Preheating curvaton perturbations
Preheating curvaton perturbations
 
  We discuss the potentially important rôle played by preheating in certain variants of the curvaton mechanism in which isocurvature perturbations of a D-flat (and F-flat) direction become converted to curvature perturbations during reheating. We discover that parametric resonance of the isocurvature components amplifies the superhorizon fluctuations by a significant amount. As an example of these effects we develop a particle physics motivated model which involves hybrid inflation with the waterfall field N being responsible for generating the ? term, the right-handed neutrino mass scale, and the Peccei-Quinn symmetry breaking scale. The rôle of the curvaton field can be played either by usual Higgs field, or the lightest right-handed sneutrino. Our new results show that it is possible to achieve the correct curvature perturbations for initial values of the curvaton fields of order the weak scale. In this model we show that the prediction for the spectral index of the final curvature perturbation only depends on the mass of the curvaton during inflation, where consistency with current observational data requires the ratio of this mass to the Hubble constant to be less-than-or-equals, slant 0.3.
  
  
  36-43
  
    
      Bastero-Gil, M.
      
        b329c554-20e8-4180-af13-faaa34be2f84
      
     
  
    
      Di Clemente, V.
      
        4f38d85a-1c05-44c2-9e50-1ab950ca843f
      
     
  
    
      King, S.F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
  
   
  
  
    
      November 2005
    
    
  
  
    
      Bastero-Gil, M.
      
        b329c554-20e8-4180-af13-faaa34be2f84
      
     
  
    
      Di Clemente, V.
      
        4f38d85a-1c05-44c2-9e50-1ab950ca843f
      
     
  
    
      King, S.F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
       
    
 
  
  
    
      
        
          Abstract
          We discuss the potentially important rôle played by preheating in certain variants of the curvaton mechanism in which isocurvature perturbations of a D-flat (and F-flat) direction become converted to curvature perturbations during reheating. We discover that parametric resonance of the isocurvature components amplifies the superhorizon fluctuations by a significant amount. As an example of these effects we develop a particle physics motivated model which involves hybrid inflation with the waterfall field N being responsible for generating the ? term, the right-handed neutrino mass scale, and the Peccei-Quinn symmetry breaking scale. The rôle of the curvaton field can be played either by usual Higgs field, or the lightest right-handed sneutrino. Our new results show that it is possible to achieve the correct curvature perturbations for initial values of the curvaton fields of order the weak scale. In this model we show that the prediction for the spectral index of the final curvature perturbation only depends on the mass of the curvaton during inflation, where consistency with current observational data requires the ratio of this mass to the Hubble constant to be less-than-or-equals, slant 0.3.
        
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      Published date: November 2005
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
  
    
  
    
  
  
        Identifiers
        Local EPrints ID: 57039
        URI: http://eprints.soton.ac.uk/id/eprint/57039
        
          
        
        
        
          ISSN: 0920-5632
        
        
          PURE UUID: c8001202-2b98-42c8-8bfb-1cd6e97bda04
        
  
    
        
          
        
    
        
          
        
    
        
          
            
          
        
    
  
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  Date deposited: 14 Aug 2008
  Last modified: 15 Mar 2024 11:04
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      Contributors
      
          
          Author:
          
            
            
              M. Bastero-Gil
            
          
        
      
          
          Author:
          
            
            
              V. Di Clemente
            
          
        
      
        
      
      
      
    
  
   
  
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