Jinying Zhao†
a,
Qihang Yang†b,
Weibin Chena,
Nuo Xua,
Qing Zhangc,
Wenhao Zhaob,
Geng-Geng Luo
a,
Qiuhong Cui
*b and
Jianhua Huang
*a
aCollege of Materials Science and Engineering, Huaqiao University, Xiamen 361021, China. E-mail: huangjianhua@hqu.edu.cn
bDepartment of Materials Science and Engineering, School of Physical Sciences and Engineering, Beijing Jiaotong University, Beijing 100044, China. E-mail: qhcui@bjtu.edu.cn
cDepartment of Materials Chemistry, Huzhou University, Huzhou 313000, China
First published on 29th September 2025
Polycyclic aromatic hydrocarbons (PAHs) containing O–B ← N groups in the backbone have demonstrated excellent optical properties but two-dimensionally (2D) extended O–B ← N perturbed PAHs have been rarely reported due to synthetic challenges. Moreover, the applications of these O–B ← N perturbed PAHs have been primarily limited to electroluminescent devices, highlighting the urgent need to explore novel functions of this class of heteroaromatic molecules. This work develops a straightforward synthesis strategy toward O–B ← N perturbed PAHs through 2–3 steps, creating a series of tetra-cycle, octa-cycle, and deca-cycle fused molecules. Photophysical characterization and theoretical simulations of these O–B ← N perturbed PAHs reveal several distinct properties, e.g., high fluorescence quantum yields (70%), aggregation induced emission (AIE) effects, and anti-Kasha emission. Then, through classic solvent diffusion or volatilization methods, these O–B ← N perturbed PAHs further self-assemble into 1D microstructures, e.g., rod or sheet shaped microwires in solutions. These microwires were, for the first time, subjected to optical waveguide measurements, revealing low optical loss coefficients ranging from 10−2 to 10−3 dB μm−1. This work develops an efficient synthesis strategy for 2D extended O–B ← N perturbed PAHs and demonstrates their pioneering applications in optical waveguides, demonstrating the great potential of these O–B ← N perturbed PAHs for micro/nanophotonics.
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Fig. 1 Chemical structures of acenes (a), 2D acenes (b), Py, TT, and PP (c) and O–B ← N perturbed Py, TT, and PP (d). |
These boron-doped polycyclic heteroaromatic molecules have been applied in various organic electronic devices, for example, OLEDs, OPVs, organic field effect transistors (OFETs), and photodetectors through solution-processing or vacuum evaporation techniques.34,35,52–54 Due to backbone rigidity and tailorable weak intermolecular interactions, these polycyclic heteroaromatic molecules can be conveniently assembled into micro- or nano-scaled crystals in appropriate solvents.55 In comparison to organic films with amorphous or semi-crystalline morphology, organic crystals, especially single crystals, exhibit fewer unfavorable grain boundaries and lower defect density, which are beneficial to the transport of charge carriers and photons.56,57 While numerous studies have been focused on the charge transport performance of molecular crystals based on boron-doped polycyclic heteroaromatic molecules,36,58 their photon transport performance, namely, optical waveguide behavior, has not been evaluated. This is particularly true for molecular crystals prepared using boron-doped PAHs, especially O–B ← N perturbed PAHs, although excellent light emission properties have been demonstrated for these molecules.
Herein, we develop a straightforward strategy to synthesize O–B ← N perturbed 2D acenes, i.e., pyrene (Py), tetracenotetracene (TT), and pentacenopentacene (PP). Pyrene is a classic 2D acene whereas TT and PP were reported in 2019 by Frigoli et al. (Fig. 1c).59 This work reveals a simple and efficient approach toward the synthesis of O–B ← N perturbed Py, TT, and PP for the first time, obtaining a series of tetra-, octa-, and deca-cycle fused heteroaromatic molecules (Fig. 1d). Unique photophysical properties e.g., high photoluminescence quantum yields, aggregation induced emission (AIE), and the anti-Kasha emission phenomenon have been found for these O–B ← N perturbed 2D acenes. Furthermore, 1D microcrystals with rod, sheet, and spindle shapes were prepared using these O–B ← N perturbed 2D acenes in solutions. The optical waveguide properties of the microcrystals were evaluated and low loss coefficients (R) of 10−3 dB μm−1 were observed, indicating that these O–B ← N perturbed PAHs are promising for micro/nanophotonic devices.
Single crystals of OBN8-C8 and OBN10-Ph were successfully obtained and X-ray crystallographic tests were performed (Tables S1 and S2). Interestingly, OBN8-C8 exhibits anti-configuration, whereas the cis-isomer is separated for OBN10-Ph (Fig. 2). Stereochemistry in single crystals is consistent with the relative electronic energies (Fig. S11). For the octa-cycle fused OBN8-C8, the backbone is a 2D extended nanobelt with a length of 13.23 Å and a width of 5.03 Å (Fig. 2a). All the backbone atoms stay in the same plane except for the two borons, which slightly depart from the skeleton by 0.57 Å due to the sp3-hybridization of the tetracoordinated boron (Fig. 2b). OBN10-Ph displays an increased length of 18.22 Å and slightly twisted skeleton, with dihedral angles of A–B, A–C, and C–D in the range of 12–15° (Fig. 2c and d). Considering the tetrahedral geometry of boron, the anti-configuration would lead to a co-planar backbone, whereas cis-substitution on boron would give rise to a twisted backbone. Usually, a twisted backbone can be energetically more favorable than co-planar ones. The steric hindrance of bulky 2-ethylhexyl would trigger anti-substitution and an unfavorable co-planar backbone in OBN8-C8 whereas phenyl-substituted OBN10-Ph would favor a cis-configuration due to the relatively smaller volume of tetra-butylbenzene. The B ← N bond lengths are ca. 1.60 Å for OBN8-C8 (Fig. S2) and OBN10-Ph (Fig. S5), similar to the values revealed in the literature.37,44 OBN8-C8 shows slipped face-to-face stacking with a C–C interaction distance of 3.36 Å (Fig. S3). The backbone of OBN8-C8 adopts typical herringbone packing style in the single crystal (Fig. S4). OBN10-Ph exhibits alternate stacking of front and back sides and abundant C–H and C–C interactions can be observed in single crystals (Fig. S6). In general, compact π–π stacking modes are absent in these O–B ← N perturbed 2D PAHs due to the steric hindrance of the side groups, which would partially avoid fluorescence (FL) quenching in solid states.
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Fig. 2 Single crystal structures of OBN8-C8 (a and b) and OBN10-Ph (c and d) determined by X-ray crystallography. The substituents of OBN10-Ph are omitted for clarity in (d). |
To get insight into the electronic structure and aromaticity, density functional theory (DFT) was adopted to simulate these O–B ← N perturbed PAHs. The electrostatic potential (ESP) maps of the O–B ← N perturbed PAHs and their precursors of BP, BP–P, and BP–N were calculated. As shown in Fig. 3a and S12, the hydroxyl (OH) and pyridine surfaces of the three precursors show strongly negative potential (red color) due to the electron-rich nature of oxygen and nitrogen. After incorporating tetracoordinated boron, the oxygen surface retains a negative potential whereas the potential on the surfaces and edges of pyridine becomes distinctly positive (green to blue), which can be attributed to strong electron donation from nitrogen to the unoccupied orbital of boron. However, for BP–Ph and BP–N, the potential on the bilaterally linked phenyl and naphthalene is not obviously changed after introducing boron into the backbone. These results suggest that the tetracoordinated boron only reduces the surface potential of the pyridine unit but has little effect on the other units of these O–B ← N perturbed PAHs, which is different from the previous B ← N embedded molecules,61 where the introduction of boron was found to remarkably change the potential of the whole skeleton from electron-rich to electron-deficient. This can be attributed to the strong electron-donating nature of oxygen, which greatly weakens the electron-accepting ability of boron. The ESP area distribution reveals an extremely positive potential of 25–30 kcal mol−1 for the O–B ← N perturbed PAHs (Fig. S13),62 corresponding to the electron-deficient edge of pyridine induced by the tetracoordinated boron.
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Fig. 3 ESP maps of OBN4-Ph, OBN8-F, OBN10-Ph, and three precursors (a) and NICS(1)zz plots (b), 2D-ICSS plots (c), and AICD plots (d) of OBN4-Ph, OBN8-F, and OBN10-Ph. |
Aromaticity of these O–B ← N perturbed PAHs was evaluated by nuclear independent chemical shifts (NICS), two dimensional iso-chemical shielding surface (2D-ICSS) maps, and anisotropy of the induced current density (AICD) analysis.63,64 As shown in Fig. 3b and S14, the two pyridine cycles exhibit apparent aromaticity with minus NICS(1)zz and the NICS(1)zz values of O–B ← N embedded cycles are in the range of +5 to +8 ppm, suggesting anti-aromaticity. As the conjugation is extended, the NICS(1)zz values gradually decrease from the inner phenyl (ca. −22 ppm) to the marginal phenyl (ca. −24 ppm), demonstrating enhanced aromaticity. Interestingly, the phenyl substituted on the boron exhibits the strongest aromaticity with NICS(1)zz values ranging from −26 to −28 ppm, elucidating that the aromaticity of the linked phenyl is negligibly impacted by the boron. These results illustrate that embedding O–B ← N into the backbone would readily destroy the aromaticity but the aromaticity of side phenyl linked to boron is not suppressed. The 2D-ICSS plots solidly support the NICS results with strong aromaticity for the pyridine and other phenyls (blue) but anti-aromaticity for the O–B ← N embedded cycles (red) (Fig. 3c). The AICD plots of OBN4-Ph show clockwise ring current for the pyridine and the phenyls linked on the boron, supporting the aromaticity (Fig. 3d). For OBN8-F and OBN10-Ph, a clockwise ring current appears on the pyridine and other phenyls but a counterclockwise ring current can be observed over the O–B ← N embedded cycles, consistent with the NICS and 2D-ICSS results.
Photophysical properties of the five O–B ← N perturbed PAHs and the three precursors were evaluated by recording the UV-Vis absorption and FL spectra in diluted chloroform. As shown in Fig. 4a, in contrast to the precursors, the O–B ← N perturbed PHAs show red-shifted absorption due to the introduction of electron-deficient boron. For octa-cycle fused PAHs (OBN8-F, OBN8-C8, and OBN8-Ph) and deca-cycle fused PAHs (OBN10-Ph), two strong absorption bands appear in the range of 250–380 nm, verifying that multiple transitions are allowed in the ultraviolet region, which may be ascribed to the π–π* or n–π* transitions. The lower energy absorption bands at 400–500 nm can be attributed to the intramolecular charge transfer (ICT) transitions. The fluorine substituted OBN8-F exhibits slightly blue-shifted ICT peaks in comparison to those of alkyl- and phenyl-substituted OBN8-C8 and OBN8-Ph, which can be explained by the additional ICT effects from the electron-rich alkyl and phenyl groups donating to the electron-deficient boron.50 From OBN4-Ph to OBN8-Ph, the bathochromic absorption can be related to the extended conjugation. However, from octa-cycle fused OBN8-Ph to deca-cycle fused OBN10-Ph, the ICT absorption is mildly blue-shifted, which can be related to the twisted backbone of OBN10-Ph, as clarified in the single crystal data. The optical bandgaps calculated from the films absorption (Fig. S25) are 2.78 eV for OBN4-Ph and ca. 2.40 eV for OBN8-C8, OBN8-Ph, and OBN10-Ph (Table 1).
Absorption | Emission | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
λsm (nm)a | λfm (nm)b | λfedge (nm)c | Eoptg (eV)d | λex (nm)e | λFLm (nm)f | Φ (%)g | Δν (nm)h | τ (ns)i | knr (108 s−1)j | |
a Absorption maximum in solutions.b Absorption maximum in films.c Absorption edges in films.d Optical bandgaps calculated by 1240/λfedge.e Excitation wavelength.f Emission peaks in solutions.g Absolute fluorescence quantum yields measured using an integrating sphere.h Stokes shifts calculated by λFLm − λsm.i FL life-times.j Non-radiative decay rates calculated by (1 − Φ)/τ. | ||||||||||
BP | 343 | 354 | 420 | 2.95 | 345 | 488 | 37.69 | 145 | 3.44 | 1.81 |
OBN4-Ph | 394/410 | 401/423 | 446 | 2.78 | 390 | 465 | 16.58 | 71 | 2.42 | 3.45 |
BP–Ph | 367 | 373 | 433 | 2.86 | 373 | 538 | 46.06 | 171 | 2.71 | 1.99 |
OBN8-F | 447/472 | — | — | — | 469 | 498 | 71.67 | 51 | 5.91 | 0.48 |
OBN8-C8 | 456/482 | 464/494 | 521 | 2.38 | 469 | 502 | 71.38 | 46 | 5.72 | 0.50 |
OBN8-Ph | 456/483 | 463/492 | 520 | 2.38 | 469 | 510 | 29.94 | 54 | 2.95 | 2.37 |
BP–N | 370 | 373 | 435 | 2.85 | 369 | 545 | 39.92 | 175 | 2.00 | 3.00 |
OBN10-Ph | 447/474 | 455/484 | 519 | 2.39 | 469 | 531 | 3.38 | 84 | 0.69 | 14.00 |
As shown in the FL spectra (Fig. 4b), the emission peaks exhibit significant hypsochromic shifts from the precursors to the O–B ← N perturbed PAHs. Therefore, sharply different Stokes shifts (Δν) between the precursors and the corresponding O–B ← N perturbed PAHs can be deduced. As summarized in Table 1 and plotted in Fig. S26, the Δν values suddenly decrease from 140–170 nm for precursors to 50–80 nm for O–B ← N perturbed PAHs. In contrast to the precursors of BP, BP–Ph, and BP–N with rotatable bonds, the reduced Stokes shifts of O–B ← N perturbed PAHs can be interpreted by the rigid backbones locked by the boron.
Fluorescence quantum yields (Φ) in solutions were measured using an integrating sphere. Interestingly, the variation of Φ values from precursors to O–B ← N perturbed PAHs is closely related to the backbones and substituents (Fig. S27). From BP–Ph to fluorine-substituted OBN8-F and alkyl-substituted OBN8-C8, the Φ values remarkably increased from 46.0% to 71.7% and 71.4% due to the increased backbone rigidity, leading to decreased non-radiative decay. Otherwise, when the substituents on the boron are phenyl, the O–B ← N perturbed PAHs display decreased Φ values in comparison to their precursors. For example, from BP to OBN4-Ph, BP–Ph to OBN8-Ph, and BP–N to OBN10-Ph, the Φ values decreased from 37.7% to 16.5%, 46% to 30.0%, and 39.9% to 3.4%, respectively. The FL life times (τ) were measured (Fig. S28) and the rates of non-radiative decay (knr) were calculated by (1 − Φ)/τ. From the precursors to the phenyl substituted backbones, the knr values apparently increase (Fig. S29). Therefore, the decreased Φ values in solutions upon anchoring phenyl to the backbone are attributable to the freely rotatable phenyl,65 resulting in enhanced non-radiative decay.
We also measured the FL spectra and Φ values of these O–B ← N perturbed PAHs dispersed in PMMA films (1% w/w) (Fig. S30) as well as in their crystal forms (Fig. S31 and Table S11). Interestingly, the Φ values significantly increase from solutions to PMMA blends for OBN4-Ph (16.5% vs. 45.5%) and slightly for OBN10-Ph (3.4% vs. 4.2%), which can be explained by the inhibited rotation of phenyls in PMMA films, giving rise to promoted radiative decay. Moreover, the Φ values in crystals are also greater than those in solutions for OBN4-Ph (45.0% vs. 16.5%) and OBN10-Ph (8.3% vs. 3.4%). These results demonstrate that OBN4-Ph and OBN10-Ph presumably have aggregation induced emission (AIE) effects. This drives us to further confirm the AIE properties of OBN4-Ph and OBN10-Ph by monitoring the FL intensity in THF/H2O mix solvents with different water fractions (fwater). As shown in Fig. S32a and 4c, the emission intensity of OBN4-Ph gradually decreases when the fwater increases from 0% to 60% but suddenly increases by 3 fold when fwater increases to 70%. For OBN10-Ph, the emission intensity monotonically increases from fwater = 0% to 80%, exhibiting typical AIE effects (Fig. S32b and 4d). Photographs of the solutions under ultraviolet light radiation (365 nm) also support the AIE properties of OBN4-Ph and OBN10-Ph (inset in Fig. 4c and d).
Time-dependent density functional theory (TD-DFT) calculations were performed to predict the transitions from the ground state to the excited states (Fig. S15 and Tables S3–S10). In general, the predicted transitions and oscillator strengths (f) agree well with the experimentally measured spectra except for some deviations observed in the higher energy transitions. We analyzed frontier orbital transitions from S0 to S1, S2, S3, S4, and S5 and schematically illustrated these processes, as shown in Fig. S16–S23. Interestingly, all the molecules exhibit allowed S0 → S1 transitions with high f values of ca. 0.05–0.60 except for OBN10-Ph, whose f value of S0 → S1 is 0.0 (Fig. S23), suggesting a forbidden transition from the ground to the first excited state. This result hints that the radiative process of OBN10-Ph from S1 to S0 also may be forbidden, following the so-called anti-Kasha emission feature.66 To further verify our guess, the excited states of OBN10-Ph were simulated. As expected, the f value of S1 → S0 (λ = 754 nm) is extremely low (0.003) whereas S3 → S0 (λ = 553 nm) and S5 → S0 (λ = 510 nm) show high f values of 0.547 and 0.251 (Fig. 4e), respectively. More importantly, the radiative rate of kr1 (1.44 × 106 s−1) is significantly smaller than those of kr3 (8.70 × 107 s−1) and kr5 (1.40 × 108 s−1) by at least one order of magnitude. These theoretical calculations preliminarily prove the anti-Kasha radiation of OBN10-Ph. To further confirm this inference, the excitation-wavelength-dependent emission spectra of OBN10-Ph in chloroform solution were measured, which is a powerful experiment to affirm the anti-Kasha emission.66 As the excitation wavelength varies from 330 to 450 nm, remarkable changes of emission spectra are observed (Fig. S33a) and the excitation-wavelength-independent peaks at 533 and 523 nm can be ascribed to transitions of S3 → S0 and S5 → S0, solidly supporting the anti-Kasha emission. For comparison, OBN8-Ph was also subjected to the same measurements (Fig. S33b), showing emission spectra independent of the excitation wavelength, consistent with regular radiation following the classic Kasha rule. High internal conversion rates (kic) of up to 1011 s−1 were calculated between S3/S5 and S1 for OBN10-Ph (Fig. S24), much faster than the FL radiation rates (ca. 109 s−1). This is different from the traditional anti-Kasha mechanism, which requires a large energy gap and small kic between S1 and adjacent excited states.67,68 Temperature-dependent FL spectra of OBN10-Ph show enhanced intensity from 80 K to 130 K (Fig. S34), evidently supporting the thermal activation processes from S1 to higher electronic states.15,26 Further elevating the temperature to 280 K gives rise to decreased FL intensity, which could be ascribed to the enhanced non-radiative decay at high temperatures. For comparison, OBN8-Ph was also subjected to temperature-resolved spectra tests and monotonically decreased intensity was observed as the temperature increased from 80 K to 300 K (Fig. S35), excluding thermal activation processes. These results evidently show that the anti-Kasha emission of OBN10-Ph can be attributed to the prohibited emission from S1, the fast internal conversion rates from S3/S5 to S1, and thermal repopulation processes from S1 to higher electronic states, e.g., S3 and S5, all of which lead to the strong emission from S3 and S5.
The phosphorescence spectra of the five O–B ← N perturbed PAHs in PMMA films (1.0 wt%) were recorded under 77 K with lifetimes (τp) in the range of 1–33 ms (Fig. S36 and S37). Cyclic voltammetry (CV) curves of these O–B ← N perturbed PAHs were measured in chloroform solutions. Electrochemical properties of OBN8-F could not be measured due to its poor solubility in solvents. As shown in Fig. S38, OBN4-Ph and OBN8-C8 exhibit reversible reduction peaks whereas OBN8-Ph displays quasi-reversible oxidation peaks. OBN10-Ph gives irreversible redox peaks due to its limited solubility. As the conjugation extends from OBN4-Ph to OBN8-Ph and OBN10-Ph, the reduction potentials (−1.26 vs. −0.78 vs. −0.60 V) gradually increase, indicating enhanced electron affinity.
Considering the excellent photoluminescence (PL) properties and extended skeleton conjugation, we selected OBN8-C8, OBN8-Ph, and OBN10-Ph to prepare microstructures using solvent diffusion or volatilization methods (Fig. S39–S41). Interestingly, well-defined microcrystals can be obtained with spindle, rod, and sheet shapes, respectively, for OBN8-C8, OBN8-Ph, and OBN10-Ph (Fig. S42–S44).
For OBN8-Ph and OBN10-Ph, upon ultraviolet excitation, the two end points of 1D microcrystals exhibit bright luminescence spots whereas the bodies are almost non-luminescent (Fig. 5a and e). It's obvious that the 1D microcrystals of OBN8-Ph and OBN10-Ph are capable of absorbing the excitation light and propagating the light wave to the end points, which is the typical feature of optical waveguides. Atomic force microscopy (AFM) images reveal a thickness of ca. 1.2 μm for OBN8-Ph microcrystals, confirming the rod shape (Fig. 5b). OBN10-Ph microcrystals show a small thickness of ca. 0.5 μm, supporting the sheet shape (Fig. 5f). Transmission electron microscopy (TEM) and selected area electron diffraction (SAED) were adopted to further examine the micromorphology and crystalline properties of the microwires. Consistent with the AFM images, the TEM images of both OBN8-Ph and OBN10-Ph microwires present smooth surfaces, which are beneficial for light wave propagation (Fig. 5c and g). The bright and uniformly distributed diffraction dots observed in the SAED patterns of OBN8-Ph and OBN10-Ph microwires demonstrate single crystalline nature throughout the whole microstructure (Fig. 5d and h). According to the single crystal XRD data, the microwires of OBN10-Ph were grown along the (202) direction. The well-defined 1D microstructures and excellent crystalline properties of these microwires are advantageous to transport exciton polaritons (EPs),69 a kind of mixed light-matter quasi-particles formed by the coupling of excitons and photons, which is a critical characteristic for optical waveguides.
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Fig. 5 FL microscopy images (a and e), AFM images (b and f), TEM images (c and g), and SAED patterns (d and h) of OBN8-Ph and OBN10-Ph microcrystals. |
The optical waveguide performance of the OBN8-Ph and OBN10-Ph microwires was evaluated by locally exciting the microwires at different positions and recording the spatially resolved PL spectra as a function of propagation distance. As shown in Fig. 6a and d, the brightness at the left tips (points 1 to 6) of both OBN8-Ph and OBN10-Ph microwires gradually decreases as the excitation positions spatially depart from the left ends. On the other hand, the emission intensities at the right tips gradually increase as the excitation points shift from left to right. Distance-dependent PL spectra were collected from points 1 to 6 by increasing the propagation distance of the source light (Fig. 6b and e). Typical light waveguide behavior is observed for OBN8-Ph and OBN10-Ph microwires with decreased intensities of PL spectra as the excitation points move from left to right. The decay of PL intensity with respect to the propagation distances (D) can be quantitatively determined by the ratio of PL intensity at the emitting ends (Itip) to the excitation intensity (Ibody). By plotting Itip/Ibody versus D and single-exponentially fitting the plots using Itip/Ibody = Aexp(−RD), the optical loss coefficient (R) can be deduced. As shown in Fig. 6c and f, low R values of 1.39 × 10−2 and 7.06 × 10−3 dB μm−1 are estimated for OBN8-Ph and OBN10-Ph microwires, respectively, which are comparable or better than those of the 1D microcrystals prepared from luminescent organic conjugated molecules based on perylene diimide, perylene, fluorene, etc. (Table S12).70–75 In general, the impressive optical waveguide performance of OBN8-Ph and OBN10-Ph can be related to their excellent PL properties and 2D extended conjugation, enabling spontaneous self-assembly into long range ordered 1D microwires. In contrast to OBN8-Ph, the lower optical loss of OBN10-Ph can be readily ascribed to the extended conjugation and distinct AIE properties. These results suggest that O–B ← N perturbed PAHs are promising candidates to prepare microstructures with excellent optical waveguide performance, which are crucial components for micro/nanophotonic devices.
The data supporting this article have been included as part of the supplementary information (SI). Supplementary information: including materials, experimental methods, molecular synthesis, X-ray crystallography, stability measurements, detailed theoretical simulations, preparation and optical waveguide tests of microcrystals, NMR, and HRMS spectra is available. See DOI: https://doi.org/10.1039/d5sc05407a.
Footnote |
† These authors contributed equally to this work. |
This journal is © The Royal Society of Chemistry 2025 |