Volume 424 - 9th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities (ARENA2022) - Dense-media radio experiments
The Radar Echo Telescope: Detection of Ultra High Energy Neutrinos and Cosmic Rays Using the Radar Echo Technique
S. Prohira, K. de Vries, P. Allison, J. Beatty, D. Besson, A. Connolly, et al. (click to show)
*: corresponding author
Full text: pdf
Pre-published on: June 12, 2023
Published on: October 25, 2023
Abstract
The SLAC T-576 beam test has shown the radar echo detection method as a feasible technique to probe high-energy-particle-initiated cascades in dense media, such as ice. Furthermore, particle-level simulations show that the radar echo method has a very promising sensitivity to investigate the flux of cosmic neutrinos at energies greater than 1 PeV. Detecting these cosmic neutrinos is the aim of the Radar Echo Telescope for Neutrinos (RET-N). To show the in-nature viability of the radar echo method, we present the Radar Echo Telescope for Cosmic Rays (RET-CR). RET-CR will provide the proof of principle necessary for the construction of RET-N by detecting, using radar, the in-ice continuation of cosmic-ray induced air showers impinging on high altitude ice sheets.
DOI: https://doi.org/10.22323/1.424.0009
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