In this paper a modification of existing mathematical model of MHD radiative
incompressible fluid flow over exponentially stretching sheet is given by
accumulating equation of mass transfer under an influence of chemical
reaction. Using local non-similarity variables method, governing equations
for heat and mass transfer of viscous fluid flow are efficiently remodeled
into the system of dimensionless partial differential equations (PDEs), and
later on the obtained system of dimensionless PDEs is tackled numerically
using MATLbuilt in solver bvp4c. Graphs of temperature, velocity and
concentration profiles are explained through variation of different values
of physical parameters. Significant effects of several parameters, for
example radiation and magnetic parameters, Eckert and Prandtl numbers on
local skin-friction coefficient, local Nusselt and Sherwood numbers are
computed in tabular form
Thermal Radiation Effects on Heat and Mass Transfer of Magnetohydrodynamics Dusty Jeffrey Fluid past an Exponentially Stretching Sheet
