Reconciling dark matter, solar and atmospheric neutrinos

Abstract

We present models that can reconcile the solar and atmospheric neutrino data with the existence of a hot dark matter component in the universe. This dark matter is a quasi-Dirac neutrino whose mass mDM arises at the one-loop level. The solar neutrino deficit is explained via nonadiabatic conversions of νe to a sterile neutrino νs and the atmospheric neutrino data via maximal νμ to ντ oscillations generated by higher order loop diagrams. For mDM ∼ 30 eV the radiative neutrino decay can lead to photons that can ionize intersteller hydrogen. in one of the models one can have observable νe to ντ oscillations rates, with no appreiable νμ oscillations at accelerator experiments. In addition, there can be observable rates for tau number violating processes such as τ→3e and τ→e + γ. In the other model one can have sizeable νe to νμ oscillation rates, as well as sizeable rates for muon number violating processes such as μ→e + γ, μ→e + majoron and μ→3e.