Exponential space-based heat source on Sakiadis flow of a dusty nanofluid using KKL model useful in solar radiation

The emission of solar energy is one of the greatest challenges due to its global impact nowadays. Further, the improved heat transport properties of the nanofluids have also important aspects in industries as well as engineering equipment and any others. Therefore, the present analysis motivates the enhancement in the heat transport enrichment of Sakiadis nanofluid by imposing Koo-Kleinstreuer-Li (KKL) model conductivity along with dusty CuO nanoparticles in water. Dust particles in conjunction with the magnetic effect and the radiative heat explore its greater role in the enhancement of the heat transport phenomena. Suitable transformation is proposed for the governing equations to get its non-dimensional form with significant parameters to characterize the flow properties. Moreover, numerical treatment using Runge-Kutta shooting is a good approach to handle the complex nonlinear system equipped with nanofluid phase and dusty phase liquids. Several factors impacting the flow phenomena have been examined graphically. In careful observation, it reveals that the augmented thermal radiation along with the heat source encourages the nanofluid phase temperature but the reverse impact is rendered in the dust phase.