The Next-Generation Radio Neutrino Observatory — Multi-Messenger Neutrino Astrophysics at Extreme Energies
by Amy Connolly, J. A. Aguilar, P. Allison, S. Archambault, S. Barnet, J. J. Beatty, D. Z. Besson, O. Botner, S. Buitink, P. Chen, B. A. Clark, C. Deaconu, S. de Kockere, M. A. DuVernois, N. van Eijndhoven, C. Finley, D. Garcia, A. Hallgren, F. Halzen, J. Hanson, K. Hanson, J. Haugen, 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, R. Khandelwal, 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, T. Stezelberger, S. Toscano, J. Torres-Espinosa, S. Unger, A. G. Vieregg, K. de Vries, S.-H. Wang, C. Welling, S. A. Wissel, and S. Yoshida
Published onSep 30, 2019
The Next-Generation Radio Neutrino Observatory — Multi-Messenger Neutrino Astrophysics at Extreme Energies
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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 10¹⁶ eV.
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