Open Access Article
Haosheng
Feng
a,
Shao-Xiong Lennon
Luo
a,
Robert G.
Croy
b,
John M.
Essigmann
b and
Timothy M.
Swager
*a
aInstitute for Soldier Nanotechnologies and Department of Chemistry, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA. E-mail: tswager@mit.edu
bDepartment of Chemistry, Department of Biological Engineering and Center for Environmental Health Sciences, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, Massachusetts 02139, USA
First published on 17th February 2023
Cu(I) from tetrakis(acetonitrile)copper(I) hexafluorophosphate ([Cu(MeCN)4]PF6) was complexed with five structurally related phosphines containing N-heterocycles. The interactions between the resulting complexes and some N-nitrosamines were studied using X-ray crystallography as well as emission spectroscopy. Upon complexation, three phosphine ligands bridge two Cu(I) centers to give paddlewheel type structures that displayed a range of emission wavelengths spanning the visible region. N-Nitrosodimethylamine (NDMA) was shown to coordinate to one of the two copper centers in some of the paddlewheel complexes in the solid state and this interaction also quenches their emissions in solution. The influence of the weakly coordinating anion on crystal and spectroscopic properties of one of the paddlewheel complexes was also examined using tetrakis(acetonitrile)copper(I) perchlorate ([Cu(MeCN)4]ClO4) as an alternative Cu(I) source. Similarly, copper(II) perchlorate hexahydrate (Cu(ClO4)2·6H2O) was used for complexation to observe the impact of metal oxidation state on the two aforementioned properties. Lastly, the spectroscopic properties of the complex between Ph2P(1-Isoquinoline) and Cu(I) was shown to exhibit solvent dependence when the counterion is ClO4−. These Cu(I) complexes are bench stable solids and may be useful materials for developing a fluorescence based detection method for N-nitrosamines.
Current detection methods for N-nitrosamines have been covered recently.1 They are often costly and time intensive, prohibiting monitoring at the consumer level. Alternative detection methods which are cheaper and less sensitive are available, but they involve chemical reactions of/with N-nitrosamines. Such methods require careful execution to avoid interference from breakdown products that may already be present in the sample, such as nitrite and amines. Therefore, it is highly desirable to develop a cost-effective method for direct detection of N-nitrosamines without the involvement of bond rearrangements.
Emission based detection methods can be highly sensitive. Unlike colorimetric measurements based on absorption which are prone to interference from ambient background light,12 emission based methods can make use of the Stokes shift of the analyte and measurement of the emitted light can be achieved without interference from the excitation signal.
Metal complexes represent a promising platform that may respond non-destructively to N-nitrosamines because they can have a vacant site suitable for coordination. N-Nitrosamines are reported to be capable of transition metal coordination,13 typically via the oxygen center.14–16 The preferred oxygen coordination is rationalized by considering resonance structures that include a polar species with a formal negative charge at oxygen, suggesting high electron density at that site (Scheme 1). This model is consistent with a computational study showing that the highest occupied molecular orbital (HOMO) has a significant contribution from oxygen.17 Preceding studies on N-nitrosamine coordination have focused on structural characterization. However, no emission measurements on the complexes were conducted.
In addition to functioning as a binding site, emissive metal complexes are also capable of having longer lifetimes (μs) compared to those of organic molecules (ns). This is a result of the stronger spin–orbit coupling of the metal18 that generates triplet states via intersystem crossing. Longer-lived species displaying phosphorescence19 and thermally activated delayed fluorescence20 have the ability to respond to dynamic quenching events wherein analyte diffusion to the excited species alters its electronic properties. Additionally, longer emission lifetimes can also eliminate background fluorescence in the environment through delayed signal acquisition after the excitation pulse.
Cu(I) based complexes are attractive phosphorescent materials because their fully filled 3d orbitals prevent internal quenching of excited states via dd transitions and hence they can be highly emissive materials.21,22 However, these complexes generally have a preferred tetrahedral geometry in the ground state and a tendency to relax to a planar excited state geometry as a result of metal ligand charge transfer processes.23,24 The result is that Cu(I) excited states can suffer from radiationless decay and low quantum yields. To minimize this undesired relaxation pathway of excited states, complexes must be designed with additional rigidity by appropriate choice of ligands.20 Multiple reviews have been written on luminescent Cu(I) complexes, covering topics such as their photophysical22,25 and structural properties26 as well as potential applications.27
One way of introducing rigidity into Cu(I) complexes is to use binuclear structures. Bidentate ligands containing P and N can create a rigid network that bind Cu(I) salts with weakly coordinating anions such as BF4− or PF6− in paddlewheel type complexes. In the case of phosphine 1 (Fig. 1), not only has the Cu(I) complex been shown to be competent of accepting several solvent molecules as ligands,28 but these materials also exhibit different photophysical parameters in the solid state. Structurally similar Ag(I) complexes29 have also been shown to have nitrile ligands that may be easily exchanged for other organic nitriles. This suggests that these and related complexes may be capable of differentiating between different coordinating analytes, including N-nitrosamines. The phenomenon of ancillary ligands affecting emission properties of Cu(I) complexes has been limited to only few previous investigations.30,31
We have been interested to determine if suitable Cu(I) paddlewheel complexes could be used for N-nitrosamine sensing. To this end we synthesized a series of structurally related phosphines containing different extended N-heterocycles in addition to the previously reported phosphines 1 and 5 (Fig. 1).28,32 We examined a series of Cu(I) complexes and how their emission properties can be tuned. Electronic and steric differences caused the complexes to have different affinities for N-nitrosamines and we have sought to elucidate factors that govern their N-nitrosamines affinity. The effect of weakly coordinating anions and metal oxidation state was also investigated using phosphine 5.
![]() | ||
| Fig. 2 Two possible structures are possible for the binuclear complexes depending on the orientation of the three ligands. Left: head-to-tail (HT) isomer and right: head-to-head (HH) isomer. | ||
Most of the obtained structures crystallized exclusively as one of the two isomers, except for 3-Cu which crystallized as a mixture of the two linkage isomers (2.1.4). One of copper ions is usually four coordinate with an additional solvent ligand assembled during crystallization, and the other copper remains three coordinate. For the HH structures, the ligand is usually acetonitrile, which binds to the copper ion bound to phosphorus.
Consistent with the resonance form of N-nitrosamines, they have a 3-center-4-electron π system and are capable of π type interactions in addition to being a σ donor. As a result of their polar structure, we expected them to be strong σ donor type ligands that could outcompete solvent for coordination to the copper centers. Upon crystallizing from solution in the presence of N-nitrosodimethylamine (NDMA), the solvent ligands are displaced in some complexes (Fig. 3e and f).
![]() | ||
| Fig. 3 Thermal ellipsoid plots of several dinuclear Cu(I) complexes obtained at the 50% probability level alongside their respective schematic representations. (a) 1-Cu, (b) major isomer of 3-Cu, (c) 4-Cu, (d) 5-Cu-ClO4, (e) 1-Cu-NDMA and (f) 4-Cu-NDMA. Hydrogen atoms, counterions (PF6−, ClO4−), solvent molecules and disordered portions have been omitted for clarity. For more detailed information on crystallography data, please refer to the ESI.† | ||
The Cu–O bond distance has a value of 2.194(3) Å, smaller than the sum of van der Waal radii35 of Cu+ and O, which are 1.73 and 1.71 Å respectively. This distance is however longer than that predicted for a Cu–O single bond36 at 1.75 Å. Taken together, this suggests that the interaction is weak. This may be intuitively rationalized since Cu+ has a filled valence shell and the higher energy vacant 4s and 4p orbitals may lack sufficient bonding interactions to the oxygen.
X-ray photoelectron spectroscopy (XPS) results showed that the measured atomic ratios closely match the expected values based on a binuclear structure (Table 1), similar to the other Cu(I) complexes reported herein. The lower than expected value for N might be attributed to some loss of the MeCN ligand under the ultra-high vacuum conditions during data collection. The N 1s spectrum can be deconvoluted into three signals representing uncoordinated and coordinated quinazoline nitrogens37 as well as acetonitrile38 (Fig. S60c†) while the two peaks in the P 2p spectrum are assigned to coordinated phosphines39 as well as PF6− anions40 (Fig. S60e†). No oxidation of Cu(I) was observed based on the absence of Cu(II) satellite peaks (Fig. S60f†).41 Together with high resolution mass spectrometry data showing reasonable fragments of a binuclear structure (4.3.2), we think that it is highly likely for 2-Cu to adopt such a structure in the solid state in the absence of a crystal structure. The single 31P NMR signal (Fig. S25†) may be consistent with a postulated HH structure (Fig. S60a†).
| C | Cu | F | N | P | |
|---|---|---|---|---|---|
| Molecular formula | 62 | 2 | 12 | 7 | 5 |
| Expected atomic ratio (%) | 70.45 | 2.27 | 13.63 | 7.95 | 5.68 |
| Measured atomic ratio (%) | 71.45 | 2.32 | 13.83 | 6.62 | 5.78 |
MeCN served as the ligand to the phosphorus rich Cu1 in both the HT and HH isomers. Cu(I) is classified as soft according to hard–soft acid base concepts,42,43 hence it may have stronger interactions with soft phosphorus, resulting in a more electron rich center compared to the other copper site. The Cu–N bond distance (1.142(3) Å) is comparable to values reported in literature for structurally similar complexes.44 The MeCN molecule also does not interact with Cu1 head on, instead making a Cu1–N4–C91 angle of 165.89(16)°. This deviation from linearity has been observed in other coordination compounds involving Cu(I) and MeCN.45,46 The MeCN molecular fragment remains largely linear with a N4–C91–C92 angle of 178.5(2)°, suggesting that there is no significant back bonding from Cu1. MeCN was not displaced when 3-Cu was crystallized in the presence of NDMA. Crystals under this condition retain MeCN coordination to the phosphorous rich Cu1, although the overall refinement quality of the structure was reduced (Fig. S58, and Table S1†).
:
2 MeCN
:
NDMA in the final refined structure. The NDMA complexation was promoted by using non-coordinating DCM as the crystallizing solvent. The geometry of binding again suggests that NDMA is acting as a σ donor, with a N4A–O1A–Cu1 angle of 123.4(14)°.
:
Cl ratio of 1
:
2 in the empirical formula determined from X-ray diffraction, which revealed a structure with a single copper center surrounded by two ligands (Fig. 4) rather than a paddlewheel structure. Interestingly, the phosphorus centers were oxidized from phosphines to their corresponding phosphine oxides.
![]() | ||
| Fig. 4 Thermal ellipsoid plot of 5-Cu-II at 50% probability alongside its schematic representation. Hydrogens and counterions are omitted for clarity. | ||
The copper adopts a pseudo square planar geometry as is common for Cu(II) complexes, with a O1–N1–O2–N2 torsion of 14.24(6)°. As both Cu(II) and ClO4− exhibit oxidative properties,49,50 either of the two species could have been responsible for the oxidation of P(III) to P(V). However, Cu(II) is the more likely oxidant on account of the stability of product when using [Cu(MeCN)4]ClO4 as a Cu(I) source as well as prior literature describing oxidation of phosphines by Cu(II).51 As the complexation reaction was carried out under air using Cu(ClO4)2·6H2O as the metal precursor, either water or molecular oxygen could have served as the oxygen source. To investigate this, we assembled 5-Cu-II from 5's phosphine oxide (5-O) and repeated our original synthesis from 5 under degassed conditions (Scheme 2). The product from the degassed reaction did not exhibit the broad 1H NMR signals attributable to 5-Cu-II (Fig. S47†), suggesting that molecular oxygen was required for the oxidation of 5 under our reaction conditions. When NDMA was present during crystallization, it was not incorporated into the structure (Fig. S57†).
![]() | ||
| Scheme 2 Two synthetic routes towards 5-Cu-II. Route A: directly from phosphine 5. Route B: oxidation of 5 to its oxide 5-O before its complexation with Cu(II). | ||
This structural motif is consistent with previous reports by Trigulova et al.52,53 who assembled structurally similar complexes directly from phosphine oxides. They could also obtain the Cu(II) complexes via the aerobic oxidation of Cu(I) and its coordinated phosphines during crystallization. In contrast, all obtained complexes with Cu(I) salts presented here were air stable as solids (several months) and in solution over the time span of crystallization (approximately 3 days), suggesting that the aryl rings on phosphine and/or the lower strain in an acyclic phosphine lowers its propensity as well as that of Cu(I) towards aerobic oxidation.
We verified that phosphine 5 did not undergo significant oxidation during emission measurements by synthesizing its oxide 5-O and characterizing its emission under the same experimental conditions. While both 5 and 5-O has an emission around 420 nm which may indicate the presence of some oxidized phosphine, it is only a minor component in 5's emission spectrum (Fig. S61†). Extrapolating this to the other phosphines examined herein suggests that their main emission component measured should originate from their unoxidized forms rather than their oxides.
Phosphine 1 has similar absorption and emission characteristics to that of triphenylphosphine (Ph3P), suggesting that its electronic structure is not significantly perturbed by the pyrimidine substituent. Phosphines 2, 4 and 5 had a local maxima at 314, 330 and 333 nm respectively, while 1 and 3 had monotonically increasing absorbance spectra with no local maxima going from 400 down to 300 nm. Complexation with Cu(I) produces a red shift in the absorption spectra and a shoulder develops towards the lower energy region, which is pronounced for complexes 2-Cu, 3-Cu and 5-Cu-PF6. This feature may be attributed to a charge transfer process between the Cu center and ligands, which has been reported upon in literature for Cu(I) based complexes.28,54 The complexes had molar absorption coefficients (ε) at 275 nm between 1.5–5.4 × 104 M−1 cm−1 (Fig. S69a†), with the complexes bearing ligands 2–5 having higher values and 1-Cu having the lowest values, likely due to the lower π conjugation in pyrimidine compared to the other N-heterocycles. ε values at other selected wavelengths are provided in Table 2.
| Compound | Solvent | λ (nm) | ε (M−1 cm−1) |
|---|---|---|---|
| 1-Cu | CHCl3 | 297 | 14 323 |
| 2-Cu | CHCl3 | 321 | 19 615 |
| 372 | 5347 | ||
| 3-Cu | CHCl3 | 281 | 53 122 |
| 325 | 30 988 |
||
| 4-Cu | MeCN | 264 | 61 849 |
| 317 | 20 082 |
||
| 330 | 24 720 |
||
| 5-Cu-PF6 | CHCl3 | 279 | 37 069 |
| 318 | 33 979 |
||
| 333 | 22 843 |
||
| 5-Cu-PF6 | MeCN | 275 | 26 002 |
| 331 | 16 891 |
||
| 5-Cu-ClO4 | CHCl3 | 279 | 38 163 |
| 316 | 28 927 |
||
| 333 | 21 976 |
||
| 5-Cu-ClO4 | MeCN | 275 | 26 725 |
| 331 | 17 327 |
||
| 5-Cu-II | MeCN | 279 | 10 416 |
| 329 | 9349 | ||
| 345 | 5817 | ||
| 5 | CHCl3 | 279 | 9134 |
| 333 | 5607 | ||
| 5 | MeCN | 279 | 8531 |
| 333 | 5515 | ||
When analyzing steady state measurements, the Raman scattering peak from residual water present in the solvent was removed by performing background subtraction using a solvent-only sample as reference. The emission spectra of the examined compounds were largely broad, consistent with a charge transfer emission pathway reported for similar compound classes (Fig. 5).231-Cu, 2-Cu, 4-Cu and 5-Cu-PF6 have single emission maxima at 610, 605, 530 and 675 nm respectively, while 3-Cu emits primarily at 530 with a slight shoulder at 495 nm. 5-Cu-PF6 has the longest emission wavelength and can be compared to 3-Cu, which is its structural isomer. The smaller degree of red shift when using 3 compared to 5 during complexation has been observed in structurally similar complexes in literature and was attributed to the phosphino substituent in the 1-position stabilizing the lowest unoccupied molecular orbital (LUMO) of isoquinoline more than when it is in the 3-position.23
:
1 integration ratio to the signal at 9.3 ppm indicates that every complex has a bound ligand as each binuclear complex has three P^N ligands.
Fig. S63† shows that the emission spectra of the vacuum treated material is identical to that of the powder, strongly suggesting that the MeCN ligand remains bound under short vacuum exposure. Likewise, we expect this to be the same for other examined complexes.
In the solid phase, 3 of the 5 complexes had their emission spectra blue shifted when compared to in solution while retaining their broad features (Fig. 6). 1-Cu's emission peak shifted from 610 nm in solution to 513 nm in the solid state, 2-Cu's shifted from 605 to 585 nm, and 5-Cu-PF6's shifted from 675 to 640 nm. This phenomenon may be attributed to solvent relaxation effects58 that typically reduce the energy gap between the excited state's ground vibrational level and the ground state. Since this non radiative relaxation pathway is inaccessible in the solid phase, a larger energy gap between excited and ground states is maintained and results in higher energy emissions.
![]() | ||
| Fig. 6 Comparing the emission spectra (λex = 365 nm) of complexes 1–4-Cu and 5-Cu-PF6 as solids (top) and in solution (bottom). Solvents used for solution phase measurements may be found in Fig. 5. | ||
In contrast, 3-Cu's emission profile became less defined and displayed a red shift in the solid phase. It now has a single peak at 600 nm instead of the two peaks in solution. Although the crystal structure suggests the presence of both HH (93%) and HT (7%) species in the solid state and both can therefore contribution to the emission signal, the contribution from the HH isomer should dominate in this case. Lastly, 4-Cu's solid emission profile is narrower and more defined than that in solution. It now displays two peaks at 525 and 550 nm as opposed to its single peak at 530 nm in solution. These observations for 3-Cu and 4-Cu suggest that the complexes may not retain their solid phase structures in solution.
The same trend of increased emission quenching with increasing amounts of NDBA was also observed for 2-Cu, 4-Cu and 5-Cu-PF6 (Fig. S64†). We also performed a preliminary selectivity study for 5-Cu-PF6 using NDBA, NDMA as well as dibutylamine (DBA). We prepared stock solutions of the three analytes in chloroform before adding different amounts to chloroform solutions of 5-Cu-PF6. The results suggest that among the three compounds, NDBA is the best emission quencher, followed by NDMA and lastly DBA (Fig. 8). Since NDBA's quenching ability is larger than the sum of that for NDMA and DBA, it is possible that the nitroso group has a synergistic effect together with the longer alkyl chains. DBA was also compared to NDBA using 4-Cu (Fig. S65†) in acetonitrile solution and DBA barely quenched its emission compared to NDBA. This suggests that the nitroso group plays an important role as an effective quencher of this class of dinuclear copper complexes. It is notable that although N-nitrosamines can undergo photofragmentation and create reactive species upon radiation at 365 nm,1 no significant changes in emission spectra were observed during the quenching studies. This suggests that the Cu(I) complexes are photochemically stable in the presence of N-nitrosamines.
In contrast with the rest of the aforementioned complexes, 3-Cu shows an unusual trend with increasing amounts of NDBA. Its emission profile actually increased in intensity between 0 and 1 equivalent of NDBA. When 2–12 equivalents of NDBA were introduced, the emission spectra first reaches an intensity plateau at 2 equivalents before getting quenched between 4 and 12 equivalents (Fig. 9, and Fig. S66†). This unexpected increase in emission intensity up to a 1
:
1 (3-Cu
:
NDBA) stoichiometry suggests that the complex undergoes a structural change upon irradiation in the presence of NDBA, possibly due to reaction with the NDBA fragmentation products. At super stoichiometric amounts of NDBA, an additional collisional quenching mechanism likely dominates.
As we observe emission quenching for complexes that did not crystallize with NDMA, it appears that the binding interaction between the NDMA oxygen and copper is rather weak. The interaction of NDMA was also investigated by NMR for 5-Cu-ClO4 (Fig. S41 and S42†) and 5-Cu-II (Fig. S46†) and both did not show significant changes in chemical shifts upon NDMA introduction. Therefore, the observed emission quenching in solution is likely a result of collisions between NDBA and the excited complexes rather than the formation of a static NDBA–Cu complex.
Due to its unusual response to NDBA among the complexes examined, more data points were collected for 3-Cu, which had a linear response towards NDBA between 0 and 1 equivalent (Fig. 9). Fitting of the data and solving for the amount of NDBA that would give a normalized emission intensity value (F0/F) corresponding to three times the standard deviation59,60 from the emission intensity at 0 equivalents NDBA (F0) gave a limit of detection value at 0.12 equivalents, or 2.8 ppm (18 μM) at the complex concentration used (150 μM) for titration (Fig. S66†).
In the emission spectra, 5-Cu-ClO4 has a similar spectral shape to 5-Cu-PF6, although the former is less emissive in CHCl3 (Fig. 10e) and has a slightly redshifted emission maximum (695 compared to 675 nm). In MeCN, the trend is reversed with the emission of 5-Cu-PF6 essentially absent whereas 5-Cu-ClO4 has a prominent emission at 458 nm (Fig. 10f). Comparisons with the emission of phosphine 5 in the two solvents demonstrate free phosphine is not present in significant amounts in solutions of 5-Cu-PF6 and 5-Cu-ClO4. Therefore, the anion appears to primarily affect the excited state rather than the ground state of the cationic core. It is possible that similar effects may be observed for the other phosphine ligands (1–4) when switching between weakly coordinating anions.
We were initially puzzled that luminescence measurements on 5-Cu-II gave a detectable signal as Cu(II) ions are often used as quenching agents.61–63 However, there is some literature precedence for luminescent complexes bearing Cu(II) where the ligands are porphyrins64–66 and salens.67 To ensure that our observed emission did not come from impurities, as well as to remove potential side reactions during our initial attempt of oxidizing phosphine 5 in presence of Cu(ClO4)2·6H2O, we assembled 5-Cu-II using an alternate route (Scheme 2). As outlined in route (B), we first oxidised phosphine 5 to its phosphine oxide 5-O. Cu(ClO4)2·6H2O was then used to introduce Cu(II) for complexation. Compared to route (A), the resulting material from route (B) gave a cleaner 1H spectrum without the sharp peaks between 7.5 and 8.6 ppm while maintaining the broad features likely due to the paramagnetic nature of the complex (Fig. S47†). No 31P signals were observed for material obtained via route (B), while a signal at −6.9 ppm was measured for material obtained from route (A). These extraneous signals do not match those from either 5 or 5-O and may hence represent intermediate species during phosphine oxidation.
Nonetheless, 5-Cu-II synthesized from route (B) still displayed luminescence in acetonitrile solution. At first glance, one possible origin for this emission may be uncoordinated 5-O, given that the normalized emission spectra of 5-Cu-II and 5-O are highly similar (Fig. S70a and S70b†). However, the pre-normalization data indicates that even at triple the concentration, 5-O has a lower emission intensity in MeCN compared to 5-Cu-II. Furthermore, the lack of a 31P signal after extended data acquisition indicates that the ligand interacts strongly with Cu(II) and no free ligands are present in solution. The excitation spectra of 5-O and 5-Cu-II are also different, suggesting that 5-Cu-II has a distinct excited state (Fig. S70c and S70d†). Hence, we believe that the complex itself is the most likely source of emission.
5-Cu-II also displayed a more intense emission in MeCN compared to 5-Cu-ClO4 and showed a slightly blue shifted maximum at 430 rather than 458 nm (Fig. 11b), even though 5-Cu-II had the lowest molar absorption coefficients (Fig. S69b†, Table 2). We were not able to produce crystal structures with NDMA, however 5-Cu-II was more sensitive to NDBA addition than 5-Cu-ClO4. Similar to 3-Cu, both 5-Cu-ClO4 and 5-Cu-II demonstrated increasing emission intensity up to one equivalent of NDBA before undergoing quenching at higher equivalents (Fig. 11b and c).
NMR spectra were acquired at the MIT Department of Chemistry Instrumentation Facility (DCIF) on Bruker Avance-III HD Nanobay (400 MHz) and Bruker Avance Neo spectrometers (400 and 500 MHz) at ambient temperatures. Referencing was performed during data acquisition using universal chemical shift referencing against the deuterated solvent used. Data in NMR spectra were reported as detailed below: chemical shift (ppm), integration, peak shape (br = broad, s = singlet, d = doublet, t = triplet, m = multiplet, qu = quintet), coupling constant (Hz). EPR spectrum was acquired on a Bruker EMX-Plus spectrometer with an X-band resonator at 4.5 K.
High resolution mass spectra (HRMS) were acquired on a JEOL AccuTOF 4G LC-plus equipped with an ionSense DART (Direct Analysis in Real Time) source for phosphines 1–5. HRMS for complexes 1-Cu–5-Cu were obtained on an Agilent 6545 mass spectrometer coupled to an Agilent Infinity 1260 LC system running a Jet Stream electrospray ionization (ESI) source.
UV-visible spectra were obtained on an Agilent Cary 4000 running software version 4.20 (468) using a 1 cm path-length quartz cuvette. Fluorescence measurements were performed at room temperature on a Horiba Jobin Yvon Fluorolog 3 and spectra acquired were corrected for solvent background signals as well as for variances in detector sensitivity for different wavelengths. Excitation measurements were made on the same instrument and the data are only corrected for solvent background signals. Quantum yield measurements were performed on a Horiba Quanta-φ F3029 integrating sphere.
Crystallographic data were collected on a Bruker Photon3 CPAD diffractometer using Mo Kα radiation. Structural solution was obtained using SHELXT-2015 and refinement was performed using SHELXL2018/3. The CIF data of complexes are deposited in the Cambridge Structural Database with CCDC numbers of 2218757, 2218758, 2218759, 2218760, 2218761, 2218762, 2218763, 2218764, 2218765 and 2218766.†
X-ray photoelectron spectroscopy (XPS) measurements were performed on a Thermo Scientific K-Alpha + X-ray photoelectron spectrometer using an Al Kα radiation source.
:
2 MeOH
:
H2O in dry ice) and brought down to −20 °C. n-BuLi (1.6 M in hexanes, 3.6 ml, 5.76 mmol) was then added dropwise in 2 batches and stirring continued for 60 min. 2-Chloropyrimidine (656.1 mg, 5.75 mmol) was then added in 4 batches under positive nitrogen flow. The cooling bath was removed and the mixture warmed up to room temperature while stirring over 4 hours. The reaction was quenched with D.I. H2O (5.8 ml) and extracted with EtOAc (3 × 5 ml). The combined organic layer was dried with brine (7 ml) before being removed in vacuo to give the crude product as a yellow solid. Recrystallisation was performed twice (MeOH
:
DCM = 5
:
1) to give the pure product as white translucent crystals (378 mg, 1.43 mmol, 25% yield). Characterization data matches literature values.
δ H (400 MHz, CDCl3, ppm): 8.73 (2 H, d, J = 5.0 Hz), 7.61–7.49 (4 H, m), 7.43–7.38 (6 H, m), 7.15 (1 H, d, J = 5.0 Hz).
δ P{H} (162 MHz, CDCl3, ppm): 1.76.
HRMS(DART+): [C16H14N2P]+m/z = 265.08811, calcd = 265.08891.
:
1 hexanes
:
EtOAc and Et3N (1 vol%) to give the desired product as a pale yellow solid (36.8 mg, 0.12 mmol, 16% yield). The purified product turns increasingly yellow over time under ambient conditions and should be stored under inert atmosphere.
31P NMR of the yellowed material shows the development of a signal likely from the phosphine oxide.
δ H (400 MHz, CDCl3, ppm): 9.35 (1 H, s), 8.00 (1 H, d, J = 8.6 Hz), 7.91–7.85 (2 H, m), 7.64, (1 H, t, J = 6.9 Hz), 7.63–7.58 (4 H, m), 7.43–7.36 (6 H, m).
δ P{H} (162 MHz, CDCl3, ppm): 1.85.
δ C (101 MHz, CDCl3, ppm): 172.29, 172.17, 159.45, 159.37, 150.00, 134.76, 134.56, 134.05, 129.13, 128.56, 128.45, 128.37, 127.90, 127.16, 123.18.
HRMS(DART+): [C20H16N2P]+m/z = 315.10445, calcd = 315.10456.
:
2 MeOH
:
H2O in dry ice) in an oven fried Schlenk flask with a stir bar. n-BuLi (3.6 ml, 1.6 M in hexanes, 5.76 mmol) was added dropwise while stirring to give a deep red solution. Stirring was continued at −20 °C for 10 min after complete addition before removing the cooling bath and stirring for a further 50 min. The 3-chloroisoquinoline solution was then added dropwise and the dark red mixture was stirred overnight (22 h) at r.t. (19 °C). D.I. H2O (5 ml) was used to quench the reaction. The aqueous layer was extracted once with EtOAc (4 ml) and the combined organic layer was washed with brine (7 ml). The solvent was then removed in vacuo to give the crude product as a viscous yellow oil which was further purified via column chromatography (hexanes
:
EtOAc) to give the desired product as a pale-yellow solid (150 mg, 9% yield). Subsequent washing of the solid by minimal cold MeOH removed remaining phosphorus impurities.
Characterization data matches literature values.
δ H (500 MHz, CDCl3, ppm): 9.35 (1 H, s), 7.98 (1 H, d, J = 8.3 Hz), 7.69–7.61 (3 H, m), 7.48–7.42 (5 H, m), 7.41–7.36 (6 H, m).
δ P{H} (203 MHz, CDCl3, ppm): −4.61.
δ C{H} (126 MHz, CDCl3, ppm): 155.98, 155.93, 152.93, 152.83, 136.44, 136.36, 135.58, 135.55, 134.33, 134.18, 130.63, 129.05, 128.67, 128.61, 127.84, 127.60, 127.51, 126.61, 125.64, 125.51.
HRMS(DART+): [C21H17NP]+m/z = 314.10884, calcd = 314.10931.
:
1 EtOH
:
H2O in dry ice) in an oven fried Schlenk flask with a stir bar. N-BuLi (3.6 ml, 1.6 M in hexanes, 5.76 mmol) was added dropwise while stirring to give a deep red solution. The cooling bath was removed after the solution was frozen and the mixture allowed to thaw at r.t. (1 h). Additional anhydrous THF (2 ml) was added to help dissolve residual yellow solid. 2-Chloroquinoline (955.8 mg, 5.84 mmol) was then added in small batches. The red solution turned darker before becoming green after 5 min and increasingly cloudy. The mixture was stirred overnight at r.t. (24 h). D.I. H2O (5 ml) was used to quench the reaction, giving an orange solution phase. The organic layer was isolated and diluted with EtOAc (10 ml) and DCM (10 ml) before filtering off undissolved solids. The filtrate was then washed with brine (5 ml) and dried over anhydrous MgSO4. The solvents were removed in vacuo to give the crude product as a viscous yellow oil which was diluted with 1
:
1 (EtOAc
:
hexane) and filtered over a pad of silica. The purified product was obtained via column chromatography (1
:
1 hexane
:
EtOAc) (317.8 mg, 1.01 mmol, 18% yield) as a pale yellow solid that turns increasingly yellow over time under ambient conditions and should be stored under inert atmosphere.
Characterization data matches literature values.
31P NMR of the yellowed material suggests some oxidation to the phosphine oxide.
δ H (500 MHz, CDCl3, ppm): 8.18 (1 H, d, J = 8.3 Hz), 8.02 (1 H, d, J = 8.3 Hz), 7.79 (1 H, d, J = 8.1 Hz), 7.73 (1 H, t, J = 6.8 Hz), 7.55 (1 H, t, J = 6.93 Hz), 7.52–7.46 (4 H, m), 7.42–7.36 (6 H, m), 7.23 (1 H, d, J = 8 Hz).
δ P (203 MHz, CDCl3, ppm): −2.15 (quintet).
δ C{H} (126 MHz, CDCl3, ppm): 164.91, 147.90, 136.37, 136.28, 135.40, 134.31, 134.16, 129.71, 129.69, 129.07, 128.67, 128.61, 127.63, 126.90, 126.84, 124.39.
HRMS(DART+): [C21H17NP]+m/z = 314.10759, calcd = 314.10931.
:
2 MeOH
:
H2O in dry ice) in an oven fried Schlenk flask with a stir bar. n-BuLi (4.2 ml, 1.6 M in hexanes, 6.72 mmol) was added dropwise while stirring to give a deep red solution. Stirring was continued at −20 °C after complete addition (15 min) before removing the cooling bath and stirring for a further 1.5 h. The 1-chloroisoquinoline solution was then added dropwise and the resulting dark green mixture was stirred overnight (21 h) at r.t. (19 °C). D.I. H2O (2.4 ml) was used to quench the reaction, giving a white precipitate which was isolated via filtration. It was then washed with H2O (10 ml) and Et2O (10 ml) before being dried to give the crude product (1.028 g, 67% yield) which was used for subsequent reactions without further purification.
Characterization data matches literature values.
δ H (400 MHz, CDCl3, ppm): 8.67–8.63 (1 H, m), 8.61 (1 H, d, J = 7.1 Hz), 7.84 (1 H, d, J = 8.2 Hz), 7.67 (1 H, t, J = 7.1 Hz), 7.60 (1 H, d, J = 5.6 Hz), 7.53 (1 H, t, J = 7.1 Hz), 7.47–7.39 (4 H, m), 7.38–7.31 (6 H, m).
δ P{H} (162 MHz, CDCl3, ppm): −8.29.
δ C{H} (101 MHz, CDCl3, ppm): 163.73, 163.63, 143.20, 135.41, 134.60, 134.40, 132.19, 131.90, 130.08, 128.92, 128.44, 128.36, 127.35, 127.33, 127.19, 127.05, 126.82, 120.43.
HRMS(DART+): [C21H17NP]+m/z = 314.10800, calcd = 314.10931.
Characterization data matches literature values.
δ H (400 MHz, CDCl3, ppm): 9.47 (1 H, d, J = 8.5 Hz), 8.65 (1 H, d, J = 5.5 Hz), 7.98–7.84 (2 H, m), 7.79–7.70 (2 H, m), 7.66 (1 H, t, J = 7.7 Hz), 7.61–7.42 (7 H, m).
δ P{H} (162 MHz, CDCl3, ppm): 28.5.
HRMS(ESI+) [C21H17NPO]+m/z = 330.1047, calcd = 330.1048.
:
1 MeOH
:
DCM (5 ml) was added to the crude material before centrifuging the mixture and isolating the supernatant. The supernatant was slowly evaporated overnight to give crystals that fluoresce green.
δ H (500 MHz, CD3OD, ppm): 9.10 (br s), 7.74 (br s), 7.44 (t, J = 7.3 Hz), 7.28 (t, J = 8.0 Hz), 7.16 (br s).
δ P (203 MHz, CD3OD, ppm): 9.84 (br s), −144.60 (quintet, J = 707 Hz, PF6−).
δ F (471 MHz, CD3OD, ppm): −74.74 (d, J = 707.4 Hz, PF6−).
HRMS(ESI+): [C48H39CuN6P3]+m/z = 855.1743, calcd = 855.1745. [C32H26CuN4P2]+m/z = 591.0922, calcd = 591.0929. [C16H13CuN2P]+m/z = 327.0109, calcd = 327.0112.
δ H (400 MHz, CDCl3, ppm) 9.94 (br s), 8.29 (br s), 8.09 (t, J = 7.7 Hz), 7.94 (br s), 7.87 (t, J = 7.1 Hz), 7.16 (br s), 7.09 (br s).
δ P{H} (162 MHz, CDCl3, ppm): 10.68 (br s), −144.03 (sept, PF6−).
δ C (101 MHz, CDCl3, ppm) 161.44, 149.10, 137.14, 133.14, 131.02, 130.80, 128.89, 128.22.
HRMS(ESI+): [C2H3CuN]+m/z = 103.9554, calcd = 103.9562. [C60H45CuN6P3]+m/z = 1005.2242, calcd = 1005.2215. [C40H30CuN4P2]+m/z = 691.1262, calcd = 691.1242. [C22H18CuN3P]+m/z = 418.0545, calcd = 418.0534. [C20H15CuN2P]+m/z = 377.0271, calcd = 377.0269.
δ H (500 MHz, CDCl3, ppm): 10.14 (br s), 9.75 (br s), 8.50 (br s), 8.25 (br s), 7.82 (br s), 7.58 (br s), 7.09 (br s).
δ P{H} (203 MHz, CDCl3, ppm): 2.56 (br s), −144.00 (quintet, PF6−).
δ C{H} (126 MHz, CDCl3, ppm) 155.78, 134.75, 132.89, 130.73, 129.04, 126.50.
HRMS(ESI+): [C2H3CuN]+m/z = 103.9554, calcd = 103.9562. [C63H48CuN3P3]+m/z = 1002.2375, calcd = 1002.2357. [C42H32CuN2P2]+m/z = 689.1352, calcd = 689.1337. [C23H19CuN2P]+m/z = 417.0590, calcd = 417.0582. [C21H16CuNP]+m/z = 376.0321, calcd = 376.0316.
δ H (500 MHz, CD3CN, ppm) 7.91 (br s), 7.80 (t, J = 8.8 Hz), 7.72 (t, J = 7.64 Hz), 7.61 (t, J = 8.0 Hz), 7.54 (t, J = 7.9 Hz), 7.50 (t, J = 7.7 (Hz)), 7.40 (t, J = 7.3 Hz).
δ P{H} (203 MHz, CD3CN, ppm): 0.26 (br s), −144.63 (sept, PF6−).
δ C (126 MHz, CD3CN, ppm): 135.18, 135.06, 131.44, 131.20, 129.81, 129.74, 129.01, 128.58, 128.06, 124.95, 124.77.
HRMS(ESI+): [C2H3CuN]+m/z = 103.9554, calcd = 103.9562. [C63H48CuN3P3]+m/z = 1002.2385, calcd = 1002.2357. [C42H32CuN2P2]+m/z = 689.1359, calcd = 689.1337. [C23H19CuN2P]+m/z = 417.0586, calcd = 417.0582. [C21H16CuNP]+m/z = 376.0317, calcd = 376.0316.
δ H (500 MHz, CDCl3, ppm): 9.42 (br s), 9.27 (br s), 8.41 (br s), 8.02 (br s), 7.68 (br s), 7.37 (br s), 7.16 (br s), 6.73.
δ F (471 MHz, CDCl3, ppm): −73 (d, PF6−).
δ P{H} (203 MHz, CDCl3, ppm): 14.60 (2 P, br s), 7.79 (1 P, br s), −144.04 (2 P, quintet, PF6−).
HRMS(ESI+): [C2H3CuN]+m/z = 103.9554, calcd = 103.9562. [C63H48CuN3P3]+m/z = 1002.2332, calcd = 1002.2357. [C42H32CuN2P2]+m/z = 689.1354, calcd = 689.1337. [C23H19CuN2P]+m/z = 417.0585, calcd = 417.0582. [C21H16CuNP]+m/z = 376.0316, calcd = 376.0316.
δ H (500 MHz, CDCl3, ppm): 9.46 (1 H d, J = 4.1 Hz), 8.42 (1 H, br s), 8.00 (1 H, d, J = 8.0 Hz), 7.66 (1 H, t, J = 6.9 Hz), 7.39 (1 H, d, J = 8.8 Hz), 7.18 7.26–6.9 (9 H, br d).
δ P (203 MHz, CDCl3, ppm): 13.41 (2 P, br s), 7.10 (1 P, br s).
HRMS(ESI+): [C2H3CuN]+m/z = 103.9554, calcd = 103.9562. [C63H48CuN3P3]+m/z = 1002.2305, calcd = 1002.2357. [C42H32CuN2P2]+m/z = 689.1333, calcd = 689.1337. [C23H19CuN2P]+m/z = 417.0586, calcd = 417.0582. [C21H16CuNP]+m/z = 376.0318, calcd = 376.0316.
δ H (500 MHz, CDCl3, ppm): 9.42 (1 H, d, J = 5.5 Hz), 8.42 (br s), 8.00 (1 H, d, J = 8.2 Hz), 7.65 (1 H, t, J = 7.3 Hz), 7.38 (1 H, d, J = 8.1 Hz), 7.25–7.69 (2 H, br d), 3.82 (10 H, s, NDMA), 3.10 (10 H, s, NDMA).
δ P (203 MHz, CDCl3, ppm): 13.34 (2 P, br s), 6.72 (1 P, br s).
δ H (500 MHz, CD3CN, ppm): 11.47 (br s), 10.39 (br s), 8.84 (br s), 8.59 (d, J = 8.7 Hz), 8.38(s), 8.30 (d, J = 8.5 Hz), 8.17 (t, J = 7.9 Hz), 7.90 (t, J = 7.9 Hz), 7.65 (t, J = 7.1 Hz), 7.60–7.50 (m), 7.24 (br s), 6.38 (br s), 5.90 (br s).
δ P (203 MHz, CD3CN, ppm): −6.88 (s).
HRMS(ESI+): [C42H32CuN2O2P2]+m/z = 721.1245, calcd = 721.1235. [C21H16CuNOP]+m/z = 392.0266, calcd = 392.0266. [C21H17NOP]+m/z = 330.1045, calcd = 330.0970. [C23H19N2OP]+m/z = 433.0535, calcd = 433.0531.
δ H (500 MHz, CD3CN, ppm): 10.7 (br s), 9.87 (br s), 8.55 (br s), 7.64 (br s), 6.68 (br s), 6.23 (br s).
δ P (203 MHz, CD3CN, ppm): no signal.
HRMS(ESI+): [C42H32CuN2O2P2]+m/z = 721.1241, calcd = 721.1235. [C21H16CuNOP]+m/z = 392.0268, calcd = 392.0266.
δ H (500 MHz, CD3CN, ppm): 11.31 (br s), 10.29 (br s), 8.78 (br s), 8.60 (d, J = 9 Hz), 8.37 (m), 8.30 (d, J = 8.3 Hz), 8.18 (t, J = 7.8 Hz), 7.90 (t, J = 7.7 Hz), 7.61–7.61 (m), 7.60–7.49 (m), 7.31 (br s), 6.45 (br s), 5.97 (br s), 3.75 (s, NDMA), 3.03 (s, NDMA).
Footnotes |
| † Electronic supplementary information (ESI) available. CCDC 2218757–2218766. For ESI and crystallographic data in CIF or other electronic format see DOI: https://doi.org/10.1039/d2dt03848j |
| ‡ Please refer to Experimental details section in ESI for more details. |
| This journal is © The Royal Society of Chemistry 2023 |