Stephanie
Montanaro
a,
Alexander J.
Gillett
b,
Sascha
Feldmann
b,
Emrys W.
Evans
b,
Felix
Plasser
a,
Richard H.
Friend
*b and
Iain A.
Wright
*a
aDepartment of Chemistry, Loughborough University, Loughborough, Leicestershire LE11 3TU, UK. E-mail: i.a.wright@lboro.ac.uk
bOptoelectronics Group, Cavendish Laboratory, University of Cambridge, Cambridge, CB3 0HE, UK. E-mail: rhf10@cam.ac.uk
First published on 6th May 2019
Employing the thiophene based quinone, benzo[1,2-b:4,5-b′]dithiophene-4,8-dione, as the electron-accepting moiety alongside N-phenylcarbazole donors to produce a donor–π–acceptor–π–donor (D–π–A–π–D) molecule has yielded a new red emitter displaying delayed fluorescence. This new molecule shows strongly (over 100 nm) red-shifted emission when compared to an anthraquinone based analogue. Cyclic voltammetry complemented by computational insights prove that this red-shift is due to the significantly stronger electron-accepting ability of the thiophene quinone compared to anthraquinone. Photophysical and computational studies of this molecule have revealed that while the presence of the thiophene containing acceptor facilitates rapid intersystem crossing which is comparable to anthraquinone analogues, the reverse intersystem crossing rate is slow and non-radiative decay is rapid which we can attribute to low-lying locally excited states. This limits the total photoluminescence quantum efficiency to less than 10% in both solution and the solid state. These results provide a useful example of how very minor structural variations can have a defining impact on the photophysical properties of new molecular materials.
Efficient red thermally activated delayed fluorescence (TADF) is challenging due to the difficulty in simultaneously obtaining both a narrow singlet–triplet gap (ΔEST) and a high fluorescence rate constant, and in overcoming the energy gap law which predicts that as the energy gap between the ground and excited states decreases, the rate of non-radiative decay (NRD) will increase.25–28 Anthraquinone has been employed in some of the most efficient red TADF materials29,30 however, electrochemical studies indicate that the thiophene containing analogue benzo[1,2-b:4,5-b′]dithiophene-4,8-dione has a significantly deeper LUMO energy (ca. 0.39 V) than anthraquinone1,31 which should give rise to red shifted optical properties. The introduction of heavy sulfur atoms may also have an impact on photophysical properties.
Therefore with the aim of producing deeper red emission arising from delayed fluorescence we decided to employ this moiety between two 3,6-di-tert-butyl-9H-carbazole electron donors separated with 1,4-phenylene spacers to produce a D–π–A–π–D type system. Here we present the synthesis and electrochemical and photophysical properties of this new molecule 1 alongside theoretical insights and some comparison with the analogous anthraquinone based molecule 2 (Scheme 1).29
Thermal gravimetric analysis (TGA) demonstrated the very high thermal stability of 1 (Fig. S1, ESI†) which displayed an initial 2% weight drop at 133 °C arising from the loss of residual solvent of crystallisation then no further changes until total decomposition shown by a 95% weight loss at 442 °C. Prior to obtaining the TGA, we attempted to obtain a melting point and observed that the crystals display interesting solid state emission characteristics reminiscent of aggregation induced emission upon heating. As isolated, the crystals are non-emissive but when a sample of recrystallised 1 was heated to 300 °C in an open glass capillary it underwent a thermally irreversible colour change from purple to red and the crystals were now red luminescent under UV light. This seems to be related to the loss of the residual solvent as observed in the TGA measurement.
Density functional theory (DFT) was used to optimise the ground state structure of 1 in toluene and the frontier orbitals were calculated using ORCA35 employing the B3LYP functional and 6-31G* basis set (Fig. 1). This revealed the HOMO and HOMO−1 as nearly isoenergetic and residing almost exclusively over the separate 9-phenylcarbazole moieties. While the calculated bond length (1.415 Å) and dihedral angle (50°) of the carbazole–phenyl bond are almost identical to those calculated for 2 (1.412 Å and 50° respectively), the dihedral angle of the thiophene–phenyl bond is 24° and the bond length is 1.47 Å which is comparable to those observed experimentally in the X-ray molecular structure of 2-phenylthiophene36 and 12° more planar than the calculated anthraquinone–phenyl bond angle of 36° in 2. Despite the increased planarity across the electron accepting core, there is little orbital overlap between the HOMO and LUMO with the LUMO distributed solely over the central dithiophene-4,8-dione core although the LUMO+1 extends across both the core and the adjacent phenyl rings.
The molecule displays a quasi-reversible (ΔEp = 130 mV) single electron reduction of the acceptor at Ered = −1.15 V which is comparable to reported values for unsubstituted benzo[1,2-b:4,5-b′]dithiophene-4,8-dione1,2 and a carbazole based reversible oxidation at Eox = +0.74 V (ΔEp = 161 mV). The magnitude of the oxidative current is significantly larger (Ip = 4.69 μA vs. 2.83 μA) than that of the reduction. This implies that the wave is actually composed of two closely overlapping single electron oxidations of the two carbazole rings such that the individual waves cannot be resolved.37 This is supported by the near-degeneracy and minimal overlap between the HOMO and HOMO−1 predicted by the DFT. Similar behaviour has also been observed in A–D–D–A type systems based upon phenothiazine dimers bearing pendant 6-hexyl-2-phenylquinolines as acceptors38 and other π-bridged bis(triarylamine)39–41 and bis(carbazole)42,43 systems.
λ abs,max (nm) | λ em,max (nm) | E g (eV) | Φ (soln.) | Φ F (soln.) | Φ (film) | Φ F (film) | |
---|---|---|---|---|---|---|---|
a Optical energy gap calculated from the onset of the lowest energy absorbance. b Excitation wavelength λex = 520 nm. c Excitation wavelength λex = 420 nm. d 1 wt% 2 in CBP film. | |||||||
1 | 298, 355, 468 | 664b | 2.14 | 0.095b | 0.084b | 0.085b | 0.064b |
2 29 | 426 | 558c | 2.43 | 0.60c | 0.43c | 0.65d | 0.12d |
First examining the steady-state absorption and photoluminescence (PL) of 1 in Fig. 3, the molecule displays a low energy absorbance at 468 nm which is assigned to the computed S2 state (Table S1, ESI†) which is an intramolecular charge transfer state (ICT) between the carbazole donors and the LUMO on the dione acceptor. This ICT also corresponds to a red emission at 664 nm. We note a significant red-shift in the absorption maximum of the ICT band from 426 nm to 468 nm and a corresponding red-shift in the PL maximum from 558 nm to 664 nm when compared to 2.29 This effect can be directly attributed to the use of the stronger electron accepting benzo[1,2-b:4,5-b′]dithiophene-4,8-dione moiety, which leads to a significant drop in the position of the LUMO and a reduced optical band gap of 2.14 eV. However, the PL quantum efficiency (PLQE) of 1 was much lower than 2, displaying values of 9.5% for a 0.5 mg mL−1 solution in oxygen-free toluene and 8.4% in non-degassed toluene compared to 60% and 43% respectively for 2. A 2 wt% film of 1 doped in polystyrene and encapsulated in an N2 atmosphere displayed a total PLQE of only 8.5%.
To examine the reasons behind the low PLQE value, we first performed transient absorption (TA) spectroscopy on a film of 2 wt% 1 doped into polystyrene. In the short-time (100 fs–1.6 ns) TA (Fig. S2, ESI†), we observe the formation of two new photo induced absorption (PIA) bands: one at 575 nm and the other in the near-infrared (NIR) at 1000 nm. In this initial short time range, we do not observe any spectral evolution of the PIAs, but the band at 575 nm seems to decay marginally more quickly than the 1000 nm feature falling to approximately 70% of its original intensity, compared to 80% for the NIR PIA.
Turning to the long timescale TA (1 ns–400 μs) in Fig. 4, we again observe the same two bands as in the short timescale TA. Both bands display bi-exponential decay kinetics which is typical of TADF behaviour.44 This suggests an initial radiative or non-radiative loss of singlet excited states to the ground state alongside forward intersystem crossing (ISC) of the remaining singlet population to the triplet manifold, prior to the delayed decay of S1 states which have formed by repopulation through reverse intersystem crossing (rISC). The band at 575 nm shows an initial prompt decay, presumably due to relaxation from S1 to S0, which is more rapid than that of the 1000 nm band with over 50% of excited state species lost after approximately 10 ns. This is followed by the much slower delayed component. This assumes no significant change in oscillator strength between the species present at early and late timescales. The decay kinetics yielded time constants of τprompt = 6.6 ns, τdelayed = 13.6 μs and τprompt = 12.0 ns, τdelayed = 12.8 μs for the 560–580 nm and 940–980 nm regions, respectively. The position, rate of decay and diminished prompt component of the long wavelength PIA indicates that a significant proportion of the species responsible for this band undergo ISC much faster than decay to S0. Therefore it may be assigned primarily to excitation of T1 to higher triplet states. An alternative explanation for discrepancies in the decay rates for the two PIAs could be the presence of multiple conformers with different intrinsic decay and ISC rates, as has been previously observed in organic D–A–D type TADF compounds.45,46 Considering these results, we suggest that the PIA at 575 nm is responsible for the majority of the prompt fluorescence.
When observing the ns–ms transient PL (trPL) of 1, a new PL band in addition to the primary ICT emission is observed at 520 nm that decays with a time constant shorter that the instrument response of our setup of ∼2 ns (Fig. 5). Similar high energy bands have been observed for a number of TADF systems and typically arise from the presence of different molecular conformations.47–49 Ultrafast transient grating PL studies on the film with an excitation wavelength of 400 nm reveal that this emission is present from the earliest timescales detectable of 200 fs and is almost completely decayed by 1 ns (Fig. S3, ESI†). Interestingly, this band is visible in the steady-state PL of the film when excited at 405 nm, but not when the excitation wavelength is 520 nm (Fig. S4, ESI†). Tellingly, this band is also not visible in the steady-state PL of 1 in a toluene solution when excited at 405 nm (Fig. S5, ESI†), ruling out emission from a high energy local excited singlet state. We know that in the solid-state, many different rotational conformers can exist in tandem, locked-in by the high energetic barrier to rotation.45 This is in contrast to solution, where the additional rotational freedom lowers this barrier and allows for the rapid interconversion between conformers, leading to an equilibrium between states that strongly favours the lower energy conformers. Important to note is that each of these stable conformers possesses their own distinct band gap,50 leading to the presence of many different species with unique band gaps in the film. Therefore, we assign this short-lived green PL to the emission from higher energy conformers, only excited by the blue pump photons. The short, sub-ns lifetime of this emission is due to rapid energy transfer from these conformers to their lower band gap neighbours in the film, which quenches the green emission.
Focussing on the primary ICT emission, we track the kinetics from the emission peak between 640–660 nm and integrate the resulting trace (Fig. 6). From this, we determine that 98% of the total PL emission occurs within the first 40 ns. The trPL decay kinetics are not readily fitted by a simple bi-exponential decay, likely due to the convolution of decays from multiple conformers. But the timescales for the decay processes appear to be broadly in-line with those observed in the TA. By combining this information with the insight gained from the TA, it is immediately apparent why the PLQE of 1 is relatively low: a significant proportion of the excited states that enter the triplet manifold do not undergo rISC and ultimately decay non-radiatively.
Revisiting the PL and TA results for the doped film and focussing on the band at 575 nm, calculation of the rate constant for: (i) the prompt radiative decay of the singlet states, kSr = 9.73 × 106 s−1; (ii) intersystem crossing, kISC = 1.42 × 108 s−1; (iii) reverse intersystem crossing, kRISC = 2.58 × 104 s−1; (iv) the non-radiative decay of the triplet state kTnr = 7.18 × 104 s−1,51,52 (using eqn (S1)–(S4), ESI†) indicates that non-radiative decay of the triplet state is occurring significantly more rapidly than any rISC. Similar calculations performed after photophysical studies of a molecule related to 2 (doped into zeonex at 2 wt%) which features an anthraquinone core bearing diphenylamine donors,46 revealed that the kSr of 1 is an order of magnitude slower while the kRISC of 1 was two orders of magnitude slower. Conversely, the kTnr of 1 is faster. The calculated values for kISC are comparable.
While, in accordance with the energy gap law, we may expect the rate of NRD to increase with decreasing emission energy, the use of the thiophene acceptor has resulted in an 85% decrease in PLQE when comparing 1 and 2 which seems particularly stark. While conformational relaxation of T1 can facilitate non-radiative decay46 another possible explanation for both the drop in kSr and the acceleration of kTnr is that strong spin–orbit coupling from the heavy sulfur atoms facilitates efficient ISC before low lying triplet states of the thiophene rings mediate NRD from T1 to S0.53–55 Revisiting our computational results we performed time-dependent DFT experiments to obtain a deeper picture of the electronic structure of the molecule. The results of the calculations (Table S1, ESI†) showed a good agreement with our experimental results. A computed ΔEST of 0.54 eV was obtained while the calculations also revealed that the T1 state of 1 is a low-energy local excitation on the benzodithiophene unit located at 1.95 eV, which is 0.77 eV lower than the bright S2 state. In total there are four triplet and one singlet state below S2 and we suggest that this high density of dark low energy states is severely inhibiting rISC and therefore limiting delayed fluorescence.
Footnote |
† Electronic supplementary information (ESI) available: Synthesis and characterisation of 1 and the experimental details for the computational, electrochemical and photophysical studies. See DOI: 10.1039/c9cp02186h |
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