Chaotic inflation in supergravity with Heisenberg symmetry
Chaotic inflation in supergravity with Heisenberg symmetry
 
  We propose the introduction of a Heisenberg symmetry of the Kähler potential to solve the problems with chaotic inflation in supergravity, as a viable alternative to the use of shift symmetry. The slope of the inflaton potential emerges from a small Heisenberg symmetry breaking term in the superpotential. The modulus field of the Heisenberg symmetry is stabilized and made heavy with the help of the large vacuum energy density during inflation. The observable predictions are indistinguishable from those of typical chaotic inflation models, however the form of the inflationary superpotential considered here may be interpreted in terms of sneutrino inflation arising from certain classes of string theory.
  
  
  428-432
  
    
      Antusch, Stefan
      
        6a8c0380-78ea-4bcb-afad-4348d84eafba
      
     
  
    
      Bastero-Gil, Mar
      
        16b57761-3a65-4b65-844f-2a63dd69af0d
      
     
  
    
      Dutta, Koushik
      
        91e0b545-4e58-405a-910e-fa74b7889fd2
      
     
  
    
      King, Steve F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
    
      Kostka, Philipp M.
      
        b9b61289-32b3-43f6-b789-bf1b6cdb5d32
      
     
  
  
   
  
  
    
      2009
    
    
  
  
    
      Antusch, Stefan
      
        6a8c0380-78ea-4bcb-afad-4348d84eafba
      
     
  
    
      Bastero-Gil, Mar
      
        16b57761-3a65-4b65-844f-2a63dd69af0d
      
     
  
    
      Dutta, Koushik
      
        91e0b545-4e58-405a-910e-fa74b7889fd2
      
     
  
    
      King, Steve F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
    
      Kostka, Philipp M.
      
        b9b61289-32b3-43f6-b789-bf1b6cdb5d32
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Antusch, Stefan, Bastero-Gil, Mar, Dutta, Koushik, King, Steve F. and Kostka, Philipp M.
  
  
  
  
   
    (2009)
  
  
    
    Chaotic inflation in supergravity with Heisenberg symmetry.
  
  
  
  
    Physics Letters B, 679 (5), .
  
   (doi:10.1016/j.physletb.2009.08.022). 
  
  
   
  
  
  
  
  
   
  
    
      
        
          Abstract
          We propose the introduction of a Heisenberg symmetry of the Kähler potential to solve the problems with chaotic inflation in supergravity, as a viable alternative to the use of shift symmetry. The slope of the inflaton potential emerges from a small Heisenberg symmetry breaking term in the superpotential. The modulus field of the Heisenberg symmetry is stabilized and made heavy with the help of the large vacuum energy density during inflation. The observable predictions are indistinguishable from those of typical chaotic inflation models, however the form of the inflationary superpotential considered here may be interpreted in terms of sneutrino inflation arising from certain classes of string theory.
        
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      Published date: 2009
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
  
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 179073
        URI: http://eprints.soton.ac.uk/id/eprint/179073
        
          
        
        
        
          ISSN: 0370-2693
        
        
          PURE UUID: d49e7b7b-02aa-4bdd-8095-904fd0e0733c
        
  
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
            
          
        
    
        
          
        
    
  
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  Date deposited: 26 Apr 2011 12:36
  Last modified: 14 Mar 2024 02:47
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      Contributors
      
          
          Author:
          
            
            
              Stefan Antusch
            
          
        
      
          
          Author:
          
            
            
              Mar Bastero-Gil
            
          
        
      
          
          Author:
          
            
            
              Koushik Dutta
            
          
        
      
        
      
          
          Author:
          
            
            
              Philipp M. Kostka
            
          
        
      
      
      
    
  
   
  
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