Yanbei Zhu
*a,
Guosheng Yang
b,
Aya Sakaguchi
c,
Tsutomu Miura
a,
Yasuyuki Shikamori
ad and
Jian Zheng
*b
aNational Institute of Advanced Industrial Science and Technology, 1-1-1 Umezono, Tsukuba, Ibaraki 305-8563, Japan. E-mail: yb-zhu@aist.go.jp
bNational Institutes for Quantum Science and Technology, 4-9-1 Anagawa, Inage-ku, Chiba-shi 263-8555, Japan. E-mail: zheng.jian@qst.go.jp
cUniversity of Tsukuba, 1-1-1 Tennodai, Tsukuba, Ibaraki 305-8577, Japan
dTohoku University, 2145-2, Narita-cho, Oarai-machi, Higashiibaraki-gun, Ibaraki 311-1313, Japan
First published on 3rd April 2025
Tandem quadrupole inductively coupled plasma mass spectrometry (ICP-QMS/QMS) provides an effective approach for separating spectral interferences without sacrificing the signal intensity due to the increased requirement for mass resolution. This feature is especially important for the analysis of rare earth elements (REEs) and radionuclides, the accurate and precise measurement of which usually suffer from severe spectral interferences. The present review covers the advances and applications of ICP-QMS/QMS in the analysis of rare earth elements and radionuclides reported in around 150 articles since 2012, when the first commercially available ICP-QMS/QMS was released. Specifically, the strategies for separating spectral interferences are highlighted, including chemical separation prior to the analysis, reaction cell technique in ICP-QMS/QMS measurement, and post-analysis mathematical correction. Subsequently, the improvements in the analytical figures of merits are summarized along with the major advancements, focusing on REEs and radionuclides of Cs, I, Sr, U and Pu. Finally, the challenges and potential solutions to address them in future works are presented.
The powerful ionization capability of high-temperature argon plasma provides high sensitivity for elemental analysis, but it causes severe spectral interferences due to the ionization of argon gas and solvent contents and the coexisting elements in the samples. CRC provides an excellent solution for spectral interference in single quadrupole (SQ-) ICP-MS.2 However, one of the problems associated with the reaction cell in SQ-ICP-MS is the complexity of reactions occurring in it due to the enormous amount of ionic species generated by the argon plasma. In ICP-QMS/QMS, the introduction of a quadrupole mass filter in front of the CRC limits the ions passing into the CRC, greatly simplifying the reactions between the ions and gas molecules. An ion of interest can be measured in the so-called on-mass mode or mass-shift mode using ICP-QMS/QMS.2 In the case of on-mass mode measurement, an ion is measured as its initial species by monitoring its initial mass-to-charge ratio (i.e. m/z) at the second quadrupole, for which the m/z is set to be identical to that for the first quadrupole (e.g. m/z = 139 for both quadrupoles to permit the passage of 139La+). By contrast, in mass-shift mode measurement, the measurement of an ion at the second quadrupole is conducted by monitoring a multi-atomic species generated in the CRC, where the m/z for the second quadrupole is set to a value higher than that for the first quadrupole (e.g. m/z = 139 and m/z = 155 for the first and the second quadrupoles to permit the passage of 139La+ and 139La16O+, respectively).
Lanthanides are usually referred to as rare earth elements (REEs) together with Sc and Y. Although fractionations among REEs occur in the environment, they essentially have similar behavior and are usually found together in natural samples owing to the similarity in their physicochemical properties.3 As a result, the fractionation of REEs based on their concentration in a sample can help understand its chemical property and history. However, the measurement of heavier (with a larger m/z) REEs (e.g. 155Gd and 165Ho) usually suffers from spectral interference of lighter REEs (e.g. 139La16O and 149Sm16O, respectively). The application of ICP-QMS/QMS has been shown to be effective to reduce this type of spectral interferences.1
Long and medium half-life radionuclides have also attracted significant attention in the application of ICP-QMS/QMS.4 This can be attributed to its excellent capability for separating spectral interferences. Most radionuclides of interest exist in extremely low concentrations, sometimes even lower than 10−10 g mL−1 (or g g−1). Consequently, the measurement of these low concentrations of radionuclides by ICP-MS often suffer spectral interferences from much higher concentrations (over 106-fold that of radionuclides) of coexisting stable or long-lived radioactive isotopes.
Thus far, numerous reviews have been published on the application of ICP-QMS/QMS; however, none focused on REEs and radionuclides.2–11 Thus, the present review concentrates on the application of ICP-QMS/QMS for the measurement of REEs and radionuclides published to date. There are two major reasons why we combined REEs and radionuclides in the present work. Firstly, REEs are often studied together with two radionuclides, i.e. U and Th; secondly, spectral interferences from co-existing elements/isotopes can be critical in the measurement of both REEs and radionuclides. Accordingly, we hope that readers can find helpful information for future studies on related topics.
![]() | ||
Fig. 1 Trend in the publications on lanthanides and radionuclides measured using ICP-QMS/QMS (dotted line shows the moving average). |
This is a profound achievement regarding the limited topics conducted with a single type of ICP-MS.
The publications covered in the present work are summarised in Tables 1–4 for reviews,2–11 REEs (lanthanides),1,12–44 RNs (radionuclides),45–141 and both REEs and RNs,142–153 respectively. Also, the distribution of publications according to the topics is plotted in Fig. 2.
Publishing year | Sample (topics) | Instrument or method | Ref. no. |
---|---|---|---|
2015 | Environmental (advances) | Atomic spectrometry | 7 |
2016 | Environmental (radionuclides) | Mass spectrometry | 6 |
2018 | Environmental (advances) | Atomic spectrometry | 8 |
2018 | Multiple matrix (advances) | ICP-QMS/QMS | 2 |
2020 | Multiple matrix (radionuclides) | CRC-ICP-MS | 4 |
2021 | Geochemical (interference separation) | ICP-MS | 5 |
2021 | Multiple matrix (trends and advances) | ICP-QMS/QMS | 10 |
2023 | Multiple matrix (REEs) | Analytical techniques | 3 |
2023 | Multiple matrix (radionuclides) | Analytical greenness | 11 |
2023 | Multiple matrix | ICP-QMS/QMS | 9 |
Publishing year | Sample | Instrument | Ref. no. |
---|---|---|---|
a CRMs, certified reference materials. | |||
2013 | Model solution | Agilent 8800 | 1 |
2015 | Nd oxide | Agilent 8800 | 12 |
2015 | Nd oxide | Agilent 8800 | 13 |
2016 | Sediment, soil | Agilent 8800 | 14 |
2016 | Quartz-rich | Agilent 8800 | 15 |
2016 | BaCO3 | Agilent 8800 | 16 |
2017 | CRMsa | Agilent 8800 | 17 |
2018 | Bone | Agilent 8800 | 18 |
2018 | Biological | Agilent 8800 | 19 |
2019 | Printed circuit boards | Agilent 8800 | 20 |
2019 | Ce chelates | Agilent 8800 | 21 |
2020 | Seawater | Agilent 8800 | 22 |
2021 | Uranium ore | Agilent 8900 | 23 |
2021 | Uranium ore | iCAP TQ | 24 |
2021 | Model solution | Agilent 8900 | 25 |
2021 | Garnet, apatite, xenotime | Agilent 8900 | 26 |
2022 | Natural water | Agilent 8900 | 27 |
2022 | Apatite | Agilent 8900 | 28 |
2022 | Sediment | Agilent 8800 | 29 |
2022 | Uranium ore | Agilent 8800 | 30 |
2022 | La2O3 material | iCAP TQ | 31 |
2022 | Shales | Not available | 32 |
2022 | River water CRMs | Agilent 8800 | 33 |
2023 | Geological | Agilent 8900 | 34 |
2023 | Coal | Not available | 35 |
2023 | Fertilizer, insect | iCAP TQ | 36 |
2023 | Olive oil | Agilent 8800 | 37 |
2023 | Geological | iCAP TQ | 38 |
2023 | Coal ash | iCAP TQ | 39 |
2024 | Environmental | Agilent 8800 | 40 |
2024 | Geological | Agilent 8900 | 41 |
2024 | Geological | Agilent 8900 | 42 |
2024 | Seafood | Agilent 8800 | 43 |
2024 | Silicate | Agilent 8900 | 44 |
Publishing year | Sample | Instrument | Isotope of interest | Ref. no. |
---|---|---|---|---|
2013 | Model solution | Agilent 8800 | I-129 | 46 |
2013 | Soil | Agilent 8800 | Sr-90 | 45 |
2013 | Model solution | Agilent 8800 | U-236, 238 | 47 |
2013 | Soil | Agilent 8800 | I-129 | 135 |
2014 | Rain water | Agilent 8800 | Cs-134, 135, 137 | 48 |
2014 | Environmental | Agilent 8800 | Cs-135, 137 | 49 |
2015 | Cigar tobacco | Agilent 8800 | U-238 | 50 |
2016 | Model solution | Agilent 8800 | U-236, 238 | 53 |
2016 | Soil and sediment | Agilent 8800 | Sr-90, Cs-137; Pu-238, 239, 240 | 51 |
2016 | River suspended particles | Agilent 8800 | Cs-135, 137; Pu-239, 240 | 52 |
2016 | Environmental | Agilent 8800 | Cs-135, 137 | 55 |
2016 | Environmental | Agilent 8800 | U-236, 238 | 54 |
2016 | Environmental | Agilent 8800 | Cs-135, 137 | 56 |
2016 | Environmental | Agilent 8800 | Cs-135, 137 | 57 |
2017 | Decommission waste | Agilent 8800 | Sr-90 | 58 |
2017 | Atmospheric particulate matter | Agilent 8800 | Sr-90 | 59 |
2017 | Groundwater and discharge water | Agilent 8800 | Ra-226 | 60 |
2017 | Soil | Agilent 8800 | U-236, 239, 240 | 61 |
2018 | Mo powder | Agilent 8800 | Th-232, U-238 | 62 |
2018 | Vegetation | Agilent 8800 | U-234, 235, 238 | 63 |
2018 | Seawater | Agilent 8800 | U-238 | 64 |
2018 | Model solution | Agilent 8900 | U-238; Np-237; Pu-240; Am-241; Cm-244 | 65 |
2018 | Environmental | Agilent 8800 | Pu-239, 240 | 66 |
2018 | Environmental | Agilent 8800 | I-129 | 136 |
2019 | Environmental and forensic | Agilent 8800 | Pu-239 | 68 |
2019 | Soil and sediment | Agilent 8800 | U-236 | 69 |
2019 | Soil | Agilent 8800 | U-236 | 70 |
2019 | CRM | Agilent 8900 | Pu-238 | 71 |
2019 | Urine | Agilent 8800 | Sr-90 | 72 |
2019 | Nuclear waste | Agilent 8800 | Cl-36; Ca-41; Ni-59, 63; Se-79; Sr-90; Zr-93; Nb-94; Tc-99; Pd-107; Sn-126; I-129; Cs-135, 137; Pm-147; Sm-151; Pu-239; Am-241 | 73 |
2019 | CaF2 sludge | Agilent 8800 | U-234, 235, 238 | 74 |
2019 | Soil | Agilent 8800 | I-129; Cs-134, 137 | 75 |
2019 | Soil and sediment | Agilent 8800 | Cs-134, 137; U-234, 235, 238 | 76 |
2019 | Soil | Agilent 8800 | Pu-239, 240 | 77 |
2020 | Uranium CRM | Agilent 8800 | U-234, 238 | 67 |
2020 | Mining residues | Agilent 8900 | U-234, 235, 238; Th-230, 232; Ra-226, 228; Pb-210 | 78 |
2020 | Environmental | Agilent 8800 | U-236, 238 | 79 |
2020 | Environmental water | Not available | Pu-239, 240 | 80 |
2020 | Environmental | Agilent 8800 | U-236, 238 | 81 |
2020 | Kaolinitic | Agilent 8800 | U-234, 235, 238; Th-230, 232 | 82 |
2020 | Medicinal herbs | Agilent 8800 | Th-232; U-238 | 83 |
2020 | Environmental | Agilent 8800 | Cs-135, 137 | 84 |
2021 | Environmental | Agilent 8800 | U-236 | 85 |
2021 | Environmental | Agilent 8900 | Pu-239, 240 | 86 |
2021 | Bone | Agilent 8800 | U-238 | 87 |
2021 | Reference materials | Agilent 8900 | U-233, 235, 238 | 88 |
2021 | Uranium material | Not available | Th-232 | 89 |
2021 | Model solution | Agilent 8800 | Cl-36; Ca-41; Ni-63; Mo-93 | 90 |
Agilent 8900 | ||||
2021 | Concrete | Agilent 8800 | Ca-41 | 91 |
2021 | Lake water, seawater, urine | Agilent 8800 | Sr-90; U-234; Am-241; Pu-239 | 92 |
2021 | Liquid sample with complex matrices | Agilent 8800 | Sr-90 | 93 |
2021 | Environmental samples | Agilent 8800 | U-236 | 94 |
2021 | Urine | Agilent 8900 | Pu-239, 240 | 95 |
2021 | Soil | Agilent 8800 | Pu-239 | 96 |
2021 | Urine | Agilent 8800 | Np-237; Pu-239, 240, 241 | 97 |
2021 | Soil | Agilent 8900 | Pu-239 | 98 |
2021 | Soil, sediment | Agilent 8800 | Am-241 | 99 |
2021 | Waste samples | Agilent 8800 | Cs-135, 137 | 100 |
2021 | Environmental samples | Agilent 8900 | Cs-135, 137 | 101 |
2022 | Model solution | Agilent 8900 | Tc-99 | 102 |
2022 | Lead metal | Agilent 8800 | Pu-239, 242 | 103 |
2022 | Soil, sediment | Agilent 8900 | Cs-135, 137 | 104 |
2022 | Model solution | Nexion 5000 | I-129 | 105 |
2022 | Model solution | Nexion 5000 | Pu-239, 240, 241, 242, 244 | 106 |
2022 | Water | Not available | Th-230, 232; U-234, 235, 238 | 107 |
2022 | Atmospheric deposition | Agilent 8800 | U-235, 236, 238 | 108 |
2022 | Soil, sediment | Agilent 8900, Nexion 5000 | Pu-239, 240, 241 | 109 |
2022 | Environmental samples | Agilent 8900 | Tc-99 | 110 |
2022 | Soil | Agilent 8900 | Am-241 | 111 |
2022 | Environmental | Agilent 8900 | I-129 | 138 |
2023 | Cotton swipes | iCAP TQ | U-234, 235, 236, 238; Pu-239, 240 | 112 |
2023 | Environmental gaseous samples | Agilent 8900 | I-129 | 113 |
2023 | Soil | Agilent 8900 | Pu-239, 240 | 114 |
2023 | Soil | Agilent 8800 | Np-237; Pu-239, 240 | 115 |
2023 | High U sample | Agilent 8800 | Pu-238, 239, 240, 241 | 116 |
2023 | Environmental samples | Agilent 8900 | U-236, 238 | 117 |
2023 | Standard | Agilent 8900 | Np-237; Am-241; Cm-244 | 118 |
2023 | Soil and sediment | Agilent 8900 | Cs-135, 137 | 119 |
2023 | Environmental samples | Agilent 8900 | Cs-135, 137 | 120 |
2023 | Water | Agilent 8900 | Pu-239, 240 | 121 |
2023 | Multiple matrix | Agilent 8800 | Ni-63; Sr-90; Zr-93; Tc-99; I-129; Np-237; Pu-239 | 122 |
2023 | Sediment samples | Agilent 8900 | Am-241 | 124 |
2023 | Urine | Agilent 8800 | U-234, 235, 238; Pu-239, 240, 241 | 125 |
2023 | Urine | Agilent 8900 | Sr-90 | 137 |
2023 | Soil | Agilent 8800 | Np-237; Pu-239, 240 | 126 |
2023 | Gd sulfate octahydrate | Agilent 8800 | Ra-226 | 123 |
2023 | Wild boars | Agilent 8900 | Cs-135, 137 | 139 |
2023 | Urine | Agilent 8800 | Sr-90 | 137 |
2023 | Decommissioning waste | Agilent 8800 | I-129 | 140 |
2024 | Model solution | Agilent 8900 | U-238; Pu-238, 239 | 127 |
2024 | Environmental samples | Agilent 8900 | Pu-239 | 128 |
2024 | Metal sample | Agilent 8800 | Th-230 | 130 |
2024 | Urine | Agilent 8900 | Np-237; Pu-239, 240, 241; Am-241; Cm-244 | 131 |
2024 | Bottled drinking water | Agilent 8900 | Po-210; Ra-226, 228; Th-230, 232; U-234, 235, 236 | 132 |
2024 | Uranium ore | Agilent 8800 | Th-230, 232; U-234 | 133 |
2024 | Biological samples | Agilent 8800 | Pu-239, 240 | 134 |
2024 | Scintillation film | Agilent 8800 | Th-232; U-238 | 129 |
2024 | Natural water | Agilent 8800 | I-129 | 141 |
Publishing year | Sample | Instrument | Element or isotope of interest | Ref. no. |
---|---|---|---|---|
2017 | River water, spring water | Agilent 8800 | REEs; Th-232; U-238 | 144 |
2019 | Arctic samples | Agilent 8900 | REEs; U-238 | 145 |
2019 | Sediment | Agilent 8800 | REEs; Th-232; U-238 | 147 |
2019 | Water and sediment | Agilent 8800 | REEs; Th-232; U-238 | 150 |
2020 | Sediment | Agilent 8800 | REEs; Th-232; U-238 | 153 |
2021 | CMX-6 | Agilent 8800 | REEs; U-234, 235, 236, 238; Pu-239, 241, 242 | 143 |
2021 | Sediment | Agilent 8800 | REEs; U-238 | 148 |
2022 | Water CRMs | Agilent 8800, Agilent 8900 | REEs; Th-232; U-238 | 142 |
2023 | Water | Agilent 8900 | REEs; U-238 | 146 |
2023 | Plant SRMs | Nexion 5000 | REEs; Th-232; U-238 | 152 |
2024 | Sediment | Agilent 8800 | REEs; U-238 | 149 |
2024 | Wheat flour | Agilent 8800 | REEs; Th-232; U-238 | 151 |
![]() | ||
Fig. 2 Distribution of publications according to the topics of lanthanides (REEs), radionuclides (RNs), both (RNs and REEs), and reviews. |
According to Tables 2–4, it can be seen that the measurement of REEs and RNs by ICP-QMS/QMS has been applied in various research fields, covering material, geological, biological, environmental, and food.
The instrument model is dominated by Agilent 8800 (together with Agilent 8900), which is partially attributed to its early availability since 2012. Alternatively, the application of iCAP TQ and Nexion 5000 has increased since 2021 and 2022, respectively. Considering that these instruments were released in different years (Agilent 8800, 2012; Agilent 8900, 2016; iCAP TQ, 2017; and Nexion 5000, 2020),9 it can be expected that the application of the latter instruments will increase apparently in the near future.
The most significant advantage of ICP-QMS/QMS is its capability to separate spectral interference, while the effectiveness of the separation depends on the reactions between the ions and gas molecules in the CRC. Therefore, choosing the optimum cell gas (or gas mixture) is an important step to take the advantage of ICP-QMS/QMS.
The cell gases investigated in the references covered in the present work are summarised in Table 5, together with the number of references for each type of gas. Among them, it can be seen that oxygen (70) is the most investigated cell gas, followed by helium (61) and ammonia gas (34). Hydrogen was also often investigated as a cell gas, which has been reported in 23 references. One of the reasons for using these gases as the cell gas is that they are usually the standard for an ICP-QMS/QMS instrument. It is notable that N2O (25) and CO2 (17) were also widely investigated although are not the standard. Also, it is noteworthy that ozone was used as a reaction gas.141
Gas | References | Count |
---|---|---|
He | 13–16, 20, 22–24, 28, 29, 34, 36, 37, 39, 40, 42, 43, 49, 60, 65, 67, 68, 73, 74, 81, 83, 86, 89–92, 94, 96, 98, 101, 102, 107, 111, 112, 115, 116, 119–122, 124–126, 131–133, 142, 144–151 and 153 | 61 |
H2 | 15, 16, 18, 22, 29, 31, 43, 51, 58, 59, 65, 71, 73, 90–93, 122, 143, 144, 146, 147 and 153 | 23 |
O2 | 1, 12, 13, 15–18, 20–25, 27, 35, 36, 39, 44–47, 51, 53, 55, 58, 59, 62, 65, 67–70, 72, 73, 75, 76, 78, 79, 81, 85, 92, 93, 98, 102, 105, 106, 108, 110, 111, 113, 114, 116–118, 121, 122, 124, 127, 131, 135, 136, 138, 140, 142, 144, 145, 147–149 and 153 | 70 |
NH3 | 1, 12–14, 16, 21, 25, 26, 28, 34, 39, 41, 51, 58, 59, 62, 66–68, 73, 77, 86, 90, 91, 95, 96, 99, 109, 116, 119, 120, 122, 134 and 144 | 34 |
N2O | 29, 32, 33, 42–44, 48, 49, 51, 52, 54, 56, 57, 81, 84, 100, 101, 116, 117, 119, 120, 127, 138, 139 and 152 | 25 |
CH4 | 51 | 1 |
C2H2 | 51 | 1 |
CO2 | 51, 68, 71, 79, 81, 94, 98, 105, 106, 112, 115, 116, 118, 127, 137, 138 and 143 | 17 |
NO | 106 and 128 | 2 |
O3 | 141 | 1 |
The dominant reaction gas used for REEs was oxygen, which is mainly attributed to its capability to form monoxide for the mass-shift measurement of REEs.1,12,16–18,20–25,27,35–37,44 However, the yields of monoxides of Eu and Yb (approximately 20%) were much lower than that of other REEs (over 90%) due to their endothermic reaction with oxygen, resulting in deteriorated sensitivity for mass-shift measurement.22,23,35,53 An improvement in the yield of monoxides of Eu and Yb by two- to three-fold could be achieved via optimization of the operating conditions of ICP-QMS/QMS in terms of a higher collision energy.27 A more reactive gas, N2O, was also applied in the measurement of REEs in mass-shift mode with higher yields of monoxide ions for the whole set of REEs, including Eu and Yb with yields of over 80%.32,33,42,44 It is notable that slightly decreased (by 5% to 10%) yields of monoxide ions were found for some REEs (e.g. La) due to the formation of dioxide ions.
On-mass mode measurements of REEs with hydrogen15,16,18,22,29,31,43 or helium12–16,20,22–24,29,34,36,37,39–43 as the cell gas were reported in multiple works, owing to their ready availability as cell gases or less challenging spectral interferences.
Ammonia gas was also investigated as a cell gas for the measurement of REEs in multiple works.1,12–14,16,28,34,39,41 It is notable that due to the formation of BaO2+ in a high-concentration Ba solution, the on-mass measurement of Eu isotopes with NH3 reaction resulted in a better performance than the mass-shift measurement with O2 reaction.16 Ammonia reaction was the most effective for separating signals of Lu and Hf for their isotopic analysis, where Lu could be measured in the on-mass mode and Hf in the mass-shift mode of ion clusters of Hf with NH3.26,28,34,41
The additional application of NH3 (in He) helped remove polyatomic interferences from 119Sn16O+, 95Mo40Ar+, 97Mo40Ar+, and 121Sb16O+.119,120
Oxygen is effective in removing the interference from 90Zr+ by transforming it to its oxide ions.45,51,58,72,92,93,122 Recently, Yang et al. demonstrated that the introduction of CO2 instead of O2 could further mitigate isobaric/polyatomic interferences, especially that caused by Zr and Ge.137
Additionally, the application of H2 and NH3 resulted in the best performance for the measurement of 90Sr+ by separating Zr- and Y-related spectral interferences.59
Oxygen was used in most works for measuring 129I+ by ICP-QMS/QMS, while on-mass measurement was selected to remove 129Xe+ and 127I1H2+ as their products from reactions with O2.46,75,105,113,135,136,140 Matsueda et al. tried to improve the analytical performance for the on-mass measurement of 129I+ using CO2 in addition to O2 as the reaction gas.105
Coralie et al. compared N2O, CO2 and O2 as the reaction gas for the mass-shift measurement of 129I+ as its monoxide ion.138 Among them, the best analytical performance was achieved with O2, resulting in a yield of approximately 15% of monoxide ion of 129I+.
In a recent study by Zhu and Asakawa, they used on-line-generated ozone (O3) as the reaction gas for the mass-shift measurement of 129I+.141 Due to its spontaneous reaction with O3, 129I+ could be measured as its monoxide ion and dioxide ion with yields of approximately 60% and 20%, respectively.
Helium was usually used as an additional gas with oxygen, CO2, and N2O, helping to improve the reactions by enhancing the collision opportunities.67,74,78,79,81,92,94,107,112,125,132,133
The dominant reaction gases used for the measurement of Pu isotopes were NH3,51,66,77,80,86,95,96,103,109,116,134 CO2,51,68,71,106,112,115,127,143 and O2,65,98,114,121,122,131 respectively. It is notable that CO2 was used more often than O2, regardless of the fact that O2 is one of the standard reaction gases for ICP-QMS/QMS independent of its manufacturer. This can be attributed to the fact that the measurements of Pu isotopes were conducted in on-mass mode with the polyatomic spectral interferences reduced by reaction with the gas molecules. The reactions with NH3 and CO2 resulted in the better removal of these spectral interferences and provided a better performance for the measurement of Pu isotopes.
Due to the extremely low concentrations (usually under ng kg−1 or ng L−1) of REEs and RNs in natural samples, pretreatment for the enrichment of the objective element and/or separating it from the sample matrix is usually required prior to measurement by ICP-QMS/QMS.
Ebeling et al. reported an automatic SPE method based on a commercially available on-line system (with Nobias chelate-PA1 column, ethylene diamine triacetate and imino-diacetate functional groups), achieving a preconcentration factor of 20 for trace elements including REEs in natural water samples.142
Ding et al. reported an SPE method using UTEVA resin (diamyl amylphosphonate) for separating REEs from the matrix of uranium ore. The recovery for each REE was over 93% with an acceptable concentration (<100 ng mL−1) of uranium in the final solution.23
Labrecque et al. compared cloud point extraction and SPE for separation of REEs in isotopic analysis.14 Regardless the fact that both methods were based on an extractive ligand of di-glycol amide analogues, the cloud point extraction method showed excellent recoveries (over 99%) for Nd, Sm, and Eu, which were superior to that obtained with the SPE method (45% to 68%).
Zhang et al. reported a solvent extraction method for the determination of REE impurities in Ce chelates.21 REEs were extracted in bis(2,4,4-trimethylpentyl)phosphinic acid at pH 4 (with the oxidation of Ce by KMnO4), and then back extracted with 5% (v/v) HNO3. A matrix separation efficiency of over 99.9% was achieved with good reproducibility, resulting in a Ce concentration under 0.1 mg L−1 remaining. The recoveries of other REEs were over 90%.
Zhu reported an Mg(OH)2 coprecipitation method for the determination of REEs in seawater samples.22 An enhancement factor of 130-fold (peak height of signal intensity) was achieved by on-line elution and measurement of the precipitate, with the removal of over 99% salt contents.
Zheng et al. reported an improved method for the removal of major elements (e.g. Ca, K, and Mg) following AMP adsorption.57 Combining a 2 mL AG MP-1M resin (anion exchange) column, a 10.5 mL AG 50W-X8 resin-packed Eppendorf pipette, and 2 mL Sr resin cartridge, sufficient removal of the matrix elements and interfering elements was achieved for the analysis of low-level 137Cs (20–1000 Bq kg−1) using large-size samples (e.g. up to 40 g soil and sediment samples). This separation method showed high separation factors (104–107) for the major matrix elements (Al, Ca, K, Mg, Na and Si) and interfering elements (105–106 for Ba, 106–107 for Mo, 104–106 for Sb and 104–105 for Sn).
It is notable that a desolvation system helped improve the signal intensity in the measurement by ICP-QMS/QMS, which was attributed to the uptake efficiency of Cs isotopes in the plasma.57,80,84,120
Strontium in urine samples was efficiently separated by phosphate co-precipitation, followed by extraction chromatography with Pre-filter resin, Eichrom TRU resin (having carbamoylphosphine oxide functional groups), and Sr resin (having 4,4′(5′)-di-t-butylcyclohexano 18-crown-6 functional groups).72 This method enabled the determination of 1 Bq 90Sr per urine sample (1–2 L) for assessing the internal exposure of workers in a radiological emergency. Yang et al. applied DGA and Sr resin cartridges for the separation of Sr, following CaF2 co-precipitation in 400 mL urine samples. In this study, stable 88Sr was used as a yield tracer for the recovery correction of 90Sr.137
In the work by Carrier et al., environmental gaseous 129I trapped in a charcoal cartridge was purified with an SPE method after acid digestion.113 The SPE method was based on Ag+-functionalized CL resin, which retained iodide as AgI. The elution of 129I was achieved with a solution of 0.35 mol per L Na2S.
Yang et al. reported a multi-step mild extraction protocol for measuring 129I in solid environmental samples.136 The first step was extraction with 10% TMAH at 90 °C, and the second step was using K2S2O8 for releasing iodine from organic matter. In the third step, the reduction of iodate was conducted using (NH4)2SO3 with the assistance of CCl4. After the removal of the organic layer in step four, iodine was extracted with NaNO2 in step five. The final step was back extraction with (NH4)2SO3.
Zacharauskas et al. used a simple combustion process at 900 °C, followed by trapping with 3% TMAH solution for measuring 129I in nuclear waste simulant samples.140
Also, other resins were reported as pretreatment for the measurement of radionuclides of uranium, including AG1X8 (a strong cation exchange resin),69,74,79 DGA,54,61,70,76,85,92,125 and TRU resins.78,132
The operating conditions for mass-shift mode measurement benefit the passing of a relatively higher mass polyatomic ion to the detector, with a negative voltage applied to the exit of the CRC, helping to improve the transmission of the ion of interest. In this case, the sensitivity depends on the yield of the polyatomic ion. The sensitivities for most elements measured in mass-shift mode with O2 (M+ → MO+) and NH3 (M+ → MNH+) were under 50% and 20%, respectively, of that obtained under no-gas condition.155
The systematic characterization of the gas cell reactions using NO, N2O and O3 was also reported, respectively.155–157 These works provide greatly valuable information for further development in the analysis of REEs and radionuclides.
Ion of interest | Interfering ions | Reaction gases | Measuring mode | Typical reactions | References |
---|---|---|---|---|---|
139La+ | 138Ba1H+ | H2 | On-mass | 138Ba1H+ → 138Ba+ | 18 and 31 |
151Eu+ | 135Ba16O+ | 135Ba16O+ → 138Ba+ | |||
169Tm+ | 153Eu16O+ | 153Eu16O+ → 138Ba+ | |||
139La+ | 138Ba1H+ | O2 | Mass-shift | 139La+ → 139La16O+ | 1, 12, 17, 18, 20–25, 27, 35, 36 and 44 |
151Eu+ | 135Ba16O+ | 151Eu+ → 151Eu16O+ | |||
169Tm+ | 153Eu16O+ | 169Tm+ → 169Tm16O+ | |||
176Lu+ | 176Hf+ | NH3 | On-mass | 176Hf+ → 176Hf14N51H12+ | 26 |
139La+ | 138Ba1H+ | N2O | Mass-shift | 139La+ → 139La16O+ | 32, 33, 42 and 44 |
151Eu+ | 135Ba16O+ | 151Eu+ → 151Eu16O+ | |||
169Tm+ | 153Eu16O+ | 169Tm+ → 169Tm16O+ | |||
135Cs+ | 135Ba+ | N2O | On-mass | 135Ba+ → 135Ba16O+ | 48, 49, 51, 52, 54, 56, 57, 84, 100, 101, 119 and 120 |
137Cs+ | 137Ba+ | 137Ba+ → 137Ba16O+ | |||
135Cs+ | 119Sn16O+, 95Mo40Ar+ | N2O, NH3 | On-mass | 119Sn16O+ → 119Sn+; 95Mo40Ar+ → 95Mo+ | 119 and 120 |
137Cs+ | 121Sb16O+, 97Mo40Ar+ | 121Sb16O+ → 121Sb+; 97Mo40Ar+ → 97Mo+ | |||
90Sr+ | 90Zr+, 89Y1H+ | O2 | On-mass | 90Zr+ → 90Zr16O+; 89Y1H+ → 89Y16O+ | 45, 51, 58, 59, 72, 92, 93 and 122 |
90Sr+ | 90Zr+, 89Y1H+ | O2, CO2 | On-mass | 90Zr+ → 90Zr16O+, 90Zr16O3+, ZrH3–4O3+, ZrH2O2+ | 137 |
90Sr+ | 90Zr+, 89Y1H+ | O2, H2, NH3 | On-mass | 90Zr+ → 90Zr16O14N41H12+; 89Y1H+ → 89Y16O14N41H12+ | 59 |
129I+ | 129Xe+, 127I1H2+ | O2 (or with CO2) | On-mass | 129Xe+ → 129Xe, 127I1H2+ → 127I+ | 46, 75, 105, 113, 135, 136 and 140 |
129I+ | 129Xe+, 127I1H2+ | O2 | Mass-shift | 129I+ → 129I16O+ | 138 |
129I+ | 129Xe+, 127I1H2+ | O3 | Mass-shift | 129I+ → 129I16O+; 129I+ → 129I16O2+ | 141 |
236U+ | 235U1H+ | O2 | Mass-shift | 235U1H+ → 235U16O+; 236U+ → 236U16O+ | 47, 54, 67, 70, 79, 81, 85, 92, 108 and 117 |
236U+ | 235U1H+ | O2, CO2 | Mass-shift | 235U1H+ → 235U16O+; 236U+ → 236U16O+ | 79 and 94 |
236U+ | 235U1H+ | N2O | Mass-shift | 235U1H+ → 235U16O2+; 236U+ → 236U16O2+ | 81 and 117 |
239Pu+ | 238U1H+ | O2 (with H2 or He) | Mass-shift | 239Pu+ → 239Pu16O2+; 238U1H+ → 238U16O2+ | 65, 98, 114, 121, 122 and 131 |
239Pu+ | 238U1H+ | CO2 (with H2 or He) | On-mass | 238U1H+ → 238U16O+, 238U16O2+ | 51, 68, 71, 106, 112, 115, 127 and 143 |
239Pu+ | 238U1H+ | NH3 | On-mass | 238U1H+ → 238U14N1H0–3+ | 51, 66, 77, 80, 86, 95, 96, 103, 109, 116 and 134 |
239Pu+ | 238U1H+ | NO | Mass-shift | 239Pu+ → 239Pu16O+; 238U1H+ → 238U16O+, 238U16O2+ | 128 |
The measurements of REEs were dominated by the mass-shift mode with O2 or N2O as the reaction gas. It is notable that the introduction of N2O as the reaction gas significantly improved the formation of monoxide ions of Eu and Yb, permitting the mass-shift measurements of a full set of REEs at high sensitivity.
The measurements of radionuclides of Cs were conducted in on-mass mode. The reactive property of N2O helps completely transform the interfering Ba ions to their oxide ions and break polyatomic ions of Sn, Sb, and Mo. The additional application of NH3 helped completely remove interferences from these polyatomic ions. The measurement of 90Sr was also conducted in on-mass mode utilizing O2 or CO2 (or with additional H2 and NH3) as the reaction gas. The on-mass and mass-shift measurements of 129I were often conducted with O2 as the reaction gas, while its monoxide ion was permitted to pass the second quadrupole for mass-shift measurement.
The measurements of radionuclides of U were conducted in mass-shift mode with O2, CO2, or N2O as the reaction gas. The shifting to oxides of 236U+ helped separate it from the interfering 235U1H+, which also shifted to the related oxides.
The measurements of radionuclides of Pu were conducted in mass-shift mode by shifting to oxide ions with O2 or NO as the reaction gas. The application of CO2 or NH3 permitted the measurement of radionuclides of Pu in on-mass mode, with interfering ions transferred to related polyatomic ions.
Dead time correction should be considered when measuring isotopic ratios with high signal intensities in pulse mode.160 The effect of dead time is more prominent for larger isotopic ratios, e.g. over 106 or under 10−6 requiring measurements with signal intensities over one million counts per second (CPS). A simple model for dead time correction is as follows: I1 = I0/(1 − I0 × t), where I1, I0, and t are the true signal intensity, observed intensity, and deadtime, respectively.
Ding et al. developed a simple and reliable chemical procedure for the separation of REEs from a uranium matrix before measurement by ICP-QMS/QMS.23 REEs were measured in mass-shift mode by using O2 as the reaction gas, which helped the effective suppression of polyatomic interferents in the measurement of REEs. The method detection limits for all REEs were below 1 pg mL−1, which ensured the precise and accurate measurement of REEs in small amounts of uranium ore samples.
Zhu compared N2O and O2 as the reaction gases for the measurement of REEs in mass-shift mode.33 The results showed that the N2O reaction apparently improved the yields of mM16O+ for Eu and Yb, which helped improve the sensitivities for the measurement of Eu and Yb in comparison to that obtained with O2 as the reaction gas. A typical sensitivity of 300000 CPS per ng per mL was obtained for REEs measured with an isotope having an isotopic abundance close to 100%. Furthermore, the N2O reaction also helped suppress Ba-related spectral interferences in the measurement of Eu and permitted the measurement of Eu in natural samples without mathematic correction of the spectral interferences. The instrumental detection limits for REEs ranged from 0.004 pg mL−1 of Tm to 0.028 pg mL−1 of La.
A comparison of the representative detection limits and sensitivities for the measurement of REEs is summarized in Table 7. It is notable that the method detection limit (MDL) cannot be simply compared due to their dependence on the pretreatment procedures. The sensitivities can be compared because they are all given as the signal intensities corresponding to 1.0 ng mL−1 of each REE. It can be seen that the measurements conducted in mass-shift mode (italic data) provided higher sensitivities in comparison to that obtained in on-mass mode. These results can be attributed to the difference in operating conditions, where in the case of on-mass mode measurement, a neutral or positive energy discrimination was applied at the under stream of the CRC, resulting in a decrease in the transmission of positively charged ions to the second quadrupole mass filter. By contrast, negative energy discrimination was applied for mass-shift mode and was beneficial for the improvement in the transmission of positively charged ions to the second quadrupole mass filter.
Element | m/z | Galusha et al.18 (H2, O2 reaction) | Ding et al.23 (O2 reaction) | Zhu33 (O2 reaction) | Zhu33 (N2O reaction) | ||||
---|---|---|---|---|---|---|---|---|---|
MDLb (ng g−1) | Sensitivityc | MDLb (pg mL−1) | Sensitivityc | IDLd (pg mL−1) | Sensitivityc | IDLd (pg mL−1) | Sensitivityc | ||
a Italic data were obtained via mass-shift mode (e.g. 139La+ → 139La16O+) measurements.b MDL, method detection limit.c Sensitivity unit, CPS per ng mL−1.d IDL, instrumental detection limit.e (i) and (ii) Different choices of isotopes for measurement. | |||||||||
La | 139 | 5.1 | 10![]() |
0.52 | 290![]() |
0.030 | 220![]() |
0.028 | 254![]() |
Ce | 140 | 4.7 | 90![]() |
0.63 | 170![]() |
0.024 | 217![]() |
0.018 | 238![]() |
Pr | 141 | 1.6 | 158![]() |
0.16 | 350![]() |
0.017 | 285![]() |
0.006 | 327![]() |
Nd | 146 | 5.6 | 16![]() |
0.69 | 61![]() |
0.022 | 48![]() |
0.026 | 59![]() |
Sm | 147 | 3.7 | 22![]() |
0.28 | 52![]() |
0.043 | 37![]() |
0.006 | 52![]() |
Eue | 151(i), 153(ii) | 1.0(i) | 41![]() |
0.98(ii) | 39![]() |
0.024(ii) | 44![]() |
0.010(ii) | 196![]() |
Gd | 157 | 5.3 | 23![]() |
0.50 | 52![]() |
0.011 | 39![]() |
0.017 | 52![]() |
Tb | 159 | 1.1 | 35![]() |
0.10 | 340![]() |
0.007 | 261![]() |
0.006 | 331![]() |
Dy | 163 | 2.8 | 22![]() |
0.15 | 90![]() |
0.033 | 66![]() |
0.016 | 86![]() |
Ho | 165 | 2.7 | 90![]() |
0.11 | 350![]() |
0.010 | 260![]() |
0.010 | 324![]() |
Er | 166 | 1.3 | 46![]() |
0.20 | 120![]() |
0.020 | 81![]() |
0.016 | 106![]() |
Tm | 169 | 0.9 | 96![]() |
0.17 | 310![]() |
0.012 | 224![]() |
0.004 | 320![]() |
Ybe | 172(i), 174(ii) | 1.3(ii) | 30![]() |
0.77(i) | 13![]() |
0.060(i) | 18![]() |
0.023(i) | 62![]() |
Lu | 175 | 1.6 | 31![]() |
0.15 | 330![]() |
0.019 | 233![]() |
0.012 | 312![]() |
It is noteworthy that the sensitivities for Eu and Yb were relatively lower when measured in mass-shift mode with oxygen as the reaction gas, which was attributed to the exothermic reactions for producing MO+ from M+. The introduction of N2O as the reaction gas helped overcome this problem and provided the best performance for measuring the whole set of REEs.
Zheng et al. developed a method to accomplish the sufficient separation of major elements (such as Ca, K, and Mg) for measuring trace radioactive Cs in large volume samples.57 The separation was achieved using a 2 mL AG MP-1M resin column, 10.5 mL AG 50W-X8 resin packed in an Eppendorf pipette, and 2 mL Sr resin cartridge, resulting in the complete removal of the interfering elements in large-size samples (up to 40 g soil and sediment samples) for the analysis of low-level 137Cs (20–1000 Bq kg−1). This separation method showed high decontamination factors (104–107) for major matrix elements (Al, Ca, K, Mg, Na and Si) and interfering elements (105–106 for Ba, 106–107 for Mo, 104–106 for Sb and 104–105 for Sn) for 10–40 g soil and sediment samples. By using an Apex-Q sample introduction system, the measurement sensitivity was significantly improved to 2.95 × 105 cps for 1 ng per mL 133Cs standard solution. Seven reference materials were used for the method validation. The JSAC-0471 (soil), JSAC-0766 (soybean) and JSAC-0776 (mushroom) reference materials collected 100–250 km southwest of the FDNPP site within the Kanto region of Japan following the Fukushima accident presented the 135Cs/137Cs isotope ratios of 0.378 ± 0.023, 0.353 ± 0.025, and 0.378 ± 0.021, respectively (decay corrected to March 11, 2011). In the case of IAEA-soil-6 (soil from the Upper Austria before the Chernobyl accident), with low 137Cs activity of 28.1 Bq kg−1, the 135Cs/137Cs ratio was measured to be 2.58 ± 0.37 (decay corrected to January 1, 2015). In the case of IAEA-385 (marine sediment from the Irish Sea), with the lowest 137Cs activity of 23.3 Bq kg, the 135Cs/137Cs ratio was measured to be 1.21 ± 0.14 (decay corrected to January 1, 2015). For IAEA-330 (Spinach) and IAEA-156 (Clover) (contaminated by radioactive Cs due to the Chernobyl accident), the 135Cs/137Cs ratio was measured to be 0.546 ± 0.031, and 0.541 ± 0.027, respectively (decay corrected to January 1, 2015). Using this ICP-QMS/QMS analytical method, Stäger et al. investigated radiocesium contamination in wild boars from Bavaria.139 Chornobyl has been widely believed to be the prime source of 137Cs in wild boars; however, using the emerging nuclear forensic fingerprint, 135Cs/137Cs ratio, they found that “old” 137Cs from global fallout significantly contributed to the total level (10–68%) in the investigated specimens that exceeded the regulatory limit (600 Bq kg−1).
Zhu et al. compared acid leaching using aqua regia and alkali fusion using LiBO2 for the recovery of radioactive Cs from large-size soil samples (1–60 g).84 Alkali fusion resulted in high recovery of >93% due to the complete decomposition, while acid leaching presented a high leaching efficiency (>85% for samples less than 10 g and even >60% for samples up to 60 g). Given that acid leaching is simple, with easy operation, less time-consuming, and more suitable for the treatment of large-size samples compared with the fusion method, acid leaching using aqua regia with a sample/acid ratio of 1:
8 at 180 °C for 2 h was recommended and used. After preconcentration by AMP-PAN, NH4HCO3, (NH4)2CO3, NH4F, NH4C2O4, NH4Ac, and NH4Citr solution could directly dissolve the AMP component, similar to ammonia solution. Considering the easy removal of NH4Cl by the heating method based on its sublimation at low temperatures (338 °C), the risk for dangerous explosion of NH4NO3 during heating, and difficulties in the removal of sulfate, NH4Cl was selected to elute Cs+ from the AMP-PAN resin. Based on the low sublimation temperature of NH4Cl (338 °C) but not CsCl, a simple heating method was developed to remove NH4Cl by sublimation. The increased recoveries of Cs from 31% to 99% with the amount of LiCl of 60 mg confirmed that a sufficient amount of particles/salt is important for preventing the loss of Cs during the sublimation of NH4Cl. A 10 mL cation exchange resin (AG50W-X8) in a column of φ1.0 × 20 cm was employed for achieving the better separation of Cs from Ba, Rb, and K. The overall decontamination factors of 4 × 107 for Ba, 4 × 106 for Li, 4 × 105 for Mo, 3 × 105 for Sn, and 2 × 105 for Sb were achieved. Also, the high throughput of 8 samples per 3 days was achieved. The measured 135Cs/137Cs atomic ratios (decay corrected to 1st Feb 2020) in soils collected from Gavle, Sweden and Feofaniya, Ukraine were similar (0.65–0.71), although the 137Cs concentrations (140–1650 Bq kg−1) were significantly different. This indicated that most of the radioactive Cs in these samples originated from the Chernobyl accident fallout. Much higher 135Cs/137Cs atomic ratios (2.08–2.68, decay corrected to 1st Feb 2020), but much lower 137Cs concentrations (3–8 Bq kg−1) were observed in soil samples from Denmark. By calculation, the contributions of radioactive Cs from the Chernobyl accident were estimated to be 31% and 51% for these two soil samples, respectively.
Tomita et al. developed a rapid analytical method for determining 90Sr in urine samples (1–2 L) to assess the internal exposure of workers in a radiological emergency.72 Strontium in a urine sample was rapidly separated by phosphate co-precipitation, followed by extraction chromatography, and the 90Sr activity was determined by ICP-QMS/QMS. Measurement in on-mass mode with an O2 reaction gas flow rate of 1 mL min−1 showed no tailing of 88Sr at m/z = 90 up to 50 mg per L Sr. The interferences of Ge, Se and Zr at m/z = 90 were successfully removed by phosphate co-precipitation, followed by extraction chromatography with a tandem column of Pre-filter, Eichrom TRU and Sr resin. This analytical method was validated by the results of the analyses of synthetic urine samples (1.2–1.6 L) containing a known amount of 90Sr together with 1 mg of each of Ge, Se, Sr and Zr. The turnaround time for Sr purification from the urine sample to 90Sr measurement was about 10 h. The detection limit of 90Sr was approximately 1 Bq per urine sample, which was lower than 15 Bq per urine after a day of intake, giving 5 mSv of unplanned exposure of worker limited by the Nuclear Regulation Authority of Japan.
Wang et al. developed an online separation and preconcentration method employing a lab-on-valve system for the analysis of 90Sr in various water/wastewater samples.93 90Sr was separated from 90Zr, an isobaric interference present at high concentrations in many samples, and other matrix components using a dual-column setup (Eichrom DGA-Branched resin and Sr resins). Subsequently, any remaining 90Zr was chemically resolved from the 90Sr in the measurement by ICP-QMS/QMS using O2 and H2 as the reaction gases. This system required small sample volumes (10 mL), minimal sample preparation compared to traditional radiometric, and other ICP-MS techniques and has a processing time of 22 min per sample. Based on a 10 mL sample size, the system limit of detection, limit of quantification and method detection limit (MDL) were 0.47 Bq L−1 (0.09 pg L−1), 1.57 Bq L−1 (0.32 pg L−1) and 1.79 Bq L−1 (0.34 pg L−1), respectively. Recovery of the IAEA 2018 Proficiency Test Exercise water sample (n = 5) was 99% with an RSD of 11.9%. Thus, this method provides a powerful tool for the rapid analysis of low levels of 90Sr.
Suzuki et al. developed a new analytical system that enables the real-time analysis of 90Sr in atmospheric particulate matter with an analytical run time of only 10 min.59 After passage of an air sample through an impactor, a small fraction of the sample is introduced into a gas-exchange device, where the air is replaced by Ar. Then, the sample is directly introduced into the ICP-QMS/QMS for measurement, where the separation of isobaric interferences on 90Sr+ from 90Zr+, 89Y1H+, and 90Y+ was investigated under various reaction gas conditions. The results showed that interferences could be minimized under the optimized conditions of 1 mL per min O2, 10 mL per min H2, and 1 mL per min NH3. The estimated background equivalent concentration and estimated detection limit of the system were 9.7 × 10−4 and 3.6 × 10−4 ng m−3, which are equivalent to 4.9 × 10−6 and 1.8 × 10−6 Bq cm−3, respectively. The recoveries of Sr in PM2.5 measured by real-time analysis compared to that obtained by simultaneously collection on the filter was 53% ± 23%, and using this recovery, the detection limit of PM2.5 was estimated to be 3.4 ± 1.5 × 10−6 Bq cm−3. Specifically, this system enabled the detection of 90Sr at concentrations of <5 × 10−6 Bq cm−3, even considering the insufficient fusion/vaporization/ionization efficiency of Sr in PM2.5.
For 90Sr analysis, the application of O2 as the reaction gas to mitigate isobaric and polyatomic interferences (e.g. 90Zr+ and 89YH+) resulted in serious polyatomic interferences due to oxides (e.g. 72Ge18O+ and 74Ge16O+). Yang et al. developed a rapid 90Sr bioassay in small-amount urine (10–400 mL) using ICP-QMS/QMS, with the introduction of the innovative reaction gas of CO2.137 After organic matter decomposition and chemical separation, stacked DGA and Sr resin cartridges were used directly for the chromatographic separation and purification of Sr. The Sr yields were measured to be 94% ± 5% (n = 12) for the whole procedure, using stable 88Sr originally in the urine sample as a yield tracer. The produced ions in the CRC demonstrated that oxygen transfer and CO2 clusterization occur after the reaction between CO2 and Zr, further mitigating the isobaric interference from 90Zr, compared to the O2 reaction gas. The false signal intensities resulting from 72Ge18O+ and 74Ge16O+ using CO2 reaction gas also deceased to about 1/5 of that using O2 reaction gas. For further method validation, the 90Sr concentrations in urine samples were measured during the PROCORAD (Association for the PROmotion of Quality COntrol in RADiotoxicological Analysis) intercomparison campaign. All the results were in good agreement with the assigned values.
Coralie et al. reported the first mass-shift measurement of 129I by ICP-QMS/QMS with O2 as the reaction gas.138 Measurements with N2O and CO2 as the reaction gases were also performed but showed lower sensitivity than that obtained with O2 reaction. Multiple surfactants were investigated as reagents to improve the sensitivity for measuring iodine. A signal gain of 2.5 was achieved by adding 3% surfactant, while this gain was independent of the type of surfactant. The optimal measurement medium for the measurement of iodine was a solution of 0.1% NH4OH (v/v), 3% Tween 20, and 10 g per L ascorbic acid, achieving the IDL and BEC values of 1.7 pg mL−1 and 2.9 pg mL−1, respectively. A ratio of 3.8 × 10−9 was achieved for the analysis of 129I/127I.
Ohno et al. developed a new method for the determination of 129I in soil samples using ICP-QMS/QMS with O2 as the reaction gas and on-mass measurement with the objective of investigating radioiodine released by the FDNPP accident.135 By measuring the 129I/127I ratio in NIST SRM 3231 Level II standard solution, they demonstrated the reliability of the developed ICP-QMS/QMS method for the measurement of the 129I/127I ratios at a level of 10−8–10−9.
Zhu and Asakawa reported the mass-shift measurement of 129I by ICP-QMS/QMS with on-line generated ozone (ca. 10.5% O3 in O2) as the reaction gas.141 Due to the exothermic reactions, the yields of oxide and dioxide ions of iodine were significantly improved by ozone reaction in comparison to that obtained by oxygen reaction. Using H2 as an additional reaction gas helped reduce the residual spectral interference of 129Xe16O+ with the measurement of 129I+ → 129I16O+, achieving the IDL and the BEC values of 0.062 pg mL−1 and 0.016 pg mL−1, respectively. The best analytical performance for 129I/127I ratio analysis was achieved by measuring (129I+ → 129I16O2+)/(127I+ → 127I16O2+), resulting in a ratio of 6.7 × 10−10 in 500 μg per mL natural iodine solution.
Jaegler and Gourgiotis measured U isotope ions as their dioxides by introducing N2O as the reaction gas while using a desolvation system (APEX Ω) for sample introduction.117 As a result, tailing from the major isotopes and hydride interference were significantly reduced and the 236U/238U isotope ratio at the 10−11 level could be precisely measured. This method has potential applications in various geochemical studies.
Lindahl et al. conducted a detailed study on the stability of ICP-QMS/QMS in measuring U concentrations and isotope ratios.88 The results showed that the drift could reach up to 100%, which is probably due to the instability of the electronic components/devices associated with the quadrupole. Thus, to solve this problem, corrections were necessary for the accuracy and the precision by means of the appropriate adjustment of the mass resolution and the sample standard bracketing method. This worked showed that the instrumental stability also requires careful attention during the mass spectrometry determination of uranium isotopes.
Huang et al. reported a rapid analytical method for the simultaneous determination of 238Pu, 239Pu, 240Pu and 241Pu using ICP-QMS/QMS after chemical separation.116 A high decontamination factor of 2.19 × 109 for the most critical interfering element (i.e. U) was obtained with effective chemical separation using two sequential TK200 columns. The interferences of 238U1H+ and 238U+ were effectively eliminated due to their conversion to UNH+ and UNH2+, respectively, with NH3 as the reaction gas for ICP-QMS/QMS. Given that Pu hardly reacts with NH3 and remains as Pu+, on-mass mode measurement was performed to realize the simultaneous determination of the hard-to-measure 238Pu, 239Pu, 240Pu and 241Pu in environmental samples at fg (i.e. 10−15 g) levels.
Zhang et al. developed a method using ICP-QMS/QMS measurement in mass-shift mode with O2 and He as the reaction gases combined with a chemical separation procedure.98 The reaction with O2 gas converted Pu+ to PuO2+, while polyatomic ions of Pb, Hg and Tl were difficult to react with O2 to form new interfering ions at m/z 271 or 272. Thus, when Pu was measured in mass-shift mode at m/z 271 and 272 (PuO2+), the interferences from Pb, Hg and Tl were completely eliminated. In addition, the lower peak tailing of 238U+ (<5 × 10−12) and the reduced 238UO2H+/238UO2+ atomic ratio (4.82 × 10−9) significantly suppressed the 238U-derived interferences. Combined with a UTEVA chromatographic separation, the overall high elimination efficiency of U interferences up to 1014 could be achieved. Thus, the wide application of the developed method for the accurate determination of fg-level 239Pu in high U samples, such as large-size deep seawater, deep layer soil and sediment, uranium debris of nuclear fuel, can be expected.
By contrast, radionuclides usually require measurement at lower pg mL−1 or even fg mL−1, as stated in the above-selected applications. As a single detector instrument, ICP-QMS/QMS provides a typical relatively standard deviation of approximately 0.1% to 0.3% for isotopic ratio measurement at 1.0 ng per mL solution. This precision is sufficient for isotopic ratio measurement in radionuclides analysis, considering the large variation in isotopic ratio of over 10 or even 100-fold.
Because of its potential for effective spectral separation without sacrificing sensitivity, ICP-QMS/QMS provides an ideal approach for measuring radionuclides. An additional merit provided by ICP-QMS/QMS is its capability for the quasi-simultaneous screening of multi-radionuclides in the full m/z range (e.g. 2 to 260), while the m/z range measured simultaneously by MC-ICP-MS usually covers a narrower range (e.g. approximately 20).
The analysis of radionuclides in solid samples also involved complicated chemical separation with multiple solid phase columns.49,52,57 Thus, it can expected that automation of these chemical separation process will be beneficial for the analysis of radionuclides by ICP-QMS/QMS.11 The works by Ohira's group showed that the use of electrodialytic devices can be an effective approach for the separation and enrichment of trace elements prior to the measurement by an instrument.169,170 This new type of technique may find application in the analysis of REEs and radionuclides by ICP-QMS/QMS in the near future.
The application of various reactive gases (H2, O2, NH3, N2O, CO2, etc.) helped separate spectral interferences in the measurement of REEs and radionuclides. One of the most challenging works in the measurement of radionuclides is the analysis of 238Pu in a uranium matrix, which contains a high concentration of 238U. The application of He and NH3 as the reaction gases resulted in a ratio of 239Pu/238U in the order of 10−9.116 However, a 1.0 ng per mL uranium solution will result in a signal intensity for 238Pu equivalent to 0.2 pg per mL Pu. Further investigation of more effective methods for the separation of Pu and U is required for the direct measurement of a much lower Pu content in a higher concentration of U samples. Ozone has been shown to be effective for separating spectral interferences in the measurement of 129I and may find more applications in the measurement of other RNs.
The Agilent 8800 and 8900 ICP-QMS/QMS have been mostly used in works on radionuclides to date. However, one of their limitations is their upper limit of m/z range for the second quadrupole, which is 260 and 275 for 8800 and 8900, respectively. This configuration limited the investigation of higher order cluster ions of actinides, e.g. the measurement of 238U(14N1H3)3+, requiring a range of up to 289. Extension of this limit to over 300 will be helpful for works on the measurement of actinides by ICP-QMS/QMS, providing sufficient investigation and application about the mechanism of related ion–molecule reactions.
In addition to He, H2, O2, and NH3, which are usually standard in the instruments, N2O and CO2 have also been widely used as reaction gases in measurement by ICP-QMS/QMS. The application of N2O and CO2 specially helped separate spectral interferences in measuring RNs of Cs, Sr, U, and Pu.
Acid digestion, acid leaching, and alkali fusion have often been used to convert solid samples to solutions, followed by chemical separation such as SPE, solvent extraction, and coprecipitation.
ICP-QMS/QMS has shown excellent performances for the analysis of REEs and RNs, which is attributed to the effectiveness of separating spectral interferences by using the well-controlled ion–molecule reactions in the reaction cell. Extension of the upper limit of the m/z range of the second quadrupole mass filter will be beneficial for further works on actinides.
This journal is © The Royal Society of Chemistry 2025 |