Models for large-scale structure

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dc.creatorPeacock, J. A.
dc.date1998-10-29
dc.date.accessioned2026-07-07T02:28:48Z
dc.date.available2026-07-07T02:28:48Z
dc.descriptionThis 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.
dc.descriptionTo appear in the Proceedings of the MPA/ESO Conference "Evolution of large-scale structure", Garching, August 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9810476
dc.identifierhttp://arxiv.org/abs/astro-ph/9810476
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13215
dc.subjectAstrophysics
dc.titleModels for large-scale structure
dc.typetext

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