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.
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
This publication is cited in the following 4 articles:
Boris N. Narozhny, “Hydrodynamic approach to two-dimensional electron systems”, Riv. Nuovo Cim., 45:10 (2022), 661
L. Santelli, P. Orlandi, R. Verzicco, “A finite-difference scheme for three-dimensional incompressible flows in spherical coordinates”, J. Comput. Phys., 424 (2021), 109848
Alexander V. Babakov, Smart Innovation, Systems and Technologies, 214, Smart Modelling For Engineering Systems, 2021, 35
Alexander V. Babakov, Alexey Y. Lugovsky, Valery M. Chechetkin, Smart Innovation, Systems and Technologies, 173, Advances in Theory and Practice of Computational Mechanics, 2020, 23