GRAVITY WITH SCALAR FIELD VISCOUS FLUID

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dc.contributor.authorMyrzakul, S R
dc.contributor.authorImankul, M
dc.contributor.authorArzimbetova, M
dc.contributor.authorMyrzakul, T R
dc.date.accessioned2021-09-14T09:25:07Z
dc.date.available2021-09-14T09:25:07Z
dc.date.issued2021
dc.description.abstractWe 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 exponentiallyen_US
dc.identifier.citationMyrzakul, 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/10.1088/1742-6596/1730/1/012021en_US
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/5770
dc.language.isoenen_US
dc.publisherJournal of Physics: Conference Seriesen_US
dc.rightsAttribution-NonCommercial-ShareAlike 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.subjectType of access: Open Accessen_US
dc.subjectscalar fielden_US
dc.titleGRAVITY WITH SCALAR FIELD VISCOUS FLUIDen_US
dc.typeArticleen_US
workflow.import.sourcescience

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