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 |
|