Please use this identifier to cite or link to this item: http://dspace.onu.edu.ua:8080/handle/123456789/5891
Full metadata record
DC FieldValueLanguage
dc.contributor.authorBrilenkov, R. D.-
dc.contributor.authorEingorn, Maxim V.-
dc.contributor.authorZhuk, Oleksandr I.-
dc.date.accessioned2015-02-23T12:13:11Z-
dc.date.available2015-02-23T12:13:11Z-
dc.date.issued2014-
dc.identifier.citationOdessa Astronomical Publicationsuk
dc.identifier.urihttp://dspace.onu.edu.ua:8080/handle/123456789/5891-
dc.descriptionOdessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2014 . – Vol.27, I. 1.uk
dc.description.abstractTo describe the density profile of dark matter halos of clusters of galaxies, we compare the approach based on the Schwarzschild-de Sitter metric with a recently developed mechanical one (discrete cosmology inside the cell of uniformity). In the first approach, the cosmological effects are completely incorporated into the cosmological constant, while in the second one the scale factor enters directly the corresponding equations. Hence, in the latter case we can take into account the effect on the density profiles not only the cosmological constant, but also other material components. Thus, we can evaluate how this dynamic impact is considerable and testable.uk
dc.language.isoenuk
dc.publisherAstroprintuk
dc.relation.ispartofseries;V. 27, I. 1, P. 23.-
dc.subjectDark matteruk
dc.subjectgalaxy clusteruk
dc.titleDifferent approaches for dark matter halos of clusters of galaxiesuk
dc.typeArticleuk
Appears in Collections:Odessa Astronomical Publications

Files in This Item:
File Description SizeFormat 
9.pdf264.29 kBAdobe PDFThumbnail
View/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.