Improving the TADF properties of deep-blue multiple-resonance emitters by strategic oxygen–sulfur replacement

Junki Ochi a, Yuki Yamasaki b, Susumu Oda c, Masakazu Kondo d, Yasuhiro Kondo e, Masahiro Hayakawa a and Takuji Hatakeyama *a
aDepartment of Chemistry, Graduate School of Science, Kyoto University, Sakyo-ku, Kyoto 606-8502, Japan. E-mail: hatake@kuchem.kyoto-u.ac.jp
bDepartment of Chemistry, Graduate School of Science and Technology, Kwansei Gakuin University, 2-1 Gakuen, Sanda, Hyogo 669-1337, Japan
cDepartment of Applied Chemistry, Graduate School of Science and Engineering, Toyo University, 2100 Kujirai, Kawagoe, Saitama 350-8585, Japan
dJNC Co., Ltd., 5-1 Goikaigan, Ichihara, Chiba 290-8551, Japan
eSK JNC Japan Co., Ltd., 5-1 Goikaigan, Ichihara, Chiba 290-8551, Japan

Received 16th July 2025 , Accepted 23rd September 2025

First published on 8th October 2025


Abstract

An oxygen–sulfur replacement for improving thermally activated delayed fluorescence (TADF) materials based on a multiple-resonance (MR) effect is reported. A comprehensive computational analysis of four possible isomers revealed that the precise placement of the sulfur atom is crucial to suppress undesired spectral red-shifts. Among them, a promising deep-blue emitter, DOB2-DABNA-C-NP-S-1, exhibits emission at 458 nm with a narrow full width at half maximum (FWHM) of 20 nm. Moreover, its reverse intersystem crossing rate constant (kRISC) of 2.9 × 106 s−1 is three times larger than that of the oxygen-based analog (9.0 × 105 s−1). An OLED device incorporating DOB2-DABNA-C-NP-S-1 as an emitter achieves ultrapure deep-blue electroluminescence at 461 nm with Commission Internationale de l’Éclairage (CIE) coordinates of (0.133, 0.077), satisfying the blue emitter standards set by the National Television System Committee (NTSC). The device demonstrates outstanding external quantum efficiencies (EQEs) of 24.3% (at maximum), 23.9% (at 1000 cd m−2), and 18.7% (at 10[thin space (1/6-em)]000 cd m−2), with the latter ranking the highest among the previously reported OLED devices employing deep-blue MR-TADF emitters.



New concepts

Introducing heavy atoms into the MR-TADF framework is one of the most common approaches to improve TADF performance. However, replacing oxygen with sulfur often causes a red-shift in photoluminescence, especially in deep-blue emitters, thereby compromising the color purity of the original oxygen-containing compounds. To address this issue, we demonstrate that regulating the LUMO energy level is key to maintaining deep-blue even after sulfur incorporation. A comprehensive analysis of four sulfur-containing isomers revealed that the careful selection of the oxygen–sulfur substitution site can effectively suppress the undesired spectral red-shift. Based on these insights, we synthesized DOB2-DABNA-C-NP-S-1 as a sulfur-incorporated MR-TADF emitter. The OLED device employing this compound exhibited deep-blue electroluminescence (461 nm) with suppressed efficiency roll-off (external quantum efficiency (EQE) = 24.3%/23.9%/18.7% at maximum/1000/10[thin space (1/6-em)]000 cd m−2) and a device lifetime (LT50) of 39 h at 500 cd m−2. Notably, an EQE of 18.7% at 10[thin space (1/6-em)]000 cd m−2 ranks among the highest reported for the deep-blue OLED using MR-TADF materials. These results demonstrate a general molecular design strategy for achieving deep-blue emission in heavy-atom incorporating MR-TADF materials, which has remained largely unexplored to date.

Introduction

Thermally activated delayed fluorescence (TADF) materials1,2 have garnered significant attention in the field of organic light-emitting diodes (OLEDs)3 due to their capability to utilize all excitons generated by electric field excitation. To enable highly efficient and color-pure TADF emission for advanced OLED technology, our group introduced a novel design principle in 2016, namely the multiple resonance (MR) effect.4 This approach provides a powerful solution for simultaneously achieving both high photoluminescence quantum yield (PLQY) and narrow full width at half maximum (FWHM). These attractive features originate from the unique electronic structure created by alternating electron-donating and electron-accepting atoms attached to a single benzene ring. This specific arrangement induces contrasting resonant features, effectively localizing the highest occupied molecular orbital (HOMO) and lowest unoccupied molecular orbital (LUMO) onto distinct carbon atoms. Consequently, MR-TADF emitters exhibit highly desirable narrow-band emission, enabling the realization of superior color purity in OLEDs without the need for energy-consuming color filtering.5,6

To improve the device performance of OLEDs fabricated with MR-TADF emitters, their reverse intersystem crossing (RISC) rate constant (kRISC) is a significant parameter because accumulated triplet excitons can lead to quenching processes such as triplet–triplet annihilation (TTA) and triplet–polaron annihilation (TPA). One of the most common strategies to enhance kRISC is introducing heavy atoms into the MR framework.7–9 For example, Shao, Wang, and coworkers first performed a direct comparison of oxygen- and sulfur-attached MR-TADF emitters and revealed the enhanced spin–orbit coupling (SOC) matrix element and accelerated RISC (Fig. 1a).10 Similarly, Park, Yasuda, and coworkers reported deep-blue MR-TADF emitters embedding sulfur atoms, whose kRISC was up to 12 times higher than that of the oxygen-bridged analog (Fig. 1b).11 Although the heavy-atom effect of sulfur (ZN = 16) is considered to be not so significant, these results clearly prove the validity of oxygen–sulfur replacement. Stimulated by these pioneering works, many research studies have been conducted from both synthetic12–25 and computational26–28 approaches, attempting to improve the TADF properties of MR-emitters. However, the incorporation of sulfur atoms often causes a red-shift in photoluminescence, especially in deep-blue emitters, thereby compromising the color purity of the original O-containing compounds (Table S7). For precise and strategic design of high-performance MR-TADF emitters, deeper understanding of the effect of oxygen–sulfur replacement is necessary.


image file: d5mh01353d-f1.tif
Fig. 1 (a) and (b) Previous examples of oxygen–sulfur replacement.10,11 (c) Molecular structure of four O3S-type isomers and their predicted excitation wavelength of the S0–S1 transition calculated at the B3LYP/6-31G(d) level of theory.

With these circumstances in mind, herein, we focus on the improvement of DOB2-DABNA-C-NP, a π-extended MR-TADF material reported by our group (Fig. 1c).29 This compound, which contains four oxygen atoms, exhibits deep-blue fluorescence (456–458 nm) and a fast kRISC (0.8–1.1 × 106 s−1), leading to a remarkable OLED performance with an external quantum efficiency (EQE) of 20.8% at 1000 cd m−2. After a comprehensive computational analysis of all four candidates generated by oxygen–sulfur replacement of DOB2-DABNA-C-NP, we expect DOB2-DABNA-C-NP-S-1 to be a promising candidate for an improved deep-blue MR-TADF emitter. Motivated by this prediction, DOB2-DABNA-C-NP-S-1 was synthesized, and its photophysical properties were investigated, revealing an improved kRISC (2.9 × 106 s−1) while maintaining pure blue emission (458 nm). The OLED device fabricated with DOB2-DABNA-C-NP-S-1 exhibited Commission Internationale d’Éclairage (CIE) coordinates of (0.133, 0.077), which satisfy the blue gamut standard defined by the National Television System Committee (NTSC). Importantly, the efficiency roll-off is highly suppressed (EQEmax = 24.3%/EQE1000 = 23.9%) because of the improved kRISC value, indicating the validity of precisely selecting the sulfur incorporation position.

Results and discussion

Molecular design

Fig. 2 shows the molecular orbitals of DOB2-DABNA-C-NP and its sulfur-incorporated analogs. Because the transition from HOMO−1 to LUMO is a main component of the S0–S1 excitation in all cases (Table S2), these two molecular orbitals are discussed here. First, regarding the HOMO−1 energy level, only small differences were observed among all compounds. This can be attributed to a faint contribution of oxygen and sulfur atoms to HOMO−1. On the other hand, the LUMO energy is largely perturbed by the oxygen–sulfur replacement. Moreover, the extent of this perturbation strongly depends on the sulfur position. In DOB2-DABNA-C-NP-S-1 and DOB2-DABNA-C-NP-S-4, their LUMO energy was slightly stabilized from DOB2-DABNA-C-NP (0.021 eV). Much larger stabilization was observed in DOB2-DABNA-C-NP-S-2 (0.061 eV) and DOB2-DABNA-C-NP-S-3 (0.149 eV), which caused a red-shift characteristic of these two isomers (Fig. 1c). Such a sulfur-position dependency can be rationalized by considering the anti-bonding character of two C–S bonds. While only one carbon atom adjacent to a sulfur atom shows a significant contribution to the LUMO in DOB2-DABNA-C-NP-S-1 and DOB2-DABNA-C-NP-S-4, clear nodes can be observed in both C–S bonds in DOB2-DABNA-C-NP-S-2 and DOB2-DABNA-C-NP-S-3, suggesting their contribution to the LUMO as an anti-bonding component. In these two isomers, therefore, the replacement by sulfur strongly shifts the LUMO energy through the perturbation of an anti-bonding character. In other words, the position where sulfur is incorporated in DOB2-DABNA-C-NP-S-1 and DOB2-DABNA-C-NP-S-4 does not largely participate in the LUMO, resulting in a small effect of the oxygen–sulfur replacement. These considerations are further supported by the population analysis, which proved that the contribution of a sulfur atom to the LUMO is larger in DOB2-DABNA-C-NP-S-2 (2.6%) and DOB2-DABNA-C-NP-S-3 (3.6%), thereby stabilizing their LUMO levels. Based on these results, we determined DOB2-DABNA-C-NP-S-1 to be a target molecule to achieve deep-blue emission and an improved OLED device performance.
image file: d5mh01353d-f2.tif
Fig. 2 HOMO−1 and LUMO of DOB2-DABNA-C-NP and its sulfur-incorporated analogs. Yellow arrows show the position of the incorporated sulfur atom.

Synthesis

The synthetic scheme of DOB2-DABNA-C-NP-S-1 is summarized in Fig. 3. The procedure is exactly the same as that for DOB2-DABNA-C-NP.29 Starting from the previously reported compound 1, the sulfur-containing unit 2, which was synthesized in four steps from the commercially available materials, was introduced via Buchwald–Hartwig amination to afford 3 in 41% yield. After that, DOB2-DABNA-C-NP-S-1 was synthesized by one-shot borylation30–32 in 55% yield. Along with DOB2-DABNA-C-NP, the introduction of steric methyl groups in an appropriate position allowed a moderate yield of the final borylation reaction.
image file: d5mh01353d-f3.tif
Fig. 3 Synthesis of DOB2-DABNA-C-NP-S-1.

Photophysical properties

Next, the photophysical properties of DOB2-DABNA-C-NP-S-1 and DOB2-DABNA-C-NP were investigated under various conditions. To assess the impact of oxygen–sulfur replacement, toluene, poly(methyl methacrylate) (PMMA), and polystyrene (PS) were selected as matrices to mitigate specific intermolecular interactions with the surrounding molecules (Table S6). Fig. 4 summarizes the representative photophysical properties measured in a 1 wt% emitter-doped PS film. As expected by the DFT calculation, DOB2-DABNA-C-NP-S-1 exhibited a fluorescence maximum of 458 nm, which is only 2 nm red-shifted from DOB2-DABNA-C-NP (456 nm). The FWHM and the energy difference between the S1 and T1 states (ΔEST) were 20 nm (117 meV) and 18 meV, respectively. These values are also comparable to those of DOB2-DABNA-C-NP, confirming little loss of its attractive deep-blue character. Nevertheless, the rate constant of reverse intersystem crossing (kRISC) of DOB2-DABNA-C-NP-S-1 (2.9 × 106 s−1) was 3.2 times larger than that of DOB2-DABNA-C-NP (9.0 × 105 s−1). Thus, the oxygen–sulfur replacement effectively enhanced the TADF properties. Measurements in toluene and PMMA exhibited consistency with those in PS (Fig. S4 and S5). In addition, DOB2-DABNA-C-NP-S-1 showed accelerated kRISC and larger ΔEST compared to DOB2-DABNA-C-NP under all conditions. Given that the increased ΔEST is disadvantageous to the RISC process, the spin–orbit coupling (SOC) matrix should be enhanced by the oxygen–sulfur replacement. Although our computational SOC values largely depended on the conformation of the diphenylamine group, the higher kRISC in DOB2-DABNA-C-NP-S-1 could be reproduced by the semi-classical Marcus equation (Fig. S1 and Table S3).33 Although intramolecular π–π interaction was observed by noncovalent interaction (NCI) analysis (Fig. S3),34 the inclusion of Grimme's dispersion correlation parameters had a negligible effect on predicting the excited state properties (Tables S4 and S5). It should be noted that effects such as the Herzberg–Teller vibronic coupling should be included for a more accurate SOC calculation.35 These results prove that a careful choice of the replacement position successfully suppresses the red-shift in fluorescence and contributes to realizing improved deep-blue emission.
image file: d5mh01353d-f4.tif
Fig. 4 Photophysical properties of (a) and (b) DOB2-DABNA-C-NP-S-1 and (c) and (d) DOB2-DABNA-C-NP in PS 1 wt%-doped film. (a) and (c) Fluorescence spectra at 300 K (blue) and 77 K with (green) and without (red) a delay time of 25 ms. (b) and (d) Transient photoluminescence decay curve at 300 K and the relevant parameters. The red curve represents the single exponential fitting data (background = 3–4), and the gray curve represents an IRF curve.

Electroluminescence properties

To evaluate the impact of the oxygen–sulfur replacement on OLED performance, a device using DOB2-DABNA-C-NP-S-1 as an emitter was fabricated with the following structure: indium tin oxide (ITO, 50 nm); N,N′-di(1-naphthyl)-N,N′-diphenyl-(1,1′-biphenyl)-4,4′-diamine (NPD, 40 nm); tris(4-carbazolyl-9-ylphenyl)amine (TCTA, 15 nm); 1,3-bis(N-carbazolyl)benzene (mCP, 15 nm); 1 wt% DOB2-DABNA-C-NP-S-1 emitter and 99 wt% DOBNA-Tol36 (20 nm); 3,4-di(9H-carbazol-9-yl)benzonitrile (3,4-2CzBN,37 10[thin space (1/6-em)]nm); 2,7-bis(2,2′-bipyridine-5-yl)triphenylene (BPy-TP2,38 20 nm); LiF (1 nm); and Al (100 nm) (Fig. 5a). The DOB2-DABNA-C-NP-S-1-fabricated device exhibited an ultrapure and narrow deep-blue emission (λEL = 461 nm, FWHM = 22 nm) (Fig. 5b). Its CIE coordinates were (0.133, 0.077), which are extremely close to the blue gamut standard defined by NTSC (CIE(x, y) = (0.14, 0.08)) (Fig. 5c). This device had a turn-on voltage of 3.4 V, showing typical semiconducting properties (Fig. 5d). While maintaining the desirable properties originally observed in the DOB2-DABNA-C-NP-fabricated device, the device performances, including EQE, current efficiency, power efficiency, and device lifetime, were improved by sulfur incorporation. The EQEs of the DOB2-DABNA-C-NP-S-1-based device reached 24.3/24.0/23.9% at the maximum, 100, and 1000 cd m−2, respectively (Fig. 5e). These values were improved from the 21.7/21.4/20.8% observed in the DOB2-DABNA-C-NP-based device. Notably, the efficiency roll-off at 1000 cd m−2 was only 1.6%, an outstanding value compared to previous MR-emitter-based deep-blue OLED devices without a sensitizer (Table S8). The current and power efficiencies of the DOB2-DABNA-C-NP-S-1-based device at the maximum, 100, and 1000 cd m−2 were 17.3/16.9/16.9 cd A−1 and 16.9/12.1/9.8 lm W−1, respectively (Fig. S13). These values also surpass those of the DOB2-DABNA-C-NP-based one (14.3/14.1/13.7 cd A−1 and 13.5/9.8/7.5 lm W−1). The half-lifetime (LT50) with an initial luminance of 500 cd m−2 was 39 h, which is 3.3 times longer than that of the previously reported DOB2-DABNA-C-NP device (Fig. S11). Notably, EQE10000 (18.7%) ranks the highest among the previously reported OLED devices employing deep-blue MR-TADF emitters (Fig. 5f and Table S9). Overall, the fast kRISC of DOB2-DABNA-C-NP-S-1, benefiting from the oxygen–sulfur replacement, contributed to improved OLED performances while maintaining pure deep-blue electroluminescence.
image file: d5mh01353d-f5.tif
Fig. 5 OLED characteristics for the devices using DOB2-DABNA-C-NP-S-1. (a) Device structures with the estimated energy levels in eV for each component. (b) Normalized EL spectra. Inset: Electroluminescence of the device. (c) Commission Internationale de l’Éclairage (CIE) (x,y) coordinates. (d) Current density–voltage (JV) characteristics (blue) and luminance–voltage (LV) characteristics (green). (e) EQE–luminance (EQE–L) characteristics. (f) Comparison of EQE values at 10[thin space (1/6-em)]000 cd m−2 with reported blue OLEDs.

Conclusions

In this study, we present a molecular design strategy for enhancing the performance of MR-TADF emitters through targeted oxygen–sulfur replacement. Rather than simple replacement, we systematically evaluated four regioisomeric sulfur analogues to determine how the substitution position influences the emission properties. Our analysis revealed that maintaining high excitation energy requires precise control over the LUMO level, which in turn depends critically on the sulfur atom's location. Among the candidates, DOB2-DABNA-C-NP-S-1 emerged as a standout compound, exhibiting deep-blue photoluminescence at 458 nm with a narrow FWHM of 20 nm. These values are comparable to those of its oxygen-based counterpart, DOB2-DABNA-C-NP, thereby maintaining its desirable deep-blue character. Notably, the sulfur incorporation led to a threefold increase in the kRISC compared to the oxygen-based emitter. The resulting OLED device delivered ultrapure deep-blue electroluminescence at 461 nm with CIE coordinates of (0.133, 0.077) and demonstrated excellent EQEs of 24.3%, 23.9%, and 18.7% at the maximum, 1000, and 10[thin space (1/6-em)]000 cd m−2, respectively. Notably, the EQE10[thin space (1/6-em)]000 value surpasses that of all the previous OLED devices employing deep-blue MR-TADF emitters. These findings emphasize the importance of site-selective oxygen–sulfur replacement and offer valuable guidelines for the development of next-generation blue-emitting MR-TADF materials containing heavy atoms.

Conflicts of interest

There are no conflicts to declare.

Data availability

The data supporting this article have been included as part of the supplementary information (SI). Supplementary information is available. See DOI: https://doi.org/10.1039/d5mh01353d.

Acknowledgements

T. H. acknowledges Japan Science and Technology Agency (JST) CREST (grant no. JPMJCR22B3), the Japan Society for the Promotion of Science (JSPS) Fund for the Core-to-Core Program Number (grant no. JPJSCCA20220004), the Promotion of Joint International Research (ILR) (grant no. 23K20039), and Grants-in-Aid for Scientific Research (grant no. 24K01569). J. O. acknowledges the JSPS Fund for the Grant-in-Aid for Research Activity Start-up (grant no. 23K19245).

Notes and references

  1. H. Uoyama, K. Goushi, K. Shizu, H. Nomura and C. Adachi, Nature, 2012, 492, 234 CrossRef CAS PubMed.
  2. J. M. Dos Santos, D. Hall, B. Basumatary, M. Bryden, D. Chen, P. Choudhary, T. Comerford, E. Crovini, A. Danos, J. De, S. Diesing, M. Fatahi, M. Griffin, A. K. Gupta, H. Hafeez, L. Hämmerling, E. Hanover, J. Haug, T. Heil, D. Karthik, S. Kumar, O. Lee, H. Li, F. Lucas, C. F. R. Mackenzie, A. Mariko, T. Matulaitis, F. Millward, Y. Olivier, Q. Qi, I. D. W. Samuel, N. Sharma, C. Si, L. Spierling, P. Sudhakar, D. Sun, E. Tankelevičiūtė, M. Duarte Tonet, J. Wang, T. Wang, S. Wu, Y. Xu, L. Zhang and E. Zysman-Colman, Chem. Rev., 2024, 124, 13736 CrossRef CAS PubMed.
  3. C. W. Tang and S. A. VanSlyke, Appl. Phys. Lett., 1987, 51, 913 CrossRef CAS.
  4. T. Hatakeyama, K. Shiren, K. Nakajima, S. Nomura, S. Nakatsuka, K. Kinoshita, J. Ni, Y. Ono and T. Ikuta, Adv. Mater., 2016, 28, 2777 CrossRef CAS PubMed.
  5. M. Mamada, M. Hayakawa, J. Ochi and T. Hatakeyama, Chem. Soc. Rev., 2024, 53, 1624 RSC.
  6. X. Wu, S. Ni, C.-H. Wang, W. Zhu and P.-T. Chou, Chem. Rev., 2025, 125, 6685 CrossRef CAS PubMed.
  7. H. J. Kim and T. Yasuda, Adv. Opt. Mater., 2022, 10, 2201714 CrossRef CAS.
  8. K. R. Naveen, P. Palanisamy, M. Y. Chae and J. H. Kwon, Chem. Commun., 2023, 59, 3685 RSC.
  9. X.-F. Luo, X. Xiao and Y.-X. Zheng, Chem. Commun., 2024, 60, 1089 RSC.
  10. F. Chen, L. Zhao, X. Wang, Q. Yang, W. Li, H. Tian, S. Shao, L. Wang, X. Jing and F. Wang, Sci. China: Chem., 2021, 64, 547 CrossRef CAS.
  11. I. S. Park, M. Yang, H. Shibata, N. Amanokura and T. Yasuda, Adv. Mater., 2022, 34, 2107951 CrossRef CAS PubMed.
  12. T. Hua, L. Zhan, N. Li, Z. Huang, X. Cao, Z. Xiao, S. Gong, C. Zhou, C. Zhong and C. Yang, Chem. Eng. J., 2021, 426, 131169 CrossRef CAS.
  13. Y. X. Hu, J. Miao, T. Hua, Z. Huang, Y. Qi, Y. Zou, Y. Qiu, H. Xia, H. Liu, X. Cao and C. Yang, Nat. Photonics, 2022, 16, 803 CrossRef CAS.
  14. I. S. Park, H. Min and T. Yasuda, Angew. Chem., Int. Ed., 2022, 61, e202205684 CrossRef CAS PubMed.
  15. X.-F. Luo, H.-X. Ni, A.-Q. Lv, X.-K. Yang, H.-L. Ma and Y.-X. Zheng, Adv. Opt. Mater., 2022, 10, 2200504 CrossRef CAS.
  16. H. Gao, S. Shen, Y. Qin, G. Liu, T. Gao, X. Dong, Z. Pang, X. Xie, P. Wang and Y. Wang, J. Phys. Chem. Lett., 2022, 13, 7561 CrossRef CAS PubMed.
  17. H. Gao, Z. Li, Z. Pang, Y. Qin, G. Liu, T. Gao, X. Dong, S. Shen, X. Xie, P. Wang, C.-S. Lee and Y. Wang, ACS Appl. Mater. Interfaces, 2023, 15, 5529 CrossRef CAS PubMed.
  18. X. Xiong, Y.-C. Cheng, K. Wang, J. Yu and X.-H. Zhang, Mater. Chem. Front., 2023, 7, 929 RSC.
  19. M. Wang, Z. Fu, R. Cheng, J. Du, T. Wu, Z. Bin, D. Wu, Y. Yang and J. Lan, Chem. Commun., 2023, 59, 5126 RSC.
  20. Z. Ye, H. Wu, Y. Xu, T. Hua, G. Chen, Z. Chen, X. Yin, M. Huang, K. Xu, X. Song, Z. Huang, X. Lv, J. Miao, X. Cao and C. Yang, Adv. Mater., 2024, 36, 2308314 CrossRef CAS PubMed.
  21. H.-X. Ni, J.-Z. Zhu, J.-J. Hu, L. Yuan, X.-J. Liao, S. Xing and Y.-X. Zheng, Adv. Opt. Mater., 2024, 12, 2401033 CrossRef CAS.
  22. L. Yuan, J.-W. Xu, Z.-P. Yan, Y.-F. Yang, D. Mao, J.-J. Hu, H.-X. Ni, C.-H. Li, J.-L. Zuo and Y.-X. Zheng, Angew. Chem., Int. Ed., 2024, 63, e202407277 CrossRef CAS PubMed.
  23. L. Yuan, Y.-F. Yang, Z.-P. Yan, J.-J. Hu, D. Mao, H.-X. Ni and Y.-X. Zheng, Adv. Funct. Mater., 2024, 34, 2403803 CrossRef CAS.
  24. J. Jin, M. Chen, H. Jiang, B. Zhang, Z. Xie and W.-Y. Wong, ACS Mater. Lett., 2024, 6, 3246 CrossRef CAS.
  25. J. Jin, M. Chen, H. Jiang, B. Zhang, Z. Xie and W.-Y. Wong, Adv. Opt. Mater., 2024, 12, 2400794 CrossRef CAS.
  26. S. M. Pratik, V. Coropceanu and J.-L. Brédas, ACS Mater. Lett., 2022, 4, 440 CrossRef CAS.
  27. S. M. Pratik, E. P. McBride, J.-L. Brédas and V. Coropceanu, Adv. Opt. Mater., 2025, 13, 2403421 CrossRef CAS.
  28. S. Nathiya, M. Panneerselvam and L. T. Costa, Phys. Chem. Chem. Phys., 2025, 27, 7265 RSC.
  29. J. Ochi, Y. Yamasaki, S. Oda, M. Kondo, A. Ikeno, Y. Kondo and T. Hatakeyama, Adv. Opt. Mater., 2025, 13, 2402939 CrossRef CAS.
  30. K. Matsui, S. Oda, K. Yoshiura, K. Nakajima, N. Yasuda and T. Hatakeyama, J. Am. Chem. Soc., 2018, 140, 1195 CrossRef CAS PubMed.
  31. S. Oda, B. Kawakami, Y. Yamasaki, R. Matsumoto, M. Yoshioka, D. Fukushima, S. Nakatsuka and T. Hatakeyama, J. Am. Chem. Soc., 2022, 144, 106 CrossRef CAS PubMed.
  32. Y. Sano, T. Shintani, M. Hayakawa, S. Oda, M. Kondo, T. Matsushita and T. Hatakeyama, J. Am. Chem. Soc., 2023, 145, 11504 CrossRef CAS PubMed.
  33. E. Cho, L. Liu, V. Coropceanu and J.-L. Brédas., J. Chem. Phys., 2020, 153, 144708 CrossRef CAS PubMed.
  34. (a) T. Lu and F. Chen, J. Comput. Chem., 2012, 33, 580 CrossRef CAS PubMed; (b) T. Lu, J. Chem. Phys., 2024, 161, 082503 CrossRef CAS PubMed.
  35. M. Hagai, N. Inai, T. Yasuda, K. J. Fujimoto and T. Yanai, Sci. Adv., 2024, 10, eadk3219 CrossRef CAS PubMed.
  36. S. Oda, W. Kumano, T. Hama, R. Kawasumi, K. Yoshiura and T. Hatakeyama, Angew. Chem., Int. Ed., 2021, 60, 2882 CrossRef CAS PubMed.
  37. Y. Tanaka, T. Takahashi, J. Nishide, Y. Hiraga, H. Nakanotani and C. Adachi, Thin Solid Films, 2016, 619, 120 CrossRef CAS.
  38. K. Togashi, S. Nomura, N. Yokoyama, T. Yasuda and C. Adachi, J. Mater. Chem. C, 2012, 22, 20689 RSC.

This journal is © The Royal Society of Chemistry 2025
Click here to see how this site uses Cookies. View our privacy policy here.