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Radiative neutrino mass model with degenerate right-handed neutrinos
https://doi.org/10.24517/00064635
https://doi.org/10.24517/0006463545a4a81e-4e6d-4341-96e5-87bbfce2e03f
| 名前 / ファイル | ライセンス | アクション |
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SC-PR-SUEMATSU-D-117.pdf (920.7 kB)
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| アイテムタイプ | 学術雑誌論文 / Journal Article(1) | |||||||
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| 公開日 | 2022-01-07 | |||||||
| タイトル | ||||||||
| タイトル | Radiative neutrino mass model with degenerate right-handed neutrinos | |||||||
| 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 | 10.24517/00064635 | |||||||
| ID登録タイプ | JaLC | |||||||
| 著者 |
Kashiwase, Shoichi
× Kashiwase, Shoichi× 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 76, 号 3, p. 117, 発行日 2016-03-01 |
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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/s10052-016-3964-5 | |||||||
| 出版者 | ||||||||
| 出版者 | Springer New York LLC | |||||||
| 抄録 | ||||||||
| 内容記述タイプ | Abstract | |||||||
| 内容記述 | The radiative neutrino mass model can relate neutrino masses and dark matter at a TeV scale. If we apply this model to thermal leptogenesis, we need to consider resonant leptogenesis at that scale. It requires both finely degenerate masses for the right-handed neutrinos and a tiny neutrino Yukawa coupling. We propose an extension of the model with a U(1) gauge symmetry, in which these conditions are shown to be simultaneously realized through a TeV scale symmetry breaking. Moreover, this extension can bring about a small quartic scalar coupling between the Higgs doublet scalar and an inert doublet scalar which characterizes the radiative neutrino mass generation. It also is the origin of the (Formula presented.) symmetry which guarantees the stability of dark matter. Several assumptions which are independently supposed in the original model are closely connected through this extension. © 2016, The Author(s). | |||||||
| 権利 | ||||||||
| 権利情報 | The final publication is available at www.springerlink.com/article/10.1140/epjc/s10052-016-3964-5 | |||||||
| 権利 | ||||||||
| 権利情報 | Copyright © The Author(s) 2016. This article is published with open access at Springerlink.com | |||||||
| 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 | http://epjc.epj.org/ | |||||||
| 関連名称 | http://epjc.epj.org/ | |||||||
