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Record W4400611390 · doi:10.1103/physrevd.111.012006

Light dark matter constraints from SuperCDMS HVeV detectors operated underground with an anticoincidence event selection

2025· article· en· W4400611390 on OpenAlexafffund
M. F. Albakry, I. Alkhatib, David Alonso-González, D. W. P. Amaral, J. Anczarski, T. Aralis, T. Aramaki, I. J. Arnquist, I. Ataee Langroudy, E. Azadbakht, C. Bathurst, R. Bhattacharyya, A. J. Biffl, P. L. Brink, M. L. Buchanan, R. Bunker, Blas Cabrera, R. Calkins, R. A. Cameron, C. Cartaro, D. G. Cerdeño, Y.-Y. Chang, M. Chaudhuri, J.-H. Chen, R. Chen, N. Chott, J. Cooley, H. Coombes, P. Cushman, R. Cyna, S. Das, F. De Brienne, S. Dharani, M. L. di Vacri, M. D. Diamond, M. Elwan, E. Fascione, E. Figueroa‐Feliciano, K. Fouts, M. Fritts, R. Germond, M. Ghaith, S. R. Golwala, J. Hall, S. A. S. Harms, K. Harris, N. Hassan, Z. Hong, E. W. Hoppe, L. Hsu, M. E. Huber, V. Iyer, D. Jardin, Varchaswi Kashyap, S. Keller, M. Kelsey, K. T. Kennard, A. Kubik, Noah Kurinsky, M. Lee, J. Leyva, J. Liu, Yihan Liu, B. Loer, E. Lopez Asamar, P. Lukens, D. B. MacFarlane, R. Mahapatra, J. S. Mammo, N. Mast, A. Mayer, H. Meyer Zu Theenhausen, É. Michaud, E. Michielin, N. Mirabolfathi, M. Mirzakhani, B. Mohanty, Diogo M. Souza Monteiro, J. Nelson, H. Neog, V. Novati, J. L. Orrell, M. D. Osborne, S. M. Oser, L. Pandey, S. Pandey, R. Partridge, D. S. Pedreros, Wen-Xi Peng, L. Perna, W. L. Perry, R. Podviianiuk, S. S. Poudel, A. Pradeep, M. Pyle, W. Rau, E. Reid, R Ren, T. Reynolds, Martín de los Rios, A. Roberts, Alan Robinson, J. Ryan, T. Saab, D. Sadek, B. Sadoulet, S. P. Sahoo, I. Saikia, J. Sander, A. Sattari, B. Schmidt, R. W. Schnee, S. Scorza, B. Serfass, Aviv Simchony, D. J. Sincavage, P. Sinervo, John Street, Huanbo Sun, Evan Tanner, G. D. Terry, D. Toback, S. Verma, A. N. Villano, B. von Krosigk, S. L. Watkins, O. Wen, Z. Williams, M. J. Wilson, J. Winchell, K. Wykoff, S. Yellin, Betty Young, T. C. Yu, B. Zatschler, S. Zatschler, A. Zaytsev, E. Zhang, Liang Zheng, A. Zuniga, M. J. Zurowski

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicDark Matter and Cosmic Phenomena
Canadian institutionsLaurentian UniversityUniversité de MontréalUniversity of TorontoQueen's UniversitySnolabUniversity of British Columbia
FundersMitchell InstitutePacific Northwest National LaboratoryDepartment of Atomic Energy, Government of IndiaAlliance de recherche numérique du CanadaDeutsche ForschungsgemeinschaftNatural Sciences and Engineering Research Council of CanadaTexas A and M UniversityCanada Excellence Research Chairs, Government of CanadaBattelleDepartment of Science and Technology, Ministry of Science and Technology, IndiaSLAC National Accelerator LaboratoryFermilabU.S. Department of EnergyNational Science Foundation
KeywordsDark matterPhysicsOverburdenParticle physicsCoupling (piping)Materials science

Abstract

fetched live from OpenAlex

This article presents constraints on dark-matter-electron interactions obtained from the first underground data-taking campaign with multiple SuperCDMS HVeV detectors operated in the same housing. An exposure of 7.63 g − days is used to set upper limits on the dark-matter-electron scattering cross section for dark matter masses between 0.5 and 1000 MeV / c 2 , as well as upper limits on dark photon kinetic mixing and axionlike particle axioelectric coupling for masses between 1.2 and 23.3 eV / c 2 . Compared to an earlier HVeV search, sensitivity was improved as a result of an increased overburden of 225 meters of water equivalent, an anticoincidence event selection, and better pile-up rejection. In the case of dark-matter-electron scattering via a heavy mediator, an improvement by up to a factor of 25 in cross section sensitivity was achieved.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.004
metaresearch head score (Gemma)0.006
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.007
Threshold uncertainty score0.024

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0040.006
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.002
Science and technology studies0.0010.001
Scholarly communication0.0020.001
Open science0.0010.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0070.001

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.009
GPT teacher head0.358
Teacher spread0.349 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designBench or experimental
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations22
Published2025
Admission routes2
Has abstractyes

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