Relativistic Hydrodynamics with AMR

Details Relativistic Hydrodynamics with AMR Relativistic Hydrodynamics with AMR

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aps..aprb13002d&link_type=abstract

American Physical Society, April Meeting, April 28 - May 1, 2001 Washington, DC Bulletin of the American Physical Society, Vol.

Astronomy and Astrophysics

Astrophysics

Scientific paper

Modeling astrophysical sources of gravitational radiation requires fully 3-D numerical simulations. Due to the range of scales involved, adaptive mesh refinement (AMR) is a critical component for successful modeling. We present a progress report on the development of a fully general relativistic hydrodynamics code for modeling such sources. Results from 3-D runs involving shocks using AMR will be shown.

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