Purificación
Cañadas
a,
Michele
Forzatti
b,
Sara
Fuertes
*a,
Antonio
Martín
a,
Michele
Sessolo
b,
Daniel
Tordera
*b and
Violeta
Sicilia
*c
aDepartamento de Química Inorgánica, Facultad de Ciencias, Instituto de Síntesis Química y Catálisis Homogénea (ISQCH), CSIC – Universidad de Zaragoza, Pedro Cerbuna 12, 50009, Zaragoza, Spain. E-mail: s.fuertes@csic.es
bInstituto de Ciencia Molecular, Universidad de Valencia, C/Catedrático J. Beltrán 2, 46980, Paterna, Spain. E-mail: daniel.tordera@uv.es
cDepartamento de Química Inorgánica, Escuela de Ingeniería y Arquitectura de Zaragoza, Instituto de Síntesis Química y Catálisis Homogénea (ISQCH), CSIC – Universidad de Zaragoza, Campus Río Ebro, Edificio Torres Quevedo, 50018, Zaragoza, Spain. E-mail: sicilia@unizar.es
First published on 4th July 2025
A set of neutral platinum(II) complexes bearing a bis-N-heterocyclic carbene (NHC) pincer ligand with stoichiometry [Pt(CR*^CCN^CR*)L] (R = Me (a), Et (b); L = Cl (2), Cbz (3), and CN (4)) have been prepared. By employing the corresponding bisimidazolium salt (1a or 1b), silver oxide and [PtCl2(cod)] we obtained the Cl derivatives. Then, the subsequent ancillary ligand exchange rendered complexes 3 and 4. Single-crystal X-ray analysis revealed no Pt–Pt contacts, but some π–π intermolecular interactions within the supramolecular structure of the Cl and CN derivatives. It also showed different crystal packings for the two polymorphs of the Cl complex (2b). In diluted solution, photophysical and computational studies disclosed the nature of the low-lying electronic transitions to be mainly 3ILCT [π(C*^C^C*) → π*(C*^C^C*)]/3MLCT [5d(Pt) → π*(C*^C^C*)] for Cl and CN derivatives and L′LCT [π(Cbz) → π*(C*^C^C*)]/L′MCT [π(Cbz) → d(Pt)] for the Cbz counterpart. The blue (2b), green (3b) and yellowish-orange (4b) emissions of 2 wt% PMMA films at λex = 370 nm exhibited very high quantum yields (QYs) reaching up to ∼99%. However, at λex > 400 nm, in the solid state or in 20 wt% PMMA films, additional structureless low-energy emissions arose from extended structures with a higher degree of aggregation. Complexes 2b–4b were used as emitters in organic light-emitting diodes (OLEDs), either with a doped or a non-doped emissive layer. Interestingly, and due to their aggregation in extended structures, their emission could be tuned from bluish green to orange just by changing the thickness of the active layers. Devices with 4b reached a maximum efficiency of 8.08% and a high luminance of 34071 cd m−2.
In the chemistry of Pt(II), molecular design, mainly of the chromophoric ligand, plays a key role in the development of efficient and stable phosphorescent complexes.4,5 In this sense, bidentate and tridentate cyclometalated N-heterocyclic carbenes (C^C* and C*^C^C*)4,6 induce a large HOMO–LUMO gap, at least of 2.8 eV required for blue emitters. Besides, their strong field nature, which pushes up the dd* states, and their rigidity, which hinders severe geometrical distortions of the complexes upon excitation, preclude nonradiative deactivation and bond-breaking processes. Therefore, Pt(C^C*) and Pt(C*^C^C*) are excellent platforms to get blue phosphorescent complexes. However, it requires the presence of strong electron-withdrawing substituents in the aromatic fragment involved in the HOMO.6 Otherwise, the emission shifts to the sky-blue or green spectral range. Additionally, these planar complexes with extended π-systems tend to establish π–π and/or Pt⋯Pt interactions with adjacent molecules in the solid state or even dispersed in films at high wt%. This happens in the absence of bulky substituents that hinder excimer/aggregate formation,7 and in these cases, the emission shifts to lower energies, appearing in the yellow, orange or red spectral range.4 Driven by the stability of this class of compounds and their photoluminescence color tunability, some of them have been used as active materials in the EML of PhOLEDs.
In this sense we recently published OLEDs based on the compounds [Pt(Cbz-C^C*bzim/im)(L^L)] (HC^C*im = 1-(4-(9H-carbazol-9-yl)phenyl)-3-methyl-1H-imidazol-2-ylidene, HC^C*bzim = 1-(4-(9H-carbazol-9-yl)phenyl)-3-methyl-1H-benzimidazol-2-ylidene; L^L acetylacetonate, 2-diphenylphosphinobenzoate, 2-diphenylphosphinophenolate). The best performing devices were obtained for [Pt(Cbz-C^C*bzim)(acac)] and [Pt(Cbz-C^C*bzim)(2-diphenylphosphinobenzoate)] in ultrathin non-doped emissive layers. They showed green EL derived from aggregates with a turn-on voltage of 2.99 V and 2.55 V, a peak luminance of 39208 and 25
837 cd m−2 and a peak current efficiency of 44.9 and 40.0 cd A−1 (12.8% and 13.4% EQE), respectively.8 A revision of complexes tested in OLEDs containing a Pt(C^C*) system is included there.8 Complexes used in PhOLEDs containing Pt(C*^C^C*) chromophores are represented in Fig. 1.
Li, Fleetham et al. reported the first complex bearing a pincer C*^C^C* fragment used as an active material in PhOLEDs, CCC1. It yielded pure-blue EL (CIE coordinates: 0.16, 0.13) and good performance, reaching an EQEmax of 15.7%.9 The same group used CCC1 as a single dopant to get white light (CIE coordinates: 0.33, 0.33) combining the emission from monomers and excimers, reaching an EQEmax of 18.2% at 10 wt%.10 Blue EL was also achieved by C. M. Che et al. using CCC2 (CIExy: 0.14, 0.23) and CCC3 (CIExy: 0.15, 0.11) with improved performances: EQEmax 19.9% and 22% respectively.11CCC4 has been recently reported by Zhu, Lee and co-workers, and was employed as a dopant sensitizer for a narrow band MR-TADF terminal emitter: ν-DABNA. Using this strategy, they obtained hyperphosphorescent pure-blue OLEDs with EQEs of up to 33.59%, and CIExy of (0.12, 0.15).12 Finally, with CCC5 Bräse, Wang et al. were able to tune the emission of monomers and excimers to get single-doped WOLEDs with CIE coordinates of (0.32, 0.36), a color rendering index (CRI) of over 83, and an EQEmax of 24.4%.13
Keeping in mind all of the above and our previous contribution to blue/green-emitting Pt(II) complexes bearing bidentate cyclometalated NHCs,14 we decided to address the synthesis of a new functionalized pincer ligand with an electron-withdrawing pendant group (CN) in the aryl ring. Several Pt(II) complexes derived from it have been prepared and fully characterized. The study of their photophysical properties with the aid of DFT and TD-DFT calculations was addressed before their use as active materials in PhOLEDs.
The 4JPt,HPh is also sensitive to the ancillary ligand (Table 1), becoming smaller as its trans influence became greater (Cl− < Cbz− < CN−). It is also worth noting the important upfield shift undergone by the resonances of the Me and Et groups on the imidazole fragments in complexes 3a/3b. This effect has been associated with the anisotropic shielding effect caused by the proximity in space of the aromatic ring current of the Cbz to them.18 Regarding the 13C{1H} NMR spectra, the CNHC (hereafter referred to as C*) resonances appear at δ > 170 ppm with 195Pt coupling constants of 1130–1176 Hz, in agreement with the existence of a σ Pt–C* bond.
δPt{1H} | 4 J Pt,HPh | δMe(im) | δEt(im) | δC* | 1 J Pt–C* | |
---|---|---|---|---|---|---|
a DMSO-d6. b CD2Cl2. c 1 J Pt–C* were determined using 1H–13C HMBC. | ||||||
1a | 4.01 | |||||
1b | 4.35, 1.55 | |||||
2a | −3998 | 16.4 | 4.14 | 171.8 | 1152.2 | |
2b | −4013 | 16.8 | 4.76, 1.50 | 173.2 | 1140.3 | |
3a | −4119 | 12.6 | 2.86 | 174.8 | 1165.0 | |
3b | −4107 | 12.6 | 3.20, 0.60 | 173.0 | 1176.2 | |
4b | −4553 | 10.6 | 4.62, 1.55 | 171.1 | 1130.1 |
The proposed structures on the basis of the NMR data were confirmed via X-ray diffraction analysis of 2b, 3b and 4b (Fig. 2 and Fig. S10, ESI†). Crystals of 2b were obtained in two polymorphic forms by slow diffusion of methanol into a saturated solution of DMF (2b and 2b·H2O). The asymmetric unit of 3b contains two molecules (Pt1 and Pt2) with similar structural details. Selected bond lengths and angles are summarized in Table 2. In these complexes, the PtII center exhibits a distorted square-planar coordination environment, with C*–Pt–C* angles of ∼157°. These angles and the Pt–C bond lengths are very similar to those observed in other PtII complexes bearing dicarbene pincer ligands.11,12,17,19 In 3b, the plane of the carbazolyl ligand is almost perpendicular to that of the molecular plane (Pt1, C1, C6, C13, N6/Pt2 C42 C35 C30 N12) with a dihedral angle of 84.55(14)°/83.77(15)° to minimize the steric repulsions. Further inspection of the crystal packing of all complexes revealed that there are no Pt–Pt contacts; but some π–π (ca. 3.49, 3.43 Å) and Pt–π offset interactions in 2b·H2O and 4b·H2O. In them, the molecules stack into 1D-staggered chains (see cyan dotted lines in Fig. 2b for 2b·H2O and Fig. S10 for 4b·H2O, ESI†). Both crystal packings show the same type of lone pair dz2[MII]–π interactions,12,20,21 with the Pt center pointing to the imidazole ring and located at the distance of 3.46 Å (2b·H2O) and 3.44 Å (4b·H2O), which is slightly smaller than the sum of the van der Waals radii (RvdW(Pt) + RvdW(C) = 3.47 Å).22,23 The extended structure is almost identical in both and is also supported by a crystallization water molecule that bridges neighboring Pt complexes (black dotted lines) via hydrogen bonding interactions with the ancillary ligand (d CN⋯O: 2.930(2) Å 4b·H2O, d Cl⋯O: 3.178(2) Å 2b·H2O) and via Csp2–H⋯O interactions with the C*^C^C* group (d C⋯O: 3.296(5) Å 4b·H2O, 3.273(4) Å 2b·H2O). However, in 2b, the Pt molecules do not stack into infinite 1D-chains; they arrange in pairs, in a head to tail fashion, through π–π interactions (ca. 3.331 Å, Fig. 2d).
2b L = Cl | 2b·H2O L = Cl | 3b (Pt1/Pt2) L = NCbz | 4b·H2O L = CCN | |
---|---|---|---|---|
Bond lengths (Å) | ||||
Pt–C* | 2.037(2) | 2.038(3) | 2.011(7)/2.028(6) | 2.029(4) |
2.028(2) | 2.030(6)/2.037(6) | |||
Pt–Cph | 1.938(2) | 1.961(6) | 1.956(6)/1.947(6) | 1.992(4) |
Pt–L | 2.3857(5) | 2.4057(13) | 2.100(5)/2.089(5) | 2.018(4) |
C–N | 1.151(3) | 1.157(7) | 1.150(9)/1.511(10) | 1.137(6) |
C11–N4 | 1.154(6) | |||
Bond angles (°) | ||||
C*–Pt–Cph | 78.99(8) | 78.89(10) | 79.4(2)/78.6(3) | 78.38(9) |
78.74(8) | 78.4(3)/79.1(2) | |||
C*–Pt–L | 100.20(6) | 101.11(10) | 100.4(2)/100.2(2) | 101.62(9) |
102.11(6) | 101.8(2)/102.0(2) | |||
C*–Pt–C* | 157.69(8) | 157.8(2) | 157.8(3)/157.7(3) | 156.76(18) |
To better understand their photophysical properties, density functional theory (DFT) and time dependent-DFT (TD-DFT) calculations were carried out at the M06/SDD(Pt)/6-31G*(ligand atom) level. The geometries of the S0 and T1 were optimized with no restrictions; see the Experimental section (ESI†) for further details. The frontier orbitals (FOs) involved in lowest energy absorptions have been represented in Fig. 4. As can be seen, in CH2Cl2, the calculated S1 transition is mainly a HOMO → LUMO one (Table S3, ESI†). The analysis of the frontier orbitals (Table S4, ESI†) revealed that for 2b and 4b, the HOMO is mainly centered on the C*^C^C* (≥50%) ligand and the platinum center (∼30%) and also on the Cl (15%) atom for complex 2b, while for 3b, the HOMO is essentially located on Cbz (91%). However, the LUMO is almost the same for all three complexes, with a great participation of the C*^C^C* (∼75%) and the Pt center (∼25%). Thus, the lowest energy absorption, S1, would be mostly attributed to a mixed ILCT/MLCT transition for 2b and 4b, whereas L′LCT [π(Cbz) → π*(C*^C^C*)]/L′MCT [π(Cbz) → d(Pt)] for 3b, confirming the early assignment made in the UV-Vis section. By comparing the calculated data corresponding to the Cl (2b) and CN (4b) complexes, they reveal that although the CN ancillary ligand does not formally contribute to the FOs, it stabilizes them due to its electron-accepting nature, causing a subtle change in the HOMO–LUMO gap with respect to that in the Cl complex. The Cbz group in 3b has a greater effect on the HOMO–LUMO gap; its good electron-donating ability fully changes the nature of the HOMO and increases its energy, while it does not modify the LUMO with respect to those of 2b and 4b, decreasing the HOMO–LUMO gap appreciably (Fig. 4).
Comp. | Medium | λ exc (nm) | λ em (nm) | τ (μs) [λem] | Φ (%) | k r × 105 (s−1) | k nr × 105 (s−1) | CIE (x, y) |
---|---|---|---|---|---|---|---|---|
a Measured at 5 × 10−5 M. b Measured at 5 × 10−4 M; kr = ΦPL/τ, knr = (1 − ΦPL)/τ. | ||||||||
2a | CH2Cl2a | 370 | 462max, 494, 525sh | 2.0 [462] | 21 | 1.05 | 3.95 | 0.17, 0.26 |
Solid | 520 | 700 | 0.5, 1.3 | 23 | 1.77 | 5.92 | 0.65, 0.34 | |
2b | CH2Cl2a | 370 | 463max, 495, 525sh | 2.3 [463] | 28 | 1.22 | 3.13 | 0.20, 0.27 |
2wt%PMMA | 370 | 464max, 494, 525sh | 6.1 [464] | 98 | 1.60 | 0.03 | 0.17, 0.26 | |
410 | 465, 494, 615max | 6.3, 1.7 [615] | 49 | 0.78 | 0.81 | 0.40, 0.35 | ||
20wt%PMMA | 370 | 464max, 494, 615 | 5.0, 1.8 [464] | 75 | 1.50 | 0.50 | 0.37, 0.35 | |
410 | 464, 494, 615max | 1.6 [615] | 55 | 3.43 | 2.81 | 0.51, 0.39 | ||
Solid | 470 | 620 | 0.6, 1.4 | 16 | 1.14 | 6.00 | 0.54, 0.43 | |
3b | CH2Cl2a | 370 | 590 | 0.8 | 30 | 3.75 | 8.75 | 0.52, 0.46 |
2wt%PMMA | 470 | 537 | 1.9 | 76 | 4.00 | 1.26 | 0.37, 0.60 | |
Solid | 500 | 575 | 0.8 | 33 | 4.12 | 8.37 | 0.49, 0.49 | |
4b | CH2Cl2a | 370 | 461max, 494, 525sh | 1.1 [461] | 10 | 0.91 | 8.18 | 0.20, 0.28 |
CH2Cl2b | 370 | 461max, 494, 525sh, 610 | 0.8 [610] | 14 | 1.75 | 10.75 | 0.40, 0.34 | |
2wt%PMMA | 370 | 461, 494, 600max | 1.5 [600] | 99 | 6.60 | 0.06 | 0.47, 0.41 | |
20wt%PMMA | 370 | 460, 494, 600max | 1.3 [600] | 75 | 5.77 | 1.92 | 0.53, 0.42 | |
480 | 600max, 680sh | 1.2, 0.3 [600] | 67 | 5.58 | 2.75 | 0.58, 0.41 | ||
Solid | 470 | 611 | 1.9, 0.6 | 66 | 3.47 | 1.79 | 0.58, 0.41 | |
550 | 695 | 2.6, 0.5 | 48 | 1.85 | 2.00 | 0.64, 0.35 |
All complexes 2a, 2b and 4b exhibit, in addition, an emerging low energy emission at λ > 600 nm. We observed that for 4b it becomes much more intense with increasing concentration (see Fig. S15, ESI†) and exhibits a monoexponential and shorter decay time than the high energy one. For 2b (Fig. S14, ESI†) and 4b the excitation spectra of the high and low-energy bands match one another and resemble their UV-vis spectra. Therefore, in all cases, an excimeric origin of the low-energy emission band can be presumed. The structured shape of the high-energy bands (λmax ∼ 460 nm) with vibrational spacing [1100–1400 cm−1] corresponding to CC/C
N stretching of the organic ligand suggests a pronounced 3IL nature of these emissions. Considering that in each case the excitation spectrum and the lower energy absorption match one another, the emission can be attributed to a mixed 3ILCT [π(C*^C^C*) → π*(C*^C^C*)]/3MLCT [5d(Pt) → π *(C*^C^C*)] excited state, in agreement with the emission lifetimes and the spin density distributions calculated for the T1 states. As shown in Fig. S17 (ESI†), these are mainly located on the C*^C^C* ligand (1.680 2b and 1.755 4b) and to a smaller extent on the Pt center (0.290 2b and 0.215 4b) and the ancillary ligands (0.030 2b and 0.030 4b). This contribution of the Pt orbitals could explain to some extent the small value of the emission decay (τ ∼ 2 μs). By contrast, the incorporation of the Cbz as an ancillary ligand (3b) results in a structureless emission band at 590 nm, clearly shifted to lower energy with respect to those for 2b and 4b. This fact is explained by the different nature of the lowest energy excited state, L′LCT [π(Cbz) → π*(C*^C^C*)]/L′MCT [π(Cbz) → d(Pt)], in accordance with calculated spin density distributions (Cbz: 0.860, C*^C^C*: 0.821, Pt: 0.319). In rigid media, especially in a 2 wt% PMMA film, the emission of 3b undergoes a clear hypsochromic shift (1672 cm−1, from 590 nm in solution to 537 nm in the film) and a significant narrowing of the full width at half maximum (FWHM) from 107 nm (3028 cm−1) in solution to 68 nm (2273 cm−1) in the film; along with an increase in the quantum yield and lifetime values (see Fig. 5b and Table 3). This luminescence rigidochromism is characteristic of the mixed charge transfer excited state,27–29 in accordance with a L′LCT/L′MCT assignment, in view of the match between excitation and absorption spectra.
The emission behaviour in rigid media of 2b and 4b, with non-bulky ancillary ligands, greatly differs from that of 3b, as observed before in solution. In PMMA films at low doping concentrations (2 wt%), 2b shows an emission whose profile depends on the excitation wavelength (see Fig. 6). When excited at λ ≤ 370 nm, 2b shows a vibronic band peak at 465 nm, similar to the one obtained in solution, together with an incipient low energy emission at λ > 600 nm. The latter becomes the maximum when λex > 400 nm at any doping concentration, 2 wt% or 20 wt% (Fig. S18, ESI†), and is the only emission band observed in the solid state (Fig. 7).
![]() | ||
Fig. 6 Normalized excitation (----) and emission (–) spectra of in 2 wt% PMMA film. Pictures of 2b (blue emitter film) and 4b (yellowish-orange emitter film) under 365 nm light. |
As previously discussed, the blue vibronic emission resembles that measured in solution, but reaches higher quantum yield (>90%), microsecond lifetimes and high radiative constants (>105 s−1, see Table 3); thus we assume the same origin (3ILCT [π(C*^C^C*) → π*(C*^C^C*)]/3MLCT [5d(Pt) → π *(C*^C^C*)]). However, the Gaussian shaped low-energy emission is probably due to existing aggregates in the ground state, in view of the different excitation spectra obtained for the high and low energy bands. The planarity of this molecule and its extended π system are responsible for the tendency to form aggregate structures involving Pt–Pt and π–π intermolecular interactions,30 even at low Pt complex loadings, like in analogous complexes [Pt(CNHC^CAr^CNHC)L] (L = Cl, CN).11,12 As a result, in 2b the emission color can be modified from blue to white (neutral and warm) and up to orange, by changing the doping concentration in PMMA films or the excitation wavelength, as illustrated by the chromaticity diagram shown in Fig. S19 (ESI†). It is worth noting that compound 2b can provide white photoluminescence (Table S5, ESI†) with high QY, correlated color temperatures (CCT) ranging from 1990 to 4159 K, acceptable color rendering index (CRI) values of 78–67 and CIE coordinates close to the Planckian locus (|Duv| ≤ 0.006, 20 wt%, Table S5, ESI†). Hence, these photometric and colorimetric parameters are fairly close to the values reported for single-doped WOLEDs based on square-planar Pt(II) complexes,13,31–35 and comply with the stipulated values for indoor solid-state illumination.36,37
For 4b in PMMA films, at any doping concentration (2 wt%, 20 wt%), the emission at λmax ∼ 600 nm, due to aggregates, is the most important or the only one, when exciting at wavelengths > 400 nm (Fig. 6 and Fig. S20, ESI†). In the solid state, the emission profile of 4b depends on the excitation wavelength (Fig. 7). In this case, upon excitation with λex > 500 nm, an additional and new structureless emission band appears at λem = 695 nm. This can be attributed to heterogeneity in the solid and the formation of higher degree aggregates, in view of the different packing arrangement possibilities observed for these kinds of complexes. In fact, both excitation and emission spectra are comparable to those obtained for 2a, with a methyl substituent in the imidazole fragments (Fig. 7). Thus, compounds 4b and 2a present a great tendency to form aggregates involving close and extended Pt⋯Pt/π⋯π interactions.
The selected device architecture was ITO (150 nm)/PEDOT:PSS (35 nm)/TAPC (20 nm)/mCP (10 nm)/Pt(II) complex/PO-T2T (45 nm)/Ba (3 nm)/Ag (100 nm). PEDOT:PSS (poly(ethylenedioxythiophene):poly(styrenesulfonate)), TAPC (1,1-bis[(di-4-tolylamino)phenyl]cyclohexane), mCP (1,3-bis(N-carbazolyl)benzene), and PO-T2T (2,4,6-tris[3-(diphenylphosphinyl)phenyl]-1,3,5-triazine) were employed as the hole-injection, hole-transport, exciton-blocking, and electron-transport materials, respectively. Ba and Ag were used for the electron injection layer and the cathode, respectively. All layers, except for PEDOT:PSS, were deposited through thermal evaporation (for further details, refer to the Experimental section, ESI†). The transport layers were selected according to their compatible energy levels with the studied emitters (Fig. S21a and b, ESI†). The frontier orbital energies of the emitters were measured by means of photoelectron spectroscopy (PESA) in air (Fig. S22a–c and Table S6, ESI†). The emissive layer (EML) consisted of a non-doped layer of either 2b or 4b. To probe the effect of the dispersion level on the emission properties of the emitters, 6 different thickness values were studied, namely 3 nm, 1 nm, 0.3 nm, 0.1 nm, 0.03 nm and 0.01 nm. It is important to note that at these thickness ranges, the molecules stop forming a neat continuous layer but are rather dispersed on the layer underneath: the lower the nominal thickness, the lower the amount of emitter molecules being deposited and the higher the average intermolecular distance.39 The stability of the active materials under 315 °C was initially checked by TGA analysis. It was also proved under vacuum deposition conditions (heating up to 250 degrees at a base pressure of 10−6 mbar) since comparison of the NMR spectrum of the remaining powder with the reference confirmed no sign of degradation (see Fig. S23, ESI†).
Emission from OLEDs with 2b was observed regardless of the EML thickness. However, both the turn-on voltage (that is, the voltage value at which the emission starts, reported here at a luminance of 1 cd m−2) and the color varied significantly across devices with different thickness values. For instance, for values in the range 0.01–0.3 nm the devices only turn on past 3 V and have a bluish-green color (Fig. S24, ESI†). The devices with an EML thickness of 1 nm turned on at 2.8 V and showed green color, while those with an EML of 3 nm turned on already starting from 2.2 V and appeared yellow. Despite these differences in color, the electroluminescence (EL) spectra of all devices could be described as a combination of the same 4 peaks (Fig. 8a). The highest energy peak is centered at 470 nm and is analogous to the high energy emission visible in the PL spectrum of the compound when measured in either CH2Cl2 or PMMA. However, unlike what is observed in the PL, here it is never the most intense peak. While it is clearly visible for thickness values in the range 0.01–0.3 nm, its intensity decreases significantly for higher thicknesses (1 nm) and completely disappears at 3 nm (Fig. S25, ESI†). The second peak is centered at 501 nm and is the most intense peak for thicknesses in the range of 0.01–0.3 nm. The peak is also visible for the 1 nm devices (albeit only as a shoulder to the lower energy peak) and is, once again, absent for 3 nm. The third peak is centered at around 530 nm, but in the range 0.01–0.3 nm, it is only present as a shoulder to the main 501 nm emission. Interestingly, this shoulder is most intense for 0.01 nm, even though it also partially depends on the applied voltage (as this peak tends to become weaker as the voltage is raised, Fig. S26, ESI†). These first three peaks are also all visible in the PL spectrum of 2b, with the same vibrational spacing, but all red-shifted by exactly 5 nm in the EL spectrum. The fourth and final peak is only visible for the highest thickness values (1 and 3 nm), even though its presence is noticeable also for 0.3 nm, and red shifts with increasing thickness. In fact, it is centered at 544 nm for 1 nm and 561 nm for 3 nm. This incipient low energy emission is analogous to that observed in the PL spectrum of the compound in rigid media at high doping concentrations or in the solid state.
As was previously discussed, this emission is expected to come from extended structures involving Pt–Pt and π–π intermolecular interactions, whose abundance increases as the thickness of the non-doped layer surpasses 1 nm where the higher density of molecules on the ultrathin active layer promotes these types of interactions. Hence, the color change across the devices can be attributed to variations in the relative peak intensity and to the shift of the lowest energy peak and is more rigorously quantified in the International Commission on Illumination (CIE) chromaticity diagram (Fig. 8b). Next, the J–V–L characteristics of the devices were measured and are illustrated in Fig. 8c. They show that the maximum brightness increases with increasing thickness, surpassing 30000 cd m−2 in the devices with an EML of thicker than 0.3 nm. The efficiency, on the other hand, only increases with thickness up to 0.1 nm (Fig. 8d), where a peak efficiency of 16.3 cd A−1 is reached (corresponding to an external quantum efficiency, EQE, of 6.44%), before starting to decrease again. This trend could be related to the efficiency of the energy transfer from the exciplexes formed by the surrounding layer to the emitter molecules, to the intrinsic emission efficiency of the different predominant species involved for the different dispersion levels and to concentration-related exciton quenching phenomena like TTA.40,41
Devices fabricated with 4b as the emitter have similar spectral properties. In fact, their color also varied from blueish green to orange for increasing thickness values (Fig. S27, ESI†), with the change being due to a variation in the relative intensity of the emission peaks in their EL spectrum (Fig. 9a and Fig. S28 and S29, ESI†), analogous to the behavior observed and discussed in emitter 2b. The only difference here is that the biggest red shift of the lowest energy excimer emission (565 nm) is already reached at 1 nm and is visible already starting from 0.1 nm. The three higher energy peaks are centered on wavelengths values (470 nm, 499 nm, and 523 nm) that are similar to those observed in the photoluminescence spectra. These observations confirm the greater tendency of this compound to aggregate, when compared to 2b, and is the reason that the x coordinate of the points in the chromaticity diagram reaches slightly higher values (CIE3nm = (0.48, 0.51), Fig. 9b).
There are, however, some differences in the J–V–L characteristics (Fig. 9c). In fact, in the case of 4b, an increase in thickness decreases the turn-on voltage only up to 0.1 nm, after which it starts to increase again, reaching over 4 V for 3 nm. This might be due to the already mentioned higher tendency to aggregate, which might affect the device conductivity and, in turn, all the electrical properties. Indeed, the same trend is also observed for the luminance and for the efficiency.
The best performing devices, luminance-wise, were those with a 0.1 nm-thick EML, which reached the highest peak luminance among all the devices described in this study (34071 cd m−2), while the most efficient ones were those with a 0.3 nm-thick EML (22.6 cd A−1 and 8.08% EQE), as illustrated in Fig. 9d and summarized in Table S7 (ESI†). Impressively, those devices were able to maintain EQE above 6% even at a very high brightness of 6000 cd m−2 and around 4.6% at 10
000 cd m−2, showing a small efficiency roll-off which is of particular interest for display applications. Interestingly, for both 2b and 4b, we could tune the emission properties by modifying the thickness of the ultrathin non-doped emissive layer, which balanced the contributions of the vibronic and excimer emission. The selected approach has the advantages of being simple (no co-evaporation required, just a single source), and both fast and cost-effective (as the active layers of the devices are ultrathin).38
Besides the EQE and the maximum brightness, the device lifetime is also a very important indicator for practical applications, especially when measured at a high brightness. Therefore, the lifetime of the brightest devices, those with a 0.1 nm-thick non-doped layer of 4b as the EML, was tested by driving them with a constant current and measuring their luminance versus time. Two different current values were employed, which correspond to initial luminance values of 245 cd m−2 and 1000 cd m−2, finding device lifetimes LT50 of 46 and 11 minutes, respectively (Fig. S30, ESI†). These values are in line with the results obtained for devices with other tetradentate platinum(II) complexes.2
As previously described, the use of Cbz as ancillary ligand in 3b changes the nature of the lowest energy excited state and causes all the emission bands to be red shifted (Fig. 5a). We exploited this property to prepare devices with orange or reddish orange emission using ultrathin undoped EMLs of 1 and 4 nm. In this case, devices turn on showing orange electroluminescence (Fig. S31, ESI†) with an identical EL spectra for the two thickness values (Fig. S30a, ESI†). Consequently, the two devices have the same CIE color coordinates of around (0.56, 0.43) (Fig. S32b, ESI†). However, they possess a different electrical behaviour: devices with an EML thickness of 4 nm achieve a higher luminance with a lower current. The better exciton utilization translates to a higher peak luminance (3107 cd m−2) and efficiency (EQE of 2.74%). At the same time, it was found via photophysical measurements that the emission of 3b undergoes a hypsochromic shift when it is dispersed in a rigid medium rather than in the solid state (537 nm compared to 575 nm, see Table 3 and Fig. 5b). The same effect can be recreated in a light emitting device when dispersing the emitter molecules by inserting them either as an ultrathin layer or as a guest in a dual component EML. We demonstrated this by fabricating OLEDs with the following architecture: ITO (150 nm)/PEDOT:PSS (35 nm)/TAPC (27.5 nm)/CBP:3b (9% or 16%, 40 nm)/BAlq (30 nm)/Ba (5 nm)/Ag (100 nm), where CBP is 4,4′-bis(N-carbazolyl)-1,1′-biphenyl and BAlq is bis(8-hydroxy-2-methylquinoline)-(4-phenylphenoxy)aluminum. Here, CBP acted as the host material and its choice was based on the emitter frontier orbital energy (Fig. S21c and d, ESI†). TAPC acted as the electron block layer, as its high LUMO level (−2.0 V) helps to confine the electrogenerated triplet excitons within the emissive layer, and BAlq as the electron transport layer. As expected, both devices exhibited identical yellowish-green EL with a peak wavelength of 526 nm with a FWHM of 61 nm (Fig. S33 and S34a, ESI†), corresponding to CIE coordinates of (0.30, 0.64) (Fig. S34b, ESI†). The emission was also stable with increasing driving voltage (Fig. S34c and d, ESI†). The devices with a doping concentration of 16% were more efficient in utilizing excitons, reaching a peak luminance of 18798 cd m−2 (Fig. S34e, ESI†) and a maximum efficiency of 1.55% (Fig. S34f, ESI†).
Footnote |
† Electronic supplementary information (ESI) available. CCDC 2431931–2431934. For ESI and crystallographic data in CIF or other electronic format see DOI: https://doi.org/10.1039/d5qm00310e |
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