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This article is cited in 1 scientific paper (total in 1 paper)
On a computational model of gravitational hydrodynamics with consideration of the radiation transfer in the diffusion approximation using tetrahedral meshes
I. M. Kulikov Institute of Computational Mathematics and Mathematical Geophysics SB RAS, pr. Acad. Lavrentyeva 6, Novosibirsk 630090, Russia
Abstract:
A new computational model of gravitational hydrodynamics with consideration of the radiation transfer in the diffusion approximation on tetrahedral meshes is proposed.
This model is a qualitative extension of the classical gravitational hydrodynamics model adapted to simulation of star formation and evolution of protoplanetary disks.
Some computational methods of solving this problem are described, and the results of numerical simulation of the solar mass cloud collapse are given.
Keywords:
mathematical modeling, computational astrophysics,
radiation transfer.
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Received: 16.02.2021 Revised: 21.03.2021 Accepted: 15.04.2021
Citation:
I. M. Kulikov, “On a computational model of gravitational hydrodynamics with consideration of the radiation transfer in the diffusion approximation using tetrahedral meshes”, Sib. Zh. Ind. Mat., 24:2 (2021), 87–96; J. Appl. Industr. Math., 15:2 (2021), 277–284
Linking options:
https://www.mathnet.ru/eng/sjim1131 https://www.mathnet.ru/eng/sjim/v24/i2/p87
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