Orateur
Dr
alessandro cuoco
(Oskar Klein Center - Stockholm University)
Description
Electrons from Dark Matter (DM) annihilation produce radiation through synchrotron and Inverse Compton Scattering (ICS) interactions in the galactic environment. This multi-wavelength emission provides a complementary mean to test the DM hypothesis. I will present constraints coming from radio observations as well as ICS constraints from gamma-ray measurements by Fermi-LAT in the Galactic Halo region.
Author
Dr
alessandro cuoco
(Oskar Klein Center - Stockholm University)
