A. G. Aksenov, A. V. Babakov, V. M. Chechetkin, “Mathematical simulation of vortex structures in rapidly rotating astrophysical objects”, Zh. Vychisl. Mat. Mat. Fiz., 2018, Volume 58, Number 8,Pages <nobr>182

This article is cited in 4 papers

Mathematical simulation of vortex structures in rapidly rotating astrophysical objects

A. G. Aksenov^a, A. V. Babakov^a, V. M. Chechetkin^b

^a Institute for Computer-Aided Design, Russian Academy of Sciences, Moscow, Russia
^b Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, Moscow, Russia

Abstract: A conservative finite-volume method is used to model rapidly rotating self-gravitating astrophysical objects. Large-scale vortex structures are obtained in evolutionary computations. The numerical simulation is based on parallel algorithms implemented on a cluster computer system.

Key words: mathematical simulation, conservative difference schemes, numerical methods, parallel algorithms, aero- and fluid dynamics, astrophysics, supernovas, gravitation, vortex structures..

UDC: 519.6, 524.3, 533

Received: 05.03.2018

DOI: 10.31857/S004446690002004-5