Speaker
Dr
Emiliano Molinaro
(TUM)
Description
We propose a UV completion of the inverse see-saw scenario of neutrino mass generation, where the Standard Model gauge group is extended by a U(1) symmetry. Within this framework, a variation of the standard thermal leptogenesis is achievable at the O(TeV) scale, owing to the presence of a viable dark matter candidate. The scalar and fermion sector of the model can be tested at LHC and in current and future experiments searching for dark matter.
Ref.:
http://arXiv.org/abs/arXiv:1108.0482
http://arXiv.org/abs/arXiv:1210.7202
Author
Dr
Emiliano Molinaro
(TUM)
