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An extension of the SM based on effective Peccei–Quinn Symmetry
https://doi.org/10.24517/00064633
https://doi.org/10.24517/0006463375f8e792-447b-4e4f-9b25-9b108550c193
| 名前 / ファイル | ライセンス | アクション |
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SC-PR-SUEMATSU-D-881.pdf (645.3 kB)
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| Item type | 学術雑誌論文 / Journal Article(1) | |||||||
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| 公開日 | 2022-01-20 | |||||||
| タイトル | ||||||||
| タイトル | An extension of the SM based on effective Peccei–Quinn Symmetry | |||||||
| 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 | 10.24517/00064633 | |||||||
| ID登録タイプ | JaLC | |||||||
| 著者 |
Suematsu, Daijiro
× Suematsu, Daijiro |
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| 著者別表示 |
末松, 大二郎
× 末松, 大二郎
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| 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 |
European Physical Journal C 巻 78, 号 11, p. 881, 発行日 2018 |
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| ISSN | ||||||||
| 収録物識別子タイプ | ISSN | |||||||
| 収録物識別子 | 1434-6044 | |||||||
| NCID | ||||||||
| 収録物識別子タイプ | NCID | |||||||
| 収録物識別子 | AA11188397 | |||||||
| DOI | ||||||||
| 関連タイプ | isIdenticalTo | |||||||
| 識別子タイプ | DOI | |||||||
| 関連識別子 | 10.1140/epjc/s10052-018-6370-3 | |||||||
| 出版者 | ||||||||
| 出版者 | Springer New York LLC | |||||||
| 抄録 | ||||||||
| 内容記述タイプ | Abstract | |||||||
| 内容記述 | Peccei–Quinn (PQ) mechanism based on a chiral global U(1) symmetry is considered to be a simple and elegant solution for strong CP problem. The fact that the mechanism could be experimentally examined through the axion search makes it much more interesting and recently it causes a lot of attention again. However, it is also known that the mechanism is annoyed by two serious problems, that is, a domain wall problem and goodness of global symmetry. Any global symmetry is considered not to be exact due to the quantum effect of gravity. In this paper, we consider a solution to these problems, in which quark mass hierarchy and mixing, neutrino mass generation and existence of dark matter are closely related. In our solution, PQ symmetry is assumed to be induced through symmetry breaking at an intermediate scale of a local U(1) symmetry, and a global U(1) symmetry which plays a role of Froggatt–Nielsen symmetry. In the lepton sector, a remnant of the PQ symmetry controls neutrino mass generation and dark matter existence. © 2018, The Author(s). | |||||||
| 権利 | ||||||||
| 権利情報 | The final publication is available at www.springerlink.com/article/10.1140/epjc/s10052-018-6370-3 | |||||||
| 権利 | ||||||||
| 権利情報 | Copyright © 2018, The Author(s). | |||||||
| 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://link.springer.com/article/10.1140/epjc/s10052-018-6370-3 | |||||||
| 関連名称 | https://link.springer.com/article/10.1140/epjc/s10052-018-6370-3 | |||||||
| 関連URI | ||||||||
| 識別子タイプ | URI | |||||||
| 関連識別子 | http://epjc.epj.org/ | |||||||
| 関連名称 | http://epjc.epj.org/ | |||||||
