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This article is cited in 4 scientific papers (total in 4 papers)
Mathematical simulation of vortex structures in rapidly rotating astrophysical objects
A. G. Aksenova, A. V. Babakova, V. M. Chechetkinb 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..
Received: 05.03.2018
Citation:
A. G. Aksenov, A. V. Babakov, V. M. Chechetkin, “Mathematical simulation of vortex structures in rapidly rotating astrophysical objects”, Zh. Vychisl. Mat. Mat. Fiz., 58:8 (2018), 182–188; Comput. Math. Math. Phys., 58:8 (2018), 1287–1293
Linking options:
https://www.mathnet.ru/eng/zvmmf10772 https://www.mathnet.ru/eng/zvmmf/v58/i8/p182
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Abstract page: | 182 | References: | 27 |
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