Mathematical simulation of vortex structures in rapidly rotating astrophysical objects

DOI10.1134/S096554251808002XzbMath1412.85001OpenAlexW2892621573WikidataQ129244208 ScholiaQ129244208MaRDI QIDQ1755606

A. V. Babakov, V. M. Chechetkin, A. G. Aksenov

Publication date: 10 January 2019

Published in: Computational Mathematics and Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1134/s096554251808002x

zbMATH Keywords

numerical methodsparallel algorithmsgravitationastrophysicsvortex structuresconservative difference schemesmathematical simulationaero- and fluid dynamicssupernovas

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Magnetohydrodynamics and electrohydrodynamics (76W05) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Galactic and stellar dynamics (85A05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Computational methods for problems pertaining to astronomy and astrophysics (85-08) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

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A finite-difference scheme for three-dimensional incompressible flows in spherical coordinates

Uses Software

• FLUX

Cites Work

• Program package FLUX for the simulation of fundamental and applied problems of fluid dynamics
• Numerical simulation of spatially unsteady jets of compressible gas on a multiprocessor computer system
• The conservative “flow” method and the calculation of the flow of a viscous heat-conducting gas past a body of finite size
• Non-Radial Oscillations and Convective Instability of Gaseous Masses.