Predictions of the constrained exceptional supersymmetric standard model
Predictions of the constrained exceptional supersymmetric standard model
 
  We discuss the predictions of a constrained version of the exceptional supersymmetric standard model (cE6SSM), based on a universal high energy soft scalar mass m0, soft trilinear coupling A0 and soft gaugino mass M1/2. We predict a supersymmetry (SUSY) spectrum containing a light gluino, a light wino-like neutralino and chargino pair and a light bino-like neutralino, with other sparticle masses except the lighter stop being much heavier. In addition, the cE6SSM allows the possibility of light exotic colour triplet charge 1/3 fermions and scalars, leading to early exotic physics signals at the LHC. We focus on the possibility of a Z? gauge boson with mass close to 1 TeV, and low values of (m0,M1/2), which would correspond to an LHC discovery using “first data”, and propose a set of benchmark points to illustrate this.
  
  
  448-456
  
    
      Athron, P.
      
        5ac03b61-f44c-466f-b6ee-28fef4e3ab27
      
     
  
    
      King, S.F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
    
      Miller, D.J.
      
        a230d4ba-cdd8-4e3b-8d96-3bc31863b7a8
      
     
  
    
      Moretti, S.
      
        b57cf0f0-4bc3-4e02-96e3-071255366614
      
     
  
    
      Nevzorov, R.
      
        29e55377-613c-4b07-b29a-49fedd1f7544
      
     
  
  
   
  
  
    
      November 2009
    
    
  
  
    
      Athron, P.
      
        5ac03b61-f44c-466f-b6ee-28fef4e3ab27
      
     
  
    
      King, S.F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
    
      Miller, D.J.
      
        a230d4ba-cdd8-4e3b-8d96-3bc31863b7a8
      
     
  
    
      Moretti, S.
      
        b57cf0f0-4bc3-4e02-96e3-071255366614
      
     
  
    
      Nevzorov, R.
      
        29e55377-613c-4b07-b29a-49fedd1f7544
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Athron, P., King, S.F., Miller, D.J., Moretti, S. and Nevzorov, R.
  
  
  
  
   
    (2009)
  
  
    
    Predictions of the constrained exceptional supersymmetric standard model.
  
  
  
  
    Physics Letters B, 681 (5), .
  
   (doi:10.1016/j.physletb.2009.10.051). 
  
  
   
  
  
  
  
  
   
  
    
      
        
          Abstract
          We discuss the predictions of a constrained version of the exceptional supersymmetric standard model (cE6SSM), based on a universal high energy soft scalar mass m0, soft trilinear coupling A0 and soft gaugino mass M1/2. We predict a supersymmetry (SUSY) spectrum containing a light gluino, a light wino-like neutralino and chargino pair and a light bino-like neutralino, with other sparticle masses except the lighter stop being much heavier. In addition, the cE6SSM allows the possibility of light exotic colour triplet charge 1/3 fermions and scalars, leading to early exotic physics signals at the LHC. We focus on the possibility of a Z? gauge boson with mass close to 1 TeV, and low values of (m0,M1/2), which would correspond to an LHC discovery using “first data”, and propose a set of benchmark points to illustrate this.
        
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      Published date: November 2009
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
  
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 144109
        URI: http://eprints.soton.ac.uk/id/eprint/144109
        
          
        
        
        
          ISSN: 0370-2693
        
        
          PURE UUID: 35da8917-5047-4e3c-998e-66e4c8eada4a
        
  
    
        
          
        
    
        
          
            
          
        
    
        
          
        
    
        
          
            
              
            
          
        
    
        
          
        
    
  
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  Date deposited: 26 Apr 2011 13:16
  Last modified: 14 Mar 2024 02:48
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      Contributors
      
          
          Author:
          
            
            
              P. Athron
            
          
        
      
        
      
          
          Author:
          
            
            
              D.J. Miller
            
          
        
      
        
      
          
          Author:
          
            
            
              R. Nevzorov
            
          
        
      
      
      
    
  
   
  
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