The dark side of the Littlest Seesaw: freeze-in, the two right-handed neutrino portal and leptogenesis-friendly fimpzillas
The dark side of the Littlest Seesaw: freeze-in, the two right-handed neutrino portal and leptogenesis-friendly fimpzillas
 
  We propose a minimal model to simultaneously account for a realistic neutrino spectrum through a type-I seesaw mechanism and a viable dark matter relic density. The model is an extension of the Littlest Seesaw model in which the two right-handed neutrinos of the model are coupled to a Z2-odd dark sector via right-handed neutrino portal couplings. In this model, a highly constrained and direct link between dark matter and neutrino physics is achieved by considering the freeze-in production mechanism of dark matter. We show that the neutrino Yukawa couplings which describe neutrino mass and mixing may also play a dominant role in the dark matter production. We investigate the allowed regions in the parameter space of the model that provide the correct neutrino masses and mixing and simultaneously give the correct dark matter relic abundance. In certain cases the right-handed neutrino mass may be arbitrarily large, for example in the range 1010–1011 GeV required for vanilla leptogenesis, with a successful relic density arising from frozen-in dark matter particles with masses around this scale, which we refer to as "fimpzillas".
  
  
  
    
      Chianese, Marco
      
        73113e4b-5eb5-4cdc-831b-90f4678588d6
      
     
  
    
      King, Stephen
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
  
   
  
  
    
    
  
    
    
  
  
    
      Chianese, Marco
      
        73113e4b-5eb5-4cdc-831b-90f4678588d6
      
     
  
    
      King, Stephen
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Chianese, Marco and King, Stephen
  
  
  
  
   
    (2018)
  
  
    
    The dark side of the Littlest Seesaw: freeze-in, the two right-handed neutrino portal and leptogenesis-friendly fimpzillas.
  
  
  
  
    Journal of Cosmology and Astroparticle Physics, [027].
  
   (doi:10.1088/1475-7516/2018/09/027). 
  
  
   
  
  
  
  
  
   
  
    
    
      
        
          Abstract
          We propose a minimal model to simultaneously account for a realistic neutrino spectrum through a type-I seesaw mechanism and a viable dark matter relic density. The model is an extension of the Littlest Seesaw model in which the two right-handed neutrinos of the model are coupled to a Z2-odd dark sector via right-handed neutrino portal couplings. In this model, a highly constrained and direct link between dark matter and neutrino physics is achieved by considering the freeze-in production mechanism of dark matter. We show that the neutrino Yukawa couplings which describe neutrino mass and mixing may also play a dominant role in the dark matter production. We investigate the allowed regions in the parameter space of the model that provide the correct neutrino masses and mixing and simultaneously give the correct dark matter relic abundance. In certain cases the right-handed neutrino mass may be arbitrarily large, for example in the range 1010–1011 GeV required for vanilla leptogenesis, with a successful relic density arising from frozen-in dark matter particles with masses around this scale, which we refer to as "fimpzillas".
         
      
      
        
          
            
  
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 The dark side of the Littlest Seesaw: freeze-in, the two right-handed neutrino portal and leptogenesis-friendly fimpzillas
     - Accepted Manuscript
   
  
  
    
  
 
          
            
          
            
           
            
           
        
        
       
    
   
  
  
  More information
  
    
      Accepted/In Press date: 6 September 2018
 
    
      e-pub ahead of print date: 17 September 2018
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
  
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 425536
        URI: http://eprints.soton.ac.uk/id/eprint/425536
        
          
        
        
        
          ISSN: 1475-7516
        
        
          PURE UUID: 725d9096-a3d2-464c-8751-eb0a0abd5f52
        
  
    
        
          
            
          
        
    
        
          
            
          
        
    
  
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  Date deposited: 24 Oct 2018 16:30
  Last modified: 16 Mar 2024 07:12
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      Contributors
      
          
          Author:
          
            
              
              
                Marco Chianese
              
              
            
            
          
        
      
        
      
      
      
    
  
   
  
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