Magneto Mixed Convection of Williamson Nanofluid Flow through a Double Stratified Porous Medium in Attendance of Activation Energy

This article aims to develop a mathematical simulation of the steady mixed convective Darcy–Forchheimer flow Williamson nanofluid over linear stretchable surface. In addition, effects Cattaneo–Christov heat and mass flux, Brownian motion, activation energy, thermophoresis are also studied. The novel aspect this study is that it incorporates thermal radiation investigate physical solutal stratification on convection transfer. First, profiles velocity energy equations were transformed toward ordinary differential equation using appropriate similarity transformation. Then, system was modified by first-order ODEs in MATLAB solved bvp4c approach. Graphs tables imply impact parameters concentration, temperature, velocity, skin friction coefficient, mass, transfer rate. outcomes show temperature concentration reduced with more significant estimation.