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Record W4415444545 · doi:10.1038/s41586-025-09599-3

Joint neutrino oscillation analysis from the T2K and NOvA experiments

2025· article· en· W4415444545 on OpenAlexafffund
S. Abubakar, M. A. Acero, B. S. Acharya, P. Adamson, Н. Анфимов, A. Antoshkin, E. Arrieta-Diaz, L. Asquith, A. Aurisano, Daniela Azevedo, H.O. Back, N. Balashov, Pierre Baldi, Bindu A. Bambah, E. F. Bannister, A. Barros, A. Baty, K. Bays, R. Bernstein, T. J. C. Bezerra, V. Bhatnagar, B. Bhuyan, J. Bian, A. C. Booth, R. Bowles, B. Brahma, C. Bromberg, N. Buchanan, A. Butkevich, S. Calvez, J. M. Carceller, T. J. Carroll, E. Catano-Mur, J. P. Cesar, R. Chirco, B. C. Choudhary, A. Christensen, M. F. Cicala, T. E. Coan, T. Contreras, A. Cooleybeck, D. Coveyou, L. Cremonesi, G. S. Davies, P. F. Derwent, P. F. Ding, K. Duffy, Kerry Dobbs, M. Dolce, D. Dueñas Tonguino, E. C. Dukes, A. Dye, R. Ehrlich, Erin Ewart, P. Filip, M. J. Frank, H. Gallagher, A. Giri, R. A. Gomes, H. Gómez, A. Habig, F. Hakl, J. Hartnell, Robert Hatcher, J. M. Hays, M. He, K. Heller, V. Hewes, A. Himmel, Tyler Horoho, A. Ivanova, B. Jargowsky, I. Kakorin, A. Kalitkina, D. M. Kaplan, A. Khanam, Burcu Kirezli, J. Kleykamp, O. Klimov, L. W. Koerner, L. Kolupaeva, R. Kralik, A. Kumar, C. D. Kuruppu, V. Kus, T. Lackey, K. Lang, P. Lasorak, J. Lesmeister, A. Lister, Jinzhi Liu, James A. Lock, M. MacMahon, S. Magill, W. A. Mann, M. T. Manoharan, M. Manrique Plata, M. L. Marshak, M. Martinez-Casales, V. Matveev, B. Mehta, M. D. Messier, H. Meyer, T. Miao, W. H. Miller, S. R. Mishra, R. Mohanta, A. Moren, A. Morozova, W. Mu, L. Mualem, M. Muether, K. Mulder, D. MYERS, D. Naples, S. Nelleri, J. K. Nelson, R. Nichol, E. Niner, A. Norman, A. Norrick, H. Oh, A. Olshevskiy, T. Olson, Mustafa Ozkaynak, A. Pal, J. Paley, L. Panda, R. B. Patterson, Greg Pawloski, R. Petti, R. Plunkett, Joshua Porter, L. R. Prais, A. Rafique, V. Raj, M. Rajaoalisoa, B. Ramson, B. Rebel, Elias Robles, P. Roy, O. Samoylov, M. C. Sánchez, S. Sánchez Falero, P. Shanahan, P. Sharma, A. Sheshukov, А. Н. Шмаков, W. Shorrock, S. Shukla, I. Singh, P. Singh, V. Singh, S. S. Chhibra, Dinesh Kumar Singha, A. Smith, J. Smolík, P. Snopok, N. Solomey, A. Sousa, K. Soustružnı́k, M. Strait, L. Suter, A. Sutton, S. K. Swain, C. Sweeney, A. A. Sztuc, N. Talukdar, P. Tas, T. Thakore, J. Thomas, E. Tiras, Michael S. Titus, Y. Torun, Daniel Tran, J. Trokan-Tenorio, J. Urheim, P. Vahle, Z. Vallari, K. J. Vockerodt, A. V. Waldron, M. Wallbank, T. K. Warburton, Carl Maria von Weber, M. Wetstein, D. Whittington, D. A. Wickremasinghe, J. Wolcott, W. Wu, Y. Xiao, B. Yaeggy, A. Yahaya, A. Yankelevich, K. Yonehara, S. Zadorozhnyy, J. Zalesak, R. Zwaska, K. Abe, S. Abe, H. Adhkary, R. Akutsu, H. Alarakia-Charles, Y. I. Alj Hakim, S. Alonso Monsalve, L. Anthony, S. Aoki, K. A. Apte, T. Arai, T. Arihara, S. Arimoto, Y. Ashida, E. T. Atkin, N. Kishore Babu, V. A. Baranov, Gareth J. Barker, G. Barr, Daniel L. Barrow, Paul Bates, L. Bathe-Peters, M. Batkiewicz, N. Baudis, V. Berardi, L. Berns, S. Bhattacharjee, Adrien Blanchet, A. Blondel, P. M. M. Boistier, S. Bolognesi, S. Bordoni, S. B. Boyd, C. Bronner, A. Bubak, M. Buizza Avanzini, J. A. Caballero, F. Cadoux, N. F. Calabria, S. Cao, S. Cap, D. Carabadjac, S. L. Cartwright, M. P. Casado, M. G. Catanesi, J. Chakrani, Anne Chalumeau, D. Cherdack, A. Chvirova, J. P. Coleman, G. Collazuol, F Cormier, A. A. L. Craplet, A. Cudd, D. D’Ago, C. Dalmazzone, T. Daret, Prokar Dasgupta, C. L. Davis, Yu. I. Davydov, P de Perio, G. De Rosa, T. Dealtry, Christopher Densham, A. Dergacheva, Rajat Banerjee, F. Di Lodovico, G. Lopez, S. Dolan, D. Douqa, T. A. Doyle, O. Drapier, K. E. Duffy, J. Dumarchez, P. Dunne, K. Dygnarowicz, A. Eguchi, J. E. Elias, S. Emery-Schrenk, G. Erofeev, A. Ershova, G. Eurin, D. Fedorova, S. Fedotov, M. Feltre, L. Feng, D. Ferlewicz, A.J. Finch, M. D. Fitton, C. Forza, M. Friend, Y. Fujii, Y. Furui, J. García-Marcos, A. C. Germer, L. Giannessi, C. Giganti, M Girgus, V. Glagolev, M. Gonin, R. González-Jiménez, J. González Rosa, E. A. G. Goodman, K. Gorshanov, P. Govindaraj, Marco Grassi, M. Guigue, Flynn Guo, S. Han, Deborah A. Harris, Robert J. Harris, T. Hasegawa, Ciaran Hasnip, S. Hassani, N. C. Hastings, Y. Hayato, I. Heitkamp, D. Henaff, Y. Hino, J. Holeczek, A. Holin, T. Holvey, N. T. Hong Van, Takashi Honjo, M. C. F. Hooft, K. Hosokawa, Jun Hu, A. K. Ichikawa, K. Ieki, M. Ikeda, T. Ishida, M. Ishitsuka, A. Izmaylov, N. Jachowicz, S. J. Jenkins, C. Jesús-Valls, Meng Jia, Jing Jiang, Julie Y. Ji, Thomas Peter Jones, P. Jonsson, S.C. Joshi, C. K. Jung, M. Kabirnezhad, A. C. Kaboth, H. Kakuno, J. Kameda, S. Karpova, V. S. Kasturi, Y. Kataoka, T. Katori, Yuta Kawamura, M. Kawaue, E. Kearns, M. Khabibullin, A. Khotjantsev, S. King, V. Kiseeva, John B. Kisiel, A. Klustová, L. Kneale, H. Kobayashi, L. Koch, S. Kodama, M. Kolupanova, A. Konaka, L. L. Kormos, Y. Koshio, K. Kowalik, Y. Kudenko, Y. Kudo, A. Kumar Jha, R. Kurjata, V. Kurochka, T. Kutter, L. Labarga, Mário Lachat, K. Lachner, J. Lagoda, S. M. Lakshmi, M. Lamers James, A. Langella, David Langridge, J. F. Laporte, D. Last, N Latham, M. Laveder, L. Lavitola, M. Lawe, D. Leon Silverio, S. Levorato, S. Lewis, Botao Li, C. Lin, R. P. Litchfield, S. L. Liu, W. Li, A. Longhin, A. Lopez Moreno, L Ludovici, X.-G. Lu, T. Lux, L. N. Machado, L. Magaletti, Kendall Mahn, K. K. Mahtani, M. Mandal, S. Manly, A. D. Marino, D. Martin, D. A. Martínez Caicedo, Lluisa Maria Mir Martinez, M. Martini, T. Matsubara, R. Matsumoto, C. Mauger, K. Mavrokoridis, N. McCauley, K. S. McFarland, C. McGrew, J. P. McKean, A. Mefodiev, G. D. Megias, Lucile Mellet, C. Metelko, M. Mezzetto, S. Miki, V. Mikola, E. W. Miller, O. Mineev, S. Mine, J. Mirabito, M. Miura, S. Moriyama, P. Morrison, Th. A. Mueller, D. Munford, Alfonso Muñoz, L. Munteanu, Y. Nagai, T. Nakadaira, K. Nakagiri, Y. Nakajima, K. Nakamura, Y. Nakano, S. Nakayama, T. Nakaya, K. Nakayoshi, C. E. R. Naseby, Doan Trang Nguyen, V.Q Nguyen, K. Niewczas, S Nishimori, Y. Nishimura, Yuji Noguchi, T. Nosek, F. Nova, J. C. Nugent, H. M. O’Keeffe, L. O’Sullivan, Ryuji Okazaki, W. Okinaga, K. Okumura, T. Okusawa, Nobuhiko Onda, N. Ospina, L. Osu, Y. Oyama, V. Paolone, J. Pasternak, D. Payne, Tim Peacock, Michael Pfaff, L. Pickering, B. Popov, A. J. Portocarrero Yrey, M. Posiadała-Zezula, Y. S. Prabhu, Hari Prasad, F. Pupilli, B. Quilain, P. T. Quyen, E. Radicioni, B. Radics, M. A. Ramírez, Richard Ramsden, P. N. Ratoff, M. Reh, G. Anthony Reina, C. Riccio, D. Riley, E. Rondio, S. Roth, N. Roy, A. Rubbia, L. Russo, A. Rychter, W. Saenz, K. Sakashita, S. Samani, F. Sánchez, W. Sands, Yoshiki J. Sato, T. Schefke, C. M. Schloesser, K. Scholberg, M. Scott, Y. Seiya, T. Sekiguchi, H. Sekiya, T. Sekiya, D. Seppala, D. Sgalaberna, A. Shaikhiev, M. Shiozawa, Y. Shiraishi, A. Shvartsman, N. Skrobova, K. Skwarczynski, D. Smyczek, M. Smy, J. T. Sobczyk, H. Sobel, A. J. Speers, R. Spina, Ajit M. Srivastava, Y. Stroke, I. A. Suslov, A. Suzuki, S. Y. Suzuki, M. Tada, S. Tairafune, A. Takeda, A. Teklu, Y. Takeuchi, H. Tanigawa, V.V. Tereshchenko, N. Thamm, C. Touramanis, N. Tran, T. Tsukamoto, M. Tzanov, Y. Uchida, M. R. Vagins, M Varghese, I.I. Vasilyev, G. Vasseur, E. Villa, U. Virginet, T. Vladisavljevic, T. Wachala, Daisuke Wakabayashi, H. T. Wallace, J. Walsh, L. Wan, D. Wark, M. O. Wascko, A. Weber, R. Wendell, Michael Wilking, C. Wilkinson, J. R. Wilson, K. Wood, C. Wret, Jingkai Xia, K. Yamamoto, Tokonatsu Yamamoto, C. Yanagisawa, Y. F. Yang, T. Yano, N. Yershov, U. Yevarouskaya, M. Yokoyama, Y Yoshimoto, Nagamitsu Yoshimura, R. Zaki, A. Zalewska, J. Zalipska, G. Zarnecki, J. Zhang, Xingyu Zhao, H. Zheng, H. Zhong, Taiyu Zhu, M. Ziembicki, E. D. Zimmerman, M. Zito, Hirotaka Ito

Bibliographic record

VenueNature · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicNeutrino Physics Research
Canadian institutionsUniversity of British ColumbiaYork UniversityTRIUMF
FundersEuropean Regional Development FundAgència de Gestió d'Ajuts Universitaris i de RecercaNatural Sciences and Engineering Research Council of CanadaInstitut National de Physique Nucléaire et de Physique des ParticulesScience and Technology Facilities CouncilHorizon 2020 Framework ProgrammeOffice of ScienceNemzeti Kutatási Fejlesztési és Innovációs HivatalInstitute for Cosmic Ray Research, University of TokyoCentre National de la Recherche ScientifiqueChina Scholarship CouncilJapan Society for the Promotion of ScienceConselho Nacional de Desenvolvimento Científico e TecnológicoEuropean CommissionMinisterio de Ciencia e InnovaciónSorbonne UniversitéGeneralitat de CatalunyaRussian Foundation for Basic ResearchRussian Science FoundationMinistry of Education, Culture, Sports, Science and TechnologyFermilabNational Science FoundationUniversity of MinnesotaUK Research and InnovationDeutsches Elektronen-SynchrotronNational Energy Research Scientific Computing CenterDeutsche ForschungsgemeinschaftCentres de Recerca de CatalunyaCERNU.S. Department of EnergyAgence Nationale de la RechercheGrantová Agentura, Univerzita KarlovaUniversidad de SevillaAgencia Estatal de InvestigaciónSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungAlliance de recherche numérique du CanadaNational Foundation for Science and Technology DevelopmentFundação de Amparo à Pesquisa do Estado de Goiás
KeywordsNeutrinoNeutrino oscillationOscillation (cell signaling)Measurements of neutrino speedCosmic neutrino backgroundSolar neutrino problemPhysics beyond the Standard Model

Abstract

fetched live from OpenAlex

Abstract The landmark discovery that neutrinos have mass and can change type (or flavour) as they propagate—a process called neutrino oscillation 1–6 —has opened up a rich array of theoretical and experimental questions being actively pursued today. Neutrino oscillation remains the most powerful experimental tool for addressing many of these questions, including whether neutrinos violate charge-parity (CP) symmetry, which has possible connections to the unexplained preponderance of matter over antimatter in the Universe 7–11 . Oscillation measurements also probe the mass-squared differences between the different neutrino mass states (Δ m 2 ), whether there are two light states and a heavier one (normal ordering) or vice versa (inverted ordering), and the structure of neutrino mass and flavour mixing 12 . Here we carry out the first joint analysis of datasets from NOvA 13 and T2K 14 , the two currently operating long-baseline neutrino oscillation experiments (hundreds of kilometres of neutrino travel distance), taking advantage of our complementary experimental designs and setting new constraints on several neutrino sector parameters. This analysis provides new precision on the $$\Delta {m}_{32}^{2}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>Δ</mml:mi> <mml:msubsup> <mml:mrow> <mml:mi>m</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>32</mml:mn> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> </mml:mrow> </mml:msubsup> </mml:mrow> </mml:math> mass difference, finding $$2.4{3}_{-0.03}^{+0.04}\times 1{0}^{-3}\,{{\rm{eV}}}^{2}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mn>2.4</mml:mn> <mml:msubsup> <mml:mrow> <mml:mn>3</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>0.03</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>0.04</mml:mn> </mml:mrow> </mml:msubsup> <mml:mo>×</mml:mo> <mml:mn>1</mml:mn> <mml:msup> <mml:mrow> <mml:mn>0</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>3</mml:mn> </mml:mrow> </mml:msup> <mml:mspace/> <mml:msup> <mml:mrow> <mml:mi>eV</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> </mml:mrow> </mml:msup> </mml:mrow> </mml:math> in the normal ordering and $$-2.4{8}_{-0.04}^{+0.03}\times 1{0}^{-3}\,{{\rm{eV}}}^{2}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>2.4</mml:mn> <mml:msubsup> <mml:mrow> <mml:mn>8</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>0.04</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>0.03</mml:mn> </mml:mrow> </mml:msubsup> <mml:mo>×</mml:mo> <mml:mn>1</mml:mn> <mml:msup> <mml:mrow> <mml:mn>0</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>3</mml:mn> </mml:mrow> </mml:msup> <mml:mspace/> <mml:msup> <mml:mrow> <mml:mi>eV</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> </mml:mrow> </mml:msup> </mml:mrow> </mml:math> in the inverted ordering, as well as a 3 σ interval on δ CP of [−1.38π, 0.30π] in the normal ordering and [−0.92π, −0.04π] in the inverted ordering. The data show no strong preference for either mass ordering, but notably, if inverted ordering were assumed true within the three-flavour mixing model, then our results would provide evidence of CP symmetry violation in the lepton sector.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation 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 score0.208
Threshold uncertainty score0.364

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0000.000

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 head0.019
GPT teacher head0.330
Teacher spread0.311 · 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 teacher head, 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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Citations17
Published2025
Admission routes2
Has abstractyes

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