6533b854fe1ef96bd12ae9aa

RESEARCH PRODUCT

The Zee–Babu model revisited in the light of new data

Miguel NebotJuan Herrero-garciaNuria RiusArcadi Santamaria

subject

PhysicsParticle physicsNuclear and High Energy PhysicsLarge Hadron Collider010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaScalar (mathematics)High Energy Physics::PhenomenologyFOS: Physical sciencesFísicaScalar potential01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesCP violationNeutrino010306 general physicsNeutrino oscillationMixing (physics)

description

We update previous analyses of the Zee-Babu model in the light of new data, e.g., the mixing angle $\theta_{13}$, the rare decay $\mu\to e \gamma$ and the LHC results. We also analyse the possibility of accommodating the deviations in $\Gamma(H\to \gamma\gamma)$ hinted by the LHC experiments, and the stability of the scalar potential. We find that neutrino oscillation data and low energy constraints are still compatible with masses of the extra charged scalars accessible to LHC. Moreover, if any of them is discovered, the model can be falsified by combining the information on the singly and doubly charged scalar decay modes with neutrino data. Conversely, if the neutrino spectrum is found to be inverted and the CP phase $\delta \neq \pi$, the masses of the charged scalars will be well outside the LHC reach.

10.1016/j.nuclphysb.2014.06.001http://dx.doi.org/10.1016/j.nuclphysb.2014.06.001