Numerical analysis of unsteady momentum and heat flow of dusty tangent hyperbolic fluid in three dimensions

This paper explores the impact of MHD and viscous dissipation with joule heating on convective stretching flow of dusty tangent hyperbolic fluid over a sheet in 3D. A time-dependent magnetic field is applied along the z-axis and the sheet being stretched along the xy-plane. The fluid and dust particles motions are coupled only through drag and heat transfer between them. The effect of viscous dissipation with convection is appreciable when the generated kinetic energy becomes appreciable as compared to the amount of heat transferred. A well known bvp4c method has been used to find the fruitful results. Graphs and tables show the facts and figures for physical properties according to different parameters. The main findings are that Increase in power law index, magnetic field, Weissenberg effect, concentration of dust particles, and unsteadiness parameter reduces the flow of fluid and solid granules.

Automated summary

This paper examines the impact of MHD and viscous dissipation with joule heating on the convective stretching flow of dusty tangent hyperbolic fluid in 3D. The findings suggest that various parameters such as the power law index, magnetic field strength, Weissenberg effect, dust particle concentration, and unsteadiness parameter can influence the flow of fluid and solid granules.