Abstract

This article explores the impact of radiation and heat absorption on magneto-convective flow of Casson nanofluid over a stretching surface in a porous medium. The convective heat and mass boundary conditions are also taken into consideration in this study. The governing models are converted into a nonlinear ODE models and they are solved analytically using homotopy analysis method (HAM). The significance of physical parameters on velocity, temperature and nano particle volume fraction are discussed graphically.

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