Geodesic
Modelling of Radiative Heat Transfer in Circumstellar Media by Monte-Carlo Method
Sibirskij žurnal čistoj i prikladnoj matematiki, Tome 11 (2011) no. 2, pp. 15-20

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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. 
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     author = {S. A. Brednikhin and B. A. Kargin},
     title = {Modelling of {Radiative} {Heat} {Transfer} in {Circumstellar} {Media} by {Monte-Carlo} {Method}},
     journal = {Sibirskij \v{z}urnal \v{c}istoj i prikladnoj matematiki},
     pages = {15--20},
     publisher = {mathdoc},
     volume = {11},
     number = {2},
     year = {2011},
     language = {ru},
     url = {http://geodesic.mathdoc.fr/item/VNGU_2011_11_2_a1/}
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S. A. Brednikhin; B. A. Kargin. Modelling of Radiative Heat Transfer in Circumstellar Media by Monte-Carlo Method. Sibirskij žurnal čistoj i prikladnoj matematiki, Tome 11 (2011) no. 2, pp. 15-20. http://geodesic.mathdoc.fr/item/VNGU_2011_11_2_a1/