The hydrodynamical modeling of the Supernovae Ia explosion by means adaptive nested meshes on supercomputers

The results of the study of an explosion point of supernova type Ia (SNIa) with using of mathematical modeling on supercomputers is given in the paper. Hydrodynamical model closed by the stellar equation of state and supplemented by Poisson equation for gravitational potential is used for modeling o...

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Bibliographic Details
Published in:Journal of physics. Conference series Vol. 1268; no. 1; pp. 12038 - 12043
Main Authors: Kulikov, Igor, Chernykh, Igor, Protasov, Viktor
Format: Journal Article
Language:English
Published: Bristol IOP Publishing 01.07.2019
Subjects:
Carbon
Combustion
Distributed memory
Equations of state
Evolution
Exact solutions
Godunov method
Numerical methods
Physics
Poisson equation
Supercomputers
Supernovae
White dwarf stars
ISSN:1742-6588, 1742-6596
Online Access:Get full text
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Summary:The results of the study of an explosion point of supernova type Ia (SNIa) with using of mathematical modeling on supercomputers is given in the paper. Hydrodynamical model closed by the stellar equation of state and supplemented by Poisson equation for gravitational potential is used for modeling of a white dwarf. The nuclear combustion of carbon, for which the analytical solution is constructed, is accounted in the model. A multilevel organization of computations on nested grids is used in the solution. The new highorder accuracy numerical method based on the Godunov method, the Rusanov scheme and the piecewise parabolic method on local stencil, adapted for computations on nested grids, is built. The parallel implementation is based on the idea of distributed computations, where the architecture with shared memory is used for modeling of the hydrodynamic evolution of white dwarfs, when the critical values of temperature and density are reached, a new task is launched on the architecture with distributed memory, in which the evolution of hydrodynamic turbulence leading to supersonic nuclear combustion of carbon is simulated.
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ISSN:1742-6588
1742-6596
DOI:10.1088/1742-6596/1268/1/012038