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GRAVITY WITH SCALAR FIELD VISCOUS FLUID

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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.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.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.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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Attribution-NonCommercial-ShareAlike 3.0 United States Except where otherwise noted, this item's license is described as Attribution-NonCommercial-ShareAlike 3.0 United States