Phenomenological Neutrino Mass Matrix for Neutrino Oscillations and Dark Matter
スポンサーリンク
概要
- 論文の詳細を見る
A phenomenological neutrino mass matrix is proposed to explain the solar and atmospheric neutrino deficits and to present the neutrino as a candidate of hot dark matter in the 3ν_L+3ν_R framework. the realization of mixing angles which can explain the solar and atmospheric neutrino problems is taken as the first criterion in this construction. The differences among neutrino mass eigenvalues are introduced as a perturbation. In this scheme the structure of a charged lepton mass matrix is not severely constrained by the solar and atmospheric neutrino date.
- 理論物理学刊行会の論文
- 1998-03-25
著者
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Suematsu D
Kanazawa Univ.
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Suematsu Daijiro
Department Of Physics Kanazawa University
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SUEMATSU Daijiro
Department of Physics, Kanazawa University
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SUEMATSU Daijiro
Institute for Theoretical Physics, Faculty of Science, Kanazawa University
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SUEMATSU Daijiro
Institute for Theoretical Physics, University of Bern
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