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Measurement of Atmospheric Neutrino Oscillations with IceCube

2013· article· en· W2045752404 on OpenAlexafffund
M. G. Aartsen, Y. Abdou, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, D. Altmann, J. Auffenberg, X. Bai, M. Baker, S. W. Barwick, V. Baum, R. Bay, J. J. Beatty, S. Bechet, J. Becker Tjus, K.-H. Becker, M. Bell, M. L. Benabderrahmane, S. BenZvi, Jens Berdermann, P. Berghaus, D. Berley, E. Bernardini, A. Bernhard, Daniel Bertrand, D. Besson, G. Binder, D. Bindig, M. Bissok, E. Blaufuss, J. Blumenthal, D. J. Boersma, S. Bohaichuk, C. Böhm, D. Bose, S. Böser, O. Botner, L. Brayeur, H.-P. Bretz, A. M. Brown, R. Bruijn, J. Brünner, M. Carson, J. Casey, M. Casier, D. Chirkin, A. Christov, B. Christy, K. Clark, F. Clevermann, S. Coenders, S. Cohen, D. F. Cowen, A. H. Cruz Silva, M. Danninger, J. Daughhetee, J. C. Davis, C. De Clercq, S. De Ridder, P. Desiati, M. de With, T. DeYoung, J. C. Díaz–Vélez, M. Dunkman, R. Eagan, B. Eberhardt, J. Eisch, R. W. Ellsworth, S. Euler, P. A. Evenson, O. Fadiran, A. R. Fazely, Anatoli Fedynitch, J. Feintzeig, T. Feusels, K. Filimonov, C. Finley, T. Fischer-Wasels, S. Flis, A. Franckowiak, Robert Franke, K. Frantzen, T. Fuchs, T. K. Gaisser, J. S. Gallagher, L. Gerhardt, L. Gladstone, T. Glüsenkamp, A. Goldschmidt, G. Golup, J. G. González, J. A. Goodman, D. Góra, D. T. Grandmont, D. Grant, A. Groß, C. Ha, A. Haj Ismail, P. Hallen, A. Hallgren, F. Halzen, K. Hanson, D. Heereman, D. Heinen, K. Helbing, R. Hellauer, S. Hickford, G. C. Hill, K. D. Hoffman, R. Hoffmann, A. Homeier, K. Hoshina, W. Huelsnitz, P. O. Hulth, K. Hultqvist, S. Hussain, A. Ishihara, E. Jacobi, J. Jacobsen, K. Jagielski, G. S. Japaridze, K. Jero, O. Jlelati, B. Kaminsky, A. Kappes, T. Karg, A. Karle, J. L. Kelley, J. Kiryluk, F. Kislat, J. Kläs, J.-H. Köhne, G. Kohnen, H. Kolanoski, L. Köpke, Claudio Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, M. Krasberg, K. Krings, G. Kroll, J. Kunnen, N. Kurahashi, T. Kuwabara, M. Labare, H. Landsman, M. J. Larson, M. Lesiak-Bzdak, M. Leuermann, J. Leute, J. Lünemann, J. Madsen, R. Maruyama, K. Mase, H. S. Matis, F. McNally, K. Meagher, M. Merck, P. Mészáros, T. Meures, S. Miarecki, E. Middell, N. Milke, J. Miller, L. Mohrmann, T. Montaruli, R. Morse, R. Nahnhauer, Uwe Naumann, Hans Niederhausen, Sarah Nowicki, D. R. Nygren, A. Obertacke, S. Odrowski, A. Olivas, M. Olivo, A. O’Murchadha, A. Palazzo, L. Paul, J. A. Pepper, C. Pérez de los Heros, C. Pfendner, D. Pieloth, E. Pinat, Norbert Pirk, J. Posselt, P. B. Price, G. T. Przybylski, L. Rädel, M. Rameez, K. Rawlins, P. Redl, R. Reimann, E. Resconi, W. Rhode, M. Ribordy, M. Richman, Benedikt Riedel, J. P. Rodrigues, C. Rott, T. Ruhe, B. Ruzybayev, D. Ryckbosch, S. M. Saba, T. Salameh, H.‐G. Sander, M. Santander, S. Sarkar, K. Schatto, F. Scheriau, T. Schmidt, M. Schmitz, S. Schoenen, S. Schöneberg, A. Schönwald, A. Schukraft, L. Schulte, O. Schulz, D. Seckel, Y. Sestayo, S. Seunarine, C. Sheremata, M. W. E. Smith, Dennis Soldin, G. M. Spiczak, C. Spiering, M. Stamatikos, Todor Stanev, A. Stasik, T. Stezelberger, R. G. Stokstad, A. Stößl, E. A. Strahler, L. R. Strom, G. W. Sullivan, H. Taavola, I. Taboada, A. Tamburro, A. Tepe, S. Ter–Antonyan, G. Tešić, S. Tilav, P. A. Toale, S. Toscano, M. Usner, N. van Eijndhoven, A. Van Overloop, J. V. Santen, M. Vehring, M. Vöge, M. Vraeghe, C. Walck, T. Waldenmaier, M. Wallraff, R. Wasserman, Ch. Weaver, M. Wellons, C. Wendt, S. Westerhoff, N. Whitehorn, K. Wiebe, C. H. Wiebusch, D. R. Williams, H. Wissing, M. Wolf, T. R. Wood, K. Woschnagg, C. Xu, Dawei Xu, Xiaolin Xu, G. Yodh, S. Yoshida, P. Zarzhitsky, J. Ziemann, Simon Zierke, M. Zoll

Bibliographic record

VenuePhysical Review Letters · 2013
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of Alberta
FundersScience and Technology Facilities CouncilHelmholtz Alliance for Astroparticle PhysicsFonds Wetenschappelijk OnderzoekBundesministerium für Bildung und ForschungNatural Sciences and Engineering Research Council of CanadaKnut och Alice Wallenbergs StiftelseDeutsche ForschungsgemeinschaftWestern Canada Research GridOffice of Polar ProgramsFonds De La Recherche Scientifique - FNRSPolarforskningssekretariatetUniversity of Wisconsin-MadisonU.S. Department of EnergyVetenskapsrådetNational Science Foundation
KeywordsPhysicsNeutrinoMuonNeutrino oscillationParticle physicsMuon neutrinoNuclear physicsEnergy (signal processing)Solar neutrinoNeutrino detector

Abstract

fetched live from OpenAlex

We present the first statistically significant detection of neutrino oscillations in the high-energy regime ($>20\text{ }\text{ }\mathrm{GeV}$) from an analysis of IceCube Neutrino Observatory data collected in 2010 and 2011. This measurement is made possible by the low-energy threshold of the DeepCore detector ($\ensuremath{\sim}20\text{ }\text{ }\mathrm{GeV}$) and benefits from the use of the IceCube detector as a veto against cosmic-ray-induced muon background. The oscillation signal was detected within a low-energy muon neutrino sample (20--100 GeV) extracted from data collected by DeepCore. A high-energy muon neutrino sample (100 GeV--10 TeV) was extracted from IceCube data to constrain systematic uncertainties. The disappearance of low-energy upward-going muon neutrinos was observed, and the nonoscillation hypothesis is rejected with more than $5\ensuremath{\sigma}$ significance. In a two-neutrino flavor formalism, our data are best described by the atmospheric neutrino oscillation parameters $|\ensuremath{\Delta}{m}_{32}^{2}|=({2.3}_{\ensuremath{-}0.5}^{+0.6})\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}3}\text{ }\text{ }{\mathrm{eV}}^{2}$ and ${sin}^{2}(2{\ensuremath{\theta}}_{23})>0.93$, and maximum mixing is favored.

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: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.005
Threshold uncertainty score0.011

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0010.002
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0000.001
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 head0.012
GPT teacher head0.227
Teacher spread0.215 · 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 designObservational
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".

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Citations73
Published2013
Admission routes2
Has abstractyes

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