Abstract
A new, very fast method for 3D radiative transfer on fully threaded grids with arbitrarily high angular resolution is presented. The method uses completely cell-based discretization, and is ideally suited for problems with diffuse background radiation, often encountered in cosmological and star formation models. We find that for accurate statistical study of intergalactic Ly α absorption lines, one needs of the order of a few hundred angular discretization elements even for models without radiative feedback from star-forming galaxies.
Original language | English |
---|---|
Pages (from-to) | 1413-1417 |
Number of pages | 5 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 362 |
Issue number | 4 |
DOIs | |
State | Published - Oct 1 2005 |
Keywords
- Intergalactic medium
- Methods: numerical
- Radiative transfer