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Shenje
a,
Yingqi
Qu
a,
Vladimir
Popik
b and
Susanne
Ullrich
*a
aDepartment of Physics and Astronomy, University of Georgia, Athens, Georgia 30602, USA. E-mail: ullrich@uga.edu
bDepartment of Chemistry, University of Georgia, Athens, Georgia 30602, USA
First published on 16th November 2021
Photo-oxa-dibenzocyclooctyne (Photo-ODIBO) undergoes photodecarbonylation under UV excitation to its bright S2 state, forming a highly reactive cyclooctyne, ODIBO. Following 321 nm excitation with sub-50 fs actinic pulses, the excited state evolution and cyclopropenone bond cleavage with CO release were characterized using femtosecond stimulated Raman spectroscopy and time-dependent density functional theory Raman calculations. Analysis of the photo-ODIBO S2 CO Raman band revealed multi-exponential intensity, peak splitting and frequency-shift dynamics. This suggests a stepwise cleavage of the two C–C bonds in the cyclopropenone structure that is completed within <300 fs after excitation. Evidence of intramolecular vibrational relaxation on the S2 state, concurrent with photodecarbonylation, with dynamics matching previous electronic transient absorption spectroscopy, was also observed. This confirms an excited state, as opposed to ground state, photodecarbonylation mechanism resulting in a vibronically excited photoproduct, ODIBO.
One-photon and multiphoton photodecarbonylation of photo-ODIBO have been demonstrated to produce the cycloalkyne ODIBO efficiently (see Scheme 1). Furthermore, while photo-ODIBO does not react with organic azides or endogenous nucleophiles, the photoconversion product, ODIBO, is highly reactive towards azides. As such, photo-ODIBO is a promising reagent for applications as described above. Further optimization of cycloaddition reaction rates consequently relies on accelerating ODIBO photogeneration which is paramount to the overall reaction kinetics.
Mechanistic studies on the photoconversion of cyclopropenones have primarily focused on electronic absorption spectroscopy supported by theory. However, the broad and overlapping electronic absorption bands of these molecules and ultrafast kinetics render it challenging to resolve the dynamics of cycloalkyne formation fully.3,8,9 Previously, Transient Absorption Spectroscopy (TAS) studies were undertaken to elucidate the photodecarbonylation mechanism. This study revealed that ODIBO formation under 321 nm illumination of photo-ODIBO occurs within less than 294 fs, consistent with the time-scale of an excited state, as opposed to ground state, dissociation process.10 The derived model concurs that the photoexcited S2 state, which is bright in absorption due to its ππ* character, undergoes intramolecular vibrational relaxation to the state minimum concurrent with CO release and formation of the ODIBO product in its lowest excited ππ* state, S1. The quantum yield for photodecarbonylation amounts to approximately 14%. On picosecond and longer time-scales the unconverted photo-ODIBO and newly formed ODIBO subsequently undergo internal conversion and intersystem crossing back to their electronic ground states. The same TAS study revealed an entirely different mechanism following 350 nm photoexcitation. In this case photodecarbonylation and product formation occur on the ground state, via an intermediate and on much longer, nanosecond timescales. This latter pathway resembles the mechanisms reported for related cyclopropenone containing molecular systems. The initial photoinduced ring-opening step results from C–C bond cleavage according to Norrish type I photochemistry and subsequent ground state photodecarbonylation mediated either by a singlet or triplet intermediate.11–13
Femtosecond Stimulated Raman Spectroscopy (FSRS) provides a new avenue for acquiring a deeper insight into the ultrafast photodecarbonylation processes. This technique combines high temporal resolution with superior spectral resolution by using a third, narrowband (0.8 nm) Raman pump beam, in addition to the pump and probe beams used in conventional TAS. This combination allows for the revelation of photochemical reaction dynamics from a vibrational motion perspective.14,15 Utilizing FSRS for direct observation of reaction product formation and molecular dissociation dynamics has also been the subject of numerous studies in the literature because of the exceptional sensitivity and tunability.16–18 With this powerful technique, excited-state vibrational Raman signatures can be monitored with a similar time resolution compared to electronic absorption. Consequently, FSRS data allows the structural evolution (bond cleavage) to be observed with femtosecond resolution, thereby providing valuable and unambiguous insights into reaction kinetics.16,18–21 Cyclopropenones have a three-membered carbon ring structure with an underlying CC double bond, with the third carbon bonded to an oxygen atom (carbonyl group). The release of the carbonyl group during decarbonylation results in a CC triple bond, signifying a dramatic change in the molecular structure. Monitoring the Raman active conjugated CC and CO bonds of photo-ODIBO, specifically the –C7C8–C23 three-membered ring (see Fig. 1) stretching modes can offer valuable information about the molecular structural evolution leading to CO release with greater spectral resolution than conventional TAS.22 At the same time, the appearance dynamics of the CC triple bond stretch elucidates on the ODIBO formation mechanism.
Fig. 1 Photo-ODIBO S2 (a), S1 (b) and S0 (c) Raman spectra calculated using B3LYP TD-DFT. Normal mode identification matching the peak frequency labels in (a), (b), and (c) are provided in Table 1, together with their respective intensities. |
Pursuant to the goal of unraveling the photodecarbonylation mechanism using insights from vibrational dynamics, FSRS experiments with 321 nm excitation were performed on photo-ODIBO and ODIBO. In addition, complimentary ground and excited state Time-Dependent Density Functional Theory (TD-DFT) Raman calculations facilitated the identification and assignment of experimental Raman bands. The combined experimental and theoretical approach leads to a frame-by-frame femtosecond visualization of the CO release and its associated sequence of bond fission and bond formation steps. Ultimately, such molecular level understanding of the photodecarbonylation process can inform the molecular design of cyclopropenone-based photoactive molecules for increased photodecarbonylation efficiency.
During the FSRS measurement, a 50 mM solution of either photo-ODIBO or 1 mM ODIBO in methanol was continuously circulated through a 3 mm pathlength quartz cuvette using a peristaltic pump.
Theoretical Raman calculations were performed in the ORCA quantum chemistry package using density functional theory (DFT).31,32 First, the ground state molecular structures were fully optimized using the Becke, 3-parameter, Lee–Yang–Parr (B3LYP) functional and Split Valence Polarization (SVP) basis set combination.33–36 Frequencies were also computed at the same level of theory to verify that there were no imaginary modes at the final relaxed structure. Next, the time-dependent DFT (TD-DFT) method was used to calculate vertical excitation for the three lowest singlets (S1, S2, and S3) for Photo-ODIBO and ODIBO. Excited-state geometry optimization was selected for the S1 and S2 states for the parent molecule photo-ODIBO and only S1 for ODIBO. Finally, the optimized ground state and excited state geometries were used as inputs for Raman calculations. A scaling factor of 0.9614 was applied to the calculated normal mode frequencies for comparison to experimental data, as reported in the literature.37,38 The same scaling factor was used for similar studies of large multi-ring molecules like flavins and coumarins utilizing the same level of DFT theory.37,39–41
Fig. 2 depicts the most relevant normal modes for photo-ODIBO (S2νCC[PO] – 1575 cm−1, S2νring[PO] – 1599 cm−1, S2νring[PO] – 1605 cm−1, and S2νCO[PO] – 1870 cm−1) and a table summarizing their local mode contributions is provided in the ESI.† It should be noted that S2νCO[PO] involves significant contributions from the three-membered ring with C7 C8–C23 atoms and, as such, it is not a pure carbonyl stretch which explains this mode's Raman activity. From these representations, it is evident that vibrations involving the carbonyl group and the underlying C7C8 double bond (see Scheme 1) in the three-membered ring dominate the spectra in Fig. 1. The Raman frequency for a conjugated carbonyl group falls in the 1600–1900 cm−1 for most compounds containing this type of chromophore.40,42 Among many other factors, this variation in frequency has been attributed to the number of ring attachments, substituents in the molecular structure, and strain in the molecules.41 Galabov et al. also showed that the carbonyl stretch frequency observed from 1715–1822 cm−1 depends on the C–CO–C angle in cyclic ketones. Smaller angles were associated with higher stretch frequencies. Since the C–CO–C angle in the photo-ODIBO S2 structure is relatively small (59.0° at the optimized geometry), the S2νCO[PO] frequency of 1870 cm−1 can be explained by this greater degree of angular strain compared to other cyclic systems.43 The C–CO–C angle at the S0 geometry is 56.9°, shifting the frequency farther to 1893 cm−1 in the calculated Raman spectrum for the S0 state. As shown in Fig. 2, the S2νCC[PO] stretching motion is also coupled with ring modes which could shift these frequencies from pure CC mode positions. The rest of the spectra show contributions from ring and C–H modes as the molecule vibrates in and out of the plane (in and out of the page). The mode visualizations for the S0 and S1 states are similar to Fig. 2 and are provided in ESI† Fig. S2 and S3.
Fig. 2 Visualization of the dominant normal modes in the calculated S2 Raman spectrum of photo-ODIBO. The red bonds in the wireframes represent oxygen atoms and arrows show direction of displacements for each frequency. Modes for the S0 and S1 state of photo-ODIBO are similar and provided in the ESI.† |
Table 1 lists the calculated Raman frequencies, intensities, and a description of the dominant displacements as a summary to Fig. 2 and ESI† Fig. S2, and S3 showing the primary normal modes for photo-ODIBO at the optimized geometries corresponding to the first three singlet states. Starting from the S2, the SnνCC[PO] and SnνCO[PO] (n = 0, 1, 2) modes systematically shift to higher frequencies for the lower-lying states. Since the normal mode frequencies are inversely proportional to bond lengths, the systematic shortening of the CC double bond explains the blueshift of the SnνCC[PO] mode. As discussed above the CO stretch frequency is also sensitive to the C–CO–C angle which induces strain into the three-membered ring as the angle decreases. Overall, the frequency shift of the SnνCO[PO] mode is less pronounced. In the S0, both single bonds are elongated while the CC double bond is shortened, hence leading to a smaller angle compared to the excited states (see ESI† Table S1) and a blueshift of the S0νCO[PO] mode. However, these simplistic explanations do not fully describe the frequency shifts of the CC and CO stretch modes due to local mode displacements involving the entire ring system (see local mode decompositions in ESI†). In the case of the SnνCO[PO] mode, for example, the localization on the carbonyl stretch changes upon electronic excitation and amounts to only 14% in the S2, 13% in S1, but 48% in S0. Not only frequencies but also Raman intensities are related to bond length parameters. Since Raman intensities are proportional to the magnitude of change in polarizability, longer bond lengths are correlated with higher intensity features due their increased polarizability. This effect is most apparent for the CO bond which has the largest length in S1 and the S1νCO[PO] intensity is more than doubled compared to the other states. The S1νCC[PO] intensity is similarly affected due to a strong involvement of the CO stretch in this mode. Furthermore, the intensities for the calculated modes listed in Table 1 are consistently higher in the S1 state compared to the S2 and S0 states, with the S0 state having the lowest intensities. Such a trend could also be related to a general shortening of bond lengths in S0. In the ground state electrons are confined to the valence orbitals whereas in the electronic excited states photoexcited electrons occupy additional previously unoccupied orbitals leading to increased polarizability.
Photo-ODIBO | Frequency (cm−1) | Intensity | Mode |
---|---|---|---|
S0 | 1604 | 494 | Ring |
1642 | 3271 | CC stretch | |
1893 | 838 | CO stretch | |
S1 | 1603 | 4745 | CC stretch |
1606 | 1200 | Ring | |
1887 | 2371 | CO stretch | |
S2 | 1575 | 2607 | CC stretch |
1599 | 1325 | Ring | |
1605 | 853 | Ring | |
1870 | 1018 | CO stretch |
Raman calculations for the photoproduct ODIBO were also undertaken to gain insight into the molecular Raman signatures after CO removal. The ground state spectrum showed an intense 2223 cm−1 vibration of the CC bond (S0νCC[OD]). Other low-intensity ring modes (1612 and 1629 cm−1) and C–H (1172 cm−1) modes were also observed (Fig. 3). For comparison, a combined plot of the Raman spectra for photo-ODIBO S2, S1, and ODIBO S0 is provided in ESI† Fig. S4. Optimization of the S1 state of ODIBO converges with a double bond between C7 and C8, where a triple bond was expected. This optimized structure results in an inconsistent Raman spectrum as a result of this double bond. Therefore, only the S0 Raman calculations are provided. Assuming the same trend as observed in photo-ODIBO calculations, it is expected that the S1νCC[OD] frequency will also be red-shifted with respect to the S0 frequency.
Fig. 3 Raman spectrum and visualizations of the molecular displacements for the dominant normal modes in ODIBO ground state. |
Rising peaks in the FSRS spectrum of photo-ODIBO are of particular interest as potential indicators of ODIBO photoproduct formation. Specifically, observation of the ODIBO CC bond stretch mode, which is expected around the 2100–2250 cm−1 region, would provide unambiguous evidence for the presence of ODIBO.47 Given that the ODIBO quantum yield is low, some of the smaller features are inspected and discussed next. Starting at around 213 fs, a peak at 2165 cm−1 (4) appeared in the spectrum as shown in Fig. 4 and is the most likely candidate for assignment to the S1νCC[OD] mode in the product, ODIBO, because it falls within the expected frequency range and also rises in intensity. For now, this peak is tentatively assigned to S1νCC[OD], but the ODIBO FSRS spectrum discussed in section 2 provides additional confirmation. The ODIBO product formation will also be further quantified by analyzing the rise-time of this S1νCC[OD] peak in Section 3.
Also visible in the Raman spectra are the growth of the 1215 (unmarked) and 2556 cm−1 (5) Raman bands around 131 fs. The lower frequency band falls in the frequency range for ring C–H vibrations and appears to blue-shift from 1215 to 1289 cm−1 in the time range of 1.1 ps, as shown. Such modes are expected for the parent and product molecules and not suitable as markers for characterization of the photodecarbonylation. The higher frequency peak at 2556 cm−1 also shows a blue shift in the 1.1 ps experimental time window; however, the peak position does not match any of the calculated Raman modes for photo-ODIBO S0, S1 or S2, or ODIBO S0. As such, its assignment remains unknown.
The FSRS spectra combined with Raman calculations for ODIBO clearly indicate that the CC stretch marker mode can provide additional evidence for ODIBO formation upon photodecarbonylation of photo-ODIBO. The observation of this mode, given the low concentration of ODIBO, suggests that it should also be detectable in the photo-ODIBO FSRS. However, it is expected that the structure of ODIBO formed upon decarbonylation will differ drastically from the structure of the directly excited product. The molecular backbone attached to the three-membered ring is significantly twisted out of plane (i.e., about the axis of the CO bond) in the photo-ODIBO S2 from which ODIBO will be formed. The decarbonylation product could then inherit this twisted backbone structure as it is formed on ultrafast time scales. Furthermore, the decarbonylation process itself involves a sequence of structural changes starting with bond fissions to release the carbonyl group followed by formation of the CC triplet bond. As the bond between C7 and C8 transitions from a double to a triple bond, the S1νCC[OD] vibrational feature is expected to appear at a frequency that is initially redshifted compared to the ODIBO FSRS. The S1νCC[OD] peak subsequently blueshifts toward the expected position with increasing bond strength. Therefore, the S1νCC[OD] Raman peak observed at 2206 cm−1 in the ODIBO FSRS lends support for assignment of the 2165 cm−1 peak in the photo-ODIBO FSRS to the same mode. A similar structural discrepancy between a decarbonylation product and the direct excitation counterpart was also observed in diphenylcyclopropenone photodecarbonylation by Kuramochi et al.22
Fig. 6a illustrates a splitting of the S2νCO[PO] band into two: a red-shifting band between 1835–1842 cm−1 (left peak) and a second peak blue-shifting in the 1868–1898 cm−1 range (right peak). At 1.1 ps, the lower frequency peak remained around 1842 cm−1 while the higher frequency had shifted to 1898 cm−1. The observed blue-shift for the S2νCO[PO] Raman peak (right peak) is analyzed first. Fig. 6a shows a progressive ∼30 cm−1 net blue shift with increasing delay-time described by a 254 fs time constant, closely matching the dynamics of the first, ultrafast component of the electronic TA spectrum (294 fs, ESI† Fig. S1, for details also see ref. 10). These matching time constants could indicate that the same process is responsible for the shift observed here, i.e., the 254 fs time constant can be assigned to intramolecular vibrational relaxation on the S2 directly after 321 nm excitation, in line with the TAS assignment.10,19,48–51 Due to anharmonicity of vibrational modes, transition frequencies between adjacent vibrational levels decrease for higher quanta of excitation. This results in a time-dependent blueshift of vibrational bands in FSRS spectra during vibrational cooling processes. Cooling either occurs through intramolecular vibrational energy redistribution to other modes (fs–ps timescales) or vibrational energy transfer to the solvent (longer ps timescales). For example, similar peak position blue-shifts have been previously observed in FSRS and time-resolved infrared spectroscopies of the para-nitroaniline NO2 stretch mode by Schrader et al. and were assigned to vibrational cooling involving energy transfer to solvent molecules. The blue-shifting trend was also observed in the CC stretch mode in β-carotene and was similarly assigned.23 Additionally, from the DFT Raman calculation in Table 1, it is also evident that internal conversion from the initially excited S2 state to S1 will likewise blue shift the CO stretch mode, because of its higher frequency in S1 compared to S2. Therefore, an admixture of the decreasing S2 population and increasing population of the S1 state could result in a time-dependent gradual shift of the right peak toward higher frequency due to close-lying and unresolved S2 and S1 CO stretches. Such excited state population changes also impact the observed decrease in intensity of Raman modes, especially for this marker S2νCO[PO] mode, which is discussed below. Overall, the blue shift dynamics of the right peak in Fig. 6a are therefore associated with S2 vibrational cooling and internal conversion dynamics of S2, i.e., SN2 → S02 vibrational relaxation occur on similar timescales as S2 → S1 internal conversion, where N represents a higher-lying vibrational level.52
A possible explanation of the splitting, which leads to an additional red-shifted peak around 1842 cm−1 could be structural changes in photo-ODIBO on the S2 state that are precursors to decarbonylation. For example, lengthening the C7–C23 and C8–C23 bonds in the three-membered ring and increasing the C–CO–C angle will cause a small red-shift (∼7 cm−1) of the S2νCO[PO] feature. This suggests the decarbonylation process competes with and occurs in parallel to the S2 vibrational cooling and internal conversion processes.
Excited-state dynamics after 321 nm excitation are analyzed further by following the intensity of the S2νCO[PO] mode as a function of pump–probe delay. Fig. 6b shows a decrease in intensity with 24–82 fs time constants for both left and right peaks discussed above; afterward, both peaks indicate similar intensity rises described by 117–119 fs time constants. The decay dynamics are ascribed to a change in polarizability during vibrational cooling, the initiation of decarbonylation on S2, and S2 → S1 internal conversion, with the latter process leading to a depopulation of the photo-ODIBO S2 state. In the case of internal conversion, the slight rise in intensity (117, 119 fs time constants, Fig. 6b) could result from the increase in photo-ODIBO S1 population consistent with the observation in the DFT Raman calculations, which showed an enhanced intensity for the S1νCO[PO] compared to the S2νCO[PO] mode. In the case of decarbonylation, the slight intensity increase with around 117, 119 fs time constants can be explained by an aborted decarbonylation in some parent molecules and re-formation of the C–C bond after initial fission. Such increase in S2 population of the original photo-ODIBO parent molecules would also increase the intensity of the measured S2νCO[PO] mode.51,53
Fig. 7a shows a portion of the photo-ODIBO Raman spectrum expanded to highlight the 2100–2300 cm−1 region peaks. Clearly, the right peak (2230 cm−1) decreases in intensity, but at 250 fs a rising peak (left) at 2165 cm−1 is observed and assigned to S1νCC[OD]. This latter peak, which is attributed to the presence of ODIBO in the photo-ODIBO FSRS, is also chosen for further dynamics analysis. The S1νCC[OD] growth is fit with a ∼99 fs rise-time, plotted in red in Fig. 7b. Notably, the rise of this mode is delayed, i.e. becomes a distinguishable feature around ∼200 fs, which is consistent with the subsequent formation of the triple bond after the bond-elongation dynamics shown in Fig. 6b. The kinetics of the 2230 cm−1 (right peak) band intensity is also plotted in black in Fig. 7b. However, the 78 fs decay and 87 fs rise time constants suggest that this 2230 cm−1 band might be unrelated to the product formation but instead represents vibrational cooling and internal conversion dynamics on the S2 state of photo-ODIBO.
Table 2 presents a summary of these primary marker modes, SnνCO[PO] and S1νCC[OD], observed in the photo-ODIBO FSRS spectra. The table also includes the expected peak positions based on TD-DFT calculations.
State and mode | Calculated (cm−1) | Experiment (cm−1) | Delay-time range |
---|---|---|---|
Photo-ODIBO S2 CO | 1870 | 1868–1881 (r) | −65–213 fs |
1835–1842 (l) | ∼213 fs–1.08 ps | ||
Photo-ODIBO S1 CO | 1887 | 1882–1898 (r) | ∼213 fs–150 ps |
1840 (l) | ∼213 fs–1.08 ps | ||
ODIBO S1 CC decarbonylation of photo-ODIBO | — | 2165–2211 | ∼213 fs–150 ps |
ODIBO S1 CCdirect photoexcitation | — | 2206–2228 | 0 fs–29 ps |
Photodecarbonylation involves a drastic change of the three-membered ring with the underlying C6C7 bond (see Scheme 1). Although the interpretation of the CC stretch (S2νCC[PO] mode), is ambiguous due to overlap with other vibrational features, it may provide additional hints as to the mechanistic details. Given that the two bands S2νCO[PO] and S2νCC[PO] (see Fig. 6b and ESI† Fig. S7) show different time constants (24–82 fs and 151 fs, respectively), a two-step decarbonylation mechanism with sequential single bond fissions is considered the most likely. Poloukhtine et al. proposed a step-wise decomposition for a series of cyclopropenones, and Elroby et al. also used this model to explain phenylcyclopropenone (IO) and cyclopropenone (HC(CO)CH) decarbonylation.54,55 Their computational results pointed to a sequential elongation of the C–C bonds in the three-membered ring resulting in CO release.55,56 According to Elroby et al.'s simulation, the C7C8 bond remains intact through the elongation of this first single bond resulting in an intermediate with one ruptured C–C bond in (place of the three-membered ring C7C8–C23). This step is followed by lengthening and eventual breaking of the next C–C bond releasing CO. Throughout this process, the underlying C7C8 bond extends slightly until the carbonyl is released and a C7C8 bond is formed.55,56 A similar model could explain the time evolution of the marker bands in the photo-ODIBO Raman spectra presented in this study. The S2νCO[PO] carbonyl stretch intensity decreases faster (24–83 fs time constant) compared to the S2νCC[PO] band (151 fs time constant) as either C7–C23 or C8–C23 elongates initially and breaks. Meanwhile, the underlying CC bond is retained until the lengthening and fission of the next C–C bond, explaining the longer lifetime for the CC bond stretch Raman intensity. With this proposal in mind, the discrepancy in the dynamics of the primary marker mode S2νCO[PO] (Fig. 6b) and S2νCC[PO] (ESI† Fig. S7) is attributed to a sequential bond fission process. With fission of the second bond, the CC bond forms and the S1νCC[OD] mode of the ODIBO product rises in ∼99 fs in the photo-ODIBO spectrum.
Scheme 2 presents a summary of the relaxation and decarbonylation processes extracted from the FSRS spectra of photo-ODIBO. Immediately after excitation, S2νCO[PO] and S2νCC[PO] mode intensities decreased with 24–82 and ∼151 fs time constants, respectively, followed by a ∼99 fs rise in the S1νCC[OD] mode, indicating the presence of the ODIBO product. The different time constants for CO and CC peak intensity alluded to a step-wise mechanism beginning with elongation of one of the two C–C bonds in the three-membered ring (C8–C23 or C7–C25) and their fission was completed within 151 fs. Subsequent CO release would then follow, leading to a delayed appearance of the rising S1νCC[OD] mode. Since only a small fraction of photo-ODIBO is converted, relaxation dynamics of the photo-ODIBO parent are also observed. Peak splitting of the S2νCO[PO] mode and blue-shifting with a 254 fs time constant matches the decay of the first ultrafast absorption spectrum in the TAS experiment, which solidified its assignment to vibrational cooling dynamics on the S2 state. Intensity dynamics of the feature indicate that S2 → S1 internal conversion may also contribute on these ultrafast timescales.
Footnote |
† Electronic supplementary information (ESI) available: Raman pump and probe spectra, photo-ODIBO and ODIBO geometries, photo-ODIBO S1 and S0 mode visualizations, local mode decompositions of normal modes, and additional FSRS peak kinetics. The fit model used to describe the three-component kinetics of the Raman intensities. See DOI: 10.1039/d1cp03512f |
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