Dark Radiation or Warm Dark Matter from long lived particle decays in the light of Planck
Dark Radiation or Warm Dark Matter from long lived particle decays in the light of Planck
 
  Although Planck data supports the standard ?CDM model, it still allows for the presence of Dark Radiation corresponding up to about half an extra standard neutrino species. We propose a scenario for obtaining a fractional “effective neutrino species” from a thermally produced particle which decays into a much lighter stable relic plus standard fermions. At lifetimes much longer than ?1 s, both the relic particles and the non-thermal neutrino component contribute to Dark Radiation. By increasing the stable-to-unstable particle mass ratio, the relic particle no longer acts as Dark Radiation but instead becomes a candidate for Warm Dark Matter with mass O(1 keV–100 GeV)O(1 keV–100 GeV). In both cases it is possible to address the lithium problem.
  
  
  77-83
  
    
      Di Bari, Pasquale
      
        3fe21e59-0eff-41bc-8faa-fdd817146418
      
     
  
    
      King, Stephen F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
    
      Merle, Alexander
      
        18b2b79d-5edb-4087-bf76-86050237604b
      
     
  
  
   
  
  
    
      July 2013
    
    
  
  
    
      Di Bari, Pasquale
      
        3fe21e59-0eff-41bc-8faa-fdd817146418
      
     
  
    
      King, Stephen F.
      
        f8c616b7-0336-4046-a943-700af83a1538
      
     
  
    
      Merle, Alexander
      
        18b2b79d-5edb-4087-bf76-86050237604b
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Di Bari, Pasquale, King, Stephen F. and Merle, Alexander
  
  
  
  
   
    (2013)
  
  
    
    Dark Radiation or Warm Dark Matter from long lived particle decays in the light of Planck.
  
  
  
  
    Physics Letters B, 724 (1-3), .
  
   (doi:10.1016/j.physletb.2013.06.003). 
  
  
   
  
  
  
  
  
   
  
    
    
      
        
          Abstract
          Although Planck data supports the standard ?CDM model, it still allows for the presence of Dark Radiation corresponding up to about half an extra standard neutrino species. We propose a scenario for obtaining a fractional “effective neutrino species” from a thermally produced particle which decays into a much lighter stable relic plus standard fermions. At lifetimes much longer than ?1 s, both the relic particles and the non-thermal neutrino component contribute to Dark Radiation. By increasing the stable-to-unstable particle mass ratio, the relic particle no longer acts as Dark Radiation but instead becomes a candidate for Warm Dark Matter with mass O(1 keV–100 GeV)O(1 keV–100 GeV). In both cases it is possible to address the lithium problem.
         
      
      
        
          
            
  
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      Published date: July 2013
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
  
    
     
        Organisations:
        Physics & Astronomy
      
    
  
    
  
  
        Identifiers
        Local EPrints ID: 369299
        URI: http://eprints.soton.ac.uk/id/eprint/369299
        
          
        
        
        
          ISSN: 0370-2693
        
        
          PURE UUID: 8c834b1c-9eca-47f6-867b-cb85ad6bbcee
        
  
    
        
          
            
          
        
    
        
          
            
          
        
    
        
          
            
          
        
    
  
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  Date deposited: 23 Sep 2014 12:49
  Last modified: 21 Aug 2025 13:34
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          Author:
          
            
              
              
                Alexander Merle
              
              
            
            
          
        
      
      
      
    
  
   
  
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