Показать сокращенную информацию
dc.contributor.author | Awad A. | |
dc.contributor.author | El Hanafy W. | |
dc.contributor.author | Nashed G. | |
dc.contributor.author | Odintsov S. | |
dc.contributor.author | Oikonomou V. | |
dc.date.accessioned | 2019-01-22T20:53:23Z | |
dc.date.available | 2019-01-22T20:53:23Z | |
dc.date.issued | 2018 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/149277 | |
dc.description.abstract | © 2018 IOP Publishing Ltd and Sissa Medialab. We investigate in detail the implications of the constant-roll condition on the inflationary era of a scalar field coupled to a teleparallel f(T) gravity. The resulting cosmological equations constitute a reconstruction technique which enables us to find either the f(T) gravity which corresponds to a given cosmological evolution, or the Hubble rate of the cosmological evolution generated by a fixed f(T) gravity. We also analyze in some detail the phase space of the constant-roll teleparallel gravity and we discuss the physical significance of the resulting fixed points and trajectories. Also we calculate the observational indices of a theory with given f(T) gravity, and we discuss all the implications of the constant-roll condition on these. As we demonstrate, the resulting theory can be compatible with the current observational data, for a wide range of values of the free parameters of the theory. | |
dc.subject | Cosmic singularity | |
dc.subject | cosmological perturbation theory | |
dc.subject | inflation | |
dc.subject | modified gravity | |
dc.title | Constant-roll inflation in f(T) teleparallel gravity | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 7 | |
dc.relation.ispartofseries-volume | 2018 | |
dc.collection | Публикации сотрудников КФУ | |
dc.source.id | SCOPUS-2018-2018-7-SID85051803939 |