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dc.contributor.authorBurgazli, A. Yu.-
dc.contributor.authorEingorn, Maxim V.-
dc.contributor.authorZhuk, Oleksandr I.-
dc.date.accessioned2015-02-23T12:22:53Z-
dc.date.available2015-02-23T12:22:53Z-
dc.date.issued2014-
dc.identifier.citationOdessa Astronomical Publicationsuk
dc.identifier.urihttp://dspace.onu.edu.ua:8080/handle/123456789/5893-
dc.descriptionOdessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2014 . – Vol.27, I. 1.uk
dc.description.abstractWe investigate the role of the scalar field assuming its presence at late stages of the Universe evolution together with dust presented by a system of an arbitrary number of gravitating masses (galaxies, groups of galaxies and clusters of galaxies) and the cosmological constant in the framework of the theory of scalar cosmological perturbations. In particular, we discuss the case of the homogeneous scalar field and its possible influence on the gravitational potentials representing metric perturbations. We also focus attention on the interconnection between the astrophysical problem and the cosmological one in the scalar field presence.uk
dc.language.isoenuk
dc.publisherAstroprintuk
dc.relation.ispartofseries;V. 27, I. 1, P. 24-25.-
dc.subjectOdessa Astronomical Publicationsuk
dc.subjectgravitational potentialuk
dc.subjectinhomogeneous Universeuk
dc.subjectperturbationsuk
dc.subjectphantomuk
dc.subjectscalar fieldsuk
dc.subjectquintessenceuk
dc.titleCosmological perturbations in presence of scalar fieldsuk
dc.typeArticleuk
Appears in Collections:Odessa Astronomical Publications

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