Scalar and vector perturbations in a universe with nonlinear perfect fluid

dc.contributor.authorCanay, Ezgi
dc.contributor.authorRuslan, Brilenkov
dc.contributor.authorEingorn, Maxim
dc.contributor.authorArapo˘glu, A. Savas
dc.contributor.authorZhuk, Oleksandr I.
dc.contributor.authorЖук, Олександр Іванович
dc.contributor.authorЖук, Александр Иванович
dc.date.accessioned2022-06-23T19:34:25Z
dc.date.available2022-06-23T19:34:25Z
dc.date.issued2021
dc.description.abstractWe study a three-component universe filled with dust-like matter in the form of discrete inhomogeneities (e.g., galaxies) and perfect fluids characterized by linear and nonlinear equations of state. Within the cosmic screening approach, we develop the theory of scalar and vector perturbations. None of the energy density contrasts associated with the distinct components is treated as small. Consequently, the derived equations are valid at both sub- and super-horizon scales and enable simulations for a variety of cosmological models.uk_UA
dc.identifier.citationThe European Physical Journal Cuk_UA
dc.identifier.doihttps://doi.org/10.1140/epjc/s10052-021-09032-9
dc.identifier.urihttps://dspace.onu.edu.ua/handle/123456789/33196
dc.language.isoenuk_UA
dc.relation.ispartofseries;Vol. 81.
dc.subjectvector perturbationsuk_UA
dc.subjectnonlinear perfect fluiduk_UA
dc.titleScalar and vector perturbations in a universe with nonlinear perfect fluiduk_UA
dc.typeArticleuk_UA
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20.Canay, E., R. Brilenkov, M. Eingorn, A. S. Arapo_lu, and A. Zhuk. 2021. Scalar.pdf
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