Perturbations to the μτ symmetry, leptogenesis, and lepton flavor violation with the type II seesaw mechanism

Manikanta Borah, Debasish Borah, Mrinal Kumar Das, and Sudhanwa Patra
Phys. Rev. D 90, 095020 – Published 21 November 2014

Abstract

We study the possibility of generating nonzero reactor mixing angle θ13 by perturbing the μτ symmetric neutrino mass matrix. The leading-order μτ symmetric neutrino mass matrix originates from a type I seesaw mechanism, whereas the perturbations to μτ symmetry originate from a type II seesaw term. We consider four different realizations of μτ symmetry, bimaximal mixing, tribimaximal mixing, hexagonal mixing, and golden ratio mixing, all giving rise to θ13=0,θ23=π4 but different nonzero values of solar mixing angle θ12. We assume a minimal μτ symmetry breaking type II seesaw mass matrix as a perturbation and calculate the neutrino oscillation parameters as a function of type II seesaw strength. We then consider the origin of nontrivial leptonic CP phase in the charged lepton sector and calculate the lepton asymmetry arising from the lightest right-handed neutrino decay by incorporating the presence of both type I and type II seesaws. We constrain the type II seesaw strength as well as the leptonic CP phase (and hence the charged lepton sector) by comparing our results with experimental neutrino oscillation parameters as well as the Planck bound on the baryon-to-photon ratio. Finally, we extend our analysis on lepton flavor violating decays like μeγ and μeee due to the exchange of a TeV scale Higgs triplet scalar within the low scale type II seesaw framework. The branching ratios for these lepton flavor processes are examined with the small type II perturbation term ω, and the estimated values are very close to the experimental bound coming from current search experiments.

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  • Received 19 August 2014

DOI:https://doi.org/10.1103/PhysRevD.90.095020

© 2014 American Physical Society

Authors & Affiliations

Manikanta Borah*, Debasish Borah, and Mrinal Kumar Das

  • Department of Physics, Tezpur University, Tezpur 784028, India

Sudhanwa Patra§

  • Center of Excellence in Theoretical and Mathematical Sciences, Siksha O Anusandhan University, Bhubaneswar 751030, India

  • *mani@tezu.ernet.in
  • dborah@tezu.ernet.in
  • mkdas@tezu.ernet.in
  • §sudha.astro@gmail.com

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Issue

Vol. 90, Iss. 9 — 1 November 2014

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