Neutrino Sources from a Multi-Messenger Perspective
High Energy Astrophysical Phenomena
2019-06-12 v1
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.
Cite
@article{arxiv.1811.07633,
title = {Neutrino Sources from a Multi-Messenger Perspective},
author = {Markus Ahlers},
journal= {arXiv preprint arXiv:1811.07633},
year = {2019}
}
Comments
7 pages, 3 figures, Proceedings of the 7th Roma International Conference on Astroparticle Physics