Constrained exceptional supersymmetric standard model
Constrained exceptional supersymmetric standard model
 
  We propose and study a constrained version of the exceptional supersymmetric standard model (E6SSM), which we call the cE6SSM, based on a universal high energy scalar mass m0, trilinear scalar coupling A0 and gaugino mass M1/2. We derive the renormalization group (RG) Equations for the cE6SSM, including the extra U(1)N gauge factor and the low-energy matter content involving three 27 representations of E6. We perform a numerical RG analysis for the cE6SSM, imposing the usual low-energy experimental constraints and successful electroweak symmetry breaking. Our analysis reveals that the sparticle spectrum of the cE6SSM involves a light gluino, two light neutralinos, and a light chargino. Furthermore, although the squarks, sleptons, and Z? boson are typically heavy, the exotic quarks and squarks can also be relatively light. We finally specify a set of benchmark points, which correspond to particle spectra, production modes, and decay patterns peculiar to the cE6SSM, altogether leading to spectacular new physics signals at the Large Hadron Collider.
  
  
  035009-[31pp]
  
    
      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
      
     
  
  
   
  
  
    
      12 August 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)
  
  
    
    Constrained exceptional supersymmetric standard model.
  
  
  
  
    Physical Review D, 80 (3), .
  
   (doi:10.1103/PhysRevD.80.035009). 
  
  
   
  
  
  
  
  
   
  
    
      
        
          Abstract
          We propose and study a constrained version of the exceptional supersymmetric standard model (E6SSM), which we call the cE6SSM, based on a universal high energy scalar mass m0, trilinear scalar coupling A0 and gaugino mass M1/2. We derive the renormalization group (RG) Equations for the cE6SSM, including the extra U(1)N gauge factor and the low-energy matter content involving three 27 representations of E6. We perform a numerical RG analysis for the cE6SSM, imposing the usual low-energy experimental constraints and successful electroweak symmetry breaking. Our analysis reveals that the sparticle spectrum of the cE6SSM involves a light gluino, two light neutralinos, and a light chargino. Furthermore, although the squarks, sleptons, and Z? boson are typically heavy, the exotic quarks and squarks can also be relatively light. We finally specify a set of benchmark points, which correspond to particle spectra, production modes, and decay patterns peculiar to the cE6SSM, altogether leading to spectacular new physics signals at the Large Hadron Collider.
        
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      Published date: 12 August 2009
 
    
  
  
    
  
    
  
    
  
    
  
    
     
    
  
    
  
    
     
        Organisations:
        High Energy Physics
      
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 144115
        URI: http://eprints.soton.ac.uk/id/eprint/144115
        
          
        
        
        
          ISSN: 1550-7998
        
        
          PURE UUID: a23925d2-fd2b-4280-b2f1-f600b5b260b2
        
  
    
        
          
        
    
        
          
            
          
        
    
        
          
        
    
        
          
            
              
            
          
        
    
        
          
        
    
  
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  Date deposited: 26 Apr 2011 12:55
  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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