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X-WR-CALNAME;VALUE=TEXT:10/5 ITC Colloquium - Paul Duffell (Berkeley)
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SUMMARY:10/5 ITC Colloquium - Paul Duffell (Berkeley)
DESCRIPTION:<p>	"Moving Mesh Astrophysics"<br><br>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.</p>
LOCATION:Pratt
STATUS:CONFIRMED
DTSTART:20171005T150000Z
DTEND:20171005T160000Z
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