dc.contributor.author |
Ignat’ev Y. |
|
dc.contributor.author |
Agathonov A. |
|
dc.date.accessioned |
2018-04-05T07:09:15Z |
|
dc.date.available |
2018-04-05T07:09:15Z |
|
dc.date.issued |
2017 |
|
dc.identifier.issn |
0202-2893 |
|
dc.identifier.uri |
http://dspace.kpfu.ru/xmlui/handle/net/129610 |
|
dc.description.abstract |
© 2017, Pleiades Publishing, Ltd. We investigate the asymptotic behavior of a cosmological model based on a phantom scalar field by qualitative analysis of the set of differential equations. We show that, as opposed to models with a classical scalar field, such models have stable asymptotic solutions with a constant value of the potential both in the infinite past and the infinite future. We also develop numerical models of the cosmological evolution with a phantom scalar field. |
|
dc.relation.ispartofseries |
Gravitation and Cosmology |
|
dc.title |
Qualitative and numerical analysis of a cosmological model based on a phantom scalar field with self-interaction |
|
dc.type |
Article |
|
dc.relation.ispartofseries-issue |
3 |
|
dc.relation.ispartofseries-volume |
23 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.relation.startpage |
230 |
|
dc.source.id |
SCOPUS02022893-2017-23-3-SID85028081692 |
|