Abstract
The field of high-energy neutrino astronomy is undergoing a rapid evolution. After the discovery of a diffuse flux of astrophysical TeV-PeV neutrinos in 2013, the IceCube observatory has recently found first compelling evidence for neutrino emission from blazars. In this brief review, I will summarize the status of these neutrino observations and highlight the strong role of multi-messenger astronomy for their interpretation.
Originalsprog | Engelsk |
---|---|
Artikelnummer | 01013 |
Tidsskrift | EPJ Web of Conferences |
Vol/bind | 209 |
Antal sider | 7 |
DOI | |
Status | Udgivet - 13 maj 2019 |
Emneord
- astro-ph.HE