Friday, October 13, 2017
2:00 pm

TAPIR Seminar

Moving Mesh Astrophysics
Paul Duffell, Postdoctoral Scholar, UC Berkeley

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.

Contact Sheri Stoll at 626-395-6608
For more information see TAPIR at Caltech
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