Due to the vast body of literature on numerical simulations of the post-combination epoch, it is possible to mention only a small fraction of all the published papers. Hence, the following summary is limited to cover just a few aspects of computational physical cosmology, and in particular those that can potentially be used to discriminate between cosmological model parameters, even within the realm of the standard model.

- 3.1 The Standard Model
- 3.2 Newtonian Order Perturbations
- 3.3 Microwave Background
- 3.4 Gravitational Lensing
- 3.5 Ly Forest
- 3.6 Galaxy Clusters

Physical and Relativistic Numerical Cosmology
Peter Anninos
http://www.livingreviews.org/lrr-1998-2
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