dc.contributor.author |
Skugoreva M. |
|
dc.contributor.author |
Toporensky A. |
|
dc.date.accessioned |
2020-01-15T21:47:41Z |
|
dc.date.available |
2020-01-15T21:47:41Z |
|
dc.date.issued |
2019 |
|
dc.identifier.issn |
1434-6044 |
|
dc.identifier.uri |
https://dspace.kpfu.ru/xmlui/handle/net/155992 |
|
dc.description.abstract |
© 2019, The Author(s). We consider the cosmological evolution of a flat anisotropic Universe in f(T) gravity in the presence of a perfect fluid. It is shown that the matter content of the Universe has a significant impact of the nature of a cosmological singularity in the model studied. Depending on the parameters of the f(T) function and the equation of state of the perfect fluid in question the well-known Kasner regime of general relativity can be replaced by a new anisotropic solution, or by an isotropic regime, or the cosmological singularity changes its nature to a non-standard one with a finite values of Hubble parameters. Six possible scenarios of the cosmological evolution for the model studied have been found numerically. |
|
dc.relation.ispartofseries |
European Physical Journal C |
|
dc.title |
Anisotropic cosmological dynamics in f(T) gravity in the presence of a perfect fluid |
|
dc.type |
Article |
|
dc.relation.ispartofseries-issue |
10 |
|
dc.relation.ispartofseries-volume |
79 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.source.id |
SCOPUS14346044-2019-79-10-SID85073206641 |
|