Alessandro
Sinopoli
a,
Fiona A.
Black
b,
Christopher J.
Wood
b,
Elizabeth A.
Gibson
*b and
Paul I. P.
Elliott
*a
aDepartment of Chemistry, University of Huddersfield, Queensgate, Huddersfield, HD1 3DH, UK. E-mail: p.i.elliott@hud.ac.uk
bSchool of Chemistry, Newcastle University, Newcastle upon Tyne, NE1 7RU, UK. E-mail: elizabeth.gibson@ncl.ac.uk
First published on 5th January 2017
A novel anchoring ligand for dye-sensitised solar cell chromophoric complexes, 1-(2,2′-bipyrid-4-yl)-1,2,3-triazole-4,5-dicarboxylic acid (dctzbpy), is described. The new dye complexes [Ru(bpy)2(dctzbpy)][PF6]2 (AS16), [Ir(ppy)2(dctzbpy)][PF6] (AS17) and [Re(dctzbpy)(CO)3Cl] (AS18) were prepared in a two stage procedure with intermediate isolation of their diester analogues, AS16-Et2, AS17-Et2 and AS18-Et2 respectively. Electrochemical analysis of AS16-Et2, AS17-Et2 and AS18-Et2 reveal reduction potentials in the range −1.50 to −1.59 V (vs. Fc+/Fc) which are cathodically shifted with respect to that of the model complex [Ru(bpy)2(dcbH2)]2+ (1) (Ered = −1.34 V, dcbH2 = 2,2′-bipyridyl-4,4′-dicarboxylic acid). This therefore demonstrates that the LUMO of the complex is correctly positioned for favourable electron transfer into the TiO2 conduction band upon photoexcitation. The higher energy LUMOs for AS16 to AS18 and a larger HOMO–LUMO gap result in blue-shifted absorption spectra and hence reduced light harvesting efficiency relative to their dcbH2 analogues. Preliminary tests on TiO2 n-type and NiO p-type DSSCs have been carried out. In the cases of the Ir(III) and Re(I) based dyes AS17 and AS18 these show inferior performance to their dcbH2 analogues. However, the Ru(II) dye AS16 (η = 0.61%) exhibits significantly greater efficiency than 1 (η = 0.1%). In a p-type cell AS16 shows the highest photovoltaic efficiency (η = 0.028%), almost three times that of cells incorporating the benchmark dye coumarin C343.
Over thirty years ago, Goodenough and co-workers15 reported the use of 4,4′-dicarboxy-2,2′-bipyridine (dcbH2, Fig. 1) as an ambidentate ligand for coordination to Ru(II) and metal oxide semiconductors. Strong electronic coupling between the MLCT excited states of dcbH2-containing Ru compounds and TiO2 has been inferred from femtosecond transient absorption spectroscopy, and the timescales extracted from such data are on the order of <25 fs.16 To this day dcbH2 remains the most efficient and widely utilised anchoring ligand for applications in DSSCs, however, a number of other carboxylate-based variant ligands have been investigated. Heuer et al. reported the design of a new bipyridine based anchoring ligand (4,5-diazafluoren-9-ylidene)malonic acid (dfm, Fig. 1) together with its corresponding complex [Ru(bpy)2(dfm)]2+ (bpy = 2,2′-bipyridyl).6 Mishra et al. prepared the complex BCT-1, [Ru(dcthbpyH)2(NCS)2][NBu4]2, where the distance between the bpy core of the ligand and its anchoring carboxylate group has been extended by the introduction of a thiophene spacer (dcthbpyH2).17 This increases charge separation upon charge injection and reduces the rate of recombination but also leads to augmentation of the light absorption properties over the corresponding dcbH2 complex. This yielded an overall conversion efficiency of 6.1% compared with the 4.8% achieved using the archetypal DSSC dye N3 ([Ru(dcbH2)2(NCS)2]). In an attempt to minimise the rate constant for charge recombination, Abrahamsson et al. introduced a phenylenethynylene unit between a bpy ligand and the surface anchoring groups (dcpebpy, Fig. 1), preparing the corresponding [Ru(dcebpy)(bpy)(NCS)2] complex. This resulted in a recombination rate three times smaller compared to that for N3.18
Whilst carboxylates represent by far the most commonly encountered anchoring moiety DSSC dyes with other anchoring groups have also been investigated. These include phoshonic acid appended copper(I) and ruthenium(II) complexes19–21 and also boronic acid derivatised complexes.22
In contrast to the wealth of literature on transition metal-based dyes for n-type DSSCs, only a few examples have been reported for NiO p-type cells.23–30 Pellegrin et al. have reported ruthenium(II)-based sensitisers for p-type DSSC devices with phosphonic acid, thiocarboxylate and catechol derived anchoring groups.29 Ji et al. have reported cyclometalated ruthenium complexes of the type [Ru(N^N)2(C^N)]+ as sensitisers for p-type DSSCs.28 Addition of a rigid biphenylene spacer between the carboxylate anchor and the aryl ring of the cyclometalated ligand led to a marked increase in device efficiency (0.05% compared to 0.009% with no spacer). Recently Wood et al. reported bis(bidentate) ruthenium(II) based dye complexes bearing electron rich carboxylate derivatised triarylamine anchoring groups yielding efficiencies of up to 0.09%.27 Massin et al. have also reported carboxylate-appended triarylamine functionalised dyes with a [(Ph2CCRu(dppe)2)] core (dppe = 1,2-bis(diphenylphosphino)ethane).25
Through the use of triazole-based “click” chemistry31 we report here the design and synthesis of the novel anchoring ligand (2,2′-bipyrid-4-yl)-1,2,3-triazole-4,5-dicarboxylic acid (dctzbpy, Fig. 1). Triazole moieties have been utilised in conjugated polymers and results suggested that the linkage is somewhat electronically insulating.32,33 Whilst this might be expected to impair to some extent the rate of charge injection into TiO2 for an immobilised dye, this could significantly retard recombination reactions thereby enhancing overall photovoltaic efficiency. The designed anchor ligand also presents conformational freedom that would enable multiple possibilities for TiO2 surface coordination modes to be envisaged. For example, the various possibilities for coordination by one carboxylate group (monodentate (a), bidentate (b) or bridging (c) in Fig. 2), both carboxylate groups (bidentate (d), tridentate (e), tetradentate (f)) or anchoring through the 4-position carboxylate with additional surface coordination of the triazole-N3 atom (g) could result in highly favourable adsorption characteristics. Further anchoring modes through hydrogen bonding between carboxylic acid and surface oxygen atoms or carboxylate with surface hydroxyl groups can also be envisaged.
We also report the preparation of ruthenium(II), iridium(III) and rhenium(I) complexes AS16-Et2 to AS18-Et2 of the initial diethyl ester of the dctzbpy ligand and subsequent photophysical and electrochemical analyses. Further, we report the hydrolysis of these complexes to their corresponding diacids AS16 to AS18 (Fig. 3) and pilot studies on their utilisation in DSSC test devices with comparison to corresponding dcbH2 complexes 1 to 3.
The 1H NMR spectrum of the product shows seven unique environments (ESI†) for the protons on the bipyridyl fragment along with two sets of signals for the ethyl groups of the ester moieties. This is consistent with the cycloaddition of the acetylene to form the triazole and loss of magnetic equivalence of the two carboxylate groups. The resonances for the triazole-appended pyridine ring appear at δ 8.85, 8.67 and 7.61 and are shifted as a result of the cycloaddition relative to those of the azide starting material (δ 8.69, 8.15 and 7.34).35
Routes to ruthenium, iridium and rhenium dctzbpy complexes [Ru(bpy)2(dctzbpy)][PF6]2 (AS16), [Ir(ppy)2(dctzbpy)][PF6] (AS17, ppyH = 2-phenylpyridine) and [Re(CO)3(dctzbpy)Cl] (AS18) respectively were investigated involving direct reaction of the acid form of the ligand with precursor complexes, however, isolation of the corresponding complexes proved problematic. Isolation of complexes of the intermediate diester ligand, AS16-Et2, AS17-Et2 and AS18-Et2, followed by hydrolysis was deemed to give better results. Thus, two-step syntheses starting from [Ru(bpy)2Cl2], [Ir(ppy)2Cl]2 and [Re(CO)5Cl] were carried out. Firstly, the above mentioned starting metal precursor complexes were reacted together with detzbpy (Scheme 1) followed by anion metathesis with NH4PF6 to yield the desired diester complexes.
As a consequence of the asymmetry of the detzbpy ligand the [Ru(bpy)2] and [Ir(ppy)2] fragments in AS16-Et2 and AS17-Et2 do not possess the C2 symmetry present in 1 and 2. Hence, each bpy and ppy ligand in AS16-Et2 and AS17-Et2 respectively is magnetically unique resulting in complicated 1H NMR spectra due to the overlap of signals (ESI†). The 1H NMR spectrum of AS18-Et2 exhibits detzbpy signals shifted to higher field in comparison with the free diester ligand by ∼0.4 ppm with the resonances for the H-6 and H-6′ position appearing at δ 9.21 and 9.06 respectively.
The final dyes AS16 to AS18 can be readily accessed by hydrolysis with KOH in acetone and subsequent neutralisation. Due to solubility issues, however, and the fact that key properties are expected to differ little after hydrolysis electrochemical characterisation is reported for the more soluble esters AS16-Et2 to AS18-Et2.
Cyclic voltammetry traces and summarised electrochemical data are presented in Fig. 4 and Table 1 respectively. The complex AS16-Et2 presents a reversible Ru(II)/(III) oxidation at +1.00 V and an irreversible reduction peak at −1.50 V assigned to the detzbpy reduction. This is followed by two further reversible reduction peaks assigned to the bpy ligands. A quasi-reversible oxidation is observed at +0.90 V for AS17-Et2, corresponding to the one-electron Ir(III)/Ir(IV) couple. The first reduction presents as a quasi-reversible process at −1.59 V again assigned to be detzbpy ligand. Complex AS18-Et2 is characterised by a quasi-reversible oxidation peak at +1.00 V, in agreement with the potential of other Re(CO)3(dcb-Et2)X-based complexes (X = halide).36 It also presents a reversible detzbpy-based reduction at −1.56 V. The oxidation potentials for these complexes are similar to those of their corresponding dcbH2-based analogues consistent with the expectation of a largely metal-based HOMO.29,36,37 The detzbpy-based reduction potentials (−1.5 to −1.6 V) are more cathodically shifted than that reported for 1 (−1.34 V)29 consistent with a higher energy LUMO as indicated in the spectroscopic data.17–19
Dye | E ox/V | E red/V |
---|---|---|
AS16-Et2 | 1.00 | −1.50 |
AS17-Et2 | 0.90 | −1.59 |
AS18-Et2 | 1.00 | −1.56 |
The isolated and purified complexes AS16-Et2 to AS18-Et2 were then refluxed in KOH/acetone and neutralised with HCl to yield the corresponding dctzbpy complexes. The analogous dcbH2 complexes [Ru(bpy)2(dcbH2)][PF6]2 (1),29 [Ir(ppy)2(dcbH2)][PF6] (2)20 and [Re(CO)3(dcbH2)(Cl)] (3)17 were also prepared for comparison. UV-Visible absorption spectra were recorded for all complexes in acetonitrile solutions at room temperature and are presented in Fig. 5 with summarised data listed in Table 2.
Complex | λ abs/nm (ε/dm3 mol−1 cm−1) | λ emmax/nm | τ/ns |
---|---|---|---|
1 | 245 (21923), 287 (44481), 308 (26079), 357 (7836), 430 (8807), 475 (9880) | 682 | 32 |
2 | 256 (30778), 289 (24016), 377 (6905) | 689 | 33 |
3 | 252 (10289), 303 (8202), 413 (1826) | 725 | 35 |
AS16 | 242 (15624), 287 (30138), 424 (4642), 456 (5719) | 638 | 34 |
AS17 | 255 (44311), 301 (23330), 364 (7771), 415 (1914) | 590 | 25 |
AS18 | 254 (20204), 297 (15317), 397 (3815) | 553 | 38 |
The comparison between the dcbH2 complexes and their dctzbpy analogues shows similar absorption profiles but with a slight blue shift in the lower energy absorptions for complexes AS16–18. All complexes show a strong band at 250–300 nm attributed to π–π* 1LC transitions together with 1MLCT bands of modest intensity (ε ≈ 5000–10000 dm3 mol−1 cm−1) above 400 nm. The blue-shifted absorption bands in the spectra of the dctzbpy complexes suggests that the LUMO is higher in energy than those for the dcbH2 analogues and that the biscarboxytriazole group is less electron withdrawing than the two carboxylate groups bonded directly to the bipyridyl core in dcbH2. Nevertheless, LUMO is correctly positioned with reference to the TiO2 Fermi level for favourable charge injection when adsorbed on a photoanode.4 These similar absorption patterns will be expected to result in comparable photovoltaic performance for the dyes AS16–18 relative to 1–3.
The complexes AS16–18 exhibit broad emission bands between 550 and 650 nm which are similarly blue-shifted relative to their dcbH2 analogues, with similar life-times at about 32 ns. This again is indicative that the LUMO of the dctzbpy ligand, and thus that of its complexes, is higher in energy with respect to dcbH2 thereby leading to the observed destabilisation of 3MLCT T1 states in these complexes.
In order to gain a more complete understanding of the photophysical and electrochemical properties imparted by the new ligand dctzbpy we turned to density functional theory (DFT) calculations. These calculations were carried out on the free acid carboxylic acid complexes AS16–18, partly to reduce computational cost of the extra alkyl groups of the ester moieties, and due to the fact that the spectroscopic absorption properties of the free acid and ester complexes differ little suggesting that they are electronically very similar. Optimised singlet ground state geometries for the three new dyes AS16–18 and model complexes 1–3 were calculated at the B3LYP level of theory using Stuttgart–Dresden relativistic small-core effective core potentials and basis sets for the metallic elements and 6-311G* basis sets for all other atoms. Molecular orbital energies (Fig. 6) and localisations (Fig. 7) were then determined in single-point calculations using the COSMO solvation model (ε = 37.5 for acetonitrile). The HOMO has significant metallic d-orbital character in all cases with additional aryl π* character in the case of AS17 and CO π* and Cl p-orbital character for AS18. In all cases the LUMO is dominated by the dctzbpy ligand and is mostly localised over the bpy fragment. For AS16 there is also a minor contribution from the bpy ligands whilst for AS17 and AS18 there is an additional contribution from the dicarboxytriazole moiety.
Fig. 7 Optimised geometries and plots of HOMO (top) and LUMO (bottom) orbitals for complexes AS16 to AS18. |
Frontier molecular orbital energies are provided in Table 3. In agreement with UV-visible absorption and emission data there is a slight destabilization of both HOMO and LUMO orbitals, but to a greater extent for the latter, for AS16–18 relative to those of their dcbH2 analogues. Thus the HOMO–LUMO gaps for the dctzbpy complexes are an average of 0.12 eV larger than for 1–3 accounting for the experimental spectroscopic data. The ground state frontier molecular orbitals of AS16–18 are thus correctly localised to facilitate optimum charge-transfer directionality with respect to the carboxylate anchor for efficient charge injection when adsorbed onto a photoanode. Moreover, the relative energy of the dctzbpy ligand localised LUMO in complexes AS16–18, being slightly higher than those of the dcbH2 analogues 1 to 3, will inevitably be favourably positioned relative the TiO2 Fermi level in order to facilitate charge injection into the electrode.
Dye | LUMO/eV | HOMO/eV | HOMO–LUMO/eV |
---|---|---|---|
1 | −7.92 | −11.26 | 3.33 |
AS16 | −7.68 | −11.10 | 3.42 |
2 | −5.65 | −8.13 | 2.48 |
AS17 | −5.41 | −8.04 | 2.63 |
3 | −3.51 | −6.00 | 2.49 |
AS18 | −3.30 | −5.94 | 2.64 |
Time-dependent DFT (TDDFT) calculations were carried out on the optimised ground state geometries of each complex in order to determine vertical excitation energies and the nature of the lowest energy singlet excited states. Simulated absorption spectra are overlaid with experimental spectra and shown in Fig. 8 and reveal that predicted transitions correlate well with the experimental spectra. The excitations to the S1 state of all complexes are primarily HOMO → LUMO in character, however, they are of low oscillator strength and will therefore contribute little to the observed absorption spectra. Consistent with the enlarged HOMO–LUMO gap in complexes AS16–18 relative to their respective dcbH2 analogues the S1 transitions occur at shorter wavelengths. The major transitions observed for all complexes between 350 and 550 nm are primarily of 1MLCT character. Higher energy intense absorptions (240 to 350 nm) are assigned as having predominantly 1LC π → π* character. The ruthenium complex AS16 presents two dominating transitions at 452 (S5) and 412 (S8) nm respectively, involving primarily HOMO−2 → LUMO+2 1MLCT character. The iridium complex AS17 exhibits one transition at 421 nm (S4) of mainly HOMO−1 → LUMO 1MLCT/1LLCT character and two transitions at 394 (S5) and 393 (S6) nm with 1MLCT/1ILCT and 1MLCT/1LLCT character respectively. The rhenium complex AS18 exhibits a strong transition at 443 nm (S2) with a predominant composition of HOMO−1 → LUMO 1MLCT character.
Fig. 8 TDDFT calculated absorption spectra for complexes AS16–18 with experimental spectra overlaid. |
The relative positioning of the frontier orbitals in the dctzbpy complexes described would indeed seem to make them amenable to application in the photovoltaic sensitisation of n-type solar cells. We therefore prepared n-type TiO2-based test DSSC devices utilising complexes AS16 to AS18 along with those of the corresponding dcbH2 analogues for comparison.
The free dye AS16 and TiO2-immobilised AS16 were analysed by FTIR spectroscopy and microscopy in an attempt to gain insight into the anchoring mode of the dctzbpy ligand. Unfortunately the data do not enable any definitive conclusions to be drawn.
The principle photovoltaic parameters for the constructed DSSC devices are listed in Table 4. The overall conversion efficiencies η were derived from the equation η = JscVocFF, where Jsc is the short circuit current density, Voc is the open circuit voltage, and FF is the fill factor. Fig. 9 shows the photocurrent–voltage and IPCE traces of the n-type DSSCs based on the new dyes.
Dye | J sc/mA cm−2 | V oc/mV | FF/% | η/% | IPCE/% |
---|---|---|---|---|---|
N719 | 10.7 | 779 | 69 | 5.76 | 65 |
1 | 0.39 | 457 | 57 | 0.1 | 6 |
AS16 | 1.18 | 662 | 78 | 0.61 | 15 |
2 | 1.44 | 633 | 78 | 0.71 | 17 |
AS17 | 0.06 | 485 | 72 | 0.02 | 3 |
3 | 0.36 | 495 | 73 | 0.13 | 6 |
AS18 | 0.24 | 532 | 73 | 0.09 | 5 |
The IPCE values are generally below 10% over the visible region of the spectrum except for those of AS16 and 2 (Fig. 9). The IPCE profiles reflect the absorption profiles of the corresponding dyes; both AS16 and 1 exhibit IPCE maxima coincident with the region in which the complexes have a 1MLCT-based absorption band between 400–500 nm. All the other complexes have absorption maxima between 370 and 420 nm so their IPCE curves show only the tail of these bands into the visible region.
The obtained photovoltaic efficiencies for complexes AS17 and AS18 are lower than those for their dcbH2 analogues determined under identical conditions. This is not unexpected and attributable to their blue-shifted absorption profiles which would result in lower light harvesting efficiency. Further, whilst the LUMO energies for AS16–18 are expected to be in the correct position relative to the TiO2 Fermi level they are higher in energy than those of 1–3. This might imply less efficient overlap of the LUMO with the TiO2 conduction band and consequently lower electron injection efficiency. The best result for the new dyes is obtained for complex AS16 with an efficiency of 0.61% (compared to 0.1% for 1 and 5.76% for the benchmark dye N719 under the same conditions). AS16 achieved the highest open circuit voltage (0.66 V) which might suggest a longer excited state electron lifetime,38 hence a higher electron density on the TiO2 surface. The efficiency for AS17 was dramatically lower than that of its dcbH2 analogue 2. Indeed, the efficiency of 2 (0.71%) exceeds that of AS16 with a reasonably strong optical absorption shoulder when adsorbed on TiO2 (ESI†) that matches the band at 450–550 nm apparent in the IPCE trace. The rhenium complexes AS18 and 3, however, showed very similar Jsc, Voc and η values to each other.
Whilst AS16 indeed shows superior performance over its dcbH2 model in the cells test the performance of the other new dyes, especially in the case of AS17, is disappointing and likely stems from the elevated LUMO associated with the dctzbpy ligand. However, we reasoned that these dyes may yield greater sensitisation efficiency than their dcbH2 analogues in p-type devices for the very same reason.24 We therefore constructed and tested NiO-based p-type cells based on the new dyes and their dcbH2 analogues 1 to 3 along with coumarin C343 as a benchmark comparison. Current–voltage and IPCE plots are provided in Fig. 10 with photovoltaic parameters listed in Table 5.
Dye | J sc/mA cm−2 | V oc/mV | FF/% | η/% | IPCE/% |
---|---|---|---|---|---|
C343 | 0.26 | 105 | 37 | 0.01 | 8 |
1 | 0.076 | 58 | 27 | 0.0012 | 2 |
AS16 | 0.69 | 94 | 42 | 0.028 | 17 |
2 | 0.069 | 134 | 40 | 0.0037 | 3 |
AS17 | 0.14 | 89 | 42 | 0.0052 | 5 |
3 | 0.16 | 77 | 45 | 0.0056 | 6 |
AS18 | 0.15 | 79 | 46 | 0.0055 | 6 |
The AS16 based cell exhibits the highest overall efficiency of all metal complex sensitised p-type cells (0.028% compared to 0.01% for C343) and the highest IPCE of 17%. As might be expected due to the dctzbpy anchoring ligand being less electron withdrawing than dcbH2 the performances of cells using AS16 and AS17 exceed those of 1 and 2 respectively. Indeed, 1 and 2 seem to be desensitisers of NiO in these cells with the current generated below 450 nm most likely stemming from photolysis of the I3− electrolyte as previously noted by Nattestad et al.39 Cells utilising AS18 and 3 yield near identical performance parameters.
The results for AS16 are generally encouraging in terms of dye development but are disappointing when considered in comparison to the benchmark N719. With further ancillary ligand development in combination with the new ligand it may be possible to arrive at much higher efficiency n-type sensitisers. Complexes of the new anchoring ligand dctzbpy may also find potential applications in p-type cells since the data show that the ruthenium(II)-based dye AS16 results in an efficiency three times that of the benchmark standard dye coumarin-C343. When combined with other ligands about a metal centre with greater electron withdrawing character this anchoring ligand provides potential for the development of far more efficient p-type sensitisers. Complexes based on the ligands described here may also find utility as photochemical solar fuel catalysts adsorbed on semiconductor nanoparticles.40 As the complexes here are luminescent and the carboxylate groups can be utilised for bioconjugation complexes bearing the dctzbpy core structure could also be used in biological imaging applications.41
The NiO films were prepared by using an F108-templated precursor solution containing NiCl2 (1 g), Pluronic® co-polymer F108 (1 g), distilled water (3 g) and ethanol (6 g) and the excess was removed by doctor blade. The film was sintered at 450 °C for 30 minutes and additional layers of precursor solution were applied and sintered until the film thickness was ca. 1.5 μm.
The Pt catalyst was deposited on the FTO glass, coating with 10 μL cm−2 of H2PtCl6 solution (5 mM ethanol solution), air dried and heated at 400 °C for 15 minutes. The dye-covered TiO2 or NiO electrodes and Pt-counter electrodes were assembled into a sandwich-type cell and sealed with a Surlyn hot-melt gasket of 60 μm thickness. A solution of 0.5 M TBP, 0.015 M I2, 0.6 M TBAI and 0.1 M GuSCN in acetonitrile was used as electrolyte in the TiO2-based n-type cells whereas an electrolyte containing 0.1 M I2 and 1 M LiI in acetonitrile was used for p-type cells.
1H NMR (400 MHz, CDCl3) δ: 8.85 (d, 3J = 5.28 Hz, 1H, py-H); 8.67 (d, 3J = 2.08 Hz, 1H, py-H); 8.65 (d, 3J = 4.44 Hz, 1H, py-H); 8.45 (d, 3J = 7.92 Hz, 1H, py-H); 7.83 (td, 3J = 7.72, 4J = 1.72 Hz, 1H, py-H); 7.61 (dd, 3J = 5.28, 4J = 2.16 Hz, 1H, py-H); 7.43 (ddd, 1H, 3J = 7.52, 4J = 4.77, 5J = 1.00, py-H); 4.47 (q, 3J = 7.12, 2H, CH2–CH3); 4.46 (q, 3J = 7.12, 2H, CH2–CH3); 1.41 (t, 3J = 7.12 Hz, 3H, CH2–CH3); 1.35 (t, 3J = 7.16 Hz, 3H, CH2–CH3).
13C{1H} NMR (100 MHz, CDCl3) δ: 159.45, 158.90, 158.61, 154.21, 150.91, 149.38, 143.36, 139.38, 137.12, 132.45, 124.69, 121.24, 117.37, 114.59, 63.93, 62.09, 14.20, 13.77.
HRMS (ESI) m/z calcd for C18H17N5O4 367.1280, found 368.1359 (M + H)+.
1H NMR (400 MHz, DMSO-d6) δ: 8.96 (d, 3J = 5.24, 1H, py-H); 8.77 (d, 3J = 4.72, 1H, py-H); 8.61 (d, 4J = 1.36, 1H, py-H); 8.54 (d, 3J = 7.96, 1H, py-H); 8.15 (t, 3J = 7.64, 1H, py-H); 7.81 (d, 3J = 5.20, 4J = 1.72, 1H, py-H); 7.64 (t, 3J = 5.48, 1H, py-H).
13C{1H} NMR (100 MHz, DMSO-d6) δ: 160.67, 158.62, 155.34, 152.77, 150.66, 148.55, 144.94, 139.97, 139.14, 134.14, 125.4, 121.45, 120.7, 116.84.
HRMS (ESI) m/z calcd for C14H9N5O4 311.0654, found 310.0582 (M − H)−.
1H NMR (400 MHz, CD3CN) δ: 8.79 (d, 3J = 2.02, 1H, bpy-H); 8.55–8.49 (m, 5H, bpy-H); 8.12–8.05 (m, 5H, bpy-H); 7.96 (d, 3J = 6.15, 1H, bpy-H); 7.83 (d, 3J = 5.32, 1H, bpy-H); 7.78 (d, 3J = 5.53, 1H, bpy-H); 7.76–7.69 (m, 3H, bpy-H); 7.55 (dd, 3J = 6.15, 3J = 2.20, 1H, bpy-H); 7.48–7.39 (m, 5H, bpy-H); 4.43 (q, 3J = 7.16, 2H, CH2–CH3); 4.31 (q, 3J = 7.07, 2H, CH2–CH3) 1.37 (t, 3J = 7.12, 3H, CH2–CH3); 1.11 (t, 3J = 7.03, 3H, CH2–CH3).
13C{1H} NMR (100 MHz, CD3CN) δ: 159.54; 159.10; 157.74; 156.97, 156.96; 156.93, 156.92; 156.88, 156.87; 156.83; 156.05; 153.52; 152.00; 151.94; 151.91; 151.83; 151.65; 143.10; 140.54, 138.19; 138.10; 138.09; 137.94, 128.41; 127.78; 127.74; 127.70; 127.62; 125.12; 125.08, 124.48; 124.43; 122.04; 119.67; 63.75; 62.25; 13.40; 13.04.
HRMS (ESI) m/z calcd for [C38H33N9O4Ru]2+ 390.5860, found 390.5864 (M)2+.
1H NMR (400 MHz, CD3CN) δ: 8.76 (d, 3J = 2.08, 1H, bpy-H); 8.55–8.46 (m, 5H, bpy-H); 8.13–8.03 (m, 5H, bpy-H); 7.92 (d, 3J = 6.12, 1H, bpy-H); 7.83–7.70 (m, 5H, bpy-H); 7.61 (d, 3J = 6.12, 4J = 2.2, 1H, bpy-H); 7.51–7.40 (m, 5H, bpy-H).
13C{1H} NMR (100 MHz, CD3CN) δ: 159.68, 159.63, 159.21, 157.86, 157.03, 156.99, 156.94, 156.90, 156.88, 156.46, 156.23, 154.69, 152.38, 151.89, 151.86, 151.84, 151.82, 151.81, 151.62, 143.42, 138.08, 138.03, 138.00, 137.96, 128.03, 127.73, 127.72, 127.66, 127.65, 124.75, 124.43, 124.40, 124.31, 121.72, 120.59.
1H NMR (400 MHz, CD3CN) δ: 8.81 (d, 3J = 1.70, 1H, bpy-H); 8.54 (d, 3J = 8.04, 1H, bpy-H); 8.20–8.13 (m, 2H, bpy-H); 8.08 (d, 3J = 8.14, 2H, ppy-H); 8.02 (dd, 3J = 5.78, 4J = 0.78, 1H, bpy-H); 7.86 (td, 3J = 7.35, 4J = 0.84, 2H, ppy-H); 7.82 (d, 3J = 7.62, 2H, ppy-H); 7.72 (dd, 3J = 5.52, 3J = 0.81, 1H, ppy-H); 7.65 (dd, 3J = 6.09, 4J = 2.17, 1H, bpy-H); 7.63 (dd, 3J = 5.96, 4J = 0.81, 1H, bpy-H); 7.56 (t, 3J = 6.30, 1H, bpy-H); 7.09–7.02 (m, 4H, ppy-H); 6.96–6.90 (m, 2H, ppy-H); 6.29 (dd, 3J = 7.75, 4J = 0.88, 1H, ppy-H); 6.26 (dd, 3J = 7.63, 4J = 0.74, 1H, ppy-H); 4.42 (q, 3J = 6.95, 2H, CH2–CH3); 4.31 (qd, 3J = 7.10, 4J = 1.15, 2H, CH2–CH3); 1.36 (t, 3J = 7.10, 3H, CH2–CH3); 1.10 (t, 3J = 7.10, 3H, CH2–CH3).
13C{1H} NMR (100 MHz, CD3CN) δ: 167.35, 167.24, 159.48, 158.15, 157.72, 154.72, 152.48, 150.99, 149.52, 149.49, 149.43, 144.40, 144.09, 143.97, 140.50, 139.62, 138.78, 138.72, 131.80, 131.59, 131.44, 130.49, 130.44, 129.26, 125.37, 124.98, 124.95, 123.66, 123.54, 123.08, 122.82, 122.76, 120.10, 120.01, 119.98, 63.81, 62.24, 13.39, 12.97.
HRMS (ESI) m/z calcd for [C40H33N7O4Ir]+ 867.2230, found 867.2228 (M+).
1H NMR (400 MHz, CD3CN) δ: 8.46 (d, 3J = 6.56 Hz, 1H, bpy-H); 8.11 (td, 3J = 6.28, 4J = 1.24 Hz, 1H, bpy-H); 8.07 (t, 3J = 5.64 Hz, 2H, ppy-H); 8.00 (bs, 1H, bpy-H); 7.97 (dd, 3J = 4.3, 4J = 0.8 Hz, 1H, bpy-H); 7.89–7.84 (m, 2H, ppy-H); 7.81 (d, 3J = 6.08 Hz, 2H, ppy-H); 7.71 (d, 3J = 4.72 Hz, 1H, bpy-H); 7.65 (d, 3J = 4.6 Hz, 1H, ppy-H); 7.63 (d, 3J = 5.16 Hz, 1H, ppy-H); 7.47 (td, 3J = 5.24, 4J = 0.72 Hz, 1H, bpy-H); 7.09–7.02 (m, 5H, bpy-H&ppy-H); 6.97–6.9 (m, 3H, ppy-H); 6.31 (dd, 3J = 6.06, 4J = 0.6 Hz, 1H, ppy-H); 6.28 (dd, 3J = 6.04, 4J = 0.52 Hz, 1H, ppy-H).
13C{1H} NMR (100 MHz, CD3CN) δ: 167.63, 167.49, 157.16, 156.23, 151.26, 150.45, 149.14, 149.11, 144.28, 144.06, 139.99, 139.88, 139.86, 139.84, 139.21, 139.16, 138.36, 138.33, 131.91, 131.67, 131.65, 131.51, 130.31, 130.27, 130.23, 128.11, 124.82, 124.78, 124.33, 123.4, 123.37, 122.32, 122.3.
1H NMR (400 MHz, CD3CN) δ: 9.21 (d, 3J = 5.96, 1H, bpy-H); 9.06 (dd, 3J = 5.38, 3J = 0.70, 1H, bpy-H); 8.70 (d, 3J = 2.10, 1H, bpy-H); 8.44 (d, 3J = 8.18, 1H, bpy-H); 8.23 (dt, 3J = 7.95 1.52, 1H, bpy-H); 7.78 (dd, 3J = 6.08, 3J = 2.34, 1H, bpy-H); 7.69 (dt, 3J = 6.49, 3J = 1.22, 1H, bpy-H); 4.44 (q, 3J = 7.13, 2H, CH2–CH3); 4.41 (q, 3J = 7.02, 2H, CH2–CH3); 1.38 (t, 3J = 7.13, 3H, CH2–CH3); 1.27 (t, 3J = 6.98, 3H, CH2–CH3).
13C{1H} NMR (100 MHz, CD3CN) δ: 197.63, 197.47, 189.26, 159.55, 157.96, 157.87, 154.73, 154.65, 153.25, 144.91, 140.59, 140.22, 131.79, 128.29, 124.65, 121.86, 119.36, 63.94, 62.24, 13.40, 13.07.
HRMS (ESI) m/z calcd for C21H17ClN5O7Re 671.0352, found 689.0694 (M + NH4)+.
1H NMR (400 MHz, DMSO-d6) δ: 8.94 (d, 3J = 5.44, 1H, bpy-H); 8.44 (d, 3J = 8.17, 1H, bpy-H); 8.22 (t, 3J = 7.78, 1H, bpy-H); 7.97 (d, 3J = 6.81, 1H, bpy-H); 7.63 (t, 3J = 6.61, 1H, bpy-H); 7.15 (d, 3J = 2.25, 1H, bpy-H); 6.14 (dd, 3J = 6.95, 4J = 2.64, 1H, bpy-H).
13C{1H} Low solubility, NMR not recorded.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c6dt02905a |
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