Numerical Simulation of 2D Relativistic Hydrodynamics Using Adaptive Mesh Refinement Technique

Details Numerical Simulation of 2D Relativistic Hydrodynamics Using Adaptive Mesh Refinement Technique Numerical Simulation of 2D Relativistic Hydrodynamics Using Adaptive Mesh Refinement Technique

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...207.7502k&link_type=abstract

American Astronomical Society Meeting 207, #75.02; Bulletin of the American Astronomical Society, Vol. 37, p.1289

Computer Science

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We have developed a code to numerically solve two-dimensional special relativistic hydrodynamics equations based on the LCPFCT algorithm for one-dimensional Newtonian hydrodynamics. We implemented our code using the PARAMESH, Parallel AMR library. We present the details of our algorithm and exhibit its performance on a series of verification tests. Our code will be combined with two-dimensional transport code to build up a code for two-dimensional special relativistic radiation hydrodynamics. The prompt and/or afterglow emission of Gamma-Ray Bursts(GRBs) will be investigated in detail with the numerical simulation of relativistic radiation hydrodynamics.
This work was supported by NASA Cooperative Agreement No. NCC 5-615.

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