Wanlin
Cai
a,
Cheng
Zhong
b,
Zi-Wei
Ma
a,
Zhuan-Yun
Cai
a,
Yue
Qiu
c,
Zubia
Sajid
a and
De-Yin
Wu
*a
aState Key Laboratory of Physical Chemistry of Solid Surface, Collaborative Innovation Center of Chemistry for Energy Materials, and Department of Chemistry, College of Chemistry and Chemical Engineering, Xiamen University, Xiamen, 361005, P. R. China. E-mail: dywu@xmu.edu.cn
bHubei Key Lab on Organic and Polymeric Optoelectronic Materials, Department of Chemistry, Wuhan University, Wuhan, Hubei 430072, P. R. China
cGrimwade Centre for Cultural Materials Conservation, School of Historical and Philosophical Studies, Faculty of Arts, University of Melbourne, Parkville, VIC 3052, Australia
First published on 30th November 2023
With favorable colour purity, multi-resonance thermally activated delayed fluorescence (MR-TADF) molecules exhibit enormous potential in high-definition displays. Due to the relatively small chemical space of MR-TADF molecules, it is challenging to improve molecular performance through domain-specific expertise alone. To address this problem, we focused on optimizing the classic molecule, DABNA-1, using machine learning (ML). Molecular morphing operations were initially employed to generate the adjacent chemical space of DABNA-1. Subsequently, a machine learning model was trained with a limited database and used to predict the properties throughout the generated chemical space. It was confirmed that the top 100 molecules suggested by machine learning present excellent electronic structures, characterized by small reorganization energy and singlet–triplet energy gaps. Our results indicate that the improvement in electronic structures can be elucidated through the view of the molecular orbital (MO). The results also reveal that the top 5 molecules present weaker vibronic peaks of the emission spectrum, demonstrating higher colour purity when compared to DABNA-1. Notably, the M2 molecule presents a high RISC rate, indicating its promising future as a high-efficiency MR-TADF molecule. Our machine-learning-assisted approach facilitates the rapid optimization of classical molecules, addressing a crucial requirement within the organic optoelectronic materials community.
In comparison to the conventional TADF molecules with donor–acceptor structures, the chemical space explored for MR-TADF molecules (the number of known MR-TADF structures) remains limited.3,12 The main design strategy for MR-TADF molecules is to combine heteroatoms with complementary electronegativity, currently with the commonly available combinations of B/N, B/O, and CO/N.1,3 As a result, it will be challenging to further improve the colour purity and the RISC rate through expert experience. As a classic well-performing MR-TADF molecule, B/N-doped compound DABNA-1 (Fig. 1) has experimentally exhibited a narrow full width at half maximum (FWHM) of 190 meV and a remarkable RISC rate of 9.9 × 103 s−1.13
Fig. 1 Schematic overview of machine-learning-assisted performance improvements for MR-TADF molecules. |
Quantum chemical calculations are perceived as a more cost-efficient alternative to experimental methods. However, large-scale computational screening costs remain substantial, particularly regarding the vibronic coupling and ΔEST calculations for MR-TADF molecules. Here, the strength of vibronic coupling can be characterized by the reorganization energy.6,7 The measure of the vibronic coupling strength (the reorganization energy) requires the calculation of excited state forces.6 The evaluation of ΔEST should be conducted by using the wave function-based methods due to the double-excitation character of electronic transitions.4,14 As a promising approach to address the challenge posed by high-cost calculations and limited computational resources, machine learning (ML) has demonstrated tremendous potential as a valuable tool in the fields of medicinal chemistry, materials chemistry, and organic synthesis.10,15–17 Over the past few years, it has received significant attention and exploration.
In this work, a cost-effective approach is presented to improve the performance of MR-TADF molecules using ML, with DABNA-1 as a representative example. The schematic overview is shown in Fig. 1. First, an ML model was trained with a limited database and subsequently used to predict the properties of the entire adjacent chemical space of DABNA-1. Second, a series of structure–property relationship analyses were conducted for the screened excellent molecules from the perspective of the molecular orbital (MO). Finally, the emission spectra and ISC/RISC rates of DABNA-1 and the top 5 MR-TADF molecules were calculated to validate the effectiveness and practicality of our machine-learning-assisted performance improvement approach.
Following the establishment of the adjacent chemical space of DABNA-1, 5000 molecules were randomly selected to construct a database for machine learning. It is commonly believed that molecules with strong structural rigidity usually present a remarkable similarity between their S0 and S1 potential energy surfaces. As a result, the reorganization energy for emission (λem) is nearly equal to the reorganization energy for absorption (λabs) (Fig. 3a).6,20,21 To eliminate the high-cost computational expenses of geometries and vibrational frequencies of the excited state, the reorganization energy under the vertical gradient (VG) approximation at S0 geometry (λVG) as well as the vertical S1–T1 energy gap (ΔEvertST) at S0 geometry (Fig. 3a) were used as descriptors to characterize colour purity and RISC rates, respectively.6 Additionally, the two individual properties (λVG and ΔEvertST) were converted into two single scores ranging from zero to one by using a logistic function (Fig. 3b and d).22 A higher score denotes a better individual property, with a score of above 0.8 indicating exceptional performance. Unfortunately, the calculated score of the two investigated properties of most molecules is below 0.8 (Fig. 3c and e). Here, to reflect the overall excellence of the two parameters of a molecule, the multi-parameter optimization (MPO) score was calculated using the formula , where ai is the score for the individual property and n is the number of individual properties.22 A high MPO score indicates that all the individual properties of the molecule are favorable.
Furthermore, a molecular graph convolutional network (GCN) was trained by using the database with 5000 molecules, incorporating relevant information such as the atomic number and hybridization, to generate a prediction model.23 The coefficient of determination and the mean absolute error were used to evaluate the GCN model, where EML and EQC denote the model-predicted value and actual value in the test data, respectively, and N represents the number of molecules in the test data.
As shown in Fig. 4a and b, the R2 values of λVG and ΔEvertST are calculated to be 0.77 and 0.72, respectively, while the MAEs of λVG and ΔEvertST are 18 meV and 50 meV, respectively. These results indicate that the prediction model can effectively estimate the two molecular properties. Applying this prediction model throughout the adjacent chemical space of DABNA-1, the top 100 molecules with the highest MPO scores were selected to conduct further quantum chemical validation. The data distributions of the initial 5000 molecules and the predicted top 100 molecules are depicted in Fig. 4c. The MPO scores of the predicted top 100 molecules are around 0.8, which demonstrates that our machine-learning-assisted performance improvement approach is very promising.
Fig. 5 (a) Similarity heatmap for the top 100 MR-TADF molecules. (b) The main core structures for the top 100 molecules. |
As shown in Fig. 6b, Core_1 and Core_3 present a noticeable decrease in reorganization energy (λem) compared to Core_0. This decrease mainly comes from the bond stretching modes around 1400–1700 cm−1 (Fig. S4, ESI†). To deeply understand the reorganization energy, λem was further decomposed into internal coordinates.26,27 In the internal coordinate representation, λem can be described as the result of alterations in bond lengths, bond angles, and dihedral angles.27 The reorganization energy resulting from alterations in bond lengths (λBL) significantly contributes to the decreased λem from Core_0 to Core_1 and Core_3 (Fig. 6c). Particularly, this decrease in λBL can be primarily attributed to the alterations in the C6–C13 and C10–C11 bonds (Fig. 6d, g, and m). It is worth noting that the bond length is associated with bond order. The bond order between the μth and νth atoms can be written as , where ni represents the occupation number of the ith MO, Ciμ and Ciν denote the MO coefficients.20,27 Therefore, λBL can be rationalized from the perspective of MO theory, specifically by using λBL ∝ (CLμCLν − CHμCHν)2, where H and L denote the HOMO and LUMO, respectively.20,27 As shown in Fig. 6a, the C6–C13 and C10–C11 bonds show the strong bonding character in the HOMO, while showing the weak bonding character in the LUMO. As molecular conjugation increases from Core_0 to Core_1 and Core_3, there is a noticeable decrease in the HOMO distribution located on the C11 and C13 atoms (Fig. 6e and k). As a result, the C6–C13 and C10–C11 bonds present a decreased bond order difference (associated with bond length alteration) between the S0 and S1 states, thus showing a decrease in λBL.
The ΔEadST values of Core_0, Core_1, Core_2 and Core_3 are calculated to be 198, 124, 214, and 141 meV, respectively. Given that the spatial overlap between the HOMO and LUMO determines the energy gap between the S1 and T1 states.28 The squares of the overlap integral of the HOMO and the LUMO (OverlapHL2) for Core_0, Core_1, Core_2 and Core_3 are calculated to be 13.40 × 10−4, 7.11 × 10−4, 9.03 × 10−4, and 7.07 × 10−4, respectively. The reduced HOMO distributions on the N1, N9, C11, C13, C17, and C18 atoms, as well as the reduced LUMO distributions on the C17 and C18 atoms (Fig. 6e, f, k, and l), are the main contributors to the decrease in ΔEadST from Core_0 to Core_1 and Core_3.
It should be noted that it is not easy to simultaneously weaken vibronic coupling and decrease ΔEST for the conventional TADF molecules. This is because decreasing ΔEST in conventional TADF molecules is achieved by enhancing the long-distance spatial separation of the HOMO and LUMO. However, this long-range electron density reorganization is accompanied by the strong vibronic coupling (the large reorganization energy).2,3
Fig. 7 (a) Chemical structures of the top 5 MR-TADF molecules. (b) Calculated λem and ΔEadST. (c) Calculated fluorescence emission spectra. |
To visually verify the superior performance of MR-TADF molecules suggested by our machine-learning-assisted approach, the fluorescence emission spectra and ISC/RISC processes from T1 to S1 were studied. With the smaller λem, the top 5 MR-TADF molecules show the weaker vibronic peak (the narrower FWHM) compared to DABNA-1 (Fig. 7c and Table 1), especially for the bottom of the low energy region in emission spectra. As a result, the top 5 MR-TADF molecules show high colour purity. Meantime, based on the smaller ΔEadST, the 5 MR-TADF molecules present an increased ratio of RISC rate kRISC(T1 → S1) to ISC rate kISC(S1 → T1) compared to DABNA-1 (Table 1), which is beneficial to enhance the exciton utilization. In particular, M2 demonstrates a promising future as a high-efficiency MR-TADF molecule. Owing to its ΔEadST of 50 meV, the calculated kRISC(T1 → S1) value of M2 can reach 8.97 × 105 s−1, indicating great potential to avoid efficiency roll-off. It should be noted that the top 5 molecules are demonstrated with high radiative rates (Table 1), although our primary focus during the ML process was not specifically on achieving high radiative rates.
DABNA-1 | M1 | M2 | M3 | M4 | M5 | |
---|---|---|---|---|---|---|
FWHM (meV) | 196 | 161 | 148 | 130 | 134 | 102 |
k ISC(S1 → T1) (s−1) | 3.52 × 105 | 5.39 × 104 | 3.83 × 106 | 9.34 × 103 | 1.71 × 105 | 2.56 × 104 |
k RISC(T1 → S1) (s−1) | 6.64 × 102 | 3.65 × 103 | 8.97 × 105 | 3.25 × 103 | 1.76 × 103 | 3.30 × 102 |
k r(S1 → S0) (s−1) | 6.72 × 107 | 1.53 × 108 | 1.57 × 108 | 1.77 × 108 | 1.07 × 108 | 4.37 × 108 |
Our structure–property analysis revealed that the top 100 MR-TADF molecules are mainly based on three core structures, and it is possible to elucidate the reorganization energy and S1–T1 energy gaps through the view of MO theory. The reduced HOMO distribution located on the C11 and C13 atoms serves as a critical determinant for the decrease in λem and ΔEadST from Core_0 to Core_1 and Core_3. Moreover, this reduced HOMO distribution is associated with the decrease in λem and ΔEadST from Core_1 to M1, M2, and M3, as well as from Core_2 to M4. On the other hand, the top 5 MR-TADF molecules show a weaker vibronic peak in the emission spectrum compared to DABNA-1. Notably, M2 with a calculated kRISC(T1 → S1) of 8.97 × 105 s−1 offers an effective solution to efficiency roll-off, thus signifying its potential as a high-efficiency MR-TADF molecule. By integrating molecular structure modification, ML, and insights from MO, we can improve the performance of MR-TADF molecules and gain a deeper understanding of the underlying improvement process.
In the era of artificial intelligence, machine learning plays an important role in discovering novel materials. Numerous efforts have been made to improve the model performance and develop low-cost and effective first-principles descriptors. However, to advance the performance of specific materials, it is crucial to generate the chemical space with high-efficiency molecules through specific morphing operations. It is worth mentioning that an efficient structure–property relationship analysis can guide the development of specific morphing operations.
To perform detailed photophysical property analyses, the S1 and T1 states of DABNA-1, the four cores, and the top 5 MR-TADF molecules were respectively optimized by using the time-dependent density functional theory (TDDFT) and unrestricted DFT in the Gaussian 16 program. The S1 and T1 excitation energies were evaluated at the SCS-CC2/cc-pVTZ level in the MRCC program.38,39 The spin–orbit coupling (SOC) matrix elements between the S1 and T1 states were calculated at the PBE0-D3BJ/def2-SVP level by using the PySOC program.40 The OverlapHL2 was obtained from the Multiwfn program.41
(1) |
The radiative decay rate (kr(S1 → S0)) can be obtained from the Einstein spontaneous emission equation44
(2) |
The ISC/RISC rate can be calculated as follows:45,46
(3) |
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d3cp04441f |
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