f (T) gravity with scalar field viscous fluid

dc.contributor.author	Myrzakul, S R
dc.contributor.author	Imankul, M
dc.contributor.author	Arzimbetova, M
dc.contributor.author	Myrzakul, T R
dc.date.accessioned	2025-01-21T04:46:44Z
dc.date.available	2025-01-21T04:46:44Z
dc.date.issued	2021
dc.identifier.issn	1742-6596
dc.identifier.other	doi:10.1088/1742-6596/1730/1/012021
dc.identifier.uri	http://rep.enu.kz/handle/enu/20930
dc.description.abstract	We focus on a viable teleparallel cosmological model with a scalar field in a flat Friedman-Robertson-Walker universe. The Lagrangian and equations of motion are obtained. The case of an inhomogeneous viscous dark energy is considered and the cosmological parameters associated with the viscosity parameter are determined. It is shown that when considering constant viscosity and state parameter, the Universe expands exponentially	ru
dc.language.iso	en	ru
dc.publisher	Journal of Physics: Conference Series	ru
dc.relation.ispartofseries	1730 (2021) 012021;
dc.title	f (T) gravity with scalar field viscous fluid	ru
dc.type	Article	ru