TL;DR
Neutrino telescopes detect high energy cosmic neutrinos, aiding in understanding astrophysical processes and multimessenger astronomy, with ongoing advancements in their design and sensitivity.
Contribution
This paper reviews the current status, recent results, and future plans of neutrino telescopes based on Cherenkov light detection.
Findings
Multiple neutrino telescopes are operational and collecting data.
Recent results have advanced understanding of high energy cosmic neutrinos.
Plans are underway to enhance the sensitivity and scale of neutrino detectors.
Abstract
The observation of high energy cosmic neutrinos can shed light on the astrophysical sites and mechanisms involved in the acceleration of protons and nuclei to the high energies observed at Earth by cosmic ray detectors. More generally, high energy neutrinos can be a key instrument in the multimessenger study of the high energy sky. Several neutrino telescopes of different sizes and capabilities are presently taking data and projects to further increase their size and sensitivity are underway.In this contribution we review the present status of neutrino telescopes based on the cherenkov ligh detection technique, their recent results and the plans to increase their sensitivity.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.