Speaker
Miguel Sánchez-Conde
(Universidad Autónoma de Madrid & IFT UAM-CSIC)
Description
The nature of dark matter (DM) in the Universe remains one of the greatest mysteries of our time. Searches for annihilation or decay products of DM particle candidates such as WIMPs have already provided stringent constraints on their properties across a wide range of masses and interaction channels. In this review talk, I will summarize the current status of these ‘indirect’ DM searches in gamma rays. I will highlight key targets, current limitations, and the role of systematic uncertainties. I will then discuss future prospects for DM sensitivity with upcoming experiments as well as emerging opportunities for exploring DM signatures in gamma rays.