arXiv · 1502.02935
Numerical code for multi-component galaxies: from N-body to chemistry and magnetic fields
Abstract
We present a numerical code for multi-component simulation of the galactic evolution. Our code includes the following parts: $N$-body is used to evolve dark matter, stellar dynamics and dust grains, gas dynamics is based on TVD-MUSCL scheme with the extra modules for thermal processes, star formation, magnetic fields, chemical kinetics and multi-species advection. We describe our code in brief, but we give more details for the magneto-gas dynamics. We present several tests for our code and show that our code have passed the tests with a reasonable accuracy. Our code is parallelized using the MPI library. We apply our code to study the large scale dynamics of galactic discs.
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S. A. Khoperskov, E. O. Vasiliev, A. V. Khoperskov, V. N. Lubimov. 2015-02-10. Numerical code for multi-component galaxies: from N-body to chemistry and magnetic fields. https://doi.org/10.1088/1742-6596/510/1/012011
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