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Unsteady non-Newtonian magnetohydrodynamic radiative thin film flow in a porous medium past an oscillating vertical belt

dc.contributor.authorDada, M.S.
dc.contributor.authorYakub, L.
dc.contributor.authorAdeyemo, A.S.
dc.date.accessioned2019-10-15T10:54:05Z
dc.date.available2019-10-15T10:54:05Z
dc.date.issued2018
dc.description.abstractThis study examines the unsteady non-Newtonian magnetohydrodynamic radiative thin film flow in a porous medium past an oscillating vertical belt. Based on the physical model of the problem, the governing momentum and energy equations are non dimensionalized and solved analytically using Optimal Homotopy Asymptotic Method (OHAM). The velocity and temperature profiles are studied for different physical parameters such as the magnetic field, radiation parameter, Grashof number, Prandtl number, and Brinkman number for both lift and drainage problems. The analytical results are presented graphically and discussed.en_US
dc.description.sponsorshipSelfen_US
dc.identifier.urihttp://hdl.handle.net/123456789/2539
dc.language.isoenen_US
dc.publisherCentrepoint Journal (Science Edition), University of Ilorin, Ilorin.en_US
dc.relation.ispartofseries24(2);175-196
dc.subjectOHAMen_US
dc.subjectThin filmen_US
dc.subjectUnsteadyen_US
dc.subjectSecond grade fluiden_US
dc.subjectBuoyancyen_US
dc.subjectViscous dissipationen_US
dc.titleUnsteady non-Newtonian magnetohydrodynamic radiative thin film flow in a porous medium past an oscillating vertical belten_US
dc.typeArticleen_US

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