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dc.contributor.author | Ignat’ev Y.G. | |
dc.date.accessioned | 2021-02-25T20:33:15Z | |
dc.date.available | 2021-02-25T20:33:15Z | |
dc.date.issued | 2020 | |
dc.identifier.issn | 0040-5779 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/161697 | |
dc.description.abstract | © 2020, Pleiades Publishing, Ltd. Abstract: Using a self-consistent field, we construct a complete theory of the macroscopic description of cosmological evolution, including a subsystem of linear equations for the evolution of perturbations and nonlinear macroscopic Einstein equations and a scalar field. We present example solutions of this system showing the principal difference between cosmological models of the early universe constructed on homogenous and locally fluctuating scalar fields. | |
dc.relation.ispartofseries | Theoretical and Mathematical Physics(Russian Federation) | |
dc.subject | asymptotic behavior | |
dc.subject | averaging local fluctuations | |
dc.subject | cosmological model | |
dc.subject | cosmological singularity | |
dc.subject | macroscopic gravitation | |
dc.subject | scalar field | |
dc.subject | self-consistent field | |
dc.title | The self-consistent field method and macroscopic Einstein equations for the early universe | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 1 | |
dc.relation.ispartofseries-volume | 204 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 927 | |
dc.source.id | SCOPUS00405779-2020-204-1-SID85088598407 |