2001
DOI: 10.1016/s0370-2693(01)01139-x
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Fermion masses and mixing angles from SU(3) family symmetry

Abstract: We propose a model based on SU (3) family symmetry which leads to a successful description of quark and lepton masses and mixing angles including approximate bi-maximal mixing in the neutrino sector suitable for the LOW or quasi-vacuum solar solutions, with the atmospheric angle predicted to be accurately maximal due to the SU (3) symmetry. The model predicts a CHOOZ angle θ 13 ∼ |V ub |. The SU (3) symmetry can also ensure the near degeneracy of squarks and sleptons needed to avoid large flavour changing neut… Show more

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Cited by 197 publications
(242 citation statements)
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“…Therefore the limit close to 10 − 3 on Λ is robust, just as stated in the literature. 9 In summary, the solution to the anomaly cancellation problem with X µ = 4 becomes somewhat marginal, X µ = 5 (Λ = O(3000 TeV) being more comfortable. But both are very close to be tested in rare process experiments perhaps before the new heavy particles could even be searched for at the LHC!…”
Section: Jhep03(2011)128mentioning
confidence: 99%
“…Therefore the limit close to 10 − 3 on Λ is robust, just as stated in the literature. 9 In summary, the solution to the anomaly cancellation problem with X µ = 4 becomes somewhat marginal, X µ = 5 (Λ = O(3000 TeV) being more comfortable. But both are very close to be tested in rare process experiments perhaps before the new heavy particles could even be searched for at the LHC!…”
Section: Jhep03(2011)128mentioning
confidence: 99%
“…(13). This equation represents the most general parameterization of the Yukawa matrices for quarks and charged leptons with an SU(3) FS [2,3]. In any supersymmetric FS, the flavon fields also couple to the sfermions through the trilinear terms…”
Section: Fermion Masses and Mfv Conditionsmentioning
confidence: 99%
“…Note that for this case the trilinear couplings (∼ z f ij ǫ p f ) will not be exactly aligned with the Yukawa couplings but will still be proportional to them and effectively we are taking 3,3) and z f 33 = c f 33 .…”
Section: Form Of the Yukawa Matrices And Soft Termsmentioning
confidence: 99%
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“…At the first glance, the hierarchical mass spectra of the quarks and the charged leptons actually suggest underlying non-Abelian flavor symmetry groups acting on the first and second generations only. 4 However, in the light of recent atmospheric [5][6][7][8][9] and solar [10][11][12][13][14][15][16][17] neutrino experimental results, it seems to be difficult to extend this idea to the neutrinos. Especially, the result that, among the different possible solutions of the solar neutrino problem, the Mikheyev-Smirnov-Wolfenstein (MSW) [18][19][20] large mixing angle (LMA) solution is the presently preferred one [21][22][23] 5 , draws a picture of the involved flavor symmetries and their breaking mechanisms that differs remarkably from the early approaches, which have been applied to the quark sector.…”
Section: Introductionmentioning
confidence: 99%