Open Access Article
Daniel
Lauriola
*,
Michael
Savina
,
Manuel
Raiwa
,
Whitney
Harmon
and
Brett
Isselhardt
Lawrence Livermore National Laboratory, Nuclear and Chemical Sciences Division, 7000 East Ave, Livermore, CA 94551, USA. E-mail: lauriola1@llnl.gov
First published on 21st October 2025
Resonance ionization mass spectrometry of gadolinium can be used for nuclear forensics and to further the understanding of stellar nucleosynthesis but has been used only a handful of times due to the high laser power required and interference from non-resonant ionization of molecules of other elements. Herein we present the development of two novel resonance ionization spectroscopy schemes for gadolinium that provide improvements in isotopic fractionation and ionization efficiency, respectively, opening new applications for gadolinium analysis. The schemes are demonstrated and compared in a mixed sample of gadolinium and neodymium.
Gadolinium (Gd) is of particular interest in nuclear forensics and presolar grain analysis due to its large neutron capture cross-section. Knowing the isotope ratios of Gd in extrasolar material such as stardust grains would increase our understanding of nucleosynthesis reactions in stars.24 Determining trace concentrations of Gd is also essential in medicine for MRI contrast and targeted radiotherapy applications.25–28
However, only two resonance ionization schemes for Gd RIMS have been reported to date.3,29 The first employs a three-laser scheme from a high-lying metastable state in the ground manifold (J = 6, E = 1
719 cm−1), populated at less than 10% below 1400 K,29 limiting the measurement effectiveness to higher temperatures.30 The second uses two colors and starts from the Gd ground state and has been successfully applied to clean samples.3 Its use in complex materials is limited by the high fluences required to saturate the two-step process. Furthermore, the first transition of this scheme exhibits a large isotope shift, complicating the simultaneous measurement and comparison of all Gd isotopes and rendering the analysis sensitive to minor laser wavelength fluctuations. To overcome this, either the laser bandwidth needs to be broadened, leading to higher total fluence to maintain saturation, and increased oxide interferences, or a large correction factor could be applied for each isotope, lowering the accuracy, particularly in low concentration measurements, where RIMS is commonly used.
To address these limitations, we have developed and characterized two new ionization schemes for Gd RIMS, both using transitions from the J = 3, E = 215 cm−1 low-lying metastable state. We investigated a one-color, two-step pathway and a two-color scheme. The one-color scheme shows minimal isotope shifts but requires higher fluence, while the two-color scheme saturates at lower fluence and suppresses oxide interference more effectively. Here, we detail the characterization of these schemes, including isotope shifts, saturation fluences, and fractionation, and benchmark them on a mixed Gd/Nd sample to demonstrate improved performance in complex matrices.
:
Sa) lasers can be coupled into the chamber through optical windows, to ionize the atoms of interest using multi-step ionization. A time-of-flight mass spectrometer determines the mass and counts of the ions produced by the laser interaction. For these specific experiments, Gd (and later Gd/Nd) was vaporized using a 1064 nm Nd:YVO4 desorption laser running at 1.5 kHz. Each ∼10 ns pulse is focused to ∼75 μm and desorbs sub-monolayer quantities of material from the sample surface, shortly thereafter a high voltage pulse is applied to eject secondary ions produced by the desorption event. One microsecond later the multi-photon ionization laser pulses interact with the gas-phase Gd atoms in a ∼1 mm2 × ∼3 mm long section to selectively ionize them. A 3 kV pulse then pushes the newly formed ions through a reflectron time-of-flight mass spectrometer, throughout which focusing and collimating optics direct them to the detector.
:
sapphire lasers were tuned to relevant wavelengths, and frequency doubled by LBO crystals to output ∼15–20 ns, 0.1–0.5 mJ UV/visible pulses. We used four different lasers so that we could directly compare ionization schemes in real time. Two of the lasers were tuned to the reference scheme (Fig. 1) and run at a repetition rate of 750 Hz. The other two were pumped at 1500 Hz, with intra-cavity Q-switches to suppress every other pulse such that the Ti
:
Sa lasers operated at 750 Hz. Data was collected at 1500 Hz with the schemes interleaved such that the reference scheme was active during odd desorption laser shots and one of the new schemes shown in Fig. 1 was active during even shots. This makes it possible to benchmark to the reference pathway at every other pulse. The fundamental wavelength of each Ti
:
Sa was stabilized to within ±1.5 picometers using a closed feedback loop consisting of a wavemeter (WS6, High Finesse) and a piezo acting on the intracavity diffraction grating, with a 15 second update rate.
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| Fig. 1 Reference ionization pathway used (left) and newly developed schemes from the low-lying metastable state (center and right). | ||
:
50 Gd/Nd by weight.
Before performing the measurements, the samples were imaged in situ using a microscope objective with ∼5 μm resolution. The desorption laser was aligned to a uniform, particle free, area near the center of the dried droplet. The desorption laser was focused to ∼75 μm to average out the effect of any possible μm sized particles or non-uniformities, not visible in the microscope images. The stage was moved to a new location whenever too much of the sample was depleted.
For wavelength scans of the reference scheme (Fig. 2a), a different method was used, since there was no other pathway to compare to. Here a single scheme was used with the Ti
:
Sa lasers running at 1.5 kHz. An intracavity electro-optic deflector was placed in the first excitation step laser and used to deflect the beam hitting the grating to induce a small change in wavelength. The deflector was pulsed at 750 Hz, such that every other shot was at a fixed wavelength corresponding to the center of the excitation line while the application of varying voltages resulted in different wavelengths for the other shots. This allowed for changing the laser wavelength without energy or pointing variations. This enabled referencing, every other pulse, to the peak of the excitation line (no voltage applied) using the same ionization scheme, without requiring the use of two separate sets of lasers.
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| Fig. 2 Wavelength scans for (a) the 1st step of the reference two-color scheme and (b) the developed one-color scheme. | ||
Transitions from the J = 5 metastable state (999 cm−1) were experimentally tested as well but are not presented here, as their ionization efficiency was approximately ten times lower; in line with an expected thermal population below ∼10% at the estimated 700 K sample temperature.
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| Fig. 3 Normalized saturation curve of the one-color scheme, and of the 2nd step of the reference scheme. | ||
849.514 cm−1 (vacuum λ = 405.937 nm) as shown in Fig. 1 schematic. The second step, using the same laser wavelength, falls ∼117 cm−1 below the ionization potential. (The electric field gradient in the LION instrument lowers the effective ionization potential of atoms by ∼140 cm−1.) Since it was not tabulated in literature and it is at a lower energy than experimental Rydberg scans performed by others,34,35 we have not assigned it to any known transition. Wavelength scans for both the reference 2-color scheme, and the new 1-color transition are shown in Fig. 2. The reference scheme isotope shift is ∼1 GHz per atomic mass unit. In the 1-color scheme the width of the peak scanned is nearly three times broader than the reference scheme. The isotope shifts are difficult to quantify due to the broad peak and the nearly perfect overlap in signal between different isotopes (Fig. 2b). Nevertheless, the 154Gd–160Gd shift is less than 0.75 GHz. Having an isotope shift that is >10× lower than the laser linewidth means that the isotopic ratios are less affected by changes in the laser wavelength and linewidth, which is ideal for isotopic analysis.
To determine the energy required to saturate the 1-color transition we adjusted the laser power with a half-wave plate/Glan laser polarizer combination. The maximum fluence for the 1-color pathway was 80 mJ cm−2. Fitting the data in Fig. 3 was performed using a standard saturation fitting function36 shown in eqn (1):
![]() | (1) |
For this transition we obtained a value of 40 (±7.2) mJ cm−2, which is more than double the combined 17.5 mJ cm−2 saturation fluence of the reference scheme (0.4 mJ cm−2 for the first excited step, 17.1 mJ cm−2 for the 2nd excited step).
This new pathway has the advantages of a nearly absent isotope shift, which is beneficial for isotopic analysis, and requires only one laser. The drawback is that a high fluence is required, potentially increasing interference from non-resonant or quasi-resonant ionization molecules such as oxides in mixed samples.
To better understand why this ionization pathway requires such a high fluence, when the first excited level is a known resonant transition, we set out to characterize the second step transition.
We deployed a second laser at the same wavelength. We set the first laser to a fluence of 1.175 mJ cm−2 which yielded no Gd ionization but was enough to populate the 1st excited state. The second laser was then set to 6.4 mJ cm−2 and scanned over a range of more than 1 nm. The resulting scan, in Fig. 4, uncovered that the second photon of the one-color transition is only weakly coupled to the continuum, and multiple neighboring transitions to second excited states are much more efficient than that of the one-color scheme.
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| Fig. 4 Normalized wavelength scan of the second step laser to search for other upper state levels. The 1-color transition wavelength is shown by the blue vertical line. | ||
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| Fig. 5 (a) First and second excited state wavelength scans to determine the isotope shifts; (b) saturation curves for the first and second excited state levels. | ||
These results show that both transitions have a significant isotope shift, in opposite directions. The first step has ∼1.2 GHz per amu for the even isotopes, and the second step shift is ∼−0.8 GHz per amu in the other direction. Since the isotope shifts are opposite, and the lasers linewidths are broad, we found that in our experiments, using saturated laser fluences, setting the 1st and 2nd excited state lasers to 405.937 nm and 405.611 nm, respectively, resulted in an isotope fractionation of <5%. This is explained by a higher excitation probability of the heavier isotopes in the first transition, followed by a higher excitation probability of the lighter ones in the second transition, due to the opposite shift. Since the shifts are not identical and opposite, and there is more structure in the second excited state, we don't expect an exact compensation of the two, as is reflected by the residual non-zero fractionation in Fig. 6.
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| Fig. 6 Isotope fractionation compared to the natural abundance of Gd for the schemes used. Results are obtained from measurements above the saturation fluence. | ||
We scanned the laser energy for both transitions and fit the curves using the fitting function defined by eqn (1). The results in Fig. 5b show that both steps saturate at very low fluences. The first shows a saturation fluence of 0.29 mJ cm−2. The second step saturates at ∼6 mJ cm−2, 3 times lower than the reference scheme (17.1 mJ cm−2 saturation).
| Reference | 1-Color | 2-Color | |
|---|---|---|---|
| Step 1 (nm) | 432.832 | 405.933 | 405.937 |
| Step 2 (nm) | 378.78 | 405.611 | |
| Sat 1 (mJ cm−2) | 0.5 | 40 | 0.29 |
| Sat 2 (mJ cm−2) | 17.5 | 5.94 | |
| Relative signal | 1 | 0.6 | 1.5 |
| Isotope shift (GHz per amu) | 1; N/A | <0.1 | +1.2;-0.8 |
Comparing these schemes we find that the main advantage of the 1-color scheme is the broad excitation peak and near absence of isotope shifts, making it more insensitive to variations in laser linewidth and power; while a high fluence is required to saturate the transition, since the second step does not appear to be coupled to a strongly resonant level. The new two-color scheme has similar isotope shifts as the reference scheme, but the saturation energy is ∼3 times lower, placing it at a strong advantage for mixed samples.
Additional measurements of the isotope fractions (Fig. 6) showed that the reference two-color scheme favors the odd isotopes over the even ones due to selection rules and shows more fractionation of 154Gd due to a narrower linewidth. The new schemes both have much lower fractionation than the reference scheme, which is nearly 20%. The 1-color scheme presents a maximal change from natural of 7% for 154Gd but is the closest to natural composition overall. The 2-color scheme differs by <5% for 154G but does show more variation in the ratio between even and odd isotopes. Lower fractionation can improve sensitivity by requiring a smaller correction when using a standard in measurements. Use of standard-sample-standard bracketing can correct for similar amount of fractionation, and is used in all mass spectrometry measurements, including RIMS.
To evaluate the selectivity of each pathway on a complex sample, we performed experiments on a sample with 1000 ppm of Gd and 1000 ppm of Nd. Fig. 7 shows two mass spectra taken in the previously described interleaving mode over a 5 minute-long acquisition. There are no interfering molecules from mass 154 to 157 and the Gd signals are comparable for both schemes, however the signals above mass 158 are significantly different due to NdO interference. The Gd-free peaks at 159 amu and 161 amu can be used as a direct comparison for the number of interfering oxides ionized. Higher interference of NdO within the Gd peaks increases the difficulty in obtaining isotopic ratios. Some corrections can be made, and an interleaved blinking scheme to compare off-resonance spectra and subtract the oxide counts, could be applied, but the uncertainty would still be increased. This solution would be especially challenging if counts per run are extremely low, and where 158Gd and 160Gd, due to their higher natural abundance, may be the only isotopes well above the detection limit.
As in the previous experiments, the new pathways were compared to the reference 2-color scheme which was interleaved at each shot. We set the reference scheme first and second excited step fluences to 1.17 mJ cm−2 and 87 mJ cm−2 respectively to ensure complete saturation and varied the 1-color and two-color scheme fluences to study the effect on signal and oxide interference. The fluence of the first step of the newly developed 2-color scheme was fixed at 1.5 mJ cm−2, far above its 0.3 mJ cm−2 saturation value.
We used 156Gd to compare the signal at different fluences as it is the most abundant interference-free isotope. The ratio of the integrated areas of 156Gd of the new schemes to the reference is shown on the right axis in Fig. 8. On the left axis we plotted the signal to oxide ratio at the 158Gd peak, for the new schemes; this is obtained by first calculating the expected 158Gd signal from the 154Gd to 157Gd peaks and the known isotopic ratio obtained from the pure Gd sample. The remaining signal, after subtracting 158Gd, is assigned to 142NdO. The highest 158Gd/142NdO ratio is 1.53 using the new two-color scheme at 7 mJ cm−2; compared to a ratio of 0.15 (red dotted line) for the reference scheme at the high 87 mJ cm−2 fluence.
The results in Fig. 8 show that in terms of oxide interference the one-color scheme performs worse than the reference 2-color scheme. At the highest fluence the signal is 0.6 times that of the reference, and the Gd/NdO ratio is also 20% lower than the reference scheme. The newly developed 2-color scheme is much better; at the highest fluence the signal is 1.3 times higher, and the Gd/NdO ratio is 1.8 times better than the reference. At 7 mJ cm−2 where the signal is nearly comparable to the reference (∼17% less) the oxide interference is suppressed by a factor of ∼14.5, providing a significant advantage in mixed sample measurements. If performing measurements far above saturation is essential, running at ∼20–25 mJ cm−2 would result in similar efficiencies to the reference scheme, while reducing the oxide interference by a factor of ∼5–8.
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| Fig. 9 Calculated population distribution of the levels in the ground state manifold of gadolinium as a function of temperatures. | ||
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