Dresden 2013 –
            
              wissenschaftliches Programm
            
          
        
        
        
        
        
      
      
  
    
  
  T 21: Astroteilchenphysik und Kosmologie (Theorie)
  Mittwoch, 6. März 2013, 16:45–19:00, WIL-B122
  
    
  
  
    
      
        
          
            
              |  | 16:45 | T 21.1 | DM@NLO and the impact of SUSY-QCD-corrections to (co-)annihilation-processes on Neutralino Dark Matter — Julia Harz, Björn Herrmann, Michael Klasen, Karol Kovařík, Quentin Le Boulc'h, •Moritz Meinecke, and Patrick Steppeler | 
        
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              |  | 17:00 | T 21.2 | Dark matter signals at the LHC: forecasts from ton-scale direct detection experiments — •Riccardo Catena | 
        
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              |  | 17:15 | T 21.3 | On the spin-dependent sensitivity of XENON100. — Mathias Garny, Alejandro Ibarra, Miguel Pato, and •Stefan Vogl | 
        
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              |  | 17:30 | T 21.4 | Multi-Component Dark Matter Systems and Their Observation Prospects — Mayumi Aoki, •Michael Duerr, Jisuke Kubo, and Hiroshi Takano | 
        
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              |  | 17:45 | T 21.5 | Ultra-high energy cosmic ray escape from gamma-ray bursts, and the cosmic ray-neutrino connection — •Philipp Baerwald, Mauricio Bustamante, Svenja Hümmer, Amyad Spector, Eli Waxman, and Walter Winter | 
        
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              |  | 18:00 | T 21.6 | Analyzing the propagation of cosmic rays — •Robert Rettig | 
        
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              |  | 18:15 | T 21.7 | Nonequilibrium QFT approach to leptogenesis — •Tibor Frossard, Mathias Garny, Andreas Hohenegger, David Mitrouskas, and Alexander Kartavtsev | 
        
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              |  | 18:30 | T 21.8 | Time Evolution of the Large-Scale Tail of Non-Helical Primordial Magnetic Fields — •Andrey Saveliev, Karsten Jedamzik, and Günter Sigl | 
        
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              |  | 18:45 | T 21.9 | The 130 GeV gamma-ray line and generic dark matter model building constraints from continuum gamma rays, radio and antiproton data — •Martin Vollmann, Masaki Asano, Torsten Bringmann, and Guenter Sigl | 
        
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