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dc.date.accessioned | 2019-01-22T20:31:49Z | |
dc.date.available | 2019-01-22T20:31:49Z | |
dc.date.issued | 2018 | |
dc.identifier.issn | 0004-640X | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/147580 | |
dc.description.abstract | © 2018, Springer Science+Business Media B.V., part of Springer Nature. It is shown that a suitable interaction between dark energy and dark matter in locally rotationally symmetric (LRS) Bianchi-I space-time can solve the coincidence problem and not contradict the accelerated expansion of present Universe. The interaction parameters are estimated from observational data. | |
dc.relation.ispartofseries | Astrophysics and Space Science | |
dc.subject | Anisotropic dark energy | |
dc.subject | Bianchi type I model | |
dc.subject | Dark energy | |
dc.title | Interacting dark sector and the coincidence problem within the scope of LRS Bianchi type I model | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 5 | |
dc.relation.ispartofseries-volume | 363 | |
dc.collection | Публикации сотрудников КФУ | |
dc.source.id | SCOPUS0004640X-2018-363-5-SID85045347255 |