UEWScholar Repository

Radiative MHD thin film flow of Williamson fluid over an unsteady permeable stretching sheet

Show simple item record

dc.contributor.author Shah Z.
dc.contributor.author Bonyah E.
dc.contributor.author Islam S.
dc.contributor.author Khan W.
dc.contributor.author Ishaq M.
dc.date.accessioned 2022-10-31T15:05:34Z
dc.date.available 2022-10-31T15:05:34Z
dc.date.issued 2018
dc.identifier.issn 24058440
dc.identifier.other 10.1016/j.heliyon.2018.e00825
dc.identifier.uri http://41.74.91.244:8080/handle/123456789/471
dc.description Shah, Z., Department of Mathematics, Abdul Wali Khan University, Mardan, Khyber Pakhtunkhwa 23200, Pakistan; Bonyah, E., Department of Information Technology Education, University of Education Winneba-(Kumasi Campus), Kumasi, 00233, Ghana; Islam, S., Department of Mathematics, Abdul Wali Khan University, Mardan, Khyber Pakhtunkhwa 23200, Pakistan; Khan, W., Department of Mathematics, Islamia College University, Peshawar, Khyber Pakhtunkhwa 25000, Pakistan; Ishaq, M., Department of Mathematics, Islamia College University, Peshawar, Khyber Pakhtunkhwa 25000, Pakistan en_US
dc.description.abstract In this research work we have examined the flow of Williamson liquid film fluid with heat transmission and having the impact of thermal radiation embedded in a permeable medium over a time dependent stretching surface. The fluid flow of liquid films is assumed in two dimensions. By using suitable similarity transformation the governing non-linear partial differential equations have been transformed into non-linear differential equations. An optimal approach has been used to acquire the solution of the modelled problem. The convergence of the technique has been shown numerically. The impact of the Skin friction and Nusslet number and their influence on thin film flow are shown numerically. Thermal radiation, unsteadiness effect and porosity have mainly focused in this paper. Furthermore, for conception and physical demonstration the entrenched parameters, like porosity parameter k, Prandtl number Pr, unsteadiness parameter S, Radiation parameter Rd, Magnetic parameter M, and Williamson fluid parameter have been discussed graphically in detail with their effect on liquid film flow. � 2018 The Authors en_US
dc.publisher Elsevier Ltd en_US
dc.subject Applied mathematics en_US
dc.subject Computational mathematics en_US
dc.title Radiative MHD thin film flow of Williamson fluid over an unsteady permeable stretching sheet en_US
dc.type Article en_US


Files in this item

Files Size Format View

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record

Search UEWScholar


Browse

My Account