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Publications in Math-Net.Ru
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Using a viscosity matrix to construct a Riemann solver for the equations of special relativistic hydrodynamics
Sib. Zh. Vychisl. Mat., 28:1 (2025), 75–87
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Using piecewise parabolic reconstruction of physical variables in Rusanov’s solver. II. Special relativistic magnetohydrodynamics equations
Sib. Zh. Ind. Mat., 27:1 (2024), 29–42
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Using piecewise parabolic reconstruction of physical variables in the Rusanov solver. I. The special relativistic hydrodynamics equations
Sib. Zh. Ind. Mat., 26:4 (2023), 49–64
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On a Godunov-type numerical scheme for describing the gas and dust components in problems of star formation
Sib. Zh. Ind. Mat., 26:1 (2023), 85–97
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Using low dissipation Lax-Friedrichs scheme for numerical modeling of relativistic flows
Sib. Zh. Vychisl. Mat., 26:4 (2023), 389–400
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Using piecewise-parabolic reconstruction of physics variables to constructing a low-dissipation HLL method for numerical solution of special relativistic hydrodynamics equations
Sib. Zh. Vychisl. Mat., 26:1 (2023), 57–75
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Supercomputer modelling of magnetohydrodynamical flows in cosmic plasma
Sib. Zh. Ind. Mat., 25:4 (2022), 14–26
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Mathematical simulation of nuclear carbon burning in White Dwarfs using a 7-isotope reaction network
Sib. Zh. Ind. Mat., 25:3 (2022), 55–66
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Mathematical modeling of high-speed collision of White Dwarfs — explosion mechanism of type Ia/Iax supernovae
Sib. Zh. Ind. Mat., 25:1 (2022), 80–91
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Using piecewise-linear reconstruction to constructing a low-dissipation HLL method for numerical solution of hydrodynamics equation
Sib. Zh. Vychisl. Mat., 25:2 (2022), 141–156
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Mathematical simulation of turbulent combustion of carbon in the problems of white dwarf mergers and explosions of the type Ia supernovae
Sib. Zh. Ind. Mat., 24:3 (2021), 30–38
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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
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Application of geodesic grids for modeling the hydrodynamic processes in spherical objects
Sib. Zh. Ind. Mat., 23:4 (2020), 77–87
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On a modification of the Rusanov solver
for the equations of special relativistic
magnetic hydrodynamics
Sib. Zh. Ind. Mat., 23:3 (2020), 53–64
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The use of the piecewise parabolic method on a local stencil for
constructing a low dissipation of a numerical solution scheme for mathematical modeling
of special relativistic hydrodynamic flows
Sib. Zh. Vychisl. Mat., 23:2 (2020), 143–154
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An algorithm for recovering the characteristics of the initial state of supernova
Zh. Vychisl. Mat. Mat. Fiz., 60:6 (2020), 1035–1044
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Development of a system for performance analysis of mobile applications
Program Systems: Theory and Applications, 7:2 (2016), 127–135
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Numerical hydrodynamics simulation of astrophysical flows at Intel Xeon Phi supercomputers
Vestn. YuUrGU. Ser. Vych. Matem. Inform., 5:4 (2016), 77–97
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A multilevel approach to algorithm and software design for exaflops supercomputers
Num. Meth. Prog., 16:4 (2015), 543–556
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Computation of discontinuous solutions of fluid dynamics equations with entropy nondecrease guarantee
Zh. Vychisl. Mat. Mat. Fiz., 54:6 (2014), 1008–1021
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Numerical and experimental simulation of wave formation during explosion welding
Trudy Mat. Inst. Steklova, 281 (2013), 16–31
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AstroPhi : a hydrodynamical code for complex modelling of astrophysical objects dynamics by means of hybrid architecture supercomputers on Intel Xeon Phi base
Vestn. YuUrGU. Ser. Vych. Matem. Inform., 2:4 (2013), 57–79
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