MétaCan
Menu
Back to cohort
Record W4405796326 · doi:10.1038/s42005-024-01896-z

DarkSide-20k sensitivity to light dark matter particles

2024· article· en· W4405796326 on OpenAlexafffund
Fabio Acerbi, P. Adhikari, P. Agnes, I. Ahmad, S. Albergo, I. F. M. Albuquerque, T. Alexander, P. Amaudruz, M. Angiolilli, E. Aprile, Raffaele Ardito, M. Atzori Corona, D. J. Auty, M. Ave, I. C. Avetisov, O. Azzolini, G. Batignani, Z. Balmforth, A. Barrado Olmedo, P. Barrillon, G. Batignani, Plaban Kumar Bhowmick, S. Blua, V. Bocci, W. Bonivento, B. Bottino, M. G. Boulay, A. Buchowicz, S. Bussino, J. Busto, M. Cadeddu, Mariano Cadoni, Roberta Calabrese, V. Camillo, A. Caminata, N. Canci, A. Capra, M. Caravati, Miguel Cárdenas‐Montes, N. Cargioli, A. Castellani, Paolo Castello, P. Cavalcante, S. Cebrián, J. M. Cela Ruiz, S. Chashin, A. Chepurnov, L. Cifarelli, D. Cintas, M. Citterio, B. Cleveland, Y. Coadou, V. Cocco, Davide Colaiuda, E. Conde Vilda, L. Consiglio, B. S. Costa, M. Czubak, Mario D’Aniello, S. D’Auria, M. Rolo, G. Darbo, S. Davini, S. De Cecco, Giorgia De Guido, G. Dellacasa, A. V. Derbin, A. Devoto, F. Di Capua, A. Di Lüdovico, L. Di Noto, P. Di Stefano, L. K. Dias, D. Díaz Mairena, Xuefeng Ding, C. Dionisi, G. Dolganov, F. Dordei, V. I. Dronik, A. Elersich, E. Ellingwood, T. Erjavec, M. Fernández Díaz, A. Ficorella, G. Fiorillo, P. Franchini, D. Franco, H. Frandini Gatti, E. Frolov, F. Gabriele, D. Gahan, C. Galbiati, G. Galiński, G. Gallina, G. Gallus, M. Garbini, P. Garcia Abia, A. Gawdzik, A. Gendotti, Aldo Ghisi, G. K. Giovanetti, V. Goicoechea Casanueva, A. Gola, L. Grandi, G. Grauso, Giovanni Grilli di Cortona, A. Grobov, M. Gromov, M. Guerzoni, M. Gulino, Chengcheng Guo, B. R. Hackett, A. L. Hallin, A. Hamer, M. Harańczyk, B. Harrop, T. Hessel, Steve J. Hill, S. Horikawa, J. Hu, F. Hubaut, J. Hucker, T. Hugues, E. Hungerford, Aldo Ianni, V. Ippolito, A. Jamil, C. Jillings, S. Jois, P. Kachru, R. Keloth, N. Kemmerich, A. Kemp, C.L. Kendziora, Masato Kimura, K. Kondo, G. Korga, L. Kotsiopoulou, S. Koulosousas, A. Kubankin, Pablo Kunzé, M. Kuss, M. Kuźniak, M. Kuźwa, M. La Commara, M. Lai, E. Le Guirriec, E. Leason, A. Leoni, L. Lidey, M. Lissia, L. Luzzi, G. Longo, O. Macfadyen, I. N. Machulin, S. Manecki, I. Manthos, A. Marasciulli, S. M. Mari, C. Mariani, J. Maricic, M. Martínez, C. J. Martoff, G. Matteucci, K. Mavrokoridis, A. B. McDonald, J. B. McLaughlin, S. Merzi, A. Messina, R. Milincic, S. Minutoli, A. Mitra, S. Moioli, J. Monroe, E. Moretti, M. Morrocchi, Tomasz Mróz, V. N. Muratova, M. Murphy, M. Murra, C. Muscas, R. Nania, M. Nessi, G. Nieradka, K. Nikolopoulos, E. Nikoloudaki, J. Nowak, K. Olchanski, A. Oleinik, V. Oleynikov, P. Organtini, A. Órtiz de Solórzano, M. Pallavicini, L. Pandola, E. Pantic, E. Paoloni, D. Papi, Grzegorz Pastuszak, G. Paternoster, A. Peck, P. A. Pegoraro, K. Pelczar, Laura A. Pellegrini, Rosana Pérez, F. Perotti, V. Pesudo, S. Piacentini, N. Pino, G. Plante, A. Pocar, M. Poehlmann, S. Pordes, P. Pralavorio, M Queiroga Bazetto, F. Ragusa, Y. Ramachers, A. Ramirez, S. Ravinthiran, M. Razeti, A. L. Renshaw, M. Rescigno, F. Retière, L. P. Rignanese, A. Rivetti, A. Roberts, C. Roberts, G. Rogers, L. Romero, M. Rossi, A. Rubbia, D. Rudik, M. Sabia, P. Salomone, O. Samoylov, W. Sands, S. Sanfilippo, D. Santone, R. Santorelli, E. M. Santos, C. Savarese, E. Scapparone, G. Schillaci, F. G. Schuckman, G. Scioli, D. A. Semenov, V. Shalamova, A. Sheshukov, M. Simeone, P. Skensved, O. Smirnov, T. Smirnova, B. Smith, A. Sotnikov, F. Spadoni, M. Spangenberg, A. Steri, V. Stornelli, C. Sunny, S. Sulis, A. Sung, Y. Suvorov, A. M. Szelc, O. A. Taborda, R. Tartaglia, A. Taylor, J. Taylor, S. Tedesco, G. Testera, K. Thieme, A. K. Thompson, A. Tonazzo, S. Torres-Lara, A. Tricomi, E. Unzhakov, T. J. Vallivilayil, M. Van Uffelen, L. Velazquez-Fernandez, T. Viant, S. Viel, A. Vishneva, R. B. Vogelaar, J. H. Vossebeld, B. Vyas, M. B. Walczak, Y. Wang, H Wang, S. Westerdale, L. Williams, R. Wojaczyński, M. Wójcik, M. Wójcik, T. Wright, Yi Xie, C. Yang, J. H. Yin, Azam Zabihi, P. Zakhary, A. Zani, Y. Zhang, Tao Zhu, A. Zichichi, G. Zuzel, M. P. Zykova

Bibliographic record

VenueCommunications Physics · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicDark Matter and Cosmic Phenomena
Canadian institutionsQueen's UniversitySnolabUniversity of AlbertaLaurentian UniversityTRIUMFCarleton University
FundersPacific Northwest National LaboratoryInstitut National de Physique Nucléaire et de Physique des ParticulesFermilabLabex UnivEarthSScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaOffice of ScienceMinisterio de Ciencia e InnovaciónIstituto Nazionale di Fisica NucleareMinisterstwo Edukacji i NaukiConselho Nacional de Desenvolvimento Científico e TecnológicoNational Natural Science Foundation of ChinaBattelleAgence Nationale de la RechercheEuropean Regional Development FundU.S. Department of EnergyFundacja na rzecz Nauki PolskiejEuropean CommissionChinese Academy of SciencesNational Science FoundationRoyal SocietyAix-Marseille UniversitéFundação de Amparo à Pesquisa do Estado de São Paulo
KeywordsWIMPPhysicsDark matterTime projection chamberWeakly interacting massive particlesNuclear physicsArgonElectronMassive particleSensitivity (control systems)Particle physicsAstrophysicsAtomic physicsScalar field dark matterCosmology

Abstract

fetched live from OpenAlex

The dual-phase liquid argon time projection chamber is presently one of the leading technologies to search for dark matter particles with masses below 10 GeV c−2. This was demonstrated by the DarkSide-50 experiment with approximately 50 kg of low-radioactivity liquid argon as target material. The next generation experiment DarkSide-20k, currently under construction, will use 1,000 times more argon and is expected to start operation in 2027. Based on the DarkSide-50 experience, here we assess the DarkSide-20k sensitivity to models predicting light dark matter particles, including Weakly Interacting Massive Particles (WIMPs) and sub-GeV c−2 particles interacting with electrons in argon atoms. With one year of data, a sensitivity improvement to dark matter interaction cross-sections by at least one order of magnitude with respect to DarkSide-50 is expected for all these models. A sensitivity to WIMP–nucleon interaction cross-sections below 1 × 10−42 cm2 is achievable for WIMP masses above 800 MeV c−2. With 10 years exposure, the neutrino fog can be reached for WIMP masses around 5 GeV c−2. The DarkSide-20k collaboration reports the sensitivity of its detector, currently under construction, to models predicting light dark matter particles. This includes Weakly Interacting Massive Particles and particles interacting with bound electrons of argon atoms.

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)0.002
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: Empirical
Teacher disagreement score0.008
Threshold uncertainty score0.025

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.000
Science and technology studies0.0010.001
Scholarly communication0.0010.001
Open science0.0010.002
Research integrity0.0010.000
Insufficient payload (model declined to judge)0.0080.002

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 head0.020
GPT teacher head0.277
Teacher spread0.257 · 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

Citations19
Published2024
Admission routes2
Has abstractyes

Explore more

Same venueCommunications PhysicsSame topicDark Matter and Cosmic PhenomenaFrench-language works237,207