Speaker
Silvia Gagliardini
(Ariel University, Sapienza Università di Roma)
Description
We estimate the neutrino flux from different kinds of galactic sources and compare it with the recently diffuse neutrino flux detected by IceCube. We find that the flux from these sources may contribute to ∼20% of the IceCube neutrino flux. Most of the sources selected in this work populate the southern hemisphere, therefore a detector like KM3NeT could help in resolving the sources out of the observed diffused galactic neutrino flux.
Primary author
Silvia Gagliardini
(Ariel University, Sapienza Università di Roma)