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Physics potential of the IceCube Upgrade for atmospheric neutrino oscillations

R. Abbasi16, M. Ackermann63, J. Adams17, S. K. Agarwalla40,*, J. A. Aguilar10, M. Ahlers21, J. M. Alameddine22, S. Ali35, N. M. Amin44 et al. (IceCube Collaboration)

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Lazar37, K. Leonard DeHolton61, A. Leszczyńska64, J. Liao4, C. Lin64, Y. T. Liu61, M. Liubarska24, C. Love49, L. Lu40, F. Lucarelli27, W. Luszczak19,20, Y. Lyu6,7, J. Madsen40, E. Magnus11, Y. Makino40, E. Manao26, S. Mancina48,∥, A. Mand40, I. C. Mariş10, S. Marka46, Z. Marka46, L. Marten1, I. Martinez-Soler13, R. Maruyama45, J. Mauro37, F. Mayhew23, F. McNally38, J. V. Mead21, K. Meagher40, S. Mechbal63, A. Medina20, M. Meier15, Y. Merckx11, L. Merten9, A. Millsop36, J. Mitchell5, L. Molchany50, T. Montaruli27, R. W. Moore24, Y. Morii15, A. Mosbrugger25, M. Moulai40, D. Mousadi63, E. Moyaux37, T. Mukherjee30, R. Naab63, M. Nakos40, U. Naumann62, J. Necker63, L. Neste55, M. Neumann43, H. Niederhausen23, M. U. Nisa23, K. Noda15, A. Noell1, A. Novikov64, A. Obertacke Pollmann15, V. O’Dell40, A. Olivas18, R. Orsoe26, J. Osborn40, E. O’Sullivan65, V. Palusova41, H. Pandya64, A. Parenti10, N. Park32, V. Parrish23, E. N. Paudel59, L. Paul50, C. Pérez de los Heros65, T. Pernice63, J. 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Søgaard21, D. Soldin53, P. Soldin1, G. Sommani9, C. Spannfellner26, G. M. Spiczak51, C. Spiering63, J. Stachurska28, M. Stamatikos20, T. Stanev64, T. Stezelberger7, T. Stürwald62, T. Stuttard21, G. W. Sullivan18, I. Taboada4, S. Ter-Antonyan5, A. Terliuk26, A. Thakuri50, M. Thiesmeyer40, W. G. Thompson13, J. Thwaites40, S. Tilav64, K. Tollefson23, S. Toscano10, D. Tosi40, A. Trettin63, A. K. Upadhyay40,*, K. Upshaw5, A. Vaidyanathan42, N. Valtonen-Mattila9,65, J. Valverde42, J. Vandenbroucke40, T. Van Eeden63, N. van Eijndhoven11, L. Van Rootselaar22, J. van Santen63, J. Vara43, F. Varsi31, M. Venugopal30, M. Vereecken37, S. Vergara Carrasco17, S. Verpoest64, D. Veske46, A. Vijai18, J. Villarreal14, C. Walck55, A. Wang4, E. H. S. Warrick59, C. Weaver23, P. Weigel14, A. Weindl30, J. Weldert41, A. Y. Wen13, C. Wendt40, J. Werthebach22, M. Weyrauch30, N. Whitehorn23, C. H. Wiebusch1, D. R. Williams59, L. Witthaus22, M. Wolf26, G. Wrede25, X. W. Xu5, J. P. Yanez24, Y. Yao40, E. Yildizci40, S. Yoshida15, R. Young35, F. Yu13, S. Yu53, T. Yuan40, A. Zegarelli9, S. Zhang23, Z. Zhang56, P. Zhelnin13, and P. Zilberman40 (IceCube Collaboration)

  • 1III. Physikalisches Institut, RWTH Aachen University, D-52056 Aachen, Germany
  • 2Department of Physics, University of Adelaide, Adelaide, 5005, Australia
  • 3Department of Physics and Astronomy, University of Alaska Anchorage, 3211 Providence Drive, Anchorage, Alaska 99508, USA
  • 4School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, Georgia 30332, USA
  • 5Department of Physics, Southern University, Baton Rouge, Louisiana 70813, USA
  • 6Department of Physics, University of California, Berkeley, California 94720, USA
  • 7Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
  • 8Institut für Physik, Humboldt-Universität zu Berlin, D-12489 Berlin, Germany
  • 9Fakultät für Physik und Astronomie, Ruhr-Universität Bochum, D-44780 Bochum, Germany
  • 10Université Libre de Bruxelles, Science Faculty CP230, B-1050 Brussels, Belgium
  • 11Vrije Universiteit Brussel (VUB), Dienst ELEM, B-1050 Brussels, Belgium
  • 12Department of Physics, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
  • 13Department of Physics and Laboratory for Particle Physics and Cosmology, Harvard University, Cambridge, Massachusetts 02138, USA
  • 14Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
  • 15Department of Physics and The International Center for Hadron Astrophysics, Chiba University, Chiba 263-8522, Japan
  • 16Department of Physics, Loyola University Chicago, Chicago, Illinois 60660, USA
  • 17Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch, New Zealand
  • 18Department of Physics, University of Maryland, College Park, Maryland 20742, USA
  • 19Department of Astronomy, Ohio State University, Columbus, Ohio 43210, USA
  • 20Department of Physics and Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, Ohio 43210, USA
  • 21Niels Bohr Institute, University of Copenhagen, DK-2100 Copenhagen, Denmark
  • 22Department of Physics, TU Dortmund University, D-44221 Dortmund, Germany
  • 23Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
  • 24Department of Physics, University of Alberta, Edmonton, Alberta, T6G 2E1, Canada
  • 25Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, D-91058 Erlangen, Germany
  • 26Physik-department, Technische Universität München, D-85748 Garching, Germany
  • 27Département de physique nucléaire et corpusculaire, Université de Genève, CH-1211 Genève, Switzerland
  • 28Department of Physics and Astronomy, University of Gent, B-9000 Gent, Belgium
  • 29Department of Physics and Astronomy, University of California, Irvine, California 92697, USA
  • 30Karlsruhe Institute of Technology, Institute for Astroparticle Physics, D-76021 Karlsruhe, Germany
  • 31Karlsruhe Institute of Technology, Institute of Experimental Particle Physics, D-76021 Karlsruhe, Germany
  • 32Department of Physics, Engineering Physics, and Astronomy, Queen’s University, Kingston, Ontario K7L 3N6, Canada
  • 33Department of Physics and Astronomy, University of Nevada, Las Vegas, Nevada 89154, USA
  • 34Nevada Center for Astrophysics, University of Nevada, Las Vegas, Nevada 89154, USA
  • 35Department of Physics and Astronomy, University of Kansas, Lawrence, Kansas 66045, USA
  • 36Department of Physics, King’s College London, London WC2R 2LS, United Kingdom
  • 37Centre for Cosmology, Particle Physics and Phenomenology—CP3, Université catholique de Louvain, Louvain-la-Neuve, Belgium
  • 38Department of Physics, Mercer University, Macon, Georgia 31207-0001, USA
  • 39Department of Astronomy, University of Wisconsin—Madison, Madison, Wisconsin 53706, USA
  • 40Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin—Madison, Madison, Wisconsin 53706, USA
  • 41Institute of Physics, University of Mainz, Staudinger Weg 7, D-55099 Mainz, Germany
  • 42Department of Physics, Marquette University, Milwaukee, Wisconsin 53201, USA
  • 43Institut für Kernphysik, Universität Münster, D-48149 Münster, Germany
  • 44Bartol Research Institute and Dept. of Physics and Astronomy, University of Delaware, Newark, Delaware 19716, USA
  • 45Department of Physics, Yale University, New Haven, Connecticut 06520, USA
  • 46Columbia Astrophysics and Nevis Laboratories, Columbia University, New York, New York 10027, USA
  • 47Department of Physics, University of Oxford, Parks Road, Oxford OX1 3PU, United Kingdom
  • 48Dipartimento di Fisica e Astronomia Galileo Galilei, Università Degli Studi di Padova, I-35122 Padova PD, Italy
  • 49Department of Physics, Drexel University, 3141 Chestnut Street, Philadelphia, Pennsylvania 19104, USA
  • 50Physics Department, South Dakota School of Mines and Technology, Rapid City, South Dakota 57701, USA
  • 51Department of Physics, University of Wisconsin, River Falls, Wisconsin 54022, USA
  • 52Department of Physics and Astronomy, University of Rochester, Rochester, New York 14627, USA
  • 53Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah 84112, USA
  • 54Department of Physics, Chung-Ang University, Seoul 06974, Republic of Korea
  • 55Oskar Klein Centre and Dept. of Physics, Stockholm University, SE-10691 Stockholm, Sweden
  • 56Department of Physics and Astronomy, Stony Brook University, Stony Brook, New York 11794-3800, USA
  • 57Department of Physics, Sungkyunkwan University, Suwon 16419, Republic of Korea
  • 58Institute of Physics, Academia Sinica, Taipei, 11529, Taiwan
  • 59Department of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama 35487, USA
  • 60Department of Astronomy and Astrophysics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
  • 61Department of Physics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
  • 62Department of Physics, University of Wuppertal, D-42119 Wuppertal, Germany
  • 63Deutsches Elektronen-Synchrotron DESY, Platanenallee 6, D-15738 Zeuthen, Germany
  • 64Bartol Research Institute and Department of Physics and Astronomy, University of Delaware, Newark, Delaware 19716, USA
  • 65Department of Physics and Astronomy, Uppsala University, Box 516, SE-75120 Uppsala, Sweden

  • *Also at Institute of Physics, Sachivalaya Marg, Sainik School Post, Bhubaneswar 751005, India.
  • Also at Department of Space, Earth and Environment, Chalmers University of Technology, 412 96 Gothenburg, Sweden.
  • Also at INFN Padova, I-35131 Padova, Italy.
  • §Also at Earthquake Research Institute, University of Tokyo, Bunkyo, Tokyo 113-0032, Japan.
  • Present address: INFN Padova, I-35131 Padova, Italy.
  • Contact author: analysis@icecube.wisc.edu

Phys. Rev. D 113, 072009 – Published 15 April, 2026

DOI: https://doi.org/10.1103/nnjw-jp1n

Abstract

The IceCube Upgrade is an extension of the existing IceCube Neutrino Observatory and will be deployed in the 2025–2026 austral summer. It will significantly improve the sensitivity of the detector to atmospheric neutrino oscillations. The existing 86-string IceCube array contains a dense in-fill known as DeepCore which is optimized to measure neutrinos with energies down to a few GeV. The IceCube Upgrade will consist of seven new densely instrumented strings placed within the DeepCore volume to further enhance the performance in the GeV energy range. The additional strings will feature new optical modules, each containing multiple photomultiplier tubes (PMTs), in contrast to the existing modules that each contain a single PMT. This will more than triple the number of PMT channels with respect to the current IceCube configuration, allowing for improved detection efficiency and reconstruction performance at GeV energies. We describe necessary updates to simulation, event selection, and reconstruction to accommodate the higher data rates observed by the upgraded detector and the addition of multi-PMT modules. We determine the expected sensitivity of the IceCube Upgrade to the atmospheric neutrino oscillation parameters sin2θ23 and Δm322, the appearance of tau neutrinos and the neutrino mass ordering. The IceCube Upgrade will provide neutrino oscillation measurements that are of similar precision to those from accelerator experiments, while providing complementarity by probing higher energies and longer baselines, and with different sources of systematic uncertainties.

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