Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-08-25
Astrofizika, 51 (2008) 109-123; Engl. trans.: Astrophysics, 51 (2008) 85-98
Astronomy and Astrophysics
Astrophysics
11 pages, 4 figures
Scientific paper
10.1007/s10511-008-0010-9
In order to choose a numerical method for solving the time dependent equations of radiative transport, we obtain an exact solution for the time dependent radiation field in a one dimensional infinite medium with monochromatic, isotropic scattering for sources with an arbitrary spatial distribution and an arbitrary time variation of their power. The Lax-Wendroff method seems to be the most suitable. Because it is assumed that radiation delay is caused by the finite speed of light, the following difficulty arises when the numerical method is used: the region of variation of the variables (dimensionless coordinate \tau and time t) is triangular (the inequality \tau< t). This difficulty is overcome by expanding the unknown functions in series in terms of small values of the time and coordinate. By comparing the numerical and exact solutions for a point source with a given time dependence for its power and with pure scattering, the steps in the variables required to obtain a desired accuracy are estimated. This numerical method can be used to calculate the intensity and polarization of the radiation from sources in the early universe during epochs close to the recombination epoch.
Kirusheva S. L.
Nagirner Dmitrij I.
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