Yong
Wang
a,
Ravi
Kanipayor
b and
Ian D.
Brindle
*a
aDepartment of Chemistry, Brock University, St. Catharines, Ontario, Canada L2S 3A1. E-mail: ibrindle@brocku.ca; Fax: +1 905 688-0748; Tel: +1 905 688 5550 ext. 4559
bChemquant Laboratories, 1210 Larny Court, Mississauga, Ontario, Canada L4W 3N4. E-mail: ravi_kanipayor@yahoo.ca; Tel: +1 705 942 8646
First published on 29th October 2013
Validation, using a prototype of a novel sample digestion device (ColdBlock™ (patent pending, WO 2011/054086 A1)), for elemental determination, has been conducted. This device utilizes focused infra-red radiation to induce speedy sample breakdown and offers an alternative technique of wet sample dissolution that combines reduced digestion time with excellent accuracy and precision. The current study explores the digestion capacity of ColdBlock™ for a variety of solid environmental samples that include difficult matrices. Two certified materials (contaminated soil SS-1, bio-solid CRM030-040) were analyzed. The technology was also used to compare results from a recent inter-laboratory evaluation of an uncertified commercial sludge sample (LPTP12-S2) using inductively coupled plasma optical emission spectroscopy (ICP-OES). Quantification of eleven major metals (Al, Ca, Cr, Cu, Fe, Mg, Mn, Ni, Pb, V, Zn) yielded recoveries from 89–108% and relative standard deviations from 0.7–3.6%, employing a common aqua regia leach that required reduced volumes of acid. Digestion times were satisfactory, since the samples required only 15–20 minutes to deliver the results described above. This technique shows great potential to improve sample throughput while maintaining the quality of analytical results for both research and commercial applications.
Ideally, sample dissolution should be achieved in an accurate, fast, uncomplicated, cost-effective, risk-free, environmentally friendly, and highly reproducible manner. The intrinsic shortcomings for open-vessel hot-block digestions are well-known, particularly for their lengthy digestion time,2,3 relatively large consumption of both sample and mineral acids,4,5 together with concomitant increased potential for contamination. Unlike hot-block methods, that employ conductive heat transfer and often takes hours of heating, microwave assisted digestion (MAD) dramatically expedites the digestion process by virtue of its ability to promote complex redox reactions by raising the temperature through the transfer of energy directly to the solvent and increasing it further by sealing the digestion vessel, thereby increasing the pressure. The overall performance of MAD has been evaluated thoroughly in a number of previous publications.6–8 Excessive build-up of pressure in closed digestion system can, however, result in the rupture of sealed vessels. Moreover, the safe working temperature of Teflon™ (PTFE) vessels, frequently used in MAD applications, is generally limited to temperatures below 260 °C. Above this temperature the vessel is subject to deformation and consequently can compromise the analysis.9 Consequently, some decomposition reactions that require high activation energy may not be achieved, due to inadequate energy input. Aside from those limitations, sample pre-digestion for organic-rich or gas-releasing samples and extended cooling stages may be required.10,11 Ybáñez et al.12 reported rather uneven distribution of microwave radiation within the oven cavity, resulting in compromised method reproducibility. Taylor et al.13 proposed an open-vessel digestion method with focused microwave radiation to resolve some of the limitations of conventional close-vessel microwave operations. However, despite the facilitation of using hydrofluoric acid for silicate-rich samples, multiple acid-addition steps and consumption of relatively large amounts of acids was still required and the reproducibility and digestion time were improved only fractionally. In addition, since many Teflon reaction tubes are made by sintering powdered PTFE, cleanup of the tubes prior to use, or between uses, can be difficult and time-consuming, due to the retention of contaminants by the reticulated surface of the tubes. Those additional handling steps, together with the need to clean complex parts, such as the lid of the digestion vessels, inevitably compromise the overall digestion efficiency and can lead to increased variation in analytical results. From the perspective of many production labs, the slowness of current digestion methods represents the rate-determining step in the analytical process. This slowness presents a significant barrier to automation of the digestion process and, ultimately, automation of the entire analytical process. Therefore, the need for new dissolution methods that address the above-mentioned weaknesses in current digestion technologies has been growing in the analytical community.
While microwave technology (MW) has successfully demonstrated speedy digestion using the microwaves to boost kinetic energy, the potential of accelerating wet digestion using other kinetic sources, such as infrared (IR) lamps, has been sought by several device manufacturers and research groups with limited success. Infrared (IR) heating sources are commercially available and can provide more intense irradiation than microwave, due to its higher energy (usually by 2–4 orders of magnitude).†14 Lopes et al.15 developed an IR-MW procedure using a domestic IR lamp to facilitate sample pre-digestion, and achieved significantly improved reproducibility. Two European manufacturers, Büchi and Gerhardt, market IR-based digesters for elemental determination. These products utilize dispersive, unfocused IR radiation to promote convective–conductive heating. The digestion time is still relatively long (typically around two hours).
In the current investigation, the IR digester employs focused short-wavelength IR irradiation which transmits infrared energy directly to the surface of sample particles and is the first IR-based digester of its kind. Its digestion performance was systematically evaluated with a variety of environmental matrices, as the first step in validating the device and exploring its potential for extension to other matrices. The device's uniquely small, focused heating zone, in contrast to its relatively cool operating environment, led to its being called the ‘ColdBlock’.
A semi-closed cooling system, incorporating a pair of mini-fans, a Peltier cooling block, and a ribbed watch glass, was devised to handle the excess heat generated during the digestion (Fig. 2). Rapid removal of the heat generated by the IR rings and by the exothermic reaction of the sample provides an advantage in that the upper part of the tube remains cool, which facilitates handling. Mini-fans are positioned at the bottom of heating chamber that blow cool air directly onto the lower part of quartz tube, enabling rapid cooling of the digestion vessel at the end of the run. The water-cooled Peltier cooling block (typically operating at 4 °C), fitted tightly into the upper-body of the thimble, thermally moderates the release of acid fume evaporated in the wake of extreme heat from IR irradiation. The selection of this powerful cooling accessory, in contrast to other ordinary cooling methods, is necessitated by its application for tougher geological matrices, that must be more completely dissolved, and where the promotion of reflux of high boiling point acids is critical. The ribbed watch glass is intended to prevent airborne contaminants from entering the reaction vessel. In addition, once a digestion starts, the gap between the ribbed watch glass and the top of quartz tube allows gaseous product, such as CO2 and NO2, to escape. Meanwhile, the chilled upper part of the quartz tube recovers much of the acid fume and thus reduces the use of acid and minimizes sample loss.
Plasma RF power (W) | 1300 |
Plasma gas flow (L min−1) | 15.0 |
Auxiliary gas flow (L min−1) | 0.5 |
Nebulizer gas flow (L min−1) | 0.8 |
Sample uptake (mL min−1) | 1.5 |
Detector | UV |
Delay time (s) | 30 |
Integration period (s) | Automatic (3–4 s) |
Sweeps | 3 |
Number of replicates | 3 |
Elements | Low (μg mL−1) | High (μg mL−1) | Wavelength (nm) | LOD (ng mL−1) |
---|---|---|---|---|
Al | 1.0 | 20 | 394.401 | 5.4 |
Ca | 1.0 | 20 | 317.933 | 2.1 |
Cr | 1.0 | 20 | 267.716 | 2.6 |
Cu | 1.0 | 20 | 327.393 | 1.4 |
Fe | 1.0 | 20 | 238.204 | 1.9 |
Mg | 1.0 | 20 | 285.213 | 0.6 |
Mn | 1.0 | 20 | 257.610 | 0.1 |
Ni | 1.0 | 20 | 231.604 | 3.2 |
Pb | 1.0 | 20 | 220.353 | 9.3 |
Ti | 1.0 | 20 | 334.940 | 0.3 |
V | 1.0 | 20 | 290.880 | 0.5 |
Zn | 1.0 | 20 | 206.200 | 1.8 |
All digestions were performed in a well-vented fume hood to address safety concerns. Approximately 0.2–0.25 grams of dried samples were accurately weighed and carefully loaded into the bottom of the quartz digestion tube. Compared with conventional EPA hot-block methods (3050, 3050B) that adopt a repeated acidifying-drying approach, sample digestion is straightforward with the ColdBlock™ digester – the reaction is completed without the sample being taken to dryness. Due to the high-organic nature of the environmental materials being tested, the first stage in the current method was to add 2 mL of concentrated nitric acid to the sample. This step aimed to remove as much organic carbon content as possible and helped to prevent excessive foaming in the following aqua regia leaching stage. Oxidation of organics was immediately observed upon starting IR heating. After approximately two minutes, the evolution of reddish NO2 fumes, a by-product of the oxidation reaction, subsided. The quartz tube was then left to cool by the mini-fans for one minute before 3 mL of concentrated HCl was added to form a modified aqua regia leaching mixture. IR heating for 10–15 minutes at higher power was allowed for the aqua regia leaching. Finally, digestates were treated with 1 mL of H2O2 to further oxidize carbon residues as well as to convert remaining NOx to more stable NO3−. The detailed digestion profiles for each environmental sample are listed in Table 3. The resultant digestates were diluted to 25 mL with ultra-pure water and filtered with a syringe-filter of 0.22 μm porosity. Further dilutions were applied to the filtrate, with appropriate dilution factors to ensure that elemental concentrations are comfortably bracketed within the calibration range.
Sample ID | SS-1 (min) | CRM031-040 (min) | LPTP12-S2 (min) |
---|---|---|---|
Step 1: add 2 mL of HNO 3 | |||
Power used: | |||
55% | 1 | ||
60% | 1 | 3 | 1 |
70% | 1 | ||
Step 2: add 3 mL of HCl | |||
60% | 1 | 1 | |
70% | 1 | 1 | 1 |
80% | 10 | 15 | 15 |
Step 3: add 2 mL of H 2 O 2 | |||
80% | 1 | 1 | 1 |
Total | 15 | 20 | 20 |
In Tables 4 and 5, analytical results for eleven major elements (Al, Ca, Cr, Cu, Fe, Mg, Mn, Ni, Pb, V, Zn) in the two CRMs are presented. Compared with the certified values, which were generated with EPA method 3050B, a hot-plate method, recoveries of analytes using the ColdBlock™ digestions were satisfactory, except for the slightly lower Cr values (89%) in CRM031-040. This low recovery may be ascribed to the relatively high inertness of chromium in more refractory phases.18,19 Precision at the 95% confidence level‡ was calculated from 4 between-run analyses for each CRM and yielded a smaller spread than certified values. The RSDs range from 0.7–3.6% for the major elements. This markedly improved between-run reproducibility at varying elemental concentration levels, compared with reported microwave data on similar soil types,20–22 may be a function of the efficiency of the focused IR heating during digestion or could, as a referee has noted, be due to other variables that might include sample homogeneity and sample size.
SS-1 (n = 4) | ||||
---|---|---|---|---|
Element | Measured (mg kg−1) | Certified (mg kg−1) | Recovery (%) | RSD (%) |
Al | 11300 ± 300 | 12163 ± 409 | 93 | 2.3 |
Ca | 52000 ± 1300 | 50265 ± 1213 | 104 | 2.6 |
Cr | 95 ± 2 | 103 ± 6.1 | 93 | 1.6 |
Cu | 410 ± 6 | 403 ± 10 | 102 | 1.4 |
Fe | 77800 ± 2100 | 72000 ± 2273 | 108 | 2.7 |
Mg | 9300 ± 200 | 9690 ± 230 | 96 | 2.7 |
Mn | 700 ± 5 | 737 ± 19 | 95 | 0.7 |
Ni | 54 ± 1 | 59.2 ± 1.3 | 92 | 1.2 |
Pb | 720 ± 30 | 764 ± 15 | 95 | 3.6 |
V | 28 ± 1 | 27.2 ± 1.4 | 104 | 1.6 |
Zn | 1010 ± 10 | 1114 ± 37 | 91 | 0.7 |
CRM031-040 | ColdBlock (n = 4) | HotBlock (n = 3)aa EPA method 3050B was applied, data provided by the Niagara Regional Lab. | ||||
---|---|---|---|---|---|---|
Element | Certified (mg kg−1) | Measured (mg kg−1) | Recovery (%) | RSD (%) | Recovery (%) | RSD (%) |
Al | 13100 ± 874 | 11900 ± 300 | 91 | 2.2 | 97.0 | 1.8 |
Ca | 49400 ± 2310 | 49400 ± 900 | 100 | 1.8 | 92.0 | 2.2 |
Cr | 243 ± 12.3 | 220 ± 5 | 89 | 2.4 | 94.0 | 2.9 |
Cu | 639 ± 21.3 | 600 ± 20 | 93 | 2.7 | 87.0 | 1.8 |
Fe | 22400 ± 999 | 22800 ± 300 | 102 | 1.4 | 82.0 | 1.9 |
Mg | 8920 ± 326 | 9000 ± 200 | 101 | 2.1 | 99.0 | 2.7 |
Mn | 1240 ± 139 | 1200 ± 30 | 95 | 2.8 | 95.0 | 3.3 |
Ni | 136 ± 8.8 | 124 ± 3 | 92 | 2.7 | 94.0 | 3.5 |
Pb | 121 ± 6.3 | 120 ± 2 | 98 | 1.7 | 96.0 | 3.0 |
V | 133 ± 8.2 | 120 ± 3 | 91 | 2.4 | 95.0 | 2.5 |
Zn | 908 ± 59 | 960 ± 10 | 106 | 0.8 | 94.0 | 3.1 |
LPTP12-S2 | ||||||
---|---|---|---|---|---|---|
Element | Assigned (mg kg−1) | Measured (mg kg−1) | SDPAa (mg kg−1) | Z | Recovery (%) | RSD (%) |
a Standard deviation for proficiency analysis. b (x: measured score; u: assigned value). | ||||||
Al | 14200 | 12900 ± 200 | 1750 | −0.83 | 91.0 | 1.8 |
Ca | 51600 | 48600 ± 1000 | 1980 | −1.28 | 96.0 | 0.7 |
Cr | 129 | 120 ± 2 | 5.78 | −0.29 | 93.0 | 1.3 |
Cu | 716 | 680 ± 20 | 64.7 | 0.08 | 95.0 | 2.5 |
Fe | 23200 | 24200 ± 500 | 1900 | 0.04 | 104.0 | 2.1 |
Mg | 10400 | 9500 ± 300 | 475 | −1.29 | 91.0 | 3.1 |
Mn | 756 | 770 ± 10 | 68.3 | −0.8 | 102.0 | 1.5 |
Ni | 373 | 370 ± 10 | 42.5 | 0.06 | 99.0 | 1.4 |
Pb | 192 | 190 ± 5 | 23.9 | −0.07 | 101.0 | 2.4 |
V | 122 | 100 ± 3 | 7.68 | 0.33 | 96.0 | 3.0 |
Zn | 833 | 820 ± 20 | 65.7 | −0.71 | 99.0 | 3.0 |
SS-1a (n = 4) | CRM031-040 (n = 4) | LPTP12-S2 (n = 4) | |||||||
---|---|---|---|---|---|---|---|---|---|
As | Sb | Se | As | Sb | Se | As | Sb | Se | |
a 1 gram of sample used and a reduced dilution factor was applied for the determination of Se. | |||||||||
Measured (mg kg−1) | 21.9 ± 1.9 | 5.7 ± 0.4 | 0.74 ± 0.06 | 208 ± 6 | 110 ± 4 | 107 ± 3 | 316 ± 8 | 103 ± 2 | 185 ± 4 |
Certified (mg kg−1) | 20.7 ± 1.0 | 5.5 ± 1.1 | 0.78 ± 0.14 | 217 ± 10 | 107 ± 20 | 120 ± 12 | 330 ± 40 | 110 ± 25 | 200 ± 30 |
Recovery (%) | 105.8 | 104.4 | 94.9 | 96.3 | 103.3 | 90.1 | 95.1 | 94.0 | 90.0 |
RSD (%) | 4.4 | 3.4 | 3.9 | 3.0 | 3.3 | 2.9 | 2.6 | 1.5 | 2.0 |
Footnotes |
† The quantum energy of microwave photons is generally in 10−6 to 10−4 eV range, whereas the energy state of infrared photons falls in 10−2 to 1.6 eV. |
‡ In accordance with the confidence level employed in publishing two certified reference materials. |
§ t(exp) = 1.22, two-tailed t(0.05, 10) = 2.23. |
This journal is © The Royal Society of Chemistry 2014 |