Right Handed Sneutrino Dark Matter in Inverse and Linear seesaw
  scenarios
  We consider supersymmetric models in which the right-handed sneutrino is a
viable WIMP dark matter candidate. These are either simple extensions of the
Minimal Supersymmetric Standard Model or models with the addition of an extra
U(1) group. All of them can explain small neutrino masses, through either the
Inverse or the Linear Seesaw mechanism. We investigate the properties of the
dark matter candidate naturally arising in these scenarios. We check for
phenomenological bounds, such as correct relic abundance, consistency with
direct detection cross section limits and laboratory constraints. Especially,
we comment on limitations of the model space due to lepton flavour violating
charged lepton decays.
