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Preprints of the Keldysh Institute of Applied Mathematics, 2008, 076, 23 pp. (Mi ipmp428)  
Numerical simulation evolution of the Crab nebula. I. Mathematical model

S. V. Bogovalov, A. V. Koldoba, G. V. Ustyugova, V. M. Chechetkin
Full-text PDF (289 kB)
Abstract: 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.
Document Type: Preprint
Language: Russian
Citation: S. V. Bogovalov, A. V. Koldoba, G. V. Ustyugova, V. M. Chechetkin, “Numerical simulation evolution of the Crab nebula. I. Mathematical model”, Keldysh Institute preprints, 2008, 076, 23 pp.
Citation in format AMSBIB
\Bibitem{BogKolUst08}
\by S.~V.~Bogovalov, A.~V.~Koldoba, G.~V.~Ustyugova, V.~M.~Chechetkin
\paper Numerical simulation evolution of the Crab nebula. I.~Mathematical model
\jour Keldysh Institute preprints
\yr 2008
\papernumber 076
\totalpages 23
\mathnet{http://mi.mathnet.ru/ipmp428}
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