Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-12-11
Astronomy and Astrophysics
Astrophysics
19 pages, 19 figures; substantial revision of content
Scientific paper
We present a new numerical approach that is able to solve the multi-dimensional radiative transfer equations in all opacity regimes on a Lagrangian, unstructured network of characteristics based on a stochastic point process. Our method reverses the limiting procedure used to derive the transfer equations, by going back to the original Markov process. Thus, we reduce this highly complex system of coupled differential equations to a simple one-dimensional random walk on a graph, which is shown to be computationally very efficient. Specifically, we use a Delaunay graph, which makes it possible to combine our scheme with a new smoothed particle hydrodynamics (SPH) variant proposed by Pelupessy et al.(2003). We show that the results of applying a two-dimensional implementation of our method with various suitable test cases agree with the analytical results, and we point out the advantages of using our method with inhomogeneous point distributions, showing examples in the progress. Hereafter, we present a supplement to our method, which can be useful in cases where the medium is optically very thin, and we conclude by stating some anticipated properties of this method in three dimensions, and announce future extensions.
Icke Vincent
Rijkhorst Erik-Jan
Ritzerveld Jelle
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