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Baryon number asymmetry and dark matter in the neutrino mass model with an inert doublet
https://doi.org/10.24517/00064642
https://doi.org/10.24517/000646427fe74078-7990-4573-b61f-eebe3167c0af
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
SC-PR-SUEMATSU-D-053001.pdf (454.4 kB)
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| Item type | 学術雑誌論文 / Journal Article(1) | |||||||
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| 公開日 | 2022-01-07 | |||||||
| タイトル | ||||||||
| タイトル | Baryon number asymmetry and dark matter in the neutrino mass model with an inert doublet | |||||||
| 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 | 10.24517/00064642 | |||||||
| 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 |
Physical Review D - Particles, Fields, Gravitation and Cosmology 巻 86, 号 5, p. 053001, 発行日 2012-09-11 |
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| ISSN | ||||||||
| 収録物識別子タイプ | ISSN | |||||||
| 収録物識別子 | 1550-7998 | |||||||
| ISSN | ||||||||
| 収録物識別子タイプ | ISSN | |||||||
| 収録物識別子 | 1550-2368 | |||||||
| NCID | ||||||||
| 収録物識別子タイプ | NCID | |||||||
| 収録物識別子 | AA00773624 | |||||||
| DOI | ||||||||
| 関連タイプ | isVersionOf | |||||||
| 識別子タイプ | DOI | |||||||
| 関連識別子 | 10.1103/PhysRevD.86.053001 | |||||||
| 出版者 | ||||||||
| 出版者 | American Physical Society | |||||||
| 抄録 | ||||||||
| 内容記述タイプ | Abstract | |||||||
| 内容記述 | The radiative neutrino mass model with an inert doublet scalar has been considered as a promising candidate which can explain neutrino masses, dark matter abundance and baryon number asymmetry if dark matter is identified with the lightest neutral component of the inert doublet. We reexamine these properties by imposing all the data of the neutrino oscillation, which are recently suggested by the reactor experiments. We find that the sufficient baryon number asymmetry seems not to be easily generated in a consistent way with all the data of the neutrino masses and mixing as long as the right-handed neutrinos are kept in TeV regions. Two possible modifications of the model are examined. © 2012 American Physical Society. | |||||||
| 権利 | ||||||||
| 権利情報 | Copyright © American Physical Society | |||||||
| 著者版フラグ | ||||||||
| 出版タイプ | AM | |||||||
| 出版タイプResource | http://purl.org/coar/version/c_ab4af688f83e57aa | |||||||
| 関連URI | ||||||||
| 識別子タイプ | URI | |||||||
| 関連識別子 | http://prd.aps.org/ | |||||||
| 関連名称 | http://prd.aps.org/ | |||||||
