Ultra- and extremely high energy neutrino astronomy
I. Sokalski (INFN, Bari)
TL;DR
This paper reviews the scientific motivations, potential sources, expected fluxes, and current and planned experiments related to ultra- and extremely high energy neutrino astronomy, emphasizing deep underwater and ice Cherenkov detectors.
Contribution
It provides a comprehensive overview of the field, highlighting recent developments and future prospects in ultra-high energy neutrino detection and astronomy.
Findings
Identification of key astrophysical sources of EHE/UHE neutrinos
Summary of current and planned neutrino detection experiments
Discussion of expected neutrino fluxes and detection challenges
Abstract
Scientific motivations for ultra- and extremely high energy neutrino astronomy are considered. Sources and expected fluxes of EHE/UHE neutrinos are briefly discussed. Operating and planned experiments on astrophysical neutrino detection are reviewed focusing on deep underwater/ice Cherenkov neutrino telescopes.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology · Neutrino Physics Research