Scalar electroweak multiplet dark matter

被引:0
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作者
Wei Chao
Gui-Jun Ding
Xiao-Gang He
Michael Ramsey-Musolf
机构
[1] Beijing Normal University,Center for advanced quantum studies, Department of Physics
[2] University of Science and Technology of China,Interdisciplinary Center for Theoretical Study and Department of Modern Physics
[3] Shanghai Jiao Tong University,Tsung
[4] National Taiwan University,Dao Lee Institute, and School of Physics and Astronomy
[5] National Center for Theoretical Sciences,Department of Physics
[6] University of Massachusetts-Amherst,Amherst Center for Fundamental Interactions
[7] California Institute of Technology,Kellogg Radiation Laboratory
来源
Journal of High Energy Physics | / 2019卷
关键词
Beyond Standard Model; Cosmology of Theories beyond the SM; Higgs Physics;
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学科分类号
摘要
We revisit the theory and phenomenology of scalar electroweak multiplet thermal dark matter. We derive the most general, renormalizable scalar potential, assuming the presence of the Standard Model Higgs doublet, H, and an electroweak multiplet Φ of arbitrary SU(2)L rank and hypercharge, Y. We show that, in general, the Φ-H Higgs portal interactions depend on three, rather than two independent couplings as has been previously considered in the literature. For the phenomenologically viable case of Y = 0 multiplets, we focus on the septuplet and quintuplet cases, and consider the interplay of relic density and spin-independent direct detection cross section. We show that both the relic density and direct detection cross sections depend on a single linear combination of Higgs portal couplings, λeff. For λeff ∼ O\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ \mathcal{O} $$\end{document}(1), present direct detection exclusion limits imply that the neutral component of a scalar electroweak multiplet would comprise a subdominant fraction of the observed DM relic density.
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