Cattaneo-Christov heat and mass flux models on time-dependent swirling flow through oscillatory rotating disk

Document Type : Research Note


1 Department of Mathematics, The Islamia University of Bahawalpur, Bahawalpur, 63100, Pakistan

2 - Department of Mathematics, The Islamia University of Bahawalpur, Bahawalpur, 63100, Pakistan. - Department of Mathematics, COMSATS University Islamabad, Sahiwal Campus, 57000, Pakistan.

3 Department of Mathematics, COMSATS University Islamabad, Sahiwal Campus, 57000, Pakistan

4 Department of Mathematics, Faculty of Science, King Khalid University, Abha 61413, Saudi Arabia



This analysis emphasis on the time invariant impressions of Cattaneo-Christov heat and mass flux theories are implemented to overcome the initial instant disturbances throughout whole medium. The motion of three-dimensional, incompressible, magnetized viscous fluid flow induced by the oscillatory disk. Porous media is used to saturate the rotating disk. Similarity transformations are accomplished to normalize the flow problem. Successive over Relaxation (SOR) technique is implemented to discuss the new findings of normalized non-linear resulting system. It is perceived that increase in porosity parameter results in decrease of oscillatory velocity profiles. The characterization of porous media is useful in geothermal and petroleum reservoirs. Time varying oscillatory curves for concentration and temperature decay for varying concentration and thermal relaxation times parameters, respectively. Moreover, an interesting nature of phase-log shift is also observed in temperature and concentration profiles. Three-dimensional flow features are also labeled for velocity, temperature and concentration fields.


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