Galactic Sources of High-Energy Neutrinos: Highlights
Francesco Vissani, Felix Aharonian
TL;DR
This paper reviews galactic high-energy neutrino sources, focusing on supernova remnants and gamma-ray sources, discussing detection prospects, expectations, and the impact of neutrino oscillation parameters.
Contribution
It provides a comprehensive overview of potential galactic neutrino sources and analyzes how recent neutrino oscillation measurements influence detection strategies.
Findings
Upper bounds on neutrino fluxes from RX J1713.7-3946
Potential neutrino detection from Vela Junior and Cygnus Region
Impact of large $ heta_{13}$ on neutrino oscillation predictions
Abstract
We overview high-energy neutrinos from galactic sources, transparent to their gamma-ray emission. We focus on young supernova remnants and in particular on RX J1713.7-3946, discussing expectations and upper bounds. We also consider the possibility to detect neutrinos from other strong galactic gamma-ray sources as Vela Junior, the Cygnus Region and the recently discovered Fermi Bubbles. We quantify the impact of the recent hint for a large value of on high-energy neutrino oscillations.
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.