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KIAM Preprint № 76, Moscow, 2008
Authors: Bogovalov S.V., Koldoba A.V., Ustyugova G.V., Chechetkin V. M.
Numerical Simulation Evolution of the Crab Nebula. I. Mathematical Model
It was presented the mathematical model of Crab nebula. Flow of the ultrarelativistic plasma described by relativistic MHD model, which included energy-momentum and Maxwell equations in Lichnerovich form. The strong anisotropic of energy flow from pulsar was taken into consideration. Approximate solution of Riemann problem for RMHD equations was proposed.
Publication language: russian,  pages: 23
Research direction:
Mathematical modelling in actual problems of science and technics
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