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Record W4409360216 · doi:10.1139/cjp-2024-0183

Accelerator-based dark matter searches

2025· article· en· W4409360216 on OpenAlexaffvenueabout
C. Hearty, K. Pachal, David Curtin, Miriam Diamond, Jaipratap Singh Grewal, Zoe Hallman, C. Miller, Gabriel Owh, R. Ren, S. H. Robertson, H. L. Russell, Mamoksh Samra, Bennett Winnicky-Lewis

Bibliographic record

VenueCanadian Journal of Physics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicDark Matter and Cosmic Phenomena
Canadian institutionsUniversity of AlbertaSimon Fraser UniversityUniversity of TorontoTRIUMFUniversity of VictoriaInstitute of Particle PhysicsUniversity of British Columbia
Fundersnot available
KeywordsPhysicsDark matterAstrophysicsAstronomyParticle physicsNuclear physics

Abstract

fetched live from OpenAlex

In this chapter, we review Canadian efforts to search for dark matter at accelerator experiments, discussing Belle II and SuperKEKB, DarkLight, and MATHUSLA. This is an important direction in the search for astrophysical dark matter, as many dark matter candidates do not have any detectable interactions at underground detectors, but could be produced directly at colliders or fixed-target experiments, whether directly or in the decay of other newly produced particles. These accelerator-based searches can also reveal other aspects of the dark sector, including the presence of dark force carriers like dark photons or Higgs bosons, which could play a crucial role in the dynamics of dark matter in the early universe or today. These investigations are therefore crucial both for discovery and to elucidate how dark matter fits into an overall theoretical framework that extends the standard model of particle physics.

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)0.002
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: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.327
Threshold uncertainty score0.650

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.003
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0040.005
Science and technology studies0.0030.001
Scholarly communication0.0030.002
Open science0.0010.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0260.004

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 head0.015
GPT teacher head0.235
Teacher spread0.220 · 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 designSimulation or modeling
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

Citations1
Published2025
Admission routes3
Has abstractyes

Explore more

Same venueCanadian Journal of Physics→Same topicDark Matter and Cosmic Phenomena→French-language works237,207→