Matthias
Balski
ab,
Heinrich
Kipphardt
*a,
Achim
Berger
a,
Sylke
Meyer
c and
Ulrich
Panne
ab
aBAM Federal Institute for Materials Research and Testing, Richard-Willstaetter-Str. 11, 12489 Berlin, Germany. E-mail: heinrich.kipphardt@bam.de; Fax: +49 30 8104 1117; Tel: +49 30 8104 1116
bHumboldt University of Berlin, Brook-Tylor-Str. 1, 12489 Berlin, Germany
cFraunhofer Center for Silicon Photovoltaics CSP, Walter-Huelse-Str. 1, 06120 Halle (Saale), Germany. E-mail: sylke.meyer@csp.fraunhofer.de; Fax: +49 345 5589 101; Tel: +49 345 5589 5116
First published on 30th August 2013
A method for the determination of 22 trace impurities in solar grade silicon after dissolution in a mixture of HF and HNO3 and subsequent matrix evaporation is reported. The presented method involves a simple, inexpensive, one-vessel sample preparation apparatus design. The recoveries of B, Na, Mg, Al, P, K, Ca, Ti, Cr, Mn, Fe, Co, Ni, Cu, Zn, Ga, Ge, As, Mo, Sb, W, and Tl at 250 μg kg−1 level are in the range of 93 to 108%. After careful selection of monitored isotopes and their respective resolutions, a sector field mass spectrometer has been used to carry out the measurements. Limits of determination down to 120 ng kg−1 have been obtained using a calibration by three-point standard addition. The method was tested on diluted NIST SRM 57b silicon powder as well as on synthetic test samples and also applied successfully on raw solar grade silicon samples in an interlaboratory comparison including NAA.
The efficiency of silicon solar cells can be deteriorated by a broad range of elements, especially transition metals, at concentrations as low as 100 ng kg−1 in the case of Mo and W2. The inhomogeneous distribution of impurities present in silicon, especially in not recrystallized raw and feedstock silicon, makes the comparison of different methods difficult. Both local and volume analyses are needed to fully characterize the material. Laser ablation (LA)-ICP-MS3 requires a minimum of sample preparation, offering excellent spatial resolution down to a few micrometers and is well suited to measure the spatial distribution of analytes and the homogeneity of the sample, but is mostly limited to materials with higher impurity contents like raw or metallurgical grade silicon due to limits of determination in the μg g−1 range. Out of the techniques analytical chemistry has to offer, only a few feature the topmost aptitude in limits of determination and multi-element capability needed for analysis of re-crystallized, e.g. by the Czochralski process, solar grade silicon, of which in turn some lack the ability of easy, reliable calibration. Namely, neutron activation analysis (NAA)4–6 and glow discharge mass spectrometry (GD-MS)5,7 are relevant instrumental methods, while wet chemical methods are usually applied with ICP-MS as a detection method.
Thermal neutron activation analysis is well suited to examine impurities in semiconductor silicon. Since the cross-section of silicon for thermal neutron capture is relatively small, the sample mass can be in grams without neutron self-shielding becoming a limiting factor. Because of a low atomic number, gamma ray attenuation is not a problem. Furthermore, on activation of silicon, only one radioactive isotope 31Si is produced which has a short half-life of 2.62 h. Thus, waiting a few half-life times before starting the measurements, interfering background from the matrix can be avoided, leading to very low detection limits in the fg g−1 range for selected elements.8,9 Etching after irradiation prevents surface and saw contaminations that otherwise might falsify the results.5 The integrated measurement approach allows monitoring of the mean, bulk crystal purity. In this way, the NAA has become a kind of accepted reference analytical method especially in the semiconductor industry. However, the capabilities of this method do not comprehend the determination of all interesting elements with the desired sensitivity. Moreover, its high instrumental requirements and expenses due to the necessity of a neutron source and radiochemical laboratory make it expensive and difficult to access. Although some efforts have been made to shorten the time requirement for NAA measurements,10 the long response time of this technique makes it not suitable for regular analysis and on-line monitoring.
Especially in comparative studies, glow discharge mass spectrometry offers a very broad range of benefits for routine analysis such as short preparation and analysis time and high sample throughput. However, quantification with this method requires matrix matched standards for calibration with small uncertainty, which are not available. Recently, a study on relative sensitivity factors has been published,11 which opens the gate to quantitative analysis with small uncertainty with this technique. However it does not cover all elements of interest. The high amount of impurities in the synthetic sample used there may also alter the physical properties of silicon, notably the conductivity, compared to rather pure solar grade silicon. This might lead to falsified results especially in direct current GD-MS. Such calibration can be performed rather with techniques like pulsed and/or radiofrequency GD-MS,12 which are way less sensitive to changes in the conductivity of the samples.
Wet chemical based approaches offer a wide range of possible couplings with different methods of atomic spectroscopy for detection. Calibration of wet-chemical methods is achieved very easily by external calibration or standard addition. Attention has to be paid to the sample preparation methods, as they tend to be time-consuming and often leading to elevated blanks owing to contamination during sample handling. Analyte losses may occur through evaporation at high-temperature steps or adsorption on container walls.
A nearly universal analytical tool for inorganic trace determination is the inductively coupled plasma (ICP), often used in coupling with mass spectrometers (MS) as an analyzer and a detector. With this multi-element technique, virtually all elements of the periodic table are accessible with very low limits of determination and a wide dynamic range. One of the main limitations of this technique is the occurrence of spectral interferences due to formation of polyatomic ions or the isobaric isotopes of different elements. A dynamic reaction cell can be used to countervail the former, while for the latter, high-resolution double-focusing sector-field (SF) spectrometers are often the only practicable solution. The other limitation is the high dilution factor after sample digestion needed to minimize the matrix load in the instrument. Even with the low instrumental limits of determination of modern sector field instruments, the detection power for direct analysis of solar silicon samples is often not sufficient for many analytes because of a typical dilution factor of 1000:1 necessary to achieve a tolerable matrix load of 1 g L−1 in the measurement solutions. Thankfully, silicon can easily be removed from the solution after dissolution in a mixture of hydrofluoric and nitric acids according to following reactions:
3Si + 4HNO3 → 3SiO2 + 4NO + 2H2O | (1) |
3SiO2 + 12HF → 3SiF4↑ + 6H2O | (2) |
The formed silicon tetrafluoride is highly volatile (b.p. = −95.2 °C) and hence can easily be evaporated, allowing lower dilution factors for the measurement.
To achieve this matrix evaporation, different approaches have been proposed. The simplest one is certainly evaporation in open beakers,13,14 which poses serious contamination issues for elements present in ambient air. Recently, microwave-assisted methods have become very popular for multi-element analysis15–18 especially for inert ceramics like silicon nitride. Allowing dissolution and evaporation in one vessel under heat and pressure they permit relatively short preparation times. Blank control is also much better owing to the environmental isolation of the sample. On the other hand, microwave digestion systems tend to be expensive and cleaning/maintenance is intensive for the apparatus. Moreover, loss of other elements forming volatile fluorides can occur, limiting the number of analytes that can be quantitatively determined. Since pure silicon readily dissolves in a mixture of HF/HNO3, microwave digestion has no relevant benefits or unique features over classic digestion methods.
In this paper, we present a simple, cost-effective method for the determination of impurities in high purity silicon by ICP-SFMS combining the benefits of the closed system and one-vessel approach taken from microwave-assisted digestion and the technical simplicity of conventional analysis. We developed a metal-free vaporization design with minimum air contact, small enough to be easily placed under a clean bench for better blank control. From a survey through several German photovoltaic companies along the value chain from raw silicon to solar cells about their impurities of concern, the analytes of interest are B, Na, Mg, Al, P, K, Ca, Ti, Cr, Mn, Fe, Co, Ni, Cu, Zn, Ga, Ge, As, Mo, Sb, W and Tl. Our approach leads to competitive limits of determination taking into account all these analytes in one analysis.
Plasma conditions | |
Rf-power/W | 1350 |
Coolant gas flow/L min−1 | 15 |
Sample gas flow/L min−1 | 1 |
Auxiliary gas flow/L min−1 | 0.95 |
Additional gas flow/L min−1 | 0.06 |
Data acquisition | |
Dwell time/ms | 100 |
No. of scans | 3 |
No. of replicates | 3 |
Measurement time/min per sample | 5 |
The isotopes 9Be, 89Y, 141Pr and 175Lu were used as internal standards and added to every sample and solution in an amount that the same final concentration (8 μg L−1) in the measurement solutions was achieved. The elements were chosen because they could not be found at notable concentrations in typical solar grade silicon samples, they formed no volatile fluorides, they showed good sensitivity and covered a wide mass range, ensuring a comprehensive compensation of instrument drift during measurement. The isotope 9Be was used to normalize the data for m/z: 0–31, 89Y for 32–100, 141Pr for 101–141 and 175Lu for 175–205.
All standard solutions, water and acids were stored in PFA flasks and containers. Measurements were performed out of 15 mL polypropylene (PP) autosampler tubes (Greiner Bio-One, Kremsmünster, Austria) which were cleaned by a procedure based on the work of Rodushkin and co-workers.19 The tubes were rinsed thoroughly with ultrapure water, filled with 5%/5% v/v subboiling HNO3/HF (referred to the commercially available concentrated, respective 65% and 40% acids) for storage and finally rinsed again with Milli-Q water prior to use. All sample manipulations were performed within class 100 laminar flow clean benches.
The containers are equipped with threaded caps with two 1/4′′ fittings, allowing the connection of the tubing leading to the storage vessels and vacuum pump at the outlet fitting, and an air aspiration port on the other end, thus providing a constant, moderate air flow transporting the evaporated acid and matrix to the storage vessels. Directly behind the outlet, a stopcock allows additional regulation of the air-flow if necessary. The aspiration is done through a short piece of PFA tubing, in which a syringe filter (PTFE membrane, 0.2 μm pore size, 25 mm diameter, NeoLab, Heidelberg, Germany) has been inserted to reduce the air-flow and minimize contamination risk. Experiments have shown that filters with smaller diameter show very non-uniform admission of air, leading to unequal evaporation times among the vessels. The graphite heating block was placed inside a laminar flow box to minimize the risk of contamination.
Two types of caps with fittings are commercially available for the sample containers: parallel (both fittings pointing upwards) or orthogonal configuration. Since the evaporated liquid already condenses in the tubing, the latter configuration has been chosen for this design, allowing easier drainage of the evaporated liquid towards the storage vessels through the horizontal fitting by the assistance of gravity in addition to the reduced pressure.
The storage vessels are two one-liter PFA containers with respectively six inlets and one outlet in the cap, mounted underneath the level of the evaporation vessels, bending the PFA tubing downwards for easier drainage. The evaporated acids and matrix are collected at the bottom of the vessels and can be removed after evaporation is completed. The two outlets of the storage vessels are connected to the vacuum pump via a T-piece.
All parts and tubing are made of PFA (stopcocks made of PTFE) and can easily be cleaned by evaporating clean acids through the system. Since sample preparation can be performed in 30 mL PFA containers fitting into the graphite block, only the caps have to be changed in order to switch between sample digestion and evaporation. Since the caps are not in contact with the sample solution and the evaporated acid does not flow back to the container, the system need not be cleaned between each evaporation. This increases the capacity utilization of the evaporation apparatus and shifts the critical time consuming cleaning procedures towards cheap and easy replaceable, small PFA containers.
The sample preparation procedure is outlined in Fig. 2. In each set of samples, three method blanks were analyzed together with nine samples. The blanks were treated exactly as the samples, only without addition of any silicon.
Silicon samples of up to 1000 mg were treated with acid etching (HNO3 + HF, 30% + 10% by volume, for ca. 10 minutes at room temperature) to remove surface contamination until any observable damage from sawing was no longer visible.
The samples were then weighed into 30 mL PFA containers with closed caps and 250 μL of an internal standard solution (Be, Y, Pr, Lu at 800 μg L−1) and 50 μL of a solution of 25 g L−1 mannitol were added. The addition of mannitol gives rise to the formation of a non-volatile complex of boron, which prevents its removal as fluoride together with silicon.20 The containers were placed in an ice bath and the total amount of 8.5 mL HF was added at once. The nitric acid was added slowly until a total addition of 4.5 mL. The reaction speed has to be controlled carefully to avoid spilling but can be automated. The addition of nitric acid takes about two hours. Cooling of the samples can be omitted with a slower addition rate of nitric acid.
The closed caps were then replaced by the evaporation caps with fittings and the containers were placed into the graphite heating block. The samples were heated to 110 °C for one hour to allow a slower and controlled evaporation of the matrix, and then further heated for 3.5 h at 150 °C to dryness. Immediate heating to 150 °C can cause clogging of the tubing.
The residues in the containers were dissolved and diluted to 5 mL using 5%/2.5% v/v HNO3/HF. These solutions were allowed to stand overnight to guarantee the total dissolution of the residues. Then, four aliquots of 1 mL each were transferred into 15 mL PP (polypropylene) tubes. One was simply filled up with Milli-Q water to a total volume of 5 mL. The remaining three were spiked with multi element standards of increasing concentration containing all elements of interest and finally filled up to 5 mL. Spiking can take place as needed according to expected concentrations or preliminary tests. The final solution contained 1% HNO3 and 0.5% HF.
The reproducibility of matrix evaporation and stability of the instrument were very good, varying less than 10% over a ten hours measurement period. Thus, if similar samples are analyzed, the sample preparation and analysis time can be considerably reduced by preparing only one standard addition for every three samples or so, relating one standard addition calibration to the following, merely diluted samples.
The zirconium monitor was made from a 1% Zr-solution (NIST 3169). Four zirconium standards were produced by filling app. 55 mg of the solution into quartz ampoules. The amount of the individual solution was determined gravimetrically. The ampoules were dried in an oven at 50 °C for one day and then subsequently sealed by melting.
The gold monitor was made out of a 981 mg L−1 Au-solution (PlasmaCAL, SCP Science, Champlain, NY, USA). This solution was diluted by a factor of 100 and from this dilute solution four gold standards were produced in the same manner as described for the zirconium standards.
The silicon samples of around 2.5 g were packed into an aluminium capsule. The aluminium capsule has two layers separated by a sieve. This means that in each layer one pair of samples could be packed. In addition to this pair of samples two Zr standards and two Au standards were packed. Blank positions were filled with quartz ampoules to prevent the samples from rattling. The aluminium capsule was closed with a crown cap. The bottom of the capsule and the cap have holes to allow water to flow through during irradiation to cool the samples and the quartz ampoules.
Neutron irradiation has been performed with the swimming pool reactor BER II of the Helmholtz-Zentrum Berlin für Materialien und Energie (HZB). To gain highest sensitivity, the DBVK irradiation facility has been chosen. This irradiation facility is located in the middle of the reactor core replacing one fuel element and has therefore the highest neutron flux available at the BER II reactor. The thermal neutron flux in this position is app. 1 × 1014 cm−2 s−1 and the epithermal flux is app. 9 × 1012 cm−2 s−1.
The samples were irradiated for 4.5 days and cooled down for 2 days. To remove surface contaminants, samples and quartz ampoules were etched with 25% hydrofluoric acid, rinsed three times with distilled water and dried by dipping into ethanol and acetone, respectively.
A high-purity germanium detector was used for gamma ray counting. To reduce background the detector was shielded with 10 cm of lead. The detector was connected to a Canberra (Meriden, CT, USA) gamma-spectrometer with 1.9 keV resolution at 1.33 MeV via a digital signal processor. Spectra from 50 to 2100 keV have been recorded. Counting times for each sample varied between 5 h (for two samples) and up to 24 h for the others. Due to these long counting times different cooling times for the samples accumulated, resulting in different limits of determination for some elements. Canberra Genie software was used to control the measurements and to accumulate and evaluate the spectra. The elemental concentrations including uncertainty calculations and calculation of the detection limits were done with the Kayzero for Windows software (k0 Ware, Heerlen, The Netherlands).
Element | Conc./ng L−1 As-supplied, n = 7 | Conc./ng L−1 Cleaned, n = 7 |
---|---|---|
Na | 84 ± 26 | 10 ± 17 |
Cu | 55 ± 12 | 3 ± 2 |
Fe | 554 ± 479 | 6 ± 4 |
P | 936 ± 178 | <100 |
Ti | 54 ± 14 | 22 ± 19 |
2HF + SiF4 ↔ H2SiF6 | (3) |
The addition of 8.5 mL HF per gram Si was a good compromise between reaction rate and evaporation with >99% Si removed.
Element | LoD/ng g−1 | LoD from[15]/ng g−1 |
---|---|---|
B | 22 | |
Na | 7.1 | |
Mg | 13 | 81 |
Al | 11 | |
P | 5.7 | |
K | 7.5 | 135 |
Ca | 53 | |
Ti | 4.2 | |
Cr | 0.27 | 2.7 |
Mn | 0.21 | 1.5 |
Fe | 1.7 | 36 |
Co | 0.26 | 0.3 |
Ni | 2.0 | 4.8 |
Cu | 0.38 | 1.2 |
Zn | 2.7 | 6 |
Ga | 0.12 | |
Ge | 0.16 | |
As | 0.65 | |
Mo | 0.25 | |
Sb | 0.17 | |
W | 0.37 | |
Tl | 0.17 |
LoD/ng g−1 for acid blank | LoD/ng g−1 for method blank | |
---|---|---|
Al | 6.8 | 11 |
Mg | 2.1 | 13 |
Ca | 18 | 53 |
Ti | 0.8 | 4.2 |
The results of the recovery experiment, the linearity of the calibration curves (r2) and their sensitivity are shown in Table 5. All recoveries are close to 100%.
Element | Recovery/% | Coefficient of determination | Slope/counts/ng mL−1 |
---|---|---|---|
B | 98 ± 3 | 1.000 | 31524 |
Na | 98 ± 3 | 1.000 | 118073 |
Mg | 101 ± 1 | 0.999 | 4512* |
Al | 96 ± 5 | 1.000 | 118016 |
P | 100 ± 3 | 0.999 | 476* |
K | 104 ± 3 | 0.999 | 2847‡ |
Ca | 108 ± 3 | 0.998 | 313* |
Ti | 100 ± 11 | 0.994 | 839* |
Cr | 103 ± 1 | 0.999 | 9265* |
Mn | 103 ± 4 | 0.999 | 12810* |
Fe | 103 ± 5 | 0.999 | 10858* |
Co | 102 ± 2 | 0.999 | 12000* |
Ni | 103 ± 3 | 0.998 | 2736* |
Cu | 99 ± 3 | 0.997 | 101442 |
Zn | 106 ± 1 | 0.999 | 420‡ |
Ga | 104 ± 5 | 0.999 | 2170‡ |
Ge | 107 ± 4 | 0.999 | 514‡ |
As | 103 ± 2 | 0.999 | 316‡ |
Mo | 101 ± 2 | 0.997 | 50566 |
Sb | 93 ± 3 | 1.000 | 74408 |
W | 96 ± 1 | 1.000 | 118541 |
Tl | 99 ± 1 | 1.000 | 361164 |
Reference cspiked/μg L−1 | c observed/μg L−1, CSP | c observed/μg L−1, BAM | |
---|---|---|---|
Ti | 4.0 ± 0.1 | 4.0 ± 3.6 | 3.8 ± 3.4 |
Co | 3.0 ± 0.1 | 3.2 ± 0.2 | 3.0 ± 0.2 |
Ni | 7.1 ± 0.1 | 7.0 ± 1.0 | 7.4 ± 1.1 |
Zn | 9.0 ± 0.1 | 8.4 ± 3.4 | 10 ± 4.0 |
Cr | 6.0 ± 0.1 | 5.8 ± 1.2 | 5.6 ± 1.1 |
Cu | 20 ± 0.1 | 19 ± 1.9 | 20 ± 2.0 |
Fe | 81 ± 0.6 | 82 ± 12 | 80 ± 12 |
Na | 10 ± 0.1 | 7.9 ± 0.4 | 9.6 ± 0.5 |
Ca | 50 ± 0.4 | 50 ± 2.5 | 50 ± 2.5 |
K | 100 ± 1 | 83 ± 17 | 106 ± 21 |
B | 252 ± 2 | 240 ± 36 | 244 ± 37 |
P | 604 ± 6 | 585 ± 59 | 612 ± 61 |
Element | Observed content/μg g−1 | Reference content/μg g−1 |
---|---|---|
a Above calibration range. | ||
B | 12.2 ± 0.5 | 12.5 ± 2.1 |
P | 15.8 ± 1.2 | 16.3 ± 1.5 |
Fea | 4622 ± 770 | 3400 ± 60 |
Ni | 18.6 ± 1.3 | 15.3 ± 1.7 |
Cu | 16.3 ± 3.9 | 17.2 ± 5.8 |
Cr | 20.3 ± 2.2 | 17.3 ± 3.3 |
Ala | 1835 ± 319 | 1690 ± 220 |
Mn | 86.0 ± 7.6 | 78.2 ± 7.2 |
Ti | 349 ± 33 | 346 ± 49 |
The results of the interlaboratory comparison on the two different feedstock silicon samples are shown in Table 8. The overall comparability of the results between the two ICP-MS methods with different sample preparation procedures and the NAA is very good and demonstrates the quality of the method presented here. Some elements like boron or phosphorus cannot be measured by NAA. Here, the two ICP-MS methods show good agreement. For a few other elements the NAA lacks the necessary limits of determination for a fair comparison. Especially for some fast-decaying isotopes, e.g. Ge and K, the LoD depends highly on the time passed between irradiation and measurement and may vary between samples by several orders of magnitude. Some elements also exhibit a vast range of content in the samples, as indicated by the uncertainty bars. The known superimposed inhomogeneity of the real material is most likely the cause for these effects.
Element | w/μg kg−1 | w/μg kg−1 | w/μg kg−1 |
---|---|---|---|
ICP-MS BAM | ICP-MS CSP | NAA HZB | |
Material A | |||
B | 4281 ± 261 | 3816 ± 511 | |
Na | 21 ± 8 | 266 ± 104 | 2.5 ± 0.3 |
Mg | <4 | 31 ± 31 | |
Al | 62 ± 16 | 83 ± 3 | |
P | 5375 ± 508 | 4864 ± 659 | |
K | 44 ± 54 | 24 ± 17 | <1500 |
Ca | 99 ± 50 | 1850 ± 1784 | |
Ti | 11 ± 4.4 | 25 ± 12 | |
Cr | 1.1 ± 0.4 | 2.3 ± 1.2 | <0.15 |
Mn | 0.4 ± 0.2 | 2.9 ± 2.3 | <80000 |
Fe | 26 ± 11 | 22 ± 16 | <5 |
Co | 0.2 ± 0.11 | 0.1 ± 0.3 | <0.008 |
Ni | 1.2 ± 1.1 | n.d. | |
Cu | <2 | n.d. | <3 |
Zn | 7.8 ± 4.0 | 56 ± 62 | <0.3 |
Ga | 0.07 ± 0.01 | n/a | <0.06 |
Ge | n/a | 319 ± 99 | 266 ± 6 |
As | 2.4 ± 0.1 | 1.5 ± 1.3 | 2.7 ± 0.1 |
Mo | <0.2 | 0.5 ± 0.8 | <0.3 |
Sb | <0.07 | 1.1 ± 1.9 | 0.02 |
W | 0.5 ± 0.4 | 1.9 ± 2.7 | <0.05 |
Tl | <0.04 | n.d. | |
Material B | |||
B | 650 ± 18 | 658 ± 20 | |
Na | 288 ± 126 | 437 ± 171 | 254 ± 194 |
Mg | 4.8 ± 1.8 | 23 ± 15 | |
Al | 75 ± 13 | 139 ± 40 | |
P | 2159 ± 55 | 1743 ± 212 | |
K | 8.5 ± 7.5 | 22 ± 22 | <2000 |
Ca | 30 ± 19 | 469 ± 246 | |
Ti | 91 ± 44 | 39 ± 12 | |
Cr | 9.1 ± 2.2 | 3.4 ± 7.5 | 9.4 ± 8 |
Mn | 5.5 ± 2.6 | 5.9 ± 1.7 | <150 |
Fe | 295 ± 68 | 363 ± 106 | 504 ± 433 |
Co | 0.7 ± 0.3 | 0.73 ± 0.51 | 0.7 ± 0.6 |
Ni | 8.3 ± 1.6 | n.d. | |
Cu | 5.1 ± 1.8 | n.d. | <40 |
Zn | 5.8 ± 4.0 | 40 ± 17 | <40 |
Ga | 5.9 ± 0.4 | n/a | 4.0 ± 5.1 |
Ge | n/a | 589 ± 126 | <60000 |
As | 41 ± 7.7 | 15.2 ± 8.2 | 47 ± 3 |
Mo | <0.2 | 0.53 ± 0.48 | <0.7 |
Sb | 3.4 ± 0.1 | 2.4 ± 1.2 | 3.5 ± 0.4 |
W | 4.3 ± 0.8 | 2.0 ± 2.0 | 1.2 ± 1.1 |
Tl | <0.04 | n.d. |
This journal is © The Royal Society of Chemistry 2014 |