A study of inclined magnetically driven Casson nanofluid using the Cattaneo-Christov heat flux model with multiple slips towards a chemically reacting radially stretching sheet

Abstract

A numerical investigation is carried out by taking into consideration a two-dimensional inclined magnetically driven Casson nanofluid near a stagnation point flowing past a chemically reacting radially stretching sheet to scrutinize the phenomena of conduction, thermal radiation, heat generation and absorption in the light of multiple slips. For the purpose of investigating the characteristics of heat transfer conscientiously, the frequently cited Cattaneo-Christov heat flux model has been taken into consideration. The equations describing the proposed flow problem have been described by employing the Buongiorno nanofluid model to explore the impact of Brownian motion, thermophoresis and thermal and mass slip conditions. A set of some appropriate similarity transformations has been incorporated for converting highly non-linear partial differential equations characterizing the designed flow model to a system of ordinary differential equations. The advantage of the efficiency of the shooting method has been taken for the numerical governance of the proposed flow equations. The impacts of apropos flow parameters on the flow velocity, concentration and temperature configurations have been examined via tables and graphs. It has been remarked that the velocity accelerates significantly and the skin friction coefficient also shows an increasing behavior by escalating the Casson parameter. Furthermore, by increasing the magnitude of the magnetic parameter, the velocity of the fluid decreases.

Keywords

Casson nanofluid / radially stretching sheet / stagnation point / magnetohydrodynamics (MHD) / heat generation/absorption / slip conditions

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