Muon g-2, 125 GeV Higgs boson, and neutralino dark matter in a flavor symmetry-based MSSM
dc.contributor.author | Babu, Kaladi S. | |
dc.contributor.author | Gogoladze, Ilia G. | |
dc.contributor.author | Shafi, Qaisar | |
dc.contributor.buuauthor | Ün, Cem Salih | |
dc.contributor.department | Uludağ Üniversitesi/Fen-Edebiyat Fakültesi/Fizik Bölümü. | tr_TR |
dc.contributor.orcid | 0000-0002-0595-8803 | tr_TR |
dc.contributor.researcherid | N-3421-2014 | tr_TR |
dc.contributor.scopusid | 55325758100 | tr_TR |
dc.date.accessioned | 2022-09-08T08:15:27Z | |
dc.date.available | 2022-09-08T08:15:27Z | |
dc.date.issued | 2014-12-16 | |
dc.description.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. | en_US |
dc.description.sponsorship | United States Department of Energy (DOE) (de-sc0010108) (DE-FG02-91ER40626) | en_US |
dc.description.sponsorship | National Science Foundation (NSF) (OCI-1053575) | en_US |
dc.description.sponsorship | Rustaveli National Science Foundation (31/98) | en_US |
dc.description.sponsorship | United States Department of Energy (DOE) (de-sc0010137) | en_US |
dc.description.sponsorship | National Science Foundation (NSF) (PHY-1342611) | en_US |
dc.identifier.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). | en_US |
dc.identifier.issn | 1550-7998 | |
dc.identifier.issn | 1550-2368 | |
dc.identifier.issue | 11 | tr_TR |
dc.identifier.scopus | 2-s2.0-84918767610 | tr_TR |
dc.identifier.uri | https://doi.org/10.1103/PhysRevD.90.116002 | |
dc.identifier.uri | https://journals.aps.org/prd/abstract/10.1103/PhysRevD.90.116002 | |
dc.identifier.uri | http://hdl.handle.net/11452/28554 | |
dc.identifier.volume | 90 | tr_TR |
dc.identifier.wos | 000348730800012 | |
dc.indexed.scopus | Scopus | en_US |
dc.indexed.wos | SCIE | en_US |
dc.language.iso | en | en_US |
dc.publisher | Amer Physical | en_US |
dc.relation.collaboration | Yurt dışı | tr_TR |
dc.relation.journal | Physical Review D | en_US |
dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi | tr_TR |
dc.rights | info:eu-repo/semantics/openAccess | en_US |
dc.subject | Family symmetry | en_US |
dc.subject | Unified theories | en_US |
dc.subject | Fermion masses | en_US |
dc.subject | Breaking | en_US |
dc.subject | Supersymmetry | en_US |
dc.subject | Predictions | en_US |
dc.subject | Unification | en_US |
dc.subject | Models | en_US |
dc.subject | Minima | en_US |
dc.subject | Astronomy & astrophysics | en_US |
dc.subject | Physics | en_US |
dc.subject.scopus | Higgs Bosons; Supersymmetry; Higgs | en_US |
dc.subject.wos | Astronomy & astrophysics | en_US |
dc.subject.wos | Physics, particles & fields | en_US |
dc.title | Muon g-2, 125 GeV Higgs boson, and neutralino dark matter in a flavor symmetry-based MSSM | en_US |
dc.type | Article | |
dc.wos.quartile | Q1 | en_US |