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Neutrino oscillation based on a $\sim$ 10 eV neutrino
We study a consistent explanation for both deficits of solar neutrino and atmospheric neutrino due to the neutrino oscillation induced by the mixing of five light neutrinos with a heavy right-handed neutrino. Although this scenario contains only one nonzero mass eigenvalue \sim 10~eV for these five...
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| Lenguaje: | eng |
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1996
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| Acceso en línea: | https://dx.doi.org/10.1016/S0370-2693(96)01588-2 http://cds.cern.ch/record/300578 |
| _version_ | 1780889443451797504 |
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| author | Suematsu, Daijiro |
| author_facet | Suematsu, Daijiro |
| author_sort | Suematsu, Daijiro |
| collection | CERN |
| description | We study a consistent explanation for both deficits of solar neutrino and atmospheric neutrino due to the neutrino oscillation induced by the mixing of five light neutrinos with a heavy right-handed neutrino. Although this scenario contains only one nonzero mass eigenvalue \sim 10~eV for these five neutrino states, it can consistently explain both deficiency. It can also naturally present a suitable hot dark matter candidate as its own feature. We propose a phenomenological model for the neutrino mass matrix which realizes such a scenario in the simple three generation left and right handed neutrino framework. |
| id | cern-300578 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 1996 |
| record_format | invenio |
| spelling | cern-3005782023-03-14T19:29:25Zdoi:10.1016/S0370-2693(96)01588-2http://cds.cern.ch/record/300578engSuematsu, DaijiroNeutrino oscillation based on a $\sim$ 10 eV neutrinoParticle Physics - PhenomenologyWe study a consistent explanation for both deficits of solar neutrino and atmospheric neutrino due to the neutrino oscillation induced by the mixing of five light neutrinos with a heavy right-handed neutrino. Although this scenario contains only one nonzero mass eigenvalue \sim 10~eV for these five neutrino states, it can consistently explain both deficiency. It can also naturally present a suitable hot dark matter candidate as its own feature. We propose a phenomenological model for the neutrino mass matrix which realizes such a scenario in the simple three generation left and right handed neutrino framework.We study a consistent explanation for both deficits of solar neutrino and atmospheric neutrino due to the neutrino oscillation induced by the mixing of five light neutrinos with a heavy right-handed neutrino. Although this scenario contains only one nonzero mass eigenvalue $\sim 10$eV for these five neutrino states, it can consistently explain both deficiency. It can also naturally present a suitable hot dark matter candidate as its own feature. We propose a phenomenological model for the neutrino mass matrix which realizes such a scenario in the simple three generation left and right handed neutrino framework.We study a consistent explanation for both deficits of solar neutrino and atmospheric neutrino due to the neutrino oscillation induced by the mixing of five light neutrinos with a heavy right-handed neutrino. Although this scenario contains only one nonzero mass eigenvalue $\sim 10$eV for these five neutrino states, it can consistently explain both deficiency. It can also naturally present a suitable hot dark matter candidate as its own feature. We propose a phenomenological model for the neutrino mass matrix which realizes such a scenario in the simple three generation left and right handed neutrino framework.We study a consistent explanation for both deficits of solar neutrino and atmospheric neutrino due to the neutrino oscillation induced by the mixing of five light neutrinos with a heavy right-handed neutrino. Although this scenario contains only one nonzero mass eigenvalue $\sim 10$eV for these five neutrino states, it can consistently explain both deficiency. It can also naturally present a suitable hot dark matter candidate as its own feature. We propose a phenomenological model for the neutrino mass matrix which realizes such a scenario in the simple three generation left and right handed neutrino framework.We study a consistent explanation for both deficits of solar neutrino and atmospheric neutrino due to the neutrino oscillation induced by the mixing of five light neutrinos with a heavy right-handed neutrino. Although this scenario contains only one nonzero mass eigenvalue $\sim 10$eV for these five neutrino states, it can consistently explain both deficiency. It can also naturally present a suitable hot dark matter candidate as its own feature. We propose a phenomenological model for the neutrino mass matrix which realizes such a scenario in the simple three generation left and right handed neutrino framework.We study a consistent explanation for both deficits of solar neutrino and atmospheric neutrino due to the neutrino oscillation induced by the mixing of light neutrinos with a heavy right-handed neutrino. We propose such a phenomenological neutrino mass matrix that realizes this scenario in the simple three generation left- and right- handed neutrino framework. Although this model contains only one nonzero mass eigenvalue ∼ 10 eV for these light neutrino states at the first approximation level, it can be expected to explain consistently both deficiencies due to the appropriate higher order corrections. A suitable hot dark matter candidate is naturally included in it as its own feature.hep-ph/9604242KANAZAWA-96-04KANAZAWA-96-04oai:cds.cern.ch:3005781996-04-04 |
| spellingShingle | Particle Physics - Phenomenology Suematsu, Daijiro Neutrino oscillation based on a $\sim$ 10 eV neutrino |
| title | Neutrino oscillation based on a $\sim$ 10 eV neutrino |
| title_full | Neutrino oscillation based on a $\sim$ 10 eV neutrino |
| title_fullStr | Neutrino oscillation based on a $\sim$ 10 eV neutrino |
| title_full_unstemmed | Neutrino oscillation based on a $\sim$ 10 eV neutrino |
| title_short | Neutrino oscillation based on a $\sim$ 10 eV neutrino |
| title_sort | neutrino oscillation based on a $\sim$ 10 ev neutrino |
| topic | Particle Physics - Phenomenology |
| url | https://dx.doi.org/10.1016/S0370-2693(96)01588-2 http://cds.cern.ch/record/300578 |
| work_keys_str_mv | AT suematsudaijiro neutrinooscillationbasedonasim10evneutrino |