Abstract
ABSTRACT The thermophysical feature of a 2D flow of a dusty Eyring-Powell fluid caused by a stretched sheet in the presence of magnetic field was assessed in the present study. The similarity transformation had been considered for transforming the dimensionless heat and fluid flow basic partial differential equations into simple ordinary equations. After that, the Runge-Kutta-Fehlberg 45 solver utilizes numerical methods to resolve the altered equations. We study and discuss in depth the flowing and heating attributes under various parameters, including the magnetic parameter, Eyring Powell fluid parameter, fluid particle interaction parameter and Prandtl number. In order to validate the reliability of the numerical solution, the findings that were produced are contrasted with the results that were achieved in the past. It has been proven numerically that the velocity of the fluid phase and particle phase both increases when the Eyring Powell fluid parameter is increased.
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