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The current research establishes magnetohydrodynamics (MHD) boundary layerflow with heat and mass transfer of a nanofluid over an exponentially extendingsheet embedded in a porous medium. During this exploration, nanoparticles,single-wall carbon nanotubes (SWCNTs) and multi-wall carbon nanotubes (MWCNTs)are recruited, while lamp fuel oil is being utilised as a base fluid for thediffusion of nano materials. The effects of warm radiation and an inclinedmagnetic field are included. In addition, rather than no-slip assumptions atthe surface, velocity slides as well as thermal upsurge are incorporated inthis study. Similarity transformations are implemented to adapt a set ofpartial differential equations into a system of non-linear ordinarydifferential equations. The bvp4c solver and Keller-box approach are employedto tackle nonlinear ordinary differential equations numerically. Thesignificance of prominent parameters such as the Darcy Forchheimer model,magnetic field, radiation, suction, velocity slip, and temperature jump isvisually probed and addressed in depth. In fact, the evolution of thecoefficient of skin friction and percentage of heat shipping (Nusselt number)for both SWCNTs and MWCNTs is presented in tabular form. The temperature goesup as the magnetic parameter rises. Temperature has been seen to be decreasedas the thermal slip parameter is improved. The results indicate that SWCNTsyield a higher coefficient of skin friction and speed of heat transformationthan MWCNTs.

Impact of Radiation and Slip Conditions on MHD Flow of Nanofluid Past an Exponentially Stretched Surface