Two-loop Radiative Corrections to Neutrino Masses in $SU(3)_L \times U(1)_N$ Gauge Models
| dc.creator | Kitabayashi, Teruyuki | |
| dc.date | 2000-10-31 | |
| dc.date.accessioned | 2026-07-07T03:43:06Z | |
| dc.date.available | 2026-07-07T03:43:06Z | |
| dc.description | We have constructed two $SU(3)_L \times U(1)_N$ gauge models with the $L^\prime = L_e-L_μ-L_τ$ symmetry, which accommodate tiny neutrino masses generated by one-loop and two-loop radiative effects. The heavy neutral leptons and heavy charged leptons are employed to specify the lepton triplets in $SU(3)_L$, respectively, accompanied by ($ϕ^0$, $ϕ^-$, $h^+$) and ($ϕ^+$, $ϕ^0$, $h^+$), where $ϕ$ stands for the standard Higgs scalar and $h^+$ is a key ingredient for radiative mechanisms. From our numerical calculations, we find that both our models are relevant to yield the VO solution to the solar neutrino problem. | |
| dc.description | Talk at Post Summer Institute 2000 on Neutrino Physics, August 21-24, 2000, Fuji-Yoshida, Japan | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0010341 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0010341 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/40102 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Two-loop Radiative Corrections to Neutrino Masses in $SU(3)_L \times U(1)_N$ Gauge Models | |
| dc.type | text |