Series Solutions for an Unsteady Flow and Heat Transfer of a Rotating Dusty Fluid with Radiation Effect
Acta mathematica Universitatis Comenianae, Tome 86 (2017) no. 1, pp. 111-126
B. J. Gireesha; S. Manjunatha; C. S. Bagewadi; B. J. Gireesha; S. Manjunatha; C. S. Bagewadi. Series Solutions for an Unsteady Flow and Heat Transfer of a Rotating Dusty Fluid with Radiation Effect. Acta mathematica Universitatis Comenianae, Tome 86 (2017) no. 1, pp. 111-126. http://geodesic.mathdoc.fr/item/AMUC_2017_86_1_a9/
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     author = {B. J. Gireesha and S. Manjunatha and C. S. Bagewadi and B. J. Gireesha and S. Manjunatha and C. S. Bagewadi},
     title = { Series {Solutions} for an {Unsteady} {Flow} and {Heat} {Transfer} of a {Rotating} {Dusty} {Fluid} with {Radiation} {Effect}},
     journal = {Acta mathematica Universitatis Comenianae},
     pages = {111--126},
     year = {2017},
     volume = {86},
     number = {1},
     url = {http://geodesic.mathdoc.fr/item/AMUC_2017_86_1_a9/}
}
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A theoretical analysis of free convective MHD flow of an unsteady rotating dustyfluid under the influence of hall current and radiation effect is carried out. The fluid flow is considered in the porous media under the influence of periodic pressure gradient and the fluid is assumed to be viscous, incompressible and electrically conducting with uniform distribution of dust particles. The governing partial differential equations are solved analytically using perturbation technique and the expressions for skin-friction is also derived. Further the effect of various pertinent parameter like magnetic parameter, rotation parameter and Hall current parameter on velocity of both fluid and dust phases are depicted graphically and the effect of radiation parameter, Grashof number and Prandtl number on temperature profile is also discussed in detail.