Vis diffuse reflectance spectra. (inset) Corresponding optical images and obtained band gaps of 2.82 and 3.14 eV, (e) photocatalytic CO2RR products under full-spectrum light irradiation, (f) photocatalytic CO2 reduction activities of the ultrathin PBOC in N2 (grey ball), atmospheric CO2 (red ball), and pure CO2 (blue ball) under full-spectrum light irradiation, (g) transient photocurrent densities with light on/off cycles under full spectrum in 0.1 M Na2SO4 electrolyte solution at an applied potential of 0.5 V vs. Ag/AgCl electrode, (h) electrochemical impendence spectroscopy, (i) Mott–Schottky plots, (j) time-resolved fluorescence spectra. Ave. τ is the average fluorescence lifetime, (k) the partial density of states (PDOS) calculated using DFT, (l) schematic illustration of the electronic band structures, and grey arrows represent the electron transition process under the light irradiation. Reproduced with permission from ref. 529. Copyright 2022 Springer Nature. | ||
The ultrathin PBOC exhibited a narrower band gap (2.82 eV) than bulk PBCOC (3.14 eV), as demonstrated by UV-Vis diffuse reflectance spectroscopy (Fig. 17d). Mott–Schottky analysis indicated an N-type semiconductor behavior, with CBM positions of −0.34 V (Fig. 17i). These band edge positions favored both CO2 reduction and O2 evolution (Fig. 17l). Enhanced charge separation and transport were confirmed by electrochemical impedance spectroscopy (EIS) (Fig. 17h), PL spectroscopy (Fig. 17j), and transient photocurrent measurements (Fig. 17g), with PBOC showing lower emission responses and longer charge carrier lifetimes.
Under Xe lamp irradiation (420 nm filter) with 1500 ppm CO2, PBOC achieved superior photocatalytic performance, producing CO and CH3OH at rates of 17.91 µmol g−1 and 26.53 µmol g−1 in 4 hours, 7.2 and 7.3 times higher than PBCOC (Fig. 17e and f). Continuous O2 production (∼48.69 µmol g−1 in 4 hours) was also observed, attributed to the oxidation of H2O. This performance exceeded that of BiOCl nanosheets and other benchmark photocatalysts, highlighting the role of Pb–Bi co-occupancy in enhancing interfacial and electronic properties. The DFT calculations revealed that Pb incorporation reduces the band gap compared to BiOCl while inducing significant polarization effects that promote charge separation. Partial density of states (PDOS) analysis revealed increased electronic states at the conduction-band edge due to Pb–Bi co-occupancy (Fig. 17k). The synergistic effects of rich catalytic centres, enhanced charge conductivity, and structural stability are crucial in achieving remarkable CO2 reduction performance, providing insights into the design of next-generation photocatalysts.529
In a report by Chen et al.,530 they discovered that the high surface area and low charge recombination characteristics of doped 2D materials could significantly enhance photocatalytic activity. Among various metal sulfides, they investigated SnS2, a naturally occurring bronze-colored n-type semiconductor with a narrow band gap (2.2–2.4 eV) known as mosaic gold. The material's narrow band gap, combined with an average photocarrier diffusion length of approximately 0.19 µm and high quantum yield, provided two distinct advantages for visible-light-driven photocatalysis. Chen et al. synthesized a carbon-doped SnS2 nanostructure (referred to as SnS2-C) to improve photocatalytic performance by suppressing charge recombination and enhancing charge transport (Fig. 18).530 The powder X-ray diffraction (p-XRD) peaks for SnS2-C were broader than those of SnS2, indicating a nanocrystalline and partially amorphous structure. The (001) interplanar spacing of SnS2-C was calculated as 0.604 nm, slightly larger than that of SnS2 (0.585 nm), suggesting lattice expansion caused by carbon doping. The HRTEM images supported these findings, showing increased interplanar spacing in SnS2-C. EDX and HAADF imaging confirmed uniform distribution of Sn, S, and C in SnS2-C (Fig. 18a and b). A reduction in the band gap was observed for SnS2-C (2.34 eV) compared to SnS2 (2.43 eV) (Fig. 18c). The UPS analysis revealed a work function of 4.4 eV for SnS2-C, higher than the 4.16 eV of SnS2. This shift indicated a change in band edge positions, which is favorable for multi-electron CO2 reduction (Fig. 18h). XPS analysis revealed binding energy shifts in SnS2-C, confirming lattice distortions caused by carbon incorporation (Fig. 18d). PL (Fig. 18f) and time-resolved PL (TRPL) (Fig. 18g) measurements provided insights into charge carrier dynamics. SnS2-C exhibited a nearly threefold lower PL intensity compared to SnS2, indicating reduced recombination of photoinduced charge carriers. TRPL spectra revealed shortened lifetimes for photogenerated electrons and holes in SnS2-C, suggesting efficient carrier separation due to nonradiative pathways facilitated by carbon doping. Under visible light, SnS2-C exhibited a maximum cumulative acetaldehyde yield of approximately 125.66 µmol/100 mgcat after 14 hours, compared to 0.55 µmol/100 mgcat for SnS2 (Fig. 18e). The solar fuel photochemical quantum efficiency (PCQE) of SnS2-C was calculated to be ∼0.72%. Mechanistic insights revealed that carbon doping helped in extending the absorption band into the longer wavelength range, promoting CO2 adsorption and reducing the dissociation barrier for the reduction process.
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| Fig. 18 Photocatalytic CO2 reduction over carbon-doped SnS2. (a) SEM images of SnS2-C, (b) high-angle annular dark-field (HAADF) image and EDX elemental mapping of C, S, Sn from selected area for SnS2-C, (c) UV-Vis diffuse reflectance and (insets) Tauc plots with both direct and indirect fittings, (d) high-resolution XPS S 2p spectra of SnS2-C and SnS2, (e) cumulative acetaldehyde formation yield of SnS2-C and SnS2, (f) normalized PL spectra of SnS2-C and SnS2, (g) summary table of TRPL slow, fast, and average lifetime calculated at both 493 and 548 nm emissions, (h) band edge positions and photocatalytic reaction mechanism: comparative band diagram of SnS2-C and SnS2, together with a proposed electron–hole separation of photo-excited electron–hole pairs in SnS2-C. Reproduced with permission from ref. 530. Copyright 2018 Springer Nature. | ||
Simulation studies suggested that the conduction band position of SnS2-C aligned favorably with the onset reduction potential energy of CO2, enabling a ten-electron reduction process critical for acetaldehyde production (Fig. 18h). The band edge tuning and microstrain-induced new electronic states in SnS2-C enhanced electron migration to the surface. Meanwhile, photogenerated holes reacted with water molecules, forming oxygen, hydrogen peroxide, or hydroxide radicals, further driving the reaction.
In summary, Chen et al.530 concluded that the enhanced photocatalytic performance of SnS2-C resulted from a combination of structural and electronic modifications, including high surface area, reduced photocarrier diffusion length, improved charge separation, and favorable band edge positions. These factors collectively enabled efficient visible-light-driven CO2 reduction and selective acetaldehyde production through a multi-electron transfer process.530
Other than doping and defect creation, there have been reports of heterostructure fabrication and metal cocatalyst loading to improve the lifetime of charge carriers in semiconductors. Yu et al.,531 presented a simple one-pot method to develop core-triple shell Mn, C-codoped ZnO hollow spheres photocatalysts for CO2 reduction. In this design, Mn ions with switchable valence states acted as “ionized cocatalysts”, enhancing CO2 adsorption and light harvesting. They also facilitated the transfer of photogenerated electrons from the ZnO conduction band to drive CO2 reduction, a process maintained by the reversible oxidation states of Mn ions. This approach bypasses the challenges of cocatalyst loading and ensuring intimate contact, as the ionized cocatalysts are embedded within the ZnO lattice, serving as active sites for CO2 activation.
Using a coordination polymer (CP) strategy, Mn, C-codoped ZnO core-triple shell hollow spheres (Mn, C-ZnO CTSHSs) were synthesized through a solvothermal method followed by controlled air annealing (Fig. 19). Characterization revealed that Mn ions substitute Zn in the ZnO lattice (Fig. 19a), acting as active centers for CO2 reduction while suppressing competitive hydrogen evolution. In situ XPS demonstrated that Mn ions restore their initial oxidation state post-reaction by capturing photogenerated electrons, showcasing a light-switchable cocatalytic behavior (Fig. 19h). This mechanism underscored the durability and efficiency of Mn as an ionized cocatalyst for practical applications.
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| Fig. 19 Photocatalytic CO2 reduction over Mn, C-codoped ZnO core-triple shell hollow spheres. (a) TEM images of the Mn, Zn-CPSs after calcination for 3 h, HAADF-STEM image of Mn, C–ZnO and EDS mapping of the sample, (b) UV-Vis light absorption of the prepared photocatalysts and the inset represents the multiple reflection effect of the incident light inside the hollow cavities, (c) wavelength dependence of the AQE and the UV-Vis absorption spectrum of 2% Mn, C-ZnO sample, (d and e) photocatalytic CO2 reduction performance of comm. ZnO and the prepared samples: time course of a CO and O2 production yields, (f) PL spectra of photocatalysts at excitation wavelength of 380 nm, (g) TRPL spectra of the samples, (h) in situ XPS analysis showed Mn 3s profiles for CO2-adsorbed Mn, C-ZnO CTSHS samples. The multiple splitting of Mn 3s (ΔS) is used to calculate the average oxidation state of Mn ions within the structure, (i) schematic illustration of CO2 activation and reduction over Mn, C-codoped ZnO sample. Reproduced with permission from ref. 531. Copyright 2021 Springer Nature. | ||
Photocatalytic experiments revealed that the 2% Mn, C-ZnO CTSHS catalyst achieved the highest CO2 reduction activity, producing CO at a rate of 0.83 µmol g−1 under simulated solar light (Fig. 19d and e). Excessive Mn doping (e.g., 5%) introduced defect states that acted as charge recombination centers, reducing efficiency. The system's apparent quantum efficiency (AQE) aligned with its light absorption spectrum (Fig. 19c). The enhanced light absorption was attributed to the hollow structure, which enabled multiple light reflections, and Mn doping, which introduced impurity states that narrowed the ZnO band gap (Fig. 19c). Additional electronic transitions, such as ligand-to-metal and metal-to-ligand charge transfers, further improved light harvesting. The PL spectra confirmed suppressed charge recombination, with the 2% Mn, C-ZnO catalyst showing the lowest PL intensity and longest charge carrier lifetime (1.1 ns) (Fig. 19f). Electrochemical impedance spectroscopy revealed reduced charge transfer resistance (Rct) in Mn-doped samples, promoting efficient charge carrier migration. The Mn species also significantly enhanced CO2 adsorption, attributed to surface oxygen species and Mn ions replacing Zn in the lattice. In situ XPS under light and dark conditions showed Mn ions alternately transferring electrons to CO2 molecules and regenerating their oxidation states upon light irradiation (Fig. 19h). This light-switchable behavior is crucial for maintaining catalyst activity without external treatments. The Mn ions also acted as Lewis base centers, facilitating CO2 adsorption and activation through a single-electron transfer to form CO2− intermediates. Subsequent proton-coupled electron transfer leads to CO production (Fig. 19i). These findings validated Mn ions as durable and efficient ionized cocatalysts in a light-responsive system.
In summary, the core-triple-shell Mn, C-codoped ZnO hollow spheres synthesized via a one-pot method exhibited superior photocatalytic performance due to their structural and functional advantages, including enhanced light absorption, efficient charge separation, and abundant active sites. The Mn species played a pivotal role in CO2 activation through electron transfer while regenerating their oxidation states under light. This study underscores the potential of hollow-structured materials and light-switchable cocatalysts for sustainable CO2 reduction and clean energy applications.531
Despite different structural modifications, the efficiency of CO2 photoreduction remained less, to enhance the efficiency of artificial photosynthesis, Li et al.457 developed a Cu2O-Pt/SiC/IrOx composite using controlled photodeposition techniques (Fig. 20). This composite was integrated into an artificial photosynthetic system featuring a Nafion membrane that separated the reduction and oxidation half-reactions. The system demonstrated exceptional photocatalytic performance under visible light, converting CO2 into HCOOH and water into O2 with yields of 896.7 and 440.7 µmol g−1 h−1, respectively, nearly in stoichiometric proportions.
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| Fig. 20 Photocatalytic CO2 reduction over direct and indirect Z-scheme heterostructure-coupled Cu2O-Pt/SiC/IrOx photosystem. (a) Schematic representation of Cu2O-Pt/SiC/IrOx synthesis via controlled photo-deposition, (b) TEM and (c) HRTEM images of Cu2O-Pt/SiC/IrOx, (d) evolutions of HCOOH and O2 as a function of illumination time, (e) the apparent quantum yield of HCOOH evolution with the wavelength of irradiation light for the separated reaction system, (f) periodic on/off photocurrent response, (g) AC Impedance, (h) the electron transfer processes in Cu2O-Pt/SiC/IrOx under light illumination, (i) PL spectra for different photocatalysts, (j) time-resolved photoluminescence spectroscopy of Cu2O-Pt/SiC/IrOx, (k) comparison for the HCOOH evolution between in the spatially separated reaction system and in the conventional one-pot reactor with different samples as the reduction side photocatalyst, (l) schematic diagram of the spatially separated Z-scheme system, (m) the proposed mechanism of the separated system for the efficient CO2 reduction and O2 evolution. Reproduced with permission from ref. 457. Copyright 2020 Springer Nature. | ||
This remarkable efficiency is attributed to the direct and indirect Z-scheme electronic structures of the composite. The direct Z-scheme facilitates efficient charge separation and prolonged carrier lifetimes, while the spatially separated reduction and oxidation units prevent product back-reactions. Unlike many photocatalysts that require sacrificial agents (e.g., triethanolamine or EDTA) to function, this system achieves sustainable and efficient photocatalysis without such additives.
Silicon carbide (SiC), a metal-free semiconductor with a moderate band gap (2.4 eV) and suitable conduction band energy (∼−1.1 V), is ideal for multi-electron CO2 reduction reactions. However, its low hole mobility and lack of active sites for CO2 adsorption hinder its photocatalytic performance. To address these challenges, the Cu2O-Pt/SiC/IrOx hybrid photocatalyst was designed with IrOx for photo-oxidation and Cu2O-Pt for photoreduction (Fig. 20a). This configuration enhanced charge carrier lifetimes and CO2 adsorption, significantly boosting efficiency.
The artificial system utilized two separate reaction chambers mimicking natural photosynthesis. One chamber, equipped with Cu2O-Pt/SiC/IrOx and Fe2+, drives CO2 reduction, while the other, containing Pt/WO3 and Fe3+, facilitates water oxidation (Fig. 20l). A Nafion membrane ensures selective ion transfer between chambers, optimizing reaction efficiency. The Cu2O-Pt/SiC/IrOx composite achieved a remarkable HCOOH yield of 896.7 µmol g−1 h−1, which is 527 times higher than pristine SiC (Fig. 20d). The system also maintained a stoichiometric ratio of O2 evolution, confirming its reliability. The photocatalytic activity of the spatially separated system was approximately 15 times greater than that of the one-pot reaction system for each photocatalyst (Fig. 20d). In the one-pot system, the re-oxidation of HCOOH by O2 likely contributed to the lower production of HCOOH and O2. Additionally, Fe3+ competes with CO2 for generated electrons, and Fe2+ competes with H2O for photogenerated holes. However, the impact of Fe2+ was likely less significant than that of Fe3+, as HCOOH and O2 evolution were even lower in the absence of added Fe3+ and Fe2+. The AQY of HCOOH evolution for the optimal Cu2O-Pt/SiC/IrOx sample aligned well with its optical absorption spectra. Under 400 nm light irradiation, the AQY of HCOOH evolution reached approximately 1.44% (Fig. 20e).
Detailed analyses, including TEM analysis, revealed the strategic spatial distribution of Pt, Cu2O, and IrOx on the SiC surface, promoting efficient electron transfer (Fig. 20b and c). Cu2O-Pt exhibited intimate contact, while IrOx was randomly deposited, ensuring optimal charge separation and migration. The PL (Fig. 20i) and time-resolved spectroscopy (Fig. 20j) confirmed reduced charge recombination rates and enhanced carrier lifetimes for the composite. Cu2O-Pt/SiC/IrOx exhibited the highest photocurrent (Fig. 20f) and the lowest AC impedance (Fig. 20g), indicating superior electron transfer and charge separation efficiency. However, a slight inconsistency arises for Cu2O-Pt/SiC and Pt/SiC, where the photocurrent and AC impedance trends do not fully align with their photocatalytic activity. This discrepancy suggested that photocatalytic activity depended not only on charge transfer and separation efficiency but also on the surface chemistry of the photocatalysts. Furthermore, Mott–Schottky and UV-Vis analyses demonstrated the Z-scheme mechanism, where photogenerated electrons and holes were effectively utilized to drive the desired reactions (Fig. 20h). When light illuminated the system, electrons from the conduction band of IrOx (+0.35 V) transferred to the valence band of SiC (+1.40 V). Simultaneously, electrons in the CB of SiC (−1.08 V) moved to Pt nanoparticles and then to the VB of Cu2O (+0.70 V), where they combined with the holes generated in Cu2O. This process, known as the direct Z-scheme, resulted in electrons accumulating in the CB of Cu2O (−1.28 V), where they reduced CO2 to HCOOH [E(CO2/HCOOH) = −0.61 V]. Meanwhile, the holes in IrOx (+1.85 V) oxidized Fe2+ to Fe3+ [E(Fe2+/Fe3+) = +0.77 V]. In the water oxidation chamber, visible light excited Pt/WO3, causing electrons in the CB of WO3 (+0.74 V) to migrate to Pt, where they reduced Fe3+ back to Fe2+ (Fig. 20m). At the same time, the holes in the VB of WO3 (+2.06 V) oxidized water to produce oxygen [E(H2O/O2) = +1.23 V]. This study underscores the significance of combining direct and indirect Z-scheme mechanisms with spatial separation for artificial photosynthesis. The hybrid system not only addresses the limitations of pristine SiC but also achieves sustainable and economically viable CO2 reduction and water oxidation.457
The size and choice of cocatalyst nanoparticles are critical for charge separation and CO2 activation, as previously demonstrated. In a notable study, Liu et al.532 developed a single-atom catalyst consisting of isolated cobalt atoms incorporated into Bi3O4Br atomic layers to facilitate charge transfer, carrier separation, and CO2 adsorption and activation. Thus, reducing the CO2 activation energy by stabilizing COOH* intermediates and shifting the rate-limiting step from COOH* formation to CO* desorption. The optimized catalyst, leveraging cobalt single atoms and ultrathin Bi3O4Br layers, achieved a CO production rate of 107.1 µmol g−1 h−1; approximately 4 and 32 times higher than atomic-layer and bulk Bi3O4Br, respectively.
The ultrathin configuration of Bi3O4Br reduced bulk charge carrier recombination due to shorter diffusion distances and provided a high ratio of unsaturated surface atoms, enhancing interfacial reactions and product selectivity. TEM images confirmed a 1.89 nm thickness of Bi3O4Br layers (Fig. 21a), while elemental mapping (Fig. 21b and c) revealed a uniform distribution of cobalt atoms (0.8 wt%). The XPS analysis showed cobalt atoms predominantly in the +2 oxidation state (Fig. 21d). The band gap energy decreased from 2.29 eV in Bi3O4Br to 2.21 eV in Co-Bi3O4Br, improving light absorption by introducing dopant energy levels (Fig. 21g and h).
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| Fig. 21 Photocatalytic CO2 reduction over isolated single atom cobalt in Bi3O4Br atomic layers. (a) Schematic representation of Cu2O-Pt/SiC/IrOx synthesis via controlled photo-deposition, (b) TEM and (c) STEM image and EDS mapping images of Co, Bi, O, and Br, (d) EXAFS spectra of Co K-edge, (e) calculated density of states of Co-Bi3O4Br, (f) XPS valence band spectra of the Bi3O4Br and Co-Bi3O4Br-1, (g) UV/Vis diffuse reflection spectra, (h) Tauc plot of Bi3O4Br and Co-Bi3O4Br-1, (i) photoreduction of CO2 into CO over Bi3O4Br and Co-Bi3O4Br materials, (j) time-resolved transient PL decay, (k) transient photocurrent responses; (l) electrochemical impedance spectroscopy pure Bi3O4Br and Co-Bi3O4Br-1, (m) surface photovoltage spectra, (n) ultrafast TA spectra of Bi3O4Br and Co-Bi3O4Br-1, (o) schematic band structure obtained according to the results in (f) and (h). Reproduced with permission from ref. 532. Copyright 2019 Springer Nature. | ||
The detailed energy-level positions of the VB edges, determined from XPS VB spectra (Fig. 21f and o), were both 1.06 eV. Consequently, the CB potentials of Bi3O4Br and Co-Bi3O4Br-1 were calculated to be −1.23 eV and −1.15 eV, respectively, meeting the thermodynamic requirements for CO2 reduction to CO. Additionally, DFT calculations indicated an increased density of states in the band gap for Co-Bi3O4Br, further confirming the facilitated transition of photogenerated electrons to the new energy levels (Fig. 21e). Ultrafast TA spectroscopy provided key insights into charge carrier dynamics (Fig. 21n). The biexponential fitting of TA spectra revealed two distinct time constants: τ1, representing electron capture from the CB into trap states, was approximately 12 ps for Bi3O4Br and 11 ps for Co-Bi3O4Br. Meanwhile, τ2, corresponding to recombination between trapped electrons and VB holes, showed a significant increase from 400 ps in Bi3O4Br to 1 ns in Co-Bi3O4Br, indicating a ∼2.5-fold improvement in carrier lifetime. This prolonged lifetime allowed trapped electrons more opportunities to participate in CO2 photoreduction, enhancing catalytic efficiency.
The Co-Bi3O4Br catalyst exhibited superior photocatalytic activity, achieving a 20-hour CO yield of 2142.1 µmol g−1 with trace methane production (Fig. 21i). It simultaneously oxidized water to O2 at an average rate of 56 µmol g−1 h−1, maintaining a near-stoichiometric CO
:
O2 ratio of 2. The apparent quantum yields reached 0.91% at 380 nm and 0.36% at 400 nm. Additional analyses, including SPV spectroscopy (Fig. 21m), photocurrent (Fig. 21k), and electrochemical impedance (Fig. 21l) measurements, confirmed enhanced charge separation, which was the reason for high CO2 reduction efficiency. The findings highlight the potential of single-atom catalysts in ultrathin layers to achieve high-efficiency, selective solar-driven CO2 conversion.532
The efficiency of CO2 reduction relies not only on effective charge separation and transfer but also on the catalyst's ability to adsorb and activate CO2 molecules at its surface. Semiconductor materials offer an additional advantage in this regard, as their surfaces can be engineered to introduce oxygen vacancies that enhance CO2 adsorption and thereby improve reduction performance. In this context, Zhang et al.53 addressed the limitation of poor CO2 adsorption by designing periodic oxygen vacancies to create periodic frustrated Lewis pairs (PFLPs) on the surface of bimetallic semiconductor oxide SrNb2O6 photocatalysts. In this configuration, the two metal centers play complementary roles: Sr2+ acts as a Lewis acid, polarizing the oxygen atoms of CO2, while Nb4+ functions as a Lewis base, interacting with the carbon atom to bend and activate the molecule, ultimately facilitating more efficient electron transfer.
The synthesis utilized electrospinning to produce SrNb2O6 nanofibers, which were subsequently vacuum-annealed in ethanol to generate surface oxygen vacancies (OVs). Comprehensive characterization using EPR confirmed the presence of OVs, while XPS analysis revealed a critical electronic shift in the O 1s spectrum, exhibiting a lattice oxygen peak at 530.6 eV and a vacancy-induced peak at 531.4 eV. This defect engineering triggered a partial reduction of Nb5+ to Nb4+, creating a bimetallic surface where Sr2+ (empty 5s orbital) acts as the Lewis acid, and Nb4+ (free 4d electron) acts as the Lewis base (Fig. 22a). Atomic-resolution ABF-STEM confirmed that these vacancies are periodically arranged, resulting in regular lattice contractions along the [100] direction that maintain the “frustrated” state necessary for high catalytic reactivity.53
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| Fig. 22 PFLP-engineered bimetallic SrNb2O6 for enhanced sunlight-driven CO2 photocatalysis. (a) Schematic illustration of the structure change from the SrNb2O6 to the SrNb2O6−x decorated with PFLPs, (b) CO and CH4 production rates of photocatalytic CO2 reduction over SrNb2O6−x-1–4 and SrNb2O6 under UV-visible light irradiation (320 nm < λ < 780 nm); black dots expressing the corresponding CO-product selectivities of these samples, (c) cycling measurements for CO2 photoreduction to CO over SrNb2O6−x-3, (d) photograph image of the photocatalytic reactor for CO2 reduction in an outdoor condition upon natural light irradiation focused by the Fresnel lens, (e) photograph images of the CO evolution through the outdoor CO2 photoreduction reaction in the way of solid–liquid condition by using 0.1 M potassium bicarbonate solution as the CO2 precursor, (f) CO production rates of the outdoor CO2 photoreduction over SrNb2O6−x-3 and SrNb2O6 upon the focused sunlight irradiation (solid–gas condition), (g) CO2 adsorption isotherms at 298 K. In situ FT-IR spectra of (h) SrNb2O6 and (i) SrNb2O6−x-3 during photocatalytic CO2 reduction with water vapor under UV-visible light irradiation for 0 to 30 min, (j) a possible four-step reaction mechanism for the photocatalytic reduction of CO2 to CO based on the synergistic effect of PFLPs distributed on SrNb2O6−x. Reproduced with permission from ref. 53. Copyright 2025, American Chemical Society. | ||
The photocatalytic performance of the SrNb2O6−x nanofibers highlighted the transformative impact of PFLP engineering on CO2 conversion efficiency and selectivity. Among the series of catalysts tested, SrNb2O6−x-3 emerged as the optimal candidate, achieving a CO production rate of 65.9 µmol g−1 h−1 under UV-visible light, which is a 3.35-fold enhancement over pristine SrNb2O6 (Fig. 22b), while simultaneously boosting CO selectivity to 98.7%. Furthermore, the catalyst demonstrated long-term stability, retaining activity over four sequential cycles with no detectable changes in crystal structure or PFLP electronic states, as confirmed by post-reaction XRD and XPS fitting (Fig. 22c). For practical scalability, the authors conducted outdoor experiments under natural sunlight focused by a Fresnel lens, where the SrNb2O6−x-3 sample maintained a CO evolution rate of 25.5 µmol g−1 h−1, significantly outperforming the 6.1 µmol g−1 h−1 observed for pure SrNb2O6 (Fig. 22d and e). This superior activity is underpinned by an increase in CO2 uptake values; the SrNb2O6−x-4 sample exhibited an adsorption capacity of 16.0 cm3 g−1, a 5.2-fold improvement over the unmodified nanofibers (3.1 cm3 g−1), attributed to the robust coordination between the Sr2+/Nb4+ pairs and CO2 molecules (Fig. 22f).
The photocatalytic mechanism of the SrNb2O6−x-3 nanofibers was driven by a sophisticated “push–pull” synergy between the periodic frustrated Lewis pairs. Ultraviolet-visible spectroscopy and UPS measurements reveal that the oxygen vacancies introduced critical midgap defect states primarily derived from Nb 4d orbitals, which not only extended light absorption but also dramatically enhanced carrier separation by trapping photogenerated electrons at the Nb4+ sites. In situ FT-IR and Raman spectroscopy provide real-time evidence of this superior kinetics; while pristine SrNb2O6 suffers from a sluggish conversion of *COOH intermediates (1595 cm−1), the SrNb2O6−x-3 sample facilitates a rapid transition from CO2 to CO, preventing surface poisoning (Fig. 22g and h). As illustrated in the proposed mechanism (Fig. 22i), the Sr2+ Lewis acid site captures CO2 through its empty 5s orbitals (the “pull”), while the adjacent Nb4+ Lewis base site donates photoinduced electrons to the carbon atom to drive the rate-determining step of *COOH formation. This localized electron accumulation at the Nb sites eventually triggers a charge-repulsive “push” effect, effectively ejecting the produced *CO from the surface. Gibbs free energy calculations confirm this pathway, showing a significantly reduced activation barrier for CO2 hydrogenation (0.57 eV vs. 0.83 eV), establishing a highly efficient catalytic cycle sustained by the PFLP-induced electronic frustration. This work showed that by bridging semiconductor photophysics with the chemical specificity of frustrated Lewis pairs, we can effectively bypass traditional kinetic barriers, managing the delicate balance between reactant activation and product desorption to achieve high-performance catalysis.53
We have discussed examples of studies targeting better utilization of charge carriers, but the first step is the generation of free carriers from excitons. The question is whether we can tune that initial transition, and this is what Xu et al.19 achieved in their work by focusing on the supercritical CO2-induced exciton effect in BiFeO3 for photocatalytic CO2 reduction. While traditional photocatalytic theories often overlook the excitonic aspect of the photoexcitation process, this study posits that the competition between bound excitons and free carriers is a crucial determinant of catalytic performance. By exploring strategies for exciton dissociation through the introduction of structural disorder, the researchers aimed to bridge the gap between initial light absorption and the generation of the free electrons and holes necessary for surface reactions.19
The synthesis utilized a supercritical carbon dioxide (SC CO2) treatment to exfoliate bulk BiFeO3 into ultrathin 2D nanosheets. TEM images confirm the successful transformation into transparent, few-layer structures (Fig. 23a) while the AFM studies showed that the resulting nanosheets possess a thickness primarily between 2.4 and 4 nm, representing roughly 6 to 10 atomic layers. Interestingly, HRTEM and Geometric Phase Analysis (GPA) reveal that the SC CO2 process does more than just exfoliate; it induces a lattice strain. This structural distortion is accompanied by the formation of oxygen vacancies (Ov) as evidenced by XPS and EPR. To probe how these oxygen vacancies alter the fundamental photophysics of the system, the authors employed femtosecond transient absorption spectroscopy (Fig. 23b–d). In the untreated BiFeO3, the TAS spectra exhibit a double-exponential decay, which is characteristic of a system dominated by a large exciton effect where carriers remain largely bound (Fig. 23b and d). However, the sample treated at 12 MPa shows a distinct shift to a triple-exponential decay model (Fig. 23c and d). In this optimized sample, the TAS kinetics reveal a more complex life cycle for the photoexcited species: the initially generated electrons undergo an ultrafast relaxation from the conduction band into exciton-mediated trap states (Fig. 23e). Unlike the bulk material, the presence of oxygen vacancies in the 2D nanosheets provides a second relaxation step where these excitons are effectively “destabilized” and dissociated into free carriers (Fig. 23e). The TA measurements specifically highlight that the 12 MPa-treated sample possesses a longer photoexcitation recovery lifetime compared to those treated at higher pressures (14 and 16 MPa), which showed only double-exponential decay (Fig. 23d). This suggests that there is a precise density of oxygen vacancies required to facilitate this exciton-to-free-carrier transition.
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| Fig. 23 Defect-engineered BiFeO3 for enhanced sunlight-driven CO2 photocatalysis. (a) Low-magnification TEM image of BiFeO3 treated with SC CO2 at 12 Mpa, The 3D plot of fs-TA spectra of (b) untreated BiFeO3, (c) treated BiFeO3 at 12 MPa of SC CO2, (d) the rise portion of the normalized PIA kinetic curves of BiFeO3 treated with SC CO2 under different pressure, near ≈605 nm, (e) schematic diagram of the photophysical process of exciton and OV-mediated trap states, (f) the yield distribution of photoreduction product CO in 1.5 h, (g) the amount of CO produced by CO2 is a function of the irradiation time of BiFeO3 treatment at different pressures, (h) EIS Nyquist plots for BiFeO3, (i) photocurrent responses of BiFeO3. Reproduced with permission from ref. 19. Copyright 2025, American Chemical Society. | ||
The impact of this enhanced exciton dissociation was clearly reflected in the photocatalytic performance and electrochemical evaluation. The BiFeO3 nanosheet was highly selective for the reduction of CO2 to CO, with the 12 MPa-treated catalyst delivering the highest yield (Fig. 23f and g). This peak performance was corroborated by a series of electrochemical tests: the 12 MPa sample exhibited the strongest photocurrent response and a reduced semicircle radius in electrochemical impedance spectroscopy, signifying significantly higher charge transfer efficiency (Fig. 23h and i). While the 2D morphology inherently shortens carrier migration distances, the authors conclude that it is the oxygen vacancy-mediated dissociation, unique to the 12 MPa treatment, that provided the surge in carrier concentration necessary to outperform the samples treated at higher pressures. By successfully bridging ultrafast photophysical insights with tangible catalytic outputs, this work demonstrated that the efficiency of CO2 reduction is not merely a matter of light absorption or surface area, but is fundamentally governed by the ability to engineer defect states that can forcibly decouple bound excitons.19
The cocatalyst offers various opportunities for enhancing CO2 photoreduction efficiency, as we discussed in previous examples. One key property of metal cocatalysts is LSPR. However, the hot carriers produced via the LSPR effect in metal photocatalysts have a much shorter lifetime compared to those generated in semiconductors, making CO2 reduction with H2O more challenging. To solve this problem, combining plasmonic metal nanostructures with semiconductors (such as TiO2) has been a widely used method by which the lifetime of hot charge carriers is prolonged. Kang et al.533 investigated the strong SPR effect of Ag particles anchored on cubic-phase LixTiO2 for the CO2 photoreduction reaction (Fig. 24). This system represents a multifunctional plasmonic–semiconductor heterostructure, where the synergy between a defect-engineered oxide support and a noble-metal cocatalyst is utilized to shift product selectivity toward reduced hydrocarbons. Their study highlighted three significant aspects: First, they successfully synthesized cubic TiO2, which activated the [101] facet. Second, Frenkel defects were introduced into some lattices by incorporating Li+ ions, creating oxygen vacancies. These vacancies increased CO2 adsorption and accelerated the rate-determining step in CO2 reduction, facilitating its conversion to CO, the initial reduction product. The vacancies also helped in decreasing the band gap and charge recombination rate, as shown by the UV-Vis and PL spectra, respectively (Fig. 24d and e). Finally, they enhanced photocatalytic activity by loading Ag nanoparticles onto the LixTiO2 cubic surface (Fig. 24a–c), leveraging SPR effects to selectively convert CO2 to CH4.
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| Fig. 24 Photocatalytic CO2 reduction using the surface plasmon resonance effect of superfine silver nanoparticles anchored on lithium titanium dioxide nanocubes. (a–c) HRTEM images of Ag@Li0.075TiO2 particle and EDS Mapping, (d) Tauc plots of TiO2 and LixTiO2 particles, (e) PL spectra; (f) UV-Vis spectra of LixTiO2 and Ag@LixTiO2 particles, (g) photocurrent curves of TiO2 and LixTiO2 particles, (h) photocurrent of Li0.075TiO2 and Ag@Li0.075TiO2 particles, (i) quantum efficiency obtained from the IPCE spectra according to the irradiation wavelength for LixTiO2 and Ag@Li0.075TiO2 particles, (j and k) catalytic performances for CO2 photoreduction on Li0.075TiO2, and Ag@Li0.075TiO2 particles under UV-light irradiation, (l) IMVS and (m) IMPS curves for Li0.075TiO2 and Ag@LixTiO2 particles, (n) recombination lifetime and (o) electron transport time determined from IMVS and IMPS curves, respectively, (p) expected mechanisms for the photoreduction of CO2 to CH4 on Ag@LixTiO2 particle under UV- and visible light irradiations. Reproduced with permission from ref. 533. Copyright 2018 Elsevier. | ||
Quantitative results revealed that Ag@Li0.075TiO2 particles yielded 49 µmol g−1 of CH4 after 10 hours of reaction under UV light. This represented an 8.2-fold increase compared to cubic TiO2 (6 µmol g−1) and a 1.5-fold increase compared to Li0.075TiO2 (33 µmol g−1). Additionally, the activity remained stable under visible light (420 and 620 nm), producing 42 and 34 µmol g−1 of CH4, respectively, after 10 hours. Without Ag nanoparticles, cubic TiO2 and LixTiO2 exhibited a CH4
:
CO product ratio of approximately 1
:
1, showing no selectivity. However, with Ag loading, the ratio shifted to 3
:
1, favoring CH4 production (Fig. 24j and k). Kang et al.533 attributed the enhanced photocatalytic performance to the LSPR effect of Ag nanoparticles, which is evident by the increase in absorption across visible regions upon loading Ag (Fig. 24f). Under SPR, light trapping on the metal surface and electron excitation into the photocatalyst resulted in significant photocurrent increases (Fig. 24g and h). Specifically, Ag@Li0.075TiO2 exhibited a photocurrent density of 57 mA cm−2 under visible light, 3.5 times higher than Li0.075TiO2, which was attributed to the stable integration of Ag particles with Li0.075TiO2. The HRTEM and elemental mapping confirmed the even distribution of Ag, Ti, and O atoms on the particle surface (Fig. 24a–c).
The study confirmed CH4 as the dominant product under UV and visible light. Using Ag@Li0.075TiO2, approximately 98% CH4 (20 µmol g−1) was produced after 10 hours of reaction under UV light (Fig. 24j and k). The quantum efficiency of Ag@Li0.075TiO2 also increased significantly across wavelengths. Under 365 nm UV light, the quantum efficiency rose from 0.56 for Li0.075TiO2 to 0.85 for Ag@Li0.075TiO2. Similar enhancements were observed under 420 and 620 nm visible light (Fig. 24l).
Impedance measurements as well as intensity modulated photocurrent/photovoltage spectroscopies (IMVS and IMPS) revealed slower electron–hole recombination (Fig. 24n) and faster electron transport times (Fig. 24o) in Ag@Li0.075TiO2 compared to Li0.075TiO2, attributed to the electron trapping and plasmonic resonant energy transfer properties of Ag. Mechanistically, under UV irradiation, LixTiO2 absorbed UV light, transferring electrons from its valence band to the conduction band. Ag trapped these electrons, maintaining charge separation. CO2 was reduced at the conduction band or Ag surface to CO or CO2− intermediates, which further reacted with protons to form CH4. Under visible light, Ag absorbed photons and transferred electrons to the LixTiO2 conduction band via SPR, reducing CO2 (Fig. 24p). This work provided a comprehensive framework for leveraging SPR effects, oxygen vacancies, and cubic morphology to improve the efficiency and selectivity of CO2 photoreduction reactions.
A cocatalyst can also be loaded onto a semiconductor using a precursor, forming a hybrid Z-scheme-metal cocatalyst system. For instance, Yong et al.534 developed a visible-light-active silver halide (AgX, where X = Cl or Br) photocatalyst by depositing it onto protonated graphitic carbon nitride (pCN) through a sonication-assisted deposition–precipitation method at room temperature (Fig. 25). This system is also an example of a multifunctional plasmonic–semiconductor heterostructure. Photoreduction of the silver halides resulted in the formation of Ag as a plasmonic metal cocatalyst. The choice of halide ions influenced the band energies and the electron dynamics of the system.
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| Fig. 25 Photocatalytic CO2 reduction over heterostructured AgX/g-C3N4 nanocomposites. (a) EDX mapping of C, N, Ag, Br, and Cl elements for AgBr/pCN. Insets show the corresponding FESEM images of the AgBr/pCN sample for elemental mapping, (b and c) UV-Vis absorption spectra of the as-synthesized samples: AgBr/pCN and AgCl/pCN hybrid heterostructures. Insets show the digital photographs and the enlarged region of visible light absorption of the samples, (d) time dependence of the rate of CH4 production over pure g-C3N4, 30AgBr/pCN and 30AgCl/pCN samples, (e) PL spectra of pCN and AgBr/pCN hybrid heterostructures, (f) PL spectra of 30AgBr/pCN, 30AgBr/pCN-M and 30AgCl/pCN samples, (g) XPS survey (Ag 3d) spectra of the 30AgBr/pCN before and after the photocatalytic reaction, (h) schematic illustration of the band structures of Ag/AgCl/pCN and Ag/AgBr/pCN hybrid nanocomposites for the photoreduction of CO2 with H2O to CH4 under the light irradiation. Reproduced with permission from ref. 534. Copyright 2016 Elsevier. | ||
The photocatalytic performance was tested for CO2 reduction to CH4 under low-power daylight bulb illumination at ambient conditions. The 30AgBr/pCN nanocomposite demonstrated superior photocatalytic activity, producing CH4 at 10.92 µmol per g catalyst, outperforming both single-phase AgBr and pCN by factors of 34.1 and 4.2, respectively (Fig. 25d). Additionally, the performance of AgBr/pCN was 1.3 times higher than AgCl/pCN, attributed to enhanced surface plasmon resonance effects and a heterojunction structure that facilitated efficient charge transfer and separation.
Structural characterization showed that AgX crystals transformed into nanoparticles on the pCN surface, as confirmed by FESEM and TEM. EDX mapping revealed a uniform distribution of elements, including C, N, Ag, Br, and Cl (Fig. 25a). The incorporation of AgX nanoparticles did not significantly alter the absorption edge of pCN but slightly enhanced its visible-light absorption. The band gap energy of AgBr (2.6 eV) enabled it to absorb more visible light compared to AgCl (3.2 eV), contributing to better photocatalytic performance (Fig. 25b and c).
Photoluminescence analysis indicated that 30AgBr/pCN effectively suppressed electron–hole recombination, which was not the case with physically mixed samples, correlating its high photocatalytic activity with efficient charge transfer (Fig. 25e and f). After multiple reaction cycles, XPS analysis confirmed a partial reduction of AgX to metallic Ag, enhancing the SPR effect (Fig. 25g). The hybridization of AgX with pCN created heterojunction interfaces, with AgBr forming a Type II heterojunction that facilitated spatial separation of charge carriers. This configuration improved charge transfer efficiency and suppressed recombination, driving the reduction of CO2 to CH4 through the well-aligned energy bands of pCN, Ag, and AgBr (Fig. 25h). The thermodynamic properties of AgBr, including a conduction band potential more negative than the CO2/CH4 reduction potential, allowed effective electron transfer to reduce CO2. Concurrently, the oxidation of H2O provided protons for the reaction, completing the photocatalytic cycle. These advancements underline the significance of AgX incorporation in improving photocatalytic efficiency and product yield.534
LSPR not only generates excited charge carriers in plasmonic metals but also enhances the electric field, significantly influencing photocatalytic reactions. Zou et al.535 demonstrated this with Au@TiO2 yolk–shell hollow spheres, where an electric field generated by LSPR boosted electron–hole pair generation, suppressed charge recombination, and improved the CO2 photoreduction yield. This system is an example of a plasmonic–semiconductor heterostructure. The LSPR-induced electromagnetic field around Au nanoparticles enhanced the separation of charge carriers in the TiO2 shell, enabling the formation of high-grade hydrocarbons like ethane (C2H6), rarely seen in prior CO2 reduction systems.
This study highlights the importance of LSPR-mediated electric fields in driving multi-electron and proton transfer reactions, a crucial step toward producing valuable carbon species. The researchers synthesized Au@TiO2 yolk–shell hollow spheres (Fig. 26a and c). Optical analysis showed a significant red-shift in the LSPR peak (575 nm) of Au@TiO2, compared to bare Au nanoparticles (540 nm), due to the high refractive index of TiO2 (Fig. 26b). Under UV-visible light, bare TiO2 hollow spheres exhibited moderate activity for CO2 photoreduction (CH4: 1.33 µmol g−1 h−1). In contrast, Au@TiO2 enhanced CH4 production (2.52 µmol g−1 h−1) and facilitated C–C coupling to generate ethane (C2H6: 1.67 µmol g−1 h−1) (Fig. 26d). This improvement was attributed primarily to the LSPR-mediated local EM field, which amplified charge carrier generation and reduced recombination losses.
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| Fig. 26 Photocatalytic CO2 reduction over plasmon–semiconductor hybrid Au@TiO2 yolk–shell hollow spheres. (a) TEM images, (b) UV-Vis diffuse reflectance spectra of TiO2 hollow spheres and Au@TiO2 yolk–shell hollow spheres, (c) schematic for the mechanism of CO2 reduction, (d) comparison of photocatalytic activity for CO2 reduction over P25, TiO2 hollow spheres, and Au@TiO2 yolk–shell hollow spheres, (e) photocurrent responses as a function of light intensity and transient decay lifetime of surface trap states, (f) the spatial distribution of local EM field enhancement on the x–y plane for Au@TiO2 yolk–shell hollow spheres from an FDTD simulation, (g and h) photocurrent responses, (i) the comparison of photocurrent of Au@TiO2 yolk–shell hollow spheres TiO2 and hollow spheres with light intensity of 128 mW cm−2, the table is the transient decay lifetime of surface trap states of Au@TiO2 yolk–shell hollow spheres and hollow spheres under light irradiation with different intensities. Reproduced with permission from ref. 535. Copyright 2015 Royal Society of Chemistry. | ||
The study also ruled out significant electron transfer between Au and TiO2 due to the minimal contact between the yolk and shell. Instead, the enhanced photocatalytic activity was driven by the intense local electric field generated by LSPR. The FDTD simulations confirmed that the electric field strength was highest near the Au nanoparticles, leading to a localized increase in charge carrier density within the TiO2 shell (Fig. 26f). This field concentration promoted the dimerization of CH3 radicals, favoring C–C coupling and ethane formation. Regions farther from the Au core primarily facilitated CH4 generation due to insufficient ˙CH3 radical concentration. The photocurrent response further validated the role of the LSPR effect. Au@TiO2 exhibited a significant enhancement in photocurrent compared to bare TiO2, confirming increased charge carrier generation (Fig. 26e and g–i). This work highlights the potential of plasmonic nanostructures like Au@TiO2 in photocatalytic CO2 reduction, offering insights into designing catalysts for artificial photosynthesis. By leveraging LSPR to enhance charge dynamics and promote complex reaction pathways, researchers can pave the way for efficient solar-driven fuel production systems.535
The previous study established the role of electric field enhancement in driving CO2 photoreduction. In another study, Long et al.536 demonstrated the long-range redox reactivity of plasmon-generated hot electrons from gold nanorods for solar-driven CO2 conversion. They designed a series of Au NR@ZnO core–shell photocatalysts with tunable shell thicknesses to achieve efficient solar-to-CH4 conversion, where hot electrons drive the photoreduction on the polar ZnO shell (Fig. 27). This system is an example of a multifunctional plasmonic–semiconductor heterostructure. Polar ZnO was selected as an electron acceptor for two main reasons: its surface polarity deforms CO2 and lowers its LUMO level, and its abundant hydroxyl groups and Brønsted acidic protons near CO2 adsorption centers aid the CH4 generation. This prevented the formation of CO2− species and thermodynamically favored CH4 production under solar light. Au NR@ZnO samples were synthesized using a low-temperature solution process, with varying precursor ratios enabling control over ZnO shell thickness (Fig. 27a). SEM and TEM images confirmed clear boundaries between the Au core and ZnO shell, with an average Au NR aspect ratio of 3
:
1 (Fig. 27b). Photocatalytic activity tests revealed that the highest CH4 and CO production rates were 17.12 µmol h−1 (gAu)−1 and 32.4 µmol h−1 (gAu)−1, respectively (Fig. 27d–f). When normalized to ZnO content, the activity variation across different shell thicknesses was minimal, confirming that ZnO thickness did not directly affect photocatalytic efficiency (Fig. 27e). Under visible light, CH4 was the primary product, while CO was exclusively produced under ultraviolet light, illustrating that the Au core and ZnO shell synergistically enhance photocatalytic activity (Fig. 27f).
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| Fig. 27 Photocatalytic CO2 reduction over plasmon–semiconductor hybrid Au NR@ZnO core–shell nanostructures. (a) The schematic diagram of the fabrication procedure of Au NR@ZnO samples, (b) TEM image of Au NR@ZnO-130 sample, (c) UV-Vis spectrum, (d) shell thickness-depended photocatalytic activity of Au NR@ZnO-x samples for photocatalytic reduction of CO2 under solar light irradiation, (e) different catalysts, (f) under different light irradiation, (g) schematic description of the generation, injection and long-range reactivity of hot electrons for the solar-to-hydrocarbon conversion, (h) the EPR spectra of Au NR@ZnO and pure ZnO samples dispersed in DMPO and methanol solution under solar light irradiation, (i) the photocurrent–time curves of Au NR@ZnO and pure ZnO samples, (j) transient absorption spectra of the Au NR@ZnO after excitation by 400 nm pulse. Electron decay kinetics at (k) 534 nm, (l) 688 nm. Reproduced with permission from ref. 536. Copyright 2020 Wiley-VCH GmBH. | ||
Transient absorption spectroscopy provided detailed insights into the charge transfer dynamics in the Au NR@ZnO system (Fig. 27j). In the steady-state UV-Vis spectrum, two characteristic plasmon peaks corresponding to the transverse and longitudinal modes of Au NRs were observed at 534 nm and 688 nm (Fig. 27c). Upon encapsulation with ZnO, a blue shift in the longitudinal peak was noted, attributed to changes in the surrounding dielectric constant. In the transient absorption spectra, bleaching at 534 nm and 688 nm confirmed the excitation of plasmon modes, while a red-shifted positive absorption peak at 470 nm indicated a volume expansion of the hot particles, reducing electron density and plasmon frequency (Fig. 27j). A significant blue shift in the bleach at 534 nm, reaching up to 130 meV, was much larger than that observed for pure Au NRs (0.15 meV). This indicated a strong interaction between the Au core and ZnO shell, suggesting efficient coupling and charge transfer.
The recovery of plasmon bleach signals provided critical data on electron relaxation dynamics. At 534 nm, the bleach recovery followed a monoexponential decay with a relaxation time of 2.1 ps, corresponding to electron–phonon interactions. Similarly, the relaxation time at 688 nm was significantly longer than that of pure Au NRs (<1 ps), highlighting the prolonged lifetime of hot electrons in the Au NR@ZnO system (Fig. 27k and l). This extended lifetime enhances the likelihood of photoexcited electrons participating in catalytic reactions (Fig. 27g).
Spin trap EPR confirmed the generation of ˙O2− and ˙CH2OH radicals, further supporting the involvement of photoinduced electrons (Fig. 27h). Electrochemical analyses demonstrated a twofold enhancement in photocurrent and a reduction in charge transfer resistance for Au NR@ZnO compared to pure ZnO (Fig. 27i). The well-distributed Au NR@ZnO core–shell structure exhibited strong synergistic effects for CO2 photoreduction. The LSPR of Au NRs extended light absorption into the visible range, driving the eight-electron CO2 reduction reaction for CH4 generation. While ZnO shell thickness did not influence the production rate, its role in prolonging electron lifetimes enhanced overall efficiency. This work highlights the potential of the Au NR@ZnO system for solar-driven CO2-to-hydrocarbon conversion.536
The research on semiconductor-plasmon hybrid systems highlights a significant gap in the understanding of purely plasmonic photocatalysts for artificial photosynthesis. Zhao et al.459 demonstrated that quantum-sized Au NPs were capable of photocatalytically reducing CO2 to CO using H2O under low-intensity irradiation at 420 nm (Fig. 28). This is an example of a purely plasmonic metal-catalysed process. This process utilized electron–hole pairs generated predominantly from interband transitions, leading to a CO production rate of 4.73 mmol g−1 h−1 with ∼100% selectivity. This rate was approximately 2.5 times higher than that observed during CO2 reduction with H2 under similar conditions. The enhanced activity is attributed to surface Au–O species formed during H2O decomposition, which improved rate-determining steps, reduced energy barriers for *CO desorption and *OOH formation, and facilitated the production of CO and O2.
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Fig. 28 Photocatalytic CO2 reduction over Au nanoparticles by interband transitions. (a) TEM image, (b) particle size distribution of Au NPs, (c) UV-Vis absorption spectrum of the Au NPs with interband and intraband absorption, (d) schematic diagram of interband and intraband (LSPR) transitions, (e) CO and O2 productions over Au NPs with 420 LED light irradiation at 200 °C, (f) wavelength-dependent AQEs of the Au photocatalyst, (g) the reaction temperatures and (h) light intensity-dependent CO production rate on Au NPs under 420 nm LED light irradiation, (i) valence-band XPS spectrum of Au, (j) schematic illustration for the electronic band structure of the ∼4 nm Au NPs, (k) photocatalytic CO2RR performance on Au NPs with H2O or H2 under 420 nm light illumination at 200 °C. The volume ratio of H2 to CO2 is 4 : 1 in the gas mixture, (l) 1H ssMAS-NMR spectra of Au samples before (black curve) and after CO2RR (3 h reaction, red curve). Reproduced with permission from ref. 459. Copyright 2022 Springer Nature. | ||
In contrast to the LSPR effect, the hot electron–hole pairs derived from interband transitions exhibit higher redox potentials and longer lifetimes. These features are advantageous for H2O oxidation and CO2 reduction. The quantum-sized Au NPs (∼4 nm) (Fig. 28a and b) with unique interband excitations under visible light irradiation demonstrated their potential for photocatalytic CO2 conversion. Their UV-Vis absorption spectrum spanned 320–800 nm, with a small peak at 520 nm attributed to the LSPR effect, while the dominant interband absorption band extending to 800 nm results from 5d–6sp transitions (Fig. 28c).
Theoretical calculations revealed two types of interband excitations: transitions from the 5d band to states near the Fermi level and transitions to unoccupied 6sp band states above the Fermi level (Fig. 28d). Under monochromatic LED light at 420 nm, photocatalytic experiments achieved CO evolution of up to 4.73 mmol g−1 h−1 and O2 evolution of 1.98 mmol g−1 h−1 (Fig. 28e). The apparent quantum efficiency peaked at 520 nm due to LSPR-enhanced light absorption, although interband transitions at shorter wavelengths also contributed significantly, confirming that the CO2-to-CO conversion process is driven mainly by interband-generated hot electrons (Fig. 28f).
Time-resolved photoluminescence analysis showed a carrier lifetime of ∼0.2 ns, which was much longer than the ∼30 fs typical of LSPR-generated carriers. This extended lifetime facilitated efficient charge transfer, improving photocatalytic activity. The photothermal effect on catalytic CO2 reduction using Au NPs was negligible because the 420 nm LED light used (73 mW cm−1) had a low intensity, even lower than solar intensity. The sample temperature only increased from 24 °C to 33 °C under irradiation. Therefore, CO2-to-CO conversion on Au NPs was likely driven by photogenerated electrons (Fig. 28h). However, a linear increase in the photocatalytic CO production rate with reaction temperature (Fig. 28g) suggested that heat input enhanced the photocatalytic CO2 reduction activity, likely due to the higher populations of adsorbates in excited vibrational states at elevated temperatures. Valence-band XPS spectra demonstrated that the electronic band structure of Au NPs was well-suited for CO2 reduction and H2O oxidation (Fig. 28i). Specifically, the hot electron energy under 420 nm light was more positive than the reduction potential of CO/CO2, while the hot hole energy was more negative than the oxidation potential of O2/H2O, enabling simultaneous CO2 reduction and H2O oxidation (Fig. 28j). In situ FTIR spectroscopy revealed the accumulation of surface-adsorbed H2O and *COOH species on the Au surface during the reaction. Replacing H2O with H2 resulted in a halving of the CO yield, underscoring the critical role of H2O in the CO2 reduction process (Fig. 28k). Further analysis using solid-state NMR and other techniques showed that immobilized H2O dissociates into *OH species on the Au surface under illumination, forming Au–O species that enhanced the efficiency of CO2 reduction (Fig. 28l).
The proposed reaction mechanism involves photogenerated hot electrons and holes driving the dissociation of H2O and the reduction of CO2. Theoretical and experimental findings collectively highlight the importance of interband transitions and surface Au–O species in improving the efficiency of CO2 reduction using quantum-sized Au NPs and H2O. These insights offer a promising direction for the development of purely plasmonic photocatalysts for artificial photosynthesis.459
Throughout the preceding sections of this review, we have emphasized that the localized electric field inherent to plasmonic systems is not merely a secondary consequence of excitation, but a primary driver of catalytic performance. Further expanding on this idea, Xiong et al.412 demonstrated the critical role of these near-field effects in achieving high-efficiency, broadband artificial photosynthesis using an Au-rod/CuPd-alloy core–shell architecture. This architecture represents a bimetallic core–shell plasmonic heterostructure. By utilizing the intense localized electric field at the CuPd surface, the authors successfully utilized low-energy NIR photons to drive the multielectron reduction of CO2 to CH4 with nearly 100% selectivity.
This catalyst design strategically positions the CuPd alloy shell as a dual-function cocatalyst that simultaneously captures CO2 molecules and positions them within the most intense regions of the plasmon-induced local field (Fig. 29a). The synthesis involved the epitaxial growth of a single-crystal CuPd shell onto Au nanorods, a structure confirmed by the preservation of ordered lattice fringes and reduced coordination numbers in XANES/EXAFS spectra, ensuring that the active Pd and Cu sites were optimally located on the outermost surface. The light-harvesting capability of these core–shell composites was a crucial feature of their performance. The UV-Vis extinction spectra (Fig. 29b and c) revealed characteristic transversal and longitudinal LSPR modes at 510 and 740 nm, respectively. Crucially, the researchers found that precise control of the CuPd shell thickness enabled a significant broadening of the absorption profile into the NIR region. This ensured that the high-density CO2 adsorbates were continuously energized by enhanced local fields across the entire solar spectrum, bridging the gap between light absorption and molecular transformation.
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| Fig. 29 Photocatalytic CO2 reduction over Au-rod/CuPd-alloy core–shell photocatalyst. (a) Schematic illustration of the role of CuPd cocatalyst in capturing CO2 molecules. UV-Vis extinction spectra of Au rod and Au rod@CuPd with (b) different CuPd shell thicknesses and (c) different Cu/Pd molar ratios, (d) average production rates of CH4 over Au rod@CuPd2 with different shell thicknesses, (e) calculated AQEs (color dots) over Au rod@CuPd2 under different monochromatic light illumination, in reference to its UV-Vis extinction spectrum (black line). In situ NAP-XPS contour plot of (f) Cu 2p3/2 and (g) Pd 3d5/2. The squares and lines in black and white indicate unilluminated and illuminated conditions, respectively. (h) The projected density of states of CO2 adsorbed on a CuPd (100) surface in the absence (left) and presence (right) of electric field pointing toward the surface. The main quasi isolated trap states are marked with orange asterisks. Reproduced with permission from ref. 412. Copyright 2023 Springer Nature. | ||
The CH4 production rate exhibited a volcano-shaped dependence on the CuPd shell thickness, highlighting a critical optimization threshold where the density of surface active sites was maximized without inducing excessive electron–phonon scattering (Fig. 29d). The AQE profile also displayed a nearly perfect overlap with the Au-rod LSPR extinction spectrum, providing insight into the role of low-energy NIR photons in driving the multielectron reduction process (Fig. 29e). To understand the how low-energy photons overcome the energy barrier to carry out the reaction, the authors utilized in situ near-ambient pressure X-ray photoelectron spectroscopy (NAP-XPS) and monitored electronic fluctuations in real-time. The analysis of the Cu 2p and Pd 3d core levels (Fig. 29f and g) revealed a distinct three-stage electronic response under illumination: a fast, reversible accumulation of hot electrons above the Fermi level, coupled with a slower, irreversible photoreduction of the metal sites. This dual-process enrichment, characterized by an instantaneous decrease in binding energy upon light exposure, effectively elevated the chemical potential of the catalytic surface, thereby benefiting catalysis.
The authors then performed DFT calculations on the PDOS, which revealed that the localized electric field played a transformative role in CO2 activation (Fig. 29h). The field induced the emergence of quasi-isolated trap states above the Fermi level, which extended the lifetime of hot electrons and facilitated a multiphoton absorption process. This allowed electrons to be re-excited by consecutive NIR photons until they gain sufficient energy to trigger the CO2RR. Furthermore, natural orbitals for chemical valence (NOCV) analysis demonstrated that the electric field dictated a highly selective orbital-specific electron redistribution. When the field pointed toward the surface, electrons were specifically driven into the antibonding π* orbitals of CO2, weakening the C–O bond and increasing its length. In contrast, the field provided negligible assistance for O–H bond cleavage in H2O molecules. The assistance of the local electric field in facilitating the directional electron transfer to CO2 molecules resulted in nearly 100% selectivity toward hydrocarbons.
The authors further improved the efficiency of the process by designing a spherical gas–solid reactor, which recaptured and reflected scattered light onto the catalyst surface. This architectural optimization facilitated enhanced multiphoton absorption, resulting in a CH4 production rate of 0.55 mmol g−1 h−1. This study used a unique idea of “orbital tuning” by the local field, which effectively overrides competing reaction pathways, establishing a sophisticated method for selective artificial photosynthesis using low-energy photons.412
The thermal DRM process has been extensively studied over the past few decades. However, the high temperatures required (600–1000 °C) and the massive energy consumption involved lead to the re-emission of CO2, as fossil fuels are burned to generate the necessary heat. To overcome these challenges, photo-assisted DRM has emerged as a promising alternative.223,542–553 This approach relies on innovative nanoscale catalyst designs that are crucial for effective sunlight harvesting while also being resistant to coke formation.
Despite the wide band gap of many semiconductors favoring catalytic reactions thermodynamically, it also limits the conversion efficiency of solar irradiation. For instance, traditional TiO2 can only utilize UV photons. However, Hu et al.552 introduced black TiO2, which featured broad-spectrum absorption, making it suitable for harvesting visible light, which constitutes the majority of natural solar irradiation (Fig. 30). The visible light absorption in black TiO2 was attributed to deep energy wells created by oxygen vacancies in the lattice (Fig. 30c) or the presence of Ti3+ in hydrogenated rutile TiO2. These defects created a donor level approximately 1.30 eV below the CB edge, which aligned with the energy of visible photons.
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| Fig. 30 Photocatalytic dry reforming of methane over defected semiconductor-cocatalyst system Pt/black TiO2. (a)TEM image of Pt/black TiO2 catalyst, (b) CO yields from CRM over Pt/black TiO2 catalyst dispersed on the light-diffuse-reflection surface of a SiO2 substrate, (c) EPR of the catalysts, (d) QE versus wavelength (λ), (e) relationship between band structure of black TiO2 and redox potentials of CO2 reforming of CH4 (CRM). Reproduced with permission from ref. 552. Copyright 2016 American Chemical Society. | ||
Although the CO2/CO redox potential is marginally more negative than the TiO2 conduction band edge at room temperature, it shifts to a more positive value above 150 °C, surpassing the CB edge and thereby favoring CO2 reduction to CO at elevated temperatures. The redox potential of CO/CH4, however, remained more negative than the energy level of Ti3+ at room temperature and above, satisfying the energy requirement for CH4 oxidation to CO (Fig. 30e).
Furthermore, platinum was incorporated into the TiO2 via impregnation, serving as an active site due to its high conductivity (Fig. 30a). Under illumination with AM 1.5, the photo-driven yields after subtracting thermal contributions) of H2 and CO (after subtracting thermal contributions) reached 95 and 191 mmol gcat−1 h−1 at 550 °C, 135 and 299 mmol gcat−1 h−1 at 650 °C, and 208 and 258 mmol gcat−1 h−1 at 700 °C (Fig. 30b). The higher CO yield compared to H2 resulted from the reaction between CO2 and H2, which consumed H2 while producing CO. The relationship between quantum efficiency and wavelength further demonstrated that wavelengths from 395 nm to 950 nm contributed to photo-assisted DRM (Fig. 30d). In this way, the integration of a Pt/black TiO2 catalyst with a light-diffusing SiO2 substrate surface resulted in a highly efficient visible light photocatalytic process for CO2 reforming of methane. This approach achieved photo CO and H2 yields that were 1000 times greater than previously reported values.552
Another wide-band gap semiconductor, Strontium titanate (SrTiO3 or STO) has been explored by Miyayuchi et al.553 as a photocatalyst for the DRM reaction (Fig. 31). However, its efficiency is generally low due to rapid electron–hole recombination. The deposition of highly dispersed Rh nanoparticles on STO (Fig. 31a) dramatically increased the catalytic activity, achieving a hydrogen production rate of 4.5 µmol min−1 under visible light illumination(Fig. 31b). This rate significantly surpassed the limitations of thermocatalysis, indicating the involvement of hot-carrier chemistry alongside the photothermal effect under illumination. Additionally, the wavelength-dependent activity showed that the reaction was particularly enhanced at wavelengths below 380 nm, which corresponded to the band gap energy of STO (3.2 eV) (Fig. 31c). This finding supported the hypothesis that the DRM reaction was primarily driven by the band gap excitation of STO.
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| Fig. 31 Photocatalytic dry reforming of methane over doped semiconductor-cocatalyst Rh/STO system. (a) A magnified HAADF-STEM image of Rh/STO, (b) Rh/STO under light irradiation (red squares), the limitation of the thermal system for DRM when using a generic catalyst (dashed line), Rh/STO under dark conditions (grey line with white diamonds) and bare STO under light irradiation (green line with green triangles), (c) UV-Vis spectrum of Rh-STO (F: optical absorption drawn by blue line) and action spectrum of DRM activity (red circles), (d) EPRspectroscopy of Rh/STO under light irradiation in N2, CO2 or CH4/CO2 atmosphere conditions, (e) Kelvin probe force microscope (KPFM) analysis on the Rh loaded STO single crystal (110), before UV light irradiation (left), and during UV light irradiation (right), (f) a band diagram that shows generation of electron–hole pairs in STO and expected redox reactions, (g) schematic dynamics of charge carriers and oxygen ions. Reproduced with permission from ref. 553. Copyright 2020 Springer Nature. | ||
Kelvin probe force microscopy (KPFM) analysis of an STO single crystal with a (110) facet covered with Rh nanoparticles revealed a more pronounced Fermi-level upshift in STO than in the Rh nanoparticles under photo illumination (Fig. 31e). This difference in Fermi-level shift further promoted electron transfer from STO to Rh. In the synthesized Rh/STO composite nanoparticles, photoillumination led to STO domains with concentrated holes and Rh domains with concentrated electrons. The presence of holes in the photoexcited STO domains was confirmed through in situ EPR at −173 °C (Fig. 31d). EPR signals observed around g = 1.97–1.99 and 2.01 corresponded to trapped electrons (Ti3+ species) and trapped holes (O−), respectively. While trapped hole peaks in the valence band of STO were clearly detected in both Rh/STO and bare STO under ultraviolet irradiation, trapped electron signals in the conduction band were absent in Rh/STO, suggesting that the excited electrons in STO's conduction band were injected into the rhodium particles.
These injected electrons in rhodium facilitated charge separation (Fig. 31f and g) and were trapped by CO2 to produce CO. The remaining O2− ions were integrated into the STO lattice, as verified by isotope trace analysis. Meanwhile, the photogenerated holes in STO's valence band migrated to the rhodium interface, where they reacted with CH4. The O2− ions from CO2 and the holes near the STO-rhodium interface further react with methane to produce H2. This process also eliminated residual carbon from methane cracking by reacting it with oxygen ions generated during CO2 reduction, resulting in stoichiometric products and conferring highly stable anti-coking properties. The trapped holes in STO domains accelerated CH4 oxidation, enhancing the DRM reaction. Remarkably, the Rh/STO composite nanoparticles retained their catalytic activity and morphology even after 10 hours of reaction under light illumination.553
Halas et al.223 synthesized plasmonic Cu nanoparticles decorated with single-atom Ru (SA-Ru) and investigated their potential for the DRM reaction (Fig. 32). This design is an example of antenna–reactor geometry. The low Ru loading in these composite nanoparticles did not affect the surface plasmon resonance of the Cu nanoparticles. This design leveraged both the photothermal effect and hot-carrier chemistry of the SA-Ru/Cu system to enhance the DRM reaction.
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| Fig. 32 Photocatalytic dry reforming of methane over Cu-single atom Ru antenna reactor system. (a) Schematic of a Cu-single-atom Ru surface alloy catalyst with the dry reforming reactants and products shown on the left, (b) reaction rate and long-term stability of photocatalytic DRM under 19.2 W cm−2 white light illumination as a function of Ru concentration of the photocatalyst nanoparticles, (c) long-term stability (filled circles), and selectivity (open circles) for photocatalysis, (d) schematics of enhanced selectivity and stability in photocatalysis via the DIET mechanism. Reproduced with permission from ref. 223. Copyright 2020 Springer Nature. | ||
Under white light illumination (19.2 W cm−2) without external heating, the catalytic activity of the SA-Ru/Cu nanoparticles significantly increased with higher SA-Ru loading (Fig. 32b). This enhancement was attributed to the local electronic inhomogeneity at the reactor site, which could facilitate hot-carrier generation. The system achieved a turnover frequency of 34 mol H2 mol Ru−1 s−1 and demonstrated photocatalytic stability over 50 hours. The combination of the single-atom doped structure and hot-carrier generation was proposed to be critical for achieving high efficiency and coking resistance. Adding a minimal fraction of Ru (Cu19.95Ru0.05) nearly tripled the initial photocatalytic reaction rate compared to pure Cu nanoparticles, and significantly improved stability, maintaining 90% of the initial activity after 5 hours of continuous operation. Raman spectroscopy indicated reduced coke formation, and the Cu19.95Ru0.05 sample showed increased selectivity for the DRM process by promoting the DRM rate and suppressing the reverse water–gas shift (rWGS) reaction (Fig. 32a).
When comparing thermocatalytic and photocatalytic activities, it was found that the photocatalytic reaction rate under white-light illumination was more than four times higher than the thermocatalytic rate at the same surface temperature of 1000 K, suggesting that the primary mechanism for photocatalytic DRM was hot-carrier-mediated (Fig. 32c). Thermocatalytic activity rapidly declined due to coking, while photocatalysis remained stable. The incorporation of plasmon-enhanced H2 desorption induced by electronic transitions (DIET),554,555 likely contributed significantly to the improved selectivity and stability observed in photocatalysis compared to thermocatalysis. The suppression of the rWGS reaction through enhanced H2 desorption prevented water formation, leading to a higher concentration of mobile Oads species capable of effectively scavenging Cads upon illumination (Fig. 32d). These combined effects highlighted the effectiveness of the SA-Ru/Cu system in facilitating efficient and stable photocatalytic DRM processes under light irradiation without external heating.223
In the previously discussed work, the light intensity needed to drive the reaction was quite high, around 19.2 W cm−2, possibly leading to temperatures reaching approximately 1000 K.223 This made it difficult to distinguish between non-thermal and photothermal effects. However, recent advancements have led to the development of a Ni–Co-loaded plasmonic catalyst for photocatalytic DRM that requires lower light power. Wang et al.556 fabricated a series of ultra-small, non-noble NiCo bimetallic quantum dots on SiO2 to study their thermal and photothermal catalytic performance in DRM (Fig. 33). This design is an example of antenna–reactor geometry. It was found that partially substituting Ni with Co in the NiCo alloy (Fig. 33a) reduced the thermocatalytic DRM performance. However, in situ irradiation DRIFTS, in situ irradiation EPR, and finite element method simulations showed that energetic hot carriers were excited in NiCo/SiO2, which directly activated CO2 and CH4. This helped overcome the thermodynamic barrier and promoted the generation of *CHO for CO rather than *C, thereby avoiding coking.
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| Fig. 33 Photocatalytic dry reforming of methane over NiCo antenna–reactor system. (a) HRTEM image of 1.2Ni-0.3Co/SiO2, (b) photo contribution to photothermal catalytic DRM performance at the external heating temperature of 700 °C, (c) UV-Vis spectra of the prepared samples, (d) DRM performance with light on and off (700 °C) each cycle corresponds to a 20 min duration for GC monitoring of the effluent products, (e) in situ EPR of 1.2Ni-0.3Co/SiO2 in the presence of CO2 under light illumination and in the dark using 5,5-dimethyl-1-pyrroline-N-oxide (DMPO) as the trapping agent, (f) FEM profiles of enhanced electric fields over monometallic and bimetallic catalysts, (g) photothermal effect on the NiCo bimetal alloy catalyst. Reproduced with permission from ref. 556. Copyright 2023 American Chemical Society. | ||
The NiCo alloy QDs were ultra-small, with an average size of less than 3 nm (Fig. 33a). The binding energy of Co shifted downwards while that of Ni shifted upwards in NiCo/SiO2, indicating electron donation from Ni to Co within the NiCo alloy QDs. For bimetallic NiCo catalysts, the light absorption capability was further enhanced, particularly for 1.2Ni-0.3Co/SiO2, which exhibited maximum light absorption (Fig. 33c). The synergy in the bimetal alloy improved photon absorption, leading to increased generation of energetic hot carriers. While 1.5Ni/SiO2 demonstrated the highest thermocatalytic DRM performance among all the samples, Co in the bimetallic alloy suppressed the activation of CO2 and CH4, as confirmed by DRIFTS and DFT analyses. In these analyses, the carbonate peaks corresponding to CO2 adsorption were lower in the bimetallic catalyst. Trends in reactant adsorption and CO desorption energies supported similar conclusions. Interestingly, 0.3Ni-1.2Co/SiO2, which was inactive in thermocatalysis, was able to trigger the reaction upon light illumination (Fig. 33b and d), demonstrating a strong synergistic effect within the bimetal alloy under light irradiation despite its negative effect on thermocatalytic DRM.
The primary driving force for photothermal catalytic DRM over 1.5Ni/SiO2 remained thermal energy, which enhanced the reaction rate without altering the reaction pathway. However, for 1.2Ni-0.3Co/SiO2, a distinct peak centered at 1238 cm−1 emerged under light irradiation, which was absent during thermocatalysis. This peak was attributed to the presence of the reactive intermediate CO2−. In situ EPR under light illumination also confirmed the presence of CO2− in the photothermal catalytic DRM process, as noticeable EPR peaks were observed when 1.2Ni-0.3Co/SiO2 was illuminated in the presence of CO2, but these peaks were absent in the dark (Fig. 33e). This provided strong evidence that energetic hot carriers were excited on 1.2Ni-0.3Co/SiO2, directly activating CO2 in the photothermal catalytic DRM process.
Additionally, heat on the surface of metal nanoparticles is generated by the decay of low-energy hot electrons. The highest temperature observed in the 1.2Ni-0.3Co/SiO2 sample suggested the greatest number of excited hot carriers on the bimetallic QDs, leading to the maximum probability of energetic hot carriers. FEM simulations were conducted to study the electric field distribution of monometallic and bimetallic catalysts (Fig. 33f), providing a better understanding of the excitation of energetic hot carriers on the bimetallic catalyst. The results indicated that the intensity of the electric field, and therefore the density of high-energy electrons, was consistently higher in NiCo bimetallic catalysts compared to Ni and Co monometallic catalysts irradiated at different light wavelengths and resulted in higher photocatalytic performance (Fig. 33g). The work was crucial in understanding how reaction pathways can change for photocatalytic and thermocatalytic systems.556
This section reviewed photocatalytic DRM over semiconductor and plasmonic catalysts, emphasizing their complementary advantages and practical considerations. Semiconductor systems provide effective charge separation and structural stability, often operating efficiently under moderate illumination, whereas plasmonic systems can harness hot-carrier and photothermal effects, typically requiring higher light intensities to achieve comparable activity. These observations suggest that, while both catalyst classes can drive DRM effectively, rational design of light absorption, carrier dynamics, and cocatalyst integration remains key to optimizing efficiency and selectivity.
N triple bond (941 kJ mol−1).558
The use of water as a hydrogen source could significantly reduce the carbon footprint of NH3 synthesis, but it would require temperatures exceeding 1000 °C in thermal catalysis, making it impractical. Solar energy, abundant in many parts of the world, especially in equatorial regions, offers a promising alternative.559–596 Utilizing solar energy through semiconductor photocatalysis could enable NH3 synthesis under near-ambient conditions. However, most photocatalysts for N2 fixation, similar to those used for photocatalytic CO2 reduction and water splitting, exhibit low activities and poor selectivity. These low rates are due to the slow N2 activation kinetics and the limited availability of charge carriers needed to drive the reduction of adsorbed N2 and water oxidation. As a result, the quantum yields for photocatalytic N2 fixation are low, with solar-to-chemical conversion efficiencies around 0.1%.
Photocatalytic N2 fixation faces greater challenges compared to H2 evolution and CO2 reduction, mainly due to the high-energy intermediates required for N2 reduction, such as N2− or N2H. For example, the reduction potential for N2− formation is as negative as −4.2 V vs. NHE, making it inaccessible for traditional semiconductors (TiO2, ZnO, Fe2O3, and CdS) without the assistance of organic scavengers or precious metal cocatalysts.597–600 Defect engineering has emerged as an effective strategy to enhance the photocatalytic activity of semiconductors by creating defects that serve as trapping centers for electrons and holes and act as active sites for the reaction.
In this context, Zhang et al.601 synthesized {001} facet-exposed BiOBr nanosheets with oxygen vacancies (OVs) using a simple solvothermal method (Fig. 34). A reference photocatalyst without OVs (BOB-001-H) was obtained by annealing BOB-001-OV in an oxygen-saturated atmosphere at 300 °C. BOB-001-H showed no significant NH3 production with or without N2 after 60 minutes, whereas BOB-001-OV produced a significant amount of NH3 (104.2 µmol h−1 gcat−1), and its wavelength-dependent activity closely matched the absorption profile (Fig. 34d). The addition of the electron scavenger AgNO3 significantly suppressed the N2 fixation activity of BOB-001-OV, indicating that the primary active species were the photoexcited electrons.
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| Fig. 34 Photocatalytic N2 fixation over defective semiconductor system BiOBr-OV. (a) SEM image of the as-prepared BiOBr, (b) effect of CO on the photocatalytic fixation of N2 over BOB-001-OV, (c) electronic energy-level diagram of BOB-001-OV, (d) N2 fixation by BOB-001-OV under monochromatic light along with its light absorption spectra, (e) transient photocurrent responses of different BiOBr photocatalysts, (f) room-temperature PL spectra decay curves of the as-prepared BiOBr photocatalysts, (g) schematic illustration for enhanced interfacial electron transfer processes induced by OVs. OVs-induced defect states first dynamically trap the directly excited electrons from the CB of BiOBr, thus suppressing the direct recombination of charge carriers (Steps 1 and 2). Subsequently, the indirect recombination of trapped electrons with photoexcited holes is also suppressed as the trapped electrons could efficiently be transferred to populate the empty antibonding orbitals of adsorbed N2 (Step 3). Reproduced with permission from ref. 601. Copyright 2015 American Chemical Society. | ||
Despite the CB potential of BiOBr being incapable of N2 reduction or solvated electrons formation (Fig. 34c), theoretical calculations revealed that the OVs on the BiOBr surface could adsorb and activate N2, modifying its electronic properties and hence reduction potential. The N2 reduction efficiency of BOB-001-OV was highly dependent on the presence of OVs. N2 temperature-programmed desorption (N2-TPD) experiments showed a single desorption peak for BOB-001-OV, related to chemisorbed N2, while no N2 adsorption was observed for BOB-001-H. The NH3 yield of different BOB-001-OV samples was linearly related to the N2-TPD peak area, suggesting that both N2 adsorption and reduction were dependent on the number of OVs.
Further experiments confirmed the role of OVs in promoting interfacial charge transfer (Fig. 34g). When the interfacial charge transfer was blocked by coating BOB-001-OV with an insulating SiO2 layer, NH3 production was significantly suppressed. Additionally, the introduction of CO in the gas mixture gradually inhibited NH3 generation, indicating that CO, with its stronger adsorption on OVs, competes with N2 (Fig. 34b). PL revealed that the OVs in BOB-001-OV acted as initial electron acceptors, increasing the lifetime of charge carriers and promoting interfacial electron transfer to adsorbed N2 (Fig. 34f). Transient photocurrent measurements further supported this, showing a significant interaction between surface OVs and N2, confirming the role of OVs in enhancing photocatalytic N2 fixation (Fig. 34e).601
Heterojunction fabrication can also achieve effective charge transport and vacancy stabilization, as demonstrated by Chen et al.602 in their study on MoS2/CdS heterojunctions (Fig. 35a and b) with abundant sulfur vacancies for photocatalytic N2 reduction (Fig. 35). The presence of sulfur vacancies in these heterojunctions was confirmed using UV-vis diffuse-reflectance spectroscopy (Fig. 35c) and EPR (Fig. 35e). Under visible light irradiation for 4 hours, the 3% MoS2/CdS heterojunctions achieved a significantly higher NH3 production (249.7 mg L−1 g−1), outperforming pure MoS2 (45.9 mg L−1 g−1) and pristine CdS (64.5 mg L−1 g−1) by 5.4 and 3.9 times, respectively (Fig. 35d). XPS analysis revealed that MoS2 and CdS are well-connected, with electron transfer occurring from CdS to MoS2, as indicated by the slightly higher binding energies of Cd2+ in the 3% MoS2/CdS sample compared to CdS alone. The MoS2/CdS samples also showed increased light absorption capacity with higher MoS2 content (Fig. 35c). The band gaps of MoS2 and CdS were calculated to be approximately 1.32 eV and 2.25 eV, respectively, with a defect-induced band gap close to 1.74 eV for 3% MoS2/CdS, attributed to sulfur vacancies originating from CdS.
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| Fig. 35 Photocatalytic N2 reduction over MoS2/CdS semiconductor heterojunction system. (a) TEM and (b) HRTEM images of 3% MoS2/CdS composites, (c) UV-Vis DRS spectra of the as-prepared MoS2, CdS, and MoS2/CdS composites, (d) Photocatalytic NH4+ production rates for MoS2, CdS, and MoS2/CdS composites containing different amounts of cocatalysts (0.3, 0.5, 1, 3, and 5%) under visible light irradiation, time course of NH4+ production, (e) EPR spectra of CdS and MoS2/CdS heterojunctions, (f) transient photocurrent response, (g) Nyquist plots of EIS, (h) TR PL spectra of CdS and MoS2/CdS heterojunctions, (i) schematic illustration of band structures and the proposed photocatalytic mechanism of N2 reduction at MoS2 and CdS heterojunctions. Reproduced with permission from ref. 602. Copyright 2022 American Chemical Society. | ||
EPR data further confirmed the formation of additional sulfur vacancies in the MoS2/CdS heterojunctions, with a shift in the EPR signature from g = 1.969 to 2.003, indicating a change in the coordination environment of Cd (Fig. 35e). The intensity of the EPR signal in the 3% MoS2/CdS sample was higher than that of CdS, demonstrating an increase in sulfur vacancies. The transient photocurrent measurements revealed that the 3% MoS2/CdS heterojunctions exhibited the highest photocurrent density, indicating the most efficient separation of photoexcited carriers (Fig. 35f). The EIS results showed that adding MoS2 to CdS reduced the semicircle diameter in the EIS spectrum, indicating improved conductivity and electron transfer (Fig. 35g). The PL spectra also demonstrated efficient charge separation in the MoS2/CdS heterojunctions, with a decrease in PL intensity and a longer decay time for the 3% MoS2/CdS sample compared to CdS alone (Fig. 35h). The average PL lifetime of the 3% MoS2/CdS heterojunction was shorter (1.2020 ns) than that of CdS (2.5465 ns), suggesting improved conductivity and faster electron migration after combining with MoS2. The Mott–Schottky analysis revealed that the ECB of MoS2, CdS, and 3% MoS2/CdS were −0.06, −0.31, and −0.28 V versus NHE, respectively. The sulfur vacancies in the 3% MoS2/CdS heterojunctions served as active sites for the chemical adsorption of N2 molecules, facilitating electron transfer into the reverse-bond π orbitals of adsorbed N2, thereby weakening the N–N triple bond (Fig. 35i). These findings underscore the importance of sulfur vacancies and enhanced charge transfer efficiency at MoS2/CdS heterojunctions in improving N2 fixation efficiency.602
The band gap of traditional semiconductors often does not align well with the N2 reduction potentials, which has spurred interest in plasmon-mediated N2 reduction and enhancing hot electron injection into N2 antibonding orbitals. Xiong et al.281 demonstrated that surface plasmons can provide sufficient energy to activate N2 through a dissociative mechanism when water and incident light are present (Fig. 36). Theoretical simulations suggested that the electric field enhanced by surface plasmons, along with plasmonic hot electrons and interfacial hybridization, played a crucial role in N2 dissociation. Specifically, AuRu core-antenna nanostructures, which had a broad light absorption cross-section and active sites, achieved an ammonia production rate of 101.4 µmol g−1 h−1 at room temperature and 2 atm pressure without any sacrificial agents. This design is an example of antenna–reactor geometry.
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| Fig. 36 Photocatalytic N2 reduction over plasmonic Au–Ru antenna–reactor system. (a) TEM image of AuRu0.31 core-antenna nanostructures, (b) catalytic ammonia production rates by bare Au, AuRu0.14, AuRu0.23, AuRu0.31, and AuRu0.39 in the first 2 h, (c) photocatalytic ammonia production rates by AuRu0.31 in the first 2 h under different light intensity, (d) calculated AQEs for N2 fixation over AuRu0.31, with its UV-Vis extinction spectrum (red line) as a reference, (e) optimized structures of N2 adsorbed on Ag22Ru6 cluster, both charged by 1e and experienced with an electric field of 1.0 × 108 V m−1. The electron density difference for α (spin-up) and β (spin-down) is normalized, and the absolute isovalue is set to 0.02. The red and green colors represent an increase and decrease in electron density, respectively. Reproduced with permission from ref. 281. Copyright 2019 American Chemical Society. | ||
The N
N bond cleavage occurs via indirect hot-electron injection into molecular orbitals or direct excitation of N2 into vibrational/electronic states. In both cases, N2 must be chemisorbed near the plasmonic metal to retain hot-electron energy and form an active metal-adsorbate complex. The AuRu core-antenna nanostructures showed a higher concentration of Ru at the antenna regions, confirming the formation of AuRu alloy antennas deposited on the Au core (Fig. 36a). These AuRu nanostructures significantly outperformed bare Au nanoparticles in catalytic ammonia production (Fig. 36b). With Ru incorporated up to 31%, the ammonia production rate increased to 101.4 µmol g−1 h−1, about 7.3 times higher than that of bare Au nanocrystals. However, with 39% Ru content, light harvesting decreased significantly, reducing N2 fixation activity (Fig. 36b). The N2 fixation catalyzed by AuRu0.31 nanostructures exhibited a nearly linear power law dependence on light intensity, indicative of a single charge-carrier reaction (Fig. 36c). The wavelength-dependent AQEs of AuRu0.31, measured under various monochromatic light irradiations, aligned well with the full extinction spectra range of AuRu nanostructures, indicating high light utilization efficiency (Fig. 36d).
Without water, DRIFTS showed no change, confirming hydrogen in ammonia came from water. Upon water addition, ammonia bands appeared, and the absence of N–N vibrations excluded an associative pathway. XPS revealed atomic N chemisorption (395.3 eV) and hydrogenated species (
NH, –NH2) at 397.2–398.0 eV. Simulations showed end-on N2 adsorption on Au22Ru6 (1.128 Å) elongating to 1.170 Å under electric field and charge effects, indicating that local fields drive N2 activation through electron transfer into antibonding orbitals (Fig. 36e).281
When a plasmonic metal nanocrystal interacts with an n-type semiconductor, a Schottky barrier forms at the nanocrystal–semiconductor interface. This barrier acts as a filter, allowing hot electrons to pass through the interface while blocking their reverse movement, thus facilitating efficient electron–hole separation. These composite systems benefit from high light-harvesting efficiency, stable activity, low electron–hole pair recombination rates, and tunable responses across the visible to near-infrared (NIR) spectrum.
In a study by Ye et al.603 Au nanocrystals anchored on ordered ultrathin TiO2 nanocavity arrays (NCAs) with abundant oxygen vacancies (denoted Au@TiO2 NCA) demonstrated that LSPR from the Au nanocrystals under NIR irradiation effectively drove the fixation of N2 to NH3 under mild conditions (Fig. 37). This system also represents a multifunctional plasmonic–semiconductor heterostructure, where the synergy between a defect-engineered oxide support and a noble-metal cocatalyst is utilized. The Au nanoparticles were uniformly arranged on the TiO2 nano cavity array (NCA) using a solid-state dewetting process (Fig. 37a and b). This setup optimized the total surface energy of the metallic Au thin film and TiO2 substrate. TiO2 NCAs served both as a support for the plasmonic Au nanoparticles and as active sites for N2 adsorption and reduction.
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| Fig. 37 Photocatalytic N2 reduction over plasmonic–semiconductor hybrid Au–TiO2 system. (a) Schematic outline of the fabrication processes for ordered and uniform Au@TiO2 NCA, (b) SEM image of the assembled Au nanoparticle arrays after thermal treatment. Scale bar: 100 nm, (c) UV-Vis-NIR absorption of TiO2 NTAs, TiO2 NCAs, and Au@TiO2 NCAs, (d) FDTD simulation of electric field enhancement over Au@TiO2 NCAs, (e) time-dependent photocatalytic ammonia production under NIR light illumination and N2 flow, (f) AQE of NH3 production on Au@TiO2 NCA as a function of wavelength, (g) illustration of the synergistic effect of the surface OVs and plasmonic Au NPs for photocatalytic N2 fixation on Au@TiO2 NCAs. Reproduced with permission from ref. 603. Copyright 2023 American Chemical Society. | ||
The process worked as follows: (1) hot electrons excited from the plasmonic Au nanocrystals overcame the Schottky barrier and were injected into the TiO2 NCA conduction band; (2) these hot electrons then diffused to the OV defect states of the TiO2 and were trapped; (3) the trapped hot electrons on the TiO2 NCA surface reduced the adsorbed N2, leading to ammonia production (Fig. 37g). The FDTD simulations showed that the LSPR-induced electric field intensity at the Au/TiO2 interface was amplified by a factor of 5 near the Au nanoparticle (Fig. 37d). XPS analysis confirmed the presence of OVs on the TiO2 NCA surface, which acted as N2 adsorption sites and introduced additional energy bands in the band gap. This facilitated electron transfer across the rutile TiO2-Au nanoparticle interface, enhancing N2 reduction to NH3. TiO2 nano tube array (NTA) and TiO2 NCA both exhibited strong absorption below 400 nm due to their large 3.0 eV band gap and weak interband transitions in the NIR region (Fig. 37c). In contrast, Au@TiO2 NCA showed an absorption peak at 1010 nm due to the LSPR effect of the Au nanoparticles. Additional absorption peaks at 605 and 550 nm were attributed to light interference through the thin TiO2 nanomembrane.
The NH3 production rate of 6.2 nmol cm−2 h−1 for TiO2 NTA and 7.7 nmol cm−2 h−1 for TiO2 NCA was observed (Fig. 37e). The improved performance of TiO2 NCA, which has an ultrathin membrane, suggested that surface OVs enhance N2 activation and interfacial electron transfer from the TiO2 surface to adsorbed N2 molecules. The addition of Au nanoparticles further increased the catalytic activity, with Au@TiO2 NCA achieving an NH3 production rate of 10.1 nmol cm−2 h−1. This was confirmed by ion chromatography.
The synergistic interaction of surface OVs and Au nanoparticles in Au@TiO2 NCA enhanced NH3 production. Hot electrons generated by the Au LSPR were injected into TiO2 and trapped at OV-induced defect states, activating adsorbed N2 for reduction (Fig. 37g). Concurrently, water oxidation on Au consumed hot holes. Au@TiO2 NCA showed slightly higher activity under λ > 400 nm than under NIR light, as the NIR LSPR band overlaps the visible region, generating more hot electrons for transfer to TiO2 OVs. The best N2 fixation occurred under full-spectrum irradiation due to combined UV-excited TiO2 electrons and Au LSPR-induced hot carriers. The excited N2 π* orbitals were stabilized by OV bands in TiO2, facilitating NH3 formation. The alignment between AQEs and the absorption spectrum confirmed that N2 photofixation was mainly driven by Au LSPR absorption (Fig. 37f).603
While heterostructures like plasmonic metal–semiconductors can improve hot charge carrier separation, many of these carriers are lost when crossing the Schottky barrier. Wang et al.604 introduced a Schottky barrier-free plasmonic semiconductor photocatalyst, MoO3−x, which excels in N2 photofixation (Fig. 38). This material not only served as an active site for N2 chemisorption but also utilized LSPR to generate hot charge carriers. Plasmonic MoO3−x showed impressive photoreactivity for NH3 production, with an apparent quantum efficiency exceeding 1% up to a wavelength of 1064 nm, and a 0.057% efficiency in solar-to-ammonia conversion without any hole scavenger (Fig. 38c).
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| Fig. 38 Photocatalytic N2 reduction over Schottky barrier-free plasmonic semiconductor MoO3−x system. (a) SEM image of the MoO3−x spheres prepared at 350 °C, (b) schematics illustrating the band structures of a conventional plasmonic metal–semiconductor hybrid photocatalyst (left), a plasmonic semiconductor photocatalyst (middle), and the plasmonic MoO3−x photocatalyst in this work (right), (c) time-dependent NH3 production amounts (left axis) and SACEs (solar to ammonia conversion efficiency) for ammonia production (right axis), (d) crystal structure of a MoO3−x model used in the DFT calculation. The red spheres represent the O atoms after relaxation. (e) DFT-calculated band structure and densities of states for the model shown in (d), (f) action spectrum of the MoO3−x spheres for N2 photofixation. The light absorption spectrum is plotted against the left axis, while the AQEs are plotted against the right axis, (g) photocurrent responses of the different materials recorded in Ar and N2 atmosphere, respectively. The visible light illumination was switched on and off repeatedly, (h) ˙OH detected through the fluorescence emission after the reaction for 60 min under the different reaction conditions. Reproduced with permission from ref. 604. Copyright 2022 Wiley-VCH GmbH. | ||
Recent studies have revealed LSPR in various semiconductors with adequate charge carrier densities.604–608 To better understand the electronic structure and N2 adsorption behavior of MoO3−x, a comprehensive density functional theory study was conducted. Intrinsic MoO3 displayed a wide band gap of over 2.29 eV, but the presence of oxygen vacancies introduced defect states close to the conduction band. This allowed for the free movement of electrons from these defect states to the conduction band, contrasting with the transfer of hot electrons from the metal to the semiconductor in traditional metal–semiconductor hybrid plasmonic photocatalysts. The calculations showed that the Fermi level is well above the defect band, indicating metallic characteristics with free charge carriers in MoO3−x (Fig. 38d and e). Scattering spectra of MoO3−x spheres (300–600 nm) showed consistent peak positions (Fig. 38a). Their dielectric response, modeled via the Drude–Lorentz approach using carrier densities from Mott–Schottky analysis, matched experimental data. The negative real dielectric values in the visible-NIR range confirmed that the observed scattering peaks originated from LSPR rather than dielectric resonance.
Hot electrons were traced as superoxide anions (˙O2−), formed when O2 gas was introduced into the reaction solution instead of N2. The photogenerated electrons reacted with O2 to form ˙O2−, while photogenerated holes were consumed by DMSO. The presence of ˙O2− was confirmed using 4-chloro-7-nitrobenzofurazan (NBD-Cl) acetonitrile solution, which showed an absorption peak at 470 nm. To confirm hot electrons' role in the N2 reduction reaction, AgNO3 was added as an electron scavenger. The N2 photofixation reaction was completely inhibited by AgNO3, and Ag nanoparticles were observed on the recovered photocatalyst, indicating that the suppression was due to hot electrons being consumed by Ag+ ions. Fluorescence measurements of hydroxyl radicals (˙OH) were used to detect hot holes. In the standard N2 photofixation system, hot holes, generated by reacting with OH−, were detected by adding terephthalic acid (TA), which fluoresces at 425 nm when reacting with ˙OH. Hot holes were only detected when both MoO3−x spheres and the light source were present, consistent with the hot electron detection results (Fig. 38h). The Schottky-barrier-free nature of MoO3−x is expected to minimize hot charge carrier loss. Electrochemical investigations confirmed the generation and consumption of hot charge carriers. MoO3−x spheres displayed clear photocurrent signals in both Ar and N2 atmospheres, confirming hot electron generation from OV-induced LSPR (Fig. 38e). In contrast, commercial MoO3 and annealed MoO3−x showed negligible photocurrent signals. The photocurrent signal's shark fin-like shape was attributed to photogenerated electron trapping at OVs, causing a delay in the signal's generation and reduction. Notably, changing from an Ar to an N2 atmosphere halved the photocurrent, likely due to electron consumption in the N2 reduction reaction.
Chemisorption of N2 was essential for photofixation. Commercial MoO3 showed a single desorption peak near 100 °C, indicating physisorption, whereas MoO3−x exhibited an additional peak around 400 °C due to N2 chemisorption at OV sites. Light absorption of MoO3−x spheres decreased with longer calcination, correlating with reduced N2 fixation, confirming the key role of OVs in catalysis. MoO3−x spheres achieved superior N2 photofixation owing to their Schottky-barrier-free structure, enabling efficient charge transport. Chemisorbed N2 at OV sites was activated under illumination, where carrier oscillations induced LSPR. LSPR decay generated hot electrons and defect-state holes; the holes oxidized H2O to O2, while the electrons reduced N2 to NH3 (Fig. 38b).604
Building upon the established advantages of single-phase Schottky-barrier-free (SBF) systems, recent research has pivoted toward enhancing the efficiency further by improving the light absorption and charge carrier utilization. One such study was reported by Wang et al.605 in which the authors engineered a MoO3−x/Ag heterostructure (Fig. 39a), designed to achieve broadband solar harvesting through the synergistic coupling of vacancy-induced and metallic LSPR modes (Fig. 39b). This catalyst is an example of Schottky barrier-free plasmonic semiconductor and plasmonic metal heterostructure photocatalyst. Critically, this architecture maintained an SBF nature by ensuring ohmic interfacial contact rather than a traditional rectifying junction. KPFM and work function analyses demonstrated that the Ag work function facilitated a downward bending of the MoO3−x conduction band, rendering the interface electronically “transparent” to hot carrier migration (Fig. 39c). This band alignment enabled the unhindered injection of plasmonic hot electrons from the Ag nanoparticles into the MoO3−x host, as evidenced by a 15 meV Fermi level shift under illumination, nearly double the shift observed in the pristine oxide.
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| Fig. 39 Photocatalytic N2 reduction over Schottky barrier free plasmonic semiconductor MoO3−x/Ag system. (a) Schematic illustrating the structure of a MoO3−x nanosphere loaded with Ag nanoparticles, (b) light absorption spectra of commercial intrinsic MoO3 nanoparticles and the MoO3−x/Ag samples with 0, 1, 5, 9, 10, 11, and 13% Ag, (c) electronic band energy levels of plasmonic Ag and MoO3−x synthesized, (d) light absorption (left axis) and measured AQE (right axis) spectra of the MoO3−x and MoO3−x/10% Ag samples under the optimized conditions, (e) light absorption difference (left axis) and AQE difference (right axis) of the MoO3−x/10% Ag sample with respect to the MoO3−x sample under the optimized conditions, (f) time-dependent production of NH3 for the MoO3−x/10% Ag sample under the optimized conditions, (g) high-magnification SEM image of the solar absorber film obtained with the backscattered electron detection mode, (h) interface structure between the solar absorber film and water. From top to bottom: the ideal interface, monolayer interface, bilayer interface, (i) light absorption (left axis) and measured AQE (right axis) spectra of the powder and film systems. Reproduced with permission from ref. 605. Copyright 2025 Wiley-VCH GmbH. | ||
The catalytic activity of this SBF architecture was most evident in its wavelength-dependent nitrogen photofixation (PCNF) performance. By optimising the Ag loading to 10 mol%, the researchers successfully balanced plasmonic hot-carrier generation with reduced light scattering, achieving a record-high solar-to-chemical conversion efficiency (SCCE) of 0.41%. A critical mechanistic “fingerprint” was observed in the correlation between the light absorption and the AQE spectra (Fig. 39d and e), specifically, the AQE enhancement peaks at approximately 466 nm, precisely matching the LSPR of the incorporated Ag nanoparticles. This alignment provided direct evidence that the ohmic contact facilitated the efficient utilization of Ag-generated hot electrons for N2 reduction. The best PCNF performance with an NH3 yield of 0.78 (±0.08) mmol gcat−1 h−1 and a SCCE of 0.14% (±0.01%) was achieved (Fig. 39f). Furthermore, the SBF nature and associated low activation energy allowed the system to leverage plasmonic photothermal effects. This synergy between broadband absorption, barrier-free transport, and photothermal assistance demonstrated how precise interfacial engineering can overcome the kinetic bottlenecks of traditional slurry-based photocatalysis.
To enhance light utilization and mass transfer, the MoO3−x/Ag nanospheres were immobilized within a porous poly(vinyl alcohol) (PVA) substrate via freeze-drying. As shown in the backscattered SEM imaging (Fig. 39g), this interlaced network provided a high surface area for catalyst distribution while maintaining a thin, hydrophilic water layer that minimised NIR light attenuation and facilitated rapid N2 diffusion to the active sites. By utilizing a bilayer configuration, elevating the catalyst-loaded PVA film above the water surface using a foam support (Fig. 39h), the authors minimised NIR light attenuation by water and bypassed the mass-transfer limitations typical of slurry reactors. This architecture allowed N2 molecules to penetrate an ultrathin water layer to reach the active sites, resulting in a 30% performance boost over submerged monolayer systems. While the mass-normalised NH3 yield followed a volcano-shaped dependence on catalyst loading, the overall SCCE remained consistently higher in the film system compared to the powder. Most notably, the AQE across the entire visible-to-NIR spectrum was significantly enhanced in the film system (Fig. 39i), proving that the integration of Schottky-barrier-free nanospheres into a porous, triphase-like interface effectively maximises both photon delivery and reactant accessibility.605
Expanding the scope of SBF systems, Wang et al.206 recently reported a WO3-based system that integrates hydrogen doping, oxygen vacancy engineering, and transition metal doping. Through a systematic screening of dopants (Mo, Bi, Ce, Fe, and V) and hydrothermal optimisation, the authors identified Mo-H0.23WO3−x nanoplates (NPLs) as the most potent configuration for simultaneous N2 fixation and H2O2 production. Morphological analysis revealed a well-defined rectangular nanoplate structure (Fig. 40a), while the synergistic presence of OVs and Mo sites, confirmed via EPR, XPS, and STEM-EDS, facilitated broadband light harvesting extending deep into the NIR region (Fig. 40b). Electronic structure analysis using Mott–Schottky and XPS valence band measurements (Fig. 40c) demonstrated that while Mo doping has a negligible impact on the overall band positions, it significantly enhances the charge transport dynamics. The conduction band and valence band potentials remained thermodynamically aligned for the coupled generation of NH3 and H2O2, yet the Mo-modified H0.23WO3−x exhibited the highest charge carrier density and photocurrent response among the series. Furthermore, the OVs were shown to serve a dual role: inducing the SBF-plasmonic state while simultaneously providing high-affinity sites for the chemisorption and activation of N2 molecules.
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| Fig. 40 Photocatalytic N2 reduction over Schottky barrier-free Mo-H0.23WO3−x photocatalyst. (a) SEM image of the Mo-H0.23WO3−x NPLs, (b) DRS data of the H0.23WO3-based NPLs, (c) electronic band alignments of the H0.23WO3-based NPLs. Time-dependent yields of (d) NH3 and (e) H2O2 for the H0.23WO3-based NPLs under the simulated solar light illumination. Light absorption spectra (blue line, left axis) and measured AQEs for (f) NH3 (red dots, right axis) and (g) H2O2 (red dots, right axis) of the Mo-H0.23WO3−x NPLs. Time dependent yields of (h) NH3 and (i) H2O2 over the PVA film, Mo-H0.23WO3−x powder, and Mo-H0.23WO3−x/PVA film. Reproduced with permission from ref. 206. Copyright 2026 Wiley-VCH GmbH. | ||
The catalytic efficacy of these H0.23WO3−x-based nanoplates was evaluated through the simultaneous photofixation of N2 and the generation of H2O2. Among the evaluated series, the Mo-H0.23WO3−x configuration delivered the most robust bifunctional performance, achieving NH3 and H2O2 production rates of 187.53 and 196.25 µmol g−1 h−1, respectively (Fig. 40d and e). A definitive link between the SBF-plasmonic properties and the catalytic output was evidenced by the monochromatic apparent quantum efficiency (AQE) measurements; the AQE profiles for both NH3 and H2O2 exhibited a high degree of overlap with the catalyst's broadband absorption spectrum (Fig. 40f and g). This spectral matching confirmed that the vacancy-induced and Mo-enhanced LSPR effectively drives the redox chemistry across the entire visible-to-NIR range. Ultimately, the Mo-H0.23WO3−x photocatalyst achieved a significant solar-to-chemical conversion efficiency of 0.090%, demonstrating the practical potential of integrating multiple defect-engineering strategies into a single barrier-free semiconductor framework.
To improve the light utilization of the system, the authors integrated the Mo-H0.23WO3−x nanoplates into the same floatable PVA-based biphasic platform previously described. This interfacial engineering resulted in a 1.64-fold and 1.66-fold enhancement in NH3 and H2O2 production rates, reaching 308.41 and 325.27 µmol g−1 h−1, respectively, compared to the powdered slurry (Fig. 40h and i). The underlying mechanism, elucidated through DFT calculations and carrier dynamics studies, revealed a sophisticated two-photon excitation process. Upon absorbing an initial photon, a hot electron was transferred to a mid-gap doping state, subsequently migrating to the high-energy region of the conduction band after absorbing a second photon. This sequential excitation was enhanced by the LSPR of the Mo-H0.23WO3−x framework, which significantly augments the generation of hot charge carriers. While the photogenerated holes in the valence band drive the oxidation of H2O to H2O2, the accumulation of hot electrons, combined with the OV-mediated chemisorption and activation of N2, facilitated high-efficiency nitrogen reduction. Collectively, these two studies highlight the transformative potential of Schottky-barrier-free architectures, where the synergy between metallic-like carrier densities, and defect-induced active sites overcomes the traditional kinetic and thermodynamic barriers of plasmonic photocatalysis.206
N triple bond (941 kJ mol−1) at ambient conditions showcase the unique ability of plasmonic hot carriers to overcome kinetic barriers that would be insurmountable for thermal or conventional photocatalytic processes.
One of the most profound insights emerging from recent studies is the shift toward Schottky-barrier-free architectures, such as the Mo-H0.23/WO3−x nanoplates. These frameworks represent a shift in how we view the metal–semiconductor interface; by eliminating the traditional depletion region, these systems allow for the seamless transport of hot electrons to catalytic sites. This architecture is particularly potent when coupled with two-photon excitation processes, where sequential energy absorption allows electrons to migrate from mid-gap states to higher-energy regions of the conduction band. This mechanism, significantly augmented by LSPR, exemplifies how researchers are now utilizing the “energy bottleneck” of traditional systems as a stepping stone to achieve higher quantum efficiencies.
Furthermore, the transition from laboratory benchmarks to practical systems has highlighted the importance of interfacial reactor engineering. The integration of catalysts into floatable PVA-based biphasic platforms addresses a critical bottleneck in traditional photocatalysis: the simultaneous optimization of light utilization and mass transport. By confining the reaction to a biphasic interface, these systems minimize light scattering by the solvent while ensuring that gaseous reactants like CO2 and N2 have direct access to the active sites. This coupling of materials science and reactor design demonstrates that the next generation of photocatalytic enhancement will likely come from the spatial management of both photons and molecules.
However, the most profound insight emerges from the recognition that both material classes converge on similar optimization strategies to transcend their individual limitations, revealing universal principles of photocatalytic enhancement that surpass the semiconductor–plasmonic divide. Both systems rely heavily on defect engineering, oxygen vacancies in semiconductors (black TiO2, In2O3−x, BiOBr) and surface defects in plasmonic metals (MoO3−x), to extend carrier lifetimes, create active sites, and modify electronic structures for enhanced catalytic performance. The ubiquitous use of heterostructure architectures, from semiconductor Z-schemes (Cu2O-Pt/SiC/IrOx) to plasmonic antenna–reactor systems (Au@AuRu/g-C3N4, DPC-C4-Ni), demonstrates that spatial separation of charge generation and utilization represents a fundamental design principle regardless of the underlying excitation mechanism. Most remarkably, the emergence of hybrid semiconductor–plasmonic systems (Au@TiO2, Ag@Li0.075TiO2, Au NR@ZnO) reveals that the future of photocatalytic design lies not in choosing between these paradigms, but in utilizing their synergistic combination where plasmonic intensity provides the initial activation energy while semiconductor persistence ensures sustained chemical conversion, ultimately achieving performance levels that exceed the sum of their individual contributions, a testament to the complementary rather than competitive nature of these two fundamental approaches to solar-driven chemistry. Further broadening this scope, the emergence of doped semiconductor nanocrystals and transition metal nitrides has introduced a versatile platform for dynamically tunable, earth-abundant plasmonic systems.606–608
A summary table compiling all photocatalyst examples discussed in this section is provided to facilitate direct comparison (Table 1).
| S. no. | Catalyst | Reaction | Reaction conditions | Product yield | Reference |
|---|---|---|---|---|---|
| 1 | In2O3−x/In2O3 | CO2 reduction with hydrogen | Batch reactor, P = 2 bar, H2/CO2 ratio = 1 : 1; Xe lamp (2 W cm−2), T = 262 °C; external heating – no; reaction time = 30 min |
CO: 1.87462 mmol h−1 m−2 | 463 |
| 2 | In2O3−x/In2O3 | CO2 reduction with hydrogen | Flow reactor, P = 1 bar, H2/CO2 ratio = 1 : 1; total flow = 1 mL min−1; Xe lamp (0.8 W cm−2), T = 300 °C; external heating – yes |
CO: 0.161 mmol h−1 m−2 | 463 |
| 3 | 0.4%GDY-IO | CO2 reduction with hydrogen | Batch reactor, P = 1.6 bar, H2/CO2 ratio = 3 : 1; Xe lamp (2 W cm−2), T = 120 °C; external heating – no; reaction time = 4 h |
CO: 0.018 mmol g−1 | 466 |
| CH4: 0.011 mmol g−1 | |||||
| C2H4: 0.0007 mmol g−1 | |||||
| C2H6: 0.0009 mmol g−1 | |||||
| C3H6: 0.0001 mmol g−1 | |||||
| C3H8: 0.0001 mmol g−1 | |||||
| 4 | Pd/TiO2 | CO2 reduction with hydrogen | Batch reactor, P = 25 bar, H2/CO2 ratio = 4 : 1; 150 W mercury lamp, T = 130 °C; external heating – no; reaction time = 3 h |
CO: 0.3556 mmol g−1 | 467 |
| CH4: 0.0463 mmol g−1 | |||||
| C2H6: 0.0396 mmol g−1 | |||||
| 5 | R-Au/MnOx-2%-PTPO (PTPO-Pt doped PbTiO3) | CO2 reduction with hydrogen | Flow reactor, P = 1 bar, H2/CO2 ratio = 3 : 1; total flow = 24 L gcat−1 h−1; Xe lamp (20 mW cm−2), T = 550 °C; external heating – yes |
CO: 235.7 mmol g−1 h−1 | 70 |
| 6 | Rh/Al2O3 | CO2 reduction with hydrogen | Flow reactor, P = 1 bar, H2/CO2 ratio = 5.5 : 1; total flow = 71 mL min−1; blue LED (4.9 W cm−2), T = 350 °C; external heating – yes |
CH4: 36 mmol h−1 g−1 | 471 |
| 7 | Black gold-Ni | CO2 reduction with hydrogen | Flow reactor, P = 1 bar, H2/CO2 ratio = 1 : 10; total flow = 11 mL min−1; Xe lamp (2.7 W cm−2), T = 223 °C; external heating – no |
CO: 2464 ± 40 mmol gNi−1 h−1 | 248 |
| 8 | Au@AuRu/g-C3N4 | CO2 reduction with hydrogen | Batch reactor, P = 10 bar, H2/CO2 ratio = 3 : 1; Xe lamp (1.1 W cm−2), T = 150 °C; external heating – yes; reaction time = 4 h |
CH4: 0.103 mmol h−1 g−1 | 477 |
| 9 | Al@Cu2O | CO2 reduction with hydrogen | Flow reactor, P = 1 bar, H2/CO2 ratio = 1 : 1; total flow = 10 mL min−1; supercontinuum fiber laser (10 W cm−2), T = 175 °C; external heating – no |
CO: 0.360 mmol cm−2 h−1 | 238 |
| 10 | Ru0.1Cu1-MgAl2O4 | CO2 reduction with hydrogen | Flow reactor, P = 1 bar, CO2/H2/Ar ratio = 1 : 3:1; total flow = 3 mL min−1; Xe lamp (1.7 W cm−2), T = 190 °C; external heating – no |
CH3OH: 640 µL g−1 h−1 | 162 |
| 11 | CuIn5S8 | CO2 reduction with water | Batch reactor, P = 1 bar; UV Xe lamp (0.05 W cm−2); external heating – no | CH4: 0.0087 mmol h−1 g−1 | 527 |
| 12 | BiOCl nanosheets | CO2 reduction with water | Batch reactor, P = 1 bar; Xe lamp (400 nm cutoff filter); external heating – no | CO: 0.1882 mmol h−1 g−1 | 528 |
| 13 | Pb0.6Bi1.4O2Cl1.4 | CO2 reduction with water | Batch reactor, P = 1 bar; CO2 (ca.1500 ppm); Xe lamp (420 nm cutoff filter); external heating – no; reaction time = 4 h | CO: 0.01791 mmol g−1 | 529 |
| CH3OH: 0.02653 mmol g−1 | |||||
| 14 | Carbon-doped SnS2 | CO2 reduction with water | Flow reactor, halogen lamp; reaction time = 13 h | Acetaldehyde: 1.2566 mmol gcat−1 | 530 |
| 15 | Mn, C-codoped ZnO | CO2 reduction with water | Batch reactor, P = 0.8 bar; Xe lamp; external heating – no; reaction time = 4 h | CO: 0.00083 mmol g−1 | 531 |
| 16 | Cu2O-Pt/SiC/IrOx | CO2 reduction with water | Batch reactor, P = 0.8 bar; Xe lamp (λ ≥ 420 nm); external heating – no; reaction time = 2 h | HCOOH: 0.8967 mmol g−1 h−1 | 457 |
| 17 | Single-atom cobalt in Bi3O4Br | CO2 reduction with water | Batch reactor, P = 0.8 bar; Xe lamp; external heating – no | CO: 0.1071 mmol g−1 h−1 | 532 |
| 18 | SrNb2O6−x-3 | CO2 reduction with water | Batch reactor, P = 1 bar; Xe lamp (320 nm < λ < 780 nm); external heating – no | CO: 0.066 mmol g−1 h−1 | 53 |
| 19 | 2D BiFeO3 | CO2 reduction with water | Batch reactor, P = 1 bar; Xe lamp (500 mW cm−2); external heating – no; reaction time = 1.5 h | CO: 0.17 mmol g−1 h−1 | 19 |
| 20 | Ag@LixTiO2 | CO2 reduction with water | Batch reactor, P = 1 bar; Xe lamp (0.1 W cm−2); external heating – no; reaction time = 10 h | CH4: 0.049 mmol g−1 | 533 |
| 21 | AgX/g-C3N4 (X = Cl and Br) | CO2 reduction with water | Flow reactor, P = 1 bar; low-power 15 W energy-saving daylight lamp (0.0085 W cm−2); external heating – no; total flow = 5 mL min−1 | CH4: 0.001092 mmol gcatalyst−1 | 534 |
| 22 | Au@TiO2 | CO2 reduction with water | Batch reactor, P = 1 bar; Xe lamp,; external heating – no | CH4: 0.00252 mmol g−1 h−1 | 535 |
| C2H6: 0.00167 mmol g−1 h−1 | |||||
| 23 | Au NR@ZnO | CO2 reduction with water | Batch reactor, P = 1.01 bar; Xe lamp; external heating – no | CH4: 0.017 mmol h−1 (gAu)−1 | 536 |
| CO: 0.032 mmol h−1 (gAu)−1 | |||||
| 24 | Au nanoparticles | CO2 reduction with water | Batch reactor, P = 1 bar; 420 nm LED (0.07 W cm−2); external heating – no, reation time = 3 h | CO: 4.73 mmol g−1 h−1 | 459 |
| 25 | Au rod@CuPd | CO2 reduction with water | Batch reactor, P = 1 bar; Xe lamp (0.4 W cm−2), T = 200 °C; external heating – yes | CH4: 0.55 mmol h−1 g−1 | 412 |
| 26 | Pt/black TiO2 | DRM | Flow reactor, CH4/CO2 = 1 : 1; P = 1 bar; total flow = 10 mL min−1; AM 1.5G Newport solar simulator (0.1 W cm−2), T = 700 °C; external heating – yes |
CO: 480 mmol g−1 h−1 | 552 |
| H2: 237 mmol g−1 h−1 | |||||
| 27 | Rh/STO | DRM | Flow reactor, CH4 : CO2 : Ar (1 : 1 : 98 in vol%); P = 1 bar; total flow = 10 mL min−1; Hg–Xe lamp (absorbed photon number 1.25 × 1017 quanta per cm2 per s); external heating – no |
CO: 0.27 mmol h−1 | 553 |
| H2: 0.27 mmol h−1 | |||||
| 28 | SA-Ru/Cu | DRM | Flow reactor, CH4 : CO2 = 1 : 1; P = 1 bar; total flow = 16 mL min−1; supercontinuum laser (19.2 W cm−2); external heating – no |
CO: 1980 mmol g−1 h−1 | 223 |
| H2: 1980 mmol g−1 h−1 | |||||
| 29 | NiCo/SiO2 | DRM | Flow reactor, CH4 : CO2 = 1 : 1; P = 1 bar; total flow = 20 mL min−1; Xe lamp (9 W cm−2), T = 700 °C; external heating – yes |
CO: 1446.1 mmol g−1 h−1 | 556 |
| H2: 1293.7 mmol g−1 h−1 | |||||
| 30 | BiOBr-OV | N2 reduction | Batch reactor; P = 1 bar; Xe lamp (420 nm cutoff); external heating – no; detection: spectrophotometry (Nessler's reagent) | NH3: 0.104 mmol h−1 gcat−1 | 601 |
| 31 | MoS2/CdS | N2 reduction | Batch reactor; P = 3 bar; Xe lamp (420 nm cutoff, 1.13 W cm−2); external heating – no; reaction time = 4 h; detection: spectrophotometry (Nessler's reagent) | NH3: 249.7 mg L−1 gcat−1 | 602 |
| 32 | AuRux | N2 reduction | Batch reactor; P = 2 bar; Xe lamp (0.4 W cm−2); external heating – no; reaction time = 2 h; detection: spectrophotometry (indophenol blue) | NH3: 0.101 mmol g−1 h−1 | 281 |
| 33 | Au/TiO2 | N2 reduction | Flow reactor; P = 1 bar; total flow = 20 mL min−1 of N2; Xe lamp (800 nm cutoff filter); external heating – no; detection: spectrophotometry (indophenol blue), ion chromatography, and 1H NMR | NH3: 10.1 nmol cm−2 h−1 | 603 |
| 34 | MoO3−x | N2 reduction | Flow reactor; P = 1 bar; total flow = 50 mL min−1 of N2; Xe lamp (0.1 W cm−2); external heating – no; reaction time = 2 h; detection: spectrophotometry (Nessler's reagent) | NH3: 0.435 mmol h−1 g−1 | 604 |
| 35 | MoO3−x/Ag | N2 reduction | Flow reactor; P = 1 bar; Xe lamp (AM 1.5 G filter, 0.1 W cm−2); external heating – no; reaction time = 2 h; detection: spectrophotometry (Nessler's reagent) | NH3: 0.30 mmol h−1 gcat−1 | 605 |
| 36 | Mo-H0.23WO3−x | N2 reduction | Flow reactor; P = 1 bar; Xe lamp (AM 1.5 G filter, 0.1 W cm−2); external heating – no; reaction time = 2 h; detection: spectrophotometry (Nessler's reagent) | NH3: 0.308 mmol h−1 g−1 | 206 |
| H2O2: 0.325 mmol h−1 g−1 |
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| Fig. 41 TA spectroscopy for coherence time, relaxation dynamics, and hot carrier temperature. (a) Interferogram envelope squared for CsPbBr3 NC (red circles) with best fit (blue line) and dephasing component (black dashed lines) decaying with e−2/T2δ. Γ is the exciton linewidth, and p(ζ, τ) is the spectral intensity, (b) time-resolved transmittance spectra of GaAs at 15 K for different time delays between the pump and probe pulses, (c) dephasing time in GaAs as a function of the carrier density. The dashed line represents the prediction by a simple Drude model, (d) normalized TA spectra with variable delays from 0.2 ps to 1.4 ps, and the inset shows fitted high energy tails using the Maxwell–Boltzmann distribution function to extract the HC temperature, (e) extracted HC temperature with a delay at different carrier density. Black line: calculated HC cooling dynamics in the absence of hot-phonon effect. All the dashed lines are calculated HC cooling dynamics in the presence of the hot-phonon effect, (f) HC cooling dynamics with a carrier density of 10.4 × 1018 cm−3 at RT. Black circles: HC temperature extracted from TA spectra. The lines show the calculated HC cooling dynamics for τph = 0.6 ps: with hot-phonon (HP) effect only (violet dashed line); with both HP and Auger heating (AH) effects (bright red line); and without HP and AH effects (magenta dotted line). Part (a) is reproduced with permission from ref. 613, copyright 2019 AAAS. Part (b) is reproduced with permission from ref. 614, copyright 1985 American Physical Society. Part (c) is reproduced with permission from ref. 615, copyright 1992 American Institute of Physics. Part (d–f) are reproduced with permission from ref. 616, copyright 2017 Springer Nature Publishing Group. | ||
Further relaxation occurs through carrier–phonon coupling until carrier energies fall below the optical phonon threshold. Although high excitation densities generally accelerate thermalization via increased carrier–carrier scattering, cooling in semiconductor nanocrystals is often slowed by competing high-density effects. These include the hot-phonon bottleneck, where non-equilibrium longitudinal optical (LO) phonons accumulate and are reabsorbed because carrier–phonon scattering outpaces phonon decay, and Auger recombination, which recycles recombination energy back into the carrier system rather than emitting photons.616,619
One prominent example illustrating these phenomena at higher excitation densities was reported by Fu et al.616 who examined hot-carrier cooling in methylammonium lead triiodide at carrier densities ∼1018 cm−3 using transient absorption spectroscopy with 2.48 eV excitation. They observed an initial photobleach at 1.64 eV from band filling that evolved into photoinduced absorption within 0.6 ps (Fig. 41d). Hot-carrier temperatures were estimated using a Maxwell–Boltzmann approximation, and the cooling curves flattened at higher carrier concentrations, indicating slower energy loss (Fig. 41e). The dominant cooling mechanism was attributed to polar Fröhlich electron–phonon coupling, where delayed emission of zone-center LO phonons (lifetime ≈ 0.6 ± 0.1 ps) produced a hot-phonon bottleneck. At still higher densities (∼1018 cm−3), Auger heating further suppressed relaxation, leading to pronounced cooling slowdown (Fig. 41f). These results reveal the strong influence of carrier density, phonon bottlenecks, and Auger processes on hot-carrier cooling.
LSPR damping initiates hot-carrier generation. Classical Drude theory describes this as gradual energy loss per oscillation cycle caused mainly by frictional loss (or electron–phonon scattering),622–626 though electron–electron interactions and rapid decay of d-band holes due to larger effective mass in noble metals also contribute.627 Hot-carrier relaxation then follows the same sequence of electron–electron, electron–phonon, and phonon–phonon scattering as in semiconductors, though with faster e–e scattering due to higher carrier density. While the formal sequence of relaxation steps is similar, the underlying excitation origin, characteristic timescales, and consequences for energy transfer and catalysis differ fundamentally between plasmonic metals and semiconductors. Toffoletti et al.628 investigated these dynamics in colloidal Au nanorods using transient absorption and 2D electronic spectroscopy (2DES). Pump–probe measurements revealed photobleaching at both plasmon modes (LSPR at 2.14 eV, TSPR at 2.37 eV) and a red-shifted, broadened positive signal from electron heating (Fig. 42a and b). Voigt-profile fits629 enabled the extraction of time-dependent plasmon shifts (Δω) and broadenings (Δγ) (Fig. 42c and d). A breathing mode with a 53 ± 5 ps period was observed, attributed to lattice expansion, and it modulated Δγ more strongly than Δω. From fluence-dependent dynamics, the electron–phonon scattering time was determined as τe–ph ≈ 1.16 ± 0.36 ps, and the phonon–phonon scattering time as τph–ph ≈ 145 ± 40 ps.
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| Fig. 42 TAS and 2DES for scattering lifetimes in Au nanorods. (a) 2D map representation of ΔA (colorscale) as a function of probing energy (eV) and pump-probe time delay (ps) with a pump pulse centered at 3.10 eV with a fluence of 700 µJ cm−2 and red horizontal lines indicate the spectral position of LSPR (2.14 eV) and TSPR (2.37 eV), (b) TA spectra at different delay times td (blue dots) and the respective fitting curves obtained using Voigt profile, (c) time evolution of Δω (upper panel) and Δγ (central panel) for LSPR. Blue dots, experimental points; red lines, fitting lines. (d) Same as (c) but for TSPR, (e) Decay associated spectra (DAS) for the three time constants extracted by the global fitting. The values of the time constants are reported in each plot. Reproduced with permission from ref. 628, copyright 2024 American Chemical Society. | ||
To resolve earlier processes within the first few hundred femtoseconds, the authors employed 2DES, which separates homogeneous and inhomogeneous linewidth contributions.630–634 The homogeneous linewidth before scattering was γLSPR = 52 ± 5 meV at t2 = 0, where t2 represents the delay between the second pump pulse and the probe pulse, and it broadened with increasing t2 due to electron–electron scattering. From the time dependence of γLSPR(t2), the authors extracted τe–e ≈ 65 ± 42 fs, refined to ∼98 ± 26 fs using global fitting, along with τe–ph ≈ 1603 ± 40 fs (Fig. 42e). The authors also identified a coherent dephasing time of ∼15 fs (45 meV linewidth). This coherent regime represents a fascinating parallel between plasmonic nanostructures and semiconductors; both systems can maintain quantum coherence on similar timescales. However, unlike semiconductors, plasmonic nanostructures exhibit significant electron–electron scattering, allowing them to achieve a Fermi–Dirac distribution much more quickly.
To provide an electron with the kinetic energy between 0.5 and 1 eV necessary for ejection from the surface, blue and UV radiation are needed for gold and silver, respectively. This requirement creates a fundamental challenge: in the visible spectrum, interband absorption competes with other absorption processes, reducing the efficiency of hot-electron extraction.
Zheng et al.637 provided clear experimental evidence separating carrier generation from direct interband excitation versus plasmon decay. Using electron-beam lithography, they fabricated devices with square Au pads and periodic Au nanowire arrays (50 nm thickness, 500 nm spacing) on 〈100〉 TiO2 substrates, forming either Schottky (Au/TiO2) or ohmic (Au/Ti/TiO2) contacts (Fig. 43a and b). This configuration allowed selective probing of carrier injection pathways. Because metals exhibit low interband absorption cross-sections but strong plasmonic absorption, Schottky contacts primarily detect high-energy carriers generated from plasmon decay, whereas ohmic contacts allow both low- and high-energy carriers to contribute (Fig. 43c and d).
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| Fig. 43 Carriers' route, band diagrams, and photocurrent mapping in Schottky and ohmic devices. Schematic of hot-carrier generation and collection. (a) Schottky and (b) ohmic barrier. Plasmonic hot-carrier generation is localized to areas of high-field enhancement, while interband absorption occurs throughout the bulk. Band diagrams show (c) an Au-TiO2 Schottky device where low-energy carriers cannot cross the barrier, and (d) an Au-Ti-TiO2 ohmic device, where carriers are freely collected due to the absence of a barrier. The wide semiconductor band gap enables preferential electron collection. (e) Schematic of TE excitations used to generate photocurrent map of a Schottky and an ohmic device using TE-polarized light. The laser wavelength is tuned to the resonance of the plasmonic nanowires (∼675 nm, wire width 273 nm). (f) Schematic of TM-polarized light excitation used to generate photocurrent maps of a Schottky and an ohmic device. Reproduced with permission from ref. 637, Copyright 2015 Springer Nature Publishing Group. | ||
Using 675 nm excitation (1.84 eV), well below the TiO2 band gap (3.03 eV), ensured that only Au was photoexcited. Under transverse electric (TE) polarization, which efficiently excites surface plasmon polaritons, Schottky devices generated localized photocurrent near the edges of nanostructures, while ohmic devices produced uniform current (Fig. 43e). Under transverse magnetic (TM) polarization, Schottky devices showed minimal signal, whereas ohmic devices still produced uniform current (Fig. 43f). These polarization-dependent responses confirm that plasmonic excitation yields significantly greater photocurrent than direct interband transitions. This work established an important design principle: interband transitions largely produce low-energy carriers, while plasmon decay provides the high-energy carriers more relevant for photocatalysis and photodetection.
Brown et al.638 provided a quantitative framework for these processes via first-principles calculations based on experimentally measured dielectric functions. They evaluated contributions from direct (interband), surface-assisted, phonon-assisted, and resistive decay channels to the plasmon linewidth (Fig. 44a–d). Their results show that, above the interband threshold (∼1.6–1.8 eV for Al, Au, Cu; ∼3.5 eV for Ag), direct transitions dominate the plasmon damping. Near the Fermi level, however, phonon-assisted decay is the primary mechanism, as electron–electron scattering is negligible, making carrier lifetime and mean free path maximum. Carrier lifetimes peak at ∼30 fs for Ag, Cu, and Au, with mean free paths of ∼50 nm (Ag > Cu > Au), while Al exhibits shorter lifetimes (∼10 fs) and shorter mean free paths (∼20 nm) (Fig. 44e–h). At energies >1 eV above the Fermi level, electron–electron scattering becomes increasingly significant, reducing mean free paths to ∼10 nm at 2 eV.
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| Fig. 44 Comparison of experimental and calculated line widths, decay rates, and hot carrier lifetimes in Al, Ag, Au, and Cu. Calculated and experimental line widths (left axis) and decay rates (right axis) in (a) Al, (b) Ag, (c) Au, and (d) Cu. The theoretical curves indicate cumulative contributions from direct (or interband) transitions alone (“Direct”), including surface-assisted transitions (“+Surface”), including phonon-assisted transitions (“+Phonon”), and including resistive losses (“+Resistive”). Hot carrier lifetimes as a function of energy, accounting for electron–electron and electron–phonon contributions for (e) Al, (f) Ag, (g) Au, and (h) Cu. For each panel, the left axis measures lifetime (blue) and the right axis measures mean free path (green). The spread in the results is because of multiple electronic states at each energy with different scattering rates due to anisotropy at the microscopic level. Reproduced with permission from ref. 638, Copyright 2015 American Chemical Society. | ||
This analysis suggests that aluminum might be the most promising option for plasmonic hot carrier generation, as it not only efficiently produces hot carriers over the broadest frequency range but also generates high-energy electrons and holes with equal probability. Compared to noble metals, it demonstrates superior transport properties for high-energy holes. However, aluminum's lower absorption cross-section compared to noble metals (Au, Ag) and its poor stability due to oxidation limit its widespread use in applications.
The size dependence of e–ph scattering in noble metal nanoparticles has been widely studied, though early reports were contradictory.152,164,639–650 Staechelin et al.647 clarified that crystallinity is the key factor: polycrystalline Au nanoparticles show negligible size dependence, whereas monocrystalline AuNPs exhibit a clear decrease in e–ph scattering rate with decreasing size. Using TA spectroscopy, they tracked spectral dynamics as a “spectral thermometer” of electron temperature (Fig. 45a). At high initial electron temperatures (∼2000 K), e–ph coupling times were ∼4.4 ps for polycrystalline AuNPs and ranged from 4.6 ps (11 nm) to 6.5 ps (39 nm) for monocrystalline particles. At low electron temperatures (∼450 K), the coupling times converge (∼1.5 ps) (Fig. 45b and c). The linear relationship between τe–ph and initial electron temperature allows the extraction of electron–phonon coupling constants. The e–ph coupling constant in polycrystalline AuNPs is size-independent, remaining approximately 4 × 1016 W m−3 K−1. However, monocrystalline AuNPs show size-dependent behavior, decreasing from 3.6 × 1016 W m−3 K−1 (11 nm) to 2.4 × 1016 W m−3 K−1 (39 nm), approaching bulk values (∼2.2–2.5 × 1016 W m−3 K−1) (Fig. 45d). This effect arises from electron-surface scattering: monocrystalline particles have longer electron mean free paths, making surface-to-volume ratio important, whereas grain boundaries in polycrystalline NPs dominate scattering, rendering size less significant. Consequently, monocrystalline AuNPs exhibit longer hot-electron lifetimes, which can enhance catalytic efficiency.
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Fig. 45 Size and ligand-dependent carrier dynamics in Au nanocrystals. (a) Dynamics of the TA bleach recovery of different AuNPs after excitation with 100 µJ cm−2 pulses. Electron–phonon coupling times vs. initial electron temperature for (b) polycrystalline and (c) monocrystalline AuNPs, (d) electron–phonon coupling constants as a function of particle diameter. Literature bulk gold values are plotted as dashed lines for comparison, (e) time behavior of the induced transmission change −ΔT/T measured for the pump ≈ 3.95 eV and probe ≈ 1.32 eV in Ag nanoparticle samples, (f) size dependence of the electron thermalization time τth (or τe–e) for Ag nanoparticles in a BaO–P2O5 (dots) and Al2O3 (triangles) matrix. The full line shows the computed τth considering both the spillout and d-electron localization effects, and the dash-dotted and dotted lines of their respective contributions, (g) vs. U normalized by the unit volume of the Au NP, (h) the observed lifetime of hot electrons versus the average number of photons absorbed per NP, for the aminated (black) and thiolated (red) Au NPs, (i) electrical conductivity of various Au nanoclusters obtained using three-layered Mie theory. Part (a–d) is reproduced with permission from ref. 647, copyright 2021 American Chemical Society. Part (e and f) is reproduced with permission from ref. 646, copyright 2000 American Physical Society. Part (g and h) is reproduced with permission from ref. 651, copyright 2013 Proceedings of the National Academy of Sciences of the United States of America. Part (i) is reproduced with permission from ref. 652, copyright 2019 American Chemical Society. | ||
Voisin et al.646 studied size-dependent e–e scattering in Ag nanoparticles (1.5–13 nm) using IR pump pulses (950 nm) for intraband excitation, which alters the occupation number (Δf) around Fermi level EF and UV probe pulses for interband detection, which is sensitive to this change. Smaller particles showed faster thermalization (shorter τe–e), while τe–e increased by a factor of two as particle size increased from 3 to 26 nm (Fig. 45e). In small nanoparticles, the high surface-to-volume ratio exposes a larger electron density to inefficient Coulomb screening, thereby enhancing e–e scattering. This reduced screening efficiency stems from (i) electron spillout at the surface and (ii) core confinement of bound d-electron, which collectively lower the electron density near the surface. By accounting for electron density spillout and d-electron surface exclusion, the model (Fig. 45f) successfully reproduces the experimental size dependence. This confirms the critical role of these surface effects, though deviations occur for particles ≤2 nm due to strong confinement.
The chemical environment surrounding nanoparticles acts like a molecular atmosphere that can dramatically affect hot carrier lifetimes. Coating nanoparticle surfaces with ligands stabilizes the particles and, in the case of metals, can alter LSPR properties by changing the effective optical refractive index in the near field.653–655 The influence of the chemical environment on hot carrier lifetime has been explored in various plasmonic nanostructures.651,656–660
Aruda et al.651 sought to clarify the mechanism behind lifetime changes when switching ligands passivating Au NPs from a dative bonded alkylamine ligand (hexadecylamine) to covalently bonded alkylthiolates (hexadecanethiolate), both of similar dimensions but different bonding characteristics. They applied a temperature-dependent Mie theory model to fit TA spectra, utilizing three fitting parameters: electronic temperature Te and two temperature-dependent damping constants. The electronic heat capacity γ relates to the initial electronic temperature Tmaxe through electronic population by laser pulse (U) via:
![]() | (3) |
The reciprocal slope of
versus U (Fig. 45g) gives the electronic heat capacity γ. They observed that γ for thiolated AuNPs is 40% higher than that of aminated AuNPs. Using the general form of the two-temperature model (TTM), the temperature-dependent electron–phonon coupling constant (g = go + g1(ΔT) where ΔT = Te − TL) was found to be 30% larger for thiolated AuNPs than aminated AuNPs. The hot electron lifetime depended on both initial electronic temperature and the number of photons absorbed per particle, as both γ and g are temperature dependent. Thiolated AuNPs exhibited 20% longer hot electron lifetimes than aminated AuNPs (Fig. 45h).
This occurs because higher γ means reduced energy exchange between electrons and lattice, thus increasing hot electron lifetime, while larger g means increased energy transfer rate, thereby decreasing hot electron lifetime. These two effects partially cancel each other, leading to a net 20% increase in hot electron lifetime. The greater impact of thiolate on both g and γ compared to amine was attributed to covalently bound thiolate enhancing the density of states near the Fermi level more than amine.
Shabaninezhad et al.652 investigated passivating ligand roles on electron–phonon relaxation dynamics in the smallest-sized gold nanoclusters. They found that Au nanoclusters passivated by aromatic rings (TBBT and Sc2Ph) show greater electron–phonon coupling times compared to nanoclusters passivated with hexane thiol ligand (SC6) (Fig. 45i). The authors explained this result by noting that in Au nanoclusters passivated by aromatic ligands, electrical conductivity decreases due to Au-π interaction and conjugation, leading to decreased free electron density.
The size dependence of carrier–phonon scattering in perovskite nanocrystals has produced apparently contradictory results: some studies report faster hot carrier cooling with decreasing size,65,663 others show slower cooling,664,665 or negligible change.666,667 Yu et al.668 resolved this by using 2D electronic spectroscopy with 10 fs resolution to study CsPbI3 nanocrystals (4.6–8.2 nm, below the exciton Bohr diameter ∼12 nm) (Fig. 46). 2DES enabled separation of rapid carrier thermalization (∼20 fs) from subsequent cooling via carrier–phonon interactions (∼260 fs), which is difficult to resolve with standard TA spectroscopy.
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| Fig. 46 Size-dependent carrier dynamics in CsPbI3 nanocrystals and electron transfer kinetics in metal/semiconductor hybrid. (a) Temporal dynamics of 2DES signals probed at excitation excess energy of ΔE = 0.15 eV and different emission energy. (b) Size-dependent lifetime parameters for hot carrier dynamics. The cooling process slows down with decreasing nanocrystal size as a signature of the phonon bottleneck effect. (c) The dynamics of hot-carrier temperature with pump fluence of 5 and 50 µJ cm−2 for the average size of a nanocrystal sample of 6.7 nm. (d) Transient absorption kinetics at 3500 nm of nanocrystalline films (green: N3/TiO2, red: Au/TiO2, grey: Au/ZrO2). The blue line shows the response of the apparatus, obtained using a silicon plate. (e) Normalized curves of shell-thickness dependence of the AgNWs plasmon photobleaching decay dynamics. The probe wavelength is 349 nm. All the experiments were conducted under a pump wavelength of 320 nm (3.87 eV) with an average power of 3 mW. Part (a–c) is reproduced with permission from ref. 668, copyright 2020 American Chemical Society. Part (d) is reproduced with permission from ref. 669, copyright 2007 American Chemical Society. Part (e) is reproduced with permission from ref. 670, copyright 2018 Springer Nature Publishing Group. | ||
Analysis of the 2D signals revealed that smaller nanocrystals exhibited slower cooling, with lifetimes more than doubling as size decreased from 8.2 to 4.6 nm (Fig. 46b). Higher excess excitation energy also prolongs hot carrier lifetimes, due to Auger heating and hot-phonon bottleneck (Fig. 46c). These results highlight the interplay between size, excitation energy, and hot phonon dynamics in controlling carrier relaxation in semiconductor nanocrystals.
Surface ligand modification profoundly influences carrier dynamics in quantum dots, as ligands can change trap states and affect intraband relaxation through various mechanisms such as phonon coupling, Auger recombination, and vibrational relaxation. Surface ligands on semiconductor nanocrystals can significantly affect exciton relaxation processes.671–675 Zhang et al.671 investigated the role of alkyl ligand chain length in hot-carrier cooling processes in CsPbBr3 nanocrystals. They used two alkyl ligands: octanoic acid, C8 (OcA), and oleic acid, C18 (OA). CsPbBr3-OcA QDs exhibited longer hot-carrier cooling lifetimes (∼504 fs) compared to CsPbBr3-OA QDs (∼387 fs). This difference demonstrates that molecular vibrations of ligands can affect carrier–phonon coupling during cooling processes. The vibrational modes of the shorter-chain OcA ligand appear to disrupt the coupling between carriers and the relevant phonon modes, impeding efficient thermal relaxation.
Schnitzenbaumer et al.672 showed that capping CdSe QDs with chalcogenides (S2−, Se2−, Te2−) changed hot electron cooling times through Auger recombination, with Te2− showing a drastic decrease in hot carrier lifetime due to trap states that act as additional recombination channels.
In both semiconductor and metal nanoparticles, controlling hot carrier lifetime through nanoparticle size is possible. However, to achieve size dependence in semiconductors, one needs to synthesize nanoparticles with dimensions small enough to show quantum confinement effects, which is clearly not the case in metal nanoparticles, where classical size effects dominate.
TiO2 is a widely studied semiconductor in such heterostructures. Upon UV excitation, broad infrared absorption arises from intraband transitions and shallow mid-gap states.677 Furube et al.669,678 demonstrated electron injection from Au nanoparticles into TiO2 within 50 fs, indicating that injection occurs before or during electron–electron scattering in Au (Fig. 46d). Similarly, Cheng et al.670 showed that electron–phonon scattering times in Ag nanowires decrease when coated with thin TiO2 shells, reflecting ultrafast electron injection, which opens up an alternate decay channel, while thicker shells enable back-transfer and thus, slower relaxation (Fig. 46e). Graphene represents a unique case due to its zero band gap and, in nanostructured or doped forms, tunable plasmonic resonance in the visible-NIR. Ding et al.679 investigated ultrafast dynamics in a graphene-Ag nanowire (AgNW) hybrid using a 400 nm pump. While isolated components showed faster decays (AgNW plasmon lifetime: 150 ± 7 fs; graphene electron–phonon interaction: 1.4–2.5 ps), the hybrid system exhibited significantly prolonged lifetimes due to hot electron transfer from Ag to graphene. In the visible region, this transfer occurred at 534 ± 108 fs, resulting in a plasmon-induced hot electron lifetime of 3.2 ± 0.8 ps. In the NIR region, dynamics were notably slower: the transfer time increased to 780 ± 92 fs due to lower kinetic energy, and the electron–phonon interaction time extended to 3.9 ± 0.9 ps, attributed to graphene's enhanced optical absorption in this range. When employed as SERS substrates for the reduction of 4-nitrobenzenethiol (4NBT) to 4,4′-dimercaptoazobenzene (DMAB), the graphene-Ag nanowire hybrid demonstrated significantly higher reaction probability and efficiency compared to isolated graphene or Ag nanowires. This superior performance is attributed to a synergistic enhancement arising from the combination of plasmonic hot-electron generation in Ag and the high carrier mobility and broadband optical absorption of graphene.
This section emphasized that the efficiency of photocatalysis is fundamentally a “race against time”, where the success of a chemical transformation depends on extracting charge carriers before they relax into heat. These examples highlight the importance of understanding coherent, non-thermal, quasi-equilibrium, and isothermal regimes for optimizing charge extraction. Semiconductor excitons persist in the nanosecond-to-microsecond range, while plasmonic hot carriers exist in the femtosecond-to-picosecond domain. This temporal mismatch is both a challenge and an opportunity: by tuning plasmonic resonance and nanostructure size, high-energy carriers can be effectively injected into semiconductors, extending their useful lifetime for chemical transformations. Smaller semiconductor nanocrystals benefit from quantum confinement and phonon bottlenecks, prolonging exciton lifetimes, whereas larger metal nanocrystals reduce surface scattering to extend hot-electron lifetimes. Hybrid architectures, such as core–shell or metal-loaded semiconductor nanoparticles, provide alternative decay pathways and energy transfer mechanisms that compete with thermalization, allowing energetic carriers to drive reactions more efficiently. Optimizing such systems requires careful consideration of: (i) matching carrier lifetimes with reaction timescales, (ii) ensuring carrier energies exceed activation barriers, (iii) positioning reactive sites within carrier diffusion lengths, and (iv) maximizing interfacial charge transfer.
Ultrafast spectroscopy has transformed our understanding from viewing photocatalysis as a simple light-absorption process to recognizing it as a complex series of temporal steps where success depends on winning the race against relaxation of the excited state. The future of photocatalytic design lies not just in choosing the right materials but in tuning their temporal dynamics to create systems where quantum precision meets classical intensity, and where the excited electrons and holes can be used to drive the chemical transformations.
Excited-state dynamics play a central role in both systems. While semiconductor photocatalysis depends on efficient charge separation and transport, plasmonic photocatalysis capitalizes on short-lived hot carriers and photothermal effects. The ongoing debate around thermal versus non-thermal contributions emphasizes the complexity of plasmonic systems and the need for deeper mechanistic insights. Throughout the review, we have stressed upon the importance of advanced characterization tools in elucidating the intricate mechanisms governing photocatalysis. These techniques are essential for mapping reaction intermediates, activation energies, and transient charge dynamics.
Looking forward, the integration of plasmonic and semiconductor functionalities offers exciting opportunities for rational catalyst design. To fully realize this potential, the field must embrace emerging computational tools like predictive modeling through machine-learning-assisted design. By establishing robust descriptors, such as d-band centers, LSPR peak positions, and interfacial charge-transfer resistance, machine learning algorithms can navigate the high-dimensional design space of hybrid catalysts. This approach allows researchers to simulate thousands of material combinations, such as complex ternary alloys or hierarchical architectures, identifying optimal configurations that would take years to discover through traditional laboratory experimentation. Simultaneously, a shift toward in situ and operando spectroscopy is essential to move beyond the “black box” understanding of the catalyst surface. Future research should prioritize multi-modal operando setups that combine vibrational spectroscopy with electronic probes, such as in situ X-ray absorption or ambient-pressure XPS. Such techniques are critical for observing the real-time reconstruction of the catalyst surface and the transient stability of active sites under high-intensity illumination.
Finally, the transition from lab-scale success to industrial application hinges on addressing scalability and the cost of noble metals. Expanding the use of earth-abundant plasmonic materials requires a focus on surface passivisation and protective encapsulation to prevent oxidative deactivation without sacrificing LSPR intensity. Beyond material innovation, the development of optimized reactor geometries is essential for maximizing photon utilization efficiency. Enhancing the light-harvesting architecture of the reactor is a critical step in translating these technologies from laboratory-scale prototypes to viable industrial-scale systems. By bridging the gap between computational prediction, rigorous operando mechanistic analysis, and the development of cost-effective materials, the field of photocatalysis is poised to move toward a new era of efficient and sustainable light-driven chemistry.
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