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Magnetic dipole effects on unsteady flow of Casson-Williamson nanofluid propelled by stretching slippery curved melting sheet with buoyancy force

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dc.contributor.author Kumar, Pradeep
dc.contributor.author Nagaraja, Basavarajappa
dc.contributor.author Almeida, Felicita
dc.contributor.author AjayKumar, Abbani Ramakrishnappa
dc.contributor.author Al-Mdallal, Qasem
dc.contributor.author Jarad, Fahd
dc.date.accessioned 2024-01-03T13:27:40Z
dc.date.available 2024-01-03T13:27:40Z
dc.date.issued 2023-12
dc.identifier.citation Kumar, Pradeep;...et.al. (2023). "Magnetic dipole effects on unsteady flow of Casson-Williamson nanofluid propelled by stretching slippery curved melting sheet with buoyancy force", tr_TR
dc.identifier.issn 20452322
dc.identifier.uri http://hdl.handle.net/20.500.12416/6845
dc.description.abstract In particular, the Cattaneo-Christov heat flux model and buoyancy effect have been taken into account in the numerical simulation of time-based unsteady flow of Casson-Williamson nanofluid carried over a magnetic dipole enabled curved stretching sheet with thermal radiation, Joule heating, an exponential heat source, homo-heterogenic reactions, slip, and melting heat peripheral conditions. The specified flow's partial differential equations are converted to straightforward ordinary differential equations using similarity transformations. The Runge–Kutta–Fehlberg 4-5th order tool has been used to generate solution graphs for the problem under consideration. Other parameters are simultaneously set to their default settings while displaying the solution graphs for all flow defining profiles with the specific parameters. Each produced graph has been the subject of an extensive debate. Here, the analysis shows that the thermal buoyancy component boosts the velocity regime. The investigation also revealed that the melting parameter and radiation parameter had counterintuitive effects on the thermal profile. The velocity distribution of nanofluid flow is also slowed down by the ferrohydrodynamic interaction parameter. The surface drag has decreased as the unsteadiness parameter has increased, while the rate of heat transfer has increased. To further demonstrate the flow and heat distribution, graphical representations of streamlines and isotherms have been offered. tr_TR
dc.language.iso eng tr_TR
dc.relation.isversionof 10.1038/s41598-023-39354-5 tr_TR
dc.rights info:eu-repo/semantics/openAccess tr_TR
dc.title Magnetic dipole effects on unsteady flow of Casson-Williamson nanofluid propelled by stretching slippery curved melting sheet with buoyancy force tr_TR
dc.type article tr_TR
dc.relation.journal Scientific Reports tr_TR
dc.contributor.authorID 234808 tr_TR
dc.identifier.volume 13 tr_TR
dc.identifier.issue 1 tr_TR
dc.contributor.department Çankaya Üniversitesi, Fen - Edebiyat Fakültesi, Matematik Bölümü tr_TR


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