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High-energy neutrinos from Galactic sources
Author(s) -
Viviairo
Publication year - 2021
Publication title -
journal of physics. conference series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.21
H-Index - 85
eISSN - 1742-6596
pISSN - 1742-6588
DOI - 10.1088/1742-6596/2156/1/012088
Subject(s) - physics , neutrino , detector , neutrino detector , telescope , focus (optics) , flux (metallurgy) , hadron , cosmic ray , astrophysics , gamma ray , energy (signal processing) , astronomy , particle physics , optics , neutrino oscillation , materials science , quantum mechanics , metallurgy
Among the galactic sources that can be detected by the KM3NeT detector, we will consider the eHWC J1825-134 source recently detected by the HAWC telescope. Moreover, we consider the source RX J1713.7-3946 and show the prospects of detection in a fully hadronic and in a lepto-hadronic scenario. Considering the IceCube detector, instead, we focus on the gamma-ray sources eHWC J1907+063 and eHWC J2019+368. We found that a detection at 3 σ or more at the IceCube detector should be within reach of the next decade. Finally, we consider also the source 2HWC J1857+027, since it is coincident with the location of a neutrino excess. For this source, we show the dependence on the specific value of the flux, on the extension and on the cut-off energy. A detection at 3σ in the next decade will depend on these parameters.

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