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Dark Matter Search Results from the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>PICO</mml:mi><mml:mtext>−</mml:mtext><mml:mn>60</mml:mn><mml:msub><mml:mrow><mml:mtext> </mml:mtext><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msub><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="normal">F</mml:mi></mml:mrow><mml:mrow><mml:mn>8</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:mrow></mml:math> Bubble Chamber

2017· article· lv· W2756902241 on OpenAlexafffund
C. Amole, M. Ardid, I. J. Arnquist, D. M. Asner, D. Baxter, E. Behnke, Pijushpani Bhattacharjee, H. Borsodi, M. Bou-Cabo, P. Campion, G. Cao, C. J. Chen, U. Chowdhury, K. Clark, J. I. Collar, P. S. Cooper, M. Crisler, Gavin Crowder, C. E. Dahl, Mala Das, S. Fallows, J. Farine, I. Felis, R. Filgas, F. Girard, G. Giroux, J. Hall, O. Harris, E. W. Hoppe, Miaochen Jin, C. B. Krauss, M. Laurin, I. Lawson, Alexandre Leblanc, I. Levine, W. H. Lippincott, F. Mamedov, Deepam Maurya, P. Mitra, T. Nania, R. Neilson, A. J. Noble, Sarah H. Olson, A. Diago Ortega, A. Plante, R.B. Podviyanuk, Shashank Priya, Alan Robinson, A. Catherine Roeder, R. Rucinski, O. Scallon, S. Seth, A. Sonnenschein, N. Starinski, I. Štekl, F. Tardif, E. Vázquez-Jáuregui, Joshua Wells, U. Wichoski, Y. Yan, V. Zacek, J. Zhang

Bibliographic record

VenuePhysical Review Letters · 2017
Typearticle
Languagelv
FieldPhysics and Astronomy
TopicDark Matter and Cosmic Phenomena
Canadian institutionsUniversité de MontréalUniversity of AlbertaLaurentian UniversitySnolabQueen's University
FundersPacific Northwest National LaboratoryDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoNatural Sciences and Engineering Research Council of CanadaOntario Ministry of Research, Innovation and ScienceMinisterstvo Školství, Mládeže a TělovýchovyDepartment of Atomic Energy, Government of IndiaCanada Foundation for InnovationUniversity of ChicagoNational Science FoundationCompute CanadaFermilabWestern Canada Research GridConsejo Nacional de Ciencia y TecnologíaBattelleU.S. Department of EnergyMinisterio de Economía y Competitividad
KeywordsPhysicsWIMPNeutronRecoilDark matterNuclear physicsMassive particleScatteringParticle physicsOptics

Abstract

fetched live from OpenAlex

New results are reported from the operation of the PICO-60 dark matter detector, a bubble chamber filled with 52 kg of C3F8 located in the SNOLAB underground laboratory.As in previous PICO bubble chambers, PICO-60 C3F8 exhibits excellent electron recoil and alpha decay rejection, and the observed multiple-scattering neutron rate indicates a single-scatter neutron background of less than 1 event per month.A blind analysis of an efficiency-corrected 1167-kg-day exposure at a 3.3-keV thermodynamic threshold reveals no single-scattering nuclear recoil candidates, consistent with the predicted background.These results set the most stringent direct-detection constraint to date on the WIMP-proton spin-dependent cross section at 3.4 × 10 -41 cm 2 for a 30-GeV c -2 WIMP, more than one order of magnitude improvement from previous PICO results.

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)0.003
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: none
Teacher disagreement score0.145
Threshold uncertainty score0.484

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.003
Meta-epidemiology (narrow)0.0020.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0060.004
Science and technology studies0.0010.000
Scholarly communication0.0020.002
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.1450.077

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 head0.019
GPT teacher head0.252
Teacher spread0.233 · 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

Citations311
Published2017
Admission routes2
Has abstractyes

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