Impact of chemical reaction in fully developed radiated mixed convective flow between two rotating disk

Flow of magnetohydrodynamic (MHD) viscous fluid between two rotating disks is modeled. Angular velocities of two disks are different. Flow is investigated for nonlinear mixed convection. Heat transfer is analyzed for nonlinear thermal radiation and heat generation/absorption. Chemical reaction is also implemented. Convective conditions of heat and mass transfer are studied. Transformations used lead to reduction of PDEs into the ODEs. The impacts of important physical variables like Prandtl number, Reynold number, Hartman number, mixed convection parameter, chemical reaction and Schmidt number on velocities, temperature and concentration are elaborated. In addition velocity and temperature gradients are physically interpreted. Our obtained results indicate that radial, axial and tangential velocities decrease for higher estimation of Hartman number. •Magnetohydrodynamic (MHD) flow of viscous fluid between two rotating disks is modeled.•Angular velocities of two disks are different.•Flow is investigated for nonlinear mixed convection.•Chemical reaction is scrutinized.•Convective conditions of heat and mass transfer are studied.