Abstract

We study the gauged U(1)_{L_mu -L_tau } scotogenic model with emphasis on latest measurement of LHCb R_{K^{(*)}} anomaly and AMS-02 positron excess. In this model, neutrino masses are induced at one-loop level with Z_2-odd particles, i.e., right-handed neutrinos N_ell (ell =e,mu ,tau ) and inert scalar doublet eta inside the loop. Meanwhile, the gauged U(1)_{L_mu -L_tau } symmetry is broken spontaneously by the scalar singlet S, resulting to the massive gauge boson Z'. Provided certain couplings to quarks induced by heavy vector-like quarks, the gauge boson Z' would contribute to the transition brightarrow s mu ^+mu ^-, hence explain the R_{K^{(*)}} anomaly. As for the Majorana fermion DM N, the gauge boson Z' and the singlet Higgs H_0 will generate various annihilation channels, among which the NNrightarrow Z'Z' and NNrightarrow Z'H_0(rightarrow Z'Z') channel could be used to interpret the AMS-02 positron excess. We give a comprehensive analysis on model parameter space with consider various current constraints. The combined analysis shows that the R_{K^{(*)}} anomaly and AMS-02 positron excess can be explained simultaneously.

Highlights

  • Tiny neutrino mass and non-baryonic dark matter (DM) are the two missing pieces of standard model (SM)

  • Except the evidences from neutrino mass and DM, the hint from flavor physics may call for the physics beyond standard model (BSM)

  • Neutrino masses are generated at one-loop level via N and η propagating in the loop as the original scotogenic model

Read more

Summary

Introduction

Tiny neutrino mass and non-baryonic dark matter (DM) are the two missing pieces of standard model (SM). An appealing pathway to link them together is the scotogenic model [1,2], which realizes tiny neutrino mass via radiative process [3,4,5] with DM running in the loop. The indirect detection experiments, such as PAMELA [132], Fermi-LAT [133], and AMS-02 [134,135,136], have reported a significance positron fraction excess in the cosmic-ray, while no obvious antiproton excess is observed [137] This can be interpreted by DM dominantly annihilating into leptonic final states [138,139,140,141,142].2.

Model setup
Neutrino mass
Ld23 M Z2
Constraints
Dark matter phenomenology
AMS-02 positron flux
AMS-02 antiproton constraint
Fermi-LAT EGRB constraint
Planck CMB constraint
Conclusion
Full Text
Paper version not known

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