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Record W2215475931 · doi:10.1103/physrevd.87.012001

T2K neutrino flux prediction

2013· article· en· W2215475931 on OpenAlexafffund
K. Abe, N. Abgrall, H. Aihara, T. Akiri, J. B. Albert, C. Andreopoulos, S. Aoki, A. Ariga, T. Ariga, S. Assylbekov, D. Autiero, M. Barbi, Gareth J. Barker, G. Barr, M. Bass, M. Batkiewicz, F. Bay, S. W. Bentham, V. Berardi, B. E. Berger, S. Berkman, I. A. Bertram, Dmitriy Beznosko, S. Bhadra, F. d. M. Blaszczyk, A. Blondel, C. Bojechko, S. B. Boyd, A. Bravar, C. Bronner, D. G. Brook-Roberge, N. J. Buchanan, R. G. Calland, S. L. Cartwright, R. Castillo, M. G. Catanesi, A. Cervera, D. Cherdack, G. Christodoulou, A. Clifton, J. P. Coleman, S. J. Coleman, G. Collazuol, K. Connolly, A. Curioni, A. Dąbrowska, I. Dankó, R. Das, S. Davis, M. Day, J. P. A. M. de André, P. de Perio, G. De Rosa, T. Dealtry, C. Densham, F. Di Lodovico, S. Di Luise, J. E. Y. Dobson, T. Duboyski, F. Dufour, J. Dumarchez, S. Dytman, M. Dziewiecki, M. Dziomba, S. Emery, A. Ereditato, L. S. Esposito, A.J. Finch, E.D. Frank, M. Friend, Y. Fujii, Y. Fukuda, V. Galymov, A. Gaudin, S. Giffin, C. Giganti, K. Gilje, T. Golan, J.J. Gómez-Cadenas, M. Gonin, N. Grant, D. Gudin, P. Guzowski, D. R. Hadley, A. Haesler, Martin Haigh, D. Hansen, T. Hara, M. Hartz, T. Hasegawa, N. C. Hastings, Y. Hayato, C. Hearty, R. L. Helmer, J. Hignight, A. Hillairet, A. Himmel, T. Hiraki, J. Holeczek, Shin Horikawa, K. Huang, A. Hyndman, A. K. Ichikawa, K. Ieki, M. Ieva, M. Ikeda, J. Imber, J. Insler, Toru Ishida, T. Ishii, S. J. Ives, K. Iyogi, A. Izmaylov, B. Jamieson, R. A. Johnson, J. H. Jo, P. Jonsson, K. K. Joo, G. Jover-Mañas, C. K. Jung, H. Kaji, T. Kajita, H. Kakuno, J. Kameda, Y. Kanazawa, D. Karlen, I. Karpikov, E. Kearns, M. Khabibullin, F. Khanam, A. Khotjantsev, D. Kiełczewska, T. Kikawa, A. Kilinski, J. Y. Kim, J. Kim, S. B. Kim, B. Kirby, J. Kisiel, P. Kitching, T. Kobayashi, G. Kogan, A. Konaka, L. L. Kormos, A. Korzenev, K. Koseki, Y. Koshio, K. Kowalik, I. Kreslo, W. Kropp, H. Kubo, Y. Kudenko, S. Kumaratunga, R. Kurjata, T. Kutter, J. Łagoda, K. Laihem, A. Laing, M. Laveder, M. Lawe, K. P. Lee, C. Licciardi, I. T. Lim, T. Lindner, C. Lister, R. P. Litchfield, A. Longhin, G. Lopez, L. Ludovici, M. Macaire, L. Magaletti, K. Mahn, M. Malek, S. Manly, A. Marchionni, A. D. Marino, J. Marteau, T. Maruyama, J. Marzec, P. Masliah, E. L. Mathie, C. Matsumura, K. Matsuoka, V. Matveev, K. Mavrokoridis, E. Mazzucato, N. McCauley, K. S. McFarland, C. McGrew, T. C. Mclachlan, M. Messina, C. Metelko, M. Mezzetto, P. Mijakowski, C. A. Miller, A. Minamino, O. Mineev, S. Mine, A. Missert, M. Miura, L. Monfregola, S. Moriyama, Th. A. Mueller, A. Murakami, M. Murdoch, S. Murphy, J. Myslik, Takanori Nagasaki, T. Nakadaira, M. Nakahata, T. Nakai, K. Nakajima, K. Nakamura, S. Nakayama, T. Nakaya, K. Nakayoshi, D. Naples, T.C. Nicholls, C. Nielsen, K. Nishikawa, Y. Nishimura, H. M. O’Keeffe, Y. Obayashi, R. Ohta, K. Okumura, W. Oryszczak, S. M. Oser, M. Otani, R. A. Owen, Y. Oyama, M. Y. Pac, V. Palladino, V. Paolone, D. Payne, G.F. Pearce, O. Perevozchikov, J.D. Perkin, E. S. Pinzon Guerra, P. Płoński, E. Poplawska, B. Popov, M. Posiadała-Zezula, J.-M. Poutissou, R. Poutissou, P. Przewłocki, B. Quilain, E. Radicioni, P. N. Ratoff, M. Ravonel, M. A. Rayner, Mark E. Reeves, E. Reinherz-Aronis, F. Retière, P. A. Rodrigues, E. Rondio, B. Rossi, S. Roth, A. Rubbia, D. Ruterbories, R. Sacco, K. Sakashita, F. Sánchez, E. Scantamburlo, K. Scholberg, J. Schwehr, M. Scott, D. I. Scully, Y. Seiya, T. Sekiguchi, H. Sekiya, M. Shibata, M. Shiozawa, S. Short, Y. Shustrov, P. Sinclair, B. Smith, R. J. E. Smith, M. Smy, J. T. Sobczyk, H. Sobel, M. Sorel, L. Southwell, P. Stamoulis, J. Steinmann, B. Still, R. Sulej, Y. Suzuki, K. Suzuki, S. Suzuki, T. Szegłowski, M. Szeptycka, R. Tacik, M. Tada, Sentaro Takahashi, A. Takeda, Y. Takeuchi, H. A. Tanaka, M. Tanaka, Ian Taylor, D. Terhorst, R. Terri, L.F. Thompson, A. Thorley, S. Tobayama, W. H. Toki, T. Tomura, Y. Totsuka, C. Touramanis, T. Tsukamoto, M. Tzanov, Y. Uchida, K. Ueno, A. Vacheret, M. R. Vagins, G. Vasseur, T. Wąchała, A. V. Waldron, C. W. Walter, J. Wang, D. Wark, M. O. Wascko, A. Weber, R. Wendell, G. Wikström, R. J. Wilkes, M. J. Wilking, C. Wilkinson, Z. Williamson, J. R. Wilson, R. J. Wilson, T. Wongjirad, Y. Yamada, K. Yamamoto, C. Yanagisawa, T. Yano, S. Yen, N. Yershov, M. Yokoyama, T. Yuan, A. Zalewska, L. Zambelli, К. Заремба, M. Ziembicki, E. D. Zimmerman, M. Zito, J. Żmuda

Bibliographic record

VenuePhysical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology · 2013
Typearticle
Languageen
FieldPhysics and Astronomy
TopicNeutrino Physics Research
Canadian institutionsInstitute of Particle PhysicsUniversity of AlbertaTRIUMFUniversity of ReginaUniversity of VictoriaUniversity of WinnipegUniversity of TorontoYork UniversityUniversity of British Columbia
FundersInstitut National de Physique Nucléaire et de Physique des ParticulesDeutsches Elektronen-SynchrotronScience and Technology Facilities CouncilCentre National de la Recherche ScientifiqueMinistry of Education, Culture, Sports, Science and TechnologyMinistry of Education and Science of the Russian FederationJapan Society for the Promotion of ScienceRussian Foundation for Basic ResearchCERNDeutsche ForschungsgemeinschaftNatural Sciences and Engineering Research Council of CanadaAlfred P. Sloan FoundationSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungU.S. Department of EnergyJapan Proton Accelerator Research ComplexMinisterio de Ciencia e InnovaciónNarodowym Centrum NaukiNational Science Foundation
KeywordsNeutrinoFlux (metallurgy)PhysicsNuclear physicsParticle physicsEnvironmental scienceMaterials science

Abstract

fetched live from OpenAlex

The Tokai-to-Kamioka (T2K) experiment studies neutrino oscillations using an off-axis muon neutrino beam with a peak energy of about 0.6 GeV that originates at the Japan Proton Accelerator Research Complex accelerator facility. Interactions of the neutrinos are observed at near detectors placed at 280 m from the production target and at the far detector---Super-Kamiokande---located 295 km away. The flux prediction is an essential part of the successful prediction of neutrino interaction rates at the T2K detectors and is an important input to T2K neutrino oscillation and cross section measurements. A FLUKA and GEANT3-based simulation models the physical processes involved in the neutrino production, from the interaction of primary beam protons in the T2K target, to the decay of hadrons and muons that produce neutrinos. The simulation uses proton beam monitor measurements as inputs. The modeling of hadronic interactions is reweighted using thin target hadron production data, including recent charged pion and kaon measurements from the NA61/SHINE experiment. For the first T2K analyses the uncertainties on the flux prediction are evaluated to be below 15% near the flux peak. The uncertainty on the ratio of the flux predictions at the far and near detectors is less than 2% near the flux peak.

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)0.002
metaresearch head score (Gemma)0.004
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: Simulation or modeling
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.009
Threshold uncertainty score0.021

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.004
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0020.002
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0060.005

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 head0.024
GPT teacher head0.337
Teacher spread0.313 · 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".

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Citations231
Published2013
Admission routes2
Has abstractyes

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Same venuePhysical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmologySame topicNeutrino Physics ResearchFrench-language works237,207