Choose timezone
Your profile timezone:
Powered by Indico
v3.3.5
In this talk, I will review recent advances in our understanding of the
multi-messenger emissions from the Milky Way Galaxy in the PeV energy range.
I will present experimental results on the cosmic ray spectrum obtained by CALET, DAMPE, and LHAASO, as well as gamma-ray observations from Fermi, HAWC, and LHAASO. Additionally, I will discuss neutrino observations of Galaxy reported by IceCube, ANTARES, and GVD-Baikal. The talk will also cover theoretical models developed to interpret these data, with a particular focus on the importance of combined modeling of cosmic ray propagation and the Galactic Magnetic Field.