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Study of 3D Dynamics of Gravitating Systems Using Supercomputers: Methods and Applications

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Parallel Computing Technologies (PaCT 2007)

Part of the book series: Lecture Notes in Computer Science ((LNTCS,volume 4671))

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Abstract

We describe parallel numerical code for solving problems of stellar dynamics. The code is based on numerical solving of Poisson and Vlasov equations in cylindrical coordinates using particle-in-cells method. The code is designed for use on supercomputers with distributed memory. We consider different possible strategies of parallelization according to initial technical parameters of numerical methods and physical conditions of the model. We present results of numerical simulations for the following problems of stellar dynamics: investigation of influence of central potential on the vertical motions of thin gravitating disk; stability of uniform sphere with anisotropic distribution of velocity; numerical approximation of equilibrium states of gravitating systems.

The present work was supported by Grant of Rosobrazovanie, contract RNP.2.2.1.1.1969; Grant of Rosobrazovanie, contract RNP.2.2.1.1.3653.

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References

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Victor Malyshkin

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© 2007 Springer-Verlag Berlin Heidelberg

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Snytnikov, N., Vshivkov, V., Snytnikov, V. (2007). Study of 3D Dynamics of Gravitating Systems Using Supercomputers: Methods and Applications . In: Malyshkin, V. (eds) Parallel Computing Technologies. PaCT 2007. Lecture Notes in Computer Science, vol 4671. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-73940-1_16

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  • DOI: https://doi.org/10.1007/978-3-540-73940-1_16

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-73939-5

  • Online ISBN: 978-3-540-73940-1

  • eBook Packages: Computer ScienceComputer Science (R0)

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