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First Direct-Detection Constraints on eV-Scale Hidden-Photon Dark Matter with DAMIC at SNOLAB

2017· article· en· W2563776882 on OpenAlexafffund
A. A. Aguilar-Arevalo, D. Amidei, X. Bertou, Melissa Butner, Gustavo Cancelo, A. Vázquez, Brenda A. Cervantes-Vergara, Á. Chavarría, Claudio Chavez, Juan Carlos D’Olivo, Juan Estrada, Guillermo Fernández Moroni, R. Gaïor, Y. Guardincerri, K. Torres, Federico Izraelevitch, A. Kavner, B. Kilminster, I. Lawson, A. Letessier‐Selvon, J. Liao, Ariel Matalon, V. B. B. Mello, Jorge Molina, P. Privitera, Karthik Ramanathan, Y. Sarkis, T. Schwarz, M. Settimo, M. Sofo Haro, R. Thomas, Javier Tiffenberg, E. Tiouchichine, D. Torres Machado, Frédéric Trillaud, X. You, J. Zhou

Bibliographic record

VenuePhysical Review Letters · 2017
Typearticle
Languageen
FieldPhysics and Astronomy
TopicDark Matter and Cosmic Phenomena
Canadian institutionsSnolab
FundersFermilabOntario Ministry of Research and InnovationDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoCanada Foundation for InnovationCoordenação de Aperfeiçoamento de Pessoal de Nível SuperiorSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroConselho Nacional de Desenvolvimento Científico e TecnológicoUniversity of ChicagoKavli FoundationUniversidad Nacional Autónoma de MéxicoAgence Nationale de la RechercheConsejo Nacional de Ciencia y TecnologíaNational Science Foundation
KeywordsPhysicsDark matterPhotonDark photonSensitivity (control systems)Scalar field dark matterKinetic energyHaloDark matter haloGalactic haloAstrophysicsLight dark matterAbsorption (acoustics)Atomic physicsDark energyGalaxyOpticsCosmologyQuantum mechanics

Abstract

fetched live from OpenAlex

We present direct detection constraints on the absorption of hidden-photon dark matter with particle masses in the range $1.2--30\text{ }\mathrm{eV}\text{ }{c}^{\ensuremath{-}2}$ with the DAMIC experiment at SNOLAB. Under the assumption that the local dark matter is entirely constituted of hidden photons, the sensitivity to the kinetic mixing parameter $\ensuremath{\kappa}$ is competitive with constraints from solar emission, reaching a minimum value of $2.2\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}14}$ at $17\text{ }\text{ }\mathrm{eV}\text{ }{c}^{\ensuremath{-}2}$. These results are the most stringent direct detection constraints on hidden-photon dark matter in the galactic halo with masses $3--12\text{ }\text{ }\mathrm{eV}\text{ }{c}^{\ensuremath{-}2}$ and the first demonstration of direct experimental sensitivity to ionization signals $<12\text{ }\text{ }\mathrm{eV}$ from dark matter interactions.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesInsufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.490
Threshold uncertainty score0.999

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.001

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 head0.244
Teacher spread0.235 · 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 teacher head, not a consensus.

Study designNot applicable
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

Citations98
Published2017
Admission routes2
Has abstractyes

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