Year: 2025
Type: conference-paper
Abstract: The Radar Echo Telescope collaboration (RET) aims to detect the cosmic neutrino flux at the highest energies through the radar echo method. Radar is a detection technique that allows for determining the position, speed and direction of a macroscopic object using radio waves. In-ice neutrino interactions leave a dense ionisation trail that can be detected using radar. We will discuss the very rich phenomenology of the expected radar signal and its features, with a first application to reconstructing the neutrino properties such as vertex position, arrival direction and energy.
DOI: 10.22323/1.501.1103
Institution: Vrije Universiteit Brussel
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
Awards: RII Track-2 FEC: The IceCube EPSCoR Initiative (IEI) - IceCube and the Data Revolution, G3100002460, Collaborative Research: WoU-MMA: The Radar Echo Telescope for Cosmic Rays and Neutrinos: Toward a Transformative Technology for Neutrino Detection, Collaborative Research: WoU-MMA: The Radar Echo Telescope for Cosmic Rays and Neutrinos: Toward a Transformative Technology for Neutrino Detection, Collaborative Research: WoU-MMA: The Radar Echo Telescope for Cosmic Rays and Neutrinos: Toward a Transformative Technology for Neutrino Detection, Radio detection of the PeV - EeV cosmic-neutrino flux
OpenAlex ID: W4414492346
FWCI:
Cites:
Cited by:
Related to: