Mathematical Simulation of Vortex Structures in Rapidly Rotating Astrophysical Objects

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

doi:10.1134/S096554251808002X

Mathematical Simulation of Vortex Structures in Rapidly Rotating Astrophysical Objects

作者: Aksenov A.G.¹, Babakov A.V.¹, Chechetkin V.M.²
隶属关系:
1. Institute for Computer-Aided Design, Russian Academy of Sciences
2. Keldysh Institute of Applied Mathematics, Russian Academy of Sciences
期: 卷 58, 编号 8 (2018)
页面: 1287-1293
栏目: Article
URL: https://journal-vniispk.ru/0965-5425/article/view/179776
DOI: https://doi.org/10.1134/S096554251808002X
ID: 179776

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详细

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.