Neutrino mixing angles in sequential dominance to NLO and NNLO
Neutrino mixing angles in sequential dominance to NLO and NNLO
 
  Neutrinos with hierarchical masses and two large mixing angles may naturally originate from sequential dominance (SD). Within this framework we present analytic expressions for the neutrino mixing angles including the next-to-leading order (NLO) and next-to-next-to-leading order (NNLO) corrections arising from the second lightest and lightest neutrino masses. The analytic results for neutrino mixing angles in SD presented here, including the NLO and NNLO corrections, are applicable to a wide class of models and may provide useful insights when confronting the models with data from high precision neutrino experiments. We also point out that for special cases of SD corresponding to form dominance (FD) the NLO and NNLO corrections both vanish. For example we study tri-bimaximal (TB) mixing via constrained sequential dominance (CSD) which involves only a NNLO correction and tri-bimaximal-reactor (TBR) mixing via partially constrained sequential dominance (PCSD) which involves a NLO correction suppressed by the small reactor angle and show that the analytic results have good agreement with the numerical results for these cases.
  neutrino physics, beyond standard model
  
  
    
      Antusch, S.
      
        5c4a4555-199c-4b90-9590-f4c392ee850c
      
     
  
    
      Boudjemaa, S.
      
        d6568698-00cc-46f3-b456-d253ad790fc6
      
     
  
    
      King, S.F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
  
   
  
  
    
      2010
    
    
  
  
    
      Antusch, S.
      
        5c4a4555-199c-4b90-9590-f4c392ee850c
      
     
  
    
      Boudjemaa, S.
      
        d6568698-00cc-46f3-b456-d253ad790fc6
      
     
  
    
      King, S.F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Antusch, S., Boudjemaa, S. and King, S.F.
  
  
  
  
   
    (2010)
  
  
    
    Neutrino mixing angles in sequential dominance to NLO and NNLO.
  
  
  
  
    Journal of High Energy Physics, 2010 (9, 96).
  
   (doi:10.1007/JHEP09(2010)096). 
  
  
   
  
  
  
  
  
   
  
    
      
        
          Abstract
          Neutrinos with hierarchical masses and two large mixing angles may naturally originate from sequential dominance (SD). Within this framework we present analytic expressions for the neutrino mixing angles including the next-to-leading order (NLO) and next-to-next-to-leading order (NNLO) corrections arising from the second lightest and lightest neutrino masses. The analytic results for neutrino mixing angles in SD presented here, including the NLO and NNLO corrections, are applicable to a wide class of models and may provide useful insights when confronting the models with data from high precision neutrino experiments. We also point out that for special cases of SD corresponding to form dominance (FD) the NLO and NNLO corrections both vanish. For example we study tri-bimaximal (TB) mixing via constrained sequential dominance (CSD) which involves only a NNLO correction and tri-bimaximal-reactor (TBR) mixing via partially constrained sequential dominance (PCSD) which involves a NLO correction suppressed by the small reactor angle and show that the analytic results have good agreement with the numerical results for these cases.
        
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      Published date: 2010
 
    
  
  
    
  
    
  
    
  
    
  
    
     
    
  
    
     
        Keywords:
        neutrino physics, beyond standard model
      
    
  
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 179047
        URI: http://eprints.soton.ac.uk/id/eprint/179047
        
          
        
        
        
        
          PURE UUID: 3e5290aa-fa59-4d52-bf33-9d9ba1120eb5
        
  
    
        
          
        
    
        
          
        
    
        
          
            
          
        
    
  
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  Date deposited: 18 Apr 2011 15:06
  Last modified: 14 Mar 2024 02:47
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      Contributors
      
          
          Author:
          
            
            
              S. Antusch
            
          
        
      
          
          Author:
          
            
            
              S. Boudjemaa
            
          
        
      
        
      
      
      
    
  
   
  
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