Physics
Scientific paper
Nov 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ijtp...36.2489k&link_type=abstract
International Journal of Theoretical Physics, Volume 36, Issue 11, pp.2489-2501
Physics
Scientific paper
Usually large 3D simulations are used to calculate the cosmic microwave background anisotropies induced by global scalar fields. By going to the large N limit and solving the equations of motion analytically, we can drastically reduce the amount of numerical computations needed, while still finding results quite similar to the corresponding functions in the texture model.
Durrer Ruth
Kunz Martin
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