Formation of the large-scale structure of the Universe

Abstract

In this review, the formation, evolution, and decay of the large-scale structure of the Universe is discussed in the context of observational data, numerical simulations, and the Cosmological Standard Model (CSM). Problems concerning measuring and interpreting cosmological parameters, determining the composition of matter, and normalizing density perturbation spectra are especially highlighted.

66 pages, 19 figures

References in corpus (3)

• Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
• A Map of the Integrated Sachs-Wolfe Signal from Luminous Red Galaxies
• Legacy data and cosmological constraints from the angular-size/redshift relation for ultra-compact radio sources

Cited by in corpus (3)

• Small-scale clumps of dark matter
• Review of scientific topics for Millimetron space observatory
• A solution to the problems of cusps and rotation curves in dark matter halos in the cosmological standard model