Large-scale structure of the Universe. The Zeldovich approximation and the adhesion model

S.N. Gurbatov^a, A.I. Saichev^a, S.F. Shandarin^b
^aDepartment of Radiophysics, Lobachevsky Nizhny Novgorod State University, prosp. Gagarina 23, Nizhny Novgorod, 603950, Russian Federation
^bDepartment of Physics and Astronomy, University of Kansas, Lawrence, USA

A semianalytic formation model for the large-scale structure of the Universe (from a few to hundreds of megaparsecs) is discussed. The model is a natural generalization of Zeldovich’s 1970 approximation and is mathematically based on the Burgers equation for low or even vanishing viscosity. It offers a natural explanation of the galaxy distribution that is observed in the scale range mentioned above and is reminiscent in its shape of a 3D mosaic or a giant cosmic web. Many predictions of the model have been confirmed by modern observations. New theoretical results related to the Burgers model are discussed together with their applications to cosmology.

PACS: 95.35.+d, 95.36.+x, 98.65.−r (all)
DOI: 10.3367/UFNe.0182.201203a.0233
URL: https://ufn.ru/en/articles/2012/3/b/
Web of Science

000305464600001
Scopus

2-s2.0-84863449582
ADS NASA

2012PhyU...55..223G
Citation: Gurbatov S N, Saichev A I, Shandarin S F "Large-scale structure of the Universe. The Zeldovich approximation and the adhesion model" Phys. Usp. 55 223–249 (2012)

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Received: 29th, April 2011, revised: 26th, September 2011, accepted: 4th, October 2011

Оригинал: Гурбатов С Н, Саичев А И, Шандарин С Ф «Крупномасштабная структура Вселенной. Приближение Зельдовича и модель слипания» УФН 182 233–261 (2012); DOI: 10.3367/UFNr.0182.201203a.0233

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