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The exact solution of the Riemann problem with non-zero tangential velocities in relativistic hydrodynamics

Published online by Cambridge University Press:  03 November 2000

JOSÉ A. PONS
Affiliation:
Departament d'Astronomia i Astrofísica, Universitat de València, 46100 Burjassot, Spain
JOSÉ Ma MARTÍ
Affiliation:
Departament d'Astronomia i Astrofísica, Universitat de València, 46100 Burjassot, Spain
EWALD MÜLLER
Affiliation:
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85748 Garching, Germany

Abstract

We have generalized the exact solution of the Riemann problem in special relativistic hydrodynamics (Martí & Müller 1994) for arbitrary tangential flow velocities. The solution is obtained by solving the jump conditions across shocks plus an ordinary differential equation arising from the self-similarity condition along rarefaction waves, in a similar way as in purely normal flow. The dependence of the solution on the tangential velocities is analysed, and the impact of this result on the development of multi-dimensional relativistic hydrodynamic codes (of Godunov type) is discussed.

Type
Research Article
Copyright
© 2000 Cambridge University Press

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