Energy reconstruction with the Radio Neutrino Observatory Greenland (RNO-G)
Presented by
C. Welling* on behalf of
J.A. Aguilar,
P. Allison,
J.J. Beatty,
H. Bernhoff,
D.Z. Besson,
N. Bingefors, O. Botner, S. Bouma, S. Buitink, K. Carter, M. Cataldo, B.A. Clark, Z. Curtis-Ginsberg, A.L. Connolly, P. Dasgupta, S. De Kockere, K.D. de Vries, C. Deaconu, M.A. DuVernois, C. Glaser, A. Hallgren, S. Hallmann, J.C. Hanson, B.L. Hendricks, B. Hokanson-Fasig, C. Hornhuber, K. Hughes, A. Karle, J.L. Kelley, S.R. Klein, R. Krebs, R. Lahmann, U.A. Latif, M. Magnuson, T. Meures, Z.S. Meyers, K. Mulrey, A. Nelles, A. Novikov, E. Oberla, B. Oeyen, H. Pandya, I. Plaisier, L. Pyras, D. Ryckbosch, O. Scholten, D. Seckel, D. Smith, D. Southall, J. Torres, S. Toscano, D. Tosi, D.J. Van Den Broeck, N. van Eijndhoven, A.G. Vieregg, S. Wissel, R. Young and A. Zinket al. (click to show)*: corresponding author
Pre-published on:
July 27, 2021
Published on:
March 18, 2022
Abstract
Starting in summer 2021, the Radio Neutrino Observatory Greenland (RNO-G) will attempt to
achieve the first detection of neutrinos with energies at the EeV scale. We present a method to
reconstruct the energy of neutrino-induced particle showers detected by RNO-G and the resolution
on the neutrino energy this would allow. We demonstrate that to further improve the neutrino
energy reconstruction, a way to identify the neutrino flavor is needed.
DOI: https://doi.org/10.22323/1.395.1033
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