6533b830fe1ef96bd1297032

RESEARCH PRODUCT

Phenomenology of dark matter from A(4) flavor symmetry

S. MorisiMarco TaosoE. PeinadoM. S. BoucennaJosé W. F. ValleM. Hirsch

subject

PhysicsNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsDark matterElectroweak interactionHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaParity (physics)Parameter space01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHiggs bosonHigh Energy Physics::ExperimentSymmetry breakingNeutrino010306 general physicsPhenomenology (particle physics)Astrophysics - Cosmology and Nongalactic Astrophysics

description

We investigate a model in which Dark Matter is stabilized by means of a Z2 parity that results from the same non-abelian discrete flavor symmetry which accounts for the observed pattern of neutrino mixing. In our A4 example the standard model is extended by three extra Higgs doublets and the Z2 parity emerges as a remnant of the spontaneous breaking of A4 after electroweak symmetry breaking. We perform an analysis of the parameter space of the model consistent with electroweak precision tests, collider searches and perturbativity. We determine the regions compatible with the observed relic dark matter density and we present prospects for detection in direct as well as indirect Dark Matter search experiments.

10.1007/jhep05(2011)037http://hdl.handle.net/10550/37397