Xiao Liu†
a,
Xue-liang Wen†b,
Yang Zhoua,
Chao Tanga,
Diandong Tangc,
Qian Wanga,
Yibo Shia,
Lin Liu
a,
Wei Suna,
Kai Fenga,
Wei-Hai Fang
*a,
Juan Qiao
*b,
Lin Shen
*a and
Xuebo Chen
*ad
aKey Laboratory of Theoretical and Computational Photochemistry of the Chinese Ministry of Education, College of Chemistry, Beijing Normal University, Beijing 100875, P. R. China. E-mail: fangwh@bnu.edu.cn; lshen@bnu.edu.cn; xuebochen@bnu.edu.cn
bKey Lab of Organic Optoelectronics and Molecular Engineering of Ministry of Education, Department of Chemistry, Tsinghua University, Beijing, 100084, P. R. China. E-mail: qjuan@mail.tsinghua.edu.cn
cDepartment of Chemistry, University of Washington, Seattle, Washington 98195, USA
dCollege of Chemistry and Molecular Sciences, Henan University, Zhengzhou 450046, P. R. China. E-mail: xuebochen@bnu.edu.cn
First published on 29th August 2025
As a class of functional materials used in organic light-emitting diodes (OLEDs), sensitizers play a crucial role in the improvement of device efficiency, color purity, and stability. In recent years, thermally activated delayed fluorescence (TADF) sensitizers have attracted much attention mainly because of their high exciton utilization efficiency by converting quenched triplet excitons into singlet excitons. Despite the experimental success of sensitization strategies in enhancing OLED performance, the lack of theoretical models for sensitizers continues to hinder further development. In the present work, we design three novel sensitizers and investigate their photophysical mechanisms in the presence of a host and/or an emitter. Based on highly accurate electronic structure calculations and non-radiative transition rates, we propose the first theoretical model to describe the dynamic behavior of sensitizers in OLEDs. This model highlights key factors for achieving ultraefficient sensitization, such as multi-channel energy transfer capabilities, large intermolecular electronic couplings, and reduced redundant energy transfer pathways in devices as well as conformational rigidity under excitation and small singlet–triplet energy splitting for ideal sensitizers. In particular, a binary system consisting of a new sensitizer as the host material and an emitter achieves excellent performance with a high external quantum efficiency of 29.2% and negligible efficiency roll-off of 5.5% at a brightness of 1000 cd m−2 for red phosphorescent OLEDs. These findings provide fundamental chemical insights into exciton dynamics and practical guidelines for material-device co-optimization in next-generation electroluminescent technologies.
In devices, energy transfer (EnT), a process via which exciton energy is transferred from a donor (e.g., a host material or sensitizer) to an acceptor (e.g., an emitter), is a key factor in the luminescence efficiency, spectral stability and efficiency roll-off. Förster resonance EnT (FRET) relies on dipole–dipole interactions between the donor and acceptor at nanometer distances, while triplet–triplet EnT (TTET, also named Dexter EnT) involves electron exchange via molecular orbital overlap between the donor and acceptor at a much shorter distance.26,27 Different energy transfer mechanisms have been proposed recently. For example, Lee et al. observed that phosphorescent sensitizers with higher dipole orientation exhibited a faster rate for direct energy transfer from the triplet to singlet states, resulting in a 2.2-fold increase in the triplet consumption rate of phosphorescent sensitizers.28 Bronstein and co-workers developed an ultra-narrowband blue emitter encapsulated by bulky alkyl chains, demonstrating that the encapsulation material can suppress the TTET channel from the sensitizer to the terminal emitter. This effect is beneficial to form fluorescent emitters via the FRET channel, thereby enhancing device efficiency.29 Based on the multiple sensitization processes relevant to FRET, Duan and co-workers designed a device using a newly developed indolocarbazole/triazine derivative as the host and achieved a maximum external quantum efficiency (EQEmax) of 23.2% and a power efficiency (PE) of 76.9 lm per W.8
Despite the experimental success of sensitization strategies in enhancing OLED performance, the lack of theoretical models for sensitizers continues to hinder further development. However, for a typical host–guest system in the presence of an additional sensitizer, the competition between FRET and TTET, the coupling between EnT and TADF, and the relationship between transition rates and molecular structures are still unclear, mainly limited by the accuracy of computational tools. Our group has developed a computational protocol by combining the complete active space self-consistent field method and its second-order perturbation theory (CASSCF//CASPT2) with the non-radiative transition rate models based on Fermi's golden rule.30–34 In the past decade, it has been successfully used to establish a quantitative relationship between intermolecular distances and EnT rates in white OLEDs and to explore the underlying mechanisms of several photocatalytic reactions.35–37
In this study, we extend the protocol to build the first theoretical model at the ab initio computational level for sensitizers in binary and ternary systems. Guided by a precision molecular orbital engineering strategy, we innovatively introduced carbonyl and sulfur atoms into donor–acceptor (D–A)-type TADF sensitizers. Specifically, the heavy atom effect of sulfur significantly enhances the SOC strength. By employing planar rigid frameworks—xanthone (XT) and thioxanthone (TX) as electron acceptors and precisely modulating the spatial separation between the triphenylamine (TPA) donor and acceptors through a carbazole (Cz) bridging unit, we effectively suppress exciton quenching induced by π–π stacking. Simultaneously, the strong electron-donating capability and three-dimensional stereoscopic configuration of TPA optimize carrier injection efficiency while regulating excited-state energy levels (Fig. 1a). Through atomic-scale tuning of donor–acceptor distances, three novel sensitizers were successfully designed and synthesized: 3-(2-(4-(diphenylamino)phenyl)-9H-carbazol-9-yl)-9H-xanthen-9-one (2O), 3-(1-(4-(diphenylamino)phenyl)-9H-carbazol-9-yl)-9H-xanthen-9-one (1O), and 3-(1-(4-(diphenylamino)phenyl)-9H-carbazol-9-yl)-9H-thioxanthen-9-one (1S). Subsequently, in device architecture construction, we implemented a theory-experiment co-design strategy by integrating tris(4-carbazoyl-9-ylphenyl) amine (TCTA) as the host and bis[2-(1-isoquinolinyl-κN)-4,6-dimethylphenyl-κC](2,4-pentanedionato-κO2,κO4)iridium (Ir(mpiq)2acac, denoted as the Ir(III) complex hereafter) as the terminal emitter and the synthesized sensitizers. Through computational simulations of the excited-state electronic structures and associated energy transfer dynamics, we elucidated the energy transfer mechanisms between sensitizers and host–guest materials, thereby systematically establishing key design principles for high-efficiency OLED sensitizers.
Based on the above electronic structure calculations, the intermolecular energy transfer rates can be estimated using the method within the general formalism of non-radiative transition models, which was first developed by Lin et al.30–34 and has been successfully applied to explore the mechanisms of white OLEDs and photocatalytic reactions by our group.35–37,47,48 Starting from the Born–Oppenheimer approximation and Fermi's golden rule, the energy transfer rate constant is given by
![]() | (1) |
The nuclear part in eqn (1), which is the so-called Franck–Condon (FC) term, can be calculated based on the multidimensional harmonic oscillator model as
![]() | (2) |
![]() | (3) |
For the TTET process, the electronic part in eqn (1) can be represented as the square of electronic coupling between two electronic states of the donor–acceptor complex, that is,
![]() | (4) |
For the FRET process, the electronic part in eqn (1) is often approximated as classical dipole–dipole interactions between the donor and acceptor.49,50 However, it is unrealistic in OLED devices developed in this work. For an emission layer doped at a concentration of 5 wt%, there is always a guest molecule in close proximity to a host molecule at a distance of less than 1 nm, possibly generating a donor–acceptor complex. Therefore, we calculate the electronic part under TTET and FRET on the same footing. In the latter case, eqn (4) can be rewritten as
![]() | (5) |
The notations in eqn (5) are the same as those in eqn (4). Unlike the nuclear part that requires electronic structure calculations on the isolated donor and isolated acceptor in different electronic states, the ground-state calculation of the donor–acceptor complex is necessary to deal with eqn (4) and (5).
Film | Structure | λem (nm) | ΦPL/Φda (%) | τp (ns) | τd (μs) | ΔEST (eV) | kr,Sb (106 s−1) | knr,Sb (106 s−1) | kISCb (106 s−1) | kRISCb (105 s−1) |
---|---|---|---|---|---|---|---|---|---|---|
a Total/delayed PLQY values.b Calculated with the assumption of knr,T = 0 and kr,T = 0. | ||||||||||
Neat | 2O | 511 | 9.7/- | 63.6 | — | 0.37 | 1.53 | 14.2 | — | — |
1O | 520 | 39.3/17.9 | 162.8 | 14.23 | 0.11 | 1.31 | 2.03 | 2.74 | 1.29 | |
1S | 531 | 20.4/15.7 | 76.8 | 3.56 | 0.09 | 0.61 | 2.38 | 9.09 | 12.1 | |
Doped | 2O | 498 | 23.6/- | 82.7 | — | — | 2.85 | 9.24 | — | — |
1O | 500 | 72.4/29.3 | 135.6 | 17.12 | — | 3.18 | 1.21 | 2.94 | 0.98 | |
1S | 528 | 63.5/52.8 | 63.6 | 7.07 | — | 1.69 | 0.97 | 12.4 | 8.36 |
Further measurements of the fluorescence and phosphorescence spectra of their neat thin films at 77 K were conducted (Fig. 2d–f). By analyzing the fluorescence and phosphorescence in the neat films, the values of ΔEST were estimated to be 0.37, 0.11, and 0.09 eV for 2O, 1O, and 1S, respectively. The relatively small ΔEST values of 1O and 1S suggest their potential for TADF characteristics. In contrast, the larger ΔEST of 2O may hinder the occurrence of the TADF process. The same tendency was observed in doped thin films (30 wt% in TCTA). To confirm their TADF properties, we measured transient photoluminescence decay curves of 1O and 1S in neat and doped thin films at 298 K. As shown in Fig. 2e, f, S4c and d, typical TADF behavior appears with both prompt (τp) and delayed (τd) lifetime components. The values of τp for 1O and 1S in neat/doped thin films are 162.8/135.6 and 76.8/63.6 ns, respectively, and the corresponding τd values are 14.23/17.12 μs for 1O and 3.56/7.07 μs for 1S. In contrast, the decay curve of 2O overlaps with the instrument response function and shows a single-exponential decay, indicating that 2O does not exhibit delayed fluorescence in either neat or doped films (Fig. 2i and S4). Furthermore, the transition rate constants for intersystem crossing (kISC), reverse intersystem crossing (kRISC), radiative transition (kr,s), and non-radiative transition (knr,s) can be obtained from experimental measurements using a previously reported model51 (Table S4). As expected, the heavy atom effect of sulfur and the small ΔEST of 1S lead to faster ISC and RISC rates in its doped film, which are an order of magnitude higher than those of 1O. The values of kRISC for 1O in neat and doped thin films are 1.29 × 105 and 0.98 × 105 s−1, respectively, and those for 1S are 1.21 × 106 and 0.84 × 106 s−1 (Table 1). Compared to other luminescent compounds, the relatively high rates indicate that triplet excitons can be efficiently converted into singlet excitons through RISC, which has been well known as a key factor for OLED applications. Therefore, 1O and 1S are likely good candidates for sensitizer applications in devices.
More factors may influence the photophysical dynamics of these molecules. The absolute photoluminescence quantum yields (PLQYs) of neat and doped thin films at 300 K are listed in Table 1. The PLQYs of 1O, 1S, and 2O in neat thin films are 39.3%, 20.4%, and 9.7%, respectively, and increase to 72.4%, 63.5%, and 23.6% in doped thin films, respectively. The relatively low PLQYs in neat thin films may be due to strong intermolecular interactions, which can easily lead to π–π stacking or molecular aggregation and consequently enhance non-radiative energy transitions (exciton quenching) and self-quenching. By doping with an appropriate host material, the intermolecular distance in the film increased. Such a change can reduce direct molecular interactions and suppress aggregation-caused quenching, thereby improving the emission efficiency.
At the cryogenic temperature of 77 K, the thermal broadening effect is significantly reduced, making any hidden anharmonic peaks more detectable. Note that even minimal anharmonicity would induce noticeable peak splitting. As shown in Fig. 2e and f, the low-temperature fluorescence spectra of 1O and 1S exhibit single peaks without characteristic Fermi resonance splitting, indicating an extremely small anharmonic coupling constant (V3). This confirms that the vibrational behavior predominantly follows the harmonic oscillator model.
The results of binary systems are summarized in Fig. 4. After the host TCTA absorbs photons and reaches the S1 state, the excitons can undergo two pathways. One is the direct channel, in which a FRET process occurs to generate the S1-state sensitizer. Another is the indirect channel, in which TCTA converts to its T1 state via intersystem crossing at the beginning, followed by a TTET process to promote the sensitizer to its T1 state and a possible reverse intersystem crossing to finally produce the S1-state sensitizer. The transition rates of these processes might correlate with the PLQYs of 1O, 1S, and 2O in doped thin films.
![]() | ||
Fig. 4 Transition rates of photophysical processes in the presence of 2O (a), 1O (b), and 1S (c) as sensitizers. |
Under photoexcitation, the photophysical behaviors of the 2O, 1O, and 1S binary systems exhibit some differences. For the 2O binary system, the TTET channel is blocked by the large triplet-state conformational change of 2O (RMSD = 0.60 Å), while the FRET rate related to the direct pathway is estimated to be 7.8 × 107 s−1. For the 1O and 1S binary systems, the direct channels are preferred with the FRET rates at 1.9 × 106 and 4.8 × 108 s−1, respectively. The RISC process dominates the efficiency of indirect channels and is one order of magnitude slower than FRET for 1O and 1S. On one hand, the relatively rapid FRET of the 1S system may lead to its high PLQY. On the other hand, it was experimentally measured that the non-radiative decay rate of 2O is stronger than its radiative decay rate (see Table 1), indicating a side channel in its direct pathway. Meanwhile, the alternative indirect pathway is accessible for 1O and 1S but obstructed for 2O, agreeing well with their different PLQYs.
Analysis of the ternary systems can help us better understand the performance of electroluminescent devices such as EQE. Starting from TCTA (S1), three possible pathways were proposed. First, the ISC transition may occur in the S1 state of TCTA, followed by two successive TTET processes to produce the Ir(III) complex in its T1 state via the triplet sensitizer (denoted as ISC–TTET–TTET). Second, the sensitizer can jump to the S1 state via FRET from TCTA (S1) and then switch to sensitizer (T1), followed by TTET to generate the triplet Ir(III) complex (denoted as FRET–ISC–TTET). Third, the sensitizer exciton in its S1 state possibly undergoes another FRET process and promotes the Ir(III) complex to its S1 state, followed by the ISC to the T1 state in the last step (denoted as FRET–FRET–ISC). Unlike photoexcitation for binary systems, the electroluminescent ternary systems can also start from TCTA (T1), leading to the fourth pathway as TTET–TTET (i.e., the first pathway without ISC for TCTA in the first step).
Different photophysical behaviors of the 2O, 1O, and 1S as sensitizer in ternary systems are summarized in Fig. 4. Similar to the binary system, the key factor in the relaxation process of the 2O ternary system is the severe conformational distortion between the T1 and S0 states of 2O, which seriously impedes all pathways involving TTET. Only the FRET–FRET–ISC channel works with a modest efficiency determined by the energy transfer process from the 2O sensitizer to the Ir(III) complex (6.5 × 106 s−1). For the 1O system, the T1 excitons undergo effective TTET–TTET at the timescale of nanoseconds (3.5 × 109 s−1), while the S1 excitons possibly transfer to the triplet Ir(III) complex through ISC–TTET–TTET, FRET–ISC–TTET, or FRET–FRET–ISC. All three processes take place at the timescale of microseconds. The pattern of the 1S ternary system is different from that of 1O. On one hand, the transition rate of TTET–TTET starting from TCTA (T1) is reduced to the timescale of microseconds (4.8 × 106 s−1). On the other hand, the most rapid relaxation channel of the S1 excitons is FRET–FRET–ISC with the rate-determining step as the FRET from the host TCTA to the 1S sensitizer (4.8 × 108 s−1). Additionally, its TADF characteristic might enhance the efficiency of reverse ISC from 1S (T1) to 1S (S1) and provide an auxiliary channel for the T1 excitons.
Another type of binary system by excluding the wide-gap host TCTA from the corresponding ternary system may eliminate redundant energy transfer pathways and possibly achieve more efficient exciton management. Take the 1O sensitizer as an example. In such a binary system, the energy transfer step from TCTA to 1O, which is less efficient than that from 1O to the Ir(III) complex, is removed, prompting the rates of TTET and FRET to 1.1 × 1010 and 1.3 × 108 s−1, respectively. The same tendency can be observed on the FRET–FRET–ISC channel for the 1S binary system, in which the EnT rate for the rate-determining step increases from 4.8 × 108 to 1.0 × 109 s−1. All theoretical research results recommend 1O and 1S as excellent candidates for host or sensitizer materials in devices.
The efficiency of photophysical processes of different sensitizers can be affected by different factors. First, conformational mismatch between the singlet and triplet 2O seriously suppresses the TTET channel, which should be responsible for its restricted performance in all systems. This suggests we pay more attention to molecular rigidity under excitation when we design a new sensitizer. Second, the multi-channel energy transfer capability of 1O makes a strong contribution to enhancing exciton utilization. Finally, the TADF characteristic of 1S, which further corresponds to heavy atoms and a small S1–T1 energy gap, provides an opportunity for T1 excitons to utilize the ultrafast FRET channel. It means that the strategy for designing a TADF emitter, for example, by introducing a multi-resonance structure or decreasing the intramolecular distance between donor and acceptor groups, can be directly applied to a sensitizer.
The relationship between the molecular structure and energy transfer efficiency can be understood based on Tables 2 and 3. First of all, as long as the sensitizer undergoes a large conformational change in different electronic states, the related energy transfer pathways would be completely obstructed. The structural rigidity becomes dominant in this case. The rates of TTET are also strongly influenced by electron exchange couplings (see Table 3). It would be very useful to carefully view the frontier molecular orbitals of the host-sensitizer and sensitizer-emitter complexes when we design a ternary OLED device. In contrast, the Franck–Condon term may play an important role in the efficiency of FRET. Except for molecular rigidity, the vibrational modes of sensitizers and anharmonic and Duschinsky effects should be studied with more sophisticated theoretical models in future research. Additionally, binary systems in which the sensitizer acts as a host are expected to exhibit superior efficiency in next-generation OLED devices relative to their ternary counterparts, owing to their simplified energy transfer pathways and accelerated charge transport kinetics.
Ed (kcal mol−1) | Ea (kcal mol−1) | RMSDd (Å) | RMSDa (Å) | FC term (hartree−1) | |H12|2 (hartree2) | kEnT (s−1) | |
---|---|---|---|---|---|---|---|
TCTA–2O | 73.6 | 78.4 | 0.21 | 0.34 | 0.07 | 4.29 × 10−9 | 7.8 × 107 |
TCTA–1O | 73.6 | 70.3 | 0.21 | 0.42 | 0.07 | 1.12 × 10−10 | 1.9 × 106 |
TCTA–1S | 73.6 | 56.8 | 0.21 | 0.34 | 3.00 | 6.18 × 10−10 | 4.8 × 108 |
2O–Ir | 78.4 | 56.1 | 0.34 | 0.09 | 9.76 | 2.52 × 10−12 | 6.5 × 106 |
1O–Ir | 70.3 | 56.1 | 0.42 | 0.09 | 1.47 | 3.25 × 10−10 | 1.3 × 108 |
1S–Ir | 56.8 | 56.1 | 0.34 | 0.09 | 3.04 | 1.27 × 10−9 | 1.0 × 109 |
Ed (kcal mol−1) | Ea (kcal mol−1) | RMSDd (Å) | RMSDa (Å) | FC term (hartree−1) | |H12|2 (hartree2) | kEnT (s−1) | |
---|---|---|---|---|---|---|---|
a The FC terms and EnT rates are neglected because of the large RMSD between 2O (S0) and 2O (T1). | |||||||
TCTA–2O | 73.3 | 61.6 | 0.20 | 0.60 | —a | 3.24 × 10−11 | —a |
TCTA–1O | 73.3 | 71.3 | 0.20 | 0.10 | 18.44 | 7.28 × 10−10 | 3.5 × 109 |
TCTA–1S | 73.3 | 55.5 | 0.20 | 0.21 | 24.36 | 1.02 × 10−11 | 6.5 × 107 |
2O–Ir | 61.6 | 51.6 | 0.60 | 0.09 | —a | 1.90 × 10−11 | —a |
1O–Ir | 71.3 | 51.6 | 0.10 | 0.09 | 104.51 | 4.04 × 10−10 | 1.1 × 1010 |
1S–Ir | 55.5 | 51.6 | 0.21 | 0.09 | 26.44 | 6.96 × 10−13 | 4.8 × 106 |
Despite the similar molecular structures of sensitizers 1O and 1S, they exhibit distinct TTET rates (1.1 × 1010 s−1 for 1O → Ir and 4.8 × 106 s−1 for 1S → Ir), which originate from the synergistic effects of Franck–Condon factors and electronic coupling integrals. The former can be seen in Fig. S18. During the S0 → T1 transition of 1O, the molecular configuration maintains good planarity (RMSD = 0.10 Å) with minimal C–O–C bond length changes (Δr < 0.02 Å). This structural rigidity results in high vibrational wavefunction overlap and a large FC factor (104.51 hartree−1). In contrast, the steric repulsion between the sulfur atom's lone pairs and aromatic π–electrons in 1S may lead to approximately 5–10° torsion on the C–S–C bridge, resulting in more significant geometric changes (RMSD = 0.21 Å and Δr ∼0.05 Å) and a reduced FC factor (26.44 hartree−1). The difference in the electronic couplings can be seen in Fig. S19. The smaller van der Waals radius of oxygen in the 1O–Ir complex enables closer D–A stacking (4 Å), enhancing orbital overlap and electronic coupling (10−10 hartree2). Conversely, the larger sulfur atom in the 1S–Ir complex increases the intermolecular distance between the donor and acceptor (5.8 Å) and causes orientation deviation, finally weakening orbital overlap and electronic coupling (10−13 hartree2). Except for the well-known heavy-atom effect during the O → S substitution in sensitizer design, our results suggest further optimizations on vibrational coupling in donor–acceptor complexes (e.g., by selecting more rigid frameworks) and excited-state geometric displacement (e.g., through intramolecular constraints to enhance complex rigidity).
In brief, theoretical research on photophysical processes of sensitizers reveals that an ideal sensitizer should simultaneously possess multi-path energy transfer capabilities in addition to conformational rigidity and TADF properties as exemplified by Monkman et al.52 More importantly, careful design of binary and ternary sensitized systems is essentially required, such as enhancing intermolecular electronic coupling and minimizing intermediate losses. Besides the well-known TADF characteristics, an effective energy transfer process between the host, sensitizer, and emitter, either FRET or TTET, also significantly contributes to achieving high EQE and low efficiency roll-off in OLED devices.
Vona (V) | Lmaxb (cd m−2) | EQEmaxc (%) | dEQE@1000 cd m−2 (%) | Roll offe (%) | λELf (nm) | FWHMg (nm) | CIE(x, y)h | |
---|---|---|---|---|---|---|---|---|
a Turn-on voltage at 1 cd m2.b Maximum brightness.c Maximum external quantum efficiency.d External quantum efficiency at a brightness of 1000 cd m−2.e Efficiency roll off at a brightness of 1000 cd m−2 is calculated using (EQEmax − EQE@1000 cd m−2)/EQEmax × 100%.f Electroluminescence peak value.g Full width at half maximum.h Commission internationale de l'Eclairage color coordinates at a brightness of 1000 cd m−2. | ||||||||
TCTA + Ir | 2.9 | 10![]() |
10.2 | 9.9 | 2.9 | 640 | 63 | (0.68, 0.29) |
TCTA + Ir-block | 2.6 | 13![]() |
22.7 | 15.4 | 32.2 | 640 | 63 | (0.70, 0.30) |
TCTA + 2O + Ir | 2.4 | 23![]() |
24.6 | 21.7 | 11.8 | 637 | 63 | (0.70, 0.30) |
TCTA + 1O + Ir | 2.5 | 22![]() |
26.2 | 24.0 | 8.4 | 637 | 60 | (0.70, 0.30) |
TCTA + 1S + Ir | 2.5 | 26![]() |
26.2 | 24.0 | 8.4 | 639 | 71 | (0.70, 0.30) |
2O + Ir | 2.2 | 27![]() |
23.9 | 21.7 | 9.2 | 636 | 64 | (0.70, 0.30) |
1O + Ir | 2.3 | 23![]() |
27.5 | 26.2 | 4.7 | 634 | 57 | (0.70, 0.30) |
1S + Ir | 2.2 | 26![]() |
29.2 | 27.6 | 5.5 | 637 | 64 | (0.70, 0.30) |
Without adding any sensitizers, the device based on TCTA and Ir(mpiq)2acac exhibited a low EQEmax of 10.2%, a low maximum brightness (Lmax) of 10440 cd m−2 and a slightly high turn-on voltage (Von) of 2.9 V (Fig. 5a and S21a). The device emitted red light with a peak wavelength at 640 nm, along with a weak band at around 450 nm (Fig. 5c and S22), which can be attributed to the emission of DPPyA. Such low EQEmax may be due to the carrier imbalance and the loss of excitons in the ETL in the device. Therefore, when we added a 5 nm electron blocking layer and reduced the thickness of the electron transport layer by 5 nm, the EQEmax increased notably to 22.7% along with a decrease of Von (2.6 V) and an increase of Lmax (13
700 cd m−2) (Fig. 5a and S21a). However, there was still a significant efficiency roll-off of 32.2% at a brightness of 1000 cd m−2.
When 2O, 1O, and 1S were incorporated as sensitizers into the EML, the devices demonstrated higher EQEmax, smaller efficiency roll-off, higher Lmax, lower Von and pure red emission with a peak wavelength of around 637 nm, corresponding to a CIE color coordinate of (0.70, 0.30), which means the complete energy transfer from TCTA and the sensitizer to the phosphorescent emitter. Specifically, the EQEmax and EQE@1000 cd m−2 significantly improved (Fig. 5a), reaching 24.6%/21.7%, 26.2%/24.0%, and 26.2%/24.0% for 2O, 1O, and 1S, showing a significant lower efficiency roll-off of 11.8%, 8.4%, and 8.4%. Meanwhile, the Lmax of the devices increased by 2–3 times, reaching 23080 cd m−2, 22
940 cd m−2, and 26
800 cd m−2, respectively, and Von decreased below 2.6 V (Fig. S21a). Such outstanding device performances could be attributed to the following factors. Firstly, there are effective multi-channel energy transfer processes of sensitizers as mentioned above. For 1O and 1S, they have multi-channel energy transfer capabilities, enhanced intermolecular electronic couplings, and optimized vibrational modes and TADF properties, as shown in the above theoretical part, which are beneficial for energy transfer efficiency, whereas for 2O, all triplet-state-involved channels are blocked by conformational mismatch, resulting in relatively limited performance. Secondly, these sensitizers possess bipolar charge transport properties with XT and TX groups for electron transport and a triphenylamine group for hole transport. Therefore, they play an important role in balancing the injection and transport of electrons and holes, reducing charge accumulation and exciton quenching, and thus alleviating efficiency roll-off at high current densities (Fig. 5a).
More importantly, theoretical calculations of energy transfer rates predict that binary systems by excluding the wide-gap host TCTA from the corresponding ternary system would eliminate redundant energy transfer pathways and achieve more efficient exciton management. Indeed, when we removed TCTA from the EML and used 2O, 1O, and 1S as the host and sensitizer simultaneously, the EQEmax and EQE@1000 cd m−2 further improved for 1O and 1S, reaching 27.5%/26.2%, and 29.2%/27.6%, showing a much lower efficiency roll-off of 4.7% and 5.5% (Fig. 5b), which are consistent with theoretical calculations of energy transfer rates. However, for 2O, the EQEmax was slightly decreased to 23.9%, which may be due to the inactive TADF properties of 2O and inferior PLQY in the neat film (Table 1). Meanwhile, the Von values of the devices based on 2O, 1O, and 1S were all further lowered (Fig. S21(b)), showing better charge injection and transport. All the devices gave pure red emission with a CIE color coordinate of (0.70, 0.30), which means complete energy transfer from the sensitizer to the phosphorescent emitter (Fig. 5c). Notably, to the best of our knowledge, in OLED devices with a binary EML structure based on Ir(mpiq)2acac and its derivatives as phosphorescent emitters, the 1S-based binary device exhibited the highest EQEmax (29.2%) and EQE@1000 cd m−2 (27.6%) and high Lmax (26990 cd m−2) (Fig. 5d, S23 and Table S11). Thus, theoretical calculations of energy transfer rates at the ab initio computational level provide structure–property relationships and rational guidance for OLED development. In future studies, theoretical-experimental collaborative explorations of more efficient sensitizers could achieve even higher performance in OLED devices.
The data supporting this article have been included as part of the SI. General information, synthesis and characterization, X-ray crystallography, OLED fabrication and measurement, estimation of photophysical parameters, thermal and electrochemical properties, photoluminescence properties, supplemental theoretical calculations, OLED device data, NMR and HRMS, tables for the absolute and relative energies and Cartesian coordinates. See DOI: https://doi.org/10.1039/d5sc03817k.
Footnote |
† These authors contributed equally (Xiao Liu and Xue-liang Wen). |
This journal is © The Royal Society of Chemistry 2025 |