One of the most fascinating mysteries of physics today is the nature of dark matter. We know from many astrophysical and cosmological observations that a large fraction of matter in the universe is non-baryonic, invisible matter, called Dark Matter (DM). DM interacts gravitationally with ordinary matter and remains hidden to us because it doesn’t interact with the electromagnetic spectrum, and is therefore invisible to current instruments.

High-energy cosmic rays, i.e., particles traversing the space at energies which are much larger than their rest masses, provide a probe of galactic high-energy processes. They may shed light on the nature of such intriguing phenomenon as Dark Matter (DM) by maybe enabling observation of DM annihilation or decay.