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Universal Extra Dimension models with right-handed neutrinos.
https://sucra.repo.nii.ac.jp/records/13771
https://sucra.repo.nii.ac.jp/records/13771f5b62a69-a9da-4903-b28e-716588143beb
名前 / ファイル | ライセンス | アクション |
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A1003468.pdf (33.1 kB)
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Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2010-03-02 | |||||
タイトル | ||||||
タイトル | Universal Extra Dimension models with 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 | |||||
著者 |
Matsumoto, Shigeki
× Matsumoto, Shigeki× 佐藤, 丈× Senami, Masato× Yamanaka, Masato |
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著者 ローマ字 | ||||||
Matsumoto, Shigeki | ||||||
著者 ローマ字 | ||||||
Sato, Joe | ||||||
著者 ローマ字 | ||||||
Senami, Masato | ||||||
著者 ローマ字 | ||||||
Yamanaka, Masato | ||||||
著者 所属 | ||||||
著者 所属 | ||||||
埼玉大学大学院理工学研究科物質科学部門 | ||||||
著者 所属(別言語) | ||||||
Institute for International Advanced Interdisciplinary Research, Tohoku University | ||||||
著者 所属(別言語) | ||||||
Department of Physics, Saitama University | ||||||
著者 所属(別言語) | ||||||
ICRR, University of Tokyo | ||||||
著者 所属(別言語) | ||||||
Department of Physics, Saitama University | ||||||
書誌情報 |
HIGH ENERGY PHYSICS AND APPLICATIONS: Proceedings of the UAE-CERN 巻 1006, 号 1, p. 122-125, 発行日 2008 |
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年月次 | ||||||
2008-4 | ||||||
出版者名 | ||||||
出版者 | American Institute of Physics | |||||
DOI | ||||||
関連タイプ | isVersionOf | |||||
識別子タイプ | DOI | |||||
関連識別子 | info:doi/10.1063/1.2927597 | |||||
関連サイト | ||||||
内容記述タイプ | Other | |||||
内容記述 | http://link.aip.org/link/?APCPCS/1006/122/1 | http://link.aip.org/link/?APCPCS/1006/122/1 | |||||
識別番号 その他 | ||||||
内容記述タイプ | Other | |||||
内容記述 | arXiv:0810.0700v1 [hep-ph] | |||||
抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | Relic abundance of dark matter is investigated in the framework of universal extra dimension (UED) models with right-handed neutrinos. These models are free from the KK graviton problem in the minimal UED model. The first KK particle of the right-handed neutrino is a dark matter candidate in this framework. When ordinary neutrino masses are large enough such as the degenerate mass spectrum case, the dark matter relic abundance can increase significantly. The scale of the extra dimension consistent with cosmological observations can be 500 GeV in the minimal setup of UED models with right-handed neutrinos. ©2008 American Institute of Physics | |||||
版 | ||||||
[著者版] | ||||||
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 | |||||
資源タイプ | ||||||
内容記述タイプ | Other | |||||
内容記述 | text | |||||
フォーマット | ||||||
内容記述タイプ | Other | |||||
内容記述 | application/pdf | |||||
作成日 | ||||||
日付 | 2010-03-02 | |||||
日付タイプ | Created | |||||
アイテムID | ||||||
A1003468 |