6533b854fe1ef96bd12af3ca

RESEARCH PRODUCT

Precise predictions for Dirac neutrino mixing

Rahul SrivastavaGauhar AbbasMehran Zahiri Abyaneh

subject

PhysicsParticle physicsSterile neutrinoNeutrino theory of light010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsDirac (video compression format)Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesSolar neutrino problem01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationMixing (physics)

description

The neutrino mixing parameters are thoroughly studied using renormalization-group evolution of Dirac neutrinos with recently proposed parametrization of the neutrino mixing angles referred as `high-scale mixing relations'. The correlations among all neutrino mixing and $CP$ violating observables are investigated. The predictions for the neutrino mixing angle $\theta_{23}$ are precise, and could be easily tested by ongoing and future experiments. We observe that the high scale mixing unification hypothesis is incompatible with Dirac neutrinos due to updated experimental data.

10.1103/physrevd.95.075005https://doi.org/10.1103/PhysRevD.95.075005