Abstract

The classical von Karman equations governing the boundary layer flow induced by a rotating disk are solved using the spectral homotopy analysis method and a novel successive linearisation method. The methods combine nonperturbation techniques with the Chebyshev spectral collocation method, and this study seeks to show the accuracy and reliability of the two methods in finding solutions of nonlinear systems of equations. The rapid convergence of the methods is determined by comparing the current results with numerical results and previous results in the literature.

Highlights

  • Most natural phenomena can be described by nonlinear equations that, in general, are not easy to solve in closed form

  • Our focus is on the original von Karman equation for the steady, laminar, axially symmetric viscous flow induced by an infinite disk rotating steadily with angular velocity Ω about the z-axis with the fluid confined to the half-space z > 0 above the disk

  • To check the accuracy of the successive linearisation method and the spectral homotopy analysis method, comparison is made with numerical solutions obtained using the Matlab bvp4c routine, which is an adaptive Lobatto quadrature scheme see 22

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Summary

Introduction

Most natural phenomena can be described by nonlinear equations that, in general, are not easy to solve in closed form. The study of the steady, laminar, and axially symmetric viscous flow induced by an infinite disk rotating steadily with constant angular velocity was pioneered by von Karman 1 He showed that the Navier-Stokes equations could be reduced to a set of ordinary differential equations and solved using an approximate integral method. Turkyilmazoglu used the homotopy analysis method to solve the equations governing the flow of a steady, laminar, incompressible, viscous, and electrically conducting fluid due to a rotating disk subjected to a uniform suction and injection through the walls in the presence of a uniform transverse magnetic field For this extended form of the von Karmam problem, the homotopy analysis method, produced secular terms in the series solution. Inter alia, that notwithstanding the fact that these two methods may involve more computations per step than the HAM, both the SHAM and SLM are efficient, robust, and converge much more rapidly compared to the standard homotopy analysis method

Governing Equations
The Spectral Homotopy Analysis Method
L2 h ξ
Successive Linearisation Method
MHD Swirling Boundary Layer Flow
Results and Discussion
Conclusions

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