| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1823635 | Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment | 2012 | 8 Pages |
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 θ13θ13 on high-energy neutrino oscillations.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Instrumentation
Authors
Francesco Vissani, Felix Aharonian,