Summary.
A kinetic solution for the relativistic Euler equations is presented. This solution describes the flow of a perfect gas in terms of the particle density n, the spatial part of the four-velocity u and the inverse temperature β. In this paper we present a general framework for the kinetic scheme of relativistic Euler equations which covers the whole range from the non-relativistic limit to the ultra-relativistic limit. The main components of the kinetic scheme are described now. (i) There are periods of free flight of duration τ M , where the gas particles move according to the free kinetic transport equation. (ii) At the maximization times t n =nτ M , the beginning of each of these free-flight periods, the gas particles are in local equilibrium, which is described by Jüttners relativistic generalization of the classical Maxwellian phase density. (iii) At each new maximization time t n >0 we evaluate the so called continuity conditions, which guarantee that the kinetic scheme satisfies the conservation laws and the entropy inequality. These continuity conditions determine the new initial data at t n . iv If in addition adiabatic boundary conditions are prescribed, we can incorporate a natural reflection method into the kinetic scheme in order to solve the initial and boundary value problem. In the limit τ M →0 we obtain the weak solutions of Euler’s equations including arbitrary shock interactions. We also present a numerical shock reflection test which confirms the validity of our kinetic approach.
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Mathematics Subject Classification (1991):65M99, 76Y05
This work is supported by the project ‘‘Long-time behaviour of nonlinear hyperbolic systems of conservation laws and their numerical approximation’’, contract # DFG WA 633/7-2.
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Kunik, M., Qamar, S. & Warnecke, G. Kinetic schemes for the relativistic gas dynamics. Numer. Math. 97, 159–191 (2004). https://doi.org/10.1007/s00211-003-0510-9
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DOI: https://doi.org/10.1007/s00211-003-0510-9