Please use this identifier to cite or link to this item: http://hdl.handle.net/11452/28554
Title: Muon g-2, 125 GeV Higgs boson, and neutralino dark matter in a flavor symmetry-based MSSM
Authors: 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
Keywords: Family symmetry
Unified theories
Fermion masses
Breaking
Supersymmetry
Predictions
Unification
Models
Minima
Astronomy & astrophysics
Physics
Issue Date: 16-Dec-2014
Publisher: Amer Physical
Citation: 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).
Abstract: 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
Appears in Collections:Scopus
Web of Science

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