Shiro Koseki*ab,
Harunobu Yoshinagaa,
Toshio Asadaab and
Takeshi Matsushitabc
aDepartment of Chemistry, Graduate School of Science, Osaka Prefecture University, 1-1 Gakuen-cho, Sakai, Osaka 599-8531, Japan. E-mail: shiro@c.s.osakafu-u.ac.jp
bThe Research Institute for Molecular Electronic Devices (RIMED), Osaka Prefecture University, 1-1 Gakuen-cho, Naka-ku, Sakai 599-8531, Japan
cJNC Petrochemical Corporation, 5-1 Goikaigan, Ichihara, Chiba 290-8551, Japan
First published on 13th April 2015
Substituent effects of NH2, NO2 and CN groups on phosphorescence in fac-tris(2-phenylpyridinato)iridium(III) [fac-Ir(ppy)3] were examined theoretically by using the multiconfiguration self-consistent field (MCSCF) method together with the SBKJC basis sets augmented by a set of polarization functions, followed by second-order configuration interaction (SOCI) and spin–orbit coupling (SOC) calculations, while time-dependent density functional theory (TD DFT) calculations provided too long wavelengths for phosphorescent peaks at the geometries optimized for triplet states even though the TD DFT predictions were qualitatively good with respect to relative spectral shifts. The strongest electron-donating substituent NH2 and the strongest electron-withdrawing substituents, NO2 and CN, were chosen for investigation of the substituent effects in the present investigation. It was found that when these electron-withdrawing substituents are introduced into the Z5 sites, the largest blue shift is obtained for the emission spectra, while the introduction of the electron-donating NH2 substituent causes a red shift of the emission spectra. This is because the Z5 site has non-negligible coefficients in the highest occupied molecular orbital (HOMO) and can interact with the π* orbitals of the substituents. This interaction makes the HOMO lower in energy. This is the reason why a large blue shift of the emission peak is obtained when one of these substituents is introduced to the Z5 sites. Based on the results of the calculation, it can be said that the best material for blue-color emission is tris(5-nitro-2-phenylpyridinato) iridium(III) [fac-Ir(5-NO2ppy)3] or tris(5-nitro-4,6-difluoro-2-phenylpyridinato)iridium(III) [fac-Ir(5-NO2-4,6-dfppy)3]. If the reactivity of the NO2 substituent in the lowest triplet state becomes troublesome in the synthesis processes and/or if it is difficult to choose host molecules for an emissive layer, tris(5-cyano-3,4,6-trifluoro-2-phenylpyridinato)iridium(III) [fac-Ir(5-CN-3,4,6-tfppy)3] would be the most appropriate for blue-color emission.
In our research group,41–57 multi-configuration self-consistent field (MCSCF) wave functions58 followed by second-order configuration interaction (SOCI) calculations59 were used for explicitly calculating spin–orbit coupling (SOC) integrals, in which the Breit–Pauli (BP) Hamiltonian is employed, in order to describe low-lying electronic states in molecules including heavy atoms, while we found that TD DFT calculations provided too long wavelengths for phosphorescent peaks at the geometries optimized for triplet states, even though the TD DFT predictions were qualitatively good with respect to relative spectral shifts. In order to avoid computational difficulties and/or time-consuming calculations in such investigations, relativistic effective-core potentials (RECPs) or model-core potentials (MCPs) and their associated basis sets need to be employed. Although MCPs have correct orbital-nodes, they are not so popular unfortunately and have less variety of selections. On the other hand, RECPs have become very popular, especially in the research fields of heavy-metal complexes, and the use of RECPs provides many merits for theoretical investigation.
When RECPs are employed for SOC calculations, the full BP Hamiltonian provides very small SOC integrals because of node-less RECP orbitals. Therefore, it is necessary to introduce effective nuclear charges (Zeff)41–47 for reasonable prediction of SOC effects. This is usually referred to as one-electron approximation, effective nuclear charge approximation, or Zeff approximation. Our research group determined Zeff's for all transition elements and reported that this approximation works very well for estimation of SOC effects in mono-hydrides of transition elements in the third through seventh groups.48–50 The di-hydrides and tetra-hydrides of rhenium atoms were also examined in our laboratory.51–54 After such successes, this method was applied to theoretical investigations of the phosphorescent processes in OLED molecules.55–57 The results of our investigations could explain the emission spectra in the parent molecules, bis[2-(2′-thienyl) pyridinato]platinum [Pt(thpy)2]55 and tris(2-phenylpyridinato)iridium(III) [Ir(ppy)3].56 We also analyzed the geometrical effects of ligands in Ir(ppy)3 and its derivatives.57 In this latest paper, we discussed the effects of introducing an auxiliary ligand, picolinate (pic) or 2,4-pentanedionate (acac) ligand, to spectral shifts of phosphorescence. When such an auxiliary ligand is introduced, an iridium complex has not only facial (fac) and meridional (mer) isomers but also additional geometrical isomers. For example, the introduction of a pic ligand provides bis[2-(4′,6′-difluorophenyl) pyridinato-N,C2′] [picolinato-N,O]iridium(III) [Ir(4,6-dfppy)2(pic)], so-called FIrpic, and this complex has four geometrical isomers, homo-N-trans (HNT), homo-C-trans (HCT), homo-cis,hetero-N-cis (HC), and homo-cis,hetero-N-trans (HT) (see the details in ref. 57). The alignment of the heaviest atoms in each ligand of HC is the same as fac-Ir(ppy)3, but the most stable isomer is not HC but HNT among these four isomers. The calculated peak of the phosphorescence appears at the wavelength of 450 nm in HNT. Although this wavelength is shorter than the corresponding observed wavelengths (468–469 nm) by about 20 nm, this series of calculations indicate that a systematic underestimation is obtained for the peak wavelengths of emission because of inadequate consideration of electron correlation effects and that the magnitudes of spectral shifts are reliable for quantitative prediction of emission peaks. The next most stable isomer, HC, is only 0.8 (DFT) or 0.9 (MCSCF + SOCI + SOC) kcal mol−1 higher than HNT and is calculated to have a phosphorescent peak at the wavelength of 412 nm. Therefore, if only the HC isomer of FIrpic can be doped into an emissive layer of OLEDs, more blue-shifted phosphorescence is expected to be observed. In this investigation, we also discussed the phosphorescent processes in bis[2-(4′,6′-difluorophenyl) pyridinato-N,C2′] [2,4-pentanedionato-O,O]iridium(III) [Ir(4,6-dfppy)2(acac)], so-called FIracac and the related complexes.57
Although large amount of investigations have been reported so far on OLED materials, it is still expected that better materials need to be developed for brighter blue phosphorescence. Therefore, we think it is valuable to theoretically examine the effects of strongest electro-donating substituent NH2 and strongest electro-withdrawing substituents, CN and NO2, since we could not find any information on the substituent effects of NH2 and NO2 groups. The methods of theoretical calculation are described in detail in the next section. In the third section, the effects of NH2, NO2, and CN substituents on the phenyl rings of ppy ligands are compared and discussed, where NH2 group should be considered to be a representative for some bulky NX2 groups (X could be alkyl, aryl or any other functional group). Finally, better phosphorescent complexes for brighter blue-color emission are suggested on the basis of the present discussion on iridium complexes.
At these stationary geometries, the molecular orbitals were optimized using the MCSCF method58 together with the state-averaging technique. The MCSCF active space includes six electrons and six orbitals, three of the orbitals mainly having an Ir d character and the remaining three orbitals having ligands' π character (principally anti-bonding) [MCSCF(6e,6)]. The electronic density was averaged among the lowest ten singlet and nine triplet states during MCSCF iterations. In order to describe electronically excited states and estimate the SOC effects among those states, SOCI wave functions59 were constructed using the MCSCF optimized orbitals, in which the external space could include only 30 orbitals that have the lowest eigenvalues of the standard MCSCF Fock operator, due to our computer resource limitations. All calculations were achieved using the GAMESS suite of program codes.64
Note that the words “HOMO” and “LUMO” are inappropriate since a set of natural orbitals optimized by the MCSCF method was used in the present investigation.65 However, for simplicity, these words will be used as our current definitions in the following discussion: HOMO means the natural orbital for which the occupation number is larger than one and the smallest among them in the ground state, and LUMO means the natural orbital for which the occupation number is smaller than one and the largest among them in the ground state.66 Additionally, it should be described that the energies of natural orbitals can be considered to be reversely proportional to their occupation numbers.
| Complex | Isomer | DFT | MCSCF | +SOCI | +SOC | Ref. |
|---|---|---|---|---|---|---|
| Ir(ppy)3 | fac | 0 | 0 | 0 | 0 | |
| Ir(ppy)3 | mer | 6.4 | 6.1 | 6.0 | 5.7 | 57 |
| Ir(3-Fppy)3 | fac | 6.5 | 9.2 | 10.4 | 10.0 | 57 |
| Ir(4-Fppy)3 | fac | 0 | 0 | 0 | 0 | 57 |
| Ir(5-Fppy)3 | fac | 4.9 | 6.6 | 6.6 | 6.5 | 57 |
| Ir(6-Fppy)3 | fac | 4.6 | 5.7 | 5.9 | 5.7 | 57 |
| Ir(3-NH2ppy)3 | fac | 9.9 | 18.5 | 19.8 | 18.9 | |
| Ir(4-NH2ppy)3 | fac | 0 | 0 | 0 | 0 | |
| Ir(5-NH2ppy)3 | fac | 10.8 | 11.7 | 12.3 | 12.1 | |
| Ir(6-NH2ppy)3 | fac | 16.3 | 18.7 | 19.0 | 18.8 | |
| Ir(3-NO2ppy)3 | fac | 33.1 | 40.9 | 40.6 | 40.2 | |
| Ir(4-NO2ppy)3 | fac | 6.5 | 15.6 | 11.7 | 11.8 | |
| Ir(5-NO2ppy)3 | fac | 0 | 0 | 0 | 0 | |
| Ir(6-NO2ppy)3 | fac | 31.7 | 44.6 | 41.5 | 41.7 | |
| Ir(3-CNppy)3 | fac | 13.8 | 18.0 | 16.3 | 15.7 | |
| Ir(4-CNppy)3 | fac | 3.1 | 7.1 | 5.7 | 5.5 | |
| Ir(5-CNppy)3 | fac | 0 | 0 | 0 | 0 | |
| Ir(6-CNppy)3 | fac | 8.4 | 19.4 | 16.9 | 16.9 | |
| Ir(4,6-dfppy)3 | fac | 0 | 0 | 0 | 0 | |
| Ir(4,6-dfppy)3 | mer | 6.1 | 5.5 | 5.5 | 5.4 | |
| Ir(3,4,6-tfppy)3 | fac | 0 | 0 | 0 | 0 | |
| Ir(3,4,6-tfppy)3 | mer | 1.7 | 0.9 | 0.7 | 0.5 |
As described in our previous paper,76 in order to reproduce experimental emission spectra, it is necessary to consider spectral broadening and anharmonicity caused by the interaction with its circumstances and the geometrical displacement between the energy minima of electronic states. However, it is too time-consuming to calculate the potential energy curves (PECs) of low-lying spin-mixed (SM) states in many complexes and it becomes difficult to obtain the wavefunctions for energetically high vibrational states in each SM state. Therefore, we decided that the peak positions of emission spectra can be assumed to be provided by the superposition of Lorentz functions centered at the electronic transition energies from excited SM states to the ground state (SM0). In these calculations, the thermal population distribution for low-lying SM states was assumed to be given at an appropriate temperature and a Lorentz function for each electronic transition was assumed to have an appropriate half-value width.77
| Complex | Isomer | Peak wavelengtha (nm) | Principal contributionb | Wavelengthc (nm) | TDM (e bohr) | TD DFTd (nm) | Expt.c (nm) | Ref. | ΔQS0−T1e (Å) |
|---|---|---|---|---|---|---|---|---|---|
| a The values in parentheses are the magnitudes of spectral shifts in comparison with that in the corresponding parent complex. The positive or negative value indicates “red shift” or “blue shift”.b The main adiabatic component is shown in parenthesis. Note that, even when the main component is singlet, the sum of triplet weights is the largest.c RT = room temperature.d TD DFT wavelengths were calculated at the uDFT geometries optimized for the lowest triplet states, where we picked up the wavelengths of the transition from the lowest triplet (d,π*) state to the ground state and no spin–orbit couplings were considered.e ΔQS0−T1 is the averaged geometrical displacement of each atom caused by the transition from the lowest triplet state to the ground state (see ref. 83). | |||||||||
| Ir(ppy)3 | fac | 491 (0) | SM3 (S1) | 501 | 0.299 | 615 | 57 | 0.0557 | |
| SM4 (T1) | 491 | 0.890 | 510 (298 K) | 71 | |||||
| 515 (RT) | 72 | ||||||||
| 517 (298 K) | 73 | ||||||||
| 494 (77 K) | 74 | ||||||||
| 509 (RT) | 75 | ||||||||
| mer | 530 (+39) | SM3 (T1) | 530 | 0.255 | 698 | 57 | 0.1611 | ||
| 511 (+20) | SM4 (S1) | 512 | 1.156 | 512 (298 K) | 71 | ||||
| Ir(3-Fppy)3 | fac | 486 (−5) | SM3 (S1) | 487 | 0.352 | 611 | 57 | 0.0619 | |
| 477 (−14) | SM4 (T1) | 476 | 0.811 | ||||||
| Ir(4-Fppy)3 | fac | 456 (−35) | SM3 (S1) | 462 | 0.233 | 603 | 57 | 0.0413 | |
| SM4 (T1) | 455 | 0.853 | |||||||
| Ir(5-Fppy)3 | fac | 517 (+26) | SM3 (T1) | 517 | 0.328 | 648 | 57 | 0.0520 | |
| 504 (+13) | SM4 (T1) | 504 | 0.888 | ||||||
| Ir(6-Fppy)3 | fac | 475 (−16) | SM3 (S1) | 483 | 0.248 | 594 | 57 | 0.0542 | |
| SM4 (T1) | 474 | 0.874 | |||||||
| Ir(3-NH2ppy)3 | fac | 510 (+19) | SM3 (S1) | 510 | 0.316 | 790 | 0.0711 | ||
| 495 (+4) | SM4 (T1) | 495 | 0.978 | ||||||
| Ir(4-NH2ppy)3 | fac | 442 (−49) | SM4 (T1) | 442 | 0.934 | 610 | 0.0318 | ||
| Ir(5-NH2ppy)3 | fac | 546 (+55) | SM3 (T1) | 546 | 0.393 | 791 | 0.0704 | ||
| 526 (+35) | SM4 (T2) | 525 | 0.962 | ||||||
| Ir(6-NH2ppy)3 | fac | 482 (−9) | SM4 (T1) | 482 | 0.974 | 598 | 0.0618 | ||
| Ir(4-NO2ppy)3 | fac | 587 (+96) | SM3 (T1) | 587 | 0.304 | 747 | 0.0419 | ||
| 561 (+70) | SM4 (T2) | 561 | 0.937 | ||||||
| Ir(5-NO2ppy)3 | fac | 404 (−87) | SM3 (S1) | 404 | 0.335 | 550 | 0.0425 | ||
| 396 (−95) | SM4 (T1) | 395 | 0.972 | ||||||
| Ir(6-NO2ppy)3 | fac | 650 (+159) | SM3 (T1) | 652 | 0.280 | 798 | 0.0572 | ||
| 644 (+153) | SM4 (S1) | 643 | 0.471 | ||||||
| Ir(3-CNppy)3 | fac | 445 (−46) | SM3 (S1) | 449 | 0.356 | 636 | 0.0500 | ||
| SM4 (T1) | 442 | 0.681 | |||||||
| Ir(4-CNppy)3 | fac | 539 (+48) | SM3 (T1) | 539 | 0.302 | 676 | 0.0533 | ||
| 522 (+31) | SM4 (T1) | 522 | 0.925 | ||||||
| Ir(5-CNppy)3 | fac | 459 (−32) | SM4 (T1) | 459 | 0.863 | 603 | 0.0403 | ||
| Ir(6-CNppy)3 | fac | 534 (+43) | SM3 (S1) | 535 | 0.331 | 634 | 0.0621 | ||
| 521 (+30) | SM4 (T1) | 521 | 0.869 | ||||||
| Ir(4,6-dfppy)3 | fac | 440 (−51) | SM4 (T1) | 440 | 0.864 | 587 | 57 | 0.0602 | |
| 468 (298 K) | 71 | ||||||||
| 469 (RT) | 75 | ||||||||
| Ir(5-NO2-4,6-dfppy)3 | fac | 374 (−117) | SM2 (T1) | 379 | 0.158 | 600 | 0.0581 | ||
| SM3 (S1) | 377 | 0.349 | |||||||
| SM4 (T1) | 373 | 0.735 | |||||||
| Ir(5-CN-4,6-dfppy)3 | fac | 409 (−82) | SM3 (S1) | 414 | 0.260 | 585 | 442 (77 K) | 85 | 0.0453 |
| SM4 (T1) | 409 | 0.789 | |||||||
| Ir(4,6-dappy)3 | fac | 440 (−51) | SM4 (T1) | 440 | 1.022 | 592 | 0.0776 | ||
| Ir(5-CN-4,6-dappy)3 | fac | 409 (−82) | SM3 (S1) | 417 | 0.126 | 585 | 0.0882 | ||
| SM4 (T1) | 409 | 0.942 | |||||||
| Ir(3,4,6-tfppy)3 | fac | 435 (−56) | SM4 (T1) | 435 | 0.808 | 594 | 456 (298 K) | 86 | 0.0480 |
| 486 (298 K) | 86 | ||||||||
| Ir(5-NO2-3,4,6-tfppy)3 | fac | 418 (−73) | SM4 (S1) | 418 | 0.095 | 592 | 0.0573 | ||
| Ir(5-CN-3,4,6-tfppy)3 | fac | 406 (−85) | SM3 (S1) | 409 | 0.278 | 595 | 0.0460 | ||
| SM4 (T1) | 405 | 0.755 | |||||||
The results57 for the introduction of F substituents can be crudely explained as follows. The main component of the phosphorescence in such heavy-metal complexes is d–π* transition or metal-to-ligand charge-transfer (MLCT). As illustrated in Fig. 3, the LUMO (see the last paragraph in Section 2) consists mainly of the lowest π* orbital of the ligands66 and has larger linear-combination-of-atomic-orbitals (LCAO) coefficients at the Z4 and Z6 sites of the phenyl rings of the ppy ligands, while negligible coefficients appear at the Z3 and Z5 sites. The blue shift of the phosphorescence is explained by energetically lifting the LUMO caused by introduction of F substituents to the Z4 and Z6 sites (Fig. 4(a)). On the other hand, introduction to the Z3 and Z5 sites rarely affects the LUMO because of small coefficients (Fig. 3). The steric effects might explain the blue shift in Ir(3-Fppy)3, but it is apparent that Ir(5-Fppy)3 has weak steric effects in the vicinity of the Z5 sites. When the HOMO was examined carefully in the parent molecule Ir(ppy)3, it was found to have non-zero coefficients at the Z5 site (Fig. 3). This orbital can interact with the occupied 2pπ orbitals of F substituents, and this interaction lifts the HOMO energetically (Fig. 4(a)). This is the reason why a red shift is predicted in Ir(5-Fppy)3.
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| Fig. 3 HOMO and LUMO in the parent molecule, fac-Ir(ppy)3, where the value of equi-surface is 0.02 e bohr−3. | ||
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| Fig. 4 Orbital interaction between a ppy ligand and a substituent in facial (fac) isomers. (a) Z = F or NH2. (b) Z = NO2 or CN. | ||
| Complex | C–N–H | C–N–H | H–N–H | Sum | Dihedral angle | |
|---|---|---|---|---|---|---|
| a See Fig. 5. | ||||||
| Ir(3-NH2ppy)3 | 118.6 | 120.5 | 120.7 | 359.8 | C2–C3–N–H | 4.8 |
| C2–C3–N–H′ | 179.8 | |||||
| 115.3 | 115.7 | 114.2 | 345.2 | C2–C3–N–H | 17.1 | |
| C2–C3–N–H′ | 154.0 | |||||
| 112.2 | 113.3 | 111.4 | 337.0 | C2–C3–N–H | 27.2 | |
| C2–C3–N–H′ | 154.5 | |||||
| Ir(4-NH2ppy)3 | 115.5 | 116.4 | 113.4 | 345.4 | C3–C4–N–H | 21.1 |
| C3–C4–N–H′ | 157.9 | |||||
| 113.9 | 114.5 | 111.7 | 340.0 | C3–C4–N–H | 24.1 | |
| C3–C4–N–H′ | 154.3 | |||||
| 113.7 | 114.2 | 111.4 | 339.3 | C3–C4–N–H | 25.2 | |
| C3–C4–N–H′ | 154.6 | |||||
| Ir(5-NH2ppy)3 | 118.4 | 118.4 | 116.4 | 353.3 | C4–C5–N–H | 32.8 |
| C4–C5–N–H′ | 156.4 | |||||
| 112.3 | 112.5 | 109.3 | 334.2 | C4–C5–N–H | 30.4 | |
| C4–C5–N–H′ | 154.3 | |||||
| 112.1 | 112.5 | 109.2 | 333.8 | C4–C5–N–H | 17.0 | |
| C4–C5–N–H′ | 167.2 | |||||
| Ir(6-NH2ppy)3 | 110.2 | 112.1 | 108.1 | 330.4 | C5–C6–N–H | 11.9 |
| C5–C6–N–H′ | 132.3 | |||||
| 110.3 | 111.6 | 108.2 | 330.1 | C5–C6–N–H | 12.3 | |
| C5–C6–N–H′ | 132.6 | |||||
| 110.1 | 112.0 | 108.0 | 330.1 | C5–C6–N–H | 10.0 | |
| C5–C6–N–H′ | 130.1 | |||||
| Complex | C–N–O | C–N–O | O–N–O | Sum | Dihedral angle | |
|---|---|---|---|---|---|---|
| Ir(4-NO2ppy)3 | 117.7 | 118.0 | 124.3 | 360.0 | C3–C4–N–O | 0.5 |
| C3–C4–N–O′ | 179.9 | |||||
| 117.7 | 118.0 | 124.2 | 360.0 | C3–C4–N–O | 1.9 | |
| C3–C4–N–O′ | 178.5 | |||||
| 117.7 | 118.7 | 123.6 | 360.0 | C3–C4–N–O | 0.1 | |
| C3–C4–N–O′ | 179.6 | |||||
| Ir(5-NO2ppy)3 | 117.0 | 118.8 | 124.2 | 360.0 | C4–C5–N–O | 0.7 |
| C4–C5–N–O′ | 179.4 | |||||
| 117.9 | 118.0 | 124.1 | 360.0 | C4–C5–N–O | 0.5 | |
| C4–C5–N–O′ | 179.6 | |||||
| 118.0 | 118.0 | 124.0 | 360.0 | C4–C5–N–O | 0.2 | |
| C4–C5–N–O′ | 179.6 | |||||
| Ir(6-NO2ppy)3 | 117.7 | 118.0 | 124.3 | 360.0 | C5–C6–N–O | 50.2 |
| C5–C6–N–O′ | 127.6 | |||||
| 117.6 | 117.7 | 124.6 | 359.9 | C5–C6–N–O | 64.8 | |
| C5–C6–N–O′ | 113.4 | |||||
| 120.4 | 121.2 | 105.0 | 346.6 | C5–C6–N–O | 19.1 | |
| C5–C6–N–O′ | 115.8 |
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| Fig. 5 Numbering of atoms. X and X′ indicate H or O (see Table 3). | ||
Experimental reports have been published on the effects of introducing diphenyl-amino (NPh2) groups to the Z4 sites.78–80 The introduction of NPh2 groups corresponds to forming parts of starburst materials for OLEDs. If a bridged bond between two phenyl rings, it becomes a popular carbazole substituent. The peak of emission spectra in Ir(4-NPh2ppy)3 is reported to be observed at the wavelength of 526–534 nm,78–80 so that the magnitude of red-shift is about 20 nm. This could be interpreted as the strong π–π interaction between the terminal phenyl groups of NPh2 and ppy ligands. As described above, we assumed to exclude such situation of strong π conjugation. Thus, it should be understood that the effects of phenyl groups are so important as those of nitrogen atoms of NPh2. Unfortunately, NPh2 groups are too large for us to carry out theoretical calculations at the present levels of theory because of our computer resources.
Likewise, the effects of NO2 and CN substituents to spectral peak shifts are completely different from those of F and NH2 substituent as shown in Table 2 (and Fig. 2). When one of these substituents is introduced to each Z4 site (Ir(4-Zppy)3), the phosphorescent peaks are split into two and shifted to the red region by 96 and 70 nm (Z = NO2) or 48 and 31 nm (Z = CN). These peaks are assigned to the transitions from SM3 and SM4 to the ground state. In the same manner, when it is introduced to the Z6 site (Ir(6-Zppy)3), the phosphorescent peak is calculated to be considerably shifted to the red region. These peaks are also split into two, respectively; the magnitudes of red shift are 159 and 153 nm for Z = NO2, and 43 and 30 nm for Z = CN. These peaks are also assigned to the transitions from SM3 and SM4 to the ground state, respectively, where the principal components of SM3 and SM4 are S1 and T1, respectively (see Table 2) and, even though the principal component of SM3 is S1, the weight of T1 is relatively large and the total weight of triplet states is larger than those of singlet states in SM3. The key difference among these substituents is the existence of low-lying π* orbitals. Only the 3p orbital can play a role of a π* orbital in F substituent and is apparently high in energy. An orbital in NH2 substituent, which is expected to play a role of π* orbital at a structure close to a planar one, must be high in energy than the π* orbitals of electron-withdrawing NO2 and CN substituents. As mentioned above, the LUMO in the parent molecule Ir(ppy)3 has large coefficients at the Z4 and Z6 sites and can strongly interact with the π* orbitals of these substituents (Fig. 3). Additionally, when the NO2 substituent is introduced to the Z4 site, attractive interaction81 can occur between the oxygen atoms of the NO2 substituent and the adjacent hydrogen atoms of the phenyl rings. These bonds must enhance the π conjugation between the ligands and the substituents and make the magnitude of the red shift larger (Fig. 4(b)). In fact, all three atoms of the NO2 substituent are located on the π plane provided by the ppy ligands in Ir(4-NO2ppy)3 (Fig. 6). This geometrical feature must be the reason why such large red shifts are obtained in these complexes. The magnitude of the red shift in Ir(4-CNppy)3 is smaller than that in Ir(4-NO2ppy)3, since attractive interaction is negligible between the terminal nitrogen atoms of CN substituent and the adjacent hydrogen atoms of the phenyl rings in Ir(4-CNppy)3.
With respect to π interaction between ligands and substituents and to attractive interaction between hydrogen atoms and adjacent oxygen or nitrogen atoms, the situation in Ir(6-Zppy)3 is similar to that in Ir(4-Zppy)3 (Z = NO2 or CN). Additionally, the Z6 sites are geometrically close to the adjacent pyridine rings or geometrically crowded, so that the NO2 substituents are somewhat displaced from the π planes of the ligands in order to minimize nuclear repulsion (Fig. 6). Nevertheless, attractive interaction81 still exists between the oxygen atoms of the NO2 substituent and the adjacent hydrogen atoms of the ligands, and π conjugation occurs in the larger space including pyridine rings. The large red shift (153/159 nm) in Ir(6-NO2ppy)3 must be attributed to this large space of π conjugation including both phenyl and pyridine rings. Thus, the introduction of these substituents to the Z4 and Z6 sites makes the LUMO explicitly lower in energy than that in the parent molecule Ir(ppy)3 (Fig. 4(b))66 and, as a result, it causes a relatively large red shift of the phosphorescent peaks in Ir(6-Zppy)3 as well as Ir(4-Zppy)3 (Z = NO2 or CN).
On the other hand, when one of these electron-withdrawing substituents is introduced to the Z5 site [Ir(5-Zppy)3], the phosphorescent peak is split into two and shifted to the blue region by 87 and 95 nm for Z = NO2, while it is shifted to the blue region by 32 nm for Z = CN (Table 2). As mentioned above, the Z5 site in the parent molecule Ir(ppy)3 has negligible coefficients in LUMO but has non-negligible coefficients in HOMO (Fig. 3), so that introduction of the substituents to the Z5 sites causes a meaningful interaction between the HOMO of the parent molecule Ir(ppy)3 and the π* orbitals of the substituents (Fig. 4(b)).82 Since the main components of the HOMO in these complexes are Ir's d orbitals, the coefficients at the Z5 sites of the ppy ligands in HOMO are explicitly smaller than those at the Z4 and Z6 sites in LUMO of the parent molecule Ir(ppy)3. This might be the reason why the magnitudes of the blue shifts are smaller than those of the red shift in Ir(4-Zppy)3 and Ir(6-Zppy)3. This interaction is also enhanced by the attractive interaction between the oxygen atoms of NO2 substituents and the adjacent hydrogen atoms of the ligands,81 since such an attractive interaction makes the NO2 substituents located on the π plane of the ligands (Fig. 6(c)). Thus, it can be understood that, in addition to the electron-withdrawing effects of these substituents, the interaction between the HOMO of the parent molecule Ir(ppy)3 and the π* orbitals of the substituents makes HOMO lower in energy66 in the target molecule (Fig. 4(b) (ref. 82)) and, as a result, a blue shift of the phosphorescence was obtained by the introduction of these substituents to the Z5 sites. Since the π* orbitals in the NO2 substituent lower HOMO in energy than that in the CN substituent,66 the magnitude of the blue shift in Ir(5-NO2ppy)3 is calculated to be large in comparison with that in the Ir(5-CNppy)3.
In order to examine the rates of non-radiative transitions in these complexes, geometrical displacements between the ground state and the lowest triplet state83 were also calculated. In most of the present complexes, the geometrical displacements were calculated to be 0.04–0.08 Å per atom. Since these displacements are comparable with that in the fac isomer of the parent molecule Ir(ppy)3 and is apparently smaller than that in the mer isomer, fast non-radiative transition is not expected to occur in these complexes. When NO2 substituents were introduced to the Z3 sites, an unexpected bond was formed between the terminal oxygen atoms of NO2 substituents and the closest carbon atoms of the adjacent ligand during geometry optimization for the lowest triplet state (indicated by a dotted circle in Fig. 6(a)). As a result, the ring of the ligand becomes pyramidal (non-planar sp3 structure). This is the reason why Ir(3-NO2ppy)3 was excluded from the present investigation.84 Such behavior of NO2 substituent may be the reason why it has not been used in experiments so far.
Unfortunately, no experimental reports could be found for Ir(5-Zppy)3 (Z = NO2 or CN). As described in the next section, experimental observation suggests that introduction of CN substituents to the Z5 sites in tris(4,6-difluoro-2-phenylpyridinato)iridium(III) [fac-Ir(4,6-dfppy)3] causes a blue shift of 27 nm (from 469 to 442).85 This is in good agreement with the present results of calculation for Ir(5-CNppy)3 with respect to the magnitude of spectral shift (from 491 to 459). It is therefore said that Ir(5-NO2ppy)3 must be the best doping material for blue color emission. When the observation at room temperature72 is taken as a reference (see Table 2), the present computational method underestimates the peak wavelength by 24 nm in the parent molecule Ir(ppy)3. If this difference is applicable to the other computational results, the phosphorescent peaks in Ir(5-NO2ppy)3 are predicted to be observed near the wavelengths of 420 and 428 nm. Thus, we would conclude that Ir(5-NO2ppy)3 is the best phosphorescent complex, but, if NO2 substituent is troublesome to use for a dopant, the secondary selection must be Ir(5-CNppy)3. However, the predicted wavelength is 483 nm after correction of the present computational underestimation. These wavelengths are too long to employ it as a blue-color emissive material. Therefore, better combinations of substituents will be examined in the next section. At the end of this section, we should emphasize that the most important point of the substituent effects is not electron-withdrawing strength but the existence of low-lying π* orbitals in substituents, though this comment may be same meaning when substituents have a π plane.
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| Fig. 7 Emission spectra in calculated by the MCSCF + SOCI + SOC method (see the caption of Fig. 2). NO2 or CN substituent is introduced to (a) Ir(4,6-dfppy)3 and its derivatives, (b) Ir(3,4,6-tfppy)3 and its derivatives, and (c) Ir(4,6-dappy)3 and its derivatives, where Ir(5-NO2-4,6-dappy)3 has very small intensity. | ||
Table 2 shows the results of calculation for Ir(5-Z-4,6-dfppy)3 (Z5 = NO2 or CN). The magnitudes of the blue shift caused by introduction of the substituents are calculated to be 66 nm for Z5 = NO2 and 31 nm for Z5 = CN, where these peaks are obtained as the overlaps of the transitions from two or three SM states to the ground state, where all these SM states has largest weights of triplet states, even though the principal component is S1 in SM3 (see Table 2). As already mentioned in the previous section, the magnitude of the blue shift is in good agreement with the experimental observation85 for Ir(5-CN-4,6-dfppy)3 after considering the present computational underestimation. Only when NO2 substituents are introduced to the Z5 site, is the magnitude reduced by 29 nm, even though the magnitude of the blue shift itself is still largest. This result can be easily understood: since no attractive interaction can occur between this substituent and the adjacent F substituents, in contrast to the case of Ir(ppy)3, NO2 substituents rotate around the C–N bonds and their oxygen atoms are displaced from the π plane provided by each ppy ligand (Fig. 8). Such geometrical rotation weakens the π interaction between the substituents and the 4,6-dfppy ligands. This must be the reason why the magnitude of the blue shift is reduced by 29 nm in Ir(5-NO2-4,6-dfppy)3. Nevertheless, the introduction of these substituents can cause effective blue shifts, and the spectral peak in Ir(5-NO2-4,6-dfppy)3 appears in the region of shorter wavelength (374 nm). This wavelength may be too short for blue-color emission, where correction of the present computational underestimation suggests that the spectral peak appears at the wavelengths of 398–403 nm. If NO2 substituent could be troublesome to use for a dopant, a better candidate would be Ir(5-CN-4,6-dfppy)3 rather than Ir(5-NO2-4,6-dfppy)3. This conclusion is consistent with the fact that the experimental observation (442 nm)85 has been reported for Ir(5-CN-4,6-dfppy)3.
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| Fig. 8 Geometrical structures of fac-Ir(5-NO2-4,6-dfppy)3. All NO2 substituents are displaced from the π plane of ppy ligands. | ||
Before finishing this subsection, it would be noteworthy to describe the effects of the third F substituent. When the third F substituent is introduced to the Z3 site in Ir(6-NO2-4,6-dfppy)3, strong π conjugation occurs between NO2 substituent and the adjacent pyridine ring and makes the spectral peak shift to red region in Ir(6-NO2-4,6-dfppy)3 unfortunately. On the other hand, when the third F substituent86 is introduced to the Z3 sites in Ir(5-CN-4,6-dfppy)3, the spectral peak is calculated to appear at the wavelength of 406 nm (Fig. 7(b)). Namely, the third F substituent provides a small magnitude of blue shift (3 nm) and helps to obtain brighter blue-color emission. After correction of the present computational underestimation, the spectral peak is estimated to appear at the wavelength of 430–435 nm for Ir(5-CN-3,4,6-tfppy)3. Note that since the geometrical displacements caused by electronic transitions are calculated to be 0.03–0.06 Å per atom for these complexes, fast non-radiative transition can be considered to rarely occur in these complexes.
When two NH2 substituents are introduced to the Z4 and Z6 sites (Ir(4,6-dappy)3), the spectral peaks are calculated to appear at the wavelength of 440 nm (Table 2 and Fig. 7(c)). As mentioned in Section 3.2, since Ir(4-NH2ppy)3 has a peak at the wavelength of 442 nm and the introduction of NH2 substituent to the Z6 site causes a small blue shift (9 nm), it is understandable that the peak in Ir(4,6-dappy)3 appears at the wavelength of 440 nm.
As mentioned above, when an NH2 substituent is introduced to the Z4 and Z6 sites, the LUMO is lifted by the interaction between the lone-pair orbitals of NH2 substituents and the LUMO of the parent molecule Ir(ppy)3. At the same time, the lone-pair orbitals of NH2 substituents interact with ligands' π orbitals, and such interaction between occupied π orbitals makes ligands' π orbitals higher in energy and closer in energy to the HOMO (principally occupied Ir's d orbitals). Under such circumstances, the introduction of an NO2 or CN substituent to the Z5 site makes the HOMO lower in energy as shown in Fig. 4(b).82 As a result, though we finally succeed in obtaining a large blue shift for Ir(5-CN-4,6-dappy)3 as shown in Table 2, the HOMO (Ir's d orbitals) were largely lowered by these interactions and it becomes closer in energy to occupied π orbitals of the ligands. As a result, their energetic order has been changed during MCSCF iterations in Ir(5-NO2-4,6-dappy)3. We recalculated several times in order to maintain Ir's d-orbital character in MCSCF active space for Ir(5-NO2-4,6-dappy)3, but the MCSCF active orbitals always lose Ir's d-orbital components and become pure π orbitals of the ligands in Ir(5-NO2-4,6-dappy)3. This fact suggests that some (π–π*) excited states are explicitly lower in energy than MLCT (d–π*) excited states in this complex and that SOC mixing between low-lying singlet and triplet states rarely occurs and only very weak or almost no phosphorescence can be observed in Ir(5-NO2-4,6-dappy)3 (see Fig. 7(c)). Thus, we unfortunately have to conclude that Ir(5-NO2-4,6-dappy)3 is inappropriate but Ir(5-CN-4,6-dappy)3 could be used as phosphorescent materials.
000 cm−1. The temperature is set to be relatively high, since the MCSCF + SOCI calculations tend to overestimate emission energies because of relatively small active space.
(N being the number of atoms). Note that the equation in our previous paper (ref. 57) is wrong.Footnote |
| † Electronic supplementary information (ESI) available. See DOI: 10.1039/c5ra04487a |
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