HK 19: Nuclear Astrophysics II
  Dienstag, 21. März 2023, 17:00–19:00, SCH/A419
  
    
  
  
    
      
        
          
            
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          17:00 | 
          HK 19.1 | 
          
            
              Gruppenbericht:
            
            
              
                Neutrino flavor instability and nucleosynthesis associated with charged-current weak interactions in black hole accretion disks — •Zewei Xiong, Lucas Johns, Meng-Ru Wu, Huaiyu Duan, Gabriel Martínez-Pinedo, and Oliver Just
              
            
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          17:30 | 
          HK 19.2 | 
          
            
            
              
                Nuclear equation of state from Δ-full chiral interactions — •Yannick Dietz, Jonas Keller, Kai Hebeler, and Achim Schwenk
              
            
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          17:45 | 
          HK 19.3 | 
          
            
            
              
                Gaussian processes for the nuclear equation of state — •Hannah Göttling, Jonas Keller, Kai Hebeler, and Achim Schwenk
              
            
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          18:00 | 
          HK 19.4 | 
          
            
            
              
                Magnetar crusts - influence of the magnetic field on the composition and the unified equation of state — •Yuliya Mutafchieva, Zhivko Stoyanov, Nicolas Chamel, John Michael Pearson, and Lyubomir Mihailov
              
            
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          18:15 | 
          HK 19.5 | 
          
            
            
              
                Supernova Simulations with Consistent Six Species Neutrino Transport — •Ignacio L. Arbina, Gabriel Martinez-Pinedo, and Tobias Fischer
              
            
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          18:30 | 
          HK 19.6 | 
          
            
            
              
                The phase structure of neutral three flavor quark matter — •Marco Hofmann, Hosein Gholami, and Michael Buballa
              
            
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          18:45 | 
          HK 19.7 | 
          
            
            
              
                Hybrid equation of state and mass radius relation — •Hosein Gholami, Marco Hofmann, and Michael Buballa
              
            
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