UTAPwiki/セミナー/初期宇宙・相対論速報

Title: A Nelson-Barr model

Speaker: Kohei Fujikura

Several solutions to the strong CP problem including QCD axion have been proposed so far. One possible solution to the strong CP problem is that CP is an exact symmetry, spontaneously broken at some scale. Nelson and Barr constructed the simple phenomenologically viable models in this framework called Nelson-Barr models [1,2]. In this talk, I will review the general features of a Nelson-Barr model and show that a Nelson-Barr model with gauge-mediated supersymmetry breaking is a plausible solution to the strong CP problem. This talk is based on Ref. [3] and the review of a Nelson-Barr model [4].
[1]:A.E. Nelson, Naturally Weak CP-violation, Phys. Lett. B 136 (1984) 387
[2]:S.M. Barr, Solving the Strong CP Problem Without the Peccei-Quinn Symmetry, Phys. Rev. Lett. 53 (1984) 329.
[3]:K. Fujikura, Y. Nakai, R. Sato and M. Yamada, Baryon Asymmetric Universe from Spontaneous CP Violation, [2202.08278]
[4]:M. Dine and P. Draper, Challenges for the Nelson-Barr Mechanism, JHEP 08 (2015) 132 [1506.05433].


トップ   編集 凍結 差分 バックアップ 添付 複製 名前変更 リロード   新規 一覧 単語検索 最終更新   ヘルプ   最終更新のRSS
Last-modified: 2022-02-24 (木) 11:03:50 (791d)