The impact of halo and subhalo properties on dark matter searches

Cosmological observations and cold dark matter N-body simulations indicate that our Universe is populated by numerous halos, where dark matter particles annihilate, potentially producing Standard Model particles. Indeed, one of the most active lines of research in dark matter physics is that of indirect searches of such dark matter annihilation products (gamma-rays, neutrinos and antimatter) in different astrophysical regions. In this talk, I will focus on the impact of different predictions of structure formation in such dark matter searches.