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The analytical solution of the Riemann problem in relativistic hydrodynamics

Published online by Cambridge University Press:  26 April 2006

José Ma Martí and
Ewald Müller
José Ma Martí
Affiliation:
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 8046 Garching b. München, Germany
Ewald Müller
Affiliation:
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 8046 Garching b. München, Germany
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Abstract

We consider the decay of an initial discontinuity in a polytropic gas in a Minkowski space–time (the special relativistic Riemann problem). In order to get a general analytical solution for this problem, we analyse the properties of the relativistic flow across shock waves and rarefactions. As in classical hydrodynamics, the solution of the Riemann problem is found by solving an implicit algebraic equation which gives the pressure in the intermediate states. The solution presented here contains as a particular case the special relativistic shock-tube problem in which the gas is initially at rest. Finally, we discuss the impact of this result on the development of high-resolution shock-capturing numerical codes to solve the equations of relativistic hydrodynamics.

Information

Type
Research Article
Information
Journal of Fluid Mechanics , Volume 258 , 10 January 1994, pp. 317 - 333
Copyright
© 1994 Cambridge University Press

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