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

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

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..836..153k&link_type=abstract

GAMMA-RAY BURSTS IN THE SWIFT ERA: Sixteenth Maryland Astrophysics Conference. AIP Conference Proceedings, Volume 836, pp. 153-

Astronomy and Astrophysics

Astrophysics

Mathematical Procedures And Computer Techniques, Hydrodynamics, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

We have developed a code to numerically solve 2-D special relativistic hydrodynamics equations based on the LCPFCT algorithm. We implemented our code using PARAMESH, the 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 2-D transport code to build a code for 2-D 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.

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