Rno-g, S. Agarwal, J.A. Aguilar, S. Ali, P. Allison, M. Betts,
D. Besson, A. Bishop, O. Botner, S. Bouma, S. Buitink, M. Cataldo, B. Clark, A. Coleman, K. Couberly, S. De Kockere, K. de Vries, C. Deaconu, C. Glaser, T. Glüsenkamp, A. Hallgren, S. Hallmann, J. Hanson, B.L. Hendricks, J. Henrichs, N. Heyer, C. Hornhuber, K. Hughes*, T. Karg, A. Karle, J. Kelley, M. Korntheuer, M. Kowalski, I. Kravchenko, R. Krebs, R. Lahmann, U.A. Latif, P. Laub, M. Liu, M. Marsee, Z.S. Meyers, M. Mikhailova, K. Mulrey, M.S. Muzio, A. Nelles, A. Novikov, A. Nozdrina, E. Oberla, B. Oeyen, N. Punsuebsay, L. Pyras, M.L. Ravn, D. Ryckbosch, F. Schlüter, O. Scholten, D. Seckel, M. Seikh, J. Stoffels, K. Terveer, S. Toscano, D. Tosi, D.J. Van Den Broeck, N. van Eijndhoven, A.G. Vieregg, A. Vijai, C. Welling, D. Williams, P. Windischhofer, S. Wissel, R. Young, A. Zink on behalf of the RNO-G collaborationet al. (click to show)
Published on:
November 07, 2024
Abstract
The Radio Neutrino Observatory in Greenland (RNO-G) is a detector under construction that will be sensitive to Askaryan emission from ultra-high energy neutrinos. Located in Summit Station, Greenland, RNO-G consists of multiple “stations” of 24 antennas each, which include deep antennas buried down to 100 m in the ice and surface antennas to improve our understanding of backgrounds. As RNO-G grows in size, so does its potential to detect the first astrophysical neutrino above 10 PeV. Seven of the planned 35 stations are currently deployed and operational, with more progress expected this summer season. In this talk, I will present our current and future sensitivity, discuss the successes and challenges with installing a neutrino observatory in a remote environment, and give an overview of our ongoing analysis efforts.