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 |
|