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.

PACS: 95.35.+d, 95.36.+x, 98.65.−r (all) DOI: 10.3367/UFNe.0181.201110a.1017 URL: https://ufn.ru/en/articles/2011/10/a/ 000299541300001 2-s2.0-84855919044 2011PhyU...54..983L Citation: Lukash V N, Mikheeva E V, Malinovsky A M "Formation of the large-scale structure of the Universe" Phys. Usp. 54 983–1005 (2011) BibTexBibNote ® (generic)BibNote ® (RIS)MedlineRefWorks Received: 28th, December 2010, revised: 26th, January 2011, accepted: 28th, February 2011 Оригинал: Лукаш В Н, Михеева Е В, Малиновский А М «Образование крупномасштабной структуры Вселенной» УФН 181 1017–1040 (2011); DOI: 10.3367/UFNr.0181.201110a.1017