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dc.contributor.author | Muharlyamov R. | |
dc.contributor.author | Pankratyeva T. | |
dc.date.accessioned | 2020-01-21T20:40:45Z | |
dc.date.available | 2020-01-21T20:40:45Z | |
dc.date.issued | 2019 | |
dc.identifier.issn | 0973-1458 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/157608 | |
dc.description.abstract | © 2019, Indian Association for the Cultivation of Science. We investigate the Bianchi type-V cosmological model with dark matter and anisotropic dark energy. It is assumed that the two sources minimally interact, so their energy-momentum tensors are conserved separately. The proportionality condition that relates the shear scalar (σ) with the expansion scalar (θ) and the assumption of a diagonal energy–momentum tensor lead to some restriction on the metric functions. A special law is introduced for skewness parameter that describes the deviation of pressure from isotropy. This law can lead to models: the little rip, the big rip and the hybrid expansion. The hybrid expansion law provides a description of the transition of the Universe from deceleration to acceleration. The Universe behavior is discussed depending on the numerical parameters of the models. | |
dc.relation.ispartofseries | Indian Journal of Physics | |
dc.subject | 04.50.Kd | |
dc.subject | Anisotropic dark energy | |
dc.subject | Bianchi type-V | |
dc.subject | Dark energy | |
dc.title | The change of the Universe epochs within the scope of Bianchi type-V model | |
dc.type | Article | |
dc.collection | Публикации сотрудников КФУ | |
dc.source.id | SCOPUS09731458-2019-SID85069453420 |