2-loop Radiative Corrections to Neutrino Masses in SU(3)L×U(1)N Gauge Model (ニュートリノをめぐって)
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概要
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We have constructed two SU(3)_L×U(1)_N gauge models with the L' = 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.
- 素粒子論グループ 素粒子研究編集部の論文
- 2001-03-20
著者
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北林 照幸
Accelerator Engineering Center, Mitsubishi Electric System & Service Engineering Co. Ltd.
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北林 照幸
Accelerator Engineering Center Mitsubishi Electric System & Service Engineering Co. Ltd.
関連論文
- Neutrino Oscillations Induced by Two-loop Radiative Effects (ニュートリノをめぐって)
- 2-loop Radiative Corrections to Neutrino Masses in SU(3)L×U(1)N Gauge Model (ニュートリノをめぐって)