Abstract

Modern developments in nanotechnology have provided a fantastic foundation for creating a better ultra-high-performing coolant known as nanofluids for many applications in manufacturing and engineering. Numerous scholars have been drawn in by the hybrid nanomaterials’ capacity to improve heat transmission more to examine the working fluid. This study uses the mathematical solution to explore the effect of viscous dissipative on the radiative-convective Williamson hybrid nanofluid flow through an angled moving plate with a magnetic impression. Focusing on certain reasonable assumptions, a nonlinear partial differential equation system is developed and then numerically solved using the bvp4c method. It is thoroughly explained how a particular collection of distinctive factors affects the motion features, shear stress, temperature field profiles and heat transfer. The motion declined with increasing Williamson fluid for both stretching and shrinking surfaces. An upsurge profile for energy is showing for radiation impression. The shear rate falls with the inclined plate and increases with the buoyancy impression.

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