Potential neutrino signals from galactic γ-ray sources

Details Potential neutrino signals from galactic γ-ray sources Potential neutrino signals from galactic γ-ray sources

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jphcs..60..243k&link_type=abstract

Journal of Physics: Conference Series, Volume 60, Issue 1, pp. 243-246 (2007).

Physics

2

Scientific paper

Recent measurements of the energy spectra of Galactic TeV γ-ray sources with the H.E.S.S. instrument have been used to calculate the expected high energy neutrino fluxes from these sources. Based on the results the expected event rates in a next generation neutrino telescope in the Mediterranean Sea, KM3NeT, have been estimated, assuming an instrumented volume of 1 km3. We find that for energies above 1TeV event rates of a few neutrinos per year can be expected from the brightest γ-ray sources. Although these rates are comparable to those of the background from atmospheric neutrinos a detection of individual sources seems possible.

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