Impacts of Stefan Blowing on Reiner–Rivlin Fluid Flow Over Moving Rotating Disk with Chemical Reaction

Kumar, Sanjay; Sharma, Kushal

doi:10.1007/s13369-022-07008-9

Cited by 28 publications

(8 citation statements)

References 44 publications

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“…Let us assume an axisymmetric steady incompressible radiative Maxwell nanofluid flow by a rotating disk [ [9] , [10] , [11] , [12] , [13] , [14] , [15] , [16] , [17] , [18] , [19] , [20] , [21] , [22] ] with the role of Darcy effect. In addition, the heat and mass transportation are also discussed with the influence of heat source/sink, thermal radiation and activation energy [ 23 ], respectively.…”

Section: Modeling Of the Problemmentioning

confidence: 99%

Darcy flow of convective and radiative Maxwell nanofluid over a porous disk with the influence of activation energy

Khan,

Hafeez,

Lone

et al. 2023

Heliyon

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Section: Modeling Of the Problemmentioning

confidence: 99%

Darcy flow of convective and radiative Maxwell nanofluid over a porous disk with the influence of activation energy

Khan,

Hafeez,

Lone

et al. 2023

Heliyon

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“…Mabood et al [30] exhibited that incompressible hydro-magnetic flow on the Maxwell nanofluid along temperature dependent thermally conductivity. Earlier study of the phenomena by various flow geometries were [31][32][33][34][35].…”

Section: Introductionmentioning

confidence: 99%

Stefan Blowing Impact and Chemically Response of Rivlin-Reiner Fluid through Moving Rotating Convected Disk

Gangadhar,

Subbarao,

et al. 2024

Preprint

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The present investigation of rotating disk system had high significance due to its many applications like that fluid thermal reactors, regulations in fluidics systems, and fluid stirring. Subject to upper functions of rotating disk, this consequences on Stefan blowing into the three-dimensional Reiner-Rivlin (R-R) fluid flow by the rotating disk affecting on the vertical direction. Thermal radiation and Cattaneo-Christov (CC) energy diffusions form was incubate into consider energy transport. This Chemical reaction is accommodated by concentration equation. These convective boundary conditions are considered by disk surfaces. The ensuing nonlinear systems are determining applying the shooting method. These obtained outcomes are visualized graphically with physical justification. The results display to Reiner–Rivlin parameters caused the downturn on radial and tangential velocities profile as well as temperatures field, both vertical movement of this disk or not movement along the noted variation in numerical values. The Curves on this temperature enhanced when the greater values of the radiations. Although this radiation fells in to this fluid surface, it enhanced the temperature on the liquid being hot particles strike the cool particles on fluid it enhanced the temperature of the liquid. This present model was calibrated into comparing the decreased model of the investigation to the previously presented article, and a close congruence was founded.

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“…Kodi et al (2022) inspected the MHD Casson nanofluid flow past a vertically placed permeable plate subject to the impact of thermal diffusivity and chemical reactions. Kumar and Sharma (2022) discussed the influences of Stefan blowing on a fluid flow past a rotary disc subject to chemical reactions. Raghunath et al (2022) inspected the time-dependent MHD flow of a liquid over an inclined permeable plate using magnetic impacts and chemical reactions.…”

Section: Introductionmentioning

confidence: 99%

Mechanical characteristics of MHD of the non-Newtonian magnetohydrodynamic Maxwell fluid flow past a bi-directional convectively heated surface with mass flux conditions

Algehyne

Lone²,

Raizah³

et al. 2023

Front. Mater.

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In engineering and manufacturing industries, stretching flow phenomena have numerous real-world implementations. Real-world applications related to stretched flow models are metalworking, crystal growth processes, cooling of fibers, and plastics sheets. Therefore, in this work, the mechanical characteristics of the magnetohydrodynamics of the non-Newtonian Maxwell nanofluid flow through a bi-directional linearly stretching surface are explored. Brownian motion, thermophoresis, and chemical reaction impacts are considered in this analysis. Additionally, thermal convective and mass flux conditions are taken into consideration. The mathematical framework of the existing problem is constructed on highly non-linear partial differential equations (PDEs). Suitable similarity transformations are used for the conversion of partial differential equations into ordinary differential equations (ODEs). The flow problem is tackled with the homotopy analysis method, which is capable of solving higher-order non-linear differential equations. Different flow profiles against various flow parameters are discussed physically. Heat and mass transference mechanisms for distinct flow factors are analyzed in a tabular form. The outcomes showed that both primary and secondary velocities are the declining functions of magnetic and Maxwell fluid parameters. The heat transfer rate rises with the cumulative values of the Brownian motion and thermal Biot number. In addition, the mass transfer rate decreases with the rising Schmidt number, Brownian motion parameter, and chemical reaction parameter, while it increases with the augmenting thermophoresis parameter. It has been highlighted that streamlines in the current work for Maxwell and Newtonian models are in fact different from one another.

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Impacts of Stefan Blowing on Reiner–Rivlin Fluid Flow Over Moving Rotating Disk with Chemical Reaction

Cited by 28 publications

References 44 publications

Darcy flow of convective and radiative Maxwell nanofluid over a porous disk with the influence of activation energy

Darcy flow of convective and radiative Maxwell nanofluid over a porous disk with the influence of activation energy

Stefan Blowing Impact and Chemically Response of Rivlin-Reiner Fluid through Moving Rotating Convected Disk

Mechanical characteristics of MHD of the non-Newtonian magnetohydrodynamic Maxwell fluid flow past a bi-directional convectively heated surface with mass flux conditions

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