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dc.contributor.author | Permyakov E. | |
dc.date.accessioned | 2018-09-17T21:15:49Z | |
dc.date.available | 2018-09-17T21:15:49Z | |
dc.date.issued | 1997 | |
dc.identifier.issn | 1064-8887 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/134755 | |
dc.description.abstract | A homogeneous, spatially flat cosmological model induced by a massless scalar field is investigated. The parameter ξ of coupling of the field with the curvature can take any value. It is shown that the range of values of ξ is divided into three regions, ξ < 0, 0 < ξ < 1/6, and ξ > 1/6, each of which is characterized by the behavior of the scale factor in it. The points ξ = 0 and ξ= 1/6 are singular. Stages with exponential and power-law inflation are found in the ranges 0 < ξ < 1/6 and ξ > 1/6. An exponential inflationary stage with acceptable cosmological consequences can occur for small positive ξ. © 1997 Plenum Publishing Corporation. | |
dc.relation.ispartofseries | Russian Physics Journal | |
dc.title | Inflation in cosmological models with a nonminimally coupled, massless scalar field | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 3 | |
dc.relation.ispartofseries-volume | 40 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 265 | |
dc.source.id | SCOPUS10648887-1997-40-3-SID53249133248 |