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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 |