Minimal Gauged U(1) Extension of the Standard Model with Classical Scale Invariance and Phenomenology

• Material Type: 博士論文
• Title: Minimal Gauged U(1) Extension of the Standard Model with Classical Scale Invariance and Phenomenology
• Author/Editor: 高橋, 大介; Daisuke, Takahashi
• Author Heading: 高橋, 大介; Daisuke, Takahashi
• Publication Date: 2018-02-21
• Publication Date (W3CDTF): 2018-02-21
• Alternative Title: スケール不変なU(1)ゲージ拡張された標準模型とその現象論
• Degree grantor/type: Okinawa Institute of Science and Technology Graduate University
• Date Granted: 2018-02-21
• Date Granted (W3CDTF): 2018-02-21
• Dissertation Number: 甲第14号
• Degree Type: Doctor of Philosophy
• Conferring No. (Dissertation): 甲第14号
• Text Language Code: eng
• Target Audience: 一般
• Note (General): Although the Standard Model (SM) is the best theory in describing phenomena among elementary particles, it suffers from several problems, such as the gauge hierarchy problem, origin of the electroweak symmetry breaking, non-zero neutrino mass, and no candidate of dark matter. For solving these problems, we consider minimal U(1) extension of the SM with the classically conformal invariance, where an anomaly-free U(1) gauge symmetry is introduced along with a U(1) Higgs field and three righthanded neutrinos (RHNs) for the seesaw mechanism generating neutrino masses. With no mass term allowed by the classically conformal invariance, the U(1) gauge symmetry is broken through the Coleman-Weinberg mechanism, which subsequently triggers the electroweak symmetry breaking. We perform parameter scan and identify regions resolving the SM Higgs vacuum instability, while satisfying the LHC Run-2 bound on the U(1) gauge boson production and the naturalness constraint. We also investigate cosmological aspects of the model. Introducing Z2 parity, one RHN being an unique parity-odd particle in the model serves as dark matter. A successful inflation scenario is possible by identifying the U(1) Higgs boson with inflaton and introducing its non-minimal gravitational coupling. Interestingly, the LHC physics and cosmological observations are complementary narrowing down the model parameter space.
• DOI: 10.15102/1394.00000258; https://doi.org/10.15102/1394.00000258
• Persistent ID (NDL): info:ndljp/pid/11063762; https://dl.ndl.go.jp/pid/11063762
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• Collection (particular): 国立国会図書館デジタルコレクション > デジタル化資料 > 博士論文; https://dl.ndl.go.jp/collections/A00014
• Acquisition Basis: 博士論文（自動収集）
• Date Accepted (W3CDTF): 2018-04-03T03:53:09+09:00
• Date Created (W3CDTF): 2018-02-21
• Format (IMT): application/pdf
• Access Restrictions: 国立国会図書館内限定公開
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• Periodical Title (URI): http://dx.doi.org/10.15102/1394.00000258; http://id.nii.ac.jp/1394/00000258/
• Data Provider (Database): 国立国会図書館 : 国立国会図書館デジタルコレクション; https://dl.ndl.go.jp