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http://hdl.handle.net/11452/28554
Başlık: | Muon g-2, 125 GeV Higgs boson, and neutralino dark matter in a flavor symmetry-based MSSM |
Yazarlar: | Babu, Kaladi S. Gogoladze, Ilia G. Shafi, Qaisar Uludağ Üniversitesi/Fen-Edebiyat Fakültesi/Fizik Bölümü. 0000-0002-0595-8803 Ün, Cem Salih N-3421-2014 55325758100 |
Anahtar kelimeler: | Family symmetry Unified theories Fermion masses Breaking Supersymmetry Predictions Unification Models Minima Astronomy & astrophysics Physics |
Yayın Tarihi: | 16-Ara-2014 |
Yayıncı: | Amer Physical |
Atıf: | Babu, K. S. vd. (2014). "Muon g-2, 125 GeV Higgs boson, and neutralino dark matter in a flavor symmetry-based MSSM". Physical Review D , 90(11). |
Özet: | We discuss the sparticle (and Higgs) spectrum in a class of flavor symmetry-based minimal super-symmetric standard models, referred to here as sMSSM. In this framework the supersymmetry breaking Lagrangian takes the most general form consistent with a grand unified symmetry such as SO(10) and a non-Abelian flavor symmetry acting on the three families with either a 2+1 or a 3 family assignment. Models based on gauged SU(2) and SO(3) flavor symmetry, as well as non-Abelian discrete symmetries such as S-3 and A(4), have been suggested which fall into this category. These models describe supersymmetry breaking in terms of seven phenomenological parameters. The soft supersymmetry breaking masses at M-GUT of all sfermions of the first two families are equal in sMSSM, which differ in general from the corresponding third family mass. In such a framework we show that the muon g - 2 anomaly, the observed Higgs boson mass of similar to 125 GeV, and the observed relic neutralino dark matter abundance can be simultaneously accommodated. The resolution of the muon g - 2 anomaly in particular yields the result that the first two generation squark masses, as well the gluino mass, should be less than or similar to 2 TeV, which will be tested at LHC14. |
URI: | https://doi.org/10.1103/PhysRevD.90.116002 https://journals.aps.org/prd/abstract/10.1103/PhysRevD.90.116002 http://hdl.handle.net/11452/28554 |
ISSN: | 1550-7998 1550-2368 |
Koleksiyonlarda Görünür: | Scopus Web of Science |
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