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Heat Transfer Research
Fator do impacto: 0.404 FI de cinco anos: 0.8 SJR: 0.264 SNIP: 0.504 CiteScore™: 0.88

ISSN Imprimir: 1064-2285
ISSN On-line: 2162-6561

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Heat Transfer Research

DOI: 10.1615/HeatTransRes.2019025546
pages 1495-1512


Amar Rauf
Department of Mathematics, The Islamia University of Bahawalpur, Bahawalpur, 63100, Pakistan; Department of Mathematics, COMSATS University Islamabad, Sahiwal 57000, Pakistan
Zaheer Abbas
Department of Mathematics, The Islamia University of Bahawalpur, Bahawalpur 63100, Pakistan
Sabir A. Shehzad
Department of Mathematics, COMSATS University Islamabad, Sahiwal 57000, Pakistan


A numerical exploration of unsteady oscillatory three-dimensional magnetohydrodynamic (MHD) flow of a viscous liquid over rotating oscillatory disk is presented. The disk stretches in the radial direction with time-based sinusoidal oscillations. Adaptation of thermal radiation with the heat source/sink is made in the energy equation while the mass equation incorporates the impacts of a chemical reaction parameter. The normalized system of partial differential equations is obtained by implementing similarity transformations. Such system of equations is solved then by the finite difference scheme and successive overrelaxation (SOR) method. The analysis is presented to study the effects of dimensionless parameters appearing in the governing equations. The results are presented in the forms of graphs and tables. It is scrutinized that the increase in the magnetic parameter falls off the flow amplitude. The fluid temperature increased with the passage of time for enhancement in radiation parameter. The increase in the Sherwood number is observed for enhanced unsteady parameter and Schmidt number.


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