Показать сокращенную информацию
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 |