ログイン
言語:

WEKO3

  • トップ
  • ランキング
To
lat lon distance
To

Field does not validate



インデックスリンク

インデックスツリー

メールアドレスを入力してください。

WEKO

One fine body…

WEKO

One fine body…

アイテム

  1. 学術雑誌論文等

Cosmological family asymmetry and CP violation

https://hiroshima.repo.nii.ac.jp/records/2008427
https://hiroshima.repo.nii.ac.jp/records/2008427
6a47397d-6aea-4222-b5aa-1ff331c8a0c7
名前 / ファイル ライセンス アクション
PhysRevD_72_016006.pdf PhysRevD_72_016006.pdf (1.2 MB)
Item type デフォルトアイテムタイプ_(フル)(1)
公開日 2023-03-18
タイトル
タイトル Cosmological family asymmetry and CP violation
言語 en
作成者 Fujihara, Takahiro

× Fujihara, Takahiro

en Fujihara, Takahiro

Search repository
Kaneko, Satoru

× Kaneko, Satoru

en Kaneko, Satoru

Search repository
Kang, Sin Kyu

× Kang, Sin Kyu

en Kang, Sin Kyu

Search repository
Kimura, Daiji

× Kimura, Daiji

en Kimura, Daiji

Search repository
Morozumi, Takuya

× Morozumi, Takuya

en Morozumi, Takuya

Search repository
Tanimoto, Morimitsu

× Tanimoto, Morimitsu

en Tanimoto, Morimitsu

Search repository
アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
権利情報
権利情報 Copyright (c) 2005 The American Physical Society.
内容記述
内容記述 We discuss how the cosmological baryon asymmetry can be achieved by the lepton family asymmetries of heavy Majorana neutrino decays and how the lepton family asymmetries are related to CP violation in neutrino oscillation, in the minimal seesaw model with two heavy Majorana neutrinos. We derive the most general formula for CP violation in neutrino oscillation in terms of the heavy Majorana masses and Yukawa mass term. It is shown that the formula is very useful to classify several models in which e, μ, and τ leptogenesis can be separately realized and to see how they are connected with low energy CP violation. To make the models predictive, we take texture with two zeros in the Dirac matrix. In particular, we find some interesting cases in which CP violation in neutrino oscillation can happen while lepton family asymmetries do not exist at all. On the contrary, we can find e-, μ-, and τ-leptogenesis scenarios in which the cosmological CP violation and low energy CP violation measurable via neutrino oscillations are very closely related to each other. By determining the allowed ranges of the parameters in the models, we predict the sizes of CP violation in neutrino oscillation and |Ve3MNS|. Finally, the leptonic unitarity triangles are reconstructed.
言語 en
出版者
出版者 American Physical Society
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
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
関連情報
識別子タイプ DOI
関連識別子 10.1103/PhysRevD.72.016006
関連情報
識別子タイプ DOI
関連識別子 http://dx.doi.org/10.1103/PhysRevD.72.016006
収録物識別子
収録物識別子タイプ ISSN
収録物識別子 1550-7998
収録物識別子
収録物識別子タイプ NCID
収録物識別子 AA00773624
開始ページ
開始ページ 016006-1
書誌情報 Physical Review D - Particles, Fields, Gravitation and Cosmology
Physical Review D - Particles, Fields, Gravitation and Cosmology

巻 72, 号 1, p. 016006-1-016006-12, 発行日 2005-07-27
旧ID 19282
戻る
0
views
See details
Views

Versions

Ver.1 2025-02-21 04:23:20.917745
Show All versions

Share

Mendeley Twitter Facebook Print Addthis

Cite as

エクスポート

OAI-PMH
  • OAI-PMH JPCOAR 2.0
  • OAI-PMH JPCOAR 1.0
  • OAI-PMH DublinCore
  • OAI-PMH DDI
Other Formats
  • JSON
  • BIBTEX

Confirm


Powered by WEKO3


Powered by WEKO3