27-31 August 2018
LVH, Luisenstraße 58, 10117 Berlin
Europe/Berlin timezone
Home > Timetable > Session details > Contribution details

Contribution Poster (A0 portrait)

LVH, Luisenstraße 58, 10117 Berlin -

Radiative Neutrino Mass via Fermion Kinetic Mixing

Speakers

  • Oleg POPOV

Primary authors

  • Oleg POPOV (Seoul Netional University of Technology and Science)

Abstract content

We propose that the radiative generation of the neutrino mass can be achieved by incorporating the kinetic mixing of fermion fields which arises radiatively at 1 loop level. As a demonstrative example of the application of the mechanism, we will present the particular case of Standard Model extension by U(1)$_D$ symmetry. As a result, we show how neutrino masses can be generated via kinetic mixing portal instead of mass matrix with residual symmetries responsible for stability of multicomponent dark matter.