Natural implementation of neutralino dark matter
Natural implementation of neutralino dark matter
 
  The prediction of neutralino dark matter is generally regarded as one of the successes of the Minimal Supersymmetric Standard Model (MSSM). However the successful regions of parameter space allowed by WMAP and collider constraints are quite restricted. We discuss fine-tuning with respect to both dark matter and Electroweak Symmetry Breaking (EWSB) and explore regions of MSSM parameter space with non-universal gaugino and third family scalar masses in which neutralino dark matter may be implemented naturally. In particular allowing non-universal gauginos opens up the bulk region that allows Bino annihilation via t-channel slepton exchange, leading to "supernatural dark matter" corresponding to no fine-tuning at all with respect to dark matter. By contrast we find that the recently proposed "well tempered neutralino" regions involve substantial fine-tuning of MSSM parameters in order to satisfy the dark matter constraints, although the fine tuning may be ameliorated if several annihilation channels act simultaneously. Although we have identified regions of "supernatural dark matter" in which there is no fine tuning to achieve successful dark matter, the usual MSSM fine tuning to achieve EWSB always remains.
  supersymmetry phenomenology, cosmology of theories beyond the SM
  
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      King, S.F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
    
      Roberts, J.P
      
        2c91ea9a-930f-4266-ae19-6c1169eb7b53
      
     
  
  
   
  
  
    
      14 September 2006
    
    
  
  
    
      King, S.F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
    
      Roberts, J.P
      
        2c91ea9a-930f-4266-ae19-6c1169eb7b53
      
     
  
       
    
 
  
  
    
      
        
          Abstract
          The prediction of neutralino dark matter is generally regarded as one of the successes of the Minimal Supersymmetric Standard Model (MSSM). However the successful regions of parameter space allowed by WMAP and collider constraints are quite restricted. We discuss fine-tuning with respect to both dark matter and Electroweak Symmetry Breaking (EWSB) and explore regions of MSSM parameter space with non-universal gaugino and third family scalar masses in which neutralino dark matter may be implemented naturally. In particular allowing non-universal gauginos opens up the bulk region that allows Bino annihilation via t-channel slepton exchange, leading to "supernatural dark matter" corresponding to no fine-tuning at all with respect to dark matter. By contrast we find that the recently proposed "well tempered neutralino" regions involve substantial fine-tuning of MSSM parameters in order to satisfy the dark matter constraints, although the fine tuning may be ameliorated if several annihilation channels act simultaneously. Although we have identified regions of "supernatural dark matter" in which there is no fine tuning to achieve successful dark matter, the usual MSSM fine tuning to achieve EWSB always remains.
        
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      Published date: 14 September 2006
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
     
        Keywords:
        supersymmetry phenomenology, cosmology of theories beyond the SM
      
    
  
    
  
    
  
  
        Identifiers
        Local EPrints ID: 57390
        URI: http://eprints.soton.ac.uk/id/eprint/57390
        
          
        
        
        
        
          PURE UUID: a21acc1a-9b14-4aba-8ed0-9d582b35c974
        
  
    
        
          
            
          
        
    
        
          
        
    
  
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  Date deposited: 14 Aug 2008
  Last modified: 15 Mar 2024 11:06
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          Author:
          
            
            
              J.P Roberts
            
          
        
      
      
      
    
  
   
  
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