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Galactic Sources of High-Energy Neutrinos: Highlights

MPG-Autoren
http://pubman.mpdl.mpg.de/cone/persons/resource/persons30244

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

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Volltexte (frei zugänglich)

1112.3911
(Preprint), 2MB

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Zitation

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.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-000E-B5C5-0
Zusammenfassung
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.