The constrained E6SSM
The constrained E6SSM
 
  We discuss the predictions of a constrained version of the exceptional supersymmetric standard model (cE6SSM), with a universal high energy soft scalar mass, soft trilinear coupling and soft gaugino mass. The spectrum includes 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. We also discuss scenarios with an extra light exotic colour triplet of fermions and scalars and a TeV scale Z', which lead to early exotic physics signals at the LHC.
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      Athron, Peter
      
        dd767afe-49c1-4ed0-ad04-0b3e4308fc36
      
     
  
    
      King, Stephen F.
      
        e9b763e5-06d2-4386-8f0d-c9b649e1f27c
      
     
  
    
      Miller, David J.
      
        4a8df40c-c7e6-4d10-8927-e26cc907f00e
      
     
  
    
      Moretti, Stefano
      
        b57cf0f0-4bc3-4e02-96e3-071255366614
      
     
  
    
      Nevzorov, Roman
      
        b67e86cd-abc5-4d17-9299-8e8eef2f3f61
      
     
  
  
   
  
  
    
      July 2009
    
    
  
  
    
      Athron, Peter
      
        dd767afe-49c1-4ed0-ad04-0b3e4308fc36
      
     
  
    
      King, Stephen F.
      
        e9b763e5-06d2-4386-8f0d-c9b649e1f27c
      
     
  
    
      Miller, David J.
      
        4a8df40c-c7e6-4d10-8927-e26cc907f00e
      
     
  
    
      Moretti, Stefano
      
        b57cf0f0-4bc3-4e02-96e3-071255366614
      
     
  
    
      Nevzorov, Roman
      
        b67e86cd-abc5-4d17-9299-8e8eef2f3f61
      
     
  
       
    
 
  
    
      
  
  
  
  
    Athron, Peter, King, Stephen F., Miller, David J., Moretti, Stefano and Nevzorov, Roman
  
  
  
  
   
    (2009)
  
  
    
    The constrained E6SSM.
  
  
  
  
    
    
    
      
        
   
  
    Proceedings of The 2009 Europhysics Conference on High Energy Physics, Krakow, Poland.
   
        
        
        15 - 21  Jul 2009.
      
    
  
  
  
      
          
          
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      Record type:
      Conference or Workshop Item
      (Paper)
      
      
    
   
    
      
        
          Abstract
          We discuss the predictions of a constrained version of the exceptional supersymmetric standard model (cE6SSM), with a universal high energy soft scalar mass, soft trilinear coupling and soft gaugino mass. The spectrum includes 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. We also discuss scenarios with an extra light exotic colour triplet of fermions and scalars and a TeV scale Z', which lead to early exotic physics signals at the LHC.
        
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      Published date: July 2009
 
    
  
  
    
  
    
  
    
     
        Venue - Dates:
        Proceedings of The 2009 Europhysics Conference on High Energy Physics, Krakow, Poland, 2009-07-15 - 2009-07-21
      
    
  
    
  
    
  
    
  
    
     
        Organisations:
        Physics & Astronomy
      
    
  
    
  
  
        Identifiers
        Local EPrints ID: 144385
        URI: http://eprints.soton.ac.uk/id/eprint/144385
        
        
        
        
          PURE UUID: 5b1ab754-0935-4740-9c31-f9039fa132b1
        
  
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
            
              
            
          
        
    
        
          
        
    
  
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  Date deposited: 18 Sep 2013 13:43
  Last modified: 09 Mar 2022 02:36
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      Contributors
      
          
          Author:
          
            
            
              Peter Athron
            
          
        
      
          
          Author:
          
            
            
              Stephen F. King
            
          
        
      
          
          Author:
          
            
            
              David J. Miller
            
          
        
      
        
      
          
          Author:
          
            
            
              Roman Nevzorov
            
          
        
      
      
      
    
  
   
  
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