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Vestnik Novosibirskogo Gosudarstvennogo Universiteta. Seriya Matematika, Mekhanika, Informatika, 2011, Volume 11, Issue 2, Pages 15–20 (Mi vngu75)  
Modelling of Radiative Heat Transfer in Circumstellar Media by Monte-Carlo Method

S. A. Brednikhina, B. A. Karginb

a Novosibirsk State University
b Institute of Computational Mathematics and Mathematical Geophysics (Computing Center), Siberian Branch of the Russian Academy of Sciences, Novosibirsk
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Abstract: The present paper is devoted to modeling of radiative heat transfer in forming planetary systems. The solution of transfer equation for dusty media of spherical polydispersive silicate particles is considered.
An algorithm of computation of temperature distribution in circumstellar disks is proposed. Coincidence of numerical results and known analytical cases is shown. Spatial distribution of optical characteristics of $\beta$-Pictoris debris disk are obtained.
Keywords: statictical modelling, radiative heat transfer.
Received: 04.12.2009
Document Type: Article
UDC: 519.245:551.521.6
Language: Russian
Citation: S. A. Brednikhin, B. A. Kargin, “Modelling of Radiative Heat Transfer in Circumstellar Media by Monte-Carlo Method”, Vestn. Novosib. Gos. Univ., Ser. Mat. Mekh. Inform., 11:2 (2011), 15–20
Citation in format AMSBIB
\Bibitem{BreKar11}
\by S.~A.~Brednikhin, B.~A.~Kargin
\paper Modelling of Radiative Heat Transfer in Circumstellar Media by Monte-Carlo Method
\jour Vestn. Novosib. Gos. Univ., Ser. Mat. Mekh. Inform.
\yr 2011
\vol 11
\issue 2
\pages 15--20
\mathnet{http://mi.mathnet.ru/vngu75}
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