Fermion masses and mixing angles from SU(3) family symmetry and unification
Fermion masses and mixing angles from SU(3) family symmetry and unification
 
  We develop a bottom–up approach to constructing a theory of fermion masses and mixing angles based on the gauge group SU(3)×G where SU(3) is a family symmetry and G contains a unified group such as SO(10) or its Pati–Salam subgroup, together with other discrete symmetries. We construct a realistic model and show that it can provide an excellent description of quark and lepton masses and mixing angles, including almost maximal atmospheric mixing and the LMA MSW solar neutrino solution. We predict a neutrino mixing angle θ13 near the current limit. The model provides the basis for a new solution to the flavour problem with a characteristic soft SUSY breaking mass spectrum.
  
  
  239-252
  
    
      King, S F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
    
      Ross, G.G.
      
        d58064ce-8a29-4bfc-b438-ef29b0a16bcb
      
     
  
  
   
  
  
    
    
  
    
      13 November 2003
    
    
  
  
    
      King, S F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
    
      Ross, G.G.
      
        d58064ce-8a29-4bfc-b438-ef29b0a16bcb
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    King, S F. and Ross, G.G.
  
  
  
  
   
    (2003)
  
  
    
    Fermion masses and mixing angles from SU(3) family symmetry and unification.
  
  
  
  
    Physics Letters B, 574 (3-4), .
  
   (doi:10.1016/j.physletb.2003.09.027). 
  
  
   
  
  
  
  
  
   
  
    
      
        
          Abstract
          We develop a bottom–up approach to constructing a theory of fermion masses and mixing angles based on the gauge group SU(3)×G where SU(3) is a family symmetry and G contains a unified group such as SO(10) or its Pati–Salam subgroup, together with other discrete symmetries. We construct a realistic model and show that it can provide an excellent description of quark and lepton masses and mixing angles, including almost maximal atmospheric mixing and the LMA MSW solar neutrino solution. We predict a neutrino mixing angle θ13 near the current limit. The model provides the basis for a new solution to the flavour problem with a characteristic soft SUSY breaking mass spectrum.
        
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      Submitted date: 27 July 2003
 
    
      Published date: 13 November 2003
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
  
    
     
        Organisations:
        Physics & Astronomy
      
    
  
    
  
  
        Identifiers
        Local EPrints ID: 57394
        URI: http://eprints.soton.ac.uk/id/eprint/57394
        
          
        
        
        
          ISSN: 0370-2693
        
        
          PURE UUID: 0ec98a28-98e4-4ef1-aefd-7332d9891736
        
  
    
        
          
            
          
        
    
        
          
        
    
  
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  Date deposited: 14 Aug 2008
  Last modified: 15 Mar 2024 11:06
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      Contributors
      
        
      
          
          Author:
          
            
            
              G.G. Ross
            
          
        
      
      
      
    
  
   
  
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