Synthesis and characterization of NON-materials. The novel 1,3,5-oxadiazine compounds NON, NON-CF3 and NON-Br were synthesized in one-step by heating the substituted arylhydrazine hydrochlorides and cyclohexylcarbaldehyde in glacial acetic acid at 60ºC for 3 h (Scheme 1). The reaction forms three heterocyclic rings and two stereogenic centres (C2 and C3 carbon atoms, Fig. 1). The reaction yields varied from moderate for NON and NON-Br (22–26%) to high for NON-CF3 (82%). Garg et al.22 previously reported that lactols and hemiaminals behave as masked carbaldehydes under conditions of Fisher indole synthesis, resulting in the formation of various indoline derivatives with two heterocyclic rings and two stereogenic centres (Scheme 1, top). Therefore, we propose that formation of the NON-R compounds occurs via an interrupted Fischer indolization.23,24 It’s worth noting that the 1,3,5-oxadiazine moiety is a powerful heterocyclic framework with applications in pharmaceuticals, agricultural, and industry. This makes the facile synthesis of NON-R (R = H, CF3 and Br) materials interesting in its own right.25–29
All NON compounds are white solids, stable in air and soluble in common polar organic solvents dichloromethane, acetone, THF and poorly soluble in hexane. The purity of the products were confirmed by 1H, 13C and 19F NMR, High-Resolution Mass Spectrometry and X-ray diffraction analysis. The thermal stability of NON-materials increases from NON-Br (235°C) to NON (256°C) to NON-CF3 (262°C, Figure S12). The central oxadiazine ring possesses two groups of distinctive proton resonances: the first as a doublet at 4.9 ppm for C1-H1, and the second is a singlet at 5.2 ppm for C2-H2 and C3-H3 (see Supplementary file). Crystals of NON-materials were grown by layering dichloromethane solutions with hexanes (Fig. 1, S8–S10). All three compounds possess meso-stereochemistry (R for C2 and S for C3). Similar stereochemical observations for the fused 1,3,5-oxadiazine rings have been reported by Ghinet et al.25 The X-ray crystal structure revealed that the central oxadiazine six-membered ring adopts a chair-conformation where the H2 and H3 atoms occupy an axial position, whereas the H1 atom occupies an equatorial position (Fig. 1). Both indoline and spiro-cyclohexyl moieties of the NON-materials point in opposite directions with respect to the central oxazine core, thus forming voids above and below the central ring, which are capable of accommodating solvent molecules (for instance, hexane, see Figure S8). Molecules of the NON-materials form a three-dimensional network through weak CH∙∙∙π, C–H∙∙∙F, C–H∙∙∙Br or CHδ+(phenyl)···δ+HC(cyclohexyl) interactions between neighbouring molecules.
Cyclic voltammetry experiments were performed to investigate the redox properties of NON, NON-Br, and NON-CF3 in 1,2-difluorobenzene solution (Figure S11). The data is summarised in Table 2. The NON compound exhibits a non-reversible oxidation at a peak potential of Ep = + 0.5 V. The NON-CF3 material shows two oxidation processes: the first one is reversible (E1/2 = + 0.90 V), while the second is irreversible with Ep at + 1.38 V. The NON-Br compound shows two reversible oxidations at E1/2 = + 0.62 and + 1.12 V. The onset of the first oxidation potential (Eonset) values were used to calculate the energy level of the highest occupied molecular orbital (EHOMO, see Table 1) for the NON-R materials. The EHOMO energy correlates with the electron-withdrawing strength of the substituent R, i.e. it increases in the line from − 5.76 (R = H) to − 5.90 (R = Br) and − 6.14 eV (R = CF3). The oxidation process of the NON compounds are likely centred on the indoline moiety, which is supported by the theoretical calculations which predict the localization of the HOMO to this region(see Fig. 3c, Table S4). The reduction potential for all three compounds was beyond the solvent discharge potential, therefore, a direct calculation of the LUMO energy level is impossible. Instead, the ELUMO energy was estimated indirectly using the equation ELUMO = Eopt−gap + EHOMO, where Eopt−gap is taken as the red-onset of the lowest energy absorption band in the UV-vis absorption spectra in a dichloromethane solution (vide infra, Table 1).
Photophysical properties. To investigate photophysical properties, UV-visible absorption (Fig. 2) and photoluminescence (Fig. 3) spectra were recorded for all NON compounds. The data is summarized in Tables 1 and 2. All compounds show a strong absorption band in the range 260–280 nm (extinction coefficient ε up to 2.8·104 M− 1 cm− 1). This has been assigned to π–π* transitions within the indoline moieties. Theoretical calculations support this assignment and predict a vertical excitation S0→S1 in the range 268–280 nm to be largely a HOMO→LUMO transition within the indolines of the NON materials (Fig. 2, Table S4). All compounds possess a low-energy absorption band at ca. 304 nm, which is assigned to hybrid π–π* and n–π* transitions due to a medium extinction coefficient up to 4·103 M− 1 cm− 1 (Table S3). Indeed, the theoretical calculations predict a mixed character for vertical transitions in the range of 318 to 330 nm (Table S6). The optical gap (Eopt−gap) values for all NON materials were calculated from the red-onset of the lowest energy absorption band: 3.72 eV for NON, 3.86 eV for NON-Br and 3.90 eV for NON-CF3. All absorption bands demonstrate very little solvatochromic effect, as shown in Fig. 2b for the compound NON-CF3 (see Supporting Files, Figures S13–S15 for all compounds). This indicates only a minor change in the dipole moment upon vertical excitation from the ground S0 to excited S1 states and is reflected in the TD-DFT theoretical calculations (Fig. 2c, Table S5).
All NON compounds exhibit featureless and narrow near-UV fluorescence with a full width at half maximum (FWHM) of 3400 cm–1 (40 nm) in MeTHF solution or Zeonex films at 295 K (Fig. 3 red line, S16–S21). The electron withdrawing substituents in the indoline moieties lead to a blue shift in emission from 338 nm for NON to 310 and 315 nm for NON-CF3 and NON-Br, respectively. This observation is corroborated by theoretical calculations that show the HOMO is localised over the indoline moieties. Therefore, increasing the electron-withdrawing strength of the substituents attached to the indoline moiety results in the stabilization of the HOMO energy level and an increase in the emission energy. The photoluminescence quantum yields (PLQY) for UV-luminescence increase from NON-Br (3%) to NON-CF3 (12%) to NON (23%) in MeTHF solution at 295 K.
All NON materials, in all media, exhibit an excited state lifetime on the nanosecond time scale in the range of 0.9–1.8 ns, which is typical for the fluorescence emission mechanism. Figure 3 depicts the emission profiles of the NON compounds in frozen MeTHF glasses at 77 K (black line, Table 2). The emission spectra of NON at 77K is dominated by a deep-blue and vibronically resolved phosphorescence, peaking at 400 nm. The excited state lifetime is too long to be measured by a gated Xenon flashlamp. However, the emission was observed with the naked eye to persist for more than 3 s after the excitation ceased. Unlike NON, the emission spectra of NON-CF3 and NON-Br compounds are dominated by UV-fluorescence (306–337 nm), with a minor contribution from the deep-blue phosphorescence component at 77 K (Fig. 3b,c). Similar to NON, the excited state lifetime of the phosphorescence is longer than 3 s, while the fluorescence excited state lifetime only slightly increases up to 5.9 ns upon cooling.
The energy levels of the singlet (S1) and triplet (T1) excited states for all NON-materials were deduced from the blue-onsets of the fluorescent and phosphorescent profiles (Fig. 3, Table 1) at 77 K. The NON and NON-CF3 materials exhibit a high triplet energy level at 3.3 eV, which is higher than the most popular host material DPEPO (3.0 eV) and on par with the most stable deep-blue OLED host material – PPBi (3.3 eV). The computed values align well with the experimental results (Table S6). The theoretical calculations show that both frontier orbitals, HOMO and LUMO, are primarily localized over the indoline rings of the NON compounds (Table S4), resulting in a large frontier orbital overlap integral (0.62–0.66) for all NON materials (Table S4). This is largely due to the absence of spatially separated donor and acceptor moieties, which results in a significant stabilization of the T1 energy level and an energy difference with the singlet excited state, ΔEST, up to 1.15 eV. Note that the central oxadiazine core with spiro-sp3 carbon atoms acts as an insulator, preventing extended conjugation between two indoline moieties for the NON-materials, which prevents further lowering of the T1 energy level.
Table 1
Cyclic Voltammetry and Additional Photophysical Parameters
| Oxidation | EHOMO | ELUMO | Eopt−gap | λabs (nm), | S1 | T1 | OH/Lc |
E1st | Eonset ox | E2nd | eV | eV | eV | (ε 103 M− 1 cm− 1) | eVb | eVb | |
NON | + 0.50 | + 0.37 | – | –5.76 | –1.90 | 3.86 | 264 (28), 294 (10.5), 304 (sh) | 3.91 | 3.35 | 0.62 |
NON-CF3 | + 0.90 (100) | + 0.75 | + 1.38 | –6.14 | –2.24 | 3.9 | 273 (21.2), 302 (sh) | 4.36 | 3.31 | 0.66 |
NON-Br | + 0.62 (90) | + 0.51 | + 1.12 | –5.90 | –2.21 | 3.69 | 270 (15.7), 304 (4.1) | 4.36 | 3.21 | 0.62 |
a In 1,2-difluorobenzene (DFB) solution, recorded using a glassy carbon electrode, concentration 1.4 mM, supporting electrolyte [nBu4N][PF6] (0.13 M), measured at 0.1 V s–1. ELUMO = Eopt gap – EHOMO eV; b S1 and T1 energy levels based on the onset values of the emission spectra blue edge in MeTHF glasses at 77 K and 298 K; c OH/L is an overlap integral between HOMO and LUMO calculated by DFT. |
Table 2
Photophysical properties of the NON-materials in MeTHF solution and 1% Zeonex matrix at 298 and 77K
| 298 K | | | kr | knr | 77K | |
| λmax (nm) | t (ns) | Φ (%, N2)a | (108 s− 1)b | (108 s− 1)c | λmax (nm) | t |
MeTHF solution |
NON | 338 | 1.4 | 23 | 1.7 | 5.5 | 337 400 | 2.6 ns > 3s |
NON-CF3 | 310 | 0.9d | 12 | 1.4 | 10 | 302 400 | 5.9 ns > 3s |
NON-Br | 315 | 1.1d | – | – | – | 302 393 | – > 3s |
1% Zeonex matrix |
NON | 336 | 1.8 | 21 | 1.2 | 4.4 | – | – |
NON-CF3 | 306 | 0.9d | 10 | 1.2 | 10 | – | – |
NON-Br | 350 | 1.1d | 3 | 0.27 | 8.7 | – | – |
a Quantum yields determined using an integrating sphere; b radiative constant kr = Φ/ t; c nonradiative constant knr = (1 – Φ)/ t. d In case of two-component lifetime t an average was used: t av =(B1/( B1 + B2))t1 + (B2/( B1 + B2))t2, where B1 and B2 are the relative amplitudes for t1 and t2, respectively. |
Device fabrication, characterisation, and performance. We assessed all NON-materials against the criteria outlined in the introduction to identify a promising host material for the development of deep-blue OLED devices. The NON-CF3 material exhibits good thermal stability, a wide energy gap (3.9 eV) thanks to a well-stabilised HOMO (–6.1 eV) and a destabilised LUMO (–2.2 eV), a high triplet energy level of 3.3 eV, and excellent volatility during the sublimation process due to three cyclohexyl groups. These attributes motivated us to test the NON-CF3 material as a host with our recently developed Carbene-Metal-Amide (CMA) TADF material P170 (Fig. 4a).30 OLED devices were fabricated via thermal vapour deposition. The device architecture is shown in Fig. 4, along with the chemical structures of the materials used. The 30 nm layer of 1,1,-bis{4-[N,N-di(4-toyl)amino]phenyl}cyclohexane (TAPC) and a 10 nm layer of 9,9′-biphenyl-2,2′-diylbis-9H-carbazole (o-CBP) function as hole transport layers. In each device, the 20 nm thick emissive layer (EML) consists of an emitting material doped at 10% by weight into the NON-CF3 host. A 45 nm layer of diphenyl-4-triphenylsilyl-phenylphosphine oxide (TSPO1) is used for electron transport. Four EML compositions were prepared using four different host materials, namely PPBi, TCP, mCP and NON-CF3 (Fig. 4a), to evaluate and compare the performance of NON-CF3.
The electroluminescence spectra for devices at 6 V are shown in Fig. 4, and a summary of the performance data for each device is given in Table 3. The use of NON-CF3 as a host material results in a blue shift of up to 31 nm for the electroluminescence from P170 compared to the other host materials tested. This leads to a highly desirable 448 nm EL from P171 with a narrow FWHM of ca. 60 nm in a NON-CF3 host. This result is favourable when comparing NON-CF3 to the DPEPO host, where the deep-blue OLED (EML: P170 10% in DPEPO) demonstrated a 30 nm wider FWHM value (ca. 90 nm).30 Therefore, a commonly cited disadvantage of organometallic TADF materials, such as their broad EL emission profiles associated with the emission occurring from a charge transfer (CT) state, could be circumvented by using the NON-CF3 host material. This enables narrow EL profiles and better CIE-colour coordinates.
Devices utilizing NON-CF3 exhibit an increased turn-on voltage, which is reported as the applied bias for luminescence to equal 1 cd m–2. This suggests a higher barrier for charge injection into the emitting layer. Figure 4 shows the current density–voltage–luminescence (J–V–L) curves for each OLED device. Devices experience luminescence roll-off when operating above 11 V, indicating a need for further improvement in the molecular design of the NON-host materials. However, the OLED devices hosted by NON-CF3 achieved an External Quantum Efficiency EQEmax value of 21.0%, the highest value among all tested host materials. Impressively, OLED devices containing P170 doped into NON-CF3 were operational at 100 cd m− 2 with an EQE of 9.2%, which is comparable to commercially available host materials such as TCP and mCP tested in this work. These findings suggest a high potential for NON-host materials to be used as host materials for deep-blue OLEDs.
Table 3
Performance data of evaporated OLEDs
OLED | Host | Von a) (V) | EQEMax (%) | EQE100b) (%) | λmax (nm) |
Au1 | 1 PPBi | 3.4 | 17.7 | 16.9 | 457 |
| 2 TCP | 3.5 | 12.3 | 9.9 | 479 |
| 3 mCP | 3.5 | 10.8 | 10.2 | 461 |
| 4 NON-CF3 | 4.2 | 21.0 | 9.2 | 448 |
a) Von at 0.1 cd m− 2; b) EQE at 100 cd m− 2 |