Arxiv:1903.01609V2 [Astro-Ph.IM] 24 Jun 2019 the Origin of Ultra-High Energy Cosmic Rays (Uhecrs) Is One of the Biggest Mysteries in Astroparticle Physics
Targeting ultra-high energy neutrinos with the ARIANNA experiment A. Ankera, S. W. Barwicka, H. Bernhoffb, D. Z. Bessonc,d, Nils Bingeforse, G. Gaswinta, C. Glasera,∗, A. Hallgrene, J. C. Hansonf, R. Lahmanna,g, U. Latifc, J. Namh, A. Novikovc,d, S. R. Kleini, S. A. Kleinfelderj, A. Nellesk,l, M. P. Paula, C. Persichillia, S. R. Shivelya, J. Tatara,m, E. Ungere, S.-H. Wangh, G. Yodha aDepartment of Physics and Astronomy, University of California, Irvine, CA 92697, USA bUppsala University Department of Engineering Sciences, Division of Electricity, Uppsala, SE-752 37 Sweden cDepartment of Physics and Astronomy, University of Kansas, Lawrence, KS 66045, USA dNational Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Moscow 115409, Russia eUppsala University Department of Physics and Astronomy, Uppsala, SE-752 37, Sweden fWhittier College Department of Physics, Whittier, CA 90602, USA gECAP, Friedrich-Alexander Universit¨atErlangen-N¨urnberg, 91058 Erlangen, Germany hDepartment of Physics and Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei 10617, Taiwan iLawrence Berkeley National Laboratory, Berkeley, CA 94720, USA jDepartment of Electrical Engineering and Computer Science, University of California, Irvine, CA 92697, USA kDESY, 15738 Zeuthen, Germany lHumbolt-Universit¨atzu Berlin, Institut f¨urPhysik, 12489 Berlin, Germany mResearch Cyberinfrastructure Center, University of California, Irvine, CA 92697 USA Abstract The measurement of ultra-high energy (UHE) neutrinos (E > 1016 eV) opens a new field of astronomy with the potential to reveal the sources of ultra-high energy cosmic rays especially if combined with observations in the electromagnetic spectrum and gravitational waves. The ARIANNA pilot detector explores the detection of UHE neutrinos with a surface array of independent radio detector stations in Antarctica which allows for a cost-effective instrumentation of large volumes.
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