Search for an eV-Scale Sterile Neutrino Using Improved High-Energy νμ Event Reconstruction in IceCube

被引:0
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作者
Abbasi, R. [17 ]
Ackermann, M. [65 ]
Adams, J. [18 ]
Agarwalla, S.K. [40 ,66 ]
Aguilar, J.A. [12 ]
Ahlers, M. [22 ]
Alameddine, J.M. [23 ]
Amin, N.M. [44 ]
Andeen, K. [42 ]
Argüelles, C. [14 ]
Ashida, Y. [53 ]
Athanasiadou, S. [65 ]
Ausborm, L. [1 ]
Axani, S.N. [44 ]
Bai, X. [50 ]
Balagopal, V.A. [40 ]
Baricevic, M. [40 ]
Barwick, S.W. [30 ]
Bash, S. [27 ]
Basu, V. [40 ]
Bay, R. [8 ]
Beatty, J.J. [20 ,21 ]
Becker Tjus, J. [11 ,67 ]
Beise, J. [63 ]
Bellenghi, C. [27 ]
Benning, C. [1 ]
Benzvi, S. [52 ]
Berley, D. [19 ]
Bernardini, E. [48 ]
Besson, D.Z. [36 ]
Blaufuss, E. [19 ]
Bloom, L. [60 ]
Blot, S. [65 ]
Bontempo, F. [31 ]
Book Motzkin, J.Y. [14 ]
Boscolo Meneguolo, C. [48 ]
Böser, S. [41 ]
Botner, O. [63 ]
Böttcher, J. [1 ]
Braun, J. [40 ]
Brinson, B. [6 ]
Brostean-Kaiser, J. [65 ]
Brusa, L. [1 ]
Burley, R.T. [2 ]
Butterfield, D. [40 ]
Campana, M.A. [49 ]
Caracas, I. [41 ]
Carloni, K. [14 ]
Carpio, J. [34 ,35 ]
Chattopadhyay, S. [40 ,66 ]
机构
[1] III. Physikalisches Institut, RWTH Aachen University, Aachen,D-52056, Germany
[2] Department of Physics, University of Adelaide, Adelaide,5005, Australia
[3] Department of Physics and Astronomy, University of Alaska Anchorage, 3211 Providence Drive, Anchorage,AK,99508, United States
[4] Department of Physics, University of Texas at Arlington, 502 Yates Street, Science Hall Rm 108, Box 19059, Arlington,TX,76019, United States
[5] CTSPS, Clark-Atlanta University, Atlanta,GA,30314, United States
[6] School of Physics, Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta,GA,30332, United States
[7] Department of Physics, Southern University, Baton Rouge,LA,70813, United States
[8] Department of Physics, University of California, Berkeley,CA,94720, United States
[9] Lawrence Berkeley National Laboratory, Berkeley,CA,94720, United States
[10] Institut für Physik, Humboldt-Universität zu Berlin, Berlin,D-12489, Germany
[11] Fakultät für Physik & Astronomie, Ruhr-Universität Bochum, Bochum,D-44780, Germany
[12] Université Libre de Bruxelles, Science Faculty CP230, Brussels,B-1050, Belgium
[13] Vrije Universiteit Brussel (VUB), Dienst ELEM, Brussels,B-1050, Belgium
[14] Department of Physics and Laboratory for Particle Physics and Cosmology, Harvard University, Cambridge,MA,02138, United States
[15] Department of Physics, Massachusetts Institute of Technology, Cambridge,MA,02139, United States
[16] Department of Physics, The International Center for Hadron Astrophysics, Chiba University, Chiba,263-8522, Japan
[17] Department of Physics, Loyola University Chicago, Chicago,IL,60660, United States
[18] Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch, New Zealand
[19] Department of Physics, University of Maryland, College Park,MD,20742, United States
[20] Department of Astronomy, Ohio State University, Columbus,OH,43210, United States
[21] Department of Physics, Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus,OH,43210, United States
[22] Niels Bohr Institute, University of Copenhagen, Copenhagen,DK-2100, Denmark
[23] Department of Physics, TU Dortmund University, Dortmund,D-44221, Germany
[24] Department of Physics and Astronomy, Michigan State University, East Lansing,MI,48824, United States
[25] Department of Physics, University of Alberta, Edmonton,AB,T6G 2E1, Canada
[26] Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen,D-91058, Germany
[27] Physik-department, Technische Universität München, Garching,D-85748, Germany
[28] Département de Physique Nucléaire et Corpusculaire, Université de Genève, Genève,CH-1211, Switzerland
[29] Department of Physics and Astronomy, University of Gent, Gent,B-9000, Belgium
[30] Department of Physics and Astronomy, University of California, Irvine,CA,92697, United States
[31] Karlsruhe Institute of Technology, Institute for Astroparticle Physics, Karlsruhe,D-76021, Germany
[32] Karlsruhe Institute of Technology, Institute of Experimental Particle Physics, Karlsruhe,D-76021, Germany
[33] Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston,ON,K7L 3N6, Canada
[34] Department of Physics and Astronomy, University of Nevada, Las Vegas,NV,89154, United States
[35] Nevada Center for Astrophysics, University of Nevada, Las Vegas,NV,89154, United States
[36] Department of Physics and Astronomy, University of Kansas, Lawrence,KS,66045, United States
[37] Centre for Cosmology, Particle Physics and Phenomenology - CP3, Université Catholique de Louvain, Louvain-la-Neuve, Belgium
[38] Department of Physics, Mercer University, Macon,GA,31207-0001, United States
[39] Department of Astronomy, University of Wisconsin Ͽ Madison, Madison,WI,53706, United States
[40] Department of Physics, Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin Ͽ Madison, Madison,WI,53706, United States
[41] Institute of Physics, University of Mainz, Staudinger Weg 7, Mainz,D-55099, Germany
[42] Department of Physics, Marquette University, Milwaukee,WI,53201, United States
[43] Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster,D-48149, Germany
[44] Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, Newark,DE,19716, United States
[45] Department of Physics, Yale University, New Haven,CT,06520, United States
[46] Columbia Astrophysics and Nevis Laboratories, Columbia University, New York,NY,10027, United States
[47] Department of Physics, University of Oxford, Parks Road, Oxford,OX1 3PU, United Kingdom
[48] Dipartimento di Fisica e Astronomia Galileo Galilei, Università Degli Studi di Padova, PD, Padova,I-35122, Italy
[49] Department of Physics, Drexel University, 3141 Chestnut Street, Philadelphia,PA,19104, United States
[50] Physics Department, South Dakota School of Mines and Technology, Rapid City,SD,57701, United States
关键词
This Letter presents the result of a 3+1 sterile neutrino search using 10.7 yr of IceCube data. We analyze atmospheric muon neutrinos that traverse the Earth with energies ranging from 0.5 to 100 TeV; incorporating significant improvements in modeling neutrino flux and detector response compared to earlier studies. Notably; for the first time; we categorize data into starting and throughgoing events; distinguishing neutrino interactions with vertices inside or outside the instrumented volume; to improve energy resolution. The best-fit point for a 3+1 model is found to be at sin2(2θ24)=0.16 and Δm412=3.5 eV2; which agrees with previous iterations of this Letter. The result is consistent with the null hypothesis of no sterile neutrinos with a p value of 3.1%. © 2024 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the https://creativecommons.org/licenses/by/4.0/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;
D O I
10.1103/PhysRevLett.133.201804
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