Abstract
We present a p‐ and n‐doped nonacene compound, NOBNacene, that represents a rare example of a linearly extended ladder‐type multiresonant thermally activated delayed fluorescence (MR‐TADF) emitter. This compound shows efficient narrow deep blue emission, with a λ PL of 410 nm, full width at half maximum, FWHM, of 38 nm, photoluminescence quantum yield, ΦPL of 71 %, and a delayed lifetime, τ d of 1.18 ms in 1.5 wt % TSPO1 thin film. The organic light‐emitting diode (OLED) using this compound as the emitter shows a comparable electroluminescence spectrum peaked at 409 nm (FWHM=37 nm) and a maximum external quantum efficiency (EQEmax) of 8.5 % at Commission Internationale de l’Éclairage (CIE) coordinates of (0.173, 0.055). The EQEmax values were increased to 11.2 % at 3 wt % doping of the emitter within the emissive layer of the device. At this concentration, the electroluminescence spectrum broadened slightly, leading to CIE coordinates of (0.176, 0.068).
Keywords: Deep Blue Emission, Multi-Resonance, Nanographene, Organic Light-Emitting Diode, Thermally Activated Delayed Fluorescence
A deep blue boron‐, nitrogen‐ and oxygen‐doped nonacene emitter that shows multi‐resonant thermally activated delayed fluorescence (MR‐TADF) is described. The emitter shows bright, deep‐blue narrowband emission in an organic light emitting diode (OLED) device.

Introduction
The performance of organic light‐emitting diodes (OLEDs) has advanced significantly since the first OLED developed by Tang and Van Slyke more than 30 years ago. [1] OLED technology is now widely adopted in a range of consumer electronics such as mobile phones, smart watches, and televisions. Singlet and triplet excitons are formed in an electroluminescent (EL) device in the ratio 1 : 3 due to the Fermionic nature of holes and electrons. [2] Commercial displays use two classes of emitters for the primary colors. [1b] Phosphorescent emitters are used for green and red, whereas triplet‐triplet annihilation (TTA) using purely organic emitters are used for the blue emitter as there is at present not a sufficiently stable blue phosphorescent OLED. [3] OLEDs with TTA emitters, however, can only achieve a maximum 62.5 % internal quantum efficiency (IQE), thus, there is still room for improvement of the overall efficiency of the device. Not surprisingly, there is a huge effort undertaken by both academia and industry to develop stable and high efficiency blue emitters that can harvest 100 % IQE in the device. [3] Furthermore, deep blue OLED light sources can find application beyond displays, [4] such as for sterilization, [5] and dental [6] and dermatological treatments. [7] Purely organic thermally activated delayed fluorescent (TADF) emitters provide a tantalizing solution as TADF OLEDs can achieve up to 100 % IQE. [8] However, donor‐acceptor (D‐A) TADF compounds show very broad emission due to the long‐range charge‐transfer (LRCT) character of the excited state and the broad range of accessible geometries in the excited state as the D and A units are connected through single bonds. [9] This results in OLEDs that show poor color purity. [10] A solution to this apparent weakness of D‐A TADF emitters was advanced by Hatakeyama et al. who demonstrated how p‐ and n‐doped nanographenes, termed multi‐resonant TADF (MR‐TADF) emitters, could also exhibit TADF but with much narrower emission profiles. [11] The narrow emission spectra were rationalized in terms of the rigid structure of these compounds together with the short‐range charge transfer (SRCT) nature of the emissive excited state. [9]
The potential of MR‐TADF compounds to act as pure blue OLED emitters was first exemplified by the DABNA series (Figure 1). [11] DABNA‐1 presents a photoluminescence maximum, λ PL, of 460 nm, a full width at half maximum, FWHM, of 30 nm, a high photoluminescence quantum yield, ΦPL, of 88 %, and a moderate singlet‐triplet energy gap, ΔE ST, of 180 meV in 1 wt % mCBP host. The corresponding OLED showed pure blue emission at λ EL, of 460 nm, with a full width at half maximum, FWHM, of 30 nm, corresponding to a Commission Internationale de l’Éclairage (CIE) y‐coordinate of 0.09, and a moderately high maximum external quantum efficiency, EQEmax, of 13.5 %. The same group reported a π‐extended version of DABNA‐1, v‐DABNA, which still represents the pinnacle of blue MR‐TADF emitter design. [12] This emitter exhibited efficient narrowband blue emission (λ PL=467 nm, FWHM=18 nm, ΦPL=90 %) and a very small ΔE ST of 17 meV in 1 wt % DOBNA‐OAr host. The OLED showed an impressive performance with an EQEmax as high as 34.4 % at λ EL of 469 nm, a FWHM of 18 nm and CIE coordinates of (0.12, 0.11). Indeed, compared to the OLED with DABNA‐1, there is a remarkable improvement in the device performance with v‐DABNA. The same group modified the structure of v‐DABNA by replacing one of the nitrogen atoms with a less electron‐donating oxygen atom as in v‐DABNA‐OMe. [13] This emitter maintained efficient and narrowband blue emission (λ PL=464 nm, FWHM=24 nm in 1 wt % DABNA‐OAr). The OLED with this derivative showed a slightly blue‐shifted EL of 465 nm (FWHM=23 nm, EQEmax=29.5 %). Kwon et al. modified the v‐DABNA core to incorporate methyl and electron‐withdrawing fluorine substituents. [14] Among their three emitters, 4F‐m‐v‐DABNA (λ PL=455 nm, FWHM=14 nm in PhMe) exhibited the most hypsochromic emission compared to the parent v‐DABNA (λ PL=467 nm, 1 wt % doped in DABNA‐OAr). [15] OLEDs with 4F‐m‐v‐DABNA showed EQEmax of 33.7 % and an impressive CIE coordinate of (0.13, 0.06). [14] Yasuda et al. investigated doping mixed donor (oxygen and sulfur) atoms within the v‐DABNA core to tune the emission into the deep blue region. [16] The new emitters all presented blue‐shifted emission compared to the parent v‐DABNA (λ PL=474 nm, 3 wt % doped in mCBP). Their bluest emitter, BOBO‐Z, emits at 445 nm, with the same FWHM of 18 nm. Both ΔE ST and the delayed lifetime (τ d) increased to 0.102 eV, and 7.7 μs, respectively. The device with this emitter showed deep blue EL (λ EL=445 nm, FWHM=18 nm, EQEmax=13.6 %, CIEy=0.04). Recently Hatakeyama et al. reported a π‐extended B,N‐doped helicene, v‐DABNA‐Mes that showed efficient and narrowband PL at λ PL=484 nm, FWHM=16 nm (ΔE ST=8.5 meV, τ D=2.4 μs, ΦPL=80 %, 1 wt % doped in PMMA). [17] The OLEDs emitted at λ EL=480 nm (FWHM=27 nm; CIEy=0.21) and showed an EQEmax=22.9 %. However, the emission was red‐shifted to the sky‐blue region due to its extended π‐conjugation. We recently reported a B,N‐doped heptacene, α‐3BNMes, that shows narrowband blue emission (λ PL=442 nm, FWHM=30 nm) in THF. [18] The hyperfluorescent (HF) [19] device with α‐3BNMes as a terminal emitter sustained blue EL (λ EL=443 nm, CIEy=0.1) with an EQEmax of 15 %. Recently, Duan et al. reported a B,N‐doped pentacene emitter, mDBIC, that emits in the deep blue (λ PL=426 nm, FWHM=26 nm) region in 2 wt % doped mCP film and was used as the terminal emitter in a HF device that showed excellent performance at the deep blue color point (λ EL=431 nm, FWHM=42 nm, EQEmax=13.5 %, CIEy=0.05). [20] Pushing the emission further into the deep blue in MR‐TADF compounds remains exceedingly difficult. The B,N‐doped heptacene system α‐3BNOH (λ PL=390 nm, ΔE ST=0.30 eV, τ d=0.45 μs, THF) [21] that we previously reported represents a rare example of a MR‐TADF purple emitter as does the B,O‐doped triangulene emitter, DOBNA (λ PL=398 nm, ΔE ST=0.18 eV, τ d=66 μs, 1 wt % in PMMA). [22]
Figure 1.

Chemical structures of a) DOBNA, DABNA‐1 and reported π‐extended blue MR‐TADF emitters. b) NOBNacene.
Building on our recent efforts to design linearly extended MR‐TADF acene emitters, here we report a boron‐, nitrogen‐, and oxygen‐doped polycyclic aromatic hydrocarbon that contains nine annulated six‐membered rings, NOBNacene, (Figure 1b). Despite the apparent large conjugation length, maintaining a regioregularity of the heteroatoms, and using oxygen donors rather than more electron‐donating nitrogen atoms results in a deep blue emission in this system. This compound represents arguably the first example of an MR‐TADF emitter possessing both electronically distinct donor (N and O) and acceptor groups (two distinct B atoms).[ 12 , 23 ] In 1.5 wt % TSPO1 doped films, NOBNacene shows narrowband emission with a λ PL of 410 nm, a FWHM of 38 nm, a high ΦPL of 71 %, and a thermally activated delayed fluorescence with a τ d of 1.18 ms. The ΔE ST was measured to be 0.30 eV. The corresponding deep blue OLED shows outstanding performance with a maximum external quantum efficiency (EQEmax) of 8.5 % at a peak electroluminescence (λ EL) of 409 nm (FWHM of 37 nm), with corresponding to Commission Internationale de l’Éclairage coordinates of (0.173, 0.055), very close to the BT.2020 requirement for the blue pixel of (0.131, 0.046). [24] NOBNacene combines the benefits of high efficiency, narrow near‐UV emission, and high color purity, representing a promising emitter design approach to high‐performance deep blue OLEDs.
Results and Discussion
The convergent synthesis of NOBNacene is outlined in Figure 2. Compound 1 was obtained in 68 % yield following a Buchwald–Hartwig cross‐coupling reaction of 3,5‐dimethylaniline with 1,2‐dichlorobenzene. The key intermediate 2 was obtained in 47 % yield by coupling two equivalents of DOBNA‐Br with 1. Electrophilic borylation of 2 with BBr3 followed by reaction with excess MesMgBr afforded NOBNacene in 45 % yield. Due to its planar structure, NOBNacene is poorly soluble in most common organic solvents. The structure and purity of the emitter were confirmed by 1H NMR spectroscopy, high‐resolution mass spectrometry (HRMS), high performance liquid chromatography‐gel permeation chromatography (HPLC‐GPC), and elemental analysis (EA). The thermal behavior of NOBNacene was investigated by thermogravimetric analysis (TGA) and differential scanning calorimetry (DSC) (Figure S20). The compound is thermally stable, with 5 % mass loss (T d) occurring above 572 °C. A broad endothermic peak was observed in the DSC, with the onset temperature at 650 °C, corresponding to the material decomposition as supported by the TGA.
Figure 2.
a) Synthesis of NOBNacene. ORTEP diagram of NOBNacene, b), c) are side views and d) is a plane view. Thermal ellipsoids show 50 % probability.
Single crystals of NOBNacene were obtained by slow evaporation of a saturated solution of the compound in THF over several days at room temperature. [25] The crystal structure is shown in Figures 2b–d. No hydrogen bonding or π–π stacking intermolecular interactions were observed for NOBNacene in the crystal structure owing to the presence of the highly twisted mesityl and xylyl groups that decorate the nonacene core. As shown in the Figure 2b, the nonacene core of NOBNacene remains nearly planar. The B‐CMes bond is longer than other bonds in the system, because of this difference in bond lengths the nonacene skeleton is slightly bent as shown in Figure 2d.
The ground [excited] state optimizations were carried out using [Time Dependent‐] Density Functional Theory [TD‐](DFT) with the PBE0 functional [26] and the 6‐31G(d,p) [27] basis set [within the Tamm‐Dancoff approximation (TDA)] in the gas phase while the excited states excitation energies were modelled with the spin‐component scaling second‐order approximate coupled‐cluster (SCS‐CC2) method. The latter wavefunction‐based method has been shown to be essential to model accurately the excited states of MR‐TADF emitters. [28] In the ground state (Figure 3a), the HOMO is mainly localized on the atoms of the central benzene ring and the DOBNA fragments while the LUMO is mainly localized on the DOBNA boron atoms with a very small contribution from the mesityl boranes. The calculated HOMO and LUMO values are −4.99 eV and −1.22 eV, respectively, resulting in a predicted HOMO–LUMO gap of 3.77 eV. This gap is smaller than both DOBNA itself (3.97 eV) [22] and the structurally related deep blue B,N‐doped heptacene derivatives, α‐3BNOH (4.20 eV) and α‐3BNMes (4.03 eV).[ 18 , 21 ]
Figure 3.
a) HOMO and LUMO electron density distribution and orbital energies of NOBNacene calculated at PBE0/6‐31G(d,p) in the gas phase (isovalue=0.02); b) Difference density plots and energies for the two lowest‐lying singlet and triplet excited states of NOBNacene calculated at SCS‐CC2/cc‐pVDZ in the gas phase (isovalue=0.001). The blue color represents an area of decreased electron density, and the yellow color represents an increased electron density between the ground and excited states. f denotes the oscillator strength for the transitions to the excited singlet states.
The difference density plots for the first singlet and triplet excited states show the alternating pattern of increasing and decreasing electron density that is characteristic of MR‐TADF emitters. The difference density plots reveal that the electron density in both the S1 and T1 states is mostly localized on the electron‐rich central part of the molecule. However, the difference density patterns of S1 and T1, while being reminiscent of SRCT excited states, are distinct from each other because of the different one‐electron transitions contributions (see Supporting Information, Tables S1 and S2). The electron density is more diffusely distributed across the entire molecular skeleton in the S2 and T2 states. A small ΔE S1T1 value of 0.12 eV is noted for NOBNacene (Table S1); however, owing to the different S1 and T1 difference density patterns, obtained from vertical excitations from the ground state, it is likely that the vertical ΔE S1T1 would not be accurate, as these excited states would exhibit different relaxation energies. [29] We therefore undertook SCS‐CC2 calculations at the optimized S1 and T1 geometries and observed that the adiabatic ΔE S1T1 increases to 0.18 eV (Figure S11 and Table S2). An intermediate T2 state is reported between S1 and T1, obtained from vertical excitation from the ground state, which suggests that RISC could occur through a spin‐vibronic coupling mechanism. The S0−S1 transition has a high oscillator strength of 0.32 from calculations with vertical excitation from the ground state, which rises to 0.40 at the relaxed S1 geometry.
Optoelectronic Characterization
We first undertook a photophysical investigation of NOBNacene in dilute THF solutions (10−5 M) at 300 K (Figure 4 and Table 1), which would provide insight into understanding the monomolecular properties of this compound. An intense absorption was noted at 229–283 nm with molar absorptivity (ϵ) ranging from 130 to 12×103 M−1 cm−1. A well‐defined, intense absorption band at 358 nm (ϵ=99×103 M−1 cm−1) and a lowest energy band at 382 nm (ϵ=50×103 M−1 cm−1) were observed corresponding to transitions mainly localized on the nonacene core as assigned from the TDA‐PBE0/6‐31G(d,p) calculations. The absorption profile is similar to that of α‐3BNOH [21] and its derivative, α‐3BNMes. [18] The lowest energy band in NOBNacene is slightly red‐shifted compared to that in α‐3BNOH (λ abs=379 nm, ϵ=14×103 M−1 cm−1) [21] but significantly blue‐shifted from that in α‐3BNMes (λ abs=419 nm, ϵ=18×103 M−1 cm−1). The photoluminescence (PL) of NOBNacene in solution is structured and of intermediate broadness (FWHM of 40 nm, 0.29 eV) compared to other reported deep blue MR‐TADF emitters, see below. [9] The emission maximum, λ PL, is at 405 nm and there is a low‐energy shoulder at 427 nm. We simulated the vibronically‐resolved emission spectrum within the undistorted harmonic model considering vibrational modes computed at the PBE0/6‐31G(d,p) level for the NOBNacene model derivative without the mesityl and xylyl substituents. We found that the broadening of the emission is essentially due to three vibrational modes with energies of 178, 643 and 1674 cm−1. The two lower‐frequency modes contribute to the main emission vibronic peak while the highest one leads to the side band (see Figures S13). The ΔE ST, calculated from the difference in the energy of the onsets of the prompt fluorescence and phosphorescence spectra at 77 K in 2‐MeTHF, is 0.31 eV (Figure S14a). This value is comparable to those of α‐3BNOH (ΔE ST=0.25 eV, 1 wt % in PMMA) [21] and α‐3BNMes (ΔE ST=0.28 eV, 1 wt % in PMMA). The photoluminescence quantum yield (ΦPL) in degassed dilute THF solution is 33 %, which decreased under air to 25 %. No delayed emission was observed in THF and the lifetime, τ PL, is 22.4 ns (Figure S15).
Figure 4.

Absorption (blue solid line), steady‐state PL in THF at 300 K (blue dotted line), and steady‐state PL of the 1.5 wt % evaporated doped thin film in TSPO1 at 300 K (violet dotted line), λ exc.=365 nm. Inset shows the PL of NOBNacene in THF at 300 K, λ exc.=365 nm.
Table 1.
Photophysical properties of NOBNacene.
|
Compound |
Medium |
λ PL [c] [nm] |
FWHM[d] [nm] |
E S1 [e] [eV] |
E T1 [e] [eV] |
ΔE ST [g] [eV] |
ΦPL [h] [%] |
τ p [i] [ns] |
τ d [i] [ms] |
k ISC [j] [s−1] |
k RISC [j] [s−1] |
k s_r [j] [s−1] |
k s_nr [k] [s−1] |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
|
NOBNacene |
Sol.[a] |
405 427 |
40 |
3.12[f] |
2.81 [f] |
0.31 |
33[a] |
22.34 |
– |
– |
– |
– |
– |
|
film[b] |
410 430 |
38 |
3.12 |
2.82 |
0.30 |
71[b] |
2.9 |
1.18 |
2.61×108 |
3.74×103 |
7.24×107 |
1.18×107 |
[a] In THF solutions (10−5 M). [b] Measured in evaporated thin films consisting of 1.5 wt % emitter in TSPO1 host under vacuum. λ exc=280 nm. [c] Steady‐state emission maximum at 300 K. λ exc=365 nm. [d] Full width at half maximum of the emission peak. [e] S1 and T1 energies were obtained from the onsets of the respective prompt fluorescence (delay: 1 ns; gate time: 100 ns) and phosphorescence spectra (delay: 1 ms; gate time: 9 ms) at 77 K. λ exc=343 nm. [f] 2‐MeTHF glass (10−6 M). [g] ΔE ST=E(S1)−E(T1). [h] Relative photoluminescence quantum yields (ΦPL) in solutions were measured by the relative method using quinine sulfate as a standard (Φr=54.6 % in 1 N H2SO4). [30] Absolute ΦPL of thin films were measured using an integrating sphere. [i] i Prompt and delayed lifetimes obtained by TCSPC and MCS, respectively. λ exc=379 nm. [j] Intersystem and reverse intersystem crossing rates were calculated using steady‐state approximation method as described in literature. [31]
We next explored the potential of this compound as an emitter in an OLED. Of the suitably high triplet energy hosts investigated (TSPO1, DPEPO, PPT, and mCP), the highest ΦPL of 71 % was obtained when the emitter is doped in TSPO1 host at 1.5 wt %; the ΦPL of this film reduced to 33 % upon exposure to air (see Table S3 for host matrix ΦPL study), suggesting strongly that there are accessible triplet excited states. The PL spectrum of NOBNacene is red‐shifted by 5 nm in the 1.5 wt % TSPO1 doped film compared to in THF solution (Figure 4a). The FWHM of the emission spectrum in the doped film is 38 nm (0.26 eV). The high‐energy peak around 410 nm is the dominant one and there is a low‐energy shoulder at 430 nm, consistent with the theoretical calculations. The emission of NOBNacene is red‐shifted by 12 nm from DOBNA (λ PL=398 nm, ΦPL=58 %, in 1 wt % PMMA). [22] The ΔE ST is 0.30 eV in the 1.5 wt % TSPO1 thin film, a value that is nearly identical to that observed in 2‐MeTHF (Figure S14).
Temperature‐dependent transient PL analysis was carried out to identify the nature of the triplet harvesting in NOBNacene. We observed a biexponential emission decay with associated prompt (τ p) and delayed (τ d) lifetimes of 2.90 ns and 1.18 ms, respectively (Figures 5a and b). The prompt component shows no temperature dependence, while the intensity of the delayed emission increases above 250 K. The temperature dependence of the delayed emission provides confirmation that NOBNacene is TADF active. TADF in emitters with large ΔE ST have previously been reported by Lu et al. [32] in a D‐A type violet emitter CZ‐MPS that exhibited a very long τ d of 4.85 ms linked to a ΔE ST of 0.58 eV. The authors ascribed the TADF to proceeding via intermediate triplet states. The k RISC value of NOBNacene was calculated to be 3.74×103 s−1, which is slower than what reported for DOBNA (1.6×104 s−1, in 1 wt % PMMA), [22] but faster than for α‐3BNMes (5.9×102 s−1, in 1 wt % PMMA). [18]
Figure 5.
Time‐resolved PL decays of NOBNacene doped thin films (cD=1.5 wt % in TSPO1 host) under various temperatures from 300 K to 100 K. The measurements were performed by using TCSPC with samples loaded in a cryostat in vacuum. a) TCSPC at a 100 ns time scale, b) MCS at a 10 ms time scale. IRF is instrumental response function. The excitation wavelength was 379 nm and the PL emission at 410 nm was recorded.
Given the high‐energy emission, the choice of host matrix with suitable high triplet energies is very limited. From the photophysical study TSPO1 was identified as the most suitable host matrix to be used in the OLED. The optimized device structure used was: ITO/HAT‐CN (5 nm)/NPB (40 nm)/TCTA (10 nm)/CzSi (10 nm)/NOBNacene (1.5–6.0 wt %) : TSPO1 (20 nm)/TSPO1 (10 nm)/TmPyPB (20 nm)/LiF (0.8 nm)/Al (100 nm), where HAT‐CN, NPB, TCTA, CzSi, TSPO1, TmPyPB, LiF are the hole injection, hole transporting, electron blocking, exciton blocking, hole blocking, electron transporting, and electron injection layers, respectively. The device structure and energy levels of each layer are illustrated in Figure S17. OLED devices were fabricated using cD of 1.5 wt %, 3.0 wt %, and 6.0 wt % to understand its effects on both carrier transport and color purity. Device performance metrics are summarized in Table 2.
Table 2.
Device data of NOBNacene in TSPO1 and DPEPO host.
|
Host |
cD [wt %] |
Von [V] |
λ EL [nm] |
FWHM/nm |
CIE (x,y) |
EQEmax [%] |
|---|---|---|---|---|---|---|
|
TSPO1 |
1.5 3.0 6.0 |
4.2 4.2 4.1 |
409 412 412 |
37 41 47 |
(0.173, 0.055) (0.176, 0.068) (0.187, 0.103) |
8.5 11.2 10.2 |
|
DPEPO |
1.5 |
5.1 |
411 |
44 |
(0.196, 0.106) |
4.2 |
The device with cD of 1.5 wt % in TSPO1 host presented narrow violet emission with a maximum at λ EL of 411 nm (FWHM=37 nm) and a shoulder at 428 nm, which are assigned as vibronic bands. The EL matches well the PL of the film at the same cD (λ PL=410 nm, FWHM=38 nm, 1.5 wt % in TSPO1). At 3 wt % doping concentration, the λ EL is nearly unchanged at 412 nm compared to the EL of the 1.5 wt % device; however, the FWHM increased slightly to 41 nm and the shoulder at 428 nm is more pronounced. The λ EL of the device with cD of 6.0 wt % is essentially the same (412 nm); however, there is significant broadening of the EL (FWHM=47 nm) due to the more pronounced shoulder at 428 nm. The broadening of emission for fused planar emitters at a higher concentration is common due to intermolecular interaction in the emitting layers. [33] Due to its high ET, we also fabricated devices using DPEPO as the host at the same cD of 1.5 wt % for comparison purposes. Besides the lower EQE, the EL spectrum is broadened (FWHM=44 nm) and the turn‐on voltage is higher by 0.9 V in the DPEPO device compared to that in TSPO1. In addition, the device showed incomplete electron confinement within the EML as evidenced by the high‐energy EL peak at 380 nm, which was assigned to emission from the TCTA layer.
The CIE coordinates of the TSPO1 devices with cD of 1.5 wt % are (0.173, 0.055), values that are very close to the Rec.2020 standard for primary blue in UHDTV (0.131, 0.046). [24] Increasing the doping concentration of the emitter resulted in the expected reduced colour purity of the device, reflected in the CIE coordinates of (0.176, 0.068) and (0.187, 0.103), respectively, for the 3 wt % and 6 wt % devices. The EQEmax (PEmax) were 8.5 % (2.06 lm W−1), 11.2 % (3.51 lm W−1) and 10.2 % (5.19 lm W−1) for devices with cD of 1.5 wt %, 3.0 wt % to 6.0 wt %, respectively. The high EQE (11.2 %) of the device at this deep blue chromaticity (CIEy<0.08) is among the highest recorded to date (Figure 6d). The device data are summarized in Table S4. A linear dependence of luminescence to current density (Figure S18) and the presence of delayed component in the transient PL analysis provide strong indications that triplet harvesting in the device occurs through TADF. Despite the high EQEmax, the efficiency roll‐off in each system is severe, which is likely due in part to the large ΔE ST of the emitter, [33] the long delayed lifetimes that result in increased TTA and STA processes, and the instability of the phosphine oxide‐based host. [34] The EL spectra were unchanged during operation, while the intensity decreased rapidly to 50 % of its initial value within 10 min. Such behavior is not uncommon in deep blue OLEDs, especially considering the electrically unstable phosphine oxide‐based TSPO1 host.
Figure 6.

OLED device performance for NOBNacene in both DPEPO and TSPO1 host. a) EL spectrum of devices at 6 V. Inset shows Image of an operating TSPO1 device (c D=1.5 wt %) under 6 V. b) Dependence of external quantum efficiency (EQE) and power efficiency (PE) on the luminance. c) Current density‐voltage‐luminance (J–V–L) characteristics of the device. d) EQEmax comparison in terms of EL peak wavelength to reported fluorescent (Fluo.) and D‐A type TADF emitters. source references for the plotted data are given in Table S4 and compared with literature devices.
Conclusion
Herein, we demonstrate an easy‐to‐access synthetic route to construct a boron, nitrogen, and oxygen doped ladder type nonacene. The emitter NOBNacene is the first example of a π‐extended MR‐TADF emitter that has nine, six‐membered rings fused along one dimension. Strikingly, this π‐extended design shows only a limited conjugation length, reflected in emission in the deep blue region in THF solution (λ PL=405 nm, FWHM=40 nm, ΦPL=33 %) and in the 1.5 wt % TSPO1 film (λ PL=410 nm, FWHM=38 nm, ΦPL=71 %, τ d=1.77 ms). This emitter design utilizes two electronically distinct boron acceptor atoms and a combination of nitrogen and oxygen donor atoms. Deep blue EL (λ EL=409 nm, FWHM=37 nm) was produced when NOBNacene was employed as the emitter in the OLED. An EQEmax of 8.5 % at CIE coordinates of (0.173, 0.055) was achieved. The EQEmax could be enhanced to 11.3 % at a higher emitter doping of 3 wt %, with only a small loss in the color purity, reflected in CIE coordinates of (0.176, 0.068). The EQEmax values reported here are among the highest reported for deep‐blue OLED devices where the λ EL<420 nm. Compared with the reported fluorescent, donor‐acceptor type TADF, and MR‐TADF based OLEDs shown in Figure 6d, the NOBNacene device combines near UV emission at 410 nm, high EQEmax of over 10 %, and deep blue color purity with CIEy of 0.06, a device performance that is promising not only for displays but also for applications that require a near UV light source.
Conflict of interest
The authors declare no conflict of interest.
1.
Supporting information
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Acknowledgments
This project has received funding from the European Union's Horizon 2020 research and innovation programme under the Marie Skłodowska Curie grant agreement No 838885 (NarrowbandSSL). S.M.S. acknowledges support from the Marie Skłodowska‐Curie Individual Fellowship (grant agreement No 838885 NarrowbandSSL). We would like to thank the Leverhulme Trust (RPG‐2016‐047) for financial support. E.Z.‐C. and I.D.W.S. acknowledge support from EPSRC (EP/L017008, EP/P010482/1). Computational resources have been provided by the Consortium des Équipements de Calcul Intensif (CÉCI), funded by the Fonds de la Recherche Scientifiques de Belgique (F.R.S.‐FNRS) under Grant No. 2.5020.11, as well as the Tier‐1 supercomputer of the Fédération Wallonie‐Bruxelles, infrastructure funded by the Walloon Region under the grant agreement n1117545. Y.O. acknowledges funding by the Fonds de la Recherche Scientifique‐FNRS under Grant n° F.4534.21 (MIS‐IMAGINE). G. R. acknowledges a grant from the “Fonds pour la formation a la Recherche dans l'Industrie et dans l'Agriculture” (FRIA) of the FRS‐FNRS. We would like to thank Mr. David Webster for the assistance with the ambient pressure photoemission spectroscopy (APS) measurements, and Dr. Joydip De for the assistance with the TGA/DSC measurements.
Madayanad Suresh S., Zhang L., Hall D., Si C., Ricci G., Matulaitis T., Slawin A. M. Z., Warriner S., Olivier Y., Samuel I. D. W., Zysman-Colman E., Angew. Chem. Int. Ed. 2023, 62, e202215522; Angew. Chem. 2023, 135, e202215522.
A previous version of this manuscript has been deposited on a preprint server (https://doi.org/10.26434/chemrxiv‐2022‐nb1sf).
Contributor Information
Ifor D. W. Samuel, Email: idws@st-andrews.ac.uk.
Eli Zysman‐Colman, Email: eli.zysman-colman@st-andrews.ac.uk.
Data Availability Statement
The research data supporting this publication can be accessed at https://doi.org/10.17630/bbf0fb10‐6225‐4422‐8b0b‐73c965e2e6ba.
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Supporting Information
Supporting Information
Data Availability Statement
The research data supporting this publication can be accessed at https://doi.org/10.17630/bbf0fb10‐6225‐4422‐8b0b‐73c965e2e6ba.



