Abstract

We discuss the modes B→K(⁎)νν¯ in the context of non-standard neutrino interactions that add incoherently to the SM rates. We consider two scenarios: an additional light neutrino; and neutrino lepton flavour violation. We find that an additional light neutrino that interacts with SM fields via a non-universal Z′ can increase RK(⁎)ν by up to a factor of two without conflicting with Bs−B¯s mixing. This model then predicts rates for Bs→τ+τ− up to six times larger than the SM. In the context of neutrino lepton flavour violation mediated by leptoquarks we find that the current experimental upper bounds on RK(⁎)ν are already more constraining than direct bounds from Bs→τℓ and B→K(⁎)τℓ modes for ℓ=e,μ.

Highlights

  • Rare B decays play an important role in understanding the dynamics of the standard model (SM) as well as being a fertile ground for the search for new physics

  • We consider possible contributions from neutrino flavour violating final states in the context of scalar and vector leptoquarks. These contributions are correlated to the charged lepton flavour violating (CLFV) modes Bs → and B → K(∗) and we find that the current limits on B → K(∗)ννare more restrictive for modes with tau-leptons

  • We have studied the modes B → K(∗)ννin the context of non-standard neutrino interactions

Read more

Summary

Introduction

Rare B decays play an important role in understanding the dynamics of the standard model (SM) as well as being a fertile ground for the search for new physics. We consider possible contributions from neutrino flavour violating final states in the context of scalar and vector leptoquarks These contributions are correlated to the charged lepton flavour violating (CLFV) modes Bs → and B → K(∗) and we find that the current limits on B → K(∗)ννare more restrictive for modes with tau-leptons. These results are usually presented as ratios, for which we obtain.

Effective Hamiltonian at the b scale
An additional light neutrino
Models with leptoquarks
The B anomalies
Findings
Summary

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

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.