Radiative Magnetohydrodynamics Casson Nanofluid Flow and Heat and Mass Transfer past on Nonlinear Stretching Surface

  1. Gurrala ThirupathiORCID Logo,
  2. Kamatam GovardhanORCID Logo and
  3. Ganji NarenderORCID Logo

Submitting author affiliation: CVR College of Engineering, Hyderabad, India

Beilstein Arch. 2021, 202165. https://doi.org/10.3762/bxiv.2021.65.v1

Published 23 Sep 2021

  • Preprint

Abstract

The magnetohydrodynamics (MHD) stagnation point Casson nanofluid flow towards stretching surface with velocity slip and convective boundary condition has been investigated in this article. Effects of thermal radiation, viscous dissipation, heat source and chemical reaction have also been incorporated. Using appropriate similarity transformation Partial Differential Equations (PDEs) are converted into Ordinary Differential Equations (ODEs) and shooting technique along with Adams–Moulton method of order four has been used to obtain the numerical results. Different physical parameters effects on velocity, temperature and concentration of nanofluid flow have been presented graphically and discussed in detail. Numerical values of the skin friction coefficient, Nusselt number and Sherwood number are also and discussed.

Keywords: Casson Nanofluid, MHD, Thermal radiation, Chemical reaction, Viscous dissipation.

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When a peer-reviewed version of this preprint is available, this information will be updated in the information box above. If no peer-reviewed version is available, please cite this preprint using the following information:

Thirupathi, G.; Govardhan, K.; Narender, G. Beilstein Arch. 2021, 202165. doi:10.3762/bxiv.2021.65.v1

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