In order to account for the observable Universe, any comprehensive theory or model of cosmology must draw from many disciplines of physics, including gauge theories of strong and weak interactions, the hydrodynamics and microphysics of baryonic matter, electromagnetic fields, and spacetime curvature, for example. Although it is difficult to incorporate all these physical elements into a single complete model of our Universe, advances in computing methods and technologies have contributed significantly towards our understanding of cosmological models, the Universe, and astrophysical processes within them. A sample of numerical calculations addressing specific issues in cosmology are reviewed in this article: from the Big Bang singularity dynamics to the fundamental interactions of gravitational waves; from the quark--hadron phase transition to the large scale structure of the Universe. The emphasis, although not exclusively, is on thosecalculations designed to test different models of cosmology against the observed Universe.
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Since a Living Reviews in Relativity article may evolve over time, please cite the access <date>, which uniquely identifies the version of the article you are referring to:
"Computational Cosmology: from the Early Universe to the Large Scale Structure",
Living Rev. Relativity 1, (1998), 9. URL (cited on <date>):
|Title||Physical and Relativistic Numerical Cosmology|
|Date||accepted 15 January 1998, published 26 January 1998|
|Title||Computational Cosmology: from the Early Universe to the Large Scale Structure|
|Date||accepted 11 August 1998, published 15 September 1998|
|Changes||Article revision that included addition of new figures, expanded existing sections, added several new sections
|Title||Computational Cosmology: From the Early Universe to the Large Scale Structure|
|Date||accepted 15 February 2001, published 20 March 2001|
|Changes||Article revision adding two new sections on 'chaotic scalar field dynamics' and 'SZ effect' and an appendix on basic equations and numerical methods.
|Date||accepted 9 December 2004, published 14 April 2005|
|Changes||Fast-track revision to include recent developments. 37 new references have been added.
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