2003/05/31 by Catherine I. Low, Raymond R. Volkas · 4 citations
Mathematics · Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Cabibbo–Kobayashi–Maskawa matrix #Discrete symmetry #Geometry #Homogeneous space #Lepton #Mathematics #Matrix (chemical analysis) #Mixing (physics) #Neutrino #Neutrino Physics Research #Neutrino oscillation #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Physics #Pontecorvo–Maki–Nakagawa–Sakata matrix #Quantum mechanics #Quark #Sterile neutrino #Symmetry (geometry) #hep-ph
paper · pdf · doi:10.1103/physrevd.68.033007
published as Phys.Rev.D68:033007,2003 · 14 pages, no figures, RevTeX4, references added
arxiv created 2003/06/04 · openalex publication_date 2003/08/08 · arxiv updated 2010/04/06 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Neutrino oscillation experiments (excluding the Liquid Scintillator Neutrino Detector experiment) suggest a tribimaximal form for the lepton mixing matrix. This form indicates that the mixing matrix is probably independent of the lepton masses, and suggests the action of an underlying discrete family symmetry. Using these hints, we conjecture that the contrasting forms of the quark and lepton mixing matrices may both be generated by such a discrete family symmetry. This idea is that the diagonalization matrices out of which the physical mixing matrices are composed have large mixing angles, which cancel out due to a symmetry when the CKM matrix is computed, but do not do so in the MNS case. However, in the cases where the Higgs bosons are singlets under the symmetry, and the family symmetry commutes with SU(2)L, we prove a no-go theorem: no discrete unbroken family symmetry can produce the required mixing patterns. We then suggest avenues for future research.