Mathematical Simulation of Vortex Structures in Rapidly Rotating Astrophysical Objects

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.

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Bibliographische Detailangaben
Veröffentlicht in:	Computational mathematics and mathematical physics 2018-08, Vol.58 (8), p.1287-1293
Hauptverfasser:	Aksenov, A. G., Babakov, A. V., Chechetkin, V. M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Computational Mathematics and Numerical Analysis Computer simulation Finite volume method Gravitation Mathematical models Mathematics Mathematics and Statistics Rotation
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Beschreibung
Zusammenfassung:	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.
ISSN:	0965-5425 1555-6662
DOI:	10.1134/S096554251808002X