Orateur
Dr
Marco Regis
(University of Turin and INFN)
Description
In most of particle dark matter (DM) models, the DM candidate injects sizable fluxes of high-energy electrons and positrons through its annihilations or decays. Emitted in regions with magnetic field, they in turn give raise to a synchrotron radiation, which typically covers radio and infrared bands. We discuss the possibility of detecting signatures of Galactic and extra-galactic DM in the isotropic total intensity and small-scale anisotropies of the radio background.
Auteur principal
Dr
Marco Regis
(University of Turin and INFN)
