WEKO3
アイテム
Neutrino mass due to the mixing among neutrinos and gauginos
https://doi.org/10.24517/00064616
https://doi.org/10.24517/00064616f37bdaee-e4b0-4b72-a323-fe76f344e0e9
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
|
|
| アイテムタイプ | 学術雑誌論文 / Journal Article(1) | |||||||
|---|---|---|---|---|---|---|---|---|
| 公開日 | 2022-01-27 | |||||||
| タイトル | ||||||||
| タイトル | Neutrino mass due to the mixing among neutrinos and gauginos | |||||||
| 言語 | ||||||||
| 言語 | eng | |||||||
| 資源タイプ | ||||||||
| 資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||||
| 資源タイプ | journal article | |||||||
| ID登録 | ||||||||
| ID登録 | 10.24517/00064616 | |||||||
| ID登録タイプ | JaLC | |||||||
| 著者 |
Suematsu, Daijiro
× Suematsu, Daijiro |
|||||||
| 著者別表示 |
末松, 大二郎
× 末松, 大二郎
|
|||||||
| 提供者所属 | ||||||||
| 内容記述タイプ | Other | |||||||
| 内容記述 | 金沢大学理工研究域数物科学系 | |||||||
| 書誌情報 |
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics 巻 506, 号 1-2, p. 131-139, 発行日 2001 |
|||||||
| ISSN | ||||||||
| 収録物識別子タイプ | ISSN | |||||||
| 収録物識別子 | 0370-2693 | |||||||
| NCID | ||||||||
| 収録物識別子タイプ | NCID | |||||||
| 収録物識別子 | AA11537044 | |||||||
| DOI | ||||||||
| 関連タイプ | isIdenticalTo | |||||||
| 識別子タイプ | DOI | |||||||
| 関連識別子 | 10.1016/S0370-2693(01)00413-0 | |||||||
| 出版者 | ||||||||
| 出版者 | Elsevier B.V. | |||||||
| 抄録 | ||||||||
| 内容記述タイプ | Abstract | |||||||
| 内容記述 | We consider the explanation of both data of the atmospheric neutrino and the solar neutrino by the neutrino mass matrix derived from the mixing of neutrinos and gauginos in the extended MSSM with an extra U(1) gauge symmetry. This scenario directly relates the neutrino mass to supersymmetry. The structure of the mass hierarchy and the mixing is determined only by the extra U(1)-charge of neutrinos. Although the model is rather simple, it may be able to realize both the small and large mixing angle solutions for the solar neutrino problem. In particular, the large mixing angle MSW solution for the solar neutrino problem can be easily realized. We discuss the relation between the extra U(1)-charge and four solutions for the solar neutrino problem. © 2001 Published by Elsevier Science B.V. | |||||||
| 権利 | ||||||||
| 権利情報 | Copyright © 2001 Elsevier (CC-BY-NC-ND) | |||||||
| 著者版フラグ | ||||||||
| 出版タイプ | VoR | |||||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||||
| 関連URI | ||||||||
| 識別子タイプ | URI | |||||||
| 関連識別子 | https://www.journals.elsevier.com/physics-letters-b/ | |||||||
| 関連名称 | https://www.journals.elsevier.com/physics-letters-b/ | |||||||