Galactic Sources of High-Energy Neutrinos: Highlights

Vissani, Francesco; Aharonian, F.A

doi:10.1016/j.nima.2011.12.079

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

Galactic Sources of High-Energy Neutrinos: Highlights

MPS-Authors

/persons/resource/persons30244

Aharonian, F.A
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;
Dublin Institute for Advanced Studies;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

1112.3911
(Preprint), 2MB

Supplementary Material (public)

There is no public supplementary material available

Citation

Vissani, F., & Aharonian, F. (2012). Galactic Sources of High-Energy Neutrinos: Highlights. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 692, 5-12. doi:10.1016/j.nima.2011.12.079.

Cite as: https://hdl.handle.net/11858/00-001M-0000-000E-B5C5-0

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 $\theta_{13}$ on high-energy neutrino oscillations.