Open Access Article
This Open Access Article is licensed under a Creative Commons Attribution-Non Commercial 3.0 Unported Licence

Constructing interfacial charge transfer channels via plasmon-mediated dual excitation in S-vacancy-rich ZnIn2S4/CuSe heterostructures for enhanced NIR-driven H2 production

Yuanyong Huang a, Cai Ninga, Xinyu Lua, Yang Chaoa, Junhao Hea, Qiankun Gaoa, Yu Yua, Zhongkai Xiea, Hailing Huoa and Weidong Shi*ab
aCollege of Environmental and Chemical Engineering, Jiangsu University of Science and Technology, Zhenjiang, 212003, P.R. China. E-mail: swd1978@ujs.edu.cn
bSchool of Chemistry and Chemical Engineering, Jiangsu University, Zhenjiang, 212013, P.R. China

Received 8th February 2026 , Accepted 6th March 2026

First published on 20th March 2026


Abstract

Conventional photocatalysts are inherently inefficient at harnessing the predominant near-infrared (NIR) component of sunlight, and their intrinsic kinetic and thermodynamic barriers further impose a severe constraint on solar-to-hydrogen (H2) conversion efficiency. However, the rational design of highly efficient, durable NIR-responsive photocatalysts that avoid scarce metal cocatalysts and toxic dyes remains a pivotal challenge. Herein, we demonstrate a new strategy for constructing a strong interfacial coupled heterojunction that strategically integrates plasmonic CuSe with S-vacancy-rich ZnIn2S4 (Vs-ZnIn2S4) to enhance NIR-driven H2 evolution through a plasmon-mediated dual excitation (PMDE) mechanism. As evidenced by ultrafast femtosecond transient absorption (fs-TA) spectroscopy and density functional theory (DFT) calculations, the rational heterointerface engineering gives rise to fast charge-transfer channels, which in turn lower the reaction energy barrier, suppress carrier recombination, and induce interfacial charge redistribution. These improvements collectively contribute to an optimized heterojunction that achieves an apparent quantum efficiency of 3.0% at 940 nm, surpassing all state-of-the-art noble-metal-free photocatalysts operating beyond 900 nm reported to date. The composite maintains its structural and catalytic integrity even under strong acidic/alkaline conditions (e.g., pH = 1 and pH = 12) and in high-salinity environments (e.g., 5.0 M NaCl solution), setting a benchmark for ultrastable NIR light-harvesting photocatalysts. This work provides novel insights into optimizing charge separation, stabilization, and accumulation during NIR-driven H2 production via PMDE.


Introduction

The global shift toward low-carbon development is driven by pressing challenges from climate change, the energy crisis, and greenhouse gas emissions.1–3 Solar-driven water splitting offers an environmentally friendly, sustainable, and scalable route to produce hydrogen (H2), positioning it as a critical component of future energy systems.4 Although photocatalytic efficiency is fundamentally determined by light harvesting, extending spectral absorption into the near-infrared (NIR) region (800–2500 nm) has become a central research target, as NIR photons account for 52% of total solar irradiance—far surpassing the UV/visible components.5–10 However, NIR-driven photocatalysis suffers from mismatched energetics and suboptimal efficiency, often due to the difficulty in balancing photon absorption, charge excitation, and surface reactions.11 Despite over four decades of research, NIR-active photocatalysts for solar H2 generation have achieved only limited progress, with both activity and stability still falling below expectations.12–23 Therefore, developing an efficient, scalable, and stable photocatalytic system capable of effectively utilizing NIR light remains a critical goal in renewable energy research. The key challenge lies in designing photocatalytic systems that can efficiently capture and utilize low-energy NIR photons to drive water splitting reactions at an industrial scale, while maintaining both high activity and long-term stability.

To date, NIR-driven photocatalytic water splitting for H2 production has primarily relied on plasmonic noble metals (e.g., Pt, Au, Ag) or organic dye sensitizers (e.g., porphyrins, phthalocyanines).24–27 Unfortunately, these systems suffer from high costs, toxicity, and photocorrosion, severely hindering catalyst sustainability and large-scale practical applications. To address these challenges, developing robust, noble metal-free NIR-active photocatalysts via tailored nanostructures and interfacial engineering has become a key research direction. For instance, Zhu et al. pioneered a 2D/2D black phosphorus/carbon nitride (BP/CN) van der Waals heterostructure, achieving efficient NIR-driven H2 evolution (0.15 µmol h−1) at λ > 780 nm for over 3 h.28 Liu et al. recently developed ultrathin CuCrP2S6 nanosheets with efficient charge transfer and long carrier lifetime, attaining a 1.03% apparent quantum efficiency (AQE) under λ = 800 nm with 16 h stability.29 Unfortunately, state-of-the-art non-precious metal NIR photocatalysts face three critical limitations: insufficient light-harvesting (λ < 800 nm), AQE values lower than 1% under NIR light, and inferior stability. These shortcomings arise from the unoptimized interplay between photon utilization, charge transport, and structural stability. To move beyond these constraints, a paradigm shift from optimizing single-component NIR-absorbing photocatalysts toward holistic multiscale engineering is imperative. Synergistic strategies involving energy band engineering, defect-state design, and heterostructural modification collectively drive simultaneous advancements in NIR photon-to-energy conversion efficiency and operational durability. However, no ultrastable noble metal-free system has yet achieved an NIR-driven AQE exceeding 2% through multiscale engineering strategies, despite their importance and high desirability.

As of the latest available research, copper chalcogenide nanocrystals (e.g., CuS, Cu1.8S, Cu7.2S4, Cu9S5, CuSe) have emerged as earth-abundant alternatives to noble metals, with strong LSPR characteristics and good structural stability.14,15,18,23,30 Endowed with intrinsic functional properties including high charge carrier mobility and potentially high carrier concentrations, these materials also exhibit superior electrical conductivity, rendering them ideal candidates for NIR-driven photocatalysis. For example, Lian et al. fabricated a CuS@ZnS core–shell nanocrystal composite modified with Pt cocatalysts, which delivered robust photocatalytic performance (0.13 µmol h−1).14 Despite these encouraging results, single-component NIR-excited copper chalcogenides still suffer from severely low photocatalytic activity (<1%), which stems from non-radiative energy transfer and falls well short of practical application requirements.10 Plasmon-mediated dual-excitation (PMDE) systems, which integrate the plasmonic effects of copper chalcogenides with compatible NIR-responsive semiconductor acceptors, are hypothesized to be a viable strategy for generating more surviving charge carriers. However, to the best of our knowledge, no reports have documented plasmonic copper chalcogenide composites that harness dual-excitation pathways to achieve highly efficient and ultrastable NIR-driven H2 evolution at wavelengths above 800 nm.

As a proof-of-concept study, the Vs-ZnIn2S4@CuSe nanocomposite was rationally designed and fabricated using a simple hydrothermal process (Fig. 1a) and employed for NIR-driven H2 production. A suite of characterization techniques was used to probe the morphology, structure, composition, and optical properties of the Vs-ZnIn2S4@CuSe heterojunctions. The robust interfacial coupling interactions within the Vs-ZnIn2S4@CuSe catalysts give rise to rapid, irreversible charge transfer pathways, effectively suppressing charge carrier recombination; meanwhile, the interfacial carrier dynamics were systematically probed via ultrafast femtosecond transient absorption (fs-TA) spectroscopy and density functional theory (DFT) calculations. The optimized heterojunction achieves the highest reported apparent quantum efficiency (AQE) of 3.0% at λ = 940 nm, setting a new benchmark for noble metal-free hybrid photocatalysts operating at wavelengths beyond 900 nm. This work presents a novel strategy for designing efficient heterojunctions for NIR-driven H2 production via a PMDE mechanism.


image file: d6sc01125j-f1.tif
Fig. 1 (a) Diagram of the formation of NIR-responsive Vs-ZnIn2S4@CuSe heterostructured photocatalysts. The morphological, structural, and elemental characteristics of the as-prepared samples are shown. Typical TEM images of pure Vs-ZnIn2S4 (b and c) and its composite with 1 wt% CuSe (d and e). Representative HRTEM images of Vs-ZnIn2S4@CuSe (f), showing the lattice fringes of ZnIn2S4 and CuSe phases. (g) HAADF-STEM and EDX elemental mapping images of Zn, In, S, Cu, and Se in Vs-ZnIn2S4@CuSe. Scale bar: 200 nm. AFM images of ZIS (h) and Z@Cu(1 wt%) (i). (j) EPR measurements of Vs-ZnIn2S4 and Z@Cu(1 wt%).

Results and discussion

Construction and structural characterization of Vs-ZnIn2S4@CuSe heterostructures

As shown in Fig. S1, CuSe, synthesized via a hydrothermal method, exhibits a hexagonal phase (Joint Committee on Power Diffraction Standards (JCPDS) No. 34-0171), which is characteristic of CuSe.31,32 The Vs-ZnIn2S4@CuSe composite predominantly exhibits the hexagonal phase of ZnIn2S4 (JCPDS No. 72–0773).7,33 The diffraction peaks for Z@Cu(1 wt%) are observed to be weaker in the composite compared to pure Vs-ZnIn2S4, suggesting that the presence of CuSe slightly alters the crystal structure of ZnIn2S4. This reduction in peak intensity may indicate changes in crystallinity or a decrease in crystallite size due to CuSe incorporation. Inductively coupled plasma optical emission spectroscopy (ICP-OES) yielded a Cu[thin space (1/6-em)]:[thin space (1/6-em)]Se ratio of 1.02[thin space (1/6-em)]:[thin space (1/6-em)]1, indicating a virtually stoichiometric 1[thin space (1/6-em)]:[thin space (1/6-em)]1 composition. Scanning electron microscopy (SEM) images show that both pure ZnIn2S4 and CuSe, and the Vs-ZnIn2S4@CuSe composites exhibit a sheet-like structure (Fig. S2). As the CuSe content increases, the stacking degree of the layers in the composite material also increases, suggesting the self-assembly nature of the material.

Transmission electron microscopy (TEM) and high-resolution TEM (HRTEM) images (Fig. 1b–f) reveal that the Vs-ZnIn2S4@CuSe composite has a thicker layered structure compared to the pure Vs-ZnIn2S4 (Fig. S3). The images confirm the successful integration of CuSe into the Vs-ZnIn2S4 structure. The lattice spacings observed in the HRTEM images are 0.32 nm, corresponding to the (102) crystal planes of ZnIn2S4, and 0.29 nm, corresponding to the (006) crystal planes of CuSe, respectively. These lattice spacings further support the successful formation of the Vs-ZnIn2S4@CuSe nanohybrid. Energy dispersive X-ray (EDX) elemental mapping confirms the uniform distribution of Zn, In, S, Cu, and Se across the composite surface. This uniform distribution indicates that CuSe is effectively integrated with Vs-ZnIn2S4 (Fig. 1g and S4). The thickness of Vs-ZnIn2S4 and Z@Cu(1 wt%) was evaluated by atomic force microscopy (AFM). AFM images reveal that pure Vs-ZnIn2S4 has a thickness of approximately 1.6 nm, and the nanocomposite Z@Cu(1 wt%) shows an increased thickness of about 5.4 nm, suggesting that CuSe incorporation results in a thicker, more layered material (Fig. 1h and i). Additionally, electron paramagnetic resonance (EPR) measurements were used to confirm the presence of sulfur (S) vacancies in the Vs-ZnIn2S4@CuSe composites. A slightly stronger signal at g = 2.003 was observed for the Vs-ZnIn2S4@CuSe composite compared to pure Vs-ZnIn2S4, suggesting a higher concentration of paramagnetic centers (Fig. 1j).14

X-ray photoelectron spectroscopy (XPS) provides detailed information on the valence states and surface chemical compositions of the Vs-ZnIn2S4@CuSe composites. As shown in Fig. S5a, the Cu 2p spectrum of CuSe nanosheets exhibits two characteristic peaks: Cu 2p3/2 at 931.9 eV and Cu 2p1/2 at 952.4 eV, corresponding to the Cu2+ species. These peaks confirm that CuSe predominantly exists in the Cu2+ oxidation state.34 The Cu 2p peaks of the Vs-ZnIn2S4@CuSe composites shift to lower binding energies by approximately 0.1 eV compared to pure CuSe, suggesting the formation of an interface between CuSe and Vs-ZnIn2S4 due to their electronic interactions. As shown in Fig. S5b, the Zn 2p3/2 and Zn 2p1/2 peaks of pure Vs-ZnIn2S4 are observed at 1021.3 eV and 1044.4 eV, respectively, indicating the presence of Zn2+ ions.35 In the Vs-ZnIn2S4@CuSe composites, these Zn 2p peaks shift to higher binding energies by about 0.1 eV. This shift suggests that the Zn2+ ions are influenced by the interaction with CuSe, resulting in a modified electronic environment around Vs-ZnIn2S4. This shift also implies the formation of a built-in electric field between CuSe and Vs-ZnIn2S4, which facilitates the transfer of photogenerated carriers at the interface, a similar phenomenon to that previously reported in plasmonic composite materials (such as WO3@ZnIn2S4).36 The In 3d spectrum of Vs-ZnIn2S4 is deconvoluted into two peaks at 452.2 eV and 444.7 eV, which correspond to the In3+ oxidation state (Fig. S5c).37 In the composites, the In 3d peaks shift to higher binding energies, similar to the behavior observed for the Zn 2p peaks. This shift further supports the formation of the built-in electric field, influencing the electronic states of In3+ in the Vs-ZnIn2S4 counterpart. The S 2p spectrum of the composites shows an S 2p3/2 peak at 161.5 eV and S 2p1/2 peak at 162.8 eV (Fig. S5d). These binding energies are slightly higher than those observed in pure Vs-ZnIn2S4, indicating a shift in the chemical environment of S2− due to the interaction with CuSe.38 The Cu 2p, Zn 2p, In 3d, and S 2p peaks all exhibit shifts in binding energy upon the formation of the Vs-ZnIn2S4@CuSe composite, indicating electronic interactions between CuSe and Vs-ZnIn2S4.

Optical characteristics and photoactivity evaluation

The ability of a photocatalyst to capture NIR photons is one of the most crucial factors in NIR-driven water splitting to produce H2.39 As shown in Fig. 2a, CuSe exhibits strong absorption in the NIR region, making it an effective material for NIR photon harvesting. In contrast, Vs-ZnIn2S4 demonstrates weak NIR absorption on its own. However, when combined in the Vs-ZnIn2S4@CuSe composites, the overall NIR light harvesting capacity is markedly enhanced, particularly with increasing CuSe loading from 0.5 wt% to 2 wt%. This enhancement is due to the LSPR effect of CuSe, which allows it to absorb more NIR light.40 When these plasmonic materials are excited by NIR photons, their free electrons resonate with the incident light, leading to enhanced light absorption and increased electron generation for the photocatalytic process.41 As a result, the Vs-ZnIn2S4@CuSe composites can achieve enhanced broad-spectrum light harvesting, including NIR light, which is typically underutilized in conventional photocatalysts.
image file: d6sc01125j-f2.tif
Fig. 2 (a) UV-vis-NIR absorption spectra of pristine CuSe and Vs-ZnIn2S4, and their composites. (b) H2 production performance of pristine CuSe and Vs-ZnIn2S4, and their corresponding composites under NIR light (λ > 800 nm) for 3 hours. (c) H2 production rates of pristine CuSe and Vs-ZnIn2S4, and their corresponding composites under NIR light (λ > 800 nm) over time. (d) Comparison of the H2 production activity with previously reported plasmonic photocatalysts under NIR light. (e) Photostability evaluation under continuous NIR light irradiation (λ > 800 nm). (f) Photostability, H2 production rate, and AQE under monochromatic NIR light, compared with currently reported NIR-responsive photocatalytic systems under similar conditions.

Photocatalytic performance was evaluated under NIR irradiation (λ > 800 nm) using triethanolamine (TEOA) as a sacrificial agent. As shown in Fig. 2b, pure-phase CuSe produced 0.58 µmol of H2 after 3 h of irradiation. Pristine Vs-ZnIn2S4, with abundant sulfur vacancies, exhibited improved performance (2.45 µmol of H2 under identical conditions), attributable to its Urbach band tail absorption that extends its photo-response into the NIR region beyond UV/visible light.7,35,42 Upon coupling CuSe with Vs-ZnIn2S4, NIR-driven H2 production was significantly enhanced. Specifically, 0.5 wt% CuSe loading yielded 6.42 µmol of H2 after 3 h, while 1 wt% loading increased H2 evolution to 11.6 µmol. However, a higher loading of 2 wt% reduced H2 production to 3.3 µmol, indicating that optimal CuSe loading (around 1 wt%) results in the best balance between NIR light absorption and efficient electron transfer.43,44 Comparative studies of sacrificial agents (Fig. S6) confirmed that TEOA provides the highest H2 evolution, likely due to its effective electron donation and catalyst stabilization.45 Consequently, TEOA was selected for subsequent photocatalytic tests. The Z@Cu(1 wt%) composite demonstrated sustained activity with 54.2 µmol of H2 generated over 15 h (Fig. 2c), highlighting its potential for practical NIR-driven water splitting. Notably, this catalyst outperformed previously reported plasmonic photocatalytic systems in the half-reaction of water splitting (Fig. 2d & Table S1), underscoring its efficiency in NIR light utilization. Moreover, the optimal sample achieved a high H2 evolution rate of 2.18 µmol h−1 at λ = 940 nm, corresponding to an apparent quantum efficiency (AQE) of 3.0%. To our knowledge, this represents the best performance reported for noble-metal-free hybrid photocatalysts at wavelengths above 900 nm (Table S2), providing a valuable benchmark for future NIR-responsive photocatalyst design. Additionally, the stability of photocatalysts is essential for their reliability, longevity, and economic feasibility in practical applications.46 The Z@Cu(1 wt%) composite maintained stable performance over 48 h of continuous NIR irradiation (Fig. 2e). In a nine-cycle stability experiment, the photocatalytic activity showed almost no degradation compared to the initial run (Fig. S7). XRD patterns collected before and after cycling revealed no significant structural changes, confirming the material's robustness (Fig. S8). Remarkably, Z@Cu(1 wt%) also retained both structural integrity and catalytic function under strongly acidic (pH = 1) and strongly alkaline (pH = 12) conditions (Fig. S9 and S10), in striking contrast to the degradation or phase transformation commonly observed for many photocatalysts in such harsh environments. Moreover, the material exhibited excellent stability in high-salt media, indicating strong resistance to ionic interference (Fig. S11)—a crucial feature for practical applications involving saline or seawater sources. To the best of our knowledge, the overall stability of Z@Cu(1 wt%) surpasses that of all previously reported non-noble-metal NIR-driven photocatalytic systems (Fig. 2f and Table S3).

Charge separation and transfer ability

To elucidate the enhanced photocatalytic activity, a series of electrochemical and photophysical characterization studies were conducted. Beyond light absorption, efficient separation of photogenerated carriers critically governs photocatalytic performance.47 Transient photocurrent measurements revealed that under NIR illumination, the current response increased with CuSe loading up to 1 wt% but declined at 2 wt% (Fig. S12), mirroring the photocatalytic activity trend. Z@Cu(1 wt%) exhibited a photocurrent density of ∼3.24 µA cm−2, markedly higher than that of pristine Vs-ZnIn2S4 (0.27 µA cm−2), indicating enhanced charge separation upon CuSe integration.48 Electron paramagnetic resonance (EPR) analysis using DMPO as a trapping agent further confirmed improved carrier separation. Under NIR light, Z@Cu(1 wt%) showed a substantially stronger ˙O2− signal than pure Vs-ZnIn2S4 (Fig. S13), consistent with more efficient photogenerated carrier separation.49 Electrochemical impedance spectroscopy (EIS) Nyquist plots displayed a smaller semicircle for Z@Cu(1 wt%) compared to Vs-ZnIn2S4 (Fig. S14), suggesting facilitated interfacial charge transfer.50 Additionally, photoluminescence (PL) spectra demonstrated significant quenching for Z@Cu(1 wt%) relative to the pristine counterpart (Fig. S15), corroborating suppressed charge recombination and enhanced separation efficiency.51

Mechanism study

To elucidate the NIR-driven water-splitting mechanism, the carrier dynamics in the Vs-ZnIn2S4@CuSe plasmonic composite were investigated using femtosecond transient absorption (fs-TA) spectroscopy. Upon 400 nm excitation and probing from 820 to 1400 nm (Fig. 3a and b), both ZIS and Z@Cu(1 wt%) show negative signals (stimulated emission, SE) at 890–980 nm, consistent with their steady-state fluorescence (Fig. S15). While ZIS exhibits two excited-state absorption (ESA) bands (960–1160 nm and 1160–1400 nm) with distinct kinetics, Z@Cu(1 wt%) presents an additional ESA band at 840–940 nm, attributed to CuSe modification. Temporal evolution analysis (Fig. 3c and d) reveals positive ESA signals in both samples following excitation (ZIS: 960–1400 nm; Z@Cu(1 wt%): 840–940 nm + 960–1400 nm). Within the initial sub-picosecond regime (0–1 ps), these ESA features decay rapidly, accompanied by the emergence of negative SE bands at 890–980 nm. For ZIS, ESA at 960–1160 nm vanishes, leaving only the 1160–1400 nm band. For Z@Cu(1 wt%), ESA at 840–940 nm and 960–1060 nm vanishes, leaving only the 1060–1400 nm band. Subsequently (1–10 ps), the SE bands in both samples narrow progressively and undergo red-shifting, while long-wavelength ESA components gradually diminish. At longer time scales (10–100 ps), the SE bands in both samples further weaken with slight additional red-shifting, concurrent with continued decay of the residual ESA signals. Finally, within the instrument response window (up to 7 ns), all transient signals nearly fully decay. Notably, Z@Cu(1 wt%) exhibits significantly shorter excited-state lifetimes than ZIS, revealing accelerated relaxation dynamics induced by CuSe modification. Global fitting analysis of the transient absorption data (Fig. 3e and f) reveals distinct species-associated difference spectra (SADS). For ZIS, the initial species (Species A, red trace) exhibits an SE band at 820–920 nm and a pronounced excited-state absorption (ESA) feature centered near 1000 nm. This excited-state species forms instantaneously upon photoexcitation. Subsequently, an ultrafast sub-500 fs relaxation (0.4 ps) populates Species B (yellow trace), characterized by: (i) the disappearance of the ∼1000 nm ESA, (ii) the emergence of a new SE band at ∼940 nm, and (iii) the appearance of an additional ESA band spanning 1100–1400 nm. This distinct spectral evolution unequivocally establishes Species A and B as separate excited-state entities, with the transformation directly attributable to the incipient stage of charge separation.52 Subsequently, Species B transforms into Species C (cyan) at 14.6 ps, accompanied by a narrowing of the SE signal. The B → C process may be attributed to the recombination of electrons and holes in the bulk phase.53 Meanwhile, the excited-state absorption (ESA) signal at longer wavelengths gradually weakens. This is followed by the conversion of Species C to Species D (purple) on a longer timescale (621.9 ps), during which the SE signal and the long-wavelength ESA signal progressively diminish. Concurrently, a new ESA signal emerges around 1000 nm, indicating relaxation to a new excited state. The C → D process is attributed to a charge transfer route.54 Finally, Species D almost completely decays within the experimental time window, with a fitted lifetime of 5 ns, which is tentatively attributed to a charge recombination process.32 Upon CuSe composite formation, the Z@Cu(1 wt%) sample exhibits an additional excited-state absorption (ESA) signal around 900 nm in the initial excited state species A (red) compared to pristine ZIS, which is attributed to the modification with CuSe. The subsequent excited-state transformation features spectral similarities to those of ZIS. Specifically, the A → B process generates a new SE signal and an ESA signal beyond 1050 nm. The timescale of this process is comparable to that observed in ZIS, indicating that the introduction of CuSe does not affect this specific relaxation pathway. Subsequently, the B → C → D process, although spectrally identical to that in ZIS, exhibits a significantly accelerated relaxation rate, and the C → D process (126.1 ps) is about five times faster. These results indicate that after CuSe modification, photogenerated carriers have more opportunities to migrate to the catalyst surface, thereby leading to enhanced water splitting performance. Additionally, kinetic traces at four wavelengths (860, 940, 1000, and 1200 nm) were selected for display (Fig. S16), demonstrating the high quality of the global fitting analysis. Furthermore, the temporal evolution profiles of species concentrations reveal that the relaxation times of the last three species (A, B, and C) in Z@Cu(1 wt%) are significantly faster than those in ZIS (Fig. S17).
image file: d6sc01125j-f3.tif
Fig. 3 (a and b) Two-dimensional (2D) pseudo-colour plot of NIR-region transient absorption spectra, with excitation at 400 nm, for pristine Vs-ZnIn2S4 and Z@Cu(1 wt%), respectively. [X-axis: probe wavelength; Y-axis: pump–probe delay; colors represent the change in absorbance (ΔA) in milli-optical density units (mOD)]. (c and d) Transient absorption (TA) spectra at different time delays, with excitation at 400 nm, for pristine Vs-ZnIn2S4 and Z@Cu(1 wt%), respectively. Global fitting analysis of the species-associated difference spectra (SADS) for (e) ZIS and (f) Z@Cu(1 wt%).

Furthermore, the study compared two modes for the photocatalytic process: PMDE and PMSE (plasmon-mediated single-excitation) modes (Fig. S18). In the PMSE mode, the performance was mediocre when 1 wt% CuSe was combined with UV-responsive (TiO2) or visible light-responsive (g-C3N4) semiconductors, suggesting that these combinations are less efficient in utilizing NIR photons for water splitting. However, in the PMDE mode, when 1 wt% CuSe was combined with NIR light-harvesting catalysts like Vs-ZnIn2S4, the performance improved remarkably. This suggests that PMDE is a more favorable approach for enhancing the NIR-driven photocatalytic process. The PMDE route seems to offer superior performance for NIR-driven water splitting because it likely promotes better electron excitation and charge separation when combined with NIR-responsive catalysts like Vs-ZnIn2S4. Building upon previously reported studies of NIR-responsive plasmonic photocatalysts and our experimental results, we propose a possible PMDE mechanism for NIR-driven water splitting (Fig. 4). Unlike traditional PMSE mechanisms for NIR-driven photoredox reactions, the PMDE pathway facilitates the generation of more surviving carriers that are essential for triggering efficient photocatalytic H2 production. In this proposed possible mechanism, the plasmonic CuSe is photochemically excited via the LSPR effect under NIR light, generating hot electrons and holes. These plasmon-induced hot electrons can then be transferred from CuSe to the NIR-activated semiconducting phase (Vs-ZnIn2S4). This transfer allows for the accumulation of hot carriers, which are crucial for highly efficient NIR-driven H2 production.


image file: d6sc01125j-f4.tif
Fig. 4 Schematic of the newly developed plasmon-mediated photocatalysts using the earth-abundant copper chalcogenide (CuSe) for NIR-driven photocatalytic H2 production. A possible band diagram and NIR-induced carrier dynamics in the plasmonic heterojunction are shown, illustrating the NIR light-driven photocatalytic reaction (Eu: the energy of the band tail, also referred to as the Urbach energy).

Theoretical calculation analysis

To further elucidate the electronic and catalytic properties of the Vs-ZnIn2S4@CuSe heterostructure, we performed density functional theory (DFT) calculations in this study. The spin-polarized DFT calculations were performed in the Device Studio-integrated Projector Augmented-Wave method package (DS-PAW), with the aid of DS-PAW for calculating the projected density of states (PDOS), Bader charge transfer, and charge density difference.55 The optimized geometries of the Vs-ZnIn2S4@CuSe heterostructure are depicted in Fig. 5a and b. From these results, it can be inferred that the lattice mismatch ratio between Vs-ZnIn2S4 and CuSe is less than 3%, which is highly favorable for the formation of a well-integrated heterojunction. Additionally, the binding energy of the Vs-ZnIn2S4@CuSe heterostructure is found to be −5.03 eV per unit cell, indicating a strong interaction between the components, which is a crucial factor for ensuring the stability of NIR-driven water splitting within the heterostructure. The charge density difference diagram, shown in Fig. 5c, represents the regions of charge accumulation and depletion, providing insights into the electron redistribution at the interface of the heterostructure. A notable depletion of charge occurs in the CuSe component, while charge accumulation is observed in the Vs-ZnIn2S4 layer. Bader charge transfer analysis reveals an approximate charge transfer of 0.16 |e| from CuSe to Vs-ZnIn2S4. This suggests that the electronic states are predominantly localized on the Vs-ZnIn2S4 side of the interface, further confirming the favorable electronic properties of this layer.56 The projected density of states (PDOS) analysis offers additional insight into the contributions of both Vs-ZnIn2S4 and CuSe to the overall electronic properties of the heterostructure. As shown in Fig. 5d, the interaction between Cu 3d orbitals and Se 3p orbitals, along with the associated electron transitions, plays a pivotal role in the NIR light absorption capabilities of CuSe. The PDOS of CuSe reflects its metallic characteristics, with a significant number of electronic states at the Fermi level (Ef), especially those derived from the Cu 3d and Se 3p orbitals, which are indicative of its electrical conductivity. Fig. 5e demonstrates how the distinct orbital densities of states of S, In, and Zn in the Vs-ZnIn2S4 layer influence its NIR absorption properties. The presence of sulfur-rich defects enhances the optical absorption of the material, particularly in the NIR region, by generating localized states near the S 2p orbitals. The contributions from S 2p and In 4d orbitals are particularly crucial, as they facilitate NIR light absorption via orbital interactions and electronic transitions. Moreover, as shown in Fig. 5f, the incorporation of CuSe into Vs-ZnIn2S4 significantly improves the electronic conductivity of the composite, primarily due to orbital hybridization and electronic interactions at the heterojunction interface. One of the critical steps in NIR-driven water splitting is the efficient adsorption of protons and water molecules on the surface of the photocatalyst (Fig. 5g and h). Upon combining with CuSe, the ΔGH value for the composite system drops drastically from 0.88 eV for pure Vs-ZnIn2S4 to 0.16 eV (Fig. 5i), suggesting that H2 generation becomes significantly easier in the composite system compared to the pure counterpart. Furthermore, the adsorption energy of water molecules is notably negative for Vs-ZnIn2S4@CuSe, indicating that water molecules are readily adsorbed onto the surface (Fig. 5j). This enhanced adsorption property is highly beneficial for NIR-driven photocatalytic water splitting, as it facilitates efficient interaction between the photocatalyst and water molecules.
image file: d6sc01125j-f5.tif
Fig. 5 (a) Top and (b) side views of the Vs-ZnIn2S4@CuSe heterostructural model. (c) Charge density difference diagram for the Vs-ZnIn2S4@CuSe heterostructure, where pink and green areas represent charge accumulation and charge depletion, respectively. The projected density of states (PDOS) of (d) CuSe, (e) Vs-ZnIn2S4, and (f) the Vs-ZnIn2S4@CuSe heterojunctions are shown, with the Fermi energy (Ef) set to zero at the midgap. (g) H+ adsorption model for the Vs-ZnIn2S4@CuSe heterojunction. (h) H2O adsorption model for the Vs-ZnIn2S4@CuSe heterojunction. (i) Gibbs free energy curves for the hydrogen evolution reaction (HER) process on CuSe, Vs-ZnIn2S4, and Vs-ZnIn2S4@CuSe heterojunctions, respectively. (j) H2O adsorption energy for CuSe, Vs-ZnIn2S4, and Vs-ZnIn2S4@CuSe heterojunctions, respectively.

Conclusions

In summary, we report on the controlled regulation of a plasmonic nanocomposite photocatalyst (Vs-ZnIn2S4@CuSe), which enables the demonstration of unique PMDE modes for highly efficient and stable NIR-driven H2 production. Photoelectrochemical characterization combined with theoretical calculations confirmed that the unique LSPR effect of CuSe species enhances NIR photon absorption, facilitates hot carrier generation, reduces the reaction energy barrier, inhibits charge recombination, and triggers interfacial charge redistribution synergistically. The optimized Vs-ZnIn2S4@CuSe nanohybrid achieves a superior H2 production rate of 2.18 µmol h−1 with an apparent quantum efficiency (AQE) of 3.0% at λ = 940 nm, representing the highest value reported to date for noble-metal-free hybrid photocatalysts at wavelengths exceeding 900 nm. Moreover, the optimized catalyst maintains long-term structural stability under harsh conditions including strong acidic, basic and high-salinity environments during continuous NIR light irradiation. This rational heterostructural interfacial coupling strategy presents an innovative paradigm for designing and constructing highly efficient and ultrastable NIR-responsive photocatalysts via PMDE. This PMDE-derived interfacial coupling strategy can be further extended to other plasmonic–semiconductor systems to harvest low-energy photons for diverse catalytic applications in the future.

Author contributions

Conceptualization: Yuanyong Huang and Weidong Shi. Formal analysis: Yuanyong Huang, Cai Ning, Yu Yu, Zhongkai Xie, and Hailing Huo. Funding acquisition: Yuanyong Huang, Cai Ning, Yu Yu, Zhongkai Xie, Hailing Huo, and Weidong Shi. Investigation: Yuanyong Huang, Xinyu Lu, Yang Chao, Junhao He, and Qiankun Gao. Methodology: Yuanyong Huang, Xinyu Lu, Yang Chao, Junhao He, and Qiankun Gao. Supervision: Weidong Shi. Writing – original draft: Yuanyong Huang and Weidong Shi. Writing – review & editing: Yuanyong Huang, Cai Ning, and Weidong Shi. All authors contributed to the discussion of the results and the preparation of the manuscript.

Conflicts of interest

There are no conflicts to declare.

Data availability

The authors declare that the data supporting the findings of this study are available within the article and its supplementary information (SI). Supplementary information is available. See DOI: https://doi.org/10.1039/d6sc01125j.

Acknowledgements

This work was supported by the National Natural Science Foundation of China (22225808, U24A20551, 22508148, 22503039, 2240082215), Jiangsu Province Innovation Support Program International Science and Technology Cooperation Project (BZ2022045), Natural Science Foundation of Jiangsu Province (BK20251008, BK20251012), Science and Technology Bureau of Zhenjiang (JC2025024), High-level Talent Cultivation Project of Jiangsu University of Science and Technology (1112932503, 1112932403, 1112932402, 1112932603) and the Special Scientific Research Project of School of Emergency Management, Jiangsu University (KY-A-02). Author Weidong Shi was partially supported by the postgraduate research opportunities program of HZWTECH (HZWTECH-PROP).

Notes and references

  1. P. Zhou, I. A. Navid, Y. J. Ma, Y. X. Xiao, P. Wang, Z. W. Ye, B. W. Zhou, K. Sun and Z. T. Mi, Nature, 2023, 613, 66–70 CrossRef CAS PubMed.
  2. B. Su, K. Tang, J. J. Cai, X. H. Lin, W. D. Xing, K. L. Liu, X. F. Lu, Y. D. Hou, W.-J. Ong and S. B. Wang, ACS Catal., 2026, 16(5), 5208–5217 CrossRef.
  3. M. Hartkorn, R. Kampes, F. Müller, L. Zedler, A. Edwards, P. Rohland, A. K. Mengele, S. Zechel, M. D. Hager, B. Dietzek-Ivanšić, M. Schmitt, J. Popp, U. S. Schubert and S. Rau, Nat. Commun., 2026, 17, 1141 CrossRef CAS PubMed.
  4. R. T. Chen, Z. F. Ren, Y. Liang, G. H. Zhang, T. Dittrich, R. Z. Liu, Y. Liu, Y. Zhao, S. Pang, H. Y. An, C. W. Ni, P. W. Zhou, K. L. Han, F. T. Fan and C. Li, Nature, 2022, 610, 296–301 CrossRef CAS PubMed.
  5. A. Rodríguez-Camargo, M. W. Terban, M. Paetsch, E. A. Rico, D. Graf, R. Hirpara, V. Duppel, I. Moudrakovski, M. Etter, N. Guijarro, C. Ochsenfeld, R. E. Dinnebier, L. Yao and B. V. Lotsch, Nat. Synth., 2025, 4, 710–719 CrossRef.
  6. Y. Y. Huang, D. Li, S. Feng, Y. J. Jia, S. H. Guo, X. J. Wu, M. Chen and W. D. Shi, Angew. Chem., Int. Ed., 2022, 61(45), e202212234 CrossRef CAS PubMed.
  7. Y. Y. Huang, H. Yang, S. Feng, C. W. Ma, P. Y. Cao, F. F. Li, X. Y. Lu and W. D. Shi, Sci. China Mater., 2024, 67, 1812–1819 CrossRef CAS.
  8. N. Li, H. K. Fan, Y. J. Dai, J. Kong and L. Ge, Appl. Surf. Sci., 2020, 508, 145200 CrossRef CAS.
  9. W. H. Xue, H. L. Sun, X. Y. Hu, X. Bai, J. Fan and E. Z. Liu, Chin. J. Catal., 2022, 43(2), 234–245 CrossRef CAS.
  10. P. Y. Hsieh, J. Y. Wu, T. F. M. Chang, C. Y. Chen, M. Sone and Y. J. Hsu, Arab. J. Chem., 2020, 13, 8372–8387 CrossRef CAS.
  11. L. L. Wang, R. J. Sa, Y. C. Wei, X. F. Ma, C. G. Lu, H. W. Huang, E. Fron, M. Liu, W. Wang, S. P. Huang, J. Hofkens, M. B. J. Roeffaers, Y.-J. Wang, J. H. Wang, J. L. Long, X. Z. Fu and R. S. Yuan, Angew. Chem., Int. Ed., 2022, 61(39), e202204561 CrossRef CAS PubMed.
  12. R. Yu, B. F. Luo, M. Chen, D. B. Xu, X. J. Wu, D. Li, Y. Y. Huang, Z. K. Xie, N. J. Shen, S. C. Meng and W. D. Shi, Int. J. Hydrogen Energy, 2023, 48(63), 24285–24294 CrossRef CAS.
  13. Z. C. Lian, Y. Kobayashi, J. J. M. Vequizo, C. S. K. Ranasinghe, A. Yamakata, T. Nagai, K. Kimoto, K. Kobayashi, K. Tanaka, T. Teranishi and M. Sakamoto, Nat. Sustain., 2022, 5, 1092–1099 CrossRef.
  14. Z. C. Lian, F. Wu, J. Z. Zi, G. S. Li, W. Wang and H. X. Li, J. Am. Chem. Soc., 2023, 145(28), 15482–15487 CrossRef CAS PubMed.
  15. Z. C. Lian, M. Sakamoto, J. J. M. Vequizo, C. S. K. Ranasinghe, A. Y. Takuro, N. K. Yoichi, K. N. Tamai and T. Teranishi, J. Am. Chem. Soc., 2019, 141(6), 2446–2450 CrossRef CAS PubMed.
  16. X. Y. Cai, M. S. Zhu, O. A. Elbanna, M. Fujitsuka, S. Kim, L. Mao, J. Y. Zhang and T. Majima, ACS Catal., 2018, 8(1), 122–131 CrossRef CAS.
  17. Z. C. Lian, F. Wu, Y. Q. Zhong, J. Z. Zi, Z. Li, X. Wang, T. Nakagawa, H. X. Li and M. Sakamoto, Appl. Catal., B, 2022, 318, 121860 CrossRef CAS.
  18. M. S. Zhu, C. Y. Zhai, M. Fujitsuka and T. Majima, Appl. Catal., B, 2018, 221, 645–651 CrossRef CAS.
  19. Y. S. Xu, M. J. Fan, W. J. Yang, Y. H. Xiao, L. T. Zeng, X. Wu, Q. H. Xu, C. L. Su and Q. J. He, Adv. Mater., 2021, 33(39), 2101455 CrossRef CAS PubMed.
  20. G. Q. Zhang, Y. S. Xu, M. Rauf, J. Y. Zhu, Y. L. Li, C. X. He, X. Z. Ren, P. X. Zhang and H. W. Mi, Adv. Sci., 2022, 9(21), 2201677 CrossRef CAS PubMed.
  21. S. S. Huang, Y. X. Zhang, C. F. Du and Y. G. Su, Chem. Commun., 2020, 56(45), 6054–6057 RSC.
  22. Y. Y. Huang, Y. P. Jian, L. H. Li, D. Li, Z. Y. Fang, W. X. Dong, Y. H. Lu, B. F. Luo, R. J. Chen, Y. C. Yang, M. Chen and W. D. Shi, Angew. Chem., Int. Ed., 2021, 60(10), 5245–5249 CrossRef CAS PubMed.
  23. Y. Lu, X. F. Jia, Z. Y. Ma, Y. Li, S. Yue, X. F. Liu and J. Y. Zhang, Adv. Funct. Mater., 2022, 32(35), 2203638 CrossRef CAS.
  24. C. W. Tsao, S. Narra, J. C. Kao, Y.-C. Lin, C.-Y. Chen, Y.-C. Chin, Z.-J. Huang, W.-H. Huang, C.-C. Huang, C.-W. Luo, J.-P. Chou, S. Ogata, M. Sone, M. H. Huang, T.-F. M. Chang, Y.-C. Lo, Y.-G. Lin, E. W.-G. Diau and Y.-J. Hsu, Nat. Commun., 2024, 15, 413 CrossRef CAS PubMed.
  25. L. Ma, D. J. Yang, X. P. Song, H.-X. Li, S.-J. Ding, L. Xiong, P.-L. Qin and X.-B. Chen, Sol. RRL, 2020, 4(1), 1900376 CrossRef CAS.
  26. J. Y. Qin and H. P. Zeng, Appl. Catal., B, 2017, 209, 161–173 CrossRef CAS.
  27. Z. L. Xia, R. Yu, H. Yang, B. F. Luo, Y. Y. Huang, D. Li, J. Y. Shi and D. B. Xu, Int. J. Hydrogen Energy, 2022, 47(27), 13340–13350 CrossRef CAS.
  28. M. S. Zhu, S. Kim, L. Mao, M. Fujitsuka, J. Y. Zhang, X. C. Wang and T. Majima, J. Am. Chem. Soc., 2017, 139(37), 13234–13242 CrossRef CAS PubMed.
  29. B. Lin, R. H. Duan, Y. H. Li, W. B. Hua, Y. Zhou, J. D. Zhou, J. Di, X. Luo, H. Li, W. T. Zhao, G. D. Yang, Z. Liu and F. C. Liu, Adv. Mater., 2024, 36(32), 2404833 CrossRef CAS PubMed.
  30. N. Li, Y. P. Qiu, L. P. Li, J. T. Zhang, S. F. Xu, Y. Q. Gao and L. Ge, Sep. Purif. Tecnol., 2025, 353, 128305 CrossRef CAS.
  31. N. Li, H. K. Fan, W. W. Zhao, Y. Q. Gao and L. Ge, Appl. Surf. Sci., 2022, 590, 153028 CrossRef CAS.
  32. H. B. Chen, Y. J. Xing, S. T. Liu, J. L. Fu, H. L. Shi, Y. J. Liang, L. J. Wang and W. Z. Wang, J. Colloid Interface Sci., 2022, 613, 103–116 CrossRef CAS PubMed.
  33. Y. C. Wang, M. J. Liu, C. X. Wu, J. P. Gao, M. Li, Z. P. Xing, Z. Z. Li and W. Zhou, Small, 2022, 18(31), 2270167 CrossRef.
  34. M. Huang, X. Wang, G. X. Jing, C. C. Meng, Y. C. Li, X. H. Li, L. Z. Fan, Y. Wan and S. H. Yang, J. Phys. Chem. Lett., 2021, 12(33), 7988–7996 CrossRef CAS PubMed.
  35. H. Yang, Y. Y. Huang, B. F. Luo, Z. K. Xie, D. Li, D. B. Xu, Y. Lei and W. D. Shi, Chem. Commun., 2024, 60, 1035–1038 RSC.
  36. Y. H. Li, M. Y. Qi, Z. R. Tang and Y. J. Xu, J. Phys. Chem. C, 2022, 126(4), 1872–1880 CrossRef CAS.
  37. X. W. Ruan, S. L. Zhao, M. H. Xu, D. X. Jiao, J. Leng, G. Z. Fang, D. P. Meng, Z. F. Jiang, S. Y. Jin, X. Q. Cui and S. K. Ravi, Adv. Energy Mater., 2024, 14(36), 2401744 CrossRef CAS.
  38. S. N. Li, L. X. Meng, W. Tian and L. Li, Adv. Energy Mater., 2022, 12(22), 2200629 CrossRef CAS.
  39. Z. Z. Chen, Y. J. Yan, K. Q. Sun, L. Tan, F. Guo, X. Du and W. L. Shi, J. Colloid Interface Sci., 2024, 661, 12–22 CrossRef CAS PubMed.
  40. N. Li, L. P. Li, Y. P. Qiu, X. H. Liu, J. T. Zhang, Y. Q. Gao and L. Ge, Nanocale, 2024, 16, 8151–8161 CAS.
  41. X. L. Liu, B. B. Huang, J. Li, B. J. Li and Z. Z. Lou, Mater. Horiz., 2024, 11, 5470–5498 RSC.
  42. X. J. Wu, D. Li, B. F. Luo, B. Y. Chen, Y. Y. Huang, T. T. Yu, N. J. Shen, L. H. Li and W. D. Shi, Appl. Catal., B, 2023, 325, 122292 CrossRef CAS.
  43. J. T. Lee, H. H. Tseng and M. Y. Wey, Sol. Energy, 2022, 231, 949–957 CrossRef CAS.
  44. W. H. Lee, C. W. Lee, G. D. Cha, B.-H. Lee, J. H. Jeong, H. Park, J. Heo, M. S. Bootharaju, S.-H. Sunwoo, J. H. Kim, K. H. Ahn, D.-H. Kim and T. Hyeon, Nat. Nanotechnol., 2023, 18, 754–762 CrossRef CAS PubMed.
  45. A. Sherryna, M. Tahir and Z. Y. Zakaria, Int. J. Hydrogen Energy, 2024, 51, 1511–1531 CrossRef CAS.
  46. Y. F. Chen, L. Soler, C. Cazorla, J. Oliveras, N. G. Bastús, V. F. Puntes and J. Llorca, Nat. Commun., 2023, 14, 6165 CrossRef CAS PubMed.
  47. Z. A. Khalil, A. Nath, K. Hannouche, N. Assaad, G. Mouchaham, A. Beauvois, V. Briois, C. Serre, M. Hmadeh, M. Daturi and M. El-Roz, Nat. Commun., 2026, 17, 308 CrossRef PubMed.
  48. D. Tan, T. F. Ding, K. d. Shen, C. Xu, S. Jin, D. Q. Hu, S. Sun and M. Z. Zhu, Chem. Sci., 2025, 16, 9326–9336 RSC.
  49. X. F. Zhou, J. M. Li, X. Cai, Q. Z. Gao, S. S. Zhang, S. Y. Yang, H. Q. Wang, X. H. Zhong and Y. P. Fang, J. Mater. Chem. A, 2020, 8, 17120–17127 RSC.
  50. Q. S. Nan, J. Ning, B. Han, H. T. Wei, X. F. Wang, Y.-Y. Gu, S. X. Zhou, G. Q. Cao, G. Z. Zhang, X. H. Li, Y. G. Jia and L. Hao, Chem. Sci., 2026, 17, 466–474 RSC.
  51. S. K. Xue, H. Tang, M. Shen, X. C. Liang, X. Y. Li, W. D. Xing, C. Yang and Z. Y. Yu, Adv. Mater., 2024, 36(16), 2311937 CrossRef CAS PubMed.
  52. D. Sebastian, A. Pallikkara, H. Bhatt, H. N. Ghosh and K. Ramakrishnan, J. Phys. Chem. C, 2022, 126(27), 11182–11192 CrossRef CAS.
  53. F. Chen, T. Y. Ma, T. R. Zhang, Y. H. Zhang and H. W. Huang, Adv. Mater., 2021, 33(10), 2005256 CrossRef CAS PubMed.
  54. C. Cheng, J. Zhang, B. Zhu, G. Liang, L. Zhang and J. Yu, Angew. Chem., Int. Ed., 2023, 62(8), e202218688 CrossRef CAS PubMed.
  55. P. E. Blöchl, Phys. Rev. B: Condens. Matter Mater. Phys., 1994, 50(24), 17953 CrossRef PubMed.
  56. C. Ning, Y. Yu, Z. H. Yang, Y. H. Wang and W. D. Shi, Chem. Phys. Lett., 2024, 856, 141637 CrossRef CAS.

Footnote

Y. Huang and C. Ning contributed equally to this work.

This journal is © The Royal Society of Chemistry 2026
Click here to see how this site uses Cookies. View our privacy policy here.