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	2021-09-14T09:25:07Z
dc.date.available	2021-09-14T09:25:07Z
dc.date.issued	2021
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	en_US
dc.identifier.citation	Myrzakul, S. R., Imankul, M., Arzimbetova, M., & Myrzakul, T. R. (2021). gravity with scalar field viscous fluid. Journal of Physics: Conference Series, 1730(1), 012021. https://doi.org/10.1088/1742-6596/1730/1/012021	en_US
dc.identifier.uri	http://nur.nu.edu.kz/handle/123456789/5770
dc.language.iso	en	en_US
dc.publisher	Journal of Physics: Conference Series	en_US
dc.rights	Attribution-NonCommercial-ShareAlike 3.0 United States	*
dc.rights.uri	http://creativecommons.org/licenses/by-nc-sa/3.0/us/	*
dc.subject	Type of access: Open Access	en_US
dc.subject	scalar field	en_US
dc.title	GRAVITY WITH SCALAR FIELD VISCOUS FLUID	en_US
dc.type	Article	en_US
workflow.import.source	science

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