Impact of ferromagnetic nanoparticles on convectively heated radiative flow of Williamson nanofluid

Recent developments in technology as well as rapid increase in world's population are the major factors that compelled the researchers to pay their attention in seeking some innovative and efficient sources of acquiring energy rather than fossil fuels. There are two basic reasons for which it got popularity firstly day by day declination of fossil fuels secondly their major harmful effects so researchers are struggling for such an alternate that can overcome these two basic problems so solar energy is proven a best solution of these issues because it is found abundantly in nature also it is environment friendly, so research community paid full attention toward it. Another solution of above faced problem is by usage of thermally more efficient fluid that is nanofluid; it is environmental friendly and energy saving too. The nonlinear partial differential equations are reduced to dimensionless form by using some suitable similarity transformations. The approximate solution was attained by MATLAB software using a pure numeric technique known as bvpc4. The effects of the salient parameters on velocity distribution, temperature of Williamson ferro fluid and concentration are physically interpreted and displayed pictorially. Temperature of Williamson ferro fluid intensifies for larger values of thermophoretic and Brownian motion parameters. Boungiorno relation has contrary behavior for concentration field Heat transfer rate dwindles against both Nt and Nb .

Automated summary

Recent developments in technology and population growth have motivated researchers to search for innovative and efficient energy sources other than fossil fuels. Solar energy and nanofluids have emerged as the best solutions, as they are abundant in nature and environmentally friendly. Researchers have used numerical techniques and MATLAB software to study the effects of different parameters on velocity distribution, temperature, and concentration.