Speaker
Dr
Marco Taoso
(IPhT Saclay Paris)
Description
Annihilations of Dark Matter in the form of WIMPs produce photon fluxes ranging from radio wavelengths to gamma-rays. In particular, low energy emissions are associated with the interactions of the WIMPs annihilation products with the intergalactic medium.
I will present constraints on the WIMPs properties from current radio surveys and I will discuss the prospects for detection with future radio data.
I will review the status of DM searches with gamma-ray spectral features and I will investigate DM models which can naturally lead to large line signals.
Primary author
Dr
Marco Taoso
(IPhT Saclay Paris)
