Chemical Reaction on Williamson Nanofluid’s Radiative MHD Dissipative Stagnation Point Flow over an Exponentially Inclined Stretching Surface with Multi-Slip Effects

A wide range oftechnological and industrial domains, including heating processors, electrical systems, mechanical systems, and others, are facing issues as a result ofthe recent developments in heat transmission. Nanofluids are a novel type ofheat transfer fluid that has the potential to provide solutions that will improve energy transfer. The current study investigates the effect ofa magnetic field on the two-dimensional flow ofWilliamson nanofluid over an exponentially inclined stretched sheet. This investigation takes into account the presence ofmulti-slip effects. We also consider the influence ofviscous dissipation, thermal radiation, chemical reactions, and suction on the fluid’s velocity. We convert the nonlinear governing partial differential equations (PDEs) ofthe fluid flow problem into dimensionless ordinary differential equations (ODEs) through the utilization ofsimilarity variables. We then use the homotopy analysis method (HAM) to numerically solve the resulting ordinary differential equations (ODEs). We demonstrate the effects ofnumerous elements on a variety ofprofiles through graphical and tabular representations. We observe a drop in the velocity profile whenever we increase either the magnetic number or the suction parameter. Higher values ofthe Williamson parameter lead to an increase in the thermal profile, while the momentum ofthe flow displays a trend in the opposite direction. The potential applications ofthis unique model include chemical and biomolecule detection, environmental cleansing, and the initiation ofradiation-induced chemical processes like polymerization, sterilization, and chemical synthesis.