Indirect, direct and collider detection of neutralino dark matter in the minimal supergravity model
Indirect, direct and collider detection of neutralino dark matter in the minimal supergravity model
 
  We examine the prospects for supersymmetry discovery in the
minimal supergravity (mSUGRA) model via indirect detection of neutralino dark matter. We investigate rates for muon detection in neutrino telescopes, and detection of photons, positrons and anti-protons by balloon and space based experiments. We compare the discovery reach in these channels with the reach for direct detection of dark matter, and also with the reach of collider experiments such as Fermilab Tevatron, CERN LHC and a ?s = 0.5–1 TeV linear e+e? collider. We pay particular attention to regions of model parameter space in accord with recent WMAP results on the dark matter density of the universe.
We find that third generation direct dark matter detection experiments should be able to cover the entire WMAP allowed portion of the hyperbolic branch/focus point (HB/FP) region of parameter space, while the IceCube neutrino telescope can cover almost all this region. This is in contrast to the case of the CERN LHC or a linear e+e? collider, where only a fraction of the HB/FP region can be accessed. In addition, we show that detection of ?s, e+s and ¯ps should occur in much of the HB/FP region, as well as in the low m1/2 portion of the A annihilation
funnel, and will be complementary to searches via colliders in these regions.
  dark matter, dark matter detectors, neutrino and gamma astronomy
  
  
  1-21
  
    
      Baer, Howard
      
        193c3082-95fb-469b-9548-e972a10e9341
      
     
  
    
      Belyaev, Alexander
      
        6bdb9638-5ff9-4b65-a8f2-34bae3ac34b3
      
     
  
    
      Krupovnickas, Tadas
      
        7fa6f110-fe0a-4d8e-8939-27cb27c79efa
      
     
  
    
      O'Farrill, Jorge
      
        83a06631-230b-401d-9d0b-ab577f83a0d2
      
     
  
  
   
  
  
    
      9 August 2004
    
    
  
  
    
      Baer, Howard
      
        193c3082-95fb-469b-9548-e972a10e9341
      
     
  
    
      Belyaev, Alexander
      
        6bdb9638-5ff9-4b65-a8f2-34bae3ac34b3
      
     
  
    
      Krupovnickas, Tadas
      
        7fa6f110-fe0a-4d8e-8939-27cb27c79efa
      
     
  
    
      O'Farrill, Jorge
      
        83a06631-230b-401d-9d0b-ab577f83a0d2
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Baer, Howard, Belyaev, Alexander, Krupovnickas, Tadas and O'Farrill, Jorge
  
  
  
  
   
    (2004)
  
  
    
    Indirect, direct and collider detection of neutralino dark matter in the minimal supergravity model.
  
  
  
  
    Journal of Cosmology and Astroparticle Physics, JCAP08 (5), .
  
   (doi:10.1088/1475-7516/2004/08/005). 
  
  
   
  
  
  
  
  
   
  
    
      
        
          Abstract
          We examine the prospects for supersymmetry discovery in the
minimal supergravity (mSUGRA) model via indirect detection of neutralino dark matter. We investigate rates for muon detection in neutrino telescopes, and detection of photons, positrons and anti-protons by balloon and space based experiments. We compare the discovery reach in these channels with the reach for direct detection of dark matter, and also with the reach of collider experiments such as Fermilab Tevatron, CERN LHC and a ?s = 0.5–1 TeV linear e+e? collider. We pay particular attention to regions of model parameter space in accord with recent WMAP results on the dark matter density of the universe.
We find that third generation direct dark matter detection experiments should be able to cover the entire WMAP allowed portion of the hyperbolic branch/focus point (HB/FP) region of parameter space, while the IceCube neutrino telescope can cover almost all this region. This is in contrast to the case of the CERN LHC or a linear e+e? collider, where only a fraction of the HB/FP region can be accessed. In addition, we show that detection of ?s, e+s and ¯ps should occur in much of the HB/FP region, as well as in the low m1/2 portion of the A annihilation
funnel, and will be complementary to searches via colliders in these regions.
        
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      Published date: 9 August 2004
 
    
  
  
    
  
    
     
        Additional Information:
        This was the first paper where discovery reach of indirect detection of neutralino dark matter was compared with the reach for direct detection dark matter experiments and also with the reach of collider experiments such as Fermilab Tevatron, CERN LHC and a sqrt (s)= 0.5-1 TeV linear e+e- collider, demonstrating a high degree of complementarity of the above experiments.
      
    
  
    
  
    
  
    
  
    
     
        Keywords:
        dark matter, dark matter detectors, neutrino and gamma astronomy
      
    
  
    
  
    
  
  
        Identifiers
        Local EPrints ID: 46724
        URI: http://eprints.soton.ac.uk/id/eprint/46724
        
          
        
        
        
          ISSN: 1475-7516
        
        
          PURE UUID: 13135d48-fa89-4911-9dd7-2c7d17f74ed2
        
  
    
        
          
        
    
        
          
            
              
            
          
        
    
        
          
        
    
        
          
        
    
  
  Catalogue record
  Date deposited: 17 Jul 2007
  Last modified: 16 Mar 2024 03:53
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      Contributors
      
          
          Author:
          
            
            
              Howard Baer
            
          
        
      
        
      
          
          Author:
          
            
            
              Tadas Krupovnickas
            
          
        
      
          
          Author:
          
            
            
              Jorge O'Farrill
            
          
        
      
      
      
    
  
   
  
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