A Shock‐patching Code for Ultrarelativistic Fluid Flows
Author(s) -
L. Wen,
A. Panaitescu,
Pablo Laguna
Publication year - 1997
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/304547
Subject(s) - riemann problem , physics , classification of discontinuities , riemann solver , convergence (economics) , shock (circulatory) , riemann hypothesis , code (set theory) , planar , flow (mathematics) , shock wave , finite volume method , mathematical analysis , mechanics , mathematics , computer science , medicine , economics , economic growth , computer graphics (images) , set (abstract data type) , programming language
We have developed a one-dimensional code to solve ultra-relativistichydrodynamic problems, using the Glimm method for an accurate treatment ofshocks and contact discontinuities. The implementation of the Glimm method isbased on an exact Riemann solver and van der Corput sampling sequence. In orderto improve computational efficiency, the Glimm method is replaced by a finitedifferencing scheme in those regions where the fluid flow is sufficientlysmooth. The accuracy and convergence of this hybrid method is investigated intests involving planar, cylindrically and spherically symmetric flows thatexhibit strong shocks and Lorentz factors of up to ~2000. This hybrid code hasproven to be successful in simulating the interaction between a thin,ultra-relativistic, spherical shell and a low density stationary medium, asituation likely to appear in Gamma-Ray Bursts, supernovae explosions, pulsarwinds and AGNs.Comment: submitted to ApJ, in press, Latex, uses AAS macro aaspp4.sty and psfig.tex (version 1.9), 12 pages, 5 figures and 4 tables, revised version (more detailed description of the numerical implementation of the Glimm method
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