2013
DOI: 10.5560/zna.2013-0041
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General Solutions for Magnetohydrodynamic Natural Convection Flow with Radiative Heat Transfer and Slip Condition over a Moving Plate

Abstract: General solutions for the magnetohydrodynamic (MHD) natural convection flow of an incompressible viscous fluid over a moving plate are established when thermal radiation, porous effects, and slip condition are taken into consideration. These solutions, obtained in closed-form by Laplace transform technique, depend on the slip coefficient and the three essential parameters Gr, Pr eff , and K eff . They satisfy all imposed initial and boundary conditions and can generate a large class of exact solutions correspo… Show more

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Cited by 33 publications
(25 citation statements)
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References 10 publications
(21 reference statements)
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“…-The solution presented in this article is more general and includes the solution corresponding to radiative problem as a special case. This conclusion is also supported by recent papers by Magyari and Pantokratoras [38], Fetecau et al [39], and Vieru et al [40], where it is explicitly shown that an evaluation of the effect of thermal radiation in the linearized Rosseland approximation does not require any additional research effort. Once the problem has been solved for a comprehensive set of values of the Prandtl number in the absence of radiation, it has been automatically solved for the radiative case too.…”
Section: Convergence Of Ham Solution and Its Comparison With A Numerisupporting
confidence: 73%
“…-The solution presented in this article is more general and includes the solution corresponding to radiative problem as a special case. This conclusion is also supported by recent papers by Magyari and Pantokratoras [38], Fetecau et al [39], and Vieru et al [40], where it is explicitly shown that an evaluation of the effect of thermal radiation in the linearized Rosseland approximation does not require any additional research effort. Once the problem has been solved for a comprehensive set of values of the Prandtl number in the absence of radiation, it has been automatically solved for the radiative case too.…”
Section: Convergence Of Ham Solution and Its Comparison With A Numerisupporting
confidence: 73%
“…In the case of no slip on the boundary, our solution (32) together with (34) is identical with the result obtained by Fetecau et al (see [24], Eq. (31) with eff = 0).…”
Section: Newtonian Fluid With/without Slip Conditionsupporting
confidence: 90%
“…As expected, the velocity field (19) is identical to that obtained by Fetecau et al [13,Eq. (31) with K eff = 0] while the shear stress (20) can be also obtained by introducing Eq.…”
Section: Solution Of the Problemsupporting
confidence: 83%