Keldysh Institute preprints, 2017, 001, 30 pages
On two-dimensional numerical QGD-modelling of spiral-vortex structures in accretion gas disks
T. G. Elizarovaa, A. A. Zlotnikb, M. A. Istominaa
a Keldysh Institute of Applied Mathematics of Russian Academy of Sciences, Moscow
b National Research University "Higher School of Economics" (HSE), Moscow
We derive new axially symmetric stationary solutions to the barotropic Euler equations with a body force in the isentropic and isothermal cases. They are used as the initial distributions in the related non-stationary problem. Basing on a quasi-hydrodynamic approach, we perform numerical experiments on the development of small initial perturbations of the azimuthal velocity and the formation of large structures like the density "sleeves". Splitting of the sleeves and decreasing of the gas angular momentum in the middle of the field are observed. Also the correctness of the shallow water approximation for describing the sleeve formation is confirmed.
The designed algorithm is universal and allows one to perform various numerical experiments of interest in astrophysics on a personal computer.
gas dynamic equations, polar coordinates, stationary solutions, accretion disk, quasi-gas dynamic approach, finite-difference approximation, numerical experiments.
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T. G. Elizarova, A. A. Zlotnik, M. A. Istomina, “On two-dimensional numerical QGD-modelling of spiral-vortex structures in accretion gas disks”, Keldysh Institute preprints, 2017, 001, 30 pp.
Citation in format AMSBIB
\by T.~G.~Elizarova, A.~A.~Zlotnik, M.~A.~Istomina
\paper On two-dimensional numerical QGD-modelling of spiral-vortex structures in accretion gas disks
\jour Keldysh Institute preprints
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