7–12 Jul 2024
Aurum, the ‘Gabriele d’Annunzio’ University and ICRANet
Europe/Rome timezone

Neutrino fluxes from different classes of galactic sources

8 Jul 2024, 16:10
20m
M3 (Palazzo Micara of the ‘Gabriele d’Annunzio’ University)

M3

Palazzo Micara of the ‘Gabriele d’Annunzio’ University

Viale Pindaro, 42, Pescara
Invited talk in a parallel session Neutrinos in the multi-messenger era Neutrinos in the multi-messenger era

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)

Presentation materials