Melting heat transfer in magnetohydrodynamic radiative Williamson fluid flow with non-uniform heat source/sink

Abstract

Abstract. We analyzed the influence of melting heat transfer in magnetohydrodynamic radiative Williamson fluid flow past an upper paraboloid of revolution with viscous dissipation. The overseeing flow and thermal distributions of insecure flow is introduced and streamlined utilizing comparable and nonsimilar transforms. The diminished coupled nonlinear differential equations are solved systematically with the assistance of a strong explanatory strategy, in particular, the shooting technique. Numerical solutions for the imperative physical channel are figured and shown. The physical components of reasonable parameters are examined through the graphs of skin friction, local Nusselt number. Rising values of Eckert number depreciate the flow and heat transfer rate.

Finite element method solution of mixed convection flow of Williamson nanofluid past a radially stretching sheet

“…Also, Dapra and Scarpi and Vasudev et al discussed peristaltic motion of a Williamson fluid injected into a rock fracture and over a permeable surface, respectively. The influence of melting heat transfer in magnetohydrodynamics (MHD) flow of Williamson fluid over an upper paraboloid of revolution and nonlinear variable thickened surface was discussed by Kumaran et al and Hayat et al, respectively. Likewise, Khudair and Al‐Khafajy and Qayyum et al analyzed the influence of heat relocation in the MHD oscillatory flow of Williamson fluid through a porous medium and between two rotating disks in that order.…”