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Neutrinos from galactic sources of cosmic rays with known gamma-ray spectra

Francesco Vissani
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Abstract

We describe a simple procedure to estimate the high-energy neutrino flux from the observed gamma-ray spectra of galactic cosmic ray sources that are transparent to their gamma radiation. We evaluate in this way the neutrino flux from the supernova remnant RX J1713.7-3946, whose very high-energy gamma-ray spectrum (assumed to be of hadronic origin) is not a power law distribution according to H.E.S.S. observations. The corresponding muon signal in neutrino telescopes is found to be about 5 events per square kilometer per year in an ideal detector.

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BibTeXRIS

Francesco Vissani. 2006-07-12. Neutrinos from galactic sources of cosmic rays with known gamma-ray spectra. https://doi.org/10.1016/j.astropartphys.2006.07.005

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