Forced convective Maxwell fluid flow through rotating disk under the thermophoretic particles motion

Numerical analysis is performed for incompressible Maxwell fluid model flow under the implications of thermophoresis and Cattaneo-Christov theory. Fluid motion is initiated by spinning of the disk. The system that comprises differential equations of partial derivatives is remodel into the system of differential equations by similarity transformations and then solved through Runge-Kutta-4 with shooting technique. The physical parameters, which emerging from derived system are discussed in graphical formats. An excellent proficiency of numerical process is analyzed by comparing the results with available literature in limiting scenario. The radial velocity initially improved and then declined by incrementing the Deborah number values. Further, it is executed that the azimuthal velocity field decays for higher magnetic parameter and Deborah number.