Models for large-scale structure

Details Models for large-scale structure Models for large-scale structure

1998-10-29

arxiv.org/abs/astro-ph/9810476v1

Astronomy and Astrophysics

Astrophysics

To appear in the Proceedings of the MPA/ESO Conference "Evolution of large-scale structure", Garching, August 1998

Scientific paper

This paper reviews selected aspects of the growth of cosmological structure, covering the following general areas: (1) expected characteristics of linear density perturbations according to various candidate theories for the origin of structure; (2) low-order theory for statistical measures of fluctuations; (3) formation of nonlinear structures and nonlinear evolution of the mass distribution; (4) the relation between the density field and the galaxy distribution; (5) constraints on cosmological models from galaxy clustering and its evolution.

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