Open Access Article
Filipa R. F.
Simoes
a,
Nitin M.
Batra
a,
Abdul-Hamid
Emwas
b and
Pedro M. F. J.
Costa
*a
aKing Abdullah University of Science and Technology (KAUST), Physical Science and Engineering Division, Thuwal 23955-6900, Saudi Arabia. E-mail: pedro.dacosta@kaust.edu.sa
bKing Abdullah University of Science and Technology (KAUST), Core Labs, Thuwal 23955-6900, Saudi Arabia
First published on 18th February 2019
Nanocarbons continue to stimulate the scientific community while their production has also started to reach the industrial scale. With the commercialization of products that are based on materials such as carbon nanotubes (CNTs), it has become imperative to implement reliable quality control protocols for the routine analysis of their chemical composition and structure. Herein, we propose alkaline oxidation (a.k.a., fusion) as a valuable approach to disintegrate the graphitic structure of carbon nanotubes. Using the certified reference material SWCNT-1, it was shown that fusion enables the subsequent determination of elemental concentrations (Ni, Co and Mo) by a routine analytical tool such as inductively coupled plasma optical emission spectroscopy (ICP-OES). Furthermore, the fusion residues were investigated, clarifying that the process does not result in the formation of non-intentional carbon compounds (e.g., carbides or carbonates) or lattice doping (e.g., B doping or Li intercalation).
Historically, two of the most reliable routine tools to quantify metal elements in CNTs are optical emission spectroscopy (OES) and mass spectrometry (MS).11,14,15 These are commonly associated with inductively coupled plasma (ICP) burners. Prior to the ICP-OES/MS analysis, the carbon material needs to be disintegrated and dispersed in a liquid (a.k.a., sample pre-treatment). Fragmenting the sturdy honeycomb-type lattice of graphitic materials effectively constitutes the critical step in the application of these analytical tools for CNTs and other nanocarbons. Dry ashing (i.e., the combustion of carbon) and wet digestion (through the use of strongly oxidizing liquid reagents, e.g., concentrated nitric acid), or eventually a combination of both, are the most common methods to disintegrate CNTs.16,17
To overcome the shortcomings related to time expenditure and the use of high amounts of reagents, novel approaches in sample pre-treatments, such as the use of microwave systems instead of furnaces, have been developed.15,18 Concurrent with these advances, some of us proposed alkaline oxidation (or “fusion”) as an alternative approach to disintegrate CNTs for ICP-based analyses.8 This treatment is normally applied to samples that are impervious to strong acids. Among these are refractory materials such as carbides19,20 and borides, ceramics,21 mineral ores,22,23 marine sediments24,25 and human bones. The application of fusion to carbon materials was previously limited to coal26 and graphite27 but, in 2016, we used it for CNTs and graphene and compared its elemental quantification results with those obtained from wet digestion.8 Among other advantages, when alkaline oxidation is applied to nanocarbons, it offers a simple two-step procedure (fusion followed by glass-bead dissolution) and avoids the use of concentrated acids and/or peroxides. Furthermore, the mass of flux employed is small, i.e., in the range of tens to hundreds of mg. In our previous work,8 due to the absence of certified reference samples, the results were not conclusive. Hence, we looked into the available standards for CNTs28,29 and found that the certified reference material (CRM) SWCNT-1 produced by the National Research Council Canada (NRC)29 would be a good candidate to validate the reliability of fusion as an ICP-OES/MS sample pre-treatment approach. Here, we re-assert and more importantly validate the applicability of the alkaline oxidation approach as an alternative sample preparation method for the quantitative chemical analysis of CNTs by ICP-OES.
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10 ratio) in a Pt crucible and then thoroughly mixing these with a vortex. The two crucibles were taken to the Claisse Eagon2 machine (Malvern Panalytical), which was operated under the optimized parameters listed in Table S1 (in ESI†). Upon cooling, two fused beads (blank and SWCNT-1 mixture) were obtained. Each of these was dissolved in 20 mL of a 10% HNO3 solution and heated for 20 minutes at 130 °C (this temperature is slightly above the boiling point of HNO3 and is used to assist in the dissolution of the glass-beads). Finally, the resulting transparent solutions were transferred to 50 mL vials and ICP-OES analysis was carried out.
| RF power | 1.2 kW |
| Plasma Ar gas flow | 16 L min−1 |
| Auxiliary Ar gas flow | 1.5 L min−1 |
| Nebulizer gas flow | 0.7 L min−1 |
| Sample uptake rate | 1 mL min−1 |
| Sample rinse time | 50 s |
| Sample pump rate | 15 rpm |
| Stabilization delay | 10 s |
The ICP-OES calibration was carried out with single-element solutions of Co, Ni and Mo at concentrations of 1, 5 and 10 mg L−1. All were derived from the respective 1000 ppm single-element standards. A quality control sample (10 mg L−1) and continuing calibration verification (5 mg L−1) solutions were also prepared in order to check the instrument performance and ensure that its precision was not degrading over the period of the analysis.
Transmission electron microscopy (TEM) imaging was generally performed on an FEI TECNAI G2 Spirit TWIN microscope at 120 kV. Further imaging and energy dispersive X-ray spectroscopy (EDS) were carried out in FEI Titan SuperTWIN operated at 300 kV and incorporating an EDAX octane silicon drift detector. To prepare the TEM sample, 1 mg of the as-received SWCNT-1 (or the grinded SWCNT-1 mixture bead) was dispersed in ethanol and drop-casted onto a Holey carbon metal grid (Au or Cu) and then dried in a vacuum oven at 70 °C.
The Raman analysis was done in a WITec Alpha 300RA system with a 532 nm laser and a UHT300 spectrometer. The powdered samples (i.e., the as-received flux and the SWCNT-1) were placed in a silicon wafer and flat-pressed, while the fusion beads were ground with an agate pestle and mortar until they became powder and transferred to the wafer. The OriginPro software was used to plot and process the Raman spectra.
The SS-NMR studies were performed on a Bruker 400 MHz AVANACIII spectrometer equipped with a 4 mm BBO magic angle spinning (MAS) probe (BrukerBioSpin, Germany). To spin a conductive material such as CNTs, the as-received SWCNT-1 was mixed and finely ground with KBr, then packed evenly into a 4 mm zirconia rotor and finally sealed at the open end with a Vespel cap. The 13C NMR spectra were all recorded under the same instrumental parameters and conditions at 12 kHz spinning rate and using one pulse program with 30 degrees flipping angle with a recycle delay time of 10 s. In addition to C, Li and B were probed with SS-NMR. The 7Li and 11B spectra were obtained with 14 kHz spinning rate using 90° one pulse program with recycle delays of 2 s and 3 s, respectively. The Bruker Topspin 3.2 software (Bruker BioSpin, Germany) was used to collect and process the raw data. The OriginPro software was used to plot the figures.
The CHN analysis was performed in a Thermo Scientific Flash 2000 Organic Elemental Analyzer, where combustion occurred for 7 s under an oxygen flow of 300 mL min−1 and a constant He flow of 140 mL min−1.
When the fusion procedure was used, the powder samples (flux and SWCNT-1 mixture) transformed into glass-like beads. Another visible effect was the color change. While the bead of the flux itself (blank) was transparent, that of the SWCNT-1 mixture exhibited a dark-blue hue (Fig. S1†). This color may originate from the formation of transition metal oxides: tetrahedral Co2+ complexes are a known ceramic colorant (e.g., cobalt blue).30 After crushing the SWCNT-1 mixture beads and reducing them to a powder, it was possible to identify and characterize minute amounts of ash. When imaged with TEM, both SWCNTs and catalyst nanoparticles were conspicuously absent, but sub-micron aggregates with no crystalline order were often observed (Fig. 1d and e). The EDS elemental survey performed on these aggregates could not identify the presence of C, Fe, Co, Ni or Mo. However, B and O were very prominent, certainly originating from the borate salt mixture (Fig. 1f). The absence of a C peak was explained by the localized nature of the EDS analysis and the much larger mass of fused flux present after the oxidation of carbon (the sample flux exhibited a 1
:
10 mass ratio of carbon-to-salt). In fact, this was evident when elemental (CHN) analysis was used to quantify the content of carbon in the as-received SWCNT-1 and respective fusion residues. Initially, C represented 90 wt% of the sample, a value that agrees well with the thermogravimetric data presented in the NRC certificate.29 The same analysis when performed in the residues provided values of <1 wt%, thereby confirming the almost complete combustion of various carbonaceous species.
To provide a more reliable overview of the flux and SWCNT-1 mixture in both their pre- and post-fusion states, less-localized means of characterization than TEM were employed. In particular, possible structural changes induced by the fusion process were evaluated with Raman spectroscopy and SS-NMR. The Raman analysis of the flux showed some variations in the pre- and post-fusion states (Fig. S2†). These were in good agreement with previously reported results31 and reflected the crystalline-to-amorphous structural changes that the salt undergoes with melting. As for SWCNT-1, the spectrum of the as-received SWCNT-1 showed intense peaks with maxima at 178 cm−1, 1582 cm−1 and 2650 cm−1 (Fig. 2a); these correspond to the characteristic normal modes of vibration for SWCNTs, i.e., the radial breathing mode (RBM), the tangential mode (G-band) and the second order harmonic of the D-mode (2D-band). Despite slight variation in the laser energy used when compared with that of the NRC certificate (532 nm versus 514 nm), the spectral agreement was clear.29 Following the fusion process, the Raman analysis of the SWCNT-1 mixture residues showed significantly changed spectra (Fig. 2b and S3†). First, and in contrast to the localized TEM and EDS probing, it was possible to identify the presence of solid carbon. Second, despite the higher noise level justified by the much smaller content of carbon present, RBM was absent but both the D- (1348 cm−1) and the G- (1585 cm−1) bands were visible. The D-band, which was practically absent in the spectrum of the as-received SWCNT-1 and commonly associated with sp3-type carbons,32,33 is very prominent in all post-fusion spectra. While the spectrum in Fig. 2b can be interpreted as the fingerprint of a glass-like carbon material, the variability of the spectral signatures in the different locations probed (cf. Fig. S3†) implies that different types of carbon nanotextures co-exist in the residues. Still, it is clear that the radial symmetry of the carbon nanotubes was eliminated.
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| Fig. 2 Raman spectra of (a) as-received SWCNT-1 and (b) fusion residues of the SWCNT-1/salt mixture. | ||
Following the Raman analysis, SS-NMR was performed using different nuclei: 7Li, 11B and 13C. As seen in Fig. S4,† the flux (alkaline salt) undergoes a rearrangement of the BO3 units, a phenomenon expected at high temperatures. As for the SWCNT-1 mixture, the 13C SS-MAS NMR analysis is shown in Fig. 3a and b. In both spectra, the same single peak is present albeit with slightly changed chemical shifts: at 121.6 ppm for the as-received SWCNT-1 (pre-fusion) and at 112.5 ppm for the SWCNT-1 mixture residues (post-fusion). This peak can be assigned to the C
C bond characteristic of the SWCNT lattice. The position of the peak in the spectrum of the as-received SWCNT-1 is consistent with the reported chemical shift of semiconducting SWCNTs,34 the additional down-field shoulder attributed to metallic 13C resonance. As for the SWCNT-1 mixture residues, there is a noticeable broadening of the equivalent peak. This observation can be explained by the overlap of chemical shift anisotropy as the post-fusion sample is expectedly composed of a much more fragmented and disordered collection of carbon particles. Furthermore, the up-field shift indicates the presence of a less electrically conductive sample. Altogether, the SS-NMR analysis concurs with the Raman spectroscopy analysis by proposing the presence of different types of carbon textures in the residues.
In order to investigate the interaction between the alkaline salt (mainly composed of boron and lithium) and the carbon nanotubes, SS-NMR analysis was carried out using the nuclei 11B and 7Li. After comparing the 11B spectrum of the fused flux (Fig. 3c, black line) with the corresponding one from the SWCNT-1 mixture (Fig. 3c, red line), it is evident that the profiles are identical. According to the literature,35,36 it can be inferred that the two resonances obtained with chemical shifts of 3 ppm and 15 ppm are due to BO4− and BO3 species. This indicates that the salt is inert, there are no chemical bonds with carbon, and boron is not doping the carbon lattice. In the case of the 7Li spectra (Fig. 3d), only one chemical environment was identified at 3 ppm. Moreover, the fused spectra were identical for the flux and SWCNT-1 mixture, providing further evidence of the chemical inertness of the salt and the absence of intercalation as well as carbides, carbonates or other carbon-containing species.
After the fusion procedure and subsequent dilution of fused fluxes (blanks) and respective SWCNT-1 mixtures, ICP-OES was used to quantify the three transition metals known to be present in higher concentrations in SWCNT-1: Co, Ni and Mo. The results are summarized in Fig. 4 alongside the corresponding NRC-certified concentrations. Six replicas were studied, which yielded average concentrations (in mg L−1) and standard deviations of 13
116 ± 316 for Co, 11
972 ± 460 for Ni, and 6253 ± 171 for Mo; these values correspond to average recoveries of 82%, 83% and 86% and are within the acceptable range when working with a CRM.37
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| Fig. 4 Concentrations of the most abundant transition metals in SWCNT-1, following a fusion pre-treatment step and measured by ICP-OES (N = 6). | ||
Footnote |
| † Electronic supplementary information (ESI) available. See DOI: 10.1039/c8ay02213e |
| This journal is © The Royal Society of Chemistry 2019 |