#  10/5 ITC Colloquium - Paul Duffell (Berkeley) 

 



####  calendar\_today Date and Time 

 **October 5, 2017** 

 11:00AM - 12:00PM EDT 

####  pin\_drop Location 

 **Pratt**  



 

 



 

 "Moving Mesh Astrophysics"  
  
Abstract: Novel methods in recent years have been developed for numerically solving the hydrodynamical and MHD equations relevant to all kinds of astrophysical flows. I will first (briefly) present one such computational technique, where the numerical grid follows the MHD flow using a "moving mesh". I will then present some astrophysical scenarios for which I have applied this method, including planet formation and high-energy transients such as supernovae and gamma ray bursts.



 

 



 

 See also:- [ 2017-18 ](/academic-year/2017-18)
- [ Colloquium ](/event-type/colloquium)
 
 

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