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Fermionic dark matter in radiative inverse seesaw model with U(1) B-L
http://hdl.handle.net/2297/32483
http://hdl.handle.net/2297/32483d589a385-3b55-4035-b502-5dba4458a799
| 名前 / ファイル | ライセンス | アクション |
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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 | 2017-10-03 | |||||
| タイトル | ||||||
| タイトル | Fermionic dark matter in radiative inverse seesaw model with U(1) B-L | |||||
| 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 |
Okada, Hiroshi
× Okada, Hiroshi× Toma, Takashi |
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| 書誌情報 |
Physical Review D - Particles, Fields, Gravitation and Cosmology 巻 86, 号 3, p. 33011, 発行日 2012-08-27 |
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| ISSN | ||||||
| 収録物識別子タイプ | ISSN | |||||
| 収録物識別子 | 1550-7998 | |||||
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| 収録物識別子タイプ | NCID | |||||
| 収録物識別子 | AA00773624 | |||||
| DOI | ||||||
| 関連タイプ | isIdenticalTo | |||||
| 識別子タイプ | DOI | |||||
| 関連識別子 | 10.1103/PhysRevD.86.033011 | |||||
| 出版者 | ||||||
| 出版者 | American Physical Society | |||||
| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | We construct a radiative inverse seesaw model with local B-L symmetry, and investigate the flavor structure of the lepton sector and the fermionic dark matter. Neutrino masses are radiatively generated through a kind of inverse seesaw framework. The Pontecorvo-Maki-Nakagawa-Sakata matrix is derived from each mixing matrix of the neutrino and charged lepton sector with a large Dirac CP phase. We show that the annihilation processes via the interactions with Higgses, which are independent on the lepton flavor violation, have to be dominant in order to satisfy the observed relic abundance by WMAP. The new interactions with Higgses allow us to be consistent with the direct detection result reported by XENON100, and it is possible to verify the model by the exposure of XENON100 (2012). © 2012 American Physical Society. | |||||
| 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 | |||||