Speaker
Description
The µνSSM solves the µ-problem of SUSY models simply using right-handed neutrinos ν’s, while simultaneously explains the origin of neutrino masses. In this context, novel signatures of SUSY at the LHC are present through the new states of the model. On the other hand, since R parity is broken, a decaying gravitino turns out to be an interesting candidate for dark matter which can be searched through gamma-ray observations such as those of the Fermi Large Area Telescope.
Summary
The µνSSM solves the µ-problem of SUSY models simply using right-handed neutrinos ν’s, while simultaneously explains the origin of neutrino masses. In this context, novel signatures of SUSY at the LHC are present through the new states of the model. On the other hand, since R parity is broken, a decaying gravitino turns out to be an interesting candidate for dark matter which can be searched through gamma-ray observations such as those of the Fermi Large Area Telescope.
