Energy reconstruction with the Radio Neutrino Observatory Greenland (RNO-G)

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 e...

Full description

Bibliographic Details
Published in:Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)
Main Authors: Welling, Christoph, Aguilar, Juan A., Allison, Patrick, Beatty, James J., Bernhoff, Hans, Besson, David Zeke, Bingefors, Nils, Botner, Olga, Bouma, Sjoerd, Buitink, Stijn, Carter, Katie, Cataldo, Maddalena, Clark, Brian A., Curtis-Ginsberg, Zachary, Connolly, Amy L., Dasgupta, Paramita, De Kockere, Simon, de Vries, Krijn D., Deaconu, Cosmin, DuVernois, Michael A., Glaser, Christian, Hallgren, Allan, Hallmann, Steffen, Hanson, Jordan C., Hendricks, Bryan, Hokanson-Fasig, Benjamin, Hornhuber, Christian, Hughes, Kaeli, Karle, Albrecht, Kelley, John L., Klein, Spencer R., Krebs, Ryan, Lahmann, Robert, Latif, Uzair Abdul, Magnuson, Mitchell, Meures, Thomas, Meyers, Zachary S., Mulrey, Katharine, Nelles, Anna, Novikov, Alexander, Oberla, Eric, Oeyen, Bob, Pandya, Hershal, Plaisier, Ilse, Pyras, Lilly, Ryckbosch, Dirk, Scholten, Olaf, Seckel, David, Smith, Daniel, Southall, Daniel, Torres, Jorge, Toscano, Simona, Tosi, Delia, Van Den Broeck, Dieder J., van Eijndhoven, Nick, Vieregg, Abigail G., Wissel, Stephanie, Young, Robert, Zink, Adrian, Rno-g, missing
Format: Conference Object
Language:English
Published: 2021
Subjects:
Online Access:https://biblio.ugent.be/publication/8716302
http://hdl.handle.net/1854/LU-8716302
https://doi.org/10.22323/1.395.1033
https://biblio.ugent.be/publication/8716302/file/8716303
Description
Summary: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.