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Record W2027988287 · doi:10.1103/physrevd.86.022005

Search for ultrahigh-energy tau neutrinos with IceCube

2012· article· en· W2027988287 on OpenAlexaff
Y. Abdou, T. Abu-Zayyad, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, D. Altmann, K. Andeen, J. Auffenberg, X. Bai, M. D. Baker, S. W. Barwick, V. Baum, R. Bay, K. Beattie, J. J. Beatty, S. Bechet, J. K. Becker, K. H. Becker, M. Bell, M. L. Benabderrahmane, S. BenZvi, Jens Berdermann, P. Berghaus, D. Berley, E. Bernardini, Daniel Bertrand, D. Besson, D. Bindig, M. Bissok, E. Blaufuss, J. Blumenthal, D. J. Boersma, C. Böhm, D. Bose, S. Böser, O. Botner, L. Brayeur, A. M. Brown, S. Buitink, K. S. Caballero‐Mora, M. Carson, M. Casier, D. Chirkin, B. Christy, F. Clevermann, S. Cohen, D. F. Cowen, A. H. Cruz Silva, M. V. D’Agostino, M. Danninger, J. Daughhetee, J. C. Davis, C. De Clercq, T. Degner, F. Descamps, P. Desiati, G. de Vries‐Uiterweerd, T. DeYoung, J. C. Díaz–Vélez, J. Dreyer, J. P. Dumm, M. Dunkman, J. Eisch, R. W. Ellsworth, O. Engdegård, 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, T. K. Gaisser, J. S. Gallagher, L. Gerhardt, L. Gladstone, T. Glüsenkamp, A. Goldschmidt, J. A. Goodman, D. Góra, D. Grant, A. Groß, S. Grullon, M. Gurtner, C. Ha, A. Haj Ismail, A. Hallgren, F. Halzen, K. Hanson, D. Heereman, P. Heimann, D. Heinen, K. Helbing, R. Hellauer, S. Hickford, G. C. Hill, K. D. Hoffman, Benjamin D. Hoffmann, A. Homeier, K. Hoshina, W. Huelsnitz, P. O. Hulth, K. Hultqvist, Shahid Hussain, A. Ishihara, E. Jacobi, J. Jacobsen, G. S. Japaridze, Henrik Johansson, A. Kappes, T. Karg, A. Karle, J. Kiryluk, F. Kislat, J.-H. Köhne, G. Kohnen, H. Kolanoski, L. Köpke, S. Kopper, D. J. Koskinen, M. Kowalski, M. Krasberg, G. Kroll, J. Kunnen, N. Kurahashi, T. Kuwabara, M. Labare, K. Laihem, H. Landsman, M. J. Larson, R. Lauer, J. Lünemann, J. Madsen, R. Maruyama, K. Mase, H. S. Matis, K. Meagher, M. Merck, P. Mészáros, T. Meures, S. Miarecki, E. Middell, N. Milke, J. Miller, T. Montaruli, R. Morse, S. M. Movit, R. Nahnhauer, J. W. Nam, Uwe Naumann, Sarah Nowicki, D. R. Nygren, S. Odrowski, A. Olivas, M. Olivo, A. O’Murchadha, S. Panknin, L. Paul, C. Pérez de los Heros, D. Pieloth, J. Posselt, P. B. Price, G. T. Przybylski, K. Rawlins, P. Redl, E. Resconi, W. Rhode, M. Ribordy, M. Richman, Benedikt Riedel, J. P. Rodrigues, F. Rothmaier, C. Rott, T. Ruhe, D. Rutledge, B. Ruzybayev, D. Ryckbosch, H.‐G. Sander, M. Santander, S. Sarkar, K. Schatto, T. Schmidt, S. Schöneberg, A. Schönwald, A. Schukraft, L. Schulte, A. Schultes, O. Schulz, M. Schunck, D. Seckel, B. Semburg, H. Seo, Y. Sestayo, S. Seunarine, A. Silvestri, M. W. E. Smith, G. M. Spiczak, C. Spiering, M. Stamatikos, Todor Stanev, T. Stezelberger, R. G. Stokstad, A. Stößl, E. A. Strahler, L. R. Strom, M. Stüer, G. W. Sullivan, H. Taavola, I. Taboada, A. Tamburro, S. Ter–Antonyan, S. Tilav, P. A. Toale, S. Toscano, N. van Eijndhoven, A. Van Overloop, J. V. Santen, M. Vehring, M. Vöge, C. Walck, T. Waldenmaier, M. Wallraff, M. Walter, R. Wasserman, Ch. Weaver, C. Wendt, S. Westerhoff, N. Whitehorn, K. Wiebe, C. H. Wiebusch, D. R. Williams, R. Wischnewski, H. Wissing, M. Wolf, T. R. Wood, K. Woschnagg, C. Xu, D. L. Xu, Xiaolin Xu, G. Yodh, S. Yoshida, P. Zarzhitsky, M. Zoll

Bibliographic record

VenuePhysical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology · 2012
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of Alberta
FundersMarsden FundJapan Society for the Promotion of ScienceScience and Technology Facilities CouncilBundesministerium für Bildung und ForschungOffice of Polar ProgramsPolarforskningssekretariatetKnut och Alice Wallenbergs StiftelseDeutsche ForschungsgemeinschaftUniversity of Wisconsin-MadisonSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungU.S. Department of EnergyVetenskapsrådetNational Science Foundation
KeywordsNeutrinoPhysicsMuonNeutrino detectorRange (aeronautics)Particle physicsAstrophysicsEnergy (signal processing)Nuclear physicsAstronomyNeutrino oscillation

Abstract

fetched live from OpenAlex

The first dedicated search for ultrahigh-energy (UHE) tau neutrinos of astrophysical origin was performed using the IceCube detector in its 22-string configuration with an instrumented volume of roughly $0.25\text{ }\text{ }{\mathrm{km}}^{3}$. The search also had sensitivity to UHE electron and muon neutrinos. After application of all selection criteria to approximately 200 live-days of data, we expect a background of $0.60\ifmmode\pm\else\textpm\fi{}0.19(\mathrm{stat})\genfrac{}{}{0}{}{+0.56}{\ensuremath{-}0.58}(\mathrm{syst})$ events and observe three events, which after inspection, emerge as being compatible with background but are kept in the final sample. Therefore, we set an upper limit on neutrinos of all flavors from UHE astrophysical sources at 90% C.L. of ${E}_{\ensuremath{\nu}}^{2}{\ensuremath{\Phi}}_{90}({\ensuremath{\nu}}_{\mathrm{x}})<16.3\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}8}\text{ }\text{ }\mathrm{GeV}\text{ }{\mathrm{cm}}^{\ensuremath{-}2}\text{ }{\mathrm{sr}\text{ }}^{\ensuremath{-}1}\text{ }{\mathrm{s}}^{\ensuremath{-}1}$ over an estimated primary neutrino energy range of 340 TeV to 200 PeV.

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)0.001
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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.004
Threshold uncertainty score0.014

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.002
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0040.001

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 head0.020
GPT teacher head0.313
Teacher spread0.293 · 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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Citations32
Published2012
Admission routes1
Has abstractyes

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