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Record W4294783129 · doi:10.1103/physrevd.107.112006

Sensitivity projections for a dual-phase argon TPC optimized for light dark matter searches through the ionization channel

2023· article· en· W4294783129 on OpenAlexafffund
P. Agnes, I. Ahmad, S. Albergo, I. F. M. Albuquerque, T. Alexander, P. Amaudruz, M. Atzori Corona, D. J. Auty, M. Ave, I. C. Avetisov, Roman Avetisov, O. Azzolini, G. Batignani, Z. Balmforth, V. Barbarian, A. Barrado Olmedo, P. Barrillon, A. Basco, G. Batignani, Elizabeth Berzin, A. Bondar, W. Bonivento, E. Borisova, B. Bottino, M. G. Boulay, G. Buccino, S. Bussino, J. Busto, A. Buzulutskov, M. Cadeddu, Mariano Cadoni, A. Caminata, N. Canci, A. Capra, S. Caprioli, M. Caravati, Miguel Cárdenas‐Montes, N. Cargioli, M. Carlini, Paolo Castello, V. Cataudella, P. Cavalcante, S. Cavuoti, S. Cebrián, J. M. Cela Ruiz, S. Chashin, A. Chepurnov, Eduard Chyhyrynets, C. Cicalò, L. Cifarelli, D. Cintas, V. Cocco, E. Conde Vilda, L. Consiglio, S. Copello, G. Covone, Stephen Cross, M. Czubak, Mario D’Aniello, S. D’Auria, M. Rolo, O. Dadoun, M. Daniel, S. Davini, A. De Candia, S. De Cecco, G. De Filippis, D. De Gruttola, S. De Pasquale, G. Rosa, G. Dellacasa, A. Derbin, A. Devoto, F. Di Capua, L. Di Noto, P. Di Stefano, C. Dionisi, G. Dolganov, F. Dordei, L. Doria, T. Erjavec, M. Fernández Díaz, G. Fiorillo, A. Franceschi, P. Franchini, D. Franco, E. Frolov, N. Funicello, F. Gabriele, D. Gahan, C. Galbiati, G. Gallina, G. Gallus, M. Garbini, P. Garcia Abia, A. Gendotti, C. Ghiano, Raffaele Aaron Giampaolo, C. Giganti, M. A. Giorgi, G. K. Giovanetti, V. Goicoechea Casanueva, A. Gola, Dylan J Gorman, R. Graciani Diaz, G. Grauso, Giovanni Grilli di Cortona, A. Grobov, M. Gromov, M. Guan, M. Guerzoni, M. Gulino, Cong Guo, B. R. Hackett, James B. Hall, A. L. Hallin, A. Hamer, H. Helton, M. Haranczyk, T Hessel, Steve J. Hill, S. Horikawa, F. Hubaut, T. Hugues, E. Hungerford, An. Ianni, V. Ippolito, C. Jillings, P. Kachru, A. Kemp, C. Kendziora, G. Keppel, A. V. Khomyakov, Masato Kimura, I. Kochanek, K. Kondo, G. Korga, S. Koulosousas, A. Kubankin, M. Kuss, M. Kuźniak, M. La Commara, M. Lai, E. Le Guirriec, E. Leason, X. Li, L. Lidey, J. Lipp, M. Lissia, L. Luzzi, O. Macfadyen, I. N. Machulin, I. Manthos, L. Mapelli, A. Margotti, S. M. Mari, C. Mariani, J. Maricic, A. Marini, M. Martínez, C. J. Martoff, A. Masoni, K. Mavrokoridis, A. Mazzi, A. Messina, R. Milincic, A. Moggi, A. Moharana, J. Monroe, M. Morrocchi, Elena Mozhevitina, Tomasz Mróz, V. Muratova, Carlo Muscas, P. Musico, R. Nania, Т. Наполитано, M. Nessi, G. Nieradka, K. Nikolopoulos, I. S. Nikulin, J. Nowak, K. Olchansky, A. Oleinik, V. Oleynikov, P. Organtini, A. Órtiz de Solórzano, L. Pagani, M. Pallavicini, L. Pandola, E. Pantic, E. Paoloni, G. Paternoster, P. A. Pegoraro, K. Pelczar, C. Pellegrino, F. Perotti, V. Pesudo, S. Piacentini, F. Pietropaolo, N. Pino, C. Pira, A. Pocar, D. M. Poehlmann, S. Pordes, P. Pralavorio, D. Price, F. Raffaelli, F. Ragusa, Y. Ramachers, A. P. D. Ramirez, M. Razeti, A. Razeto, A. L. Renshaw, M. Rescigno, F. Resnati, F. Retière, L. P. Rignanese, C. Ripoli, A. Rivetti, A. Roberts, C. Roberts, J. Rode, G. Rogers, L. Romero, M. Rossi, A. Rubbia, S. Jois, Tim Saffold, O. Samoylov, W. Sands, S. Sanfilippo, D. Santone, R. Santorelli, C. Savarese, E. Scapparone, G. Scioli, D. A. Semenov, A. Shchagin, A. Sheshukov, M. Simeone, P. Skensved, M. D. Skorokhvatov, O. Smirnov, T. Smirnova, B. Smith, A. Sokolov, M. Spangenberg, A. Sotnikov, A. Steri, S. Stracka, V. Strickland, M. Stringer, Sara Sulis, A. Sung, Y. Suvorov, A. M. Szelc, C. Türkoğlu, R. Tartaglia, A. Taylor, J. Taylor, S. Tedesco, G. Testera, K. Thieme, T. N. Thorpe, A. Tonazzo, S. Torres-Lara, A. Tricomi, E. Unzhakov, T. Vallivilayil John, Marco Van Uffelen, T. Viant, S. Viel, A. Vishneva, M. Wada, J. H. Vossebeld, M. B. Walczak, Y. Wang, S. Westerdale, R. Wheadon, L. Williams, I. Wingerter-Seez, R. Wojaczyński, M. Wójcik, T. Wright, Y. Xie, Chao Yang, Azam Zabihi, P. Zakhary, A. Zani, A. Zichichi, G. Zuzel, M. P. Zykova

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicDark Matter and Cosmic Phenomena
Canadian institutionsSnolabQueen's UniversityLaurentian UniversityUniversity of AlbertaCarleton UniversityTRIUMF
FundersPacific Northwest National LaboratoryHigh Energy PhysicsEuropean CommissionMinisterio de Ciencia e InnovaciónInstituto Nazionale di Fisica NucleareNatural Sciences and Engineering Research Council of CanadaInstitut National de Physique Nucléaire et de Physique des ParticulesScience and Technology Facilities CouncilHorizon 2020 Framework ProgrammeOffice of ScienceIstituto Nazionale di Fisica NucleareLaboratori Nazionali del Gran SassoMinisterstwo Edukacji i NaukiNarodowe Centrum NaukiMinistero dell’Istruzione, dell’Università e della RicercaConselho Nacional de Desenvolvimento Científico e TecnológicoLabex UnivEarthSU.S. Department of EnergyNational Natural Science Foundation of ChinaBattelleAgence Nationale de la RechercheEuropean Regional Development FundFundacja na rzecz Nauki PolskiejChinese Academy of SciencesFermilabUK Research and InnovationNational Science FoundationRoyal SocietyFundação de Amparo à Pesquisa do Estado de São Paulo
KeywordsPhysicsDark matterSensitivity (control systems)DetectorElectronNuclear physicsTime projection chamberParticle physicsOpticsElectronic engineering

Abstract

fetched live from OpenAlex

Dark matter lighter than $10\text{ }\text{ }\mathrm{GeV}/{c}^{2}$ encompasses a promising range of candidates. A conceptual design for a new detector, DarkSide-LowMass, is presented, based on the DarkSide-50 detector and progress toward DarkSide-20k, optimized for a low-threshold electron-counting measurement. Sensitivity to light dark matter is explored for various potential energy thresholds and background rates. These studies show that DarkSide-LowMass can achieve sensitivity to light dark matter down to the solar neutrino fog for GeV-scale masses and significant sensitivity down to $10\text{ }\text{ }\mathrm{MeV}/{c}^{2}$ considering the Migdal effect or interactions with electrons. Requirements for optimizing the detector's sensitivity are explored, as are potential sensitivity gains from modeling and mitigating spurious electron backgrounds that may dominate the signal at the lowest energies.

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)0.001
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.746
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0000.001
Science and technology studies0.0010.000
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 head0.034
GPT teacher head0.422
Teacher spread0.388 · 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

Citations30
Published2023
Admission routes2
Has abstractyes

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