Neutralino dark matter in the USSM
Neutralino dark matter in the USSM
 
  This paper provides a comprehensive discussion of neutralino dark matter within classes of extended supersymmetric models referred to as the USSM containing one additional SM singlet Higgs plus an extra Z', together with their superpartners the singlino and bino'. These extra states of the USSM can significantly modify the nature and properties of neutralino dark matter relative to that of the minimal (or even next-to-minimal) supersymmetric standard models. We derive the Feynman rules for the USSM and calculate the dark matter relic abundance and direct detection rates for elastic scattering in the USSM for interesting regions of parameter space where the largest differences are expected. 
  supersymmetry phenomenology
  
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      Kalinowski, J.
      
        4fc1d464-b529-44e4-91ac-5dfb852c8b66
      
     
  
    
      King, S.F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
    
      Roberts, J.P.
      
        48b7fd03-832c-4ae9-9259-bf9b98daa361
      
     
  
  
   
  
  
    
      January 2009
    
    
  
  
    
      Kalinowski, J.
      
        4fc1d464-b529-44e4-91ac-5dfb852c8b66
      
     
  
    
      King, S.F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
    
      Roberts, J.P.
      
        48b7fd03-832c-4ae9-9259-bf9b98daa361
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Kalinowski, J., King, S.F. and Roberts, J.P.
  
  
  
  
   
    (2009)
  
  
    
    Neutralino dark matter in the USSM.
  
  
  
  
    Journal of High Energy Physics, 2009 (JHEP01), .
  
   (doi:10.1088/1126-6708/2009/01/066). 
  
  
   
  
  
  
  
  
   
  
    
      
        
          Abstract
          This paper provides a comprehensive discussion of neutralino dark matter within classes of extended supersymmetric models referred to as the USSM containing one additional SM singlet Higgs plus an extra Z', together with their superpartners the singlino and bino'. These extra states of the USSM can significantly modify the nature and properties of neutralino dark matter relative to that of the minimal (or even next-to-minimal) supersymmetric standard models. We derive the Feynman rules for the USSM and calculate the dark matter relic abundance and direct detection rates for elastic scattering in the USSM for interesting regions of parameter space where the largest differences are expected. 
        
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      Published date: January 2009
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
     
        Keywords:
        supersymmetry phenomenology
      
    
  
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 144107
        URI: http://eprints.soton.ac.uk/id/eprint/144107
        
          
        
        
        
        
          PURE UUID: a9414eba-8902-4229-8e5a-ee50ab9e7a6f
        
  
    
        
          
        
    
        
          
            
          
        
    
        
          
        
    
  
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  Date deposited: 26 Apr 2011 13:28
  Last modified: 14 Mar 2024 00:45
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      Contributors
      
          
          Author:
          
            
            
              J. Kalinowski
            
          
        
      
        
      
          
          Author:
          
            
            
              J.P. Roberts
            
          
        
      
      
      
    
  
   
  
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