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Inflation in a modified radiative seesaw model
https://doi.org/10.24517/00064641
https://doi.org/10.24517/000646411d3d9c47-f769-46d9-8421-93875b1553ba
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
SC-PR-SUEMATSU-D-113013.pdf (508.7 kB)
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| アイテムタイプ | 学術雑誌論文 / Journal Article(1) | |||||||
|---|---|---|---|---|---|---|---|---|
| 公開日 | 2022-01-07 | |||||||
| タイトル | ||||||||
| タイトル | Inflation in a modified radiative seesaw model | |||||||
| 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 | 10.24517/00064641 | |||||||
| ID登録タイプ | JaLC | |||||||
| 著者 |
Budhi, Romy H. S.
× Budhi, Romy H. S.× 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 90, 号 11, p. 113013, 発行日 2014-12-23 |
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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.90.113013 | |||||||
| 出版者 | ||||||||
| 出版者 | American Physical Society | |||||||
| 抄録 | ||||||||
| 内容記述タイプ | Abstract | |||||||
| 内容記述 | The existence of the inflationary era in the early Universe seems to be strongly supported by recent CMB observations. However, only a few realistic inflation scenarios which have close relation to particle physics seem to have been known unfortunately. The radiative neutrino mass model with inert doublet dark matter is a promising model for the present experimental issues which cannot be explained within the standard model. In order to make the model include inflation, we extend it by a complex scalar field with a specific potential. This scalar could be closely related to the neutrino mass generation at a TeV scale as well as inflation. We show that the inflation favored by the CMB observations could be realized even if inflaton takes sub-Planck values during inflation. © 2014 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/ | |||||||
