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Published August 1, 2022 | Supplemental Material + Submitted + Published
Journal Article Open

Improved measurement of neutrino oscillation parameters by the NOvA experiment

Acero, M. A.
Adamson, P.
Aliaga, L.
Anfimov, N.
Antoshkin, A.
Arrieta-Diaz, E.
Asquith, L.
Aurisano, A.
Back, A.
Backhouse, C.
Baird, M.
Balashov, N.
Baldi, P.
Bambah, B. A.
Bashar, S.
Bays, K.
Bernstein, R.
Bhatnagar, V.
Bhattarai, D.
Bhuyan, B.
Bian, J.
Blair, J.
Booth, A. C.
Bowles, R.
Bromberg, C.
Buchanan, N.
Butkevich, A.
Calvez, S.
Carroll, T. J.
Catano-Mur, E.
Choudhary, B. C.
Christensen, A.
Coan, T. E.
Colo, M.
Cremonesi, L.
Davies, G. S.
Derwent, P. F.
Ding, P.
Djurcic, Z.
Dolce, M.
Doyle, D.
Dueñas Tonguino, D.
Dukes, E. C.
Duyang, H.
Ehrlich, R.
Elkins, M.
Ewart, E.
Feldman, G. J.
Filip, P.
Franc, J.
Frank, M. J.
Gallagher, H. R.
Gandrajula, R.
Gao, F.
Giri, A.
Gomes, R. A.
Goodman, M. C.
Grichine, V.
Groh, M.
Group, R.
Guo, B.
Habig, A.
Hakl, F.
Hall, A.
Hartnell, J.
Hatcher, R.
Hausner, H.
He, M.
Heller, K.
Hewes, J.
Himmel, A.
Holin, A.
Huang, J.
Jargowsky, B.
Jarosz, J.
Jediny, F.
Johnson, C.
Judah, M.
Kakorin, I.
Kaplan, D. M.
Kalitkina, A.
Keloth, R.
Klimov, O.
Koerner, L. W.
Kolupaeva, L.
Kotelnikov, S.
Kralik, R.
Kullenberg, Ch.
Kubu, M.
Kumar, A.
Kuruppu, C. D.
Kus, V.
Lackey, T.
Lang, K.
Lasorak, P.
Lesmeister, J.
Lin, S.
Lister, A.
Liu, J.
Lokajicek, M.
Magill, S.
Manrique Plata, M.
Mann, W. A.
Marshak, M. L.
Martinez-Casales, M.
Matveev, V.
Mayes, B.
Méndez, D. P.
Messier, M. D.
Meyer, H.
Miao, T.
Miller, W. H.
Mishra, S. R.
Mislivec, A.
Mohanta, R.
Moren, A.
Morozova, A.
Mu, W.
Mualem, L. ORCID icon
Muether, M.
Mufson, S.
Mulder, K.
Naples, D.
Nayak, N.
Nelson, J. K.
Nichol, R.
Niner, E.
Norman, A.
Norrick, A.
Nosek, T.
Oh, H.
Olshevskiy, A.
Olson, T.
Ott, J.
Paley, J.
Patterson, R. B. ORCID icon
Pawloski, G.
Petrova, O.
Petti, R.
Phan, D. D.
Plunkett, R. K.
Porter, J. C. C.
Rafique, A.
Psihas, F.
Raj, V.
Rajaoalisoa, M.
Ramson, B.
Rebel, B.
Rojas, P.
Roy, P.
Ryabov, V.
Samoylov, O.
Sanchez, M. C.
Sánchez Falero, S.
Shanahan, P.
Sheshukov, A.
Singh, P.
Singh, V.
Smith, E.
Smolik, J.
Snopok, P.
Solomey, N.
Sousa, A.
Soustruznik, K.
Strait, M.
Suter, L.
Sutton, A.
Swain, S.
Sweeney, C.
Sztuc, A.
Talaga, R. L.
Tapia Oregui, B.
Tas, P.
Thakore, T.
Thayyullathil, R. B.
Thomas, J.
Tiras, E.
Tripathi, J.
Trokan-Tenorio, J.
Tsaris, A.
Torun, Y.
Urheim, J.
Vahle, P.
Vallari, Z.
Vasel, J.
Vokac, P.
Vrba, T.
Wallbank, M.
Warburton, T. K.
Wetstein, M.
Whittington, D.
Wickremasinghe, D. A.
Wojcicki, S. G.
Wolcott, J.
Wu, W.
Xiao, Y.
Yallappa Dombara, A.
Yankelevich, A.
Yonehara, K.
Yu, S.
Yu, Y.
Zadorozhnyy, S.
Zalesak, J.
Zhang, Y.
Zwaska, R.
NOvA Collaboration

Abstract

We present new ν_µ→νₑ, ν_μ→ν_μ, ν̅_μ→ν̅ₑ, and ν̅_μ→νν̅_μ oscillation measurements by the NOvA experiment, with a 50% increase in neutrino-mode beam exposure over the previously reported results. The additional data, combined with previously published neutrino and antineutrino data, are all analyzed using improved techniques and simulations. A joint fit to the νₑ, ν_μ, ν̅ₑ, and ν̅_μ candidate samples within the 3-flavor neutrino oscillation framework continues to yield a best-fit point in the normal mass ordering and the upper octant of the θ₂₃ mixing angle, with Δm²₃₂ = (2.41±0.07) × 10⁻³ eV² and sin²θ₂₃ = 0.57^(+0.03)_(−0.04). The data disfavor combinations of oscillation parameters that give rise to a large asymmetry in the rates of νe and ν⎯⎯⎯e appearance. This includes values of the CP-violating phase in the vicinity of δ_(CP) = π/2 which are excluded by >3σ for the inverted mass ordering, and values around δ_(CP) = 3π/2 in the normal ordering which are disfavored at 2σ confidence.

Additional Information

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Funded by SCOAP3. (Received 19 August 2021; accepted 27 April 2022; published 3 August 2022) This document was prepared by the NOvA Collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by the U.S. Department of Energy; the U.S. National Science Foundation; the Department of Science and Technology, India; the European Research Council; the MSMT CR, GA UK, Czech Republic; the RAS, RFBR, Russian Ministry of Education and Science (RMES), RSF, and BASIS Foundation, Russia; CNPq and FAPEG, Brazil; STFC, UKRI, and the Royal Society, United Kingdom; and the State and University of Minnesota. We are grateful for the contributions of the staffs of the University of Minnesota at the Ash River Laboratory and of Fermilab.

Attached Files

Published - PhysRevD.106.032004.pdf

Submitted - 2108.08219.pdf

Supplemental Material - 2020_3flavor_paper_supplimental_round2PRD.pdf

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Additional details

Created:
August 20, 2023
Modified:
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