Anika Mauel‡
a,
Björn Pötzschner‡a,
Nora Meidesb,
Renée Siegel
a,
Peter Strohriegl*b and
Jürgen Senker
*a
aDepartment of Inorganic Chemistry III, University of Bayreuth, Universitätsstraße 30, 95447 Bayreuth, Germany. E-mail: Juergen.senker@uni-bayreuth.de
bDepartment of Macromolecular Chemistry I, University of Bayreuth, Universitätsstraße 30, 95447 Bayreuth, Germany. E-mail: Peter.strohriegl@uni-bayreuth.de
First published on 7th April 2022
Weathering of microplastics made of commodity plastics like polystyrene, polypropylene and polyethylene introduces polar polymer defects as a result of photooxidation and mechanical stress. Thus, hydrophobic microplastic particles gradually become hydrophilic, consisting of polar oligomers with a significant amount of oxygen-bearing functional groups. This turnover continuously changes interactions between microplastics and natural colloidal matter. To be able to develop a better understanding of this complex weathering process, quantification of the corresponding defect proportions is a first and essential step. Using polystyrene, 13C enriched at the α position to 23%, we demonstrate that 13C cross polarisation (CP) NMR spectroscopy allows for probing the typical alcohol, peroxo, keto and carboxyl defects. Even the discrimination between in- and end-chain ketones, carboxylic acids and esters as well as ketal functions was possible. Combined with multiCP excitation, defect proportions could be determined with excellent accuracy down to 0.1%. For materials with 13C in natural abundance, this accounts for a detection limit of roughly 1%. The best trade-off between measurement time and accuracy for the quantification of the defect intensities for multiCP excitation was obtained for CP block lengths shorter than 250 μs and total build-up times longer than 2 ms. Further measurement time reduction is possible by using multiCP excitation to calibrate intensities obtained from series of 13C CP MAS NMR spectra. As photooxidation is an important degradation mechanism for microplastics in the environment, we expect these parameters to be transferable for probing defect proportions of weathered microplastics in general.
Degradation of plastics in natural environments plays an important role in understanding the interaction of MP particles with their abiotic and biotic surroundings.12,15,16 Starting from hydrophobic materials, the combination of fragmentation and photooxidation creates substantial numbers of chain scissions, polar defects and crosslinks.17–19 Weathering gradually changes MP polymer chains to highly polar, heavily branched, medium-sized oligomers.17 Polar and charged groups expressed on particle surfaces favour particle cell interactions and cellular responses,20 as well as the formation of an ecocorona by adsorption of natural inorganic and organic colloidal particles21,22 or by deposition of biofilms due to microbe activity.23,24 This in turn enhances the uptake by microorganisms.25,26 Considering that, e.g., weathered PS MP particles accumulate hazardous peroxo groups with proportions of several per cent,17 the uptake of weathered MP is likely to have negative effects on the organisms.26,27 Additionally, the small particle sizes enable fast transport and thus a global distribution.22,28–30
The underlying degradation mechanisms of commodity plastics are meanwhile well understood.2,3,17–19,31–33 PE, PP and PS consist of an aliphatic backbone and aliphatic or aromatic side chains. Light- and stress-induced radical formation in the presence of oxygen leads to (photo)oxidation, subsequent chain scissions and crosslinking (Fig. S4†).18,34–36 As a consequence, a broad variety of functional groups is formed, with the most frequent ones being alcohols, peroxo units, aldehydes, keto groups, carboxy functions and vinyl units.17,18,37–41 The individual defect proportions depend on several factors like chemical composition, solar and stress intensity, oxygen fugacity, salinity, temperature fluctuation and more. As the defect types vary in polarity and the ability to form charges as a function of the pH, a prediction of MP physicochemical properties and subsequent model building is not possible without quantifying the defect proportions.17
Typical defect proportions are on the order of a few per cent, which makes their quantification challenging.17,18 In the past, mostly Fourier Transform Infrared (FTIR), Raman (Ra) and Nuclear Magnetic Resonance (NMR) spectroscopy were used for this purpose.3,17,20,36,42,43 FTIR and Raman spectroscopy are very sensitive and are able to probe defect proportions down to a few per mill, if optimal conditions are reached.3,41 Nevertheless, the detection limit for Ra spectroscopy is influenced by fluorescence.41 FTIR spectroscopy is often used in a semiquantitative fashion by reporting a carbonyl index, which estimates the integral proportion of carbonyl-containing functional groups. Several methods are established to determine the carbonyl index, each leading to a range of possible values.44 Especially, when the attenuated total reflection (ATR) technique is used, the results become surface dependent and require concentration-dependent calibration.3,41 E.g., for weathered LDPE particles, significantly higher carboxyl proportions were detected with FTIR spectroscopy compared to 13C MAS NMR spectroscopy, which was attributed to a preferential accumulation of carboxyl groups close to the surfaces.45 NMR spectroscopy is an element sensitive bulk method and can be used in a quantitative fashion.46 If the samples are soluble, 1H liquid-state NMR spectroscopy provides sufficient sensitivity.42 Nevertheless, an unambiguous assignment is challenging, as most photooxidation defects consist of quaternary carbon atoms.20,47 Using 13C as probe instead, provides a better resolution, however, reduces the sensitivity and often requires labelling. Additionally, signal intensities are influenced by cross relaxation, as the decoupling times, during which the proton bath is saturated, are on the order of the spin–lattice relaxation times.34,37,40,48 They are also influenced by anisotropic spin–spin relaxation, due to the medium slow polymer dynamics.
Polymer defects were also probed using high-resolution 13C solid-state NMR spectroscopy.38,39,49–51 As cross relaxation between 1H and 13C is inefficient for the typically short free induction decay (FID) times, single-pulse (SP) excitation promises sufficient resolution and quantitative intensities.38,39,50 Slow spin–lattice relaxation, however, leads to extremely long measurement times. Most studies thus rely on 13C labelling for probing the weak defect signals. Alternatively, 1H–13C cross polarisation (CP) was applied to enhance sensitivity and reduce measurement times.48,49 As CP excitation is not quantitative, this approach requires calibration.48,49 As an alternative to the insensitive but quantitative SP excitation, recently, the multiCP technique was successfully invoked.17 MultiCP relies on a series of short, successive CP bursts separated by a short waiting period, where the polarisation is stored.52 In this way, T1ρ effects are minimized, allowing the signal intensity of carbon species with small build-up rates to develop properly. 1H–13C multiCP NMR spectra are, therefore, expected to obtain a quantitative character, if the total polarization transfer times are long enough, and were used for a broad variety of materials covering porous, organic and hybrid materials as well as polymers.17,53–58 In particular, for chemical units with small effective heteronuclear dipole sums caused by low proton densities in their vicinity17,53,56,57 and fast molecular dynamics,52,54 significant improvements with deviations from the quantitative intensities below 10% could be reached.57
The quantitative determination of proportions, as low as the ones observed for photooxidative defects, is even more challenging with 13C MAS NMR spectroscopy. Although recently, multiCP excitation was applied to determine quantitative 13C MAS NMR spectra of weathered PS, the low sensitivity coming along with natural abundance prevented to optimise the experimental conditions for the defect resonances themselves.17 However, previous studies suggest that this is crucial.51–57 Depending on the material properties, the number of CP blocks and the block length needed to be varied between 3 to 10 and 15 μs to 1 ms. Therefore, we performed a case study, evaluating the performance of multiCP for the defect quantification of weathered PS MP particles. These were prepared from partially 13C enriched PS (PS-13C) by accelerated weathering. The obtained results provide guidelines for the optimal setup of multiCP experiments in order to excite the markedly different defects introduced upon weathering. As the defect types are similar for most commodity plastics like PE and PP, our results impact on the quantification of polymer defects for a major part of weathered MP in the environment.
Weathering time | Number of blocks, n | Block length, τblockmultiCP | Total pol. time, τtotCP | Waiting time, tz |
---|---|---|---|---|
0 h | 12 | 250 μs | 3000 μs | 3 s |
2400 h | 20 | 150 μs | 3000 μs | 2 s |
13 | 150 μs | 1950 μs | 2 s | |
13 | 150 μs | 1950 μs | 3 s | |
20 | 150 μs | 3000 μs | 3 s | |
12 | 250 μs | 3000 μs | 3 s | |
6 | 500 μs | 3000 μs | 3 s | |
3 | 1000 μs | 3000 μs | 3 s | |
8 | 250 μs | 2000 μs | 3 s | |
1900 h | 8 | 250 μs | 2000 μs | 3 s |
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Fig. 1 Comparison of 13C CP MAS NMR spectra of PS-13C (black) and PS in natural abundance (red) of the particle samples weathered for 2400 h. Both spectra are normalized to the intensity of the ipso carbon resonance at 149 ppm and were shifted horizontally for a better overview (full-scale spectra are given in Fig. S6†). Inset: 13C multiCP MAS spectrum of pristine PS-13C. The relative intensities for the resonances of the ipso carbon(III), the aromatic carbons (IV, V and VI) and the aliphatic carbons (I (enriched), II) were determined by deconvolution. |
13C CP MAS NMR spectra acquired for a set of PS-13C samples after various weathering times are shown in Fig. 2. The improved S/N ratios allow for a more detailed signal assignment due to a better resolution and the possibility to apply spectral editing by contact-time dependent CP measurements. Even for short weathering times, the seven typical resonances (a–e) of the emerging defects were observed. Surprisingly, also for the pristine PS-13C resonances characteristic for alcohol and peroxide units (region around 70–90 ppm) were found. This suggests that already the processing, e.g. the grinding, of the samples introduces some defects, due to the emergence of radicals in the presence of strong mechanical forces,59 as PS-13C is free of any additives.
Contact-time dependent measurements (Fig. 3a) reveal pronounced differences for the build-up behaviour. We use a classic I–S model for the CP build-up60 for the refinement. It reads as
![]() | (1) |
![]() | ||
Fig. 3 (a) Contact-time dependent intensities of the characteristic resonances for weathered PS-13C. The intensities were derived by deconvolution of the 13C CP NMR spectra acquired with contact times between 100 μs and 15 ms. The build-up curve for each defect signal (circles) was normalized to the maximum intensity and refined using eqn (1) (solid lines). The determined values for TIS and T1H1ρ are given in Table S3.† (b) CP build-up time TIS derived from the contact-time dependent build-up curves obtained from the refinements of the CP spectra for the different resonances: (from left to right: ketone groups (a), carboxy groups and esters (b), ketals (c), peroxide groups (d), alcohols (e), ipso carbon, aromatic CH carbons, aliphatic CH and CH2 carbons). The shoulders in resonance (a) and (b) were evaluated together with the main peaks of resonance (a) and (b), respectively, since for short CP build-up times shoulder and main peak could not be resolved and the shape of the resonances for longer build-up times does not change for different build up times (Fig. S7†). Due to the heavily superimposed resonances for the aliphatic CH and CH2 groups, these two signals were also treated with one build-up curve. Typical TIS ranges for quaternary carbons and CHn groups are marked by dashed lines. |
The build-up time constant TIS varies between 90 μs and 1700 μs (Fig. 3b and Table S3†) and the relaxation time constants of 1H within the rotating frame T1H1ρ differ between 1800 μs and 3900 μs (Table S3†). The TIS values for the joint refinement of the CH2 and CH units of the aliphatic backbone and aromatic CH‘s are smaller than 100 μs and thus within the expected range.59 TIS decreases with the number of protons in the vicinity of a carbon atom, and is particularly small if the protons are covalently attached to carbon atoms. The other eight resonances have longer or much longer built-up times ranging from 150 μs for the alcohol resonance to 1700 μs for a resonance at 110 ppm. This resonance could not be detected in previous studies carried out on samples without 13C enrichment due to the small proportion of the corresponding defect. The TIS values for these signals agree with the previous assignment to quaternary carbon atoms, not directly bound to a proton.17,18,37,38
In this way, we assigned (a) ketones (≈200 ppm), (b) carboxy units (172 ppm), (c) ketals (105 ppm), (d) peroxide groups (85 ppm) and (e) alcohols (76 ppm). Due to the improved S/N ratio, a distinction between the alcohol and the peroxide signals is now possible, proving that both defect types are present in weathered PS, which was an open debate up to now.17,18,47 Additionally, the signals for ketone and carboxy groups split into two resonances each (Fig. 2, peaks a/a' and b/b' and Fig S7†). For the ketone signal group, the chemical shift difference of 7 ppm is characteristic for the difference between (a) in- and (a') end-chain ketones. Both types of defects occur, with the low field-shifted in-chain ketones (204 ppm) being less frequent than the end-chain ketones (197 ppm). The intensity ratio of both resonances (1.7 ± 0.3) suggests that roughly 40% in-chain ketones are formed. The splitting for the carboxy resonances implies that, although the majority of –CO2R units consist of carboxylic acids (b), also esters (b') are formed. Their intensity ratio of 4 ± 1 shows that approximately 20% ester groups are formed. The resonance at 105 ppm (c) expresses the typical shift range for vinylidene carbon atoms, which might be a result of the disproportionation reaction (Fig. S4†).18,37 However, the long TIS value of 1.7 ms, contradicts this assignment since it is characteristic for quaternary carbon units. Thus, it is more likely, that this signal is caused by (hemi)ketal formation (Fig. S4†) by a subsequent reaction of the ketones.61 This also explains why this resonance occurs only in later weathering stages after formation of a substantial amount of ketones.
The occurrence of ester and ketal functionalities, suggests two additional crosslinking mechanisms. While C–C bond formation by pairing two radicals dominates early weathering stages, the formation of esters and ketals will become important for later stages, as they require the presence of carboxylic acids, ketones and alcohols in substantial amounts. This explains the surprisingly high crosslinking rates previously observed for weathered PS.17
The accuracy of the defect proportions thus crucially depends on how accurate the quantitative relative intensities can be determined for the corresponding resonances within the 13C multiCP spectra. The high sensitivity provided by PS-13C, enables us to explore the parameter space of the multiCP experiment in a systematic fashion, in particular, for the defect signals. Thus, it provides guidelines and trends to improve the accuracy of future experiments on weathered MP. The multiCP NMR sequence (Fig. S5†) used for this work, is adopted from ref. 51. It consists of a series of n short CP blocks. Between the blocks, a z-filter stores the 1H and 13C polarisation along the external magnetic field. It allows decayed 1H polarisation to relax according to T1H1 and flips back the 1H and 13C polarisation into the xy plane of the doubly rotating frame before the next CP burst. Thus, already created polarisation does not decay and is added to the one generated within the next block.51 If the waiting time tz during the z-filter is much shorter than the spin–lattice relaxation of 13C nuclei and much longer than the one of 1H nuclei (T1H1 ≪ tz ≪ T13C1) and the block length of the individual CP blocks does not become too short, the I–S model can be applied and the intensity build-up of a resonance with a nominal intensity of one follows eqn (2):54
![]() | (2) |
The individual blocks of multiCP experiments should be much shorter than T1H1ρ, to avoid relaxation within the rotating frame. With values between 1.8 ms and 3.9 ms obtained for T1H1ρ (Table S3†), we carried out a set of experiments with block lengths from 1 ms down to 150 μs. According to eqn (2), the total contact time τtotCP should be on the order of or larger than 3 × TIS, which accounts for roughly 95% transfer efficiency. With values for TIS (Table S3†) between 90 μs (CHn groups) and 1000 μs (carboxy units), we chose to record two series of measurements with τtotCP either set to 2 ms or 3 ms. Finally, the waiting time tz during the z-filter should allow for the spin–lattice relaxation of the decayed 1H polarisation and should thus be on the order of 2 × T1H1. However, to avoid significant decay of 13C polarisation, tz ≪ T13C1 also has to be fulfilled. T1H1 was determined to 1.5 s and T13C1 was estimated to be larger than 60 s. Therefore, we explored the influence of tz by collecting 13C multiCP NMR spectra with tz being either 2 s or 3 s. Furthermore, three samples with weathering times of 0 h, 1900 h, and 2400 h were probed. The latter two samples were chosen to guarantee meaningful defect proportions. An overview of all multiCP experiments and values for I∞ for each resonance (eqn (2)) are given in Tables 1 and S4.† With some limitations, I∞ might be used to correct the intensities obtained from multiCP experiments. Additionally, it allows to estimate whether the chosen block lengths and number of blocks are appropriate to avoid heavy losses due to T1H1ρ. To benefit from eqn (2) though, TIS and T1H1ρ need to be determined separately, which might not always be feasible for studies on complex materials like microplastics.
For the chosen block lengths τblockmultiCP and number of blocks n, I∞ varies between 0.60 and 0.98 (Table S4†) suggesting that significant deviations for the intensities are to be expected, in particular for longer τblockmultiCP and smaller n. This trend (Fig. 4 and Table S5†) is nicely reproduced for the relative intensities for the three main resonances of PS-13C (ipso carbon, aromatic CH and aliphatic CH/CH2). For τblockmultiCP of 500 μs and 1 ms (n adjusted to yield a τtotCP of 3 ms) the relative intensities of the signals of the aromatic CH groups and the aliphatic CH/CH2 units are significantly smaller than the expected stoichiometric values (1:
5
:
≈22). The deviation becomes stronger for longer block lengths. For τblockmultiCP = 1 ms, the aromatic CH and aliphatic units are underestimated by roughly 20% to 30% (Fig. 4).
This demonstrates that the block lengths need to be kept short enough to avoid polarisation loss due to T1H1ρ, in particular, for chemical units with small TIS (e.g. CH and CH2) and thus fast build-ups. Consequently, the number of blocks becomes large to adjust the long τtotCP necessary to accommodate for quaternary carbon atoms with large TIS values (Table S3†). For τblockmultiCP of 250 μs and 150 μs the expected relative intensities were obtained. With respect to a nominal intensity of 1 for I(Cipso), I(CHaro) scatters between 5.1 and 5.5 and I(Caliphatic) lies between 21.1 and 22.6. This implies that convergence is reached and that quantitative intensities and thus proportions can be calculated with an accuracy of roughly 10%, estimated from the variation of the determined relative intensities. As similar relative intensities were also obtained for τtotCP = 2 ms, the influence of the total contact-time is less severe in the chosen regime. Especially, for the τblockmultiCP = 150 us measurements (see Fig. S8†), the spectral shape and thus the relative intensities do not change when reducing τtotCP from 3 ms (20 blocks) to 2 ms (13 blocks) or when reducing the waiting time tz to 2 s (Fig. S8†). This indicates that we are already in the limit of sufficient long waiting times tz and total contact-times τtotCP.
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Fig. 4 Comparison of the relative intensities for the aromatic CH units (top) and the aliphatic CH/CH2 groups (bottom) for various multiCP experiments before (blue) and after correcting with I∞ (orange). All relative intensities are given after normalising the intensity for the ipso carbon to one (Table S5†). For small block length average relative intensities of 1![]() ![]() ![]() ![]() |
Using I∞ to correct for lost polarisation during the individual CP blocks allows for compensating the major part of the polarisation losses (Fig. 4). For 13C multiCP experiments with τblockmultiCP = 500/1000 μs average relative intensities of 4.9 for I(CHaromatic) and 19.7 for I(Caliphatic) were reached. Although they are close to the plateau values of 5.4 and 22.0 established from the shorter block lengths, the remaining differences are on the order of 10%. They might be caused by deviations from the I–S model due to coherent polarization transfer, which should be strongest for the proton bearing groups. For smaller τblockmultiCP, I∞ approaches unity and thus leads to small corrections only. Within the limit of the aimed for accuracy of 10%, I∞ might then be neglected. This is important, as for many complex materials the determination of TIS and T1H1ρ, needed to calculate I∞, is challenging and would reduce the applicability of multiCP experiments.
In a second step, the intensities determined from the 13C multiCP NMR spectra were used to calibrate the 13C CP NMR spectra. Calibration factors ci were derived for every resonance as described above (Fig. 5, blue bars and Table S6†). In particular, for the analysis of the defect resonances, the calibration is advantageous, for two reasons. First, a direct comparison to expected proportions is not feasible since the latter are not known in advance. Second, the defect intensities are weak, on the order of roughly 10% of the total accumulated intensity and their intensity changes are easier recognized in the calibration factors ci. Due to its very weak intensity, we exclude the ketal resonance at 110 ppm from this analysis. For comparison, the ci values were also corrected with I∞ (Fig. 5, orange bars and Table S7†), to test how well the I–S model (eqn (2)) can be used to account for polarisation losses, if the block length τblockmultiCP of the CP blocks becomes too long. The general CP conditions were chosen to be the same for both the CP and multiCP experiments. To obtain better S/N ratios though, all CP NMR spectra were obtained with a contact time τtotCP of 2 ms, due to the markedly higher signal intensity compared to 3 ms. Fig. 6 shows the typical differences between a 13C CP (τtotCP = 2ms) and a 13C multiCP spectrum (τCP = 250 μs with 12 blocks and τtotCP = 3 ms). Interestingly, with these conditions the defect intensities derived from the CP NMR spectra are overestimated compared to the quantitative values obtained from the multiCP experiments. As a consequence, all ci values for the defects are smaller than one (Fig. 5).
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Fig. 5 Comparison of calibration factors ci (blue) for the major polymer defects. The ci were derived by dividing the intensities of resonance i, obtained from the 13C multiCP NMR spectrum, by the ones extracted from the 13C CP NMR spectrum. Both NMR spectra are normalised to the same total intensity. Calibration factors ci which are corrected for polarisation loss due to T1H1ρ within the CP blocks according to eqn (2) are given in orange. |
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Fig. 6 Comparison of 13C CP (τtotCP = 2 ms; black line) and multiCP 13C (τblockmultiCP = 250 μs with 12 blocks and τtotCP = 3 ms; red line) MAS NMR spectra for PS-13C weathered for 2400 h. Both spectra are normalized to the same total intensity (full scale spectra are given in Fig. S9†). |
As observed for intensities of the main PS-13C resonances within the 13C multiCP NMR spectra, the ci values for the defects converge for τblockmultiCP smaller than 250 μs to values between 0.6 and 0.7 depending on the defect type. This trend holds for τtotCP of 2 ms and 3 ms as well as for tz of 2 s and 3 s equally, demonstrating that both total contact-times and waiting times are long enough, to guarantee a sufficient polarisation build-up for the polymer defects. For τblockmultiCP larger than 500, the calibration factors grow and approach one for τblockmultiCP = 1000 μs. Correcting the 13C multiCP NMR spectra with I∞ before calibration improves the ci values for τblockmultiCP of 500 μs and 1000 μs markedly. For smaller block lengths the correction is negligible. We attribute the increase in ci for longer τblockmultiCP to polarisation losses for the resonances of the aromatic and aliphatic CH and CH2 units. They exhibit the smallest I∞ of around 0.6 (Table S4†) and thus should suffer the strongest losses.
Underestimating the intensities of the main PS resonances, in turn, leads to an overestimation of the defect intensities and thus an increase for ci. Nevertheless, the corrected ci values do not reach the plateau derived from the experimental data for the smaller block length, suggesting that additional polarisation losses due to, e.g., T13C1ρ and T13C1 relaxation as well as coherent polarisation transfer, beyond the I–S model, are playing a role. While the calibration factors ci for the ipso carbon atoms exhibit the same trend as for the defect ci values, the ones for the aromatic and aliphatic CH and CH2 units are apparently independent of the conditions chosen for the multiCP experiments. As they share similar build-up and relaxation behaviour and account for 95% of the total spectral intensity, calibration leads to constant ci values (Fig. 4).
To show that the optimized experimental conditions for the multiCP experiment (τblockmultiCP = 250 μs, 12 blocks) are meaningful also for samples in natural abundance we remeasured a sample of commercial PS (weathered for 3200 h) from ref. 17, which was previously obtained with a block length of 500 μs and 6 blocks. The comparison between both spectra is given in Fig. S10.† As expected from Fig. 4, the intensity of the aromatic and aliphatic proton bearing groups is enhanced by roughly 20%. Especially the expected intensity ratios 1:
5
:
2 of the three main polystyrene resonances (ipso C, aromatic CH's and aliphatic CH/CH2) are correctly reproduced. In consequence, the total defect proportions amounting to 13% are roughly 20% smaller than the previously reported ones (16.5%).17 This matches the expected trends of the correction factors shown in Fig. 5.
Applying the proposed calibration method, the intensities derived from the 13C CP MAS NMR spectroscopic experiments were calibrated according to the correction factors for τblockmultiCP = 150 μs and 20 blocks (Table S6†). From these spectral intensities, the proportion of the respective defects was calculated according to Meides et al.,17 additionally considering the selective 13C enrichment of 23% at the α position of PS (see ESI† for calculations). Within the probed weathering time, the proportions for all defect types grow with a linear trend. Rates between 6.6 × 10−6 h−1 and 7.7 × 10−6 h−1 were observed, demonstrating that all defect types grow at similar rates. Considering that weathering in our controlled weathering experiment is roughly 5 times faster compared to average central European conditions, the maximum gain of total defect proportions of PS microplastic particles in the environment is extrapolated to roughly 5% per year (Fig. 7). The rates are slightly smaller than observed for commercial non-additivated PS in natural abundance.17 For shorter weathering times, the improved S/N ratio allows for probing even very small defect proportions down to 0.1%. In this way, we show that the implied induction period for ketone formation17 was caused by a lack of sensitivity. Here, a continuous increase of the ketone proportions was observed.
In addition to the typical alcohol, peroxo, keto and carboxy functions already described earlier,17 the higher sensitivity for PS-13C allowed to distinguish between in- and end-chain ketones, carboxylic acids and esters. Even (hemi)ketal functionalities in very low proportions could be identified. The presence of ester and ketal groups suggest that carboxylic acids and ketones react with alcohol units for longer weathering times. They thus introduce two additional crosslinking mechanisms, besides radical pairing and subsequent C–C bond formation. For selected PS-13C samples (0 h, 1900 h and 2400 h weathering times), we characterised 1H and 13C spin–lattice relaxation, which exhibits averaged time constants of 1.5 s (T1H1) and ≈60 s (T13C1) in the laboratory frame and of 3 ms (T1H1ρ) and ≈100 ms (T13C1ρ) in the double rotating frame. The CP build-up time constants TIS, determined via contact-time dependent measurements, vary markedly from 90 μs for CH/CH2 units up to 1 ms for carboxy units. Remarkably, although all defect types are quaternary in nature, already their TIS values reach down to 150 μs.
The broad spread for TIS requires a careful setup for the multiCP experiments. We explored the influence of essential parameters, like number of CP blocks, their block length and the waiting time between the successive blocks, to determine ideal conditions and guidelines for samples with 13C in natural abundance, where an adjustment on the defect resonances themselves is not possible. While the effect on the main resonances of PS-13C (Cipso, CHaromatic and Caliphatic) was best studied on the relative intensities of the 13C multiCP NMR spectra, for the defect resonances i the calibration factors ci = ImultiCPi/ICPi turned out to be more meaningful. We found convergence for all resonances (both main and defects) for total contact-times (τtotCP) and waiting times (tz) longer than 2 ms and 2 s, respectively. This matches previously reported guidelines,51,54 where tz > 2 × T1H1, tz < T13C1 and τtotCP ≈ 3 × TIS should be adjusted. While chemical units with large TIS values turned out to be relative insensitive with respect to the CP block length (τblockmultiCP), in particular, the intensities for the aromatic and aliphatic CH and CH2 units showed large deviations from expected relative intensities for longer block lengths. For a block length of 1 ms already a polarisation loss on the order of 20 to 30% occurred. This effect could be avoided for block length smaller than 250 μs and the best conditions were observed for 150 μs. Thus, to reach a total contact-time larger than 2 ms, a minimum of 8 and 13 blocks is required, respectively.
As weathered MP generally contains a broad mix of defects and functional groups, which may cover the whole range between quaternary and primary carbon atoms, multiCP experiments with block lengths shorter than 250 μs and total contact times longer than 2 ms are advisable for future experiments. This opposes, to a certain extent, previous studies on other complex materials,51–57 where often significantly longer block length were used. The necessary short block lengths, however, increase the measurement time markedly, as the number of repetitions will be large. Collecting 13C multiCP NMR spectra for whole sample series is thus not feasible. We, therefore, suggest to calibrate conventional 13C CP NMR spectra with selectively acquired multiCP experiments. Our results demonstrate that the proposed strategy offers a reasonable fast and accurate way to characterise polymer defects for MP even for 13C in natural abundance and for the low inherent defect proportions. We expect that both the calibration and the obtained parameter range are applicable to other types of commodity plastics and thus will help to overcome the challenge of determining average stoichiometries for weathered MP. In addition, the presented approach will be transferable to a broad range of organic, inorganic and hybrid materials supporting structure determination of complex materials.
Footnotes |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/d2ra00470d |
‡ These authors contributed equally to this work. |
This journal is © The Royal Society of Chemistry 2022 |