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Record W4213300604 · doi:10.1103/physrevd.93.052014

Dark matter search results from the PICO-60<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mrow><mml:msub><mml:mrow><mml:mi>CF</mml:mi></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msub></mml:mrow><mml:mi mathvariant="normal">I</mml:mi></mml:mrow></mml:math>bubble chamber

2016· article· lv· W4213300604 on OpenAlexafffund
C. Amole, M. Ardid, D. M. Asner, D. Baxter, E. Behnke, Pijushpani Bhattacharjee, H. Borsodi, M. Bou-Cabo, S. J. Brice, D. Broemmelsiek, K. Clark, J. I. Collar, P. S. Cooper, M. Crisler, C. E. Dahl, Simon Daley, Mala Das, F. Debris, N. Dhungana, S. Fallows, J. Farine, I. Felis, R. Filgas, F. Girard, G. Giroux, A. Grandison, M. Hai, J. Hall, O. Harris, Miaochen Jin, C. B. Krauss, M. Lafrenière, M. Laurin, I. Lawson, I. Levine, W. H. Lippincott, E. Mann, Deepam Maurya, P. Mitra, R. Neilson, A. J. Noble, A. Plante, R. Podviianiuk, Shashank Priya, E. Ramberg, Alan Robinson, R. Rucinski, M. Ruschman, O. Scallon, S. Seth, P. Šimon, A. Sonnenschein, I. Štekl, E. Vázquez-Jáuregui, Joshua Wells, U. Wichoski, V. Zacek, J. Zhang, I. A. Shkrob

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2016
Typearticle
Languagelv
FieldPhysics and Astronomy
TopicDark Matter and Cosmic Phenomena
Canadian institutionsUniversity of AlbertaUniversité de MontréalLaurentian UniversityUniversity of TorontoSnolabQueen's University
FundersPacific Northwest National LaboratorySaha Institute of Nuclear Physics, Department of Atomic Energy, Government of IndiaOffice of ScienceMinisterstvo Školství, Mládeže a TělovýchovyNatural Sciences and Engineering Research Council of CanadaDepartment of Atomic Energy, Government of IndiaUniversity of ChicagoCanada Foundation for InnovationU.S. Department of EnergyMinisterio de Economía y CompetitividadNational Science Foundation
KeywordsPhysicsDark matterPopulationAstrophysicsParticle physics

Abstract

fetched live from OpenAlex

New data are reported from the operation of the PICO-60 dark matter detector, a bubble chamber filled with 36.8 kg of ${\mathrm{CF}}_{3}\mathrm{I}$ and located in the SNOLAB underground laboratory. PICO-60 is the largest bubble chamber to search for dark matter to date. With an analyzed exposure of 92.8 livedays, PICO-60 exhibits the same excellent background rejection observed in smaller bubble chambers. Alpha decays in PICO-60 exhibit frequency-dependent acoustic calorimetry, similar but not identical to that reported recently in a ${\mathrm{C}}_{3}{\mathrm{F}}_{8}$ bubble chamber. PICO-60 also observes a large population of unknown background events, exhibiting acoustic, spatial, and timing behaviors inconsistent with those expected from a dark matter signal. These behaviors allow for analysis cuts to remove all background events while retaining 48.2% of the exposure. Stringent limits on weakly interacting massive particles interacting via spin-dependent proton and spin-independent processes are set, and most interpretations of the DAMA/LIBRA modulation signal as dark matter interacting with iodine nuclei are ruled out.

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)0.001
metaresearch head score (Gemma)0.001
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.011
Threshold uncertainty score0.031

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0020.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0090.004

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 head0.017
GPT teacher head0.290
Teacher spread0.273 · 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 designObservational
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

Citations138
Published2016
Admission routes2
Has abstractyes

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