Cattaneo–Christov heat flux model on Blasius–Rayleigh–Stokes flow through a transitive magnetic field and Joule heating
This article addresses the Cattaneo–Christov heat flux, radiation and joule heating model as applied to a Blasius–Rayleigh–Stokes flow through a transitive magnetic field. The mathematical models are converted into a pair of self-similarity equations by applying appropriate transformations. The redu...
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Published in | Physica A Vol. 548; p. 123991 |
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Main Authors | , , , , |
Format | Journal Article |
Language | English |
Published |
Elsevier B.V
15.06.2020
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Subjects | |
Online Access | Get full text |
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Summary: | This article addresses the Cattaneo–Christov heat flux, radiation and joule heating model as applied to a Blasius–Rayleigh–Stokes flow through a transitive magnetic field. The mathematical models are converted into a pair of self-similarity equations by applying appropriate transformations. The reduced similarity equivalences are then solved numerically by the Runge–Kutta–Fehlberg 45th-order method. To better perceive the problem, the flow and energy transfer characteristics are explored for distinct values of different factors. From this analysis we found that Higher values of Q increase the f′η field and its interrelated thickness of the boundary layer. The temperature of the fluid and its interrelated layer thickness enhances for boost up values ofγ . Also found that the streamline graphs are dominant for Q=2 when compared with Q=0.5. The presence of Q has more impact on the results when compared to the case where Q is absent. The local RexCfx and NuxRex−12 scale back for increasing values of ω.
•The streamline graphs are dominant for Q=2 when compared with Q=0.5.•θ(η) field rises of enhanced values of R.•An intensification in the f′(η) field is seen with the increment of ω and Q.•Interrelated thickness of the thermal boundary layer decays for higher values of Pr.•The heat transfer rate is greater in the presence of R than in the absence of R.•The presence of Q has more impact on the results when compared to the case where Q is absent. |
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ISSN: | 0378-4371 1873-2119 |
DOI: | 10.1016/j.physa.2019.123991 |