DYNAMICS OF COSMIC BODIES IN THE OPEN UNIVERSE

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dc.contributor.authorKudinova, A. V.
dc.contributor.authorEingorn, Maxim V.
dc.contributor.authorZhuk, Oleksandr I.
dc.date.accessioned2014-03-22T09:21:47Z
dc.date.available2014-03-22T09:21:47Z
dc.date.issued2012
dc.descriptionOdessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2012 . – Vol.25/2.uk
dc.description.abstractABSTRACT. As it has been recently demonstrated,the mathematical model with the hyperbolic space(or, in other words, with the negative spatial curvature)is the most appropriate one for describing the inhomogeneous Universe at late stages of its evolution in the framework of the theory of scalar perturbations. In this model we develop a dynamic approach and investigate nonrelativistic motion of two, three and even more cosmic bodies against the cosmological background, perturbed locally by density inhomogeneities (namely, galaxies).uk
dc.identifier.citationOdessa Astronomical Publicationsuk
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/4743
dc.language.isoenuk
dc.publisherAstroprintuk
dc.relation.ispartofseries;vol. 25, issue 2, p. 130-132.
dc.subjectinhomogeneous Universeuk
dc.subjectLocal Groupuk
dc.subjectHubble flowsuk
dc.titleDYNAMICS OF COSMIC BODIES IN THE OPEN UNIVERSEuk
dc.typeArticleuk
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