Multimessenger Potential of the Radio Neutrino Observatory in Greenland
Presented by
M.S. Muzio* on behalf of
on behalf of the RNO-G collaboration,
J.A.A. Aguilar,
P. Allison,
D.Z. Besson,
A. Bishop,
O. Botner, S. Bouma, S. Buitink, W. Castiglioni, M. Cataldo, B.A. Clark, A. Coleman, K. Couberly, P. Dasgupta, S. De Kockere, K.D. de Vries, C. Deaconu, M.A. DuVernois, A. Eimer, C. Glaser, T. Glüsenkamp, A. Hallgren, S. Hallmann, J.C. Hanson, B. Hendricks, J. Henrichs, N. Heyer, C. Hornhuber, K. Hughes, T. Karg, A. Karle, J.L. Kelley, M. Korntheuer, M. Kowalski, I. Kravchenko, R. Krebs, R. Lahmann, P. Lehmann, U.A. Latif, P. Laub, H. Liu, J. Mammo, M.J. Marsee, Z.S. Meyers, M. Mikhailova, K. Michaels, K. Mulrey, A. Nelles, A. Novikov, A. Nozdrina, E. Oberla, B. Oeyen, I. Plaisier, N. Punsuebsay, L. Pyras, D. Ryckbosch, F. Schlüter, O. Scholten, D. Seckel, M.F.H. Seikh, D.J.B. Smith, J. Stoffels, D. Southall, K. Terveer, S. Toscano, D. Tosi, D.J. Van Den Broeck, N. van Eijndhoven, A.G. Vieregg, J.Z. Vischer, C. Welling, D.R. Williams, S.A. Wissel, R. Young and A. Zinket al. (click to show)*: corresponding author
Pre-published on:
August 17, 2023
Published on:
September 27, 2024
Abstract
The Radio Neutrino Observatory in Greenland (RNO-G) is the only ultrahigh energy (UHE, ${\gtrsim}30$ PeV) neutrino monitor of the Northern sky and will soon be the world's most sensitive high-uptime detector of UHE neutrinos. Because of this, RNO-G represents an important piece of the multimessenger landscape over the next decade. In this talk, we will highlight RNO-G's multimessenger capabilities and its potential to provide key information in the search for the most extreme astrophysical accelerators. In particular, we will highlight opportunities enabled by RNO-G's unique field-of-view, its potential to constrain the sources of UHE cosmic rays, and its complementarity with IceCube at lower energies.
DOI: https://doi.org/10.22323/1.444.1485
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