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Record W4414487630 · doi:10.48550/arxiv.2504.13089

Absorption of Fermionic Dark Matter in the PICO-60 C$_{3}$F$_{8}$ Bubble Chamber

2025· preprint· en· W4414487630 on OpenAlexafffund
E. Adams, B. Ali, Rajan Anderson-Dornan, I. J. Arnquist, Mei Bai, D. Baxter, E. Behnke, B. Broerman, C. J. Chen, K. Clark, J. I. Collar, P. S. Cooper, D. J. Cranshaw, C. Cripe, M. Crisler, C. E. Dahl, Mala Das, Subir K. Das, S. Fallows, J. Farine, R. Filgas, A. García-Viltres, G. Giroux, O. Harris, H. Hawley-Herrera, T. Hillier, E. W. Hoppe, C. M. Jackson, M. Jin, C. B. Krauss, M. Laurin, I. Lawson, A. Leblanc, H. Leng, I. Levine, C. Licciardi, W. H. Lippincott, Q. Malin, P. Mitra, V. Monette, C. Moore, R. Neilson, A. J. Noble, H. Nozard, Sanjoy Kumar Pal, M.-C. Piro, S. Priya, C. Rethmeier, Mathieu Robert, A. E. Robinson, J. Savoie, S. J. Sekula, A. Sonnenschein, N. Starinski, I. Štekl, M. Tripathi, E. Vázquez-Jáuregui, U. Wichoski, William Woodley, V. Zacek, J. Zhang

Bibliographic record

VenueOSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) · 2025
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicDark Matter and Cosmic Phenomena
Canadian institutionsCarleton UniversityLaurentian UniversityUniversité de MontréalUniversity of AlbertaQueen's University
FundersPacific Northwest National LaboratoryNuclear PhysicsNatural Sciences and Engineering Research Council of CanadaDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoFermilabHigh Energy PhysicsOntario Ministry of Research and InnovationOffice of ScienceFundación Marcos MoshinskyAlliance de recherche numérique du CanadaČeské Vysoké Učení Technické v PrazeBattelleU.S. Department of EnergyUniversity of ChicagoNational Science Foundation
KeywordsDark matterBubbleAbsorption (acoustics)Bubble chamberSensitivity (control systems)Parameter spaceField (mathematics)

Abstract

fetched live from OpenAlex

Fermionic dark matter absorption on nuclear targets via neutral current interactions is explored using a non-relativistic effective field theory framework. An analysis of data from the PICO-60 C$_{3}$F$_{8}$ bubble chamber sets leading constraints on spin-independent absorption for dark matter masses below 23 MeV/$\textit{c}^2$ and establishes the first limits on spin-dependent absorptive interactions. These results demonstrate the sensitivity of bubble chambers to low-mass dark matter and underscore the importance of absorption searches in expanding the parameter space of direct detection experiments.

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)0.000
metaresearch head score (Gemma)0.000
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: Bench or experimental
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.003
Threshold uncertainty score0.008

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.001
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.000

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 head0.010
GPT teacher head0.233
Teacher spread0.223 · 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

Citations0
Published2025
Admission routes2
Has abstractyes

Explore more

Same venueOSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information)→Same topicDark Matter and Cosmic Phenomena→French-language works237,207→