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The Next-Generation Radio Neutrino Observatory -- Multi-Messenger Neutrino Astrophysics at Extreme Energies

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arxiv 1907.12526 v3 pith:WNF3AXU5 submitted 2019-07-29 astro-ph.HE

J. A. Aguilar , P. Allison , S. Archambault , J. J. Beatty , D. Z. Besson , O. Botner , S. Buitink , P. Chen
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B. A. Clark A. Connolly C. Deaconu S. de Kockere M. A. DuVernois N. van Eijndhoven C. Finley D. Garcia A. Hallgren F. Halzen J. Hanson K. Hanson C. Pérez de los Heros K. D. Hoffman B. Hokanson-Fasig K. Hughes K. Hultqvist A. Ishihara A. Karle J. L. Kelley S. R. Klein M. Kowalski I. Kravchenko U. A. Latif T. C. Liu M.-Y. Lu K. Mase R. Morse J. Nam A. Nelles E. Oberla C. Pfendner Y. Pan I. Plaisier S. Prohira S. Robertson J. Rolla D. Ryckbosch F. G. Schröder D. Seckel A. Shultz D. Smith D. Southall E. O'Sullivan S. Toscano J. Torres-Espinosa E. Unger A. G. Vieregg K. de Vries S.-H. Wang C. Welling S. A. Wissel S. Yoshida
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classification astro-ph.HE
keywords energiesneutrinoastrophysicsenablingextremeinstrumentmulti-messengerneutrinos
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abstract

RNO is the mid-scale discovery instrument designed to make the first observation of neutrinos from the cosmos at extreme energies, with sensitivity well beyond current instrument capabilities. This new observatory will be the largest ground-based neutrino telescope to date, enabling the measurement of neutrinos above $10^{16}$ eV, determining the nature of the astrophysical neutrino flux that has been measured by IceCube at higher energies, similarly extending the reach of multi-messenger astrophysics to the highest energies, and enabling investigations of fundamental physics at energies unreachable by particle accelerators on Earth.

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