The nEXO Radioassay Program
Pith reviewed 2026-05-10 09:48 UTC · model grok-4.3
The pith
The nEXO radioassay program provides some of the most restrictive constraints on natural radioactivity in materials.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
A compilation of radioassay data on numerous materials achieves some of the most restrictive constraints on their natural radioactivity content, supporting the design of the nEXO detector and similar experiments.
What carries the argument
The radioassay program using multiple measurement techniques to quantify trace radioactivity levels in candidate materials.
If this is right
- Experiments can select materials based on these limits to achieve lower backgrounds.
- Reduces duplication of radioassay work across the rare-event search community.
- Supports the sensitivity goals of the nEXO neutrinoless double-beta decay search.
- Provides a reference for future material screening programs.
Where Pith is reading between the lines
- The results may inform material choices in other fields requiring ultra-low radioactivity, such as quantum sensors.
- Independent verification of these limits on production materials would strengthen their utility.
- Extension to additional material types or isotopes could further expand the resource.
Load-bearing premise
The reported assay results accurately represent the radioactivity levels in the materials to be used without systematic biases or contamination.
What would settle it
An independent measurement finding radioactivity levels substantially higher than the upper limits reported here.
Figures
read the original abstract
Material radioactivity compilations, such as the one presented here, are important enablers of science. They are useful for the selection of radiopure materials used in the design and construction of low-energy rare-event search experiments. They allow researchers developing such experiments to save time on material studies and avoid costly duplication of effort. The data presented here were generated in support of the planned nEXO double-beta decay search. This work contains among the most restrictive constraints on the natural radioactivity content of materials of general interest to the low-radioactivity community, found in any tabulation of this kind. In this study, various techniques were employed; they are described here.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript compiles radioassay results obtained via multiple standard techniques (ICP-MS, gamma spectroscopy, and others) for a range of materials under consideration for the nEXO double-beta decay detector. It tabulates upper limits on natural radioactivity (primarily U/Th/K chains) and asserts that these limits are among the most restrictive available in the low-radioactivity literature.
Significance. If the reported limits hold, the compilation provides a practical resource that can reduce redundant assay work for other low-background experiments. The multi-technique data set strengthens the credibility of the constraints for material selection in rare-event searches.
minor comments (3)
- [Abstract] The abstract states that 'various techniques were employed' but does not enumerate them or indicate how many materials were assayed; adding a short list would improve immediate clarity for readers.
- [Results tables] Tables presenting the final limits should include a column or footnote that explicitly shows the dominant systematic uncertainty for each entry (e.g., calibration, efficiency, or background subtraction) so that the quoted upper bounds can be evaluated without consulting the full methods text.
- [Introduction] The manuscript references prior radioassay compilations only in passing; a brief comparison table or paragraph quantifying how many of the new limits improve on the best previous values would strengthen the claim of providing 'among the most restrictive constraints.'
Simulated Author's Rebuttal
We thank the referee for the positive summary and recommendation of minor revision. No specific major comments were provided in the report, so we have no points to address individually. The manuscript compiles radioassay data supporting nEXO and similar experiments; we stand by the presented limits and multi-technique approach as described.
Circularity Check
No significant circularity
full rationale
The paper is a direct experimental compilation of radioassay measurements (ICP-MS, gamma spectroscopy, etc.) reporting upper limits on natural radioactivity in materials for nEXO. It contains no derivations, equations, fitted parameters, predictions, or first-principles results that could reduce to inputs by construction. The central claim of 'among the most restrictive constraints' is a factual statement about the sensitivity of the tabulated data, not a derived quantity. No self-citations function as load-bearing premises, and the work is self-contained against external benchmarks as a data tabulation.
Axiom & Free-Parameter Ledger
Reference graph
Works this paper leans on
-
[1]
Decay counting is based on the determination of the 40K, 228Ac, 212Pb, 212Bi, 208Tl, 234mPa, 226Ra, 214Pb, 214Bi decay rates. The conversion of activ- ities into background event rates is often indepen- dent of assumptions about decay-chain equilibrium. While non-destructive, this approach typically of- fers limited sensitivity (tens of ppt for Th and U, ...
-
[2]
The atom counting approach for natK, 232Th, and 238U only requires limited amounts of samples (g- scale and smaller), offers fast turn-around (days to weeks per unique sample) and has excellent sensitivity (sub-ppt, equating toµBq/kg or sub- µBq/kg), but is destructive. This approach is gen- erally sensitive to much lower activities than decay counting, b...
work page 1978
-
[3]
B. Loer, P. Harrington, B. Archambault, E. Fuller, B. Pierson, I. Arnquist, K. Harouaka, T. Schlieder, D. Kim, A. Melville, B. Niedzielski, J. Yoder, K. Ser- niak, W. Oliver, J. Orrell, R. Bunker, B. VanDevender, and M. Warner, J. Instrum.19, P09001 (2024)
work page 2024
-
[4]
M. Agostini, G. Benato, J. A. Detwiler, J. Men´ endez, and F. Vissani, Rev. Mod. Phys.95, 025002 (2023)
work page 2023
-
[5]
Adhikariet al.(nEXO Collaboration), J
G. Adhikariet al.(nEXO Collaboration), J. Phys. G49, 015104 (2021)
work page 2021
-
[6]
N. Abgrallet al.(LEGEND-1000 Collaboration), Legend-1000 preconceptual design report (2021), arXiv:2107.11462 [physics.ins-det]
-
[7]
The CUPID Interest Group (CUPID Collaboration), CU- PID pre-CDR (2019), arXiv:1907.09376 [physics.ins-det]
work page Pith review arXiv 2019
-
[8]
Arpesellaet al.(BOREXINO Collaboration), As- tropart
C. Arpesellaet al.(BOREXINO Collaboration), As- tropart. Phys.18, 1 (2002)
work page 2002
-
[9]
Armengaudet al.(EDELWEISS Collaboration), As- tropart
E. Armengaudet al.(EDELWEISS Collaboration), As- tropart. Phys.47, 1 (2013)
work page 2013
-
[10]
D. Leonard, P. Grinberg, P. Weber, E. Baussan, Z. Djur- cic, G. Keefer, A. Piepke, A. Pocar, J.-L. Vuilleumier, J.-M. Vuilleumier,et al., Nucl. Instrum. Methods A591, 490 (2008)
work page 2008
-
[11]
D. Leonard, D. Auty, T. Didberidze, R. Gornea, P. Grin- berg, R. MacLellan, B. Methven, A. Piepke, J.-L. Vuilleu- mier,et al., Nucl. Instrum. Methods A871, 169 (2017)
work page 2017
-
[12]
D. Budj´ aˇ s, A. Gangapshev, J. Gasparro, W. Hampel, M. Heisel, G. Heusser, M. Hult, A. Klimenko, V. Kuzmi- nov, M. Laubenstein, W. Maneschg, H. Simgen, A. Smol- nikov, C. Tomei, and S. Vasiliev, Appl. Radiat. Isot.67, 755 (2009), 5th international conference on radionuclide metrology - low-level radioactivity measurement tech- niques ICRM-LLRMT’08
work page 2009
-
[13]
Akeribet al.(LUX Collaboration), Astropart
D. Akeribet al.(LUX Collaboration), Astropart. Phys. 62, 33 (2015)
work page 2015
-
[14]
D. S. Akeribet al.(LZ Collaboration), Eur. Phys. J. C 80, 1044 (2020)
work page 2020
-
[15]
Abgrallet al.(MAJORANA Collaboration), Nucl
N. Abgrallet al.(MAJORANA Collaboration), Nucl. In- strum. Methods A828, 22 (2016)
work page 2016
-
[16]
´Alvarezet al.(NEXT Collaboration), J
V. ´Alvarezet al.(NEXT Collaboration), J. Instrum.8, T01002 (2013)
work page 2013
- [17]
- [18]
-
[19]
Aprileet al.(XENON Collaboration), Eur
E. Aprileet al.(XENON Collaboration), Eur. Phys. J. C 77, 890 (2017)
work page 2017
-
[20]
Abeet al.(XMASS Collaboration), J
K. Abeet al.(XMASS Collaboration), J. Instrum.15, P09027 (2020)
work page 2020
-
[21]
J. B. Albertet al.(EXO-200 Collaboration), Phys. Rev. C92, 015503 (2015)
work page 2015
-
[22]
G. Heusser, M. Laubenstein, and H. Neder, inRadionu- clides in the Environment, Radioactivity in the Environ- ment, Vol. 8, edited by P. Povinec and J. Sanchez-Cabeza (Elsevier, 2006) pp. 495–510
work page 2006
-
[23]
N. Ackermann, H. Bonet, C. Buck, O. Chkvorets, J. Hak- enm¨ uller, G. Heusser, M. Laubenstein, M. Lindner, W. Maneschg, J. Schreiner, and H. Strecker, Appl. Ra- diat. Isot.194, 110652 (2023)
work page 2023
-
[24]
Some older measurements were taken with a less efficient muon detection system, prior to it being upgraded
- [25]
-
[26]
B. LaFerriere, T. Maiti, I. Arnquist, and E. Hoppe, Nucl. Instrum. Methods A775, 93 (2015)
work page 2015
-
[27]
I. Arnquist, M. di Vacri, and E. Hoppe, Nucl. In- strum. Methods A965, 163761 (2020)
work page 2020
-
[28]
I. J. Arnquist, C. Beck, M. L. di Vacri, K. Harouaka, and R. Saldanha, Nucl. Instru. Methods A959, 163573 (2020)
work page 2020
-
[29]
I. J. Arnquist, M. L. di Vacri, N. Rocco, R. Saldanha, T. Schlieder, R. Patel, J. Patil, M. Perez, and H. Uka, EPJ Tech. Instrum.10, 17 (2023)
work page 2023
-
[30]
K. Harouaka, E. W. Hoppe, and I. J. Arnquist, J. Anal. At. Spectrom.35, 2859 (2020)
work page 2020
-
[31]
M. L. di Vacri, I. J. Arnquist, H. O. Back, M. Bliss, M. Bronikowski, E. Edwards, B. R. Hackett, E. W. Hoppe, S. M. Lyons, N. D. Rocco, R. Rosero, A. Seifert, A. Swindle, and M. Yeh, J. Radioanal. Nucl. Chem.331, 5597 (2022)
work page 2022
-
[32]
I. J. Arnquist, E. W. Hoppe, M. Bliss, and J. W. Grate, Anal. Chem.90, 1432 (2018). 19
work page 2018
-
[33]
American Society for Quality, Sampling procedures and tables for inspection by variables for percent nonconform- ing, ASQ/ANSI Z1.9-2003 (R2018) (2018)
work page 2003
-
[34]
Agrawalet al.(AMoRE Collaboration), Front
A. Agrawalet al.(AMoRE Collaboration), Front. Phys. 12, 1362209 (2024)
work page 2024
- [35]
-
[36]
D. Chernyak, I. J. Arnquist, T. Daniels, S. W. Finch, L. Hissong, M. Hughes, R. MacLellan, A. Piepke, A. Pocar, R. Roshong, R. Saldanha, , and R. H. M. Tsang, Phys. Rev. C , (2025)
work page 2025
-
[37]
J.-X. Wang, T. C. Andersen, and J. J. Simpson, Nucl. In- strum. Methods A421, 601 (1999)
work page 1999
-
[38]
T. Andersen, I. Blevis, J. Boger, E. Bonvin, M. Chen, B. Cleveland, X. Dai, F. Dalnoki-Veress, G. Doucas, J. Farine,et al., Nucl. Instrum. Methods A501, 399 (2003)
work page 2003
-
[39]
J. Farine (2005) pp. 199–208, https://pubs.aip.org/aip/acp/article- pdf/785/1/199/12046559/199 1 online.pdf
work page 2005
- [40]
- [41]
- [42]
- [43]
-
[44]
T. Sz¨ ucs, D. Bemmerer, D. Degering, A. Domula, M. Grieger, F. Ludwig, K. Schmidt, J. Steckling, S. Turkat, and K. Zuber, Eur. Phys. J. A55, 174 (2019)
work page 2019
-
[45]
T. Roosendaal, C. Overman, G. Ortega, T. Schlieder, N. Rocco, L. Horkley, K. Hobbs, K. Harouaka, J. Orrell, et al., Nucl. Instrum. Methods A1087, 171402 (2026)
work page 2026
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.