6533b835fe1ef96bd129f4ab

RESEARCH PRODUCT

Bound-state dark matter and Dirac neutrino mass

José W. F. ValleÓScar ZapataMario ReigDiego Restrepo

subject

PhysicsConservation lawParticle physicsSIMPLE (dark matter experiment)010308 nuclear & particles physicsDirac (video compression format)Dark matterHadronHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Recoil0103 physical sciencesBound stateHigh Energy Physics::ExperimentNeutrino010306 general physics

description

We propose a simple theory for the idea that cosmological dark matter (DM) may be present today mainly in the form of stable neutral hadronic thermal relics. In our model neutrino masses arise radiatively from the exchange of colored DM constituents, giving a common origin for both dark matter and neutrino mass. The exact conservation of $B-L$ symmetry ensures dark matter stability and the Dirac nature of neutrinos. The theory can be falsified by dark matter nuclear recoil direct detection experiments, leading also to possible signals at a next generation hadron collider.

10.1103/physrevd.97.115032http://arxiv.org/abs/1803.08528