Flavor physics and fine tuning in theory space
Flavor physics and fine tuning in theory space
 
  Recently a new class of composite Higgs models have been developed which give rise to naturally light Higgs bosons without supersymmetry. Based on the chiral symmetries of “theory space,” involving replicated gauge groups and appropriate gauge symmetry breaking patterns, these models allow the scale of the underlying strong dynamics giving rise to the composite particles to be as large as of order 10 TeV, without any fine tuning to prevent large corrections to Higgs boson mass(es) of order 100 GeV. 
In this paper we show that the size of flavor violating interactions arising generically from underlying flavor dynamics constrains the scale of the Higgs boson compositeness to be greater than of order 75 TeV, implying that significant fine-tuning is required. Without fine-tuning, the low-energy structure of the composite Higgs model alone is not sufficient to eliminate potential problems with flavor-changing neutral currents or excessive CP violation; solving those problems requires additional information or assumptions about the symmetries of the underlying flavor or strong dynamics. We also consider the weaker, but more model-independent, bounds which arise from limits on weak isospin violation.
  
  
  035008-[6pp]
  
    
      Chivukula, R. Sekhar
      
        18c2855f-65d6-4e48-a4db-d008d952d060
      
     
  
    
      Evans, Nick
      
        33dfbb52-64dd-4c1f-9cd1-074faf2be4b3
      
     
  
    
      Simmons, Elizabeth H.
      
        84221232-93b5-42d5-8c6f-e3b5c89eb351
      
     
  
  
   
  
  
    
      21 August 2002
    
    
  
  
    
      Chivukula, R. Sekhar
      
        18c2855f-65d6-4e48-a4db-d008d952d060
      
     
  
    
      Evans, Nick
      
        33dfbb52-64dd-4c1f-9cd1-074faf2be4b3
      
     
  
    
      Simmons, Elizabeth H.
      
        84221232-93b5-42d5-8c6f-e3b5c89eb351
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Chivukula, R. Sekhar, Evans, Nick and Simmons, Elizabeth H.
  
  
  
  
   
    (2002)
  
  
    
    Flavor physics and fine tuning in theory space.
  
  
  
  
    Physical Review D, 66 (3), .
  
   (doi:10.1103/PhysRevD.66.035008). 
  
  
   
  
  
  
  
  
   
  
    
      
        
          Abstract
          Recently a new class of composite Higgs models have been developed which give rise to naturally light Higgs bosons without supersymmetry. Based on the chiral symmetries of “theory space,” involving replicated gauge groups and appropriate gauge symmetry breaking patterns, these models allow the scale of the underlying strong dynamics giving rise to the composite particles to be as large as of order 10 TeV, without any fine tuning to prevent large corrections to Higgs boson mass(es) of order 100 GeV. 
In this paper we show that the size of flavor violating interactions arising generically from underlying flavor dynamics constrains the scale of the Higgs boson compositeness to be greater than of order 75 TeV, implying that significant fine-tuning is required. Without fine-tuning, the low-energy structure of the composite Higgs model alone is not sufficient to eliminate potential problems with flavor-changing neutral currents or excessive CP violation; solving those problems requires additional information or assumptions about the symmetries of the underlying flavor or strong dynamics. We also consider the weaker, but more model-independent, bounds which arise from limits on weak isospin violation.
        
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      Published date: 21 August 2002
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
  
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 28763
        URI: http://eprints.soton.ac.uk/id/eprint/28763
        
          
        
        
        
          ISSN: 1550-7998
        
        
          PURE UUID: d294bd45-ec67-4dd6-a846-dd51d881e4e0
        
  
    
        
          
        
    
        
          
            
          
        
    
        
          
        
    
  
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  Date deposited: 05 May 2006
  Last modified: 15 Mar 2024 07:27
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      Contributors
      
          
          Author:
          
            
            
              R. Sekhar Chivukula
            
          
        
      
        
      
          
          Author:
          
            
            
              Elizabeth H. Simmons
            
          
        
      
      
      
    
  
   
  
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