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On the Transfer of Resonant‐Line Radiation in Mesh Simulations
Author(s) -
Argyro Tasitsiomi
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/505682
Subject(s) - photon , radiative transfer , slab , discretization , adaptive mesh refinement , physics , computational physics , line (geometry) , cube (algebra) , space (punctuation) , polygon mesh , mesh generation , statistical physics , computer science , mathematical analysis , algorithm , optics , mathematics , geometry , finite element method , computer graphics (images) , geophysics , thermodynamics , operating system
The last decade has seen applications of Adaptive Mesh Refinement (AMR)methods for a wide range of problems from space physics to cosmology. With theadvent of these methods, in which space is discretized into a mesh of manyindividual cubic elements, the contemporary analog of the extensively studiedline radiative transfer (RT) in a semi-infinite slab is that of RT in a cube.In this study we provide an approximate solution of the RT equation, as well asanalytic expressions for the probability distribution functions (pdfs) of theproperties of photons emerging from a cube, and compare them with thecorresponding slab problem. These pdfs can be used to perform fastresonant-line RT in optically thick AMR cells where, otherwise, it could takeunrealistically long times to transfer even a handful of photons.Comment: 5 two-column pages, 2 figures; matches accepted version, to appear on Ap

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