Introduction

Neptunium is commonly measured in the nuclear field for various applications such as radioactive waste management, environmental samples or nuclear fuel characterization [1,2,3,4,5,6]. In the field of nuclear fuel characterization, it is of great importance to obtain experimental data after irradiation in order to qualify nuclear database and neutronic calculation codes. 237Np has three main ways of production [1, 7, 8] in the nuclear reactor:

  1. 1.

    a (n, 2n) reaction inducing the production of 237Np from 238U.

  2. 2.

    a 236U atom, produced by the reaction of 235U with a neutron, generating 237U by neutron capture which then becomes 237Np by β-decay.

  3. 3.

    237Np can be produced by α-decay of 241Am, produced into the reactor.

Insufficient knowledge about the 236U neutron capture cross section can therefore lead to uncertainties in the back-end of spent nuclear fuel or reprocessed uranium-recycling studies due to the underestimation of the amount of 237Np and by consequence of 238Pu in the spent fuel which is produced by neutron capture of 237Np [9, 10].

In order to gain better knowledge of nuclear data of radionuclides, some specific irradiation campaigns have been realized in dedicated experimental nuclear reactors. One of them was performed in the 1980’s: UO2 pellets doped with the 236U isotope were irradiated in the experimental pressurized water reactor Melusine in Grenoble (France) [11,12,13,14] and stored after irradiation during more than 30 years. After irradiation, the measurements of the 237Np/238U ratio could help to understand the underestimation of 237Np in the spent fuel. In these experimental samples, the predicted 237Np/238U ratio varied between 10 × 10–6 mol·mol−1 and 100 × 10–6 mol·mol−1.

Numerous techniques make it possible to measure 237Np in different matrices as referenced and reviewed in [1, 15]. 237Np can be determined by either alpha spectrometry [16,17,18], alpha liquid scintillation with rejection of β–γ emitters [19, 20], neutron activation analysis [18], high-resolution gamma spectroscopy (HRGS) [18, 21, 22] or mass spectrometry techniques such as glow discharge mass spectrometry (GDMS) [8], accelerator mass spectrometry [23, 24] or inductively coupled plasma mass spectrometry (ICP-MS) [6, 16, 17, 21, 25,26,27,28]. The latter technique has in the last 20 years become more and more utilized due to its rapidity, high sample throughput, and low limit of detection (< fg/g) [20, 29] compared to the other techniques. ICP-MS can be also hyphenated with separative techniques to measure 237Np [30, 31]. Another major advantage of the ICP-MS technique, as the other mass spectrometric techniques, comes from the absence of isobaric interference at the m/z ratio = 237 amu [21].

If in the environmental samples, the main difficulty is the chemical separation to eliminate the matrix from the 237Np fraction [18, 27], in the case of nuclear samples, the most challenging point is the presence of high amounts of uranium relative to Np. In addition to this, the studied UO2 pellets contain an unusual amount of 236U. Therefore, in the ICP-MS technique, the peak tail coming from the 238U isotope or molecular interferences (i.e., 236UH+) can lead to inaccuracies if these phenomena are not properly corrected [16]. In quadrupole ICP-MS (Q-ICP-MS) techniques, 237Np as well as other elements present in nuclear samples can be measured using the external calibration curve method or the gravimetric standard addition method [6]. The literature has also described the use of multi collection ICP-MS (MC-ICP-MS) without performing measurements in the multi-collection mode [32].

In the Nuclear Isotopic and Elemental Analytical development Laboratory (LANIE) of the French Atomic and Alternative Energies Commission (CEA) Paris-Saclay, the 237Np/238U ratio is precisely determined with a two-step method: the first step consists in measuring the 237Np concentration using Q-ICP-MS; the second is to establish the 238U concentration using single isotope dilution mass spectrometry (IDMS). The latter step requires the additional determination of the uranium isotope composition. This conventional approach was limited for some samples analyzed in the present study in relation to the significant abundance sensitivity of the Q-ICP-MS technique: some of the samples had an estimated 237Np/238U around 10 × 10–6 mol·mol−1 with as a direct consequence the potential difficulties of precisely measuring the 237Np in such samples. To overcome this issue, a new method was developed on a multi-collection inductively coupled plasma mass spectrometer (MC-ICP-MS). This approach, based on a calibration curve, uses a Faraday cup to determine 238U and a secondary electron multiplier (SEM) equipped with a retarding potential quadrupole filter (RPQ) to measure 237Np. In this configuration, the SEM allows the measurement of a low signal of 237Np and the RPQ filter improves the abundance sensitivity of the instrument. This novel method makes it possible to analyze relatively low elemental 237Np/238U ratios from 10 × 10–6 mol·mol−1 to 100 × 10–6 mol·mol−1 without a prior chemical separation step and without the need for uranium isotope composition determination as is required for the IDMS approach.

The aim of the present article was to present the methodology used for developing and validating the direct measurement of the 237Np/238U ratio using MC-ICP-MS. After a detailed description of the method, also including the instrumentation, the analytical condition and the mathematical equations, the validation realized in two steps is presented. Firstly, a simulated sample gravimetrically prepared with certified reference solutions was measured using the new approach on MC-ICP-MS and compared to the value derived from the certificates. Secondly, a comparison was made with the conventional approach (IDMS for 238U measurement + Q-ICP-MS for 237Np measurement) on two samples. The results obtained on six UO2 dissolved pellets and a simplified uncertainty assessment model was established and discussed.

Experimental

Reagents and reference material solutions

High purity 67–70% nitric acid (PlasmaPURE, from SCP Science, Baie d’Urfé, Canada) and ultrapure water (resistivity of 18.2 MΩ cm, Milli-Q system, Millipore, Milford, USA) were used to prepare the reagents and clean all the materials.

A natural uranium solution produced by the CEA Commission for the Establishment of Analytical Methods (CEA-Marcoule/ISEC/DMRC/CETAMA) was selected as the reference solution. The concentration of this solution was 196.21 ± 0.20 g·kg−1 as a result of the Eqrain 15 interlaboratory comparison circuit organized by CETAMA [33]. A fraction of this stock solution was gravimetrically diluted in HNO3 3 M to reach a concentration of 1149.6 ± 1.8 µg·g−1. A certified reference solution for 237Np ([Np] = 1.008 ± 0.006 g·L−1) obtained from the CEA Marcoule/ISEC/DMRC/CETAMA was gravimetrically diluted in HNO3 1 M in order to reach a concentration of 316.2 ± 2.0 ng·g−1. These two diluted solutions, kept under weight control, were used at each analytical session to prepare standard solutions for the calibration curve by Q-ICP-MS and MC-ICP-MS or for the preparation of simulated samples.

From those solutions, a “simulated sample” containing a 100 µg·g−1 solution of uranium with a 237Np/238U ratio of (28.40 ± 0.19) × 10–6 mol·mol−1 was gravimetrically prepared. This ratio was in the range of the 237Np/238U ratios to be determined in the irradiated UO2 pellet samples (see next paragraph). The given uncertainty was the expanded uncertainty (k = 2) obtained by combining uncertainties from the reference solutions and the weights.

For the Q-ICP-MS analysis, a bismuth solution (1000 mg·L−1) in HNO3 2% from (SPEX CertiPrep, Metuchen, USA), certified in content, was used to prepare an internal standard solution to correct the signal drift.

For isotopic dilution measurements (IDMS) of 238U concentration, a 233U spike, called IRMM-040 and certified by the European Commission—Joint Research Centre—Geel, formerly Institute of Reference Materials and Measurements, was used. This certified reference material was gravimetrically diluted at a concentration of 96.50 ± 0.17 µg·g−1 and its isotopic composition was also certified at 233U/U = 98.0430 ± 0.0057%.

UO 2 -irradiated pellet samples

The analyzed samples described in this article were 236U isotope-doped UO2 pellets. They had been irradiated in the 1980’s in the Melusine reactor in CEA Grenoble for experimental purposes. After their irradiation cycle, the pellets have been stored in the COMIR facility (CEA Marcoule) for more than 30 years. Recently, they have been dissolved in hot cells in the Atalante Facility (CEA Marcoule) in 9 M boiling nitric acid for several hours [34] and aliquots of the dissolution solutions were shipped to the LANIE. According to the neutron calculation code, in 2018, the ratio of interest 237Np/238U varied between 10 × 10–6 and 100 × 10–6 mol·mol−1 and the ratio 238Pu/238U was < 2 × 10–6 mol·mol−1, allowing the direct measurement of 238U by MC-ICP-MS without any chemical separation. The neutron calculation indicated also that the 236U/238U ratios varied between 0.001 and 0.015 depending on the studied sample.

Instrumentation and methods

Direct measurement of the 237 Np/ 238 U ratio by MC-ICP-MS

From the U and Np diluted reference solutions described above, Np/U standard solutions were gravimetrically prepared before each experimental session in HNO3 2%. The aimed concentration in 238U was around 200 ng·g−1. For each standard solution, the appropriate amount of neptunium solution was added in order to frame the expected 237Np/238U atomic ratio in the analyzed samples (Table 1).

Table 1 Experimental setup of each analytical session

Aliquots of the UO2 samples were diluted in HNO3 2% to reach a uranium concentration of 200 ng·g−1.

Direct 237Np/238U ratio measurements were carried out on a NEPTUNE Plus MC-ICP-MS (Thermo Scientific, Bremen, Germany). The source of this instrument has been modified to be surrounded by a glovebox in order to handle radioactive samples. The introduction system was composed of a 100 µL·min−1 PFA micronebulizer (Elemental scientific, ESI, USA) and a dual quartz spray chamber arrangement (cyclonic + scott) connected to a PC3 Peltier chiller (Elemental Scientific, ESI, USA). Operating parameters are given in Table 2.

Table 2 ICP-MS parameters during 237Np/238U determinations

The sensitivity and the signal stability were optimized daily on a tune solution containing uranium and were greater or equal to 0.1 V/ppb during all analytical sessions which represent a 238U signal greater or equal to 20 V (for 200 ppb).

Analyses were performed at low mass resolution in static mode. Faraday cups and the central secondary electron multiplier (SEM) equipped with a retarding potential quadrupole (RPQ) were used (Table 3), and such filter reduces the abundance sensitivity by a factor around 100. If needed (i.e., if the SEM had not been used for several months), a cleanup of the SEM was realized by detecting 5 mV of 238U for at least 2 h. Intercalibration gains and baselines for the Faraday cups were electronically determined before each analytical session. The reproducibility of the electronic gains was better than 20 ppm·day−1. The SEM/Faraday cup yield was also determined by measuring a 5 mV 238U signal on the central cup and SEM at the beginning and the end of a session. Even if this yield was not used for calculation, its value should be greater than 80% to ensure that the detector was working in good operating conditions. SEM dark noise was also measured before the analytical sessions and was always found below 0.2 cps.

Table 3 Detector configuration on the MC-ICP-MS

Detector configurations for each analytical step are given in Table 3. As shown in this table, uranium isotopes were determined on Faraday cups and 237Np on the SEM. The cups measuring 234U, 235U and 238U were connected to 1011 Ω and 236U to 1012 Ω amplifiers.

The analytical sequences were composed of consecutive quantifications of blank (HNO3 2%), standard and sample measurements. The blank method contained 1 block of 10 cycles with an integration time of 8 s. The sample (or standard) method was divided into 2 blocks of 10 cycles, each cycle being analyzed with an integration time of 8 s (Table 3).

In order to correct the 237Np/238U raw data, abundance sensitivity measurements were performed at the beginning and the end of the day by establishing the 237/238U ratio in a 200-ppb natural uranium solution. The ion beam at mass 237 was measured on the SEM and the 238U+ ion beam on H1 Faraday cup. The hydride rate was also determined twice in an analytical session by measuring—in the same natural uranium solution—the 238U+ signal on the L1 Faraday cup and the 238UH+ species on the SEM.

For the hydride determination, the amplifier connected to L1 had to be a 1011 Ω amplifier to avoid saturation. The methods contained 10 cycles of measurements with an integration time of 16 s. The cup configurations for abundance sensitivity and hydride methods are given in Table 3. Except for one analytical session where the value is around 1.3 ppm, the abundance sensitivity was established as being below 1 ppm. The abundance sensitivity was systematically higher at the end of the analytical session as the pressure in the analyzer increased during the day but remained quite close to the specifications of the manufacturer (< 1 ppm on the SEM). The hydride rate (ie. Ratio 238UH+/238U+) was around 1 × 10–5—3 × 10–5 (depending on the analytical session) and stayed relatively stable throughout the day. These values were in agreement with the manufacturer’s recommendation (~ 1 × 10–5).

237Np+ raw data were corrected for the blank, the abundance sensitivity (average of the measurements) and the mean hydride rate according the following Eq. (1):

$${}^{237}Np_{corr.}^{ + } = {}^{237}Np_{raw}^{ + } - blk_{237} - \left( {\frac{{{}^{238}UH^{ + } }}{{{}^{238}U^{ + } }}} \right) \times \left( {{}^{236}U_{raw}^{ + } - blk_{236} } \right) - \left( {\frac{237}{{{}^{238}U^{ + } }}} \right) \times \left( {{}^{238}U_{raw}^{ + } - blk_{238} } \right)$$
(1)

Here:

237Np+corr. is the intensity of 237Np+ corrected in cps,

237Np+raw is the intensity of 237Np+ without correction in cps,

blk236, blk237 and blk238 are respectively the intensities at masses 236, 237, and 238 in the HNO3 2% solution in cps,

the \(\left( {\frac{{^{238} UH^{ + } }}{{^{238} U^{ + } }}} \right)\) and the \(\left( {\frac{237}{{^{238} U^{ + } }}} \right)\) ratios are respectively the mean hydride rate and mean abundance sensitivity measured with the 200 ppb U solution at the beginning and at the end of the session,

236U+raw and 238U+raw are respectively the measured intensity of 236U+ and 238U+ converted into cps.

The measured atomic ratio 237Np/238U is given as Eq. (2):

$$\left( {\frac{{^{237} Np}}{{^{238} U}}} \right)_{{{\text{measured}}}} = \left( {\frac{{^{237} Np_{corr.}^{ + } }}{{^{238} U^{ + } - blk_{238} }}} \right)$$
(2)

237 Np/ 238 U determination by Q-ICP-MS and IDMS measurements

In order to validate the new approach proposed in this study, the 237Np/238U ratio of several dissolved spent nuclear fuel samples was quantified by a two-step approach involving the 237Np determination by Q-ICP-MS and the 238U determination by IDMS for cross-comparison. This is the reference method used in the laboratory to characterize the 237Np/238U ratio and it consists in determining the U concentration in the spent fuel using isotopic dilution mass spectrometry associated with thermal ionization mass spectrometry (TIMS) measurements, and in establishing the content of 237Np using an external calibration curve by Q-ICP-MS.

In the present research work, this method was only used on two of the dissolved pellets (with 237Np/238U around 70 × 10–6 and 90 × 10–6 mol·mol−1), and these two samples were indeed analyzed before the direct measurement method was developed. The results obtained at that time were then used to validate the MC-ICP-MS method.

Determining the 238 U concentration by isotope dilution mass spectrometry (IDMS)

According to the simplified isotopic dilution Eq. (3) [35], the 238U concentration in the sample \(C_{{238_{U - Sa} }}\) can be established with knowledge of:

  1. 1.

    The molar mass (MSa) of each sample. They were quantified beforehand by Thermal Ionization Mass Spectrometry (TIMS). As those experiments are beyond the scope of this article, they are not described here but similar experiments can be found in [36] in the case of cerium samples.

  2. 2.

    The ratio (238U/233U)sp, the molar mass (Msp), the isotope abundance in 233U (233U)sp, given in the reference material certificate.

  3. 3.

    The concentration of uranium CU-sp in the spike, calculated with the certificate and the dilution data.

  4. 4.

    The data coming from Spike-sample mixtures as described below.

    $$C_{{^{238} U - Sa}} = C_{U - Sp} \times \frac{{m_{Sp} }}{{m_{Sa} }} \times \frac{{M_{Sa} }}{{M_{Sp} }} \times \left( {^{233} U} \right)_{Sp} \times \left[ {\left( {\frac{{^{238} U}}{{^{233} U}}} \right)_{Blend} - \left( {\frac{{^{238} U}}{{^{233} U}}} \right)_{Sp} } \right]$$
    (3)

For each sample, two IRMM-040 spike-sample mixtures were prepared in a glovebox through weighing (mSp weight of the spike and mSa weight of the sample). The mixtures were then dried on a hot plate.

Chemical separation using a 100–200 mesh AG 1-X4 resin (Biorad, Hercules, CA, USA) was realized on the mixtures in a nitric acid medium in order to separate the uranium from the matrix and interfering elements (protocol described in [37]).

The separated uranium fraction was then diluted in order to reach a concentration of 50 ng·µL−1 in HNO3 2% to be analyzed by Thermal Ionization Mass Spectrometry (TIMS) using the total evaporation technique [38,39,40,41] in order to determine the (238U/233U)blend ratio. A 1µL-droplet of each mixture was then deposited with a pipet on a 99.99% degassed side Re-filament, and the droplet is dried by applying a current though the filament. Filaments were loaded in a nuclearized thermal ionization mass spectrometer Sector 54 from GV Instruments (Manchester, UK) suitable for to handling radioactive samples, as described previously [42, 43].

Determining the 237 Np concentration by a Q-ICP-MS external calibration curve

This method consists in measuring the 237Np content by an external calibration curve.

From the diluted reference material solutions, 6 standard solutions were freshly prepared for each experimental session in HNO3 2%, and each one contained about 2 ng·g−1 of bismuth (internal standard) and a variable concentration of neptunium (from [237Np] = 0 to 2 ng·g−1). Additionally, a CETAMA natural uranium solution of 10 µg·g−1 uranium and 2 ng·g−1 bismuth was prepared (matrix solution) to determine the abundance sensitivity and hydride rate.

Aliquots of each sample were gravimetrically diluted into HNO3 2% and mixed with bismuth solution in order to reach a uranium concentration of 10 µg·g−1 and a bismuth concentration of 2 ng·g−1. The 237Np concentration was then established on those dilutions.

A quadrupole Inductively Coupled Plasma Mass spectrometer (ICP-MS) ‘‘X series’’ from Thermo Electron (Winsford, UK) was used for these measurements. The source of this instrument had been modified and was surrounded by a glovebox to handle radioactive samples as previously described in [44, 45]. Sample introduction in the plasma was realized via a quartz cyclonic spray chamber connected to a PC3 Peltier chiller (Elemental Scientific, ESI, USA) and a quartz concentric nebulizer (400 µL·min−1). Operating parameters are given in Table 2. Tuning and calibration of the instrument were performed before each analytical session using a multi-elemental solution containing indium and uranium at concentrations of about 1 ppb in order to obtain a stability better than 2% on the ion beams and a sensitivity in the range of 300,000 cps and 500,000 cps. Oxides and the doubly-charged species rate were kept as low as possible (respectively 140Ce16O+/140Ce+ < 3% and 138Ba2+/138Ba+  < 3%).

Q-ICP-MS makes it possible to determine of 209Bi, 237Np, 234U, 235U and 236U in each standard solution. Due to the high concentration of the 238U isotope in the solutions, it was not measured to avoid any risk of detector saturation. A dwell time of 40 ms/analyte was selected and 200 sweeps were realized in each run. For the standards and samples, 10 runs per analysis were performed. As less precision was required for the blank (HNO3 2%) and for the matrix solution, only 3 and 5 runs were performed, respectively.

The analytical sequence consisted in analyzing HNO3 2% (blank), standard solutions and samples. The natural uranium solution with a concentration of 10 µg·g−1 was also examined at the beginning, in the middle and at the end of the analytical session in order to establish the hydride rate measured at masses 239 (238UH+) and the calculated 238U+ ion beam intensity derived from the 234U+ ion beam intensity and isotopic composition. This estimation of the 238U+ ion beam was necessary, as the 238U+ ion beam was too high to be directly measured. The abundance sensitivity of the instrument was quantified with masses 237 and estimated 238U+ ion beam intensity. During the various analytical sessions, the abundance sensitivity was between 1.9 and 3 ppm and the hydride rate between 8 × 10–5 and 1.2 × 10–4.

Results and discussion

The results for the samples (UO2 pellets solution and simulated sample) were obtained during four different analytical sessions. The 237Np/238U ratio of each standard solution and the analyzed samples during those analytical runs are given in Table 1. As already mentioned above, standards had been prepared in order to bracket the samples to be analyzed in the session. Generally, except for the first session where a higher range of standards was analyzed, standards with a 237Np/238U ratio between 0 and 100 × 10–6 mol·mol−1 were used. For each measurement (standards and samples), the 237Np signal intensity was corrected according to Eq. (1) and the (237Np/238U)measured was determined using Eq. (2). The corrections due to hydride rate (236UH+) and the abundance sensitivity represent respectively a number of counts per second < 350 cps and between 600 and 2300 cps depending on the analytical conditions. The hydride rate contribution is at least twice lower than the abundance sensitivity contribution, this latest being the most important correction. The contribution of the hydride correction to the total signal on mass 237 amu is < 0.5%; the contribution of the abundance sensitivity is < 5% depending on the conditions.

In each analytical session, for the standards, a calibration curve of the “reference” 237Np/238U ratios (calculated with weight and certificates) versus the experimentally obtained ratios was plotted. An example of such a calibration curve is given in Fig. 1. A linear regression model was used and the slope (a) and intercept (b) of the regression line were determined for each analytical session according to the model. Table 4 gives the values obtained for each parameter (a) and (b). As shown in the table, in each analytical session, the coefficient of determination was R2 > 0.9999 demonstrating a good correlation between the measured and reference values using a linear model.

Fig. 1
figure 1

Plot representing an example of a calibration curve used during this study. The 237Np/238U calculated using the dilution weight and the certificates is plotted versus the measured 237Np/238U ratio. The dots are the results of the standard measurements, and the dashed line is the linear regression model used to determine the 237Np/238U ratio in the sample

Table 4 Parameters of each linear regression for the four calibration curves determined during the study

Validation of direct measurements by MC-ICP-MS

The validation of the method was done in two steps, by measuring:

  1. 1.

    the gravimetrically prepared “simulated sample” on the Neptune Plus and comparing it with the 237Np/238U ratio derived from certificates and weight (Fig. 2),

  2. 2.

    two samples (237Np/238U ≈ 70 × 10–6 mol·mol−1 and 237Np/238U ≈ 90 × 10–6 mol·mol.−1), with both the new MC-ICP-MS direct method and the classical “IDMS + Q-ICP-MS” approach (Fig. 3)

Fig. 2
figure 2

Results obtained by MC-ICP-MS of the 237Np/238U ratio for a “simulated solution”: the black line represents the reference value derived from certificates and weight. The dashed line corresponds to the uncertainties (k = 2) of the reference value. The triangles are the results obtained during the 1st analytical session and the circles are the results from the 2nd session. The error bars represent the expanded uncertainties (k = 2) of the measurements using the model given in Eq. 4

Fig. 3
figure 3

Comparison between the classical “Q-ICP-MS + IDMS” method (squares) and the new method by MC-ICP-MS (black dots) for two samples (around 70 × 10–6 and 90 × 10–6 mol·mol.−1). The indicated values are the bias compared to the classical method. The represented expanded uncertainties are given with a coverage factor of 2

Concerning the simulated sample, as observed in Fig. 2, the relative difference between the value measured with the MC-ICP-MS and the reference value obtained by weighing was around 0.2% for the 1st analytical session and 0.4% for the second. The experimental values were within the expanded uncertainties of the reference value (0.64%), and the method could therefore be validated for the 30 × 10–6 mol·mol−1 reference solution. It should be noted that the represented expanded measurement uncertainties (k = 2) were those found when following the model that will be discussed in the next paragraph.

Similarly, Fig. 3 represents a comparison of the results obtained with the classical method and direct measurements on MC-ICP-MS for two dissolved pellet samples with 237Np/238U ratios around 70 × 10–6 and 90 × 10–6 mol·mol−1. As the “Q-ICP-MS + IDMS” approach was the reference method, results are indicated with a bias of 0% (square on the figure). For those two values, the expanded uncertainties (k = 2) were the combination of the standard uncertainties originating from the IDMS method (around 0.2%) for 238U determination and the reproducibility from several 237Np determinations (around 1.5% -1.75%, k = 1). For the direct measurements, differences of 0.8% and 0.65% were observed between the reference method (dot on the figure) and the new MC-ICP-MS direct approach. The expanded uncertainties of the MC-ICP-MS method calculated according to the model that will be described in the next paragraph were respectively 0.95% and 0.87% (k = 2). At that point, an important advantage of the newly developed method could already be noticed: the uncertainties were three times below those determined by Q-ICP-MS + IDMS. The observed bias was insignificant within the uncertainties wherefore these two sets of experiments proved that the new method was validated.

Results and uncertainty assessment

Pellet samples were analyzed in different analytical sessions (see Table 1) and Table 5 gives the results for each sample. The indicated values are averages of several measurements. Absolute and relative combined expanded uncertainties are also listed with a coverage factor of 2 and the indicated relative expanded uncertainties are defined as the maximum of the individual uncertainties. For each measurement, the standard uncertainties were combined used the following model (Eq. 4):

$$u_{rel} = \sqrt {u_{rel, reg}^{2} + u_{rel, MRC}^{2} + u_{rel,meas}^{2} + u_{rel,lt}^{2} }$$
(4)
Table 5 Results obtained on dissolved UO2 pellets

Here:

urel, MRC is the uncertainty of the reference U-Np mixtures (urel, MRC = 0.32%).

urel, meas is the relative standard deviation of the measured 237Np/238U ratio of the sample. This contribution varied between 0.1% and 0.3% depending on the day and the analytical conditions.

urel, reg is the uncertainty of the linear regression. This uncertainty was determined via excel by calculating the impact of the slope and intercept uncertainties on the 237Np/238U ratio. It depended on the value of 237Np/238U and on the conditions of the analytical session. In Fig. 4, urel, reg is plotted versus the 237Np/238U ratio, and as can be seen the relative uncertainty decreased when the ratio increased. Moreover, it was clear that this uncertainty was dependent on the analytical session. It varied between 0.04% and 0.72%.

Fig. 4
figure 4

The standard uncertainty (k = 1) for the linear regression versus the 237Np/238U ratio for the different analytical sessions

urel,lt is an uncertainty parameter linked to the reproducibility between different analytical sessions. Some measurements were performed on different dates, and the standard deviation between the various measurements is plotted in Fig. 5. As observed on this graph, the standard deviation did not exceed 0.2. This absolute value was converted into a relative contribution and added to the uncertainties.

Fig. 5
figure 5

Plot representing the u(lt)abs contribution (k = 1) versus the 237Np/238U ratio. The black line represents the value 0.2

By combining these contributions using Eq. 4, a relative expanded uncertainty (k = 2) varying between 0.81% for the samples with the highest 237Np/238U ratio and 2.75% for the samples with the lowest 237Np/238U ration was calculated (Table 5). These values were globally equivalent to or lower than the expanded uncertainties obtained with the usual method which were generally around 2–4%. Figure 6 presents two examples of uncertainty budgets: one with the budget of the lowest 237Np/238U ratio (around 10 × 10–6 mol·mol−1) and one with the highest (around 100 × 10–6 mol·mol−1). The uncertainty budget was quite different for the 2 examples. For the higher 237Np/238U-sample, the biggest contribution to the uncertainty (i.e., up to 65% to the final value) was that of the U-Np reference mixtures and the second main contributor was the parameter called ult which represented around 25—30% of the contribution. This tendency changed for the lowest ratios, for which the main contribution became the parameter linked to measuring the external reproducibility (ult) (more than 60%), followed by the uncertainty of linear regressions. Regardless of the 237Np/238U, the uncertainty originating from the measurement itself brought the smallest contribution.

Fig. 6
figure 6

Uncertainty budget on two samples: one with 237Np/238U = 10 × 10–6 mol·mol−1 and one with 237Np/238U = 100 × 10–6 mol·mol−1

Conclusion

A new method to directly measure the 237Np/238U atomic ratio has been successfully developed and applied on real irradiated samples in which the amount of 238Pu was negligible. The method made it possible to measure low 237Np/238U ratios (around 10 × 10–6 mol·mol−1), which could not be quantified by the conventional laboratory approach. This described method did not require prior chemical separation steps and used a MC-ICP-MS equipped with Faraday cups and an ion counter detector. It was achievable to measure samples with a 237Np/238U ratio varying from 10 × 10–6 mol·mol−1 to 100 × 10–6 mol·mol−1. The method was validated by carrying out measurements of a simulated solution and by comparing the obtained results on two real samples with the more commonly used technique “Q-ICP-MS + IDMS”.

The described approach displayed multiple advantages:

  1. 1.

    Analytically, since the RPQ improved the abundance sensitivity, this direct method allowed measurements of atomic ratios close to 10 × 10–6 mol·mol−1 which would not be possible with the commonly used technique.

  2. 2.

    It suppresses the chemical separation step, reducing the number of steps in the glovebox and also the duration of radiation exposure for the analysts.

  3. 3.

    Knowledge of the isotope composition of uranium is not required for such measurements.

  4. 4.

    The relative expanded uncertainties obtained were between 2.75% and 0.81% for an elemental ratio varying between 10 × 10–6 mol·mol−1 and 100 × 10–6 mol·mol−1 which was lower than or equivalent to the uncertainties obtained by the commonly used technique.