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Application of DSMC method to astrophysical flows

Published online by Cambridge University Press:  26 May 2016

Takuya Matsuda ,
Hiromi Mizutani  and
Henri. M. J. Boffin
Takuya Matsuda
Affiliation:
Dept. of Earth and Planetary Sciences, Kobe University, Kobe 657-8501, Japan
Hiromi Mizutani
Affiliation:
Dept. of Earth and Planetary Sciences, Kobe University, Kobe 657-8501, Japan
Henri. M. J. Boffin
Affiliation:
Royal Observatory of Belgium, 3 av. Circulaire, 1180 Brussels

Abstract

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The Direct Simulation Monte Carlo (DSMC) method, developed originally to calculate rarefied gas dynamical problems, is applied to continuous flow including shocks assuming that the Knudsen number is sufficiently small. In particular, we study the formation of spiral shocks in the accretion disc of a close binary system. The method involves viscosity and thermal conduction automatically, and can thus simulate turbulent viscosity.

Type
Posters
Information
Symposium - International Astronomical Union , Volume 208: Astrophysical Supercomputing using Particle Simulations , 2003 , pp. 425 - 426
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Bird, G.A. 1994, Molecular Gas Dynamics and the Direct Simulation of Gas Flows (Oxford Science Publications)CrossRefGoogle Scholar