Speaker
Óscar Macías
(Virginia Tech)
Description
Indirect dark matter detection is a powerful search method that allows to explore a very wide range of the dark matter mass spectrum. I will present our recent results in which we exploit multi-messenger astrophysical observations to explore the allowed parameter space for various archetypal dark matter candidates with masses in the range 10 GeV to 10^16 GeV. Throughout my talk, I will explain our efforts to account for the systematic astrophysical uncertainties impacting our results.
Author
Óscar Macías
(Virginia Tech)
