Abstract
The development of ground-breaking solar power technologies is considered to be one of the critical clarifications towards satisfying an increasing demand of energy worldwide. The use of solar energy had a remarkable benefit in current span. Furthermore, in numerous utilizations, there is a sympathetic requirement for augmenting the poor thermal conductivity of standard materials so as to develop effective heat transfer fluids. Nanofluids are fluid disturbances of nanoparticles and extensive analysis has been presented on nanofluid application in heat transfer developments. The crucial objective of this article is to scrutinize numerically the structure of unsteady 3D radiative flow of magneto-Carreau nanofluid. The Buongiorno's relation is utilized to visualize the effects of thermophoresis and Brownian motion on the Carreau nanoliquid. The convective heated surface is ponder for heat transfer mechanisms. Additionally, zero nanoparticle mass flux condition on the surface of the boundary is accounted. An appropriate conversion is used to alter the PDEs into ODEs and then elucidated numerically via bvp4c tactic. The impact of distinct parameters for shear thinning/thickening liquids on velocity component, nanoliquid temperature and concentration of Carreau fluid are reported graphically. It is deceptive that the temperature of the Carreau nanoliquid declines as the Prandtl number Pr augment. Additionally, it is reported from these plots that the concentration of Carreau nanoliquid decay as the Brownian motion parameter boost up and opposite performance is being acknowledged for thermophoresis parameter.