Full one-loop electro-weak corrections to three-jet observables at the Z pole and beyond
Full one-loop electro-weak corrections to three-jet observables at the Z pole and beyond
 
  We describe the impact of the full one-loop EW terms of O(αs αEM3) entering the electron-positron into three-jet cross-section from √s = MZ to TeV scale energies. We include both factorisable and non-factorisable virtual corrections, photon bremsstrahlung but not the real emission of W± and Z bosons. Their importance for the measurement of αS from jet rates and shape variables is explained qualitatively and illustrated quantitatively.
  standard model, NLO computations
  
  1-32
  
  
    
      Carloni-Calame, C.M.
      
        443f480b-3508-4002-82b8-92c9f93c06f6
      
     
  
    
      Moretti, S.
      
        b57cf0f0-4bc3-4e02-96e3-071255366614
      
     
  
    
      Piccinini, F.
      
        749c37ee-226a-40d2-9168-6225fa29c14b
      
     
  
    
      Ross, D.A
      
        eb79bbfe-fb97-4bb3-813c-98f278e5a55f
      
     
  
  
   
  
  
    
      26 June 2009
    
    
  
  
    
      Carloni-Calame, C.M.
      
        443f480b-3508-4002-82b8-92c9f93c06f6
      
     
  
    
      Moretti, S.
      
        b57cf0f0-4bc3-4e02-96e3-071255366614
      
     
  
    
      Piccinini, F.
      
        749c37ee-226a-40d2-9168-6225fa29c14b
      
     
  
    
      Ross, D.A
      
        eb79bbfe-fb97-4bb3-813c-98f278e5a55f
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Carloni-Calame, C.M., Moretti, S., Piccinini, F. and Ross, D.A
  
  
  
  
   
    (2009)
  
  
    
    Full one-loop electro-weak corrections to three-jet observables at the Z pole and beyond.
  
  
  
  
    Journal of High Energy Physics, 47 (3), .
  
   (doi:10.1088/1126-6708/2009/03/047). 
  
  
   
  
  
  
  
  
   
  
    
      
        
          Abstract
          We describe the impact of the full one-loop EW terms of O(αs αEM3) entering the electron-positron into three-jet cross-section from √s = MZ to TeV scale energies. We include both factorisable and non-factorisable virtual corrections, photon bremsstrahlung but not the real emission of W± and Z bosons. Their importance for the measurement of αS from jet rates and shape variables is explained qualitatively and illustrated quantitatively.
        
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      Published date: 26 June 2009
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
     
        Keywords:
        standard model, NLO computations
      
    
  
    
     
        Organisations:
        Physics & Astronomy
      
    
  
    
  
  
        Identifiers
        Local EPrints ID: 144583
        URI: http://eprints.soton.ac.uk/id/eprint/144583
        
          
        
        
        
        
          PURE UUID: 1bb4d44d-84cb-4ebd-9151-bf1948fdaf28
        
  
    
        
          
        
    
        
          
            
              
            
          
        
    
        
          
        
    
        
          
            
          
        
    
  
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  Date deposited: 14 Apr 2010 13:24
  Last modified: 14 Mar 2024 02:48
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      Contributors
      
          
          Author:
          
            
            
              C.M. Carloni-Calame
            
          
        
      
        
      
          
          Author:
          
            
            
              F. Piccinini
            
          
        
      
        
      
      
      
    
  
   
  
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