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Record W4401250395 · doi:10.1103/physrevd.110.032003

New methods and simulations for cosmogenic induced spallation removal in Super-Kamiokande-IV

2024· article· en· W4401250395 on OpenAlexafffund
S. Locke, A. Coffani, K. Abe, C. Bronner, Y. Hayato, M. Ikeda, S. Imaizumi, Hiroshi Itô, J. Kameda, Y. Kataoka, M. Miura, S. Moriyama, Y. Nagao, M. Nakahata, Y. Nakajima, S. Nakayama, T. Okada, K. Okamoto, A. Orii, G. Pronost, H. Sekiya, M. Shiozawa, Y. Sonoda, Y. Suzuki, A. Takeda, Y. Takemoto, A. Takenaka, Hidekazu Tanaka, T. Yano, K. Hirade, Y. Kanemura, S. Miki, S. Watabe, S. Han, T. Kajita, K. Okumura, T. Tashiro, J. Xia, X. Wang, G. D. Megias, D. Bravo, L. Labarga, Ll. Marti, Bryan Zaldívar, B. W. Pointon, F. d. M. Blaszczyk, E. Kearns, J. L. Raaf, J. L. Stone, L. Wan, T. Wester, J. Bian, N. J. Griskevich, W. R. Kropp, S. Mine, M. B. Smy, H. W. Sobel, Volodymyr Takhistov, P. Weatherly, A. Yankelevich, J. Hill, J. Y. Kim, I. T. Lim, R. G. Park, B. Bodur, K. Scholberg, C. W. Walter, L. Bernard, O. Drapier, S. El Hedri, A. Giampaolo, M. Gonin, Th. A. Mueller, Pascal Paganini, B. Quilain, A. D. Santos, T. Ishizuka, T. Nakamura, J. S. Jang, J. G. Learned, L. H. V. Anthony, A. A. Sztuc, Y. Uchida, D. Martin, M. Scott, V. Berardi, J. Chakrani, E. Radicioni, N. F. Calabria, L. N. Machado, G. De Rosa, G. Collazuol, F. Iacob, M. Lamoureux, N. Ospina, M. Mattiazzi, L. Ludovici, Y. Nishimura, Y. Maewaka, S. Cao, M. Friend, T. Hasegawa, T. Ishida, T. Kobayashi, M. Jakkapu, T. Nakadaira, K. Nakamura, Y. Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, Y. Nakano, T. Shiozawa, Atsumu Suzuki, Y. Takeuchi, S. Yamamoto, Y. Kotsar, H. Ozaki, A. Ali, Yosuke Ashida, J. Feng, S. Hirota, A. K. Ichikawa, T. Kikawa, M. Mori, T. Nakaya, R. A. Wendell, P. Fernández, N. McCauley, P. Mehta, K. M. Tsui, Y. Fukuda, Y. Itow, H. Menjo, T. Niwa, K. Sato, M Tsukada, P. Mijakowski, J. Łagoda, S. M. Lakshmi, J. Zalipska, C. K. Jung, C. Vilela, Alexander S. Wilkinson, C. Yanagisawa, J. Jiang, Katsuro Hagiwara, Masayuki Harada, T. Horai, H. Ishino, S. Ito, Y. Koshio, W. Y., N. Piplani, S. Sakai, H. Kitagawa, G. Barr, D. Barrow, L. Cook, A. Goldsack, S. Samani, D. Wark, F. Nova, T. Boschi, F. Di Lodovico, M. Taani, S. Zsoldos, J. Gao, J. Migenda, J. Yang, S. J. Jenkins, M. Malek, J. M. McElwee, O. Stone, M. D. Thiesse, L.F. Thompson, H. Okazawa, S. B. Kim, I. Yu, J. W. Seo, K. Nishijima, M. Koshiba, K. Iwamoto, N. Ogawa, M. Yokoyama, K. Martens, M. R. Vagins, K. Nakagiri, M. Kuze, S. Izumiyama, T. Yoshida, M. Inomoto, M. Ishitsuka, R. Matsumoto, K. Ohta, M. Shinoki, T. Suganuma, T. Kinoshita, J.F. Martin, H. A. Tanaka, T. Towstego, R. Akutsu, M. Hartz, A. Konaka, P. de Perio, N. W. Prouse, Shaomin Chen, Benda Xu, Yang Zhang, M. Posiadała-Zezula, B. Richards, B. Jamieson, J. Walker, A. Minamino, G. Pintaudi, R. Sasaki

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicNeutrino Physics Research
Canadian institutionsUniversity of WinnipegBritish Columbia Institute of TechnologyUniversity of Toronto
FundersHORIZON EUROPE Marie Sklodowska-Curie ActionsJapan Society for the Promotion of ScienceNarodowe Centrum NaukiMinisterio de Ciencia e InnovaciónMinistry of Education, Culture, Sports, Science and TechnologyKerman Neuroscience Research Center, Kerman University of Medical SciencesScience and Technology Facilities CouncilNational Research FoundationNatural Sciences and Engineering Research Council of CanadaU.S. Department of EnergyEuropean CommissionNational Natural Science Foundation of ChinaNational Science FoundationCompute CanadaNational Research Foundation of Korea
KeywordsSpallationNeutrinoPhysicsMuonNuclear physicsHadronCosmic raySpallation Neutron SourceCherenkov detectorNeutrino detectorNeutronParticle physicsCherenkov radiationDetectorNeutrino oscillationOptics

Abstract

fetched live from OpenAlex

Radioactivity induced by cosmic muon spallation is a dominant source of backgrounds for O ( 10 MeV ) neutrino interactions in water Cherenkov detectors. In particular, it is crucial to reduce backgrounds to measure the solar neutrino spectrum and find neutrino interactions from distant supernovae. In this paper we introduce new techniques to locate muon-induced hadronic showers and efficiently reject spallation backgrounds. Applying these techniques to the solar neutrino analysis with an exposure of 2790 × 22.5 kton · day increases the signal efficiency by 12.6%, approximately corresponding to an additional year of detector running. Furthermore, we present the first spallation simulation at Super-Kamiokande, where we model hadronic interactions using . The agreement between the isotope yields and shower pattern in this simulation and in the data gives confidence in the accuracy of this simulation, and thus opens the door to use it to optimize muon spallation removal in new data with gadolinium-enhanced neutron capture detection. Published by the American Physical Society 2024

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)0.003
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: Methods · Consensus signal: Methods
Teacher disagreement score0.024
Threshold uncertainty score0.048

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.003
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.001
Science and technology studies0.0010.001
Scholarly communication0.0010.001
Open science0.0020.001
Research integrity0.0020.001
Insufficient payload (model declined to judge)0.0080.001

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 head0.058
GPT teacher head0.546
Teacher spread0.488 · 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
GenreMethods

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

Citations8
Published2024
Admission routes2
Has abstractyes

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