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The Theory of Large-Scale Structure of the Universe: Local Properties and Global Topology

Published online by Cambridge University Press:  04 August 2017

A. G. Doroshkevich ,
S. F. Shandarin  and
Ya.B. Zeldovich
A. G. Doroshkevich
Affiliation:
Keldysh Institute of Applied Mathematics, USSR Academy of Sciences, Moscow 125047, USSR
S. F. Shandarin
Affiliation:
Keldysh Institute of Applied Mathematics, USSR Academy of Sciences, Moscow 125047, USSR
Ya.B. Zeldovich
Affiliation:
Keldysh Institute of Applied Mathematics, USSR Academy of Sciences, Moscow 125047, USSR

Abstract

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Properties of the large-scale distribution of galaxies are considered. Particular attention is paid to properties of the large-scale structures such as anisotropy of superclusters and the existence of large regions practically devoid of galaxies. Another question discussed in detail is the link between superclusters and formation of a network or cellular structure. An explanation of the latter is proposed in the frame of the fragmentation scenario. The role of the neutrino rest mass is discussed.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 104: Early Evolution of the Universe and Its Present Structure , 1983 , pp. 387 - 391
Copyright
Copyright © Reidel 1983 

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