Galactic Sources of High-Energy Neutrinos: Highlights
arXiv:1112.3911 · doi:10.1016/j.nima.2011.12.079
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.
8 pages, 11 figures. Accepted for publication in NIM A
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Cited by in corpus (12)
- Hadronic gamma-rays from RX J1713.7-3946?
- Reevaluation of the Prospect of Observing Neutrinos from Galactic Sources in the Light of Recent Results in Gamma Ray and Neutrino Astronomy
- The natural parametrization of cosmic neutrino oscillations
- Prospects for Detecting Galactic Sources of Cosmic Neutrinos with IceCube: An Update
- On the potential of Cherenkov Telescope Arrays and KM3 Neutrino Telescopes for the detection of extended sources
- The fraction of muon tracks in cosmic neutrinos
- Status of the KM3NeT project
- Searching for High Energy Neutrino counterpart signals; The case of the Fermi Bubbles signal and of Dark Matter annihilation in the inner Galaxy
- Neutrinos from the gamma-ray source eHWC J1825-134: predictions for Km detectors
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- Neutrinos from collapsars
- Neutrinos from Cosmic Accelerators Including Magnetic Field and Flavor Effects