Thermal Radiation Effect on Heat and Mass Transfer MHD Ternary Nanofluid Jet Flow over the Stretching Surface with Respect to Reacting Bio-Active Mixers

This article has tried to study the jet flow of the ternary nanofluid suspended with motile microorganisms across a porous medium under the influence of radiation energy. These conditions have been carefully considered to enhance the heating conductivity of the nanoparticles. The ternary nanofluids (rGo-CoFe2O4-TiO2/H2O) enhanced thermal conductivity due to (TiO2) and (rGo) improves its performance in heat exchange model and thermal energy storage solutions. The inclusion of magnetic nanoparticles (CoFe2O4) gives rise to magnetohydrodynamic (MHD) effects, allowing for control of flow and heat transfer through external magnetic fields. In this study, thermophoresis and Brownian motion have been observed using the modified Buongiorno's model. The numerical solutions of the governing equations for various parameters have been calculated by the "bvp4c" method in the MATLAB software. The obtained graph represents the results of axial velocity, temperature, concentration, and motile density profiles for the ternary nanofluid. The study observed that by increasing radiation, magnetic, and mixed convection parameters, the velocity of the fluid gets enhanced. The concentration of the fluid is majorly enhanced by the increment of the thermophoresis parameter. Meanwhile, the motile density increases with the fall of the bio-convection Schmidt number. In addition, tables of skin friction coefficient, Nusselt number, Sharewood number, and motile density number displayed significant results. This model can be utilized in rocket engines, medical sciences, water jets, atmospheric science, agriculture, Cooling, and heating systems.