Calculating the inhomogeneous reionization of the universe
A numerical scheme for the solution of the three-dimensional, frequency- and time-dependent radiative transfer equation with variable optical depth is developed for modelling the reionization of the Universe. Until now, the main difficulty in simulating the inhomogeneous reionization has been the...
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| Language: | English |
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2009
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| Online Access: | http://hdl.handle.net/2429/10847 |