Abstract

We study the structure of the neutrino-mass matrix in the minimal gauged hbox {U}(1)_{L_mu -L_tau } model, where three right-handed neutrinos are added to the Standard Model in order to obtain non-zero masses for the active neutrinos. Because of the hbox {U}(1)_{L_mu -L_tau } gauge symmetry, the structure of both Dirac and Majorana mass terms of neutrinos is tightly restricted. In particular, the inverse of the neutrino-mass matrix has zeros in the (mu ,mu ) and (tau ,tau ) components, namely, this model offers a symmetric realization of the so-called two-zero-minor structure in the neutrino-mass matrix. Due to these constraints, all the CP phases – the Dirac CP phase delta and the Majorana CP phases alpha _2 and alpha _3 – as well as the mass eigenvalues of the light neutrinos m_i are uniquely determined as functions of the neutrino mixing angles theta _{12}, theta _{23}, and theta _{13}, and the squared mass differences Delta m_{21}^2 and Delta m_{31}^2. We find that this model predicts the Dirac CP phase delta to be delta simeq 1.59pi –1.70pi (1.54pi –1.78pi ), the sum of the neutrino masses to be sum _{i}m_i simeq 0.14–0.22 eV (0.12–0.40 eV), and the effective mass for the neutrinoless double-beta decay to be langle m_{beta beta }rangle simeq 0.024–0.055 eV (0.017–0.12 eV) at 1sigma (2sigma ) level, which are totally consistent with the current experimental limits. These predictions can soon be tested in future neutrino experiments. Implications for leptogenesis are also discussed.

Highlights

  • Due to these constraints, all the CP phases – the Dirac CP phase δ and the Majorana CP phases α2 and α3 – as well as the mass eigenvalues of the light neutrinos mi are uniquely determined as functions of the neutrino mixing angles θ12, θ23, and θ13, and the squared mass differences m m231

  • We find that this model predicts the Dirac CP phase δ to be δ 1.59π –1.70π (1.54π –1.78π ), the sum of the neutrino masses to be i mi 0.14–0.22 eV (0.12–0.40 eV), and the effective mass for the neutrinoless double-beta decay to be mββ 0.024–0.055 eV (0.017–0.12 eV) at 1σ (2σ ) level, which are totally consistent with the current experimental limits

  • We have studied the structure of the neutrino-mass matrix in the minimal gauged U(1)Lμ−Lτ model

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Summary

Introduction

Offer promising candidates for dark matter in the Universe [18,19,20,21,22]. For other recent studies on gauged U(1)Lμ−Lτ models, see Refs. [23,24,25,26,27,28,29,30,31,32,33,34,35]. It turns out that the observed neutrino mixing structure can be obtained only when the U(1)Lμ−Lτ -breaking scalar field has the U(1)Lμ−Lτ charge ±1 In this case, the (μ, μ) and (τ, τ ) components of the Majorana mass matrix for the right-handed neutrinos remain zero even after the. (e, τ ), (μ, e), and (τ, e) components in Eq (2) can be induced after the scalar field acquires a VEV, while the (μ, μ) and (τ, τ ) can be generated if the scalar has the U(1)Lμ−Lτ charge ± 2 In the latter case, the Majorana mass matrix becomes block-diagonal, which makes it unable to explain the observed neutrino mixing angles.

In terms of the squared mass differences m m 22
Predictions for the neutrino parameters
Implications for Leptogenesis
Conclusions
A Miscellaneous formulas
R2 and R3
Neutrino-mass matrix MνL
Cubic equation for cos δ
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