Effects of Induced Magnetic Field, Hall Current and Radiative Heat on 3-D Unsteady Hydromagnetic Stagnation Flow of a Casson Fluid

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dc.contributor.advisorWinifred Mutukuen_US
dc.contributor.authorKyalo, Muli Gabriel
dc.date.accessioned2023-08-14T14:07:17Z
dc.date.available2023-08-14T14:07:17Z
dc.date.issued2023
dc.descriptionA Research Project Submitted in Partial Fulfilment of the Requirements for the Award of the Degree of Master of Science (Applied Mathematics) in the School of Pure and Applied Sciences of Kenyatta University, March 2023.en_US
dc.description.abstractIn this study, 3-D stagnation flow of an MHD viscous electrically conducting Casson fluid including effects of induced magnetic field, Hall current and radiative heat is analyzed. The unsteady state model governing the flow is analyzed by first coming up with non-linear partial differential equations. Secondly, similarity transformation is done to change the nonlinear partial differential equations which are non-linear to ordinary differential equations, in order to account for the boundary layer and ease the computation. The ordinary differential equations obtained are then solved numerically using the collocation method via the MATLAB software. Analysis is then done to investigate effects of flow parameters like Hall current, magnetic parameters, temperature field, the Casson parameter and unsteadiness parameter.en_US
dc.description.sponsorshipKenyatta Universityen_US
dc.identifier.urihttp://ir-library.ku.ac.ke/handle/123456789/26843
dc.language.isoenen_US
dc.publisherKenyatta Universityen_US
dc.subjectInduced Magnetic Fielden_US
dc.subjectHall Currenten_US
dc.subjectRadiative Heaten_US
dc.subject3-D Unsteady Hydromagnetic Stagnation Flowen_US
dc.subjectCasson Fluiden_US
dc.titleEffects of Induced Magnetic Field, Hall Current and Radiative Heat on 3-D Unsteady Hydromagnetic Stagnation Flow of a Casson Fluiden_US
dc.typeThesisen_US
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