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 |
|