Description
The existence of Dark Matter is one of the most important indications of physics beyond the Standard Model of particle physics. A promising class of Dark Matter candidate is represented by new massively interactive particles.
Direct Detection experiments can potentially find some of these candidates due the possible interactions of Dark Matter with Standard Model, in our case these possible interactions arise at first order radiative corrections.
On this talk we will introduce the models considered, the calculation of the radiative correction and finally the possible phenomenology of these different candidates to Dark Matter in the context of Direct Detection
Speaker
David Cabo Almeida
(University of Messina (Italy))
