Speaker
Aldo Morselli
(INFN Roma Tor Vergata)
Description
Detection of gamma rays and cosmic rays from the annihilation or decay of dark matter particles is a promising method for identifying dark matter, understanding its intrinsic properties, and mapping its distribution in the universe. I will review rthe current status and discuss the prospects for indirect searches to robustly identify or exclude a dark matter signal using upcoming experiments at energies below and above Fermi energy range.
Primary author
Aldo Morselli
(INFN Roma Tor Vergata)
