Abstract

In this work we study the viable parameter space of the scalar sector in the type-II seesaw model. In identifying the allowed parameter space, we employ constraints from low energy precision measurements, theoretical considerations and the 125-GeV Higgs data. These tools prove effective in constraining the model parameter space. Moreover, the triplet also offers a rich collider phenomenology from having additional scalars that have unique collider signatures. We find that direct collider searches for these scalars can further probe various parts of the viable parameter space. These parts can be parametrized by the electroweak scalar triplet vacuum expectation value, the mass splitting of the singly- and doubly-charged scalars, and the doubly-charged Higgs mass. We find that different regions of the viable parameter space give rise to different collider signatures, such as the same-sign dilepton, the same-sign W and the multilepton signatures. By investigating various LEP and LHC measurements, we derive the most updated constraints over the whole range of parameter space of the type-II seesaw model.

Highlights

  • Mechanism, Λ is the mass of right-handed neutrinos transforming as singlets under the SM gauge groups [2,3,4,5]

  • In this work we study the viable parameter space of the scalar sector in the type-II seesaw model

  • We find that different regions of the viable parameter space give rise to different collider signatures, such as the same-sign dilepton, the same-sign W and the multilepton signatures

Read more

Summary

The model

We give a brief overview of the type-II seesaw model. We demonstrate how scalar masses are expressed in terms of model parameters. It is followed by a discussion on neutrino mass generation in the framework of type-II seesaw mechanism

Scalar sector
Neutrino sector
Constraints on model parameters
Electroweak precision constraints
Higgs data
Viable model parameter space
Lepton flavor violation constraints
Collider phenomenology
Conclusions and discussions
Findings
A Dependence on neutrino mass parameters
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call