Speaker
Francesco Lorenzo Villante
(Istituto Nazionale di Fisica Nucleare)
Description
We present updated predictions for the very high energy neutrino (and gamma-ray) flux from the Galactic Plane. Our calculations includes the diffuse emission produced by interactions of CR with the interstellar gas and the cumulative flux produced by sources that are too faint to be resolved (either by neutrino or gamma-ray telescopes). The diffuse flux calculation includes the possibility of hardening of the cosmic-ray spectral index in the inner Galaxy, recently suggested by Fermi-LAT observations, and implements the galactic-extragalactic transition for CR at PeV energies. We benchmark our predictions with recent gamma-ray data and compare them with recent results of neutrino telescopes.
| Neutrino Properties | NA |
|---|---|
| Neutrino Telescopes & Multi-messenger | neutrinos from galactic and extragalactic sources |
| Neutrino Theory & Cosmology | NA |
| Data Science and Detector R&D | NA |
Authors
Francesco Lorenzo Villante
(Istituto Nazionale di Fisica Nucleare)
Giulia Pagliaroli
(Istituto Nazionale di Fisica Nucleare)
Vittoria Vecchiotti
