Abstract
The search for diffuse fluxes of cosmic neutrinos is among the main objectives of high-energy neutrino astronomy. The future Mediterranean deep-sea neutrino telescope KM3NeT, due to its multi-km 3 instrumented volume will have unprecedented sensitivity for the observation of these fluxes. Detection of diffuse neutrino fluxes of different origins (extragalactic, from inner Galaxy and cosmogenic) in the KM3NeT neutrino telescope is discussed in this paper.
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