Melting and heat generating influences on radiative flow of two-phase magneto-Williamson nanofluid via stretchable surface with slippage velocity and activation energy

• DOI: 10.1080/10407782.2024.2322703
• Publication Date: 2024-03-07T13:55:25Z
• Authors: Imran Ullah; Wasim Jamshed; Nek Muhammad Katbar; Mohamed R. Eid; Faisal Z. Duraihem; Siti Suzilliana P...; Rabha W. Ibrahim; Afrah M. AlDerea
• Keywords: Slippage; Heat flow; Magneto

Melting heat and solutal transference in a magnetohydrodynamic flowing of Williamson nanofluid have been described, with the mathematical model guided by Arrhenius activation energy, chemically reactive species, convective boundary restrictions. By implementing suitable similarity conversions, regulating equations partial differential (PDEs) (formed continuity, impetus, concentricity components) are condensed to an arrangement ordinary (ODEs). These commonalities nonlinear form, which includes fluid's velocity, heat, concentration changes. Finally, standard Keller box approach is used solve this ODEs system computationally (KBM). Under influence parameters, computational results tallied displayed diagrams. The friction force factor, local Nusselt, Sherwood values tabulated. Furthermore, contours plotted versus fluid thickness. attributes flowing, melting transfer, mass debated depth toward end study. Among most important outcomes that reached rate transport heightened between 52.5 55.2% detraction magnetic field, Weissenberg number, Brownian motion. We also found there inverse relationship transmission generating factor.