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Record W2805519466 · doi:10.1109/tns.2018.2875668

VUV-Sensitive Silicon Photomultipliers for Xenon Scintillation Light Detection in nEXO

2018· article· en· W2805519466 on OpenAlexafffund
A. Jamil, T. Ziegler, P. Hufschmidt, Gordon Li, L. Lupin-Jimenez, Thilo Michel, I. Ostrovskiy, F. Retière, Judith Schneider, M. Wagenpfeil, Amal Alamre, J. B. Albert, G. Anton, I. J. Arnquist, I. Badhrees, P. S. Barbeau, D. Beck, V. Belov, Trilochan Bhatta, F. Bourque, J. Brodsky, A. Brown, T. Brunner, A. Burenkov, G. F. Cao, Liqiang Cao, W. R. Cen, C. Chambers, Serge A. Charlebois, M. Chiu, B. T. Cleveland, Minor J. Coon, M. Côté, A. Craycraft, W. Cree, J. Dalmasson, T. Daniels, L. Darroch, S. J. Daugherty, J. Daughhetee, S. Delaquis, A. Der Mesrobian-Kabakian, R. DeVoe, J. Dilling, Ying Ding, M. J. Dolinski, A. Dragone, J. Echevers, L. Fabris, D. Fairbank, W. M. Fairbank, J. Farine, Soheyla Feyzbakhsh, Réjean Fontaine, D. Fudenberg, G. Gallina, G. Giacomini, R. Gornea, G. Gratta, E. V. Hansen, Devin K. Harris, M. Hasan, M. Heffner, E. W. Hoppe, A. House, M. Hughes, Y. Ito, A. Iverson, C. E. Jessiman, M. J. Jewell, X. S. Jiang, A. Karelin, L. J. Kaufman, T. Koffas, S. Kravitz, R. Krücken, A. Kuchenkov, K.S. Kumar, Y. Lan, A. C. Larson, D. S. Leonard, S. Li, Z. Li, C. Licciardi, Y. H. Lin, Peng Lv, R. MacLellan, B. Mong, David C. Moore, K. Murray, J. Newby, Zhe Ning, O. Njoya, F. Nolet, O. Nusair, K. Odgers, A. Odian, M. Oriunno, J. L. Orrell, G.S. Ortega, C.T. Overman, Samuel Parent, A. Piepke, A. Pocar, J.‐F. Pratte, Delong Qiu, V. Radeka, E. Raguzin, T. Rao, S. Rescia, A. Robinson, T. Rossignol, P.C. Rowson, N. Roy, R. Saldanha, S. Sangiorgio, Susann Schmidt, A. Schubert, D. Sinclair, A. K. Soma, G. St-Hilaire, V. Stekhanov, T. Stiegler, X. Sun, M. Tarka, J. Todd, T. Tolba, T.I. Totev, R. Tsang, T. Tsang, F. Vachon, B. Veenstra, V. Veeraraghavan, G. Visser, J.-L. Vuilleumier, Qiuhong Wang, J. Watkins, M. Weber, W. Wei, Liangjian Wen, U. Wichoski, Gerrit Wrede, Sen Wu, Wei Wu, Q. Xia, L. Yang, Y.-R. Yen, O. Zeldovich, Xuhao Zhang, Jinmiao Zhao, Ye-Ling Zhou

Bibliographic record

VenueIEEE Transactions on Nuclear Science · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicDark Matter and Cosmic Phenomena
Canadian institutionsMcGill UniversityUniversité de SherbrookeLaurentian UniversityCarleton UniversityTRIUMF
FundersPacific Northwest National LaboratoryOak Ridge National LaboratoryLawrence Livermore National LaboratoryMcGill UniversityHigh Energy PhysicsUniversité de SherbrookeInternational Science and Technology Cooperation ProgrammeFonds de recherche du Québec – Nature et technologiesNuclear PhysicsNatural Sciences and Engineering Research Council of CanadaUniversity of Illinois at Urbana-ChampaignRussian Foundation for Basic ResearchBayerisch-Kalifornischen HochschulzentrumYale UniversitySchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungCanada First Research Excellence FundUniversity of South DakotaNational Science FoundationTRIUMFBrookhaven National LaboratoryRaymond and Beverly Sackler Institute for Biological, Physical and Engineering Sciences, Yale UniversityU.S. Department of EnergyOffice of ScienceRensselaer Polytechnic Institute
KeywordsXenonSilicon photomultiplierPhotomultiplierScintillationAvalanche photodiodeOpticsDetectorPhysicsScintillatorNoble gasOptoelectronicsMaterials scienceNuclear physics

Abstract

fetched live from OpenAlex

Future ton-scale liquefied noble gas detectors depend on efficient light detection in the vacuum ultraviolet (VUV) range. In the past years, silicon photomultipliers (SiPMs) have emerged as a valid alternative to standard photomultiplier tubes or large-area avalanche photodiodes. The next-generation double-beta decay experiment, nEXO, with a 5-ton liquid xenon time projection chamber will use SiPMs for detecting the 175-nm xenon scintillation light, in order to achieve an energy resolution of$\boldsymbol {\sigma }/\boldsymbol {Q_{\beta \beta }} = 1$%. This paper presents recent measurements of the VUV-HD generation SiPMs from Fondazione Bruno Kessler, Trento, Italy, in two complementary setups. It includes measurements of the photon-detection efficiency (PDE) with gaseous xenon scintillation light in a vacuum setup and dark measurements in a dry nitrogen gas setup. We report improved PDE at 175 nm compared to previous generation devices that would meet the criteria of nEXO. Furthermore, we present the projected nEXO detector light collection and energy resolution that could be achieved by using these SiPMs.

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)0.000
metaresearch head score (Gemma)0.001
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 score0.003
Threshold uncertainty score0.009

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0010.001
Open science0.0010.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.001

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 head0.238
Teacher spread0.229 · 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

Citations44
Published2018
Admission routes2
Has abstractyes

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