Speaker
Description
Dark Matter (DM) existence is a milestone of the cosmological standard model and, yet, its very nature discovery still remains a mystery. In this talk, I discuss a new way to probe properties of light-particle dark matter candidates which exploits the nature of the cosmic-ray (CR) transport inside starburst nuclei (SBNs). Indeed, SBNs are considered CR reservoirs, trapping them for ∼10^5 years up to ∼ PeVs energies, leading to copious production of gamma-rays and neutrinos. As a result, interactions between DM and protons might indelibly change CR transport in these galaxies, perturbing the gamma-rays and neutrino production. I will show that current gamma-ray observations pose strict limits on the elastic cross section down to σ_χp≃10^-34 cm^-2 for DM masses m_χ≤10^-3 MeV and that they have considerable room for improvement with the future gamma-ray measurements in the 0.1-10 TeV range from the Cherenkov Telescope Array.
