6533b82bfe1ef96bd128e178

RESEARCH PRODUCT

Right Handed Sneutrino Dark Matter in Inverse and Linear seesaw scenarios

Valentina De Romeri

subject

PhysicsHistoryParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesSupersymmetryLightest Supersymmetric ParticleComputer Science ApplicationsEducationHigh Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryHigh Energy Physics::ExperimentNeutrinoLeptonMinimal Supersymmetric Standard ModelAstrophysics - Cosmology and Nongalactic Astrophysics

description

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.

yearjournalcountryeditionlanguage
2012-09-07
http://arxiv.org/abs/1209.1465