Ye
Tian†
,
Wenlong
Xu†
,
Jian
Zhu†
,
Jiayu
Lu
,
Zhaohang
Chen
,
Fakhari
Alam
,
Honglei
Shen
*,
Xi
Kang
* and
Manzhou
Zhu
Department of Chemistry and Centre for Atomic Engineering of Advanced Materials, Key Laboratory of Structure and Functional Regulation of Hybrid Materials of Ministry of Education, Anhui Province Key Laboratory of Chemistry for Inorganic/Organic Hybrid Functionalized Materials, Anhui University, Hefei, Anhui 230601, P. R. China. E-mail: shenhonglei_chem@163.com; kangxi_chem@ahu.edu.cn
First published on 3rd November 2025
The rational design of emissive copper nanoclusters presents a significant challenge due to their inherent instability and complex coordination chemistry. In this study, we propose a reductant-mediated strategy to precisely regulate the atomic structure and photophysical properties of copper nanoclusters. The strong reductant sodium borohydride (NaBH4) yields a non-emissive Cu14(DMP)6(PPh2py)8 species, while the mild reductant borane tert-butylamine complex leads to the formation of a tetrahedral Cu4(PPh2py)4Cl2 cluster, which exhibits a remarkable crystallization-induced emission enhancement (CIEE). Hirshfeld surface analysis of the Cu4 nanocluster indicates that multiple non-covalent interactions—such as H⋯H, C–H⋯π, and Cl⋯H contacts—stabilize the molecular packing, effectively suppressing non-radiative decay pathways and contributing to the CIEE phenomenon. This work highlights the crucial role of reductants in modulating copper nanocluster structures and offers novel insights into the design of efficient copper-based emitters.
Photoluminescence (PL) is among the most intriguing features of Cu nanoclusters, characterized by their strong emissions, significant Stokes shifts, and long excited-state lifetimes.12,25–32 These properties make them promising candidates for optoelectronic and luminescent devices. To enhance the PL performance of Cu nanoclusters, strategies such as ligand modification,33–35 heteroatom doping,36–38 aggregation-induced emission (AIE),39–44 and environmental tuning (e.g., solvent,15,45,46 pH,47 and temperature48) have been explored. Crystallization-induced emission enhancement (CIEE), a specialized form of AIE, has proven particularly effective for improving Cu nanocluster emission.27,49–52 In the crystalline state, ordered molecular packing strengthens intermolecular interactions while restricting intramolecular vibrations/rotations, thereby suppressing non-radiative decay and enhancing radiative recombination.49–52 Despite this progress, a fundamental question remains unresolved: how can copper cluster formation be precisely directed during nucleation and growth to yield atomically defined structures with tailored luminescence properties? In this regard, the choice of reducing agents—a critical yet underexplored synthetic parameter—may serve as a powerful tool for guiding the structural evolution and emission characteristics of Cu nanoclusters.
Herein, we demonstrate that the reducing agent (sodium borohydride, NaBH4, vs. borane tert-butylamine complex, TBAB) profoundly influences the formation and PL behavior of Cu nanoclusters. Specifically, NaBH4 yields non-emissive Cu14(DMP)6(PPh2py)8 (Cu14), while TBAB generates tetrahedral Cu4(PPh2py)4Cl2 (Cu4), which exhibits bright emission in both solution and solid states with pronounced CIEE (Scheme 1). Notably, embedding Cu4 into a poly(methyl methacrylate) (PMMA) matrix via sol–gel processing enhances PL intensity and increases the PL quantum yield (PLQY) nearly 20-fold compared to the solution state. This improvement arises from the reduced non-radiative decay, mediated by intermolecular non-covalent interactions (H⋯H, C–H⋯π, and Cl⋯H interactions). This work highlights the pivotal role of reducing agents in directing Cu nanocluster structures, offering new insights for designing high-performance luminescent copper nanomaterials.
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| Scheme 1 Illustration of the reductant-selected formation of copper nanoclusters and their different PL behavior in the crystal state. | ||
The atomic structures of the Cu4 and Cu14 nanoclusters were determined by SC-XRD. The Cu4 nanocluster crystallizes in a monoclinic crystal system (space group: P21/c), with two pairs of enantiomers present in each unit cell (Fig. S1 and Table S1). As illustrated in Fig. 1a, the nanocluster features a tetrahedral Cu4 core that is stabilized by four phosphine (PPh2py) ligands and two chloride (Cl) ligands. Each Cu atom in the core exhibits a mixed coordination environment involving N (from the ring of PPh2py), P, and Cl ligands, collectively rigidifying the core–shell framework (Fig. 1a). In contrast, the Cu14 nanocluster crystallizes in a triclinic crystal system (space group: P
), with one cluster per unit cell (Fig. S2, Table S2). The cubic Cu14 core is protected by six DMP ligands and eight PPh2py ligands (Fig. 1b), with a simpler coordination sphere dominated by S (from DMP) and P sites. The absence of nitrogen or halogen coordination in Cu14 likely reduces structural rigidity compared to Cu4. Besides, Cu4 exhibits longer Cu–Cu bond lengths and shorter Cu–P bond lengths compared to Cu14 (Table S3), which directly influence its photophysical properties. The shorter Cu–P bonds enhance orbital overlap between copper atoms and phosphine ligands, facilitating ligand-to-metal charge transfer (LMCT). The longer Cu–Cu bonds weaken vibrational coupling between copper atoms, reducing non-radiative transitions. Additionally, the Cu–N and Cu–Cl interactions in Cu4 enhance molecular rigidity and intermolecular interactions, contributing to its stability and superior optical performance.
Electrospray ionization mass spectrometry (ESI-MS) confirmed the molecular compositions. For Cu4, the dominant peak at m/z = 1377.9 corresponds to [Cu4(PPh2py)4Cl2]+, while the minor peak at m/z = 1114.9 matches [Cu4(PPh2py)3Cl2]+ (Fig. 1c). Experimental isotope patterns align precisely with simulated patterns, validating the crystal structure. Similarly, ESI-MS analysis of Cu14 verified its composition and purity (Fig. 1d).
X-ray photoelectron spectroscopy (XPS) analysis confirmed the presence of expected elements in Cu4 and Cu14 nanoclusters (Fig. S3 and S4). High-resolution Cu 2p spectra reveal mixed Cu+/Cu0 species in Cu14, with peaks at 932.5 eV and 952.4 eV. In contrast, Cu4 exhibits higher binding energies in Cu 2p spectra (Fig. S5), indicative of elevated Cu oxidation states. Cu LMM Auger electron spectroscopy further confirms that Cu4 contains more oxidized Cu species than Cu14 (Fig. S6). These differences correlate with reductant strength: the milder reducing environment of TBAB promotes partial oxidation in Cu4, while NaBH4 drives Cu14 toward reduced states. By combining the ESI-MS and XPS results, the Cu4 nanocluster should be in a “+2”-charge state while Cu14 is an electrically neutral molecule. However, both clusters presented “+1”-charged signals in the mass spectra, suggesting a potential electron-gaining or electron-losing behavior of the two clusters in the mass spectrometry environment.
Optical properties were investigated via UV-vis and PL spectroscopy. The UV-vis spectrum of Cu4 shows a shoulder peak at 265 nm and two prominent bands at 315 and 390 nm. In contrast, Cu14 displays a dominant absorption peak at 265 nm, accompanied by a weaker shoulder at 350 nm (Fig. 2a). The main absorption peak of Cu4 at 390 nm represents a significant 40 nm redshift compared to Cu14, reflecting structural differences in core–shell geometry and electronic configurations of the two nanoclusters.
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| Fig. 2 (a) UV-vis spectra and (b) PL spectra of Cu4 (red) and Cu14 (blue) nanoclusters in CH2Cl2 solution (λex = 365 nm). All samples were measured at the same optical density of 0.05. | ||
PL measurements reveal stark contrasts of the two nanoclusters in the solution state: Cu14 is non-emissive in solution, while Cu4 exhibits strong emission with the emissive peak centered at 573 nm (Fig. 2b). In the crystalline state, Cu14 remains virtually non-emissive, while Cu4 shows a significant increase in PL intensity (Fig. S7). In this context, the crystalline state of Cu4 nanocluster demonstrates markedly enhanced PL emission, with emission intensity greatly surpassing that observed in solution, demonstrating its CIEE behavior.
To evaluate the PL behavior of Cu4 in monodisperse (solution), amorphous (film), and crystalline states, we fabricated a Cu4-based composite film using PMMA as the polymer matrix. Under 365 nm UV excitation, all samples emitted visible emission with distinct color shifts dependent on their physical state (Fig. 3a). The corresponding CIE chromaticity coordinates confirmed a progressive color shift from yellow to green, with coordinates of (0.46, 0.51) for the solution, (0.42, 0.52) for the film, and (0.37, 0.53) for crystalline Cu4 (Fig. 3b). Besides, steady-state fluorescence tests of Cu4 crystals demonstrated that such a nanocluster was singly emissive (Fig. S8). Quantitative photophysical measurements revealed that the solution-state Cu4 exhibited weak emission, with a PLQY of only 1.2%. However, when embedded in the PMMA matrix, the PLQY increased substantially to 21.2%. This enhancement is attributed to the restriction of intramolecular motion through AIE, even in the amorphous state (Fig. 3c). Notably, the crystalline form exhibited the highest PLQY of 35.4%, indicative of a strong CIEE effect. Additionally, a PL emission intensity test was conducted to compare the stability of the Cu4 cluster in both crystal and film states. The results demonstrate that both forms retain their PL properties after exposure to the atmosphere for three months (Fig. S9).
To elucidate the emission mechanism behind the Cu4 nanocluster, we calculated the radiative (kr) and non-radiative (knr) rate constants based on the measured PLQY and lifetime data (Table S4). Time-resolved fluorescence measurements revealed progressively increased lifetimes: 0.1 μs (solution), 1.8462 μs (film), and 2.6133 μs (crystal) (Fig. 3d). Notably, the knr values for both the Cu4-based film and crystalline samples decreased by approximately one order of magnitude compared to the solution state. This dramatic reduction confirms that Cu4 aggregation effectively suppresses non-radiative decay pathways, significantly enhancing the PL efficiency of the cluster materials.
In the Cu4 crystal lattice, most PPh2py phenyl rings engage in intercluster interactions: H⋯H (2.173–2.736 Å), C–H⋯π (2.883–3.146 Å), and Cl⋯H (2.705 Å) interactions (Fig. S10). To probe the molecular origins of the CIEE in Cu4, we conducted Hirshfeld surface analysis and 2D fingerprint mapping to investigate the intermolecular interactions that influence the crystal packing. The dnorm surface reveals close short-range contacts, particularly C–H⋯π (red dots) and Cl⋯H interactions (red circle) (Fig. 4a and Fig. S11). The shape index map displays complementary red/blue triangular features, indicative of C–H⋯π stacking interactions (Fig. 4b), while the curvedness map shows extended flat regions that further support the presence of these C–H⋯π contacts (Fig. 4c). Fingerprint analysis quantifies all intermolecular interactions (Fig. 4d), with C⋯H/H⋯C interactions dominating, emphasizing the crucial role of C–H⋯π interactions in stabilizing the crystal lattice (Fig. 4e). Additionally, Cl⋯H/H⋯Cl contacts suggest that chlorine–hydrogen interactions also serve as an auxiliary stabilizing factor (Fig. 4f). This dense network of non-covalent interactions rigidifies the structure, restricting intramolecular ligand rotation/vibration. By elevating the energy barrier for vibrational relaxation, these constraints suppress non-radiative decay pathways, thereby enhancing PL quantum efficiency and driving the pronounced CIEE behavior in Cu4. Furthermore, Hirshfeld surface analysis of Cu14 reveals that its surface is mostly governed by weak intermolecular interactions, such as H⋯H and C–H⋯π interactions (Fig. S12). Compared to the Cu4 cluster, interactions like Cl⋯H bonds were not present in the Cu14 surface, suggesting its significantly weaker intermolecular interactions and non-CIEE behavior.
CCDC 2468154 contains the supplementary crystallographic data for this paper.54
Footnote |
| † These authors contributed equally to this work. |
| This journal is © The Royal Society of Chemistry 2025 |