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Evolution of density and velocity profiles of matter in large voids

We analyse the evolution of cosmological perturbations which leads to the formation of large voids in the distribution of galaxies. We assume that perturbations are spherical and all components of the Universe - radiation, matter and dark energy - are continuous media with ideal fluid energy-momentu...

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Bibliographic Details
Main Authors: Tsizh, M., Novosyadlyj, B.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2016
Series:Advances in Astronomy and Space Physics
Online Access:http://dspace.nbuv.gov.ua/handle/123456789/119947
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