Non-universal gaugino mass GUT models in the light of dark matter and LHC constraints

被引:0
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作者
Joydeep Chakrabortty
Subhendra Mohanty
Soumya Rao
机构
[1] Indian Institute of Technology,Department of Physics
[2] ,undefined
[3] Physical Research Laboratory,undefined
[4] Department of Theoretical Physics and Centre for Theoretical Sciences,undefined
[5] Indian Association for the Cultivation of Science,undefined
来源
Journal of High Energy Physics | / 2014卷
关键词
Supersymmetry Phenomenology;
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摘要
We perform a comprehensive study of SU(5), SO(10) and E(6) supersymmetric GUT models where the gaugino masses are generated through the F-term breaking vacuum expectation values of the non-singlet scalar fields. In these models the gauginos are non-universal at the GUT scale unlike in the mSUGRA scenario. We discuss the properties of the LSP which is stable and a viable candidate for cold dark matter. We look for the GUT scale parameter space that leads to the the lightest SM like Higgs mass in the range of 122-127 GeV compatible with the observations at ATLAS and CMS, the relic density in the allowed range of WMAP-PLANCK and compatible with other constraints from colliders and direct detection experiments. We scan universal scalar \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$ \left( {m_0^G} \right) $\end{document}, trilinear coupling A0 and SU(3)C gaugino mass \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$ \left( {m_3^G} \right) $\end{document} as the independent free parameters for these models. Based on the gaugino mass ratios at the GUT scale, we classify 25 SUSY GUT models and find that of these only 13 models satisfy the dark matter and collider constraints. Out of these 13 models there is only one model where there is a sizeable SUSY contribution to muon (g−2).
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