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Record W3030735633 · doi:10.1103/physrevd.102.091101

Constraints on low-mass, relic dark matter candidates from a surface-operated SuperCDMS single-charge sensitive detector

2020· article· en· W3030735633 on OpenAlexafffund
D. W. P. Amaral, T. Aralis, T. Aramaki, I. J. Arnquist, E. Azadbakht, S. Banik, D. Barker, C. Bathurst, D. Bauer, L. V. S. Bezerra, R. Bhattacharyya, Tobias Binder, M. A. Bowles, P. L. Brink, R. Bunker, B. Cabrera, R. Calkins, R. A. Cameron, C. Cartaro, D. G. Cerdeño, Y.-Y. Chang, R. Chen, N. Chott, J. Cooley, H. Coombes, Jacqueline Corbett, P. Cushman, F. De Brienne, M. L. di Vacri, M. D. Diamond, E. Fascione, E. Figueroa‐Feliciano, C. W. Fink, K. Fouts, M. Fritts, G. Gerbier, R. Germond, M. Ghaith, S. R. Golwala, H. R. Harris, Nick Herbert, B. A. Hines, M. Hollister, Z. Hong, E. W. Hoppe, L. Hsu, M. E. Huber, V. Iyer, D. Jardin, A. Jastram, M. H. Kelsey, A. Kubik, N. A. Kurinsky, R. E. Lawrence, A. Li, B. Loer, E. Lopez Asamar, P. Lukens, Danika Marina Macdonell, D. B. MacFarlane, R. Mahapatra, V. Mandic, N. Mast, A. Mayer, Eva Michaud, E. Michielin, N. Mirabolfathi, B. Mohanty, J. D. Morales Mendoza, S.S. Nagorny, J. K. Nelson, H. Neog, V. Novati, J. L. Orrell, S. M. Oser, W. A. Page, P. Pakarha, R. Partridge, R. Podviianiuk, F. Ponce, S. S. Poudel, M. Pyle, W. Rau, E. Reid, R. Ren, T. Reynolds, A. Roberts, Alan Robinson, H. E. Rogers, T. Saab, B. Sadoulet, J. Sander, Amirmohammad Sattari, R. W. Schnee, S. Scorza, B. Serfass, D. J. Sincavage, C. Stanford, M. Stein, John Street, D. Toback, R. Underwood, S. Verma, A. N. Villano, B. von Krosigk, S. L. Watkins, L. Wills, J. S. Wilson, M. J. Wilson, J. Winchell, D. H. Wright, S. Yellin, Betty Young, To Chin Yu, E. Zhang, H. G. Zhang, X. Zhao, Liang Zheng

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicDark Matter and Cosmic Phenomena
Canadian institutionsUniversité de MontréalQueen's UniversityUniversity of British ColumbiaUniversity of TorontoTRIUMF
FundersSLAC National Accelerator LaboratoryPacific Northwest National LaboratoryDeutsche ForschungsgemeinschaftNatural Sciences and Engineering Research Council of CanadaDepartment of Atomic Energy, Government of IndiaBattelleDepartment of Science and Technology, Ministry of Science and Technology, IndiaFermilabHigh Energy PhysicsU.S. Department of EnergyNational Science Foundation
KeywordsPhysicsDark matterElectronAtomic physicsDetectorKinetic energyParticle physicsNuclear physicsOptics

Abstract

fetched live from OpenAlex

This article presents an analysis and the resulting limits on light dark matter inelastically scattering off of electrons, and on dark photon and axionlike particle absorption, using a second-generation SuperCDMS high-voltage eV-resolution detector. The 0.93 g Si detector achieved a 3 eV phonon energy resolution; for a detector bias of 100 V, this corresponds to a charge resolution of 3% of a single electron-hole pair. The energy spectrum is reported from a blind analysis with 1.2 g-days of exposure acquired in an above-ground laboratory. With charge carrier trapping and impact ionization effects incorporated into the dark matter signal models, the dark matter-electron cross section ${\overline{\ensuremath{\sigma}}}_{e}$ is constrained for dark matter masses from 0.5 to ${10}^{4}\text{ }\text{ }\mathrm{MeV}/{c}^{2}$; in the mass range from 1.2 to $50\text{ }\text{ }\mathrm{eV}/{c}^{2}$ the dark photon kinetic mixing parameter $ϵ$ and the axioelectric coupling constant ${g}_{ae}$ are constrained. The minimum 90% confidence-level upper limits within the above-mentioned mass ranges are ${\overline{\ensuremath{\sigma}}}_{e}=8.7\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}34}\text{ }\text{ }{\mathrm{cm}}^{2}$, $ϵ=3.3\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}14}$, and ${g}_{ae}=1.0\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}9}$.

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: Bench or experimental · Consensus signal: Bench or experimental
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.002
Threshold uncertainty score0.009

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.003
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0010.000
Insufficient payload (model declined to judge)0.0020.000

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 head0.014
GPT teacher head0.323
Teacher spread0.309 · 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

Citations168
Published2020
Admission routes2
Has abstractyes

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