Abstract
Decay energy spectroscopy (DES) is an increasingly popular technique for measuring isotopic composition of actinide samples for nuclear safeguards applications. Current approaches for actinide DES utilize milligram-scale external gold absorbers (> 0.1 nJ/K) that are integrated with actinide samples through mechanical kneading and are thermally connected to microcalorimeters using indium or gold wire bonds. This leads to relatively slow sensor rise time and, consequently, limits counting speed to a few counts per second. We are developing faster metallic magnetic calorimeter-based DES by integrating actinide samples with magnetic sensor materials. This reduces signal rise time and enables high counting speed while maintaining the ability to knead the radioactive source with the absorber. We have measured signal rise time of 0.7 μs with a 1.5 mg external gold absorber using this approach. We also demonstrated online DES operation using an Ortec DSPEC 50, a commercially available data acquisition system developed for semiconductor detectors.
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1 Introduction
Accurate analysis of nuclear material composition is critical for nuclear safeguards. The current state-of-the-art method for analyzing nuclear samples is a combination of thermal-ionization mass spectrometry (TIMS) and alpha spectroscopy [1]. While this technique is precise, development of an independent analysis method is highly desired to improve reliability of nuclear material accountancy [2]. Decay energy spectroscopy (DES) is a promising, complementary technique for measuring nuclear material composition that identifies and quantifies radioactive nuclides by measuring temperature increase resulting from radioactive decay [3]. Nuclear samples are encapsulated by a gold foil (referred to as the absorber), mechanically kneaded with the absorber, then thermally connected to a microcalorimeter sensor, such as a metallic magnetic calorimeter (MMC) or transition-edge sensor (TES) [4, 5].
Actinide DES for nuclear safeguards applications has several important considerations. First, a relatively large mass of radioactive material needs to be analyzed due to their long half-lives. For example, U-238 has a half-life and specific activity of 4.5 billion years and 12,400 decays per second per gram, respectively. Hence, isotopic analysis of a typical uranium nuclear safeguards sample requires 100 s of micrograms to be analyzed if a result is desired within the several hours available in a single magnetization cycle of an adiabatic demagnetization refrigerator. Consequently, large absorbers must be used to encapsulate the sample. Second, the absorbers are typically mounted separate from and externally coupled to the microcalorimeter. This allows samples to be routinely replaced by technicians while the microcalorimeter remains in the experimental setup. Various ways of sample attachment have been developed that provide both high-energy resolution and simple, repeatable sample attachment [6,7,8]. Third, actinides should be completely encapsulated by and mechanically kneaded into absorber foils to improve energy resolution [7]. Figure 1 shows our standard MMC-based DES implementation in which gold wire bonds are used to attach the absorber to the MMC. 10 to 90% signal rise time was limited to order 100 μs at 20 mK, which is consistent with previous reports [6]. While this rise time is sufficient for low-activity samples, both nuclear safeguards and forensics applications can greatly benefit from the ability to process higher count-rate samples. Examples include quicker isotopic ratio determination, reduction of uncertainties due to counting statistics, and the ability to process samples containing high-activity nuclear fission products.
We are developing new approaches for routine actinide DES that significantly improve counting speed over current implementations. Absorbers are integrated with paramagnetic sensors to improve thermal coupling. We present two techniques for improving MMC speed and compare them to our standard approach.
2 MMC-based DES Configurations
2.1 Method 1
This configuration mechanically presses the gold absorber against the Au:Er or Ag:Er sputtered paramagnetic sensor. This pressure contact thermally connects the absorber to the MMC via conduction electrons by Wiedemann–Franz law [9]; thus, boundary thermal resistance can be minimal and fast signal readout can be achieved. A clamp provides the force needed for the pressure contact, as shown in Fig. 2. Challenges include unknown thermal conductance of the mechanical contact at low temperatures and risk of cross contaminating the MMC surface by improperly encapsulated actinide samples.
2.2 Method 2
This technique laminates the absorber with a paramagnetic foil using a roll mill. Next, the laminated package is placed directly onto an MMC superconducting pickup coil that has no sputtered paramagnet layer, as shown in Fig. 3. This provides better integration of the absorber to the paramagnetic sensor and fast sensor response time [10]. Challenges to this method include synthesizing magnetic foils free of magnetic contamination and inconsistent paramagnet-pickup coil coupling due to non-negligible gaps between the sensor and pickup coil.
3 Results
Figure 4 shows a comparison of signals measured from three DES configurations: wire bond, Method 1, and Method 2. As shown in Table 1, Method 1 resulted in greater than an order of magnitude reduction in signal rise time when compared to our wire-bond technique. This result was reproducible in multiple experiments. Rise time associated with Method 2 was nearly an order of magnitude shorter than that of Method 1. To first order, signal decay time is a function of thermal conductance between the absorber and thermal bath, which differed for each pulse shown in Fig. 4. Future studies will work to decrease decay time and make heat sinking more consistent.
The Method 2 configuration results in sub-microsecond signal rise time, which is similar to that of large-volume high-purity germanium (HPGe) semiconductor gamma-ray detectors. This enables use of commercial-off-the-shelf (COTS) data acquisition systems for pulse processing with trapezoidal filtering [11]. Trapezoidal filtering is preferred for fast counting experiments due to its short signal integration time, fewer pileup events, and consequently, less detector dead time when compared to Weiner optimal filtering [12]. A preliminary implementation of the Method 2 MMC configuration exposed an external Gd-148 alpha-emitting source to a paramagnetic foil mounted upon a bare MMC pickup coil [10]. Data from this experiment were filtered using three methods to the produce pulse-height spectra shown in Fig. 5. Histograms shown in light gray and dark gray were generated by offline processing of raw, triggered pulses, and utilized Weiner optimal and trapezoidal filtering techniques, respectively. Offline trapezoidal shaping rise and flat-top times were 20 and 1 microseconds, respectively. Data shown in black correspond to online pulse processing using a DSPEC 50 HPGe digital signal processing unit. Rise and flat-top times for online analysis were 14 and 1 microsecond, respectively. Weiner optimal filtering resulted in a full width at half-maximum (FWHM) energy resolution of 16.4 keV. Offline trapezoidal filtering and DSPEC 50 energy resolution were 24.1 and 26.6 keV, respectively. As expected, DSPEC 50 and offline trapezoidal filtering resulted in similar energy resolution.
4 Conclusion and Discussion
We have demonstrated two methods for decreasing signal rise time in DES MMCs. Direct clamping of the actinide absorber to the MMC sputtered paramagnet produced a signal rise time of ~ 6 microseconds, while integrating the actinide absorber directly with a paramagnetic foil resulted in a 0.7-microsecond rise time. Signal throughput is fundamentally limited by rise time because decay time can be adjusted, though it cannot be faster than the rise time. Hence the techniques presented in this work indicate that signal throughput can be increased by over an order of magnitude when compared to our current MMC-based DES implementation. The result is directly applicable and beneficial to both nuclear safeguards and forensics. Additionally, faster MMC response time benefits pulse-shape discrimination efforts associated with the MAGNETO-DM dark matter experiment and can mitigate pulse-pileup effects that distort the high-statistics beta-decay spectrum measured in the MAGNETO- υ sterile neutrino experiment [13, 14].
Future work will include shortening signal decay time, as this parameter must also be decreased to enable analysis of high-activity samples. Temperature stability and energy resolution will be improved to enable plutonium isotopic analysis. Lastly, use of COTS digital acquisition systems will continue to be explored, as this capability makes MMC-based DES more user-friendly.
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Acknowledgements
This work was performed under the auspices of the US Department of Energy by Lawrence Livermore National Laboratory under contract DEAC52-07NA27344. Lawrence Livermore National Security, LLC. The work presented in this paper was funded by the National Nuclear Security Administration of the Department of Energy, Office of International Nuclear Safeguards, the US Department of State, Bureau of International Security and Nonproliferation, Laboratory Directed Research and Development program of Lawrence Livermore National Laboratory (23-LW-043), and DOE Office of Science HEP Advanced Detector R&D program. LLNL-JRNL-855959
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N. H. wrote the main manuscript, conducted the experiments discussed in the text, and performed data analysis shown in Fig. 4. G. K. is the principal investigator for this project. He guided experimental efforts, performed data analysis for Fig. 5, and provided background and context for the manuscript. S. B. performed proof-of-concept calculations and simulations for this work and provided guidance for experiments. He also assisted in interpretating data measured in this work. All authors reviewed the manuscript.
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Hines, N., Boyd, S.T.P. & Kim, GB. Progress Toward Fast Decay Energy Spectroscopy for Actinide Analysis. J Low Temp Phys 216, 285–291 (2024). https://doi.org/10.1007/s10909-024-03132-y
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DOI: https://doi.org/10.1007/s10909-024-03132-y