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Development of an analysis to probe the neutrino mass ordering with atmospheric neutrinos using three years of IceCube DeepCore data

2020· article· en· W2997107489 on OpenAlexafffund
M. G. Aartsen, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, Cyril Martin Alispach, K. Andeen, T. Anderson, I. Ansseau, G. Anton, C. Argüelles, J. Auffenberg, Spencer Axani, Paul Backes, H. Bagherpour, X. Bai, Anastasia Maria Barbano, S. W. Barwick, V. Baum, R. Bay, J. J. Beatty, K. H. Becker, J. Becker Tjus, S. BenZvi, D. Berley, E. Bernardini, D. Besson, G. Binder, D. Bindig, E. Blaufuss, Summer Blot, C. Böhm, M. Börner, S. Böser, O. Botner, Etienne Bourbeau, J. Bourbeau, Federica Bradascio, J. Braun, H.-P. Bretz, S. Bron, Jannes Brostean-Kaiser, A. Burgman, Raffaela Busse, T. Carver, Kunal Deoskar, E. Cheung, D. Chirkin, K. Clark, Lew Classen, G. H. Collin, J. M. Conrad, Paul Coppin, Pablo Correa, D. F. Cowen, R. Cross, Pranav Dave, J. P. A. M. de André, C. De Clercq, James DeLaunay, H.-P. Dembinski, S. De Ridder, P. Desiati, K. D. de Vries, G. de Wasseige, M. de With, T. DeYoung, A. F. Díaz, J. C. Díaz–Vélez, Hrvoje Dujmović, M. Dunkman, Emily Dvorak, B. Eberhardt, Thomas Ehrhardt, B. Eichmann, P. Eller, J. J. Evans, P. A. Evenson, S. Fahey, A. R. Fazely, J. Felde, K. Filimonov, C. Finley, A. Franckowiak, Edward Friedman, Alexander Fritz, T. K. Gaisser, J. S. Gallagher, Erik Ganster, S. Garrappa, L. Gerhardt, K. Ghorbani, Theo Glauch, T. Glüsenkamp, A. Goldschmidt, J. G. González, D. Grant, Z. Griffith, M. Günder, Mehmet Gündüz, Christian Haack, A. Hallgren, L. Halve, F. Halzen, K. Hanson, D. Hebecker, D. Heereman, K. Helbing, R. Hellauer, Felix Henningsen, S. Hickford, J. Hignight, G. C. Hill, K. D. Hoffman, R. Hoffmann, Tobias Hoinka, Benjamin Hokanson-Fasig, K. Hoshina, F. Huang, M. E. Huber, K. Hultqvist, Mirco Hünnefeld, Raamis Hussain, S. In, N. Iovine, A. Ishihara, E. Jacobi, G. S. Japaridze, Minjin Jeong, K. Jero, B. J. P. Jones, Woosik Kang, A. Kappes, David Kappesser, T. Karg, Martina Karl, A. Karle, U. Katz, M. Kauer, J. L. Kelley, Ali Kheirandish, J. Kim, T. Kintscher, J. Kiryluk, T. Kittler, Ramesh Koirala, H. Kolanoski, L. Köpke, Claudio Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, K. Krings, G. Krückl, N. Kulacz, S. Kunwar, N. Kurahashi, A. Kyriacou, M. Labare, J. L. Lanfranchi, M. J. Larson, Frederik Hermann Lauber, Jeffrey Lazar, M. Leuermann, Qinrui Liu, Elisa Lohfink, L. Lu, Francesco Lucarelli, J. Lünemann, William Luszczak, J. Madsen, G. Maggi, K. B. M. Mahn, Yuya Makino, K. Mallot, Sarah Mancina, Ioana Codrina Mariş, R. Maruyama, K. Mase, R. Maunu, K. Meagher, M. Medici, Andrés Medina, Maximilian Meier, S. Meighen-Berger, T. Menne, G. Merino, T. Meures, S. Miarecki, Jessie Micallef, G. Momenté, T. Montaruli, R. W. Moore, Marjon Moulai, R. Nagai, R. Nahnhauer, P. Nakarmi, Uwe Naumann, G. Neer, Hans Niederhausen, Sarah Nowicki, D. R. Nygren, A. Obertacke Pollmann, A. Olivas, A. O’Murchadha, Erin O’Sullivan, T. Palczewski, Hershal Pandya, D. V. Pankova, N. Park, P. Peiffer, C. Pérez de los Heros, D. Pieloth, E. Pinat, A. Pizzuto, M. Plum, P. B. Price, G. T. Przybylski, Christoph Raab, Amirreza Raissi, M. Rameez, L. Rauch, K. Rawlins, I. C. Rea, R. Reimann, B. Relethford, Giovanni Renzi, E. Resconi, W. Rhode, M. Richman, S. Robertson, Martin Rongen, C. Rott, T. Ruhe, D. Ryckbosch, D. Rysewyk, I. Safa, S. E. Sanchez Herrera, Alexander Sandrock, J. Sandroos, M. Santander, S. Sarkar, K. Satalecka, M. Schaufel, P. Schlunder, T. Schmidt, A. Schneider, J. Schneider, L. Schumacher, S. Sclafani, D. Seckel, S. Seunarine, M. Silva, R. Snihur, Jan Soedingrekso, D. Soldin, S. Söldner‐Rembold, M. Song, G. M. Spiczak, Christian Spiering, Juliana Stachurska, M. Stamatikos, T. Stanev, A. Stasik, Robert Stein, J. Stettner, A. Steuer, T. Stezelberger, R. G. Stokstad, A. Stößl, N. L. Strotjohann, Thomas Stuttard, G. W. Sullivan, M. Sutherland, I. Taboada, F. Tenholt, S. Ter–Antonyan, A. Terliuk, S. Tilav, L. Tomankova, Christoph Tönnis, S. Toscano, D. Tosi, M. Tselengidou, C. F. Tung, A. Turcati, R. Turcotte, Colin Turley, B. Ty, E. Unger, Martin Unland Elorrieta, M. Usner, J. Vandenbroucke, W. Van Driessche, D. van Eijk, N. van Eijndhoven, S. Vanheule, J. V. Santen, M. Vraeghe, C. Walck, A. Wallace, M. Wallraff, N. Wandkowsky, T. B. Watson, C. Weaver, M. J. Weiss, J. Weldert, Chris Wendt, Johannes Werthebach, S. Westerhoff, B. J. Whelan, N. Whitehorn, K. Wiebe, C. H. Wiebusch, L. Wille, D. R. Williams, L. Wills, Martin Wolf, J. Wood, T. R. Wood, K. Woschnagg, G. Wrede, Steven Wren, Dawei Xu, Xiaolin Xu, Y. Xu, G. Yodh, S. Yoshida, Tiantian Yuan

Bibliographic record

VenueThe European Physical Journal C · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of AlbertaSnolab
FundersJapan Society for the Promotion of ScienceDeutsches Elektronen-SynchrotronScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaOffice of Polar ProgramsCollege of Engineering, Michigan State UniversityInstitute for Global Prominent Research, Chiba UniversityRWTH Aachen UniversityChiba UniversityKnut och Alice Wallenbergs StiftelseVillum FondenNational Research Foundation of KoreaFonds Wetenschappelijk OnderzoekMarsden FundBundesministerium für Bildung und ForschungHelmholtz Alliance for Astroparticle PhysicsDanmarks GrundforskningsfondNational Science FoundationBelgian Federal Science Policy OfficeDeutsche ForschungsgemeinschaftMichigan State UniversityNational Research FoundationWestern Canada Research GridFonds De La Recherche Scientifique - FNRSPolarforskningssekretariatetCompute CanadaMarquette UniversityUniversity of Wisconsin-MadisonU.S. Department of EnergyVetenskapsrådet
KeywordsNeutrinoPhysicsParticle physicsAstronomyAstrophysics

Abstract

fetched live from OpenAlex

Abstract The Neutrino Mass Ordering (NMO) remains one of the outstanding questions in the field of neutrino physics. One strategy to measure the NMO is to observe matter effects in the oscillation pattern of atmospheric neutrinos above $$\sim 1\,\mathrm {GeV}$$ ∼1GeV , as proposed for several next-generation neutrino experiments. Moreover, the existing IceCube DeepCore detector can already explore this type of measurement. We present the development and application of two independent analyses to search for the signature of the NMO with three years of DeepCore data. These analyses include a full treatment of systematic uncertainties and a statistically-rigorous method to determine the significance for the NMO from a fit to the data. Both analyses show that the dataset is fully compatible with both mass orderings. For the more sensitive analysis, we observe a preference for normal ordering with a p-value of $$p_\mathrm {IO} = 15.3\%$$ pIO=15.3% and $$\mathrm {CL}_\mathrm {s}=53.3\%$$ CLs=53.3% for the inverted ordering hypothesis, while the experimental results from both analyses are consistent within their uncertainties. Since the result is independent of the value of $$\delta _\mathrm {CP}$$ δCP and obtained from energies $$E_\nu \gtrsim 5\,\mathrm {GeV}$$ Eν≳5GeV , it is complementary to recent results from long-baseline experiments. These analyses set the groundwork for the future of this measurement with more capable detectors, such as the IceCube Upgrade and the proposed PINGU detector.

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)0.009
metaresearch head score (Gemma)0.012
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: none
GenreCandidate signal: Methods · Consensus signal: none
Teacher disagreement score0.022
Threshold uncertainty score0.049

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0090.012
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.002
Bibliometrics0.0030.002
Science and technology studies0.0010.001
Scholarly communication0.0020.001
Open science0.0020.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0010.000

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 head0.034
GPT teacher head0.246
Teacher spread0.212 · 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".

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Citations22
Published2020
Admission routes2
Has abstractyes

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Same venueThe European Physical Journal CSame topicAstrophysics and Cosmic PhenomenaFrench-language works237,207